namespace Gambit::DarkBit #

[No description available]

Namespaces #

Classes #

Types #

Functions #

Attributes #

Types Documentation #

enum SimYieldChannelCheck #

Result of SimYieldTable::checkChannel.

enum InterpolationOptions1D #

Generic one-dimensional integration container for linear interpolation and cubic splines.

enum InterpolationOptions2D #

Two-dimensional integration container for bilinear interpolation and bicubic splines.

enum cascadeMC_SpecialEvents #

Special events for event loop.

typedef simpleHistContainter #

typedef std::map<str, std::map<str, Gambit::DarkBit::SimpleHist> > Gambit::DarkBit::simpleHistContainter;

typedef stringIntMap #

typedef std::map<str, int> Gambit::DarkBit::stringIntMap;

typedef stringFunkMap #

typedef std::map<str, daFunk::Funk> Gambit::DarkBit::stringFunkMap;

Functions Documentation #

function IC22_full #

void IC22_full(
    nudata & result
)

Likelihood calculators for different IceCube event samples These functions all include the likelihood of the background-only model for the respective sample. We define the final log-likelihood as delta = sum over analyses of (lnL_model - lnL_BG), conservatively forbidding delta > 0 in order to always just use the neutrino likelihood as a limit. This ignores small low-E excesses caused by impending breakdown of approximations used in IceCube response data and the nulike likelihood at very low E. This implies conditioning on all but one parameter (e.g. the cross-section), such that including any particular IC analysis adds just one additional degree of freedom to the fit.

22-string IceCube sample: predicted signal and background counts, observed counts and likelihoods.

Option nulike_speed: Speed setting for nulike backend (default 3)

function IC79WH_full #

void IC79WH_full(
    nudata & result
)

79-string IceCube WH sample: predicted signal and background counts, observed counts and likelihoods.

Option nulike_speed: Speed setting for nulike backend (default 3)

function IC79WL_full #

void IC79WL_full(
    nudata & result
)

79-string IceCube WL sample: predicted signal and background counts, observed counts and likelihoods.

Option nulike_speed: Speed setting for nulike backend (default 3)

function IC79SL_full #

void IC79SL_full(
    nudata & result
)

79-string IceCube SL sample: predicted signal and background counts, observed counts and likelihoods.

Option nulike_speed: Speed setting for nulike backend (default 3)

function IC22_signal #

void IC22_signal(
    double & result
)

22-string extractor module functions

function IC22_bg #

void IC22_bg(
    double & result
)

function IC22_nobs #

void IC22_nobs(
    int & result
)

function IC22_loglike #

void IC22_loglike(
    double & result
)

function IC22_bgloglike #

void IC22_bgloglike(
    double & result
)

function IC22_pvalue #

void IC22_pvalue(
    double & result
)

function IC79WH_signal #

void IC79WH_signal(
    double & result
)

79-string WH extractor module functions

function IC79WH_bg #

void IC79WH_bg(
    double & result
)

function IC79WH_nobs #

void IC79WH_nobs(
    int & result
)

function IC79WH_loglike #

void IC79WH_loglike(
    double & result
)

function IC79WH_bgloglike #

void IC79WH_bgloglike(
    double & result
)

function IC79WH_pvalue #

void IC79WH_pvalue(
    double & result
)

function IC79WL_signal #

void IC79WL_signal(
    double & result
)

79-string WL extractor module functions

function IC79WL_bg #

void IC79WL_bg(
    double & result
)

function IC79WL_nobs #

void IC79WL_nobs(
    int & result
)

function IC79WL_loglike #

void IC79WL_loglike(
    double & result
)

function IC79WL_bgloglike #

void IC79WL_bgloglike(
    double & result
)

function IC79WL_pvalue #

void IC79WL_pvalue(
    double & result
)

function IC79SL_signal #

void IC79SL_signal(
    double & result
)

79-string SL extractor module functions

function IC79SL_bg #

void IC79SL_bg(
    double & result
)

function IC79SL_nobs #

void IC79SL_nobs(
    int & result
)

function IC79SL_loglike #

void IC79SL_loglike(
    double & result
)

function IC79SL_bgloglike #

void IC79SL_bgloglike(
    double & result
)

function IC79SL_pvalue #

void IC79SL_pvalue(
    double & result
)

function CMC_dummy #

void CMC_dummy(
    DarkBit::stringFunkMap & result
)

function createSpectrum #

void createSpectrum(
    Spectrum & outSpec
)

function createDecays #

void createDecays(
    DecayTable & outDecays
)

function TH_ProcessCatalog_WIMP #

void TH_ProcessCatalog_WIMP(
    TH_ProcessCatalog & result
)

Option mWIMP: WIMP mass in GeV (required)

Option sv: Cross-section in cm3/s (required)

Option brList<std::vector>: List of branching ratios (required)

Option mWIMP: WIMP mass in GeV (required)

function DarkMatter_ID_WIMP #

void DarkMatter_ID_WIMP(
    std::string & result
)

function DarkMatterConj_ID_WIMP #

void DarkMatterConj_ID_WIMP(
    std::string & result
)

function WIMP_properties_WIMP #

void WIMP_properties_WIMP(
    WIMPprops & props
)

function DD_couplings_WIMP #

void DD_couplings_WIMP(
    DM_nucleon_couplings & result
)

Option gps: gps (default 0)

