file examples/DarkBit_standalone_MSSM.cpp
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Namespaces
| Name |
|---|
| DarkBit::Functown |
Functions
| Name | |
|---|---|
| QUICK_FUNCTION(DarkBit , SLHA_pseudonyms , NEW_CAPABILITY , createSLHA1Names , mass_es_pseudonyms , () , (MSSM_spectrum, Spectrum) ) | |
| int | main(int argc, char * argv[]) |
Detailed Description
Author:
- Christoph Weniger
- Sebastian Wild
- Pat Scott
- Jonathan Cornell
- Torsten Bringmann
- Anders Kvellestad
- Ankit Beniwal
- Patrick Stoecker
Date:
- 2016 Feb
- 2016 Aug
- 2016 Nov
- 2016-2017
- 2019, 2022
- 2020 Feb
- 2020
- 2023
Example of GAMBIT DarkBit standalone main program.
Authors (add name and date if you modify):
Functions Documentation
function QUICK_FUNCTION
QUICK_FUNCTION(
DarkBit ,
SLHA_pseudonyms ,
NEW_CAPABILITY ,
createSLHA1Names ,
mass_es_pseudonyms ,
() ,
(MSSM_spectrum, Spectrum)
)
Option inputFileNamestd::string: Input SLHA (required)
Option inputFileNamestd::string: Input SLHA (required)
function main
int main(
int argc,
char * argv[]
)
Source code
// GAMBIT: Global and Modular BSM Inference Tool
// *********************************************
/// \file
///
/// Example of GAMBIT DarkBit standalone
/// main program.
///
/// *********************************************
///
/// Authors (add name and date if you modify):
///
/// \author Christoph Weniger
/// \date 2016 Feb
///
/// \author Sebastian Wild
/// \date 2016 Aug
///
/// \author Pat Scott
/// \date 2016 Nov
///
/// \author Jonathan Cornell
/// \date 2016-2017
///
/// \author Torsten Bringmann
/// \date 2019, 2022
///
/// \author Anders Kvellestad
/// \date 2020 Feb
///
/// \author Ankit Beniwal
/// \date 2020
///
/// \author Patrick Stoecker
/// \date 2023
///
/// *********************************************
#include "gambit/Elements/standalone_module.hpp"
#include "gambit/DarkBit/DarkBit_rollcall.hpp"
#include "gambit/Elements/spectrum_factories.hpp"
#include "gambit/Elements/mssm_slhahelp.hpp"
#include "gambit/Models/SimpleSpectra/MSSMSimpleSpec.hpp"
#include "gambit/Utils/util_functions.hpp"
using namespace DarkBit::Functown; // Functors wrapping the module's actual module functions
using namespace BackendIniBit::Functown; // Functors wrapping the backend initialisation functions
QUICK_FUNCTION(DarkBit, decay_rates, NEW_CAPABILITY, createDecays, DecayTable, ())
QUICK_FUNCTION(DarkBit, MSSM_spectrum, OLD_CAPABILITY, createSpectrum, Spectrum, ())
QUICK_FUNCTION(DarkBit, SLHA_pseudonyms, NEW_CAPABILITY, createSLHA1Names, mass_es_pseudonyms, (), (MSSM_spectrum, Spectrum))
QUICK_FUNCTION(DarkBit, cascadeMC_gammaSpectra, OLD_CAPABILITY, CMC_dummy, DarkBit::stringFunkMap, ())
namespace Gambit
{
namespace DarkBit
{
// Dummy functor for returning empty cascadeMC result spectra
void CMC_dummy(DarkBit::stringFunkMap& result)
{
DarkBit::stringFunkMap sfm;
result = sfm;
}
// Create spectrum object from SLHA file
void createSpectrum(Spectrum& outSpec)
{
using namespace Pipes::createSpectrum;
/// Option inputFileName<std::string>: Input SLHA (required)
std::string inputFileName = runOptions->getValue<std::string>("filename");
std::cout << "Loading spectrum from: " << inputFileName << std::endl;
outSpec = spectrum_from_SLHA<MSSMSimpleSpec>(inputFileName, Spectrum::mc_info(), Spectrum::mr_info());
}
// Create decay object from SLHA file
void createDecays(DecayTable& outDecays)
{
using namespace Pipes::createDecays;
/// Option inputFileName<std::string>: Input SLHA (required)
std::string inputFileName = runOptions->getValue<std::string>("filename");
std::cout << "Loading decays from: " << inputFileName << std::endl;
outDecays = DecayTable(inputFileName, 0, true);
}
// Create SLHA1 pseudonyms from Spectrum object
void createSLHA1Names(mass_es_pseudonyms& names)
{
const double gauge_mixing_tol = 0.5;
const bool tol_invalidates_pt = true;
const bool debug = false;
names.refill(Pipes::createSLHA1Names::Dep::MSSM_spectrum->get_HE(), gauge_mixing_tol, tol_invalidates_pt, debug);
}
}
}
int main(int argc, char* argv[])
{
std::cout << std::endl;
std::cout << "Welcome to the DarkBit MSSM standalone program!" << std::endl;
std::cout << std::endl;
std::cout << "********************************************************************************" << std::endl;
std::cout << "Usage: DarkBit_standalone_MSSM SLHA_file (spectrum) (output)" << std::endl;
std::cout << std::endl;
std::cout << "SLHA_file: SLHA file used to intialise the program (required)" << std::endl;
std::cout << "(spectrum): name of output file for gamma-ray spectrum (default: BACKENDNAME_dNdE.dat)" << std::endl;
std::cout << "(output): name of output file for observables and likelihoods (default: DarkBit_standalone_MSSM.out)" << std::endl;
std::cout << std::endl;
std::cout << "The SLHA files for the MSSM-7 benchmarks in the DarkBit paper are located in " << std::endl;
std::cout << "DarkBit/data/benchmarks/ " << std::endl;
std::cout << "********************************************************************************" << std::endl;
std::cout << std::endl;
try
{
if (argc == 1)
{
std::cout << "Please provide name of SLHA file at command line." << std::endl;
exit(1);
}
std::string filename = argv[1];
std::string outname_dNdE_spectrum = "dNdE.dat";
if (argc >= 3) outname_dNdE_spectrum = argv[2];
std::string outname_data = "DarkBit_standalone_MSSM.out";
if (argc >= 4) outname_data = argv[3];
// ---- Initialise logging and exceptions ----
initialise_standalone_logs("runs/DarkBit_standalone_MSSM/logs/");
logger()<<"Running DarkBit standalone example"<<LogTags::info<<EOM;
model_warning().set_fatal(true);
// Initialise settings for printer (required)
YAML::Node printerNode = get_standalone_printer("cout", "runs/DarkBit_standalone_MSSM/logs/","");
Printers::PrinterManager printerManager(printerNode, false);
set_global_printer_manager(&printerManager);
// ---- Check which backends are present ----
if (not Backends::backendInfo().works["gamLike1.0.1"]) backend_error().raise(LOCAL_INFO, "gamLike 1.0.1 is missing!");
if (not Backends::backendInfo().works["DDCalc2.3.0"]) backend_error().raise(LOCAL_INFO, "DDCalc 2.3.0 is missing!");
if (not Backends::backendInfo().works["nulike1.0.9"]) backend_error().raise(LOCAL_INFO, "nulike 1.0.9 is missing!");
// ---- Useful variables ----
//
// Prepare a str-str-double map of maps to hold the results.
// We will add results for the individual backends as
// results["oh2"]["MicrOmegas_MSSM3.6.9.2"] = ...
// results["oh2"]["DarkSUSY_MSSM6.1.1"] = ...
//
std::map<std::string, std::map<std::string,double> > results;
results["oh2"] = std::map<std::string,double>();
results["oh2_lnL"] = std::map<std::string,double>();
results["sigma_SI_p"] = std::map<std::string,double>();
results["sigma_SD_p"] = std::map<std::string,double>();
results["LUX_2016_lnL"] = std::map<std::string,double>();
results["IceCube_79_lnL"] = std::map<std::string,double>();
results["sigmav0"] = std::map<std::string,double>();
results["FermiLAT_dwarfsph_lnL"] = std::map<std::string,double>();
std::map<std::string, std::string> results_units;
results_units["oh2"] = "";
results_units["oh2_lnL"] = "";
results_units["sigma_SI_p"] = "cm^2";
results_units["sigma_SD_p"] = "cm^2";
results_units["LUX_2016_lnL"] = "";
results_units["IceCube_79_lnL"] = "";
results_units["sigmav0"] = "cm^3/s";
results_units["FermiLAT_dwarfsph_lnL"] = "";
std::vector<std::string> result_output_order = {
"oh2",
"oh2_lnL",
"sigma_SI_p",
"sigma_SD_p",
"LUX_2016_lnL",
"IceCube_79_lnL",
"sigmav0",
"FermiLAT_dwarfsph_lnL",
};
// A string to refer to the current backend being used for calculations
std::string current_backend = "";
// Keep track of which backends are not installed
std::vector<std::string> backends_not_built;
// ---- Initialize models ----
// Initialize halo model
ModelParameters* Halo_primary_parameters = Models::Halo_Einasto::Functown::primary_parameters.getcontentsPtr();
Halo_primary_parameters->setValue("rho0", 0.4);
Halo_primary_parameters->setValue("rhos", 0.08);
Halo_primary_parameters->setValue("vrot", 235.);
Halo_primary_parameters->setValue("v0", 235.);
Halo_primary_parameters->setValue("vesc", 550.);
Halo_primary_parameters->setValue("rs", 20.);
Halo_primary_parameters->setValue("r_sun", 8.5);
Halo_primary_parameters->setValue("alpha", 0.17);
// --- Resolve halo dependencies ---
ExtractLocalMaxwellianHalo.notifyOfModel("Halo_Einasto");
ExtractLocalMaxwellianHalo.resolveDependency(&Models::Halo_Einasto::Functown::primary_parameters);
ExtractLocalMaxwellianHalo.reset_and_calculate();
GalacticHalo_Einasto.notifyOfModel("Halo_Einasto");
GalacticHalo_Einasto.resolveDependency(&Models::Halo_Einasto::Functown::primary_parameters);
GalacticHalo_Einasto.reset_and_calculate();
// Initialize nuclear_params_fnq model
ModelParameters* nuclear_params_fnq = Models::nuclear_params_fnq::Functown::primary_parameters.getcontentsPtr();
nuclear_params_fnq->setValue("fpd", 0.034);
nuclear_params_fnq->setValue("fpu", 0.023);
nuclear_params_fnq->setValue("fps", 0.14);
nuclear_params_fnq->setValue("fnd", 0.041);
nuclear_params_fnq->setValue("fnu", 0.019);
nuclear_params_fnq->setValue("fns", 0.14);
nuclear_params_fnq->setValue("deltad", -0.40);
nuclear_params_fnq->setValue("deltau", 0.74);
nuclear_params_fnq->setValue("deltas", -0.12);
// Resolve other dependencies related directly to the GAMBIT Models
DD_couplings_DarkSUSY_DS5.notifyOfModel("nuclear_params_fnq");
DD_couplings_DarkSUSY_DS5.resolveDependency(&Models::nuclear_params_fnq::Functown::primary_parameters);
DD_couplings_DarkSUSY_MSSM.notifyOfModel("nuclear_params_fnq");
DD_couplings_DarkSUSY_MSSM.resolveDependency(&Models::nuclear_params_fnq::Functown::primary_parameters);
DD_couplings_MicrOmegas.notifyOfModel("MSSM30atQ");
DD_couplings_MicrOmegas.notifyOfModel("nuclear_params_fnq");
DD_couplings_MicrOmegas.resolveDependency(&Models::nuclear_params_fnq::Functown::primary_parameters);
// ---- Initialize spectrum and decays from SLHA file ----
createSpectrum.setOption<std::string>("filename", filename);
createSpectrum.reset_and_calculate();
createSLHA1Names.resolveDependency(&createSpectrum);
createSLHA1Names.reset_and_calculate();
createDecays.setOption<std::string>("filename", filename);
createDecays.reset_and_calculate();
// Check that the decay table contains ~chi0_2 (if it doesn't,
// we do not use information from the SLHA decay block)
bool decays = true;
try { createDecays(0).at("~chi0_2"); }
catch(std::exception& e)
{
decays = false;
cout << "It appears that the decay block is missing from the SLHA file. Decay widths\n"
"will be determined by the backends." << endl;
}
// Set identifier for DM particle
DarkMatter_ID_MSSM.resolveDependency(&createSpectrum);
DarkMatter_ID_MSSM.reset_and_calculate();
DarkMatterConj_ID_MSSM.resolveDependency(&createSpectrum);
DarkMatterConj_ID_MSSM.reset_and_calculate();
// Assume for direct and indirect detection likelihoods that dark matter
// density is always the measured one (regardless of relic density results)