Option gns: gns (default 0)

Option gpa: gpa (default 0)

Option gna: gna (default 0)

function DarkBit_error #

error & DarkBit_error()

function DarkBit_warning #

warning & DarkBit_warning()

function lnL_pbarAMS02 #

void lnL_pbarAMS02(
    map_str_dbl & result
)

function lnL_pbarAMS02_uncorr #

void lnL_pbarAMS02_uncorr(
    double & result
)

function lnL_pbarAMS02_corr #

void lnL_pbarAMS02_corr(
    double & result
)

function parabola #

double parabola(
    double x,
    const double params[]
)

H.E.S.S.-likelihood-related interpolation routines.

function intersect_parabola_line #

double intersect_parabola_line(
    double a,
    double b,
    double sign,
    const double pparams[]
)

function rho_integrand #

double rho_integrand(
    double rho,
    void * params
)

function rad_integrand #

double rad_integrand(
    double rad,
    void * params
)

function erg_integrand #

double erg_integrand(
    double erg,
    void * params
)

function alt_erg_integrand #

double alt_erg_integrand(
    double erg,
    void * params
)

function gaussian_nuisance_lnL #

double gaussian_nuisance_lnL(
    double theo,
    double obs,
    double sigma
)

function gStar #

double gStar(
    double T
)

Various capabilities and functions to provide SM physics as well as QCD input for axions.

Supported models: QCDAxion

function gStar_S #

double gStar_S(
    double T
)

function QCDAxion_ZeroTemperatureMass_Nuisance_lnL #

void QCDAxion_ZeroTemperatureMass_Nuisance_lnL(
    double & result
)

function QCDAxion_AxionPhotonConstant_Nuisance_lnL #

void QCDAxion_AxionPhotonConstant_Nuisance_lnL(
    double & result
)

function log_chi #

double log_chi(
    double T,
    double beta,
    double Tchi
)

function QCDAxion_TemperatureDependence_Nuisance_lnL #

void QCDAxion_TemperatureDependence_Nuisance_lnL(
    double & result
)

function ALPS1_signal_general #

double ALPS1_signal_general(
    double power,
    double nm1,
    double m_ax,
    double gagg
)

Likelihoods for ALPS 1 (LSW), CAST (helioscopes), and ADMX, UF, RBF (haloscopes).

Supported models: GeneralALP

function calc_ALPS1_signal_vac #

void calc_ALPS1_signal_vac(
    double & result
)

function calc_ALPS1_signal_gas #

void calc_ALPS1_signal_gas(
    double & result
)

function ALPS1_lnL_general #

double ALPS1_lnL_general(
    double s,
    double mu,
    double sigma
)

function calc_lnL_ALPS1 #

void calc_lnL_ALPS1(
    double & result
)

function calc_CAST2007_signal_vac #

void calc_CAST2007_signal_vac(
    std::vector< double > & result
)

function calc_CAST2017_signal_vac #

void calc_CAST2017_signal_vac(
    std::vector< std::vector< double > > & result
)

function CAST_lnL_general #

double CAST_lnL_general(
    std::vector< double > s,
    const std::vector< double > bkg_counts,
    const std::vector< int > sig_counts
)

function calc_lnL_CAST2007 #

void calc_lnL_CAST2007(
    double & result
)

function calc_lnL_CAST2017 #

void calc_lnL_CAST2017(
    double & result
)

function calc_Haloscope_signal #

void calc_Haloscope_signal(
    double & result
)

function calc_lnL_Haloscope_ADMX1 #

void calc_lnL_Haloscope_ADMX1(
    double & result
)

Approximated likelihood for the AxionDarkMatterEXperiment (ADMX).

function calc_lnL_Haloscope_ADMX2 #

void calc_lnL_Haloscope_ADMX2(
    double & result
)

function calc_lnL_Haloscope_UF #

void calc_lnL_Haloscope_UF(
    double & result
)

function calc_lnL_Haloscope_RBF #

void calc_lnL_Haloscope_RBF(
    double & result
)

function SpecialFun1 #

double SpecialFun1(
    double T
)

Capabilities relating to axion cosmology. Currently only provides the energy density in axions today due to the realignment mechanism.

Supported models: GeneralALP

function SpecialFun3 #

double SpecialFun3(
    double T
)

function hubble_rad_dom #

double hubble_rad_dom(
    double T
)

function axion_mass_temp #

double axion_mass_temp(
    double T,
    double beta,
    double Tchi
)

function equation_Tosc #

double equation_Tosc(
    double T,
    void * params
)

function calc_AxionOscillationTemperature #

void calc_AxionOscillationTemperature(
    double & result
)

function scal_field_eq #

int scal_field_eq(
    double tau,
    const double y[],
    double f[],
    void * params
)

function scal_field_eq_jac #

int scal_field_eq_jac(
    double tau,
    const double y[],
    double * dfdy,
    double dfdt[],
    void * params
)

function RD_oh2_Axions #

void RD_oh2_Axions(
    double & result
)

function calc_RParameter #

void calc_RParameter(
    double & result
)

Capabilities relating to astrophysical observations (R-parameter, H.E.S.S. telescope search, cooling hints).

Supported models: GeneralALP

function calc_lnL_RParameter #

void calc_lnL_RParameter(
    double & result
)

function calc_lnL_WDVar_G117B15A #

void calc_lnL_WDVar_G117B15A(
    double & result
)

function calc_lnL_WDVar_R548 #

void calc_lnL_WDVar_R548(
    double & result
)

function calc_lnL_WDVar_PG1351489 #

void calc_lnL_WDVar_PG1351489(
    double & result
)

function calc_lnL_WDVar_L192 #

void calc_lnL_WDVar_L192(
    double & result
)

function calc_lnL_SN1987A #

void calc_lnL_SN1987A(
    double & result
)

function calc_PhotonFluence_SN1987A_Conversion #

void calc_PhotonFluence_SN1987A_Conversion(
    double & result
)

function calc_PhotonFluence_SN1987A_Decay #

void calc_PhotonFluence_SN1987A_Decay(
    double & result
)

function calc_lnL_HESS_GCMF #

void calc_lnL_HESS_GCMF(
    double & result
)

function calc_lnL_XENON1T_Anomaly #

void calc_lnL_XENON1T_Anomaly(
    double & result
)

Capability for the XENON1T likelihood from 2006.10035.

The signal model consists of 3 components: Primakoff, ABC, and Fe57.

function dRdE #

double dRdE(
    double E,
    void * params
)

function calc_lnL_XENON1T_DM_Anomaly #

void calc_lnL_XENON1T_DM_Anomaly(
    double & result
)

function calc_lnL_XENON1T_Anomaly_NuisanceParameters #

void calc_lnL_XENON1T_Anomaly_NuisanceParameters(
    double & result
)

function cascadeMC_InitialStates #

void cascadeMC_InitialStates(
    std::set< std::string > & result
)

Identification of hard-process final states for which yield tables do not exist.

Structure #

1. Go through process catalog and find all hard-process final states that require yields to be calculated with the cascade code. These will constitute initial states for the cascade code. To this end, check whether yield tables exist for two-body channels, and whether one-particle decay yield tables exist for single particles.

2. Calculate via the cascade code the missing energy spectra.

3. Put together the full spectrum.

Option ignore_all: Ignore all missing hard process final states (default false)

Option ignore_two_body: Ignore two-body missing final states (default false)

Option ignore_three_body: Ignore three-body missing final states (default false)

function cascadeMC_FinalStates #

void cascadeMC_FinalStates(
    std::set< std::string > & states
)

Function for retrieving list of final states for cascade decays.

function cascadeMC_DecayTable #

void cascadeMC_DecayTable(
    DarkBit::DecayChain::DecayTable & table
)

Function setting up the decay table used in decay chains.

function cascadeMC_LoopManager #

void cascadeMC_LoopManager(
    std::string & result
)

Loop manager for cascade decays.

Option cMC_maxEvents: Maximum number of cascade MC runs (default 20000)

function cascadeMC_EventCount #

void cascadeMC_EventCount(
    std::map< std::string, int > & counts
)

Event counter for cascade decays.

function cascadeMC_GenerateChain #

void cascadeMC_GenerateChain(
    DarkBit::DecayChain::ChainContainer & chain
)

Function for generating decay chains.

Option cMC_maxChainLength: Maximum chain length, -1 is infinite (default -1)

Option cMC_Emin: Cutoff energy for cascade particles (default 0)

function cascadeMC_sampleSimYield #

void cascadeMC_sampleSimYield(
    const SimYieldTable & table,
    const DarkBit::DecayChain::ChainParticle * endpoint,
    std::string finalState,
    const TH_ProcessCatalog & catalog,
    std::map< std::string, std::map< std::string, SimpleHist > > & histList,
    std::string initialState,
    double weight,
    int cMC_numSpecSamples
)

Function for sampling SimYieldTables (tabulated spectra). This is a convenience function used in cascadeMC_Histograms, and does not have an associated capability.

function cascadeMC_Histograms #

void cascadeMC_Histograms(
    std::map< std::string, std::map< std::string, SimpleHist > > & result
)

Function responsible for histogramming, and evaluating end conditions for event loop.

Option cMC_numSpecSamples: number of samples to draw from tabulated spectra (default 25)

Option cMC_endCheckFrequency: number of events to wait between successive checks of the convergence criteria (default 25)

Option cMC_gammaBGPower: power-law slope to assume for astrophysical background (default -2.5)

Option cMC_gammaRelError: max allowed relative error in bin with highest expected signal-to-background (default 0.20)

Option cMC_NhistBins: Number of histogram bins (default 140)

Option cMC_binLow: Histogram min energy in GeV (default 0.001)

Option cMC_binHigh: Histogram max energy in GeV (default 10000)

@TODO: consider implementing specific convergence criteria for other final states

function cascadeMC_fetchSpectra #

void cascadeMC_fetchSpectra(
    std::map< std::string, daFunk::Funk > & spectra,
    std::string finalState,
    const std::set< std::string > & ini,
    const std::set< std::string > & fin,
    const std::map< std::string, std::map< std::string, SimpleHist > > & h,
    const std::map< std::string, int > & eventCounts
)

Convenience function for getting a daFunk::Funk object of a given spectrum. This function has no associated capability. Function retrieving specific spectra (like cascadeMC_gammaSpectra) should call this function.

function print_spectrum_debug_info #

void print_spectrum_debug_info(
    const str & fs,
    const std::map< std::string, daFunk::Funk > & spectra
)

Debug print function for cascase spectra.