RD_fraction_one.reset_and_calculate();
//
// ======= Initializations that can be done once =======
//
// Initialize nulike backend
Backends::nulike_1_0_9::Functown::nulike_bounds.setStatus(FunctorStatus::Active);
nulike_1_0_9_init.reset_and_calculate();
// Initialize gamLike backend
gamLike_1_0_1_init.reset_and_calculate();
//
// ======= Perform all calculations for backend DarkSUSY 5.1.3 =======
//
current_backend = "DarkSUSY5.1.3";
if (not Backends::backendInfo().works[current_backend])
{
backends_not_built.push_back(current_backend);
}
else
{
// Initialize DarkSUSY 5 backend
DarkSUSY_5_1_3_init.notifyOfModel("MSSM30atQ");
DarkSUSY_5_1_3_init.resolveDependency(&createSpectrum);
DarkSUSY_5_1_3_init.resolveDependency(&createDecays);
if (decays) DarkSUSY_5_1_3_init.setOption<bool>("use_dsSLHAread", false);
else DarkSUSY_5_1_3_init.setOption<bool>("use_dsSLHAread", true);
DarkSUSY_5_1_3_init.reset_and_calculate();
// Initialize DarkSUSY 5 Local Halo Model
DarkSUSY5_PointInit_LocalHalo_func.resolveDependency(&ExtractLocalMaxwellianHalo);
DarkSUSY5_PointInit_LocalHalo_func.resolveDependency(&RD_fraction_one);
DarkSUSY5_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dshmcom);
DarkSUSY5_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dshmisodf);
DarkSUSY5_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dshmframevelcom);
DarkSUSY5_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dshmnoclue);
DarkSUSY5_PointInit_LocalHalo_func.reset_and_calculate();
// Relic density calculation with GAMBIT routines and DarkSUSY 5:
RD_spectrum_SUSY_DS5.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::mspctm);
RD_spectrum_SUSY_DS5.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::widths);
RD_spectrum_SUSY_DS5.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::intdof);
RD_spectrum_SUSY_DS5.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::pacodes);
RD_spectrum_SUSY_DS5.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::DSparticle_code);
// Below true if charginos and neutralinos are included in coannihilations:
RD_spectrum_SUSY_DS5.setOption<bool>("CoannCharginosNeutralinos", true);
// Below true if sfermions are included in coannihilations:
RD_spectrum_SUSY_DS5.setOption<bool>("CoannSfermions", true);
// Maximum sparticle mass to be icluded in coannihilations, in units of DM mass:
RD_spectrum_SUSY_DS5.setOption<double>("CoannMaxMass", 1.6);
RD_spectrum_SUSY_DS5.reset_and_calculate();
RD_spectrum_ordered_func.resolveDependency(&RD_spectrum_SUSY_DS5);
RD_spectrum_ordered_func.reset_and_calculate();
RD_annrate_DS5prep_func.resolveDependency(&RD_spectrum_SUSY_DS5);
RD_annrate_DS5prep_func.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::rdmgev);
RD_annrate_DS5prep_func.reset_and_calculate();
RD_eff_annrate_DS5_MSSM.notifyOfModel("MSSM30atQ");
RD_eff_annrate_DS5_MSSM.resolveDependency(&RD_annrate_DS5prep_func);
RD_eff_annrate_DS5_MSSM.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dsanwx);
RD_eff_annrate_DS5_MSSM.reset_and_calculate();
RD_oh2_DS5_general.resolveDependency(&RD_spectrum_ordered_func);
RD_oh2_DS5_general.resolveDependency(&RD_eff_annrate_DS5_MSSM);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dsrdthlim);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dsrdtab);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dsrdeqn);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dsrdwintp);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::DSparticle_code);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::widths);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::rdmgev);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::rdpth);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::rdpars);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::rdswitch);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::rdlun);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::rdpadd);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::rddof);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::rderrors);
RD_oh2_DS5_general.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::rdtime);
RD_oh2_DS5_general.setOption<int>("fast", 1); // 0: normal; 1: fast; 2: dirty
RD_oh2_DS5_general.reset_and_calculate();
results["oh2"][current_backend] = RD_oh2_DS5_general(0);
lnL_oh2_Simple.resolveDependency(&RD_oh2_DS5_general);
lnL_oh2_Simple.reset_and_calculate();
// Save the result
results["oh2_lnL"][current_backend] = lnL_oh2_Simple(0);
// ---- Set up basic internal structures for direct & indirect detection ----
// Set up process catalog based on DarkSUSY annihilation rates
TH_ProcessCatalog_DS5_MSSM.resolveDependency(&createSpectrum);
TH_ProcessCatalog_DS5_MSSM.resolveDependency(&createDecays);
TH_ProcessCatalog_DS5_MSSM.resolveDependency(&DarkMatter_ID_MSSM);
TH_ProcessCatalog_DS5_MSSM.resolveDependency(&DarkMatterConj_ID_MSSM);
TH_ProcessCatalog_DS5_MSSM.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dssigmav);
TH_ProcessCatalog_DS5_MSSM.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dsIBffdxdy);
TH_ProcessCatalog_DS5_MSSM.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dsIBhhdxdy);
TH_ProcessCatalog_DS5_MSSM.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dsIBwhdxdy);
TH_ProcessCatalog_DS5_MSSM.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dsIBwwdxdy);
TH_ProcessCatalog_DS5_MSSM.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::IBintvars);
TH_ProcessCatalog_DS5_MSSM.reset_and_calculate();
// Set generic WIMP mass object
WIMP_properties.notifyOfModel("MSSM30atQ");
WIMP_properties.resolveDependency(&DarkMatter_ID_MSSM);
WIMP_properties.resolveDependency(&DarkMatterConj_ID_MSSM);
WIMP_properties.resolveDependency(&createSpectrum);
WIMP_properties.reset_and_calculate();
mwimp_generic.resolveDependency(&WIMP_properties);
mwimp_generic.reset_and_calculate();
// Set generic annihilation rate in late universe (v->0 limit)
sigmav_late_universe.resolveDependency(&TH_ProcessCatalog_DS5_MSSM);
sigmav_late_universe.resolveDependency(&DarkMatter_ID_MSSM);
sigmav_late_universe.resolveDependency(&DarkMatterConj_ID_MSSM);
sigmav_late_universe.reset_and_calculate();
// Save the result
results["sigmav0"][current_backend] = sigmav_late_universe(0);
// ---- Direct detection -----
// Calculate DD couplings with DarkSUSY
// DD_couplings_DarkSUSY_DS5.notifyOfModel("nuclear_params_fnq");
// DD_couplings_DarkSUSY_DS5.resolveDependency(&Models::nuclear_params_fnq::Functown::primary_parameters);
DD_couplings_DarkSUSY_DS5.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::DD_couplings);
DD_couplings_DarkSUSY_DS5.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::mspctm);
DD_couplings_DarkSUSY_DS5.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::ddcom);
// The below calculates the DD couplings using the full 1 loop calculation of
// Drees Nojiri Phys.Rev. D48 (1993) 3483
DD_couplings_DarkSUSY_DS5.setOption<bool>("loop", true);
// Setting the below to false approximates the squark propagator as 1/m_sq^2 to avoid poles.
// To reproduce numbers in Tables 11/12 of DarkBit paper (https://arxiv.org/abs/1705.07920), set "pole" to true.
DD_couplings_DarkSUSY_DS5.setOption<bool>("pole", false);
DD_couplings_DarkSUSY_DS5.reset_and_calculate();
// Calculate DD couplings for DDCalc
DDCalc_Couplings_WIMP_nucleon.resolveDependency(&DD_couplings_DarkSUSY_DS5);
DDCalc_Couplings_WIMP_nucleon.reset_and_calculate();
// Initialize DDCalc backend
Backends::DDCalc_2_3_0::Functown::DDCalc_CalcRates_simple.setStatus(FunctorStatus::Active);
Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment.setStatus(FunctorStatus::Active);
Backends::DDCalc_2_3_0::Functown::DDCalc_LogLikelihood.setStatus(FunctorStatus::Active);
DDCalc_2_3_0_init.resolveDependency(&ExtractLocalMaxwellianHalo);
DDCalc_2_3_0_init.resolveDependency(&RD_fraction_one);
DDCalc_2_3_0_init.resolveDependency(&mwimp_generic);
DDCalc_2_3_0_init.resolveDependency(&DDCalc_Couplings_WIMP_nucleon);
DDCalc_2_3_0_init.reset_and_calculate();
// Calculate direct detection rates for LUX 2016
LUX_2016_Calc.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment);
LUX_2016_Calc.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_CalcRates_simple);
LUX_2016_Calc.reset_and_calculate();
// Calculate direct detection likelihood for LUX 2016
LUX_2016_GetLogLikelihood.resolveDependency(&LUX_2016_Calc);
LUX_2016_GetLogLikelihood.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment);
LUX_2016_GetLogLikelihood.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_LogLikelihood);
LUX_2016_GetLogLikelihood.reset_and_calculate();
// Save the result
results["LUX_2016_lnL"][current_backend] = LUX_2016_GetLogLikelihood(0);
sigma_SI_p_simple.resolveDependency(&mwimp_generic);
sigma_SI_p_simple.resolveDependency(&DD_couplings_DarkSUSY_DS5);
sigma_SI_p_simple.reset_and_calculate();
// Save the result
results["sigma_SI_p"][current_backend] = sigma_SI_p_simple(0);
sigma_SD_p_simple.resolveDependency(&mwimp_generic);
sigma_SD_p_simple.resolveDependency(&DD_couplings_DarkSUSY_DS5);
sigma_SD_p_simple.reset_and_calculate();
// Save the result
results["sigma_SD_p"][current_backend] = sigma_SD_p_simple(0);
// ---- Gamma-ray yields ----
// Initialize tabulated gamma-ray yields
GA_SimYieldTable_DS5.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dshayield);
GA_SimYieldTable_DS5.reset_and_calculate();
Combine_SimYields.resolveDependency(&GA_SimYieldTable_DS5);
// Here we need to establish the dependency chain from Combine_SimYields down to cascadeMC_gammaSpectra
// *before* Combine_SimYields runs in order for it to correctly realise that it needs to enable gammas.
cascadeMC_InitialStates.resolveDependency(&Combine_SimYields);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_InitialStates);
Combine_SimYields.reset_and_calculate();
// Identify process as annihilation rather than decay
DM_process_from_ProcessCatalog.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
DM_process_from_ProcessCatalog.resolveDependency(&DarkMatter_ID_MSSM);
DM_process_from_ProcessCatalog.reset_and_calculate();
// Set up initial states for cascade MC
cascadeMC_InitialStates.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_InitialStates.resolveDependency(&TH_ProcessCatalog_DS5_MSSM);
cascadeMC_InitialStates.resolveDependency(&DarkMatter_ID_MSSM);
cascadeMC_InitialStates.resolveDependency(&DarkMatterConj_ID_MSSM);
cascadeMC_InitialStates.resolveDependency(&DM_process_from_ProcessCatalog);
cascadeMC_InitialStates.reset_and_calculate();
// Infer for which type of final states particles MC should be performed
cascadeMC_FinalStates.setOption<std::vector<std::string>>("cMC_finalStates", daFunk::vec<std::string>("gamma"));
// Here we need to establish the dependency chain from cascadeMC_FinalStates down to cascadeMC_gammaSpectra
// *before* cascadeMC_FinalStates runs in order for it to correctly realise that it needs to enable gammas.