function cascadeMC_gammaSpectra #

void cascadeMC_gammaSpectra(
    std::map< std::string, daFunk::Funk > & spectra
)

Function requesting and returning gamma ray spectra from cascade decays.

function cascadeMC_electronSpectra #

void cascadeMC_electronSpectra(
    std::map< std::string, daFunk::Funk > & spectra
)

Function requesting and returning electron spectra from cascade decays.

function cascadeMC_positronSpectra #

void cascadeMC_positronSpectra(
    std::map< std::string, daFunk::Funk > & spectra
)

Function requesting and returning positron spectra from cascade decays.

function cascadeMC_antiprotonSpectra #

void cascadeMC_antiprotonSpectra(
    std::map< std::string, daFunk::Funk > & spectra
)

Function requesting and returning pbar spectra from cascade decays.

function cascadeMC_antideuteronSpectra #

void cascadeMC_antideuteronSpectra(
    std::map< std::string, daFunk::Funk > & spectra
)

Function requesting and returning Dbar spectra from cascade decays.

function WIMP_properties #

void WIMP_properties(
    WIMPprops & props
)

Retrieve the struct of WIMP properties.

function mwimp_generic #

void mwimp_generic(
    double & result
)

Retrieve the DM mass in GeV for generic models (GeV)

function spinwimpx2_generic #

void spinwimpx2_generic(
    unsigned int & result
)

Retrieve the DM spin (times two) generic models.

function wimp_sc_generic #

void wimp_sc_generic(
    bool & result
)

Retrieve whether or not the DM is self conjugate or not.

function sigmav_late_universe #

void sigmav_late_universe(
    double & result
)

Retrieve the total thermally-averaged annihilation cross-section for indirect detection (cm^3 / s).

function sigmav_late_universe_MicrOmegas #

void sigmav_late_universe_MicrOmegas(
    double & result
)

function DM_process_from_ProcessCatalog #

void DM_process_from_ProcessCatalog(
    std::string & result
)

Information about the nature of the DM process in question (i.e. decay or annihilation) to use the correct scaling for ID in terms of the DM density, phase space, etc.

function profile_gNFW #

double profile_gNFW(
    double rhos,
    double rs,
    double alpha,
    double beta,
    double gamma,
    double r
)

Generalized NFW dark matter halo profile function.

function profile_Einasto #

double profile_Einasto(
    double rhos,
    double rs,
    double alpha,
    double r
)

Einasto dark matter halo profile function.

function GalacticHalo_gNFW #

void GalacticHalo_gNFW(
    GalacticHaloProperties & result
)

Module function to generate GalacticHaloProperties for gNFW profile.

function GalacticHalo_Einasto #

void GalacticHalo_Einasto(
    GalacticHaloProperties & result
)

Module function to generate GalacticHaloProperties for Einasto profile.

function ExtractLocalMaxwellianHalo #

void ExtractLocalMaxwellianHalo(
    LocalMaxwellianHalo & result
)

Module function providing local density and velocity dispersion parameters.

function UnitTest_DarkBit #

void UnitTest_DarkBit(
    int & result
)

Central unit test routine.

Dumps various DM related results into yaml files for later inspection.

Option filenamestd::string: Output filename (default UnitTest.yaml)

Option GA_AnnYield::Emin: Minimum energy in GeV (default 0.1)

Option GA_AnnYield::Emax: Maximum energy in GeV (default 1e4)

Option GA_AnnYield::nbins: Number of energy bins (default 26)

function get_finalState_mass #

double get_finalState_mass(
    const std::string & finalState
)

Helper function to get the mass of a given final state particle.

function DarkMatter_ID_DiracSingletDM #

void DarkMatter_ID_DiracSingletDM(
    std::string & result
)

function DarkMatterConj_ID_DiracSingletDM #

void DarkMatterConj_ID_DiracSingletDM(
    std::string & result
)

function DD_nonrel_WCs_DiracSingletDM_Z2 #

void DD_nonrel_WCs_DiracSingletDM_Z2(
    NREO_DM_nucleon_couplings & result
)

Direct detection couplings for the DiracSingletDM_Z2 model.

function DD_rel_WCs_flavscheme_DiracSingletDM_Z2 #

void DD_rel_WCs_flavscheme_DiracSingletDM_Z2(
    map_str_dbl & result
)

Relativistic Wilson Coefficients for direct detection, defined in the flavour scheme

function TH_ProcessCatalog_DiracSingletDM_Z2 #

void TH_ProcessCatalog_DiracSingletDM_Z2(
    DarkBit::TH_ProcessCatalog & result
)

Set up process catalog for the DiracSingletDM_Z2 model.

function DD_couplings_DarkSUSY_DS5 #

void DD_couplings_DarkSUSY_DS5(
    DM_nucleon_couplings & result
)

Get direct detection couplings from initialized DarkSUSY 5.

Option rescale_couplings: Rescaling factor for WIMP-nucleon couplings (default 1.)

function DD_couplings_DarkSUSY_MSSM #

void DD_couplings_DarkSUSY_MSSM(
    DM_nucleon_couplings & result
)

Get direct detection couplings from DarkSUSY 6 initialized with MSSM module.