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_FinalStates.reset_and_calculate();
// Collect decay information for cascade MC
cascadeMC_DecayTable.resolveDependency(&TH_ProcessCatalog_DS5_MSSM);
cascadeMC_DecayTable.resolveDependency(&Combine_SimYields);
cascadeMC_DecayTable.reset_and_calculate();
// cascadeMC_LoopManager.setOption<int>("cMC_maxEvents", 100000);
// cascadeMC_Histograms.setOption<double>("cMC_endCheckFrequency", 25);
// cascadeMC_Histograms.setOption<double>("cMC_gammaRelError", .05);
// cascadeMC_Histograms.setOption<int>("cMC_numSpecSamples", 25);
// cascadeMC_Histograms.setOption<int>("cMC_NhistBins", 300);
// Set up MC loop manager for cascade MC
cascadeMC_LoopManager.resolveDependency(&cascadeMC_InitialStates);
std::vector<functor*> nested_functions = initVector<functor*>(
&cascadeMC_GenerateChain, &cascadeMC_Histograms, &cascadeMC_EventCount);
cascadeMC_LoopManager.setNestedList(nested_functions);
// Perform MC step for cascade MC
cascadeMC_GenerateChain.resolveDependency(&cascadeMC_DecayTable);
cascadeMC_GenerateChain.resolveLoopManager(&cascadeMC_LoopManager);
// Generate histogram for cascade MC
cascadeMC_Histograms.resolveDependency(&cascadeMC_GenerateChain);
cascadeMC_Histograms.resolveDependency(&TH_ProcessCatalog_DS5_MSSM);
cascadeMC_Histograms.resolveDependency(&Combine_SimYields);
cascadeMC_Histograms.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_Histograms.resolveLoopManager(&cascadeMC_LoopManager);
// Check convergence of cascade MC
cascadeMC_EventCount.resolveLoopManager(&cascadeMC_LoopManager);
// Start cascade MC loop
cascadeMC_LoopManager.reset_and_calculate();
// Infer gamma-ray spectra for recorded MC results
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_InitialStates);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_Histograms);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_EventCount);
cascadeMC_gammaSpectra.reset_and_calculate();
// Calculate total gamma-ray yield (cascade MC + tabulated results)
GA_AnnYield_General.resolveDependency(&TH_ProcessCatalog_DS5_MSSM);
GA_AnnYield_General.resolveDependency(&GA_SimYieldTable_DS5);
GA_AnnYield_General.resolveDependency(&DarkMatter_ID_MSSM);
GA_AnnYield_General.resolveDependency(&DarkMatterConj_ID_MSSM);
GA_AnnYield_General.resolveDependency(&cascadeMC_gammaSpectra);
GA_AnnYield_General.reset_and_calculate();
// Dump spectrum into file
dump_gammaSpectrum.resolveDependency(&GA_AnnYield_General);
dump_gammaSpectrum.setOption<std::string>("filename", current_backend + "_" + outname_dNdE_spectrum);
dump_gammaSpectrum.reset_and_calculate();
// Calculate Fermi LAT dwarf likelihood
lnL_FermiLATdwarfs_gamLike.resolveDependency(&GA_AnnYield_General);
lnL_FermiLATdwarfs_gamLike.resolveDependency(&RD_fraction_one);
lnL_FermiLATdwarfs_gamLike.resolveDependency(&DM_process_from_ProcessCatalog);
lnL_FermiLATdwarfs_gamLike.resolveBackendReq(&Backends::gamLike_1_0_1::Functown::lnL);
lnL_FermiLATdwarfs_gamLike.reset_and_calculate();
// Save the result
results["FermiLAT_dwarfsph_lnL"][current_backend] = lnL_FermiLATdwarfs_gamLike(0);
// ---- IceCube limits ----
// Infer WIMP capture rate in Sun
capture_rate_Sun_const_xsec_DS5.resolveDependency(&mwimp_generic);
capture_rate_Sun_const_xsec_DS5.resolveDependency(&sigma_SI_p_simple);
capture_rate_Sun_const_xsec_DS5.resolveDependency(&sigma_SD_p_simple);
capture_rate_Sun_const_xsec_DS5.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dsntcapsuntab);
capture_rate_Sun_const_xsec_DS5.resolveDependency(&DarkSUSY5_PointInit_LocalHalo_func);
capture_rate_Sun_const_xsec_DS5.reset_and_calculate();
// Infer WIMP equilibration time in Sun
equilibration_time_Sun.resolveDependency(&TH_ProcessCatalog_DS5_MSSM);
equilibration_time_Sun.resolveDependency(&DarkMatter_ID_MSSM);
equilibration_time_Sun.resolveDependency(&DarkMatterConj_ID_MSSM);
equilibration_time_Sun.resolveDependency(&mwimp_generic);
equilibration_time_Sun.resolveDependency(&capture_rate_Sun_const_xsec_DS5);
equilibration_time_Sun.reset_and_calculate();
// Infer WIMP annihilation rate in Sun
annihilation_rate_Sun.resolveDependency(&equilibration_time_Sun);
annihilation_rate_Sun.resolveDependency(&capture_rate_Sun_const_xsec_DS5);
annihilation_rate_Sun.reset_and_calculate();
// Infer neutrino yield from Sun
nuyield_from_DS.resolveDependency(&TH_ProcessCatalog_DS5_MSSM);
nuyield_from_DS.resolveDependency(&mwimp_generic);
nuyield_from_DS.resolveDependency(&sigmav_late_universe);
nuyield_from_DS.resolveDependency(&DarkMatter_ID_MSSM);
nuyield_from_DS.resolveDependency(&DarkMatterConj_ID_MSSM);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::dsgenericwimp_nusetup);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::neutrino_yield);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::DS_neutral_h_decay_channels);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_5_1_3::Functown::DS_charged_h_decay_channels);
nuyield_from_DS.reset_and_calculate();
// Calculate number of events at IceCube
IC79WH_full.resolveDependency(&mwimp_generic);
IC79WH_full.resolveDependency(&annihilation_rate_Sun);
IC79WH_full.resolveDependency(&nuyield_from_DS);
IC79WH_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79WH_full.reset_and_calculate();
IC79WL_full.resolveDependency(&mwimp_generic);
IC79WL_full.resolveDependency(&annihilation_rate_Sun);
IC79WL_full.resolveDependency(&nuyield_from_DS);
IC79WL_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79WL_full.reset_and_calculate();
IC79SL_full.resolveDependency(&mwimp_generic);
IC79SL_full.resolveDependency(&annihilation_rate_Sun);
IC79SL_full.resolveDependency(&nuyield_from_DS);
IC79SL_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79SL_full.reset_and_calculate();
// Calculate IceCube likelihood
IC79WH_bgloglike.resolveDependency(&IC79WH_full);
IC79WH_bgloglike.reset_and_calculate();
IC79WH_loglike.resolveDependency(&IC79WH_full);
IC79WH_loglike.reset_and_calculate();
IC79WL_bgloglike.resolveDependency(&IC79WL_full);
IC79WL_bgloglike.reset_and_calculate();
IC79WL_loglike.resolveDependency(&IC79WL_full);
IC79WL_loglike.reset_and_calculate();
IC79SL_bgloglike.resolveDependency(&IC79SL_full);
IC79SL_bgloglike.reset_and_calculate();
IC79SL_loglike.resolveDependency(&IC79SL_full);
IC79SL_loglike.reset_and_calculate();
IC79_loglike.resolveDependency(&IC79WH_bgloglike);
IC79_loglike.resolveDependency(&IC79WH_loglike);
IC79_loglike.resolveDependency(&IC79WL_bgloglike);
IC79_loglike.resolveDependency(&IC79WL_loglike);
IC79_loglike.resolveDependency(&IC79SL_bgloglike);
IC79_loglike.resolveDependency(&IC79SL_loglike);
IC79_loglike.reset_and_calculate();
// Save the result
results["IceCube_79_lnL"][current_backend] = IC79_loglike(0);
} // End of DarkSUSY 5.1.3 calculations
//
// ======= Perform all calculations for backend DarkSUSY_MSSM 6.1.1 =======
//
current_backend = "DarkSUSY_MSSM6.1.1";
if (not Backends::backendInfo().works[current_backend])
{
backends_not_built.push_back(current_backend);
}
else
{
// Initialize DarkSUSY 6 MSSM backend
DarkSUSY_MSSM_6_1_1_init.notifyOfModel("MSSM30atQ");
DarkSUSY_MSSM_6_1_1_init.resolveDependency(&createSpectrum);
DarkSUSY_MSSM_6_1_1_init.resolveDependency(&createDecays);
if (decays) DarkSUSY_MSSM_6_1_1_init.setOption<bool>("use_dsSLHAread", false);
else DarkSUSY_MSSM_6_1_1_init.setOption<bool>("use_dsSLHAread", true);
DarkSUSY_MSSM_6_1_1_init.reset_and_calculate();
// Initialize DarkSUSY 6 Local Halo Model
DarkSUSY_PointInit_LocalHalo_func.resolveDependency(&ExtractLocalMaxwellianHalo);
DarkSUSY_PointInit_LocalHalo_func.resolveDependency(&RD_fraction_one);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dshmcom);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dshmisodf);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dshmframevelcom);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dshmnoclue);
DarkSUSY_PointInit_LocalHalo_func.reset_and_calculate();
// Relic density calculation with GAMBIT routines and DarkSUSY 6:
RD_spectrum_MSSM.resolveDependency(&createDecays);
RD_spectrum_MSSM.resolveDependency(&createSpectrum);
RD_spectrum_MSSM.resolveDependency(&DarkMatter_ID_MSSM);
// Below true if charginos and neutralinos are included in coannihilations:
RD_spectrum_MSSM.setOption<bool>("CoannCharginosNeutralinos", true);
// Below true if sfermions are included in coannihilations:
RD_spectrum_MSSM.setOption<bool>("CoannSfermions", true);
// Maximum sparticle mass to be icluded in coannihilations, in units of DM mass:
RD_spectrum_MSSM.setOption<double>("CoannMaxMass", 1.6);
RD_spectrum_MSSM.reset_and_calculate();
RD_spectrum_ordered_func.resolveDependency(&RD_spectrum_MSSM);
RD_spectrum_ordered_func.reset_and_calculate();
RD_annrate_DSprep_MSSM_func.resolveDependency(&RD_spectrum_ordered_func);
RD_annrate_DSprep_MSSM_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dsancoann);
RD_annrate_DSprep_MSSM_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::DSparticle_code);
RD_annrate_DSprep_MSSM_func.reset_and_calculate();
RD_eff_annrate_DS_MSSM.notifyOfModel("MSSM30atQ");
RD_eff_annrate_DS_MSSM.resolveDependency(&RD_annrate_DSprep_MSSM_func);
RD_eff_annrate_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dsanwx);
RD_eff_annrate_DS_MSSM.reset_and_calculate();
RD_oh2_DS6pre4_ini_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dsrdcom);
RD_oh2_DS6pre4_ini_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::rdpars);
RD_oh2_DS6pre4_ini_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::rdtime);
RD_oh2_DS6pre4_ini_func.setOption<int>("fast", 1); // 0: normal; 1: fast; 2: dirty
RD_oh2_DS6pre4_ini_func.reset_and_calculate();
RD_oh2_DS_general.resolveDependency(&RD_spectrum_ordered_func);
RD_oh2_DS_general.resolveDependency(&RD_eff_annrate_DS_MSSM);
RD_oh2_DS_general.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dsrdstart);
RD_oh2_DS_general.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dsrdens);
// Note that this one has to come *last* since it's a conditional dependency
RD_oh2_DS_general.resolveDependency(&RD_oh2_DS6pre4_ini_func);
RD_oh2_DS_general.reset_and_calculate();
// Save the result
results["oh2"][current_backend] = RD_oh2_DS_general(0);
lnL_oh2_Simple.resolveDependency(&RD_oh2_DS_general);
lnL_oh2_Simple.reset_and_calculate();
// Save the result
results["oh2_lnL"][current_backend] = lnL_oh2_Simple(0);
// Set up process catalog based on DarkSUSY annihilation rates
TH_ProcessCatalog_DS_MSSM.resolveDependency(&createSpectrum);
TH_ProcessCatalog_DS_MSSM.resolveDependency(&createDecays);
TH_ProcessCatalog_DS_MSSM.resolveDependency(&DarkMatter_ID_MSSM);
TH_ProcessCatalog_DS_MSSM.resolveDependency(&DarkMatterConj_ID_MSSM);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dssigmav0);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dssigmav0tot);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dsIBffdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dsIBhhdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dsIBwhdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dsIBwwdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::IBintvars);
TH_ProcessCatalog_DS_MSSM.reset_and_calculate();
// Set generic WIMP mass object
WIMP_properties.notifyOfModel("MSSM30atQ");
WIMP_properties.resolveDependency(&DarkMatter_ID_MSSM);
WIMP_properties.resolveDependency(&DarkMatterConj_ID_MSSM);
WIMP_properties.resolveDependency(&createSpectrum);
WIMP_properties.reset_and_calculate();
mwimp_generic.resolveDependency(&WIMP_properties);
mwimp_generic.reset_and_calculate();
// Set generic annihilation rate in late universe (v->0 limit)
sigmav_late_universe.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
sigmav_late_universe.resolveDependency(&DarkMatter_ID_MSSM);
sigmav_late_universe.resolveDependency(&DarkMatterConj_ID_MSSM);
sigmav_late_universe.reset_and_calculate();
// Save the result
results["sigmav0"][current_backend] = sigmav_late_universe(0);
// ---- Gamma-ray yields ----
// Initialize tabulated gamma-ray yields
GA_SimYieldTable_DarkSUSY.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dsanyield_sim);
GA_SimYieldTable_DarkSUSY.reset_and_calculate();
Combine_SimYields.resolveDependency(&GA_SimYieldTable_DarkSUSY);
// Here we need to establish the dependency chain from Combine_SimYields down to cascadeMC_gammaSpectra
// *before* Combine_SimYields runs in order for it to correctly realise that it needs to enable gammas.