Option rescale_couplings: Rescaling factor for WIMP-nucleon couplings (default 1.)

function DD_couplings_MicrOmegas #

void DD_couplings_MicrOmegas(
    DM_nucleon_couplings & result
)

Get direct detection couplings from initialized MicrOmegas.

function sigma_SI_p_simple #

void sigma_SI_p_simple(
    double & result
)

Simple calculator of the spin-independent WIMP-proton cross-section.

function sigma_SI_n_simple #

void sigma_SI_n_simple(
    double & result
)

Simple calculator of the spin-independent WIMP-neutron cross-section.

function sigma_SD_p_simple #

void sigma_SD_p_simple(
    double & result
)

Simple calculator of the spin-dependent WIMP-proton cross-section.

function sigma_SD_n_simple #

void sigma_SD_n_simple(
    double & result
)

Simple calculator of the spin-dependent WIMP-neutron cross-section.

function sigma_SI_vnqn_FermionicHiggsPortal #

void sigma_SI_vnqn_FermionicHiggsPortal(
    map_intpair_dbl & result
)

Calculation of SI cross sections at a reference momentum q0 for the fermionic Higgs portal models If required add equivalent function for spin-dependent cross section

function sigma_SD_vnqn_FermionicHiggsPortal #

void sigma_SD_vnqn_FermionicHiggsPortal(
    map_intpair_dbl & result
)

Calculation of SD cross section at a reference momentum q0 for the fermionic Higgs portal models

There is no SD contribution to fermionic Higgs portal models So this is just set to 0 (or close enough) Modify if needed

function DDCalc_Couplings_WIMP_nucleon #

void DDCalc_Couplings_WIMP_nucleon(
    DD_coupling_container & result
)

DDCalc initialisation.

function DDCalc_Couplings_NR_WCs #

void DDCalc_Couplings_NR_WCs(
    DD_coupling_container & result
)

function TH_ProcessCatalog_DMEFT #

void TH_ProcessCatalog_DMEFT(
    DarkBit::TH_ProcessCatalog & result
)

function DarkMatter_ID_DMEFT #

void DarkMatter_ID_DMEFT(
    std::string & result
)

function DarkMatterConj_ID_DMEFT #

void DarkMatterConj_ID_DMEFT(
    std::string & result
)

function DD_rel_WCs_flavscheme_DMEFT #

void DD_rel_WCs_flavscheme_DMEFT(
    map_str_dbl & result
)

Relativistic Wilson Coefficients for direct detection DMEFT basis is the same as that used in DirectDM

function TH_ProcessCatalog_DMsimpVectorMedDiracDM #

void TH_ProcessCatalog_DMsimpVectorMedDiracDM(
    TH_ProcessCatalog & result
)

function DarkMatter_ID_DMsimpVectorMedDiracDM #

void DarkMatter_ID_DMsimpVectorMedDiracDM(
    std::string & result
)

function DarkMatterConj_ID_DMsimpVectorMedDiracDM #

void DarkMatterConj_ID_DMsimpVectorMedDiracDM(
    std::string & result
)

function DD_rel_WCs_flavscheme_DMsimpVectorMedDiracDM #

void DD_rel_WCs_flavscheme_DMsimpVectorMedDiracDM(
    map_str_dbl & result
)

Relativistic Wilson Coefficients for direct detection DMsimpVectorMedDiracDM basis is the same as that used in DirectDM

function TH_ProcessCatalog_DMsimpVectorMedMajoranaDM #

void TH_ProcessCatalog_DMsimpVectorMedMajoranaDM(
    TH_ProcessCatalog & result
)

function DarkMatter_ID_DMsimpVectorMedMajoranaDM #

void DarkMatter_ID_DMsimpVectorMedMajoranaDM(
    std::string & result
)

function DarkMatterConj_ID_DMsimpVectorMedMajoranaDM #

void DarkMatterConj_ID_DMsimpVectorMedMajoranaDM(
    std::string & result
)

function DD_rel_WCs_flavscheme_DMsimpVectorMedMajoranaDM #

void DD_rel_WCs_flavscheme_DMsimpVectorMedMajoranaDM(
    map_str_dbl & result
)

Relativistic Wilson Coefficients for direct detection DMsimpVectorMedMajoranaDM basis is the same as that used in DirectDM

function TH_ProcessCatalog_DMsimpVectorMedScalarDM #

void TH_ProcessCatalog_DMsimpVectorMedScalarDM(
    TH_ProcessCatalog & result
)

function DarkMatter_ID_DMsimpVectorMedScalarDM #

void DarkMatter_ID_DMsimpVectorMedScalarDM(
    std::string & result
)

function DarkMatterConj_ID_DMsimpVectorMedScalarDM #

void DarkMatterConj_ID_DMsimpVectorMedScalarDM(
    std::string & result
)

function DD_rel_WCs_flavscheme_DMsimpVectorMedScalarDM #

void DD_rel_WCs_flavscheme_DMsimpVectorMedScalarDM(
    map_str_dbl & result
)