cascadeMC_InitialStates.resolveDependency(&Combine_SimYields);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_InitialStates);
Combine_SimYields.reset_and_calculate();
// Identify process as annihilation rather than decay
DM_process_from_ProcessCatalog.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
DM_process_from_ProcessCatalog.resolveDependency(&DarkMatter_ID_MSSM);
DM_process_from_ProcessCatalog.reset_and_calculate();
// Set up initial states for cascade MC
cascadeMC_InitialStates.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_InitialStates.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
cascadeMC_InitialStates.resolveDependency(&DarkMatter_ID_MSSM);
cascadeMC_InitialStates.resolveDependency(&DarkMatterConj_ID_MSSM);
cascadeMC_InitialStates.resolveDependency(&DM_process_from_ProcessCatalog);
cascadeMC_InitialStates.reset_and_calculate();
// Infer for which type of final states particles MC should be performed
cascadeMC_FinalStates.setOption<std::vector<std::string>>("cMC_finalStates", daFunk::vec<std::string>("gamma"));
// Here we need to establish the dependency chain from cascadeMC_FinalStates down to cascadeMC_gammaSpectra
// *before* cascadeMC_FinalStates runs in order for it to correctly realise that it needs to enable gammas.
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_FinalStates.reset_and_calculate();
// Collect decay information for cascade MC
cascadeMC_DecayTable.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
cascadeMC_DecayTable.resolveDependency(&Combine_SimYields);
cascadeMC_DecayTable.reset_and_calculate();
// Set up MC loop manager for cascade MC
cascadeMC_LoopManager.resolveDependency(&cascadeMC_InitialStates);
std::vector<functor*> nested_functions = initVector<functor*>(
&cascadeMC_GenerateChain, &cascadeMC_Histograms, &cascadeMC_EventCount);
cascadeMC_LoopManager.setNestedList(nested_functions);
// Perform MC step for cascade MC
cascadeMC_GenerateChain.resolveDependency(&cascadeMC_DecayTable);
cascadeMC_GenerateChain.resolveLoopManager(&cascadeMC_LoopManager);
// Generate histogram for cascade MC
cascadeMC_Histograms.resolveDependency(&cascadeMC_GenerateChain);
cascadeMC_Histograms.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
cascadeMC_Histograms.resolveDependency(&Combine_SimYields);
cascadeMC_Histograms.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_Histograms.resolveLoopManager(&cascadeMC_LoopManager);
// Check convergence of cascade MC
cascadeMC_EventCount.resolveLoopManager(&cascadeMC_LoopManager);
// Start cascade MC loop
cascadeMC_LoopManager.reset_and_calculate();
// Infer gamma-ray spectra for recorded MC results
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_InitialStates);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_Histograms);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_EventCount);
cascadeMC_gammaSpectra.reset_and_calculate();
// Calculate total gamma-ray yield (cascade MC + tabulated results)
GA_AnnYield_General.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
GA_AnnYield_General.resolveDependency(&GA_SimYieldTable_DarkSUSY);
GA_AnnYield_General.resolveDependency(&DarkMatter_ID_MSSM);
GA_AnnYield_General.resolveDependency(&DarkMatterConj_ID_MSSM);
GA_AnnYield_General.resolveDependency(&cascadeMC_gammaSpectra);
GA_AnnYield_General.reset_and_calculate();
// Dump spectrum into file
dump_gammaSpectrum.resolveDependency(&GA_AnnYield_General);
dump_gammaSpectrum.setOption<std::string>("filename", current_backend + "_" + outname_dNdE_spectrum);
dump_gammaSpectrum.reset_and_calculate();
// Calculate Fermi LAT dwarf likelihood
lnL_FermiLATdwarfs_gamLike.resolveDependency(&GA_AnnYield_General);
lnL_FermiLATdwarfs_gamLike.resolveDependency(&RD_fraction_one);
lnL_FermiLATdwarfs_gamLike.resolveDependency(&DM_process_from_ProcessCatalog);
lnL_FermiLATdwarfs_gamLike.resolveBackendReq(&Backends::gamLike_1_0_1::Functown::lnL);
lnL_FermiLATdwarfs_gamLike.reset_and_calculate();
// Save the result
results["FermiLAT_dwarfsph_lnL"][current_backend] = lnL_FermiLATdwarfs_gamLike(0);
// ---- Direct detection and IceCube limits ----
// Calculate DD couplings with DarkSUSY
DD_couplings_DarkSUSY_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::DD_couplings);
DD_couplings_DarkSUSY_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::ddcomlegacy);
DD_couplings_DarkSUSY_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::ddmssmcom);
// The below calculates the DD couplings using the full 1 loop calculation of
// Drees Nojiri Phys.Rev. D48 (1993) 3483
DD_couplings_DarkSUSY_MSSM.setOption<bool>("loop", true);
// Setting the below to false approximates the squark propagator as 1/m_sq^2 to avoid poles.
DD_couplings_DarkSUSY_MSSM.setOption<bool>("pole", false);
DD_couplings_DarkSUSY_MSSM.reset_and_calculate();
// Calculate DD couplings for DDCalc
DDCalc_Couplings_WIMP_nucleon.resolveDependency(&DD_couplings_DarkSUSY_MSSM);
DDCalc_Couplings_WIMP_nucleon.reset_and_calculate();
// Initialize DDCalc backend
Backends::DDCalc_2_3_0::Functown::DDCalc_CalcRates_simple.setStatus(FunctorStatus::Active);
Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment.setStatus(FunctorStatus::Active);
Backends::DDCalc_2_3_0::Functown::DDCalc_LogLikelihood.setStatus(FunctorStatus::Active);
DDCalc_2_3_0_init.resolveDependency(&ExtractLocalMaxwellianHalo);
DDCalc_2_3_0_init.resolveDependency(&RD_fraction_one);
DDCalc_2_3_0_init.resolveDependency(&mwimp_generic);
DDCalc_2_3_0_init.resolveDependency(&DDCalc_Couplings_WIMP_nucleon);
DDCalc_2_3_0_init.reset_and_calculate();
// Calculate direct detection rates for LUX 2016
LUX_2016_Calc.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment);
LUX_2016_Calc.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_CalcRates_simple);
LUX_2016_Calc.reset_and_calculate();
// Calculate direct detection likelihood for LUX 2016
LUX_2016_GetLogLikelihood.resolveDependency(&LUX_2016_Calc);
LUX_2016_GetLogLikelihood.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment);
LUX_2016_GetLogLikelihood.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_LogLikelihood);
LUX_2016_GetLogLikelihood.reset_and_calculate();
// Save the result
results["LUX_2016_lnL"][current_backend] = LUX_2016_GetLogLikelihood(0);
sigma_SI_p_simple.resolveDependency(&mwimp_generic);
sigma_SI_p_simple.resolveDependency(&DD_couplings_DarkSUSY_MSSM);
sigma_SI_p_simple.reset_and_calculate();
// Save the result
results["sigma_SI_p"][current_backend] = sigma_SI_p_simple(0);
sigma_SD_p_simple.resolveDependency(&mwimp_generic);
sigma_SD_p_simple.resolveDependency(&DD_couplings_DarkSUSY_MSSM);
sigma_SD_p_simple.reset_and_calculate();
// Save the result
results["sigma_SD_p"][current_backend] = sigma_SD_p_simple(0);
// Infer WIMP capture rate in Sun
capture_rate_Sun_const_xsec.resolveDependency(&mwimp_generic);
capture_rate_Sun_const_xsec.resolveDependency(&sigma_SI_p_simple);
capture_rate_Sun_const_xsec.resolveDependency(&sigma_SD_p_simple);
capture_rate_Sun_const_xsec.resolveDependency(&RD_fraction_one);
capture_rate_Sun_const_xsec.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dssenu_capsuntab);
capture_rate_Sun_const_xsec.resolveDependency(&ExtractLocalMaxwellianHalo);
capture_rate_Sun_const_xsec.resolveDependency(&DarkSUSY_PointInit_LocalHalo_func);
capture_rate_Sun_const_xsec.reset_and_calculate();
// Infer WIMP equilibration time in Sun
equilibration_time_Sun.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
equilibration_time_Sun.resolveDependency(&DarkMatter_ID_MSSM);
equilibration_time_Sun.resolveDependency(&DarkMatterConj_ID_MSSM);
equilibration_time_Sun.resolveDependency(&mwimp_generic);
equilibration_time_Sun.resolveDependency(&capture_rate_Sun_const_xsec);
equilibration_time_Sun.reset_and_calculate();
// Infer WIMP annihilation rate in Sun
annihilation_rate_Sun.resolveDependency(&equilibration_time_Sun);
annihilation_rate_Sun.resolveDependency(&capture_rate_Sun_const_xsec);
annihilation_rate_Sun.reset_and_calculate();
// Infer neutrino yield from Sun
nuyield_from_DS.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
nuyield_from_DS.resolveDependency(&mwimp_generic);
nuyield_from_DS.resolveDependency(&sigmav_late_universe);
nuyield_from_DS.resolveDependency(&DarkMatter_ID_MSSM);
nuyield_from_DS.resolveDependency(&DarkMatterConj_ID_MSSM);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::dsgenericwimp_nusetup);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::neutrino_yield);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::DS_neutral_h_decay_channels);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_1_1::Functown::DS_charged_h_decay_channels);
nuyield_from_DS.reset_and_calculate();
// Calculate number of events at IceCube
IC79WH_full.resolveDependency(&mwimp_generic);
IC79WH_full.resolveDependency(&annihilation_rate_Sun);
IC79WH_full.resolveDependency(&nuyield_from_DS);
IC79WH_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79WH_full.reset_and_calculate();
IC79WL_full.resolveDependency(&mwimp_generic);
IC79WL_full.resolveDependency(&annihilation_rate_Sun);
IC79WL_full.resolveDependency(&nuyield_from_DS);
IC79WL_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79WL_full.reset_and_calculate();
IC79SL_full.resolveDependency(&mwimp_generic);
IC79SL_full.resolveDependency(&annihilation_rate_Sun);
IC79SL_full.resolveDependency(&nuyield_from_DS);
IC79SL_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79SL_full.reset_and_calculate();
// Calculate IceCube likelihood
IC79WH_bgloglike.resolveDependency(&IC79WH_full);
IC79WH_bgloglike.reset_and_calculate();
IC79WH_loglike.resolveDependency(&IC79WH_full);
IC79WH_loglike.reset_and_calculate();
IC79WL_bgloglike.resolveDependency(&IC79WL_full);
IC79WL_bgloglike.reset_and_calculate();
IC79WL_loglike.resolveDependency(&IC79WL_full);
IC79WL_loglike.reset_and_calculate();
IC79SL_bgloglike.resolveDependency(&IC79SL_full);
IC79SL_bgloglike.reset_and_calculate();
IC79SL_loglike.resolveDependency(&IC79SL_full);
IC79SL_loglike.reset_and_calculate();
IC79_loglike.resolveDependency(&IC79WH_bgloglike);
IC79_loglike.resolveDependency(&IC79WH_loglike);
IC79_loglike.resolveDependency(&IC79WL_bgloglike);
IC79_loglike.resolveDependency(&IC79WL_loglike);
IC79_loglike.resolveDependency(&IC79SL_bgloglike);
IC79_loglike.resolveDependency(&IC79SL_loglike);
IC79_loglike.reset_and_calculate();
// Save the result
results["IceCube_79_lnL"][current_backend] = IC79_loglike(0);
} // End of DarkSUSY_MSSM 6.1.1 calculations
//
// ======= Perform all calculations for backend DarkSUSY_MSSM 6.2.5 =======
//
current_backend = "DarkSUSY_MSSM6.2.5";
if (not Backends::backendInfo().works[current_backend])
{
backends_not_built.push_back(current_backend);
}
else
{
// Initialize DarkSUSY 6 MSSM backend
DarkSUSY_MSSM_6_2_5_init.notifyOfModel("MSSM30atQ");
DarkSUSY_MSSM_6_2_5_init.resolveDependency(&createSpectrum);
DarkSUSY_MSSM_6_2_5_init.resolveDependency(&createDecays);
if (decays) DarkSUSY_MSSM_6_2_5_init.setOption<bool>("use_dsSLHAread", false);
else DarkSUSY_MSSM_6_2_5_init.setOption<bool>("use_dsSLHAread", true);
DarkSUSY_MSSM_6_2_5_init.reset_and_calculate();
// Initialize DarkSUSY 6 Local Halo Model
DarkSUSY_PointInit_LocalHalo_func.resolveDependency(&ExtractLocalMaxwellianHalo);
DarkSUSY_PointInit_LocalHalo_func.resolveDependency(&RD_fraction_one);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dshmcom);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dshmisodf);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dshmframevelcom);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dshmnoclue);
DarkSUSY_PointInit_LocalHalo_func.reset_and_calculate();
// Relic density calculation with GAMBIT routines and DarkSUSY 6:
RD_spectrum_MSSM.resolveDependency(&createDecays);
RD_spectrum_MSSM.resolveDependency(&createSpectrum);
RD_spectrum_MSSM.resolveDependency(&DarkMatter_ID_MSSM);
// Below true if charginos and neutralinos are included in coannihilations:
RD_spectrum_MSSM.setOption<bool>("CoannCharginosNeutralinos", true);
// Below true if sfermions are included in coannihilations:
RD_spectrum_MSSM.setOption<bool>("CoannSfermions", true);
// Maximum sparticle mass to be icluded in coannihilations, in units of DM mass:
RD_spectrum_MSSM.setOption<double>("CoannMaxMass", 1.6);
RD_spectrum_MSSM.reset_and_calculate();
RD_spectrum_ordered_func.resolveDependency(&RD_spectrum_MSSM);
RD_spectrum_ordered_func.reset_and_calculate();
RD_annrate_DSprep_MSSM_func.resolveDependency(&RD_spectrum_ordered_func);
RD_annrate_DSprep_MSSM_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dsancoann);
RD_annrate_DSprep_MSSM_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::DSparticle_code);
RD_annrate_DSprep_MSSM_func.reset_and_calculate();
RD_eff_annrate_DS_MSSM.notifyOfModel("MSSM30atQ");
RD_eff_annrate_DS_MSSM.resolveDependency(&RD_annrate_DSprep_MSSM_func);
RD_eff_annrate_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dsanwx);
RD_eff_annrate_DS_MSSM.reset_and_calculate();
RD_oh2_DS6pre4_ini_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dsrdcom);
RD_oh2_DS6pre4_ini_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::rdpars);
RD_oh2_DS6pre4_ini_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::rdtime);
RD_oh2_DS6pre4_ini_func.setOption<int>("fast", 1); // 0: normal; 1: fast; 2: dirty
RD_oh2_DS6pre4_ini_func.reset_and_calculate();
RD_oh2_DS_general.resolveDependency(&RD_spectrum_ordered_func);
RD_oh2_DS_general.resolveDependency(&RD_eff_annrate_DS_MSSM);
RD_oh2_DS_general.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dsrdstart);
RD_oh2_DS_general.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dsrdens);
// Note that this one has to come *last* since it's a conditional dependency
RD_oh2_DS_general.resolveDependency(&RD_oh2_DS6pre4_ini_func);
RD_oh2_DS_general.reset_and_calculate();
// Save the result
results["oh2"][current_backend] = RD_oh2_DS_general(0);
lnL_oh2_Simple.resolveDependency(&RD_oh2_DS_general);
lnL_oh2_Simple.reset_and_calculate();
// Save the result
results["oh2_lnL"][current_backend] = lnL_oh2_Simple(0);
// Set up process catalog based on DarkSUSY annihilation rates
TH_ProcessCatalog_DS_MSSM.resolveDependency(&createSpectrum);
TH_ProcessCatalog_DS_MSSM.resolveDependency(&createDecays);
TH_ProcessCatalog_DS_MSSM.resolveDependency(&DarkMatter_ID_MSSM);
TH_ProcessCatalog_DS_MSSM.resolveDependency(&DarkMatterConj_ID_MSSM);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dssigmav0);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dssigmav0tot);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dsIBffdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dsIBhhdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dsIBwhdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dsIBwwdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::IBintvars);
TH_ProcessCatalog_DS_MSSM.reset_and_calculate();
// Set generic WIMP mass object
WIMP_properties.notifyOfModel("MSSM30atQ");
WIMP_properties.resolveDependency(&DarkMatter_ID_MSSM);
WIMP_properties.resolveDependency(&DarkMatterConj_ID_MSSM);
WIMP_properties.resolveDependency(&createSpectrum);
WIMP_properties.reset_and_calculate();
mwimp_generic.resolveDependency(&WIMP_properties);
mwimp_generic.reset_and_calculate();
// Set generic annihilation rate in late universe (v->0 limit)
sigmav_late_universe.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
sigmav_late_universe.resolveDependency(&DarkMatter_ID_MSSM);
sigmav_late_universe.resolveDependency(&DarkMatterConj_ID_MSSM);
sigmav_late_universe.reset_and_calculate();
// Save the result
results["sigmav0"][current_backend] = sigmav_late_universe(0);
// ---- Gamma-ray yields ----
// Initialize tabulated gamma-ray yields
GA_SimYieldTable_DarkSUSY.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dsanyield_sim);
GA_SimYieldTable_DarkSUSY.reset_and_calculate();
Combine_SimYields.resolveDependency(&GA_SimYieldTable_DarkSUSY);
// Here we need to establish the dependency chain from Combine_SimYields down to cascadeMC_gammaSpectra
// *before* Combine_SimYields runs in order for it to correctly realise that it needs to enable gammas.
cascadeMC_InitialStates.resolveDependency(&Combine_SimYields);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_InitialStates);
Combine_SimYields.reset_and_calculate();
// Identify process as annihilation rather than decay
DM_process_from_ProcessCatalog.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
DM_process_from_ProcessCatalog.resolveDependency(&DarkMatter_ID_MSSM);
DM_process_from_ProcessCatalog.reset_and_calculate();
// Set up initial states for cascade MC
cascadeMC_InitialStates.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_InitialStates.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
cascadeMC_InitialStates.resolveDependency(&DarkMatter_ID_MSSM);
cascadeMC_InitialStates.resolveDependency(&DarkMatterConj_ID_MSSM);
cascadeMC_InitialStates.resolveDependency(&DM_process_from_ProcessCatalog);
cascadeMC_InitialStates.reset_and_calculate();
// Infer for which type of final states particles MC should be performed
cascadeMC_FinalStates.setOption<std::vector<std::string>>("cMC_finalStates", daFunk::vec<std::string>("gamma"));
// Here we need to establish the dependency chain from cascadeMC_FinalStates down to cascadeMC_gammaSpectra
// *before* cascadeMC_FinalStates runs in order for it to correctly realise that it needs to enable gammas.