Relativistic Wilson Coefficients for direct detection DMsimpVectorMedScalarDM basis is the same as that used in DirectDM

function TH_ProcessCatalog_DMsimpVectorMedVectorDM #

void TH_ProcessCatalog_DMsimpVectorMedVectorDM(
    TH_ProcessCatalog & result
)

function DarkMatter_ID_DMsimpVectorMedVectorDM #

void DarkMatter_ID_DMsimpVectorMedVectorDM(
    std::string & result
)

function DarkMatterConj_ID_DMsimpVectorMedVectorDM #

void DarkMatterConj_ID_DMsimpVectorMedVectorDM(
    std::string & result
)

function DD_nonrel_WCs_DMsimpVectorMedVectorDM #

void DD_nonrel_WCs_DMsimpVectorMedVectorDM(
    NREO_DM_nucleon_couplings & result
)

function DarkMatter_ID_AnnihilatingDM_mixture #

void DarkMatter_ID_AnnihilatingDM_mixture(
    std::string & result
)

function DarkMatterConj_ID_AnnihilatingDM_mixture #

void DarkMatterConj_ID_AnnihilatingDM_mixture(
    std::string & result
)

function DarkMatter_ID_DecayingDM_mixture #

void DarkMatter_ID_DecayingDM_mixture(
    std::string & result
)

function DarkMatterConj_ID_DecayingDM_mixture #

void DarkMatterConj_ID_DecayingDM_mixture(
    std::string & result
)

function energy_injection_spectrum_ProcessCatalog #

void energy_injection_spectrum_ProcessCatalog(
    DarkAges::Energy_injection_spectrum & spectrum
)

The energy injection spectrum from the ProcessCatalog and FCMC.

function TH_ProcessCatalog_AnnihilatingDM_mixture #

void TH_ProcessCatalog_AnnihilatingDM_mixture(
    TH_ProcessCatalog & result
)

Set up process catalog for AnnihilatingDM_mixture.

function TH_ProcessCatalog_DecayingDM_mixture #

void TH_ProcessCatalog_DecayingDM_mixture(
    TH_ProcessCatalog & result
)

Set up process catalog for DecayingDM_mixture.

function boost_dNdE #

daFunk::Funk boost_dNdE(
    daFunk::Funk dNdE,
    double gamma,
    double mass
)

Boosts an energy spectrum of isotropic particles into another frame (and isotropizes again). Parameters: gamma: Lorentz boost factor dNdE: Spectrum mass: mass of particle.

function getYield #

daFunk::Funk getYield(
    const str & yield,
    const bool is_annihilation,
    const str & DMid,
    const str & DMbarid,
    TH_ProcessCatalog catalog,
    SimYieldTable table,
    double line_width,
    stringFunkMap cascadeMC_spectra
)

Helper function returning yield from a given DM process.

function GA_AnnYield_General #

void GA_AnnYield_General(
    daFunk::Funk & result
)

General routine to derive gamma-ray annihilation yield. This function returns kdN/dE(sv)/mDM**2 (E, v) [cm^3/s/GeV^3] the energy spectrum of photons times sigma*v/m^2, as function of energy (in GeV) and velocity (as a fraction of c), multiplied by k=1 for self-conjugate DM or k=1/2 for non-self conjugate. By default, only the v=0 component is calculated.

Option line_width: Set relative line width used in gamma-ray spectra (default 0.03)

function GA_DecayYield_General #

void GA_DecayYield_General(
    daFunk::Funk & result
)

General routine to derive gamma-ray decay yield. This function returns dN/dE*(Gamma)/mDM (E) [1/s/GeV^2] the energy spectrum of photons times Gamma/m, as function of energy (in GeV).

Option line_width: Set relative line width used in gamma-ray spectra (default 0.03)

function electron_AnnYield_General #

void electron_AnnYield_General(
    daFunk::Funk & result
)

General routine to derive electron annihilation yield. This function returns kdN/dE(sv)/mDM**2 (E, v) [cm^3/s/GeV^3] the energy spectrum of electrons times sigma*v/m^2, as function of energy (in GeV) and velocity (as a fraction of c), multiplied by k=1 for self-conjugate DM or k=1/2 for non-self conjugate. By default, only the v=0 component is calculated.

Option line_width: Set relative line width used in gamma-ray spectra (default 0.03)

function electron_DecayYield_General #

void electron_DecayYield_General(
    daFunk::Funk & result
)

General routine to derive electron decay yield. This function returns dN/dE*(Gamma)/mDM (E) [1/s/GeV^2] the energy spectrum of electrons times Gamma/m, as function of energy (in GeV).

Option line_width: Set relative line width used in gamma-ray spectra (default 0.03)

function positron_AnnYield_General #

void positron_AnnYield_General(
    daFunk::Funk & result
)

General routine to derive positron annihilation yield. This function returns kdN/dE(sv)/mDM**2 (E, v) [cm^3/s/GeV^3] the energy spectrum of positrons times sigma*v/m^2, as function of energy (in GeV) and velocity (as a fraction of c), multiplied by k=1 for self-conjugate DM or k=1/2 for non-self conjugate. By default, only the v=0 component is calculated.

Option line_width: Set relative line width used in gamma-ray spectra (default 0.03)

function positron_DecayYield_General #

void positron_DecayYield_General(
    daFunk::Funk & result
)

General routine to derive positron decay yield. This function returns dN/dE*(Gamma)/mDM (E) [1/s/GeV^2] the energy spectrum of positrons times Gamma/m, as function of energy (in GeV).

Option line_width: Set relative line width used in gamma-ray spectra (default 0.03)

function antiproton_AnnYield_General #

void antiproton_AnnYield_General(
    daFunk::Funk & result
)

General routine to derive antiproton annihilation yield. This function returns kdN/dE(sv)/mDM**2 (E, v) [cm^3/s/GeV^3] the energy spectrum of antiprotons times sigma*v/m^2, as function of energy (in GeV) and velocity (as a fraction of c), multiplied by k=1 for self-conjugate DM or k=1/2 for non-self conjugate. By default, only the v=0 component is calculated.