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_FinalStates.reset_and_calculate();
// Collect decay information for cascade MC
cascadeMC_DecayTable.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
cascadeMC_DecayTable.resolveDependency(&Combine_SimYields);
cascadeMC_DecayTable.reset_and_calculate();
// Set up MC loop manager for cascade MC
cascadeMC_LoopManager.resolveDependency(&cascadeMC_InitialStates);
std::vector<functor*> nested_functions = initVector<functor*>(
&cascadeMC_GenerateChain, &cascadeMC_Histograms, &cascadeMC_EventCount);
cascadeMC_LoopManager.setNestedList(nested_functions);
// Perform MC step for cascade MC
cascadeMC_GenerateChain.resolveDependency(&cascadeMC_DecayTable);
cascadeMC_GenerateChain.resolveLoopManager(&cascadeMC_LoopManager);
// Generate histogram for cascade MC
cascadeMC_Histograms.resolveDependency(&cascadeMC_GenerateChain);
cascadeMC_Histograms.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
cascadeMC_Histograms.resolveDependency(&Combine_SimYields);
cascadeMC_Histograms.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_Histograms.resolveLoopManager(&cascadeMC_LoopManager);
// Check convergence of cascade MC
cascadeMC_EventCount.resolveLoopManager(&cascadeMC_LoopManager);
// Start cascade MC loop
cascadeMC_LoopManager.reset_and_calculate();
// Infer gamma-ray spectra for recorded MC results
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_InitialStates);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_Histograms);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_EventCount);
cascadeMC_gammaSpectra.reset_and_calculate();
// Calculate total gamma-ray yield (cascade MC + tabulated results)
GA_AnnYield_General.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
GA_AnnYield_General.resolveDependency(&GA_SimYieldTable_DarkSUSY);
GA_AnnYield_General.resolveDependency(&DarkMatter_ID_MSSM);
GA_AnnYield_General.resolveDependency(&DarkMatterConj_ID_MSSM);
GA_AnnYield_General.resolveDependency(&cascadeMC_gammaSpectra);
GA_AnnYield_General.reset_and_calculate();
// Dump spectrum into file
dump_gammaSpectrum.resolveDependency(&GA_AnnYield_General);
dump_gammaSpectrum.setOption<std::string>("filename", current_backend + "_" + outname_dNdE_spectrum);
dump_gammaSpectrum.reset_and_calculate();
// Calculate Fermi LAT dwarf likelihood
lnL_FermiLATdwarfs_gamLike.resolveDependency(&GA_AnnYield_General);
lnL_FermiLATdwarfs_gamLike.resolveDependency(&RD_fraction_one);
lnL_FermiLATdwarfs_gamLike.resolveDependency(&DM_process_from_ProcessCatalog);
lnL_FermiLATdwarfs_gamLike.resolveBackendReq(&Backends::gamLike_1_0_1::Functown::lnL);
lnL_FermiLATdwarfs_gamLike.reset_and_calculate();
// Save the result
results["FermiLAT_dwarfsph_lnL"][current_backend] = lnL_FermiLATdwarfs_gamLike(0);
// ---- Direct detection and IceCube limits ----
// Calculate DD couplings with DarkSUSY
DD_couplings_DarkSUSY_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::DD_couplings);
DD_couplings_DarkSUSY_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::ddcomlegacy);
DD_couplings_DarkSUSY_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::ddmssmcom);
// The below calculates the DD couplings using the full 1 loop calculation of
// Drees Nojiri Phys.Rev. D48 (1993) 3483
DD_couplings_DarkSUSY_MSSM.setOption<bool>("loop", true);
// Setting the below to false approximates the squark propagator as 1/m_sq^2 to avoid poles.
DD_couplings_DarkSUSY_MSSM.setOption<bool>("pole", false);
DD_couplings_DarkSUSY_MSSM.reset_and_calculate();
// Calculate DD couplings for DDCalc
DDCalc_Couplings_WIMP_nucleon.resolveDependency(&DD_couplings_DarkSUSY_MSSM);
DDCalc_Couplings_WIMP_nucleon.reset_and_calculate();
// Initialize DDCalc backend
Backends::DDCalc_2_3_0::Functown::DDCalc_CalcRates_simple.setStatus(FunctorStatus::Active);
Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment.setStatus(FunctorStatus::Active);
Backends::DDCalc_2_3_0::Functown::DDCalc_LogLikelihood.setStatus(FunctorStatus::Active);
DDCalc_2_3_0_init.resolveDependency(&ExtractLocalMaxwellianHalo);
DDCalc_2_3_0_init.resolveDependency(&RD_fraction_one);
DDCalc_2_3_0_init.resolveDependency(&mwimp_generic);
DDCalc_2_3_0_init.resolveDependency(&DDCalc_Couplings_WIMP_nucleon);
DDCalc_2_3_0_init.reset_and_calculate();
// Calculate direct detection rates for LUX 2016
LUX_2016_Calc.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment);
LUX_2016_Calc.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_CalcRates_simple);
LUX_2016_Calc.reset_and_calculate();
// Calculate direct detection likelihood for LUX 2016
LUX_2016_GetLogLikelihood.resolveDependency(&LUX_2016_Calc);
LUX_2016_GetLogLikelihood.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment);
LUX_2016_GetLogLikelihood.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_LogLikelihood);
LUX_2016_GetLogLikelihood.reset_and_calculate();
// Save the result
results["LUX_2016_lnL"][current_backend] = LUX_2016_GetLogLikelihood(0);
sigma_SI_p_simple.resolveDependency(&mwimp_generic);
sigma_SI_p_simple.resolveDependency(&DD_couplings_DarkSUSY_MSSM);
sigma_SI_p_simple.reset_and_calculate();
// Save the result
results["sigma_SI_p"][current_backend] = sigma_SI_p_simple(0);
sigma_SD_p_simple.resolveDependency(&mwimp_generic);
sigma_SD_p_simple.resolveDependency(&DD_couplings_DarkSUSY_MSSM);
sigma_SD_p_simple.reset_and_calculate();
// Save the result
results["sigma_SD_p"][current_backend] = sigma_SD_p_simple(0);
// Infer WIMP capture rate in Sun
capture_rate_Sun_const_xsec.resolveDependency(&mwimp_generic);
capture_rate_Sun_const_xsec.resolveDependency(&sigma_SI_p_simple);
capture_rate_Sun_const_xsec.resolveDependency(&sigma_SD_p_simple);
capture_rate_Sun_const_xsec.resolveDependency(&RD_fraction_one);
capture_rate_Sun_const_xsec.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dssenu_capsuntab);
capture_rate_Sun_const_xsec.resolveDependency(&ExtractLocalMaxwellianHalo);
capture_rate_Sun_const_xsec.resolveDependency(&DarkSUSY_PointInit_LocalHalo_func);
capture_rate_Sun_const_xsec.reset_and_calculate();
// Infer WIMP equilibration time in Sun
equilibration_time_Sun.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
equilibration_time_Sun.resolveDependency(&DarkMatter_ID_MSSM);
equilibration_time_Sun.resolveDependency(&DarkMatterConj_ID_MSSM);
equilibration_time_Sun.resolveDependency(&mwimp_generic);
equilibration_time_Sun.resolveDependency(&capture_rate_Sun_const_xsec);
equilibration_time_Sun.reset_and_calculate();
// Infer WIMP annihilation rate in Sun
annihilation_rate_Sun.resolveDependency(&equilibration_time_Sun);
annihilation_rate_Sun.resolveDependency(&capture_rate_Sun_const_xsec);
annihilation_rate_Sun.reset_and_calculate();
// Infer neutrino yield from Sun
nuyield_from_DS.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
nuyield_from_DS.resolveDependency(&mwimp_generic);
nuyield_from_DS.resolveDependency(&sigmav_late_universe);
nuyield_from_DS.resolveDependency(&DarkMatter_ID_MSSM);
nuyield_from_DS.resolveDependency(&DarkMatterConj_ID_MSSM);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::dsgenericwimp_nusetup);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::neutrino_yield);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::DS_neutral_h_decay_channels);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_2_5::Functown::DS_charged_h_decay_channels);
nuyield_from_DS.reset_and_calculate();
// Calculate number of events at IceCube
IC79WH_full.resolveDependency(&mwimp_generic);
IC79WH_full.resolveDependency(&annihilation_rate_Sun);
IC79WH_full.resolveDependency(&nuyield_from_DS);
IC79WH_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79WH_full.reset_and_calculate();
IC79WL_full.resolveDependency(&mwimp_generic);
IC79WL_full.resolveDependency(&annihilation_rate_Sun);
IC79WL_full.resolveDependency(&nuyield_from_DS);
IC79WL_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79WL_full.reset_and_calculate();
IC79SL_full.resolveDependency(&mwimp_generic);
IC79SL_full.resolveDependency(&annihilation_rate_Sun);
IC79SL_full.resolveDependency(&nuyield_from_DS);
IC79SL_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79SL_full.reset_and_calculate();
// Calculate IceCube likelihood
IC79WH_bgloglike.resolveDependency(&IC79WH_full);
IC79WH_bgloglike.reset_and_calculate();
IC79WH_loglike.resolveDependency(&IC79WH_full);
IC79WH_loglike.reset_and_calculate();
IC79WL_bgloglike.resolveDependency(&IC79WL_full);
IC79WL_bgloglike.reset_and_calculate();
IC79WL_loglike.resolveDependency(&IC79WL_full);
IC79WL_loglike.reset_and_calculate();
IC79SL_bgloglike.resolveDependency(&IC79SL_full);
IC79SL_bgloglike.reset_and_calculate();
IC79SL_loglike.resolveDependency(&IC79SL_full);
IC79SL_loglike.reset_and_calculate();
IC79_loglike.resolveDependency(&IC79WH_bgloglike);
IC79_loglike.resolveDependency(&IC79WH_loglike);
IC79_loglike.resolveDependency(&IC79WL_bgloglike);
IC79_loglike.resolveDependency(&IC79WL_loglike);
IC79_loglike.resolveDependency(&IC79SL_bgloglike);
IC79_loglike.resolveDependency(&IC79SL_loglike);
IC79_loglike.reset_and_calculate();
// Save the result
results["IceCube_79_lnL"][current_backend] = IC79_loglike(0);
} // End of DarkSUSY_MSSM 6.2.5 calculations
//
// ======= Perform all calculations for backend DarkSUSY_MSSM 6.4.0 =======
//
current_backend = "DarkSUSY_MSSM6.4.0";
if (not Backends::backendInfo().works[current_backend])
{
backends_not_built.push_back(current_backend);
}
else
{
// Initialize DarkSUSY 6 MSSM backend
DarkSUSY_MSSM_6_4_0_init.notifyOfModel("MSSM30atQ");
DarkSUSY_MSSM_6_4_0_init.resolveDependency(&createSpectrum);
DarkSUSY_MSSM_6_4_0_init.resolveDependency(&createDecays);
if (decays) DarkSUSY_MSSM_6_4_0_init.setOption<bool>("use_dsSLHAread", false);
else DarkSUSY_MSSM_6_4_0_init.setOption<bool>("use_dsSLHAread", true);
DarkSUSY_MSSM_6_4_0_init.reset_and_calculate();
// Initialize DarkSUSY 6 Local Halo Model
DarkSUSY_PointInit_LocalHalo_func.resolveDependency(&ExtractLocalMaxwellianHalo);
DarkSUSY_PointInit_LocalHalo_func.resolveDependency(&RD_fraction_one);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dshmcom);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dshmisodf);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dshmframevelcom);
DarkSUSY_PointInit_LocalHalo_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dshmnoclue);
DarkSUSY_PointInit_LocalHalo_func.reset_and_calculate();
// Relic density calculation with GAMBIT routines and DarkSUSY 6:
RD_spectrum_MSSM.resolveDependency(&createDecays);
RD_spectrum_MSSM.resolveDependency(&createSpectrum);
RD_spectrum_MSSM.resolveDependency(&DarkMatter_ID_MSSM);
// Below true if charginos and neutralinos are included in coannihilations:
RD_spectrum_MSSM.setOption<bool>("CoannCharginosNeutralinos", true);
// Below true if sfermions are included in coannihilations:
RD_spectrum_MSSM.setOption<bool>("CoannSfermions", true);
// Maximum sparticle mass to be icluded in coannihilations, in units of DM mass:
RD_spectrum_MSSM.setOption<double>("CoannMaxMass", 1.6);
RD_spectrum_MSSM.reset_and_calculate();
RD_spectrum_ordered_func.resolveDependency(&RD_spectrum_MSSM);
RD_spectrum_ordered_func.reset_and_calculate();
RD_annrate_DSprep_MSSM_func.resolveDependency(&RD_spectrum_ordered_func);
RD_annrate_DSprep_MSSM_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dsancoann);
RD_annrate_DSprep_MSSM_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::DSparticle_code);
RD_annrate_DSprep_MSSM_func.reset_and_calculate();
RD_eff_annrate_DS_MSSM.notifyOfModel("MSSM30atQ");
RD_eff_annrate_DS_MSSM.resolveDependency(&RD_annrate_DSprep_MSSM_func);
RD_eff_annrate_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dsanwx);
RD_eff_annrate_DS_MSSM.reset_and_calculate();
RD_oh2_DS6_ini_func.resolveDependency(&RD_spectrum_ordered_func);
RD_oh2_DS6_ini_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::rdpars);
RD_oh2_DS6_ini_func.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::rdtime);
RD_oh2_DS6_ini_func.setOption<int>("fast", 1); // 0: normal; 1: fast; 2: dirty
RD_oh2_DS6_ini_func.reset_and_calculate();
RD_oh2_DS_general.resolveDependency(&RD_spectrum_ordered_func);
RD_oh2_DS_general.resolveDependency(&RD_eff_annrate_DS_MSSM);
RD_oh2_DS_general.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dsrdstart);
RD_oh2_DS_general.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dsrdens);
// Note that this one has to come *last* since it's a conditional dependency
RD_oh2_DS_general.resolveDependency(&RD_oh2_DS6_ini_func);
RD_oh2_DS_general.reset_and_calculate();
// Save the result
results["oh2"][current_backend] = RD_oh2_DS_general(0);
lnL_oh2_Simple.resolveDependency(&RD_oh2_DS_general);
lnL_oh2_Simple.reset_and_calculate();
// Save the result
results["oh2_lnL"][current_backend] = lnL_oh2_Simple(0);
// Set up process catalog based on DarkSUSY annihilation rates
TH_ProcessCatalog_DS_MSSM.resolveDependency(&createSpectrum);
TH_ProcessCatalog_DS_MSSM.resolveDependency(&createDecays);
TH_ProcessCatalog_DS_MSSM.resolveDependency(&DarkMatter_ID_MSSM);
TH_ProcessCatalog_DS_MSSM.resolveDependency(&DarkMatterConj_ID_MSSM);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dssigmav0);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dssigmav0tot);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dsIBffdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dsIBhhdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dsIBwhdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dsIBwwdxdy);
TH_ProcessCatalog_DS_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::IBintvars);
TH_ProcessCatalog_DS_MSSM.reset_and_calculate();
// Set generic WIMP mass object
WIMP_properties.notifyOfModel("MSSM30atQ");
WIMP_properties.resolveDependency(&DarkMatter_ID_MSSM);
WIMP_properties.resolveDependency(&DarkMatterConj_ID_MSSM);
WIMP_properties.resolveDependency(&createSpectrum);
WIMP_properties.reset_and_calculate();
mwimp_generic.resolveDependency(&WIMP_properties);
mwimp_generic.reset_and_calculate();
// Set generic annihilation rate in late universe (v->0 limit)
sigmav_late_universe.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
sigmav_late_universe.resolveDependency(&DarkMatter_ID_MSSM);
sigmav_late_universe.resolveDependency(&DarkMatterConj_ID_MSSM);
sigmav_late_universe.reset_and_calculate();
// Save the result
results["sigmav0"][current_backend] = sigmav_late_universe(0);
// ---- Gamma-ray yields ----
// Initialize tabulated gamma-ray yields
GA_SimYieldTable_DarkSUSY.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dsanyield_sim);
GA_SimYieldTable_DarkSUSY.reset_and_calculate();
Combine_SimYields.resolveDependency(&GA_SimYieldTable_DarkSUSY);
// Here we need to establish the dependency chain from Combine_SimYields down to cascadeMC_gammaSpectra
// *before* Combine_SimYields runs in order for it to correctly realise that it needs to enable gammas.
cascadeMC_InitialStates.resolveDependency(&Combine_SimYields);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_InitialStates);
Combine_SimYields.reset_and_calculate();
// Identify process as annihilation rather than decay
DM_process_from_ProcessCatalog.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
DM_process_from_ProcessCatalog.resolveDependency(&DarkMatter_ID_MSSM);
DM_process_from_ProcessCatalog.reset_and_calculate();
// Set up initial states for cascade MC
cascadeMC_InitialStates.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_InitialStates.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
cascadeMC_InitialStates.resolveDependency(&DarkMatter_ID_MSSM);
cascadeMC_InitialStates.resolveDependency(&DarkMatterConj_ID_MSSM);
cascadeMC_InitialStates.resolveDependency(&DM_process_from_ProcessCatalog);
cascadeMC_InitialStates.reset_and_calculate();
// Infer for which type of final states particles MC should be performed
cascadeMC_FinalStates.setOption<std::vector<std::string>>("cMC_finalStates", daFunk::vec<std::string>("gamma"));
// Here we need to establish the dependency chain from cascadeMC_FinalStates down to cascadeMC_gammaSpectra
// *before* cascadeMC_FinalStates runs in order for it to correctly realise that it needs to enable gammas.
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_FinalStates.reset_and_calculate();
// Collect decay information for cascade MC
cascadeMC_DecayTable.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
cascadeMC_DecayTable.resolveDependency(&Combine_SimYields);
cascadeMC_DecayTable.reset_and_calculate();
// Set up MC loop manager for cascade MC
cascadeMC_LoopManager.resolveDependency(&cascadeMC_InitialStates);
std::vector<functor*> nested_functions = initVector<functor*>(
&cascadeMC_GenerateChain, &cascadeMC_Histograms, &cascadeMC_EventCount);
cascadeMC_LoopManager.setNestedList(nested_functions);
// Perform MC step for cascade MC
cascadeMC_GenerateChain.resolveDependency(&cascadeMC_DecayTable);
cascadeMC_GenerateChain.resolveLoopManager(&cascadeMC_LoopManager);
// Generate histogram for cascade MC
cascadeMC_Histograms.resolveDependency(&cascadeMC_GenerateChain);
cascadeMC_Histograms.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
cascadeMC_Histograms.resolveDependency(&Combine_SimYields);
cascadeMC_Histograms.resolveDependency(&cascadeMC_FinalStates);
cascadeMC_Histograms.resolveLoopManager(&cascadeMC_LoopManager);
// Check convergence of cascade MC
cascadeMC_EventCount.resolveLoopManager(&cascadeMC_LoopManager);
// Start cascade MC loop
cascadeMC_LoopManager.reset_and_calculate();
// Infer gamma-ray spectra for recorded MC results
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_InitialStates);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_Histograms);
cascadeMC_gammaSpectra.resolveDependency(&cascadeMC_EventCount);
cascadeMC_gammaSpectra.reset_and_calculate();
// Calculate total gamma-ray yield (cascade MC + tabulated results)
GA_AnnYield_General.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
GA_AnnYield_General.resolveDependency(&GA_SimYieldTable_DarkSUSY);
GA_AnnYield_General.resolveDependency(&DarkMatter_ID_MSSM);
GA_AnnYield_General.resolveDependency(&DarkMatterConj_ID_MSSM);
GA_AnnYield_General.resolveDependency(&cascadeMC_gammaSpectra);
GA_AnnYield_General.reset_and_calculate();
// Dump spectrum into file
dump_gammaSpectrum.resolveDependency(&GA_AnnYield_General);
dump_gammaSpectrum.setOption<std::string>("filename", current_backend + "_" + outname_dNdE_spectrum);
dump_gammaSpectrum.reset_and_calculate();
// Calculate Fermi LAT dwarf likelihood
lnL_FermiLATdwarfs_gamLike.resolveDependency(&GA_AnnYield_General);
lnL_FermiLATdwarfs_gamLike.resolveDependency(&RD_fraction_one);
lnL_FermiLATdwarfs_gamLike.resolveDependency(&DM_process_from_ProcessCatalog);
lnL_FermiLATdwarfs_gamLike.resolveBackendReq(&Backends::gamLike_1_0_1::Functown::lnL);
lnL_FermiLATdwarfs_gamLike.reset_and_calculate();
// Save the result
results["FermiLAT_dwarfsph_lnL"][current_backend] = lnL_FermiLATdwarfs_gamLike(0);
// ---- Direct detection and IceCube limits ----
// Calculate DD couplings with DarkSUSY
DD_couplings_DarkSUSY_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::DD_couplings);
DD_couplings_DarkSUSY_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::ddcomlegacy);
DD_couplings_DarkSUSY_MSSM.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::ddmssmcom);
// The below calculates the DD couplings using the full 1 loop calculation of
// Drees Nojiri Phys.Rev. D48 (1993) 3483
DD_couplings_DarkSUSY_MSSM.setOption<bool>("loop", true);
// Setting the below to false approximates the squark propagator as 1/m_sq^2 to avoid poles.