Option line_width: Set relative line width used in gamma-ray spectra (default 0.03)

function antiproton_DecayYield_General #

void antiproton_DecayYield_General(
    daFunk::Funk & result
)

General routine to derive antiproton decay yield. This function returns dN/dE*(Gamma)/mDM (E) [1/s/GeV^2] the energy spectrum of antiprotons times Gamma/m, as function of energy (in GeV).

Option line_width: Set relative line width used in gamma-ray spectra (default 0.03)

function antideuteron_AnnYield_General #

void antideuteron_AnnYield_General(
    daFunk::Funk & result
)

General routine to derive antideuteron annihilation yield. This function returns kdN/dE(sv)/mDM**2 (E, v) [cm^3/s/GeV^3] the energy spectrum of antideuterons times sigma*v/m^2, as function of energy (in GeV) and velocity (as a fraction of c), multiplied by k=1 for self-conjugate DM or k=1/2 for non-self conjugate. By default, only the v=0 component is calculated.

Option line_width: Set relative line width used in gamma-ray spectra (default 0.03)

function antideuteron_DecayYield_General #

void antideuteron_DecayYield_General(
    daFunk::Funk & result
)

General routine to derive antideuteron decay yield. This function returns dN/dE*(Gamma)/mDM (E) [1/s/GeV^2] the energy spectrum of antideuterons times Gamma/m, as function of energy (in GeV).

Option line_width: Set relative line width used in gamma-ray spectra (default 0.03)

function Combine_SimYields #

void Combine_SimYields(
    SimYieldTable & result
)

Combined SimYieldTable containing final yields of all stable particles.

function GA_SimYieldTable_DS5 #

void GA_SimYieldTable_DS5(
    SimYieldTable & result
)

Gamma-ray SimYieldTable based on DarkSUSY5 tabulated results. (DS6 below)

Option allow_yield_extrapolation: Spectra extrapolated for masses beyond Pythia results (default false)

function SimYieldTable_DarkSUSY #

SimYieldTable SimYieldTable_DarkSUSY(
    const str & yield,
    const bool allow_yield_extrapolation,
    double(*)(double &, double &, int &, char *, int &, int &, int &) dsanyield,
    safe_ptr< Options > runOptions
)

Construct a SimYieldTable based on DarkSUSY6 tabulated results.

function GA_SimYieldTable_DarkSUSY #

void GA_SimYieldTable_DarkSUSY(
    SimYieldTable & result
)

Gamma-ray SimYieldTable based on DarkSUSY6 tabulated results.

Option allow_yield_extrapolation: Spectra extrapolated for masses beyond Pythia results (default false)

function positron_SimYieldTable_DarkSUSY #

void positron_SimYieldTable_DarkSUSY(
    SimYieldTable & result
)

Positron SimYieldTable based on DarkSUSY6 tabulated results.

Option allow_yield_extrapolation: Spectra extrapolated for masses beyond Pythia results (default false)

function antiproton_SimYieldTable_DarkSUSY #

void antiproton_SimYieldTable_DarkSUSY(
    SimYieldTable & result
)

Anti-proton SimYieldTable based on DarkSUSY6 tabulated results.

Option allow_yield_extrapolation: Spectra extrapolated for masses beyond Pythia results (default false)

function antideuteron_SimYieldTable_DarkSUSY #

void antideuteron_SimYieldTable_DarkSUSY(
    SimYieldTable & result
)

Anti-deuteron SimYieldTable based on DarkSUSY6 tabulated results.

Option allow_yield_extrapolation: Spectra extrapolated for masses beyond Pythia results (default false)

function GA_SimYieldTable_MicrOmegas #

void GA_SimYieldTable_MicrOmegas(
    SimYieldTable & result
)

Gamma-ray SimYieldTable based on MicrOmegas tabulated results.

function positron_SimYieldTable_MicrOmegas #

void positron_SimYieldTable_MicrOmegas(
    SimYieldTable & 
)

Positron SimYieldTable based on MicrOmegas tabulated results.

function SimYieldTable_PPPC #

SimYieldTable SimYieldTable_PPPC(
    const str & yield,
    bool allow_yield_extrapolation,
    double(*)(double, double, std::string) PPPC_yield,
    safe_ptr< Options > runOptions
)

function PPPC_dNdE_gamma #

double PPPC_dNdE_gamma(
    double m,
    double x,
    std::string channel
)

Conveninence function to get the gamma yield from the interpolated PPPC tables.

function PPPC_dNdE_positron #

double PPPC_dNdE_positron(
    double m,
    double x,
    std::string channel
)

Conveninence function to get the positiron yield from the interpolated PPPC tables.

function GA_SimYieldTable_PPPC #

void GA_SimYieldTable_PPPC(
    SimYieldTable & result
)

Gamma-ray SimYieldTable based on PPPC4DMID Cirelli et al. 2010.

Option allow_yield_extrapolation: Spectra extrapolated for masses beyond Pythia results (default false)

function positron_SimYieldTable_PPPC #

void positron_SimYieldTable_PPPC(
    SimYieldTable & result
)

Positron SimYieldTable based on PPPC4DMID Cirelli et al. 2010.

Option allow_yield_extrapolation: Spectra extrapolated for masses beyond Pythia results (default false)

function GA_SimYieldTable_empty #

void GA_SimYieldTable_empty(
    SimYieldTable & result
)

Bypasses to skip specific yields in FullSimYieldTable.

function positron_SimYieldTable_empty #

void positron_SimYieldTable_empty(
    SimYieldTable & result
)

function antiproton_SimYieldTable_empty #

void antiproton_SimYieldTable_empty(
    SimYieldTable & result
)

function antideuteron_SimYieldTable_empty #

void antideuteron_SimYieldTable_empty(
    SimYieldTable & result
)

function electron_SimYieldTable_from_positron_SimYieldTable #

void electron_SimYieldTable_from_positron_SimYieldTable(
    SimYieldTable & result
)

Electron SimYieldTable based on positron table.

function dump #

int dump(
    const str & filename,
    const daFunk::Funk & spectrum
)

Helper function to dump any spectra.

function dump_gammaSpectrum #

void dump_gammaSpectrum(
    int & result
)

Helper function to dump gamma-ray spectra.

function dump_electronSpectrum #

void dump_electronSpectrum(
    int & result
)

Helper function to dump electron spectra.

function dump_positronSpectrum #

void dump_positronSpectrum(
    int & result
)

Helper function to dump positron spectra.

function dump_antiprotonSpectrum #

void dump_antiprotonSpectrum(
    int & result
)

Helper function to dump anti-proton spectra.

function dump_antideuteronSpectrum #

void dump_antideuteronSpectrum(
    int & result
)

Helper function to dump anti-deuteron spectra.

function DarkMatter_ID_MajoranaSingletDM #

void DarkMatter_ID_MajoranaSingletDM(
    std::string & result
)

function DarkMatterConj_ID_MajoranaSingletDM #

void DarkMatterConj_ID_MajoranaSingletDM(
    std::string & result
)

function DD_nonrel_WCs_MajoranaSingletDM_Z2 #

void DD_nonrel_WCs_MajoranaSingletDM_Z2(
    NREO_DM_nucleon_couplings & result
)

Direct detection couplings for the MajoranaSingletDM_Z2 model. Non-relativistic Wilson Coefficients for direct detection

function DD_rel_WCs_flavscheme_MajoranaSingletDM_Z2 #

void DD_rel_WCs_flavscheme_MajoranaSingletDM_Z2(
    map_str_dbl & result
)

Relativistic Wilson Coefficients for direct detection, defined in the flavour scheme

function TH_ProcessCatalog_MajoranaSingletDM_Z2 #

void TH_ProcessCatalog_MajoranaSingletDM_Z2(
    DarkBit::TH_ProcessCatalog & result
)

Set up process catalog for the MajoranaSingletDM_Z2 model.

function DSgamma3bdy #

double DSgamma3bdy(
    double(*)(int &, double &, double &) IBfunc,
    int IBch,
    double Eg,
    double E1,
    double M_DM,
    double m_1,
    double m_2
)

Fully initialize DarkSUSY to the current model point.

Only selected MSSM parameter spaces are implemented. Returns bool indicating if point initialization was successful, which is essentially always true for models that satisfy the dependency resolver.

Supported models: MSSM63atQ Wrapper around DarkSUSY kinematic functions

function TH_ProcessCatalog_DS5_MSSM #

void TH_ProcessCatalog_DS5_MSSM(
    DarkBit::TH_ProcessCatalog & result
)

Initialization of Process Catalog based on DarkSUSY 5 calculations.

Option ignore_three_body: Ignore three-body final states (default false)

function TH_ProcessCatalog_DS_MSSM #

void TH_ProcessCatalog_DS_MSSM(
    DarkBit::TH_ProcessCatalog & result
)

Initialization of Process Catalog based on DarkSUSY 6 calculations.

Option ignore_three_body: Ignore three-body final states (default false)

function DarkMatter_ID_MSSM #

void DarkMatter_ID_MSSM(
    std::string & result
)

function DarkMatterConj_ID_MSSM #

void DarkMatterConj_ID_MSSM(
    std::string & result
)

function RD_spectrum_MSSM #

void RD_spectrum_MSSM(
    RD_spectrum_type & result
)

Collects spectrum information about coannihilating particles, resonances and threshold energies.

Option CoannCharginosNeutralinos: Specify whether charginos and neutralinos are included in coannihilations (default: true)

Option CoannSfermions: Specify whether sfermions are included in coannihilations (default: true)

Option CoannMaxMass: Maximal sparticle mass to be included in coannihilations, in units of DM mass (default: 1.6)

function RD_spectrum_SUSY_DS5 #

void RD_spectrum_SUSY_DS5(
    RD_spectrum_type & result
)

Collects spectrum information about coannihilating particles, resonances and threshold energies – directly from DarkSUSY 5.

Option CoannCharginosNeutralinos: Specify whether charginos and neutralinos are included in coannihilations (default: true)

Option CoannSfermions: Specify whether sfermions are included in coannihilations (default: true)

Option CoannMaxMass: Maximal sparticle mass to be included in coannihilations, in units of DM mass (default: 1.6)

function RD_spectrum_from_ProcessCatalog #

void RD_spectrum_from_ProcessCatalog(
    RD_spectrum_type & result
)

Collects information about resonances and threshold energies