DD_couplings_DarkSUSY_MSSM.setOption<bool>("pole", false);
DD_couplings_DarkSUSY_MSSM.reset_and_calculate();
// Calculate DD couplings for DDCalc
DDCalc_Couplings_WIMP_nucleon.resolveDependency(&DD_couplings_DarkSUSY_MSSM);
DDCalc_Couplings_WIMP_nucleon.reset_and_calculate();
// Initialize DDCalc backend
Backends::DDCalc_2_3_0::Functown::DDCalc_CalcRates_simple.setStatus(FunctorStatus::Active);
Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment.setStatus(FunctorStatus::Active);
Backends::DDCalc_2_3_0::Functown::DDCalc_LogLikelihood.setStatus(FunctorStatus::Active);
DDCalc_2_3_0_init.resolveDependency(&ExtractLocalMaxwellianHalo);
DDCalc_2_3_0_init.resolveDependency(&RD_fraction_one);
DDCalc_2_3_0_init.resolveDependency(&mwimp_generic);
DDCalc_2_3_0_init.resolveDependency(&DDCalc_Couplings_WIMP_nucleon);
DDCalc_2_3_0_init.reset_and_calculate();
// Calculate direct detection rates for LUX 2016
LUX_2016_Calc.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment);
LUX_2016_Calc.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_CalcRates_simple);
LUX_2016_Calc.reset_and_calculate();
// Calculate direct detection likelihood for LUX 2016
LUX_2016_GetLogLikelihood.resolveDependency(&LUX_2016_Calc);
LUX_2016_GetLogLikelihood.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment);
LUX_2016_GetLogLikelihood.resolveBackendReq(&Backends::DDCalc_2_3_0::Functown::DDCalc_LogLikelihood);
LUX_2016_GetLogLikelihood.reset_and_calculate();
// Save the result
results["LUX_2016_lnL"][current_backend] = LUX_2016_GetLogLikelihood(0);
sigma_SI_p_simple.resolveDependency(&mwimp_generic);
sigma_SI_p_simple.resolveDependency(&DD_couplings_DarkSUSY_MSSM);
sigma_SI_p_simple.reset_and_calculate();
// Save the result
results["sigma_SI_p"][current_backend] = sigma_SI_p_simple(0);
sigma_SD_p_simple.resolveDependency(&mwimp_generic);
sigma_SD_p_simple.resolveDependency(&DD_couplings_DarkSUSY_MSSM);
sigma_SD_p_simple.reset_and_calculate();
// Save the result
results["sigma_SD_p"][current_backend] = sigma_SD_p_simple(0);
// Infer WIMP capture rate in Sun
capture_rate_Sun_const_xsec.resolveDependency(&mwimp_generic);
capture_rate_Sun_const_xsec.resolveDependency(&sigma_SI_p_simple);
capture_rate_Sun_const_xsec.resolveDependency(&sigma_SD_p_simple);
capture_rate_Sun_const_xsec.resolveDependency(&RD_fraction_one);
capture_rate_Sun_const_xsec.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dssenu_capsuntab);
capture_rate_Sun_const_xsec.resolveDependency(&ExtractLocalMaxwellianHalo);
capture_rate_Sun_const_xsec.resolveDependency(&DarkSUSY_PointInit_LocalHalo_func);
capture_rate_Sun_const_xsec.reset_and_calculate();
// Infer WIMP equilibration time in Sun
equilibration_time_Sun.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
equilibration_time_Sun.resolveDependency(&DarkMatter_ID_MSSM);
equilibration_time_Sun.resolveDependency(&DarkMatterConj_ID_MSSM);
equilibration_time_Sun.resolveDependency(&mwimp_generic);
equilibration_time_Sun.resolveDependency(&capture_rate_Sun_const_xsec);
equilibration_time_Sun.reset_and_calculate();
// Infer WIMP annihilation rate in Sun
annihilation_rate_Sun.resolveDependency(&equilibration_time_Sun);
annihilation_rate_Sun.resolveDependency(&capture_rate_Sun_const_xsec);
annihilation_rate_Sun.reset_and_calculate();
// Infer neutrino yield from Sun
nuyield_from_DS.resolveDependency(&TH_ProcessCatalog_DS_MSSM);
nuyield_from_DS.resolveDependency(&mwimp_generic);
nuyield_from_DS.resolveDependency(&sigmav_late_universe);
nuyield_from_DS.resolveDependency(&DarkMatter_ID_MSSM);
nuyield_from_DS.resolveDependency(&DarkMatterConj_ID_MSSM);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::dsgenericwimp_nusetup);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::neutrino_yield);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::DS_neutral_h_decay_channels);
nuyield_from_DS.resolveBackendReq(&Backends::DarkSUSY_MSSM_6_4_0::Functown::DS_charged_h_decay_channels);
nuyield_from_DS.reset_and_calculate();
// Calculate number of events at IceCube
IC79WH_full.resolveDependency(&mwimp_generic);
IC79WH_full.resolveDependency(&annihilation_rate_Sun);
IC79WH_full.resolveDependency(&nuyield_from_DS);
IC79WH_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79WH_full.reset_and_calculate();
IC79WL_full.resolveDependency(&mwimp_generic);
IC79WL_full.resolveDependency(&annihilation_rate_Sun);
IC79WL_full.resolveDependency(&nuyield_from_DS);
IC79WL_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79WL_full.reset_and_calculate();
IC79SL_full.resolveDependency(&mwimp_generic);
IC79SL_full.resolveDependency(&annihilation_rate_Sun);
IC79SL_full.resolveDependency(&nuyield_from_DS);
IC79SL_full.resolveBackendReq(&Backends::nulike_1_0_9::Functown::nulike_bounds);
IC79SL_full.reset_and_calculate();
// Calculate IceCube likelihood
IC79WH_bgloglike.resolveDependency(&IC79WH_full);
IC79WH_bgloglike.reset_and_calculate();
IC79WH_loglike.resolveDependency(&IC79WH_full);
IC79WH_loglike.reset_and_calculate();
IC79WL_bgloglike.resolveDependency(&IC79WL_full);
IC79WL_bgloglike.reset_and_calculate();
IC79WL_loglike.resolveDependency(&IC79WL_full);
IC79WL_loglike.reset_and_calculate();
IC79SL_bgloglike.resolveDependency(&IC79SL_full);
IC79SL_bgloglike.reset_and_calculate();
IC79SL_loglike.resolveDependency(&IC79SL_full);
IC79SL_loglike.reset_and_calculate();
IC79_loglike.resolveDependency(&IC79WH_bgloglike);
IC79_loglike.resolveDependency(&IC79WH_loglike);
IC79_loglike.resolveDependency(&IC79WL_bgloglike);
IC79_loglike.resolveDependency(&IC79WL_loglike);
IC79_loglike.resolveDependency(&IC79SL_bgloglike);
IC79_loglike.resolveDependency(&IC79SL_loglike);
IC79_loglike.reset_and_calculate();
// Save the result
results["IceCube_79_lnL"][current_backend] = IC79_loglike(0);
} // End of DarkSUSY_MSSM 6.4.0 calculations
//
// ======= Perform all calculations for backend MicrOmegas_MSSM 3.6.9.2 =======
//
current_backend = "MicrOmegas_MSSM3.6.9.2";
if (not Backends::backendInfo().works[current_backend])
{
backends_not_built.push_back(current_backend);
}
else
{
// Initialize MicrOmegas backend
MicrOmegas_MSSM_3_6_9_2_init.notifyOfModel("MSSM30atQ");
MicrOmegas_MSSM_3_6_9_2_init.resolveDependency(&createSpectrum);
MicrOmegas_MSSM_3_6_9_2_init.resolveDependency(&createDecays);
MicrOmegas_MSSM_3_6_9_2_init.resolveDependency(&createSLHA1Names);
// Use decay table if it is present:
if (decays) MicrOmegas_MSSM_3_6_9_2_init.setOption<bool>("internal_decays", false);
else MicrOmegas_MSSM_3_6_9_2_init.setOption<bool>("internal_decays", true);
MicrOmegas_MSSM_3_6_9_2_init.reset_and_calculate();
// For the below VXdecay = 0 - no 3 body final states via virtual X
// 1 - annihilations to 3 body final states via virtual X
// 2 - (co)annihilations to 3 body final states via virtual X
MicrOmegas_MSSM_3_6_9_2_init.setOption<int>("VZdecay", 0);
MicrOmegas_MSSM_3_6_9_2_init.setOption<int>("VWdecay", 0);
MicrOmegas_MSSM_3_6_9_2_init.reset_and_calculate();
// Relic density calculation with MicrOmegas
RD_oh2_Xf_MicrOmegas.notifyOfModel("MSSM30atQ");
RD_oh2_Xf_MicrOmegas.resolveBackendReq(&Backends::MicrOmegas_MSSM_3_6_9_2::Functown::darkOmega);
RD_oh2_Xf_MicrOmegas.setOption<int>("fast", 1); // 0: accurate; 1: fast
RD_oh2_Xf_MicrOmegas.setOption<double>("Beps", 1e-5); // Beps=1e-5 recommended, Beps=1 switches coannihilation off
RD_oh2_Xf_MicrOmegas.reset_and_calculate();
RD_oh2_MicrOmegas.resolveDependency(&RD_oh2_Xf_MicrOmegas);
RD_oh2_MicrOmegas.reset_and_calculate();
// Save the result
results["oh2"][current_backend] = RD_oh2_MicrOmegas(0);
lnL_oh2_Simple.resolveDependency(&RD_oh2_MicrOmegas);
lnL_oh2_Simple.reset_and_calculate();
// Save the result
results["oh2_lnL"][current_backend] = lnL_oh2_Simple(0);
// <sigma v> (v->0 limit) self-annihilation calculation with MicrOmegas:
sigmav_late_universe_MicrOmegas.notifyOfModel("MSSM30atQ");
sigmav_late_universe_MicrOmegas.resolveBackendReq(&Backends::MicrOmegas_MSSM_3_6_9_2::Functown::calcSpectrum);
sigmav_late_universe_MicrOmegas.reset_and_calculate();
results["sigmav0"][current_backend] = sigmav_late_universe_MicrOmegas(0);
// Direct detection calculations with Micromegas
// Calculate DD couplings with Micromegas
// DD_couplings_MicrOmegas.notifyOfModel("MSSM30atQ");
// DD_couplings_MicrOmegas.notifyOfModel("nuclear_params_fnq");
// DD_couplings_MicrOmegas.resolveDependency(&Models::nuclear_params_fnq::Functown::primary_parameters);
DD_couplings_MicrOmegas.resolveBackendReq(&Backends::MicrOmegas_MSSM_3_6_9_2::Functown::nucleonAmplitudes);
DD_couplings_MicrOmegas.resolveBackendReq(&Backends::MicrOmegas_MSSM_3_6_9_2::Functown::FeScLoop);
DD_couplings_MicrOmegas.resolveBackendReq(&Backends::MicrOmegas_MSSM_3_6_9_2::Functown::mocommon_);
// The below includes neutralino-gluon scattering via a box diagram
DD_couplings_MicrOmegas.setOption<bool>("box", true);
DD_couplings_MicrOmegas.reset_and_calculate();
// Calculate DD couplings for DDCalc
DDCalc_Couplings_WIMP_nucleon.resolveDependency(&DD_couplings_MicrOmegas);
DDCalc_Couplings_WIMP_nucleon.reset_and_calculate();
// Set generic WIMP mass object
WIMP_properties.notifyOfModel("MSSM30atQ");
WIMP_properties.resolveDependency(&DarkMatter_ID_MSSM);
WIMP_properties.resolveDependency(&DarkMatterConj_ID_MSSM);
WIMP_properties.resolveDependency(&createSpectrum);
WIMP_properties.reset_and_calculate();
mwimp_generic.resolveDependency(&WIMP_properties);
mwimp_generic.reset_and_calculate();
// Initialize DDCalc backend
Backends::DDCalc_2_3_0::Functown::DDCalc_CalcRates_simple.setStatus(FunctorStatus::Active);
Backends::DDCalc_2_3_0::Functown::DDCalc_Experiment.setStatus(FunctorStatus::Active);
Backends::DDCalc_2_3_0::Functown::DDCalc_LogLikelihood.setStatus(FunctorStatus::Active);
DDCalc_2_3_0_init.resolveDependency(&ExtractLocalMaxwellianHalo);
DDCalc_2_3_0_init.resolveDependency(&RD_fraction_one);
DDCalc_2_3_0_init.resolveDependency(&mwimp_generic);
DDCalc_2_3_0_init.resolveDependency(&DDCalc_Couplings_WIMP_nucleon);
DDCalc_2_3_0_init.reset_and_calculate();
sigma_SI_p_simple.resolveDependency(&mwimp_generic);
sigma_SI_p_simple.resolveDependency(&DD_couplings_MicrOmegas);
sigma_SI_p_simple.reset_and_calculate();
// Save the result
results["sigma_SI_p"][current_backend] = sigma_SI_p_simple(0);
sigma_SD_p_simple.resolveDependency(&mwimp_generic);
sigma_SD_p_simple.resolveDependency(&DD_couplings_MicrOmegas);
sigma_SD_p_simple.reset_and_calculate();
// Save the result
results["sigma_SD_p"][current_backend] = sigma_SD_p_simple(0);
} // End of MicrOmegas_MSSM 3.6.9.2 calculations
//
// ======= Construct the output string =======
//
std::stringstream results_ss;
for(const std::string& result_key : result_output_order)
{
const std::map<std::string,double>& backends_result_map = results.at(result_key);
results_ss << result_key;
if (results_units.at(result_key) != "") { results_ss << " [" << results_units.at(result_key) << "]"; }
results_ss << " :" << endl;
for(const auto& kv : backends_result_map)
{
const std::string& backendname = kv.first;
const double& result = kv.second;
results_ss << " " << backendname << ": " << result << " " << results_units.at(result_key) << endl;
}
results_ss << endl;
}
//
// ======= Output the result string to screen =======
//
cout << endl;
cout << "==== RESULTS ====" << endl;
cout << endl;
cout << results_ss.str();
cout << endl;
// Let the user know what they are missing...
if (backends_not_built.size() > 0)
{
cout << endl;
cout << "NOTE: The following backend(s) are not present:" << endl;
for (const std::string& backend_name : backends_not_built)
{
cout << " - " << backend_name << endl;
}
cout << "If you want results from these backends you need to build them first." << endl;
cout << endl;
}
//
// ======= Output the result string to file =======
//
std::fstream file;
file.open(outname_data, std::ios_base::out);
file << results_ss.str();
file.close();
}
catch (std::exception& e)
{
std::cout << "DarkBit_standalone_MSSM has exited with fatal exception: " << e.what() << std::endl;
}
return 0;
}
Updated on 2024-07-18 at 13:53:34 +0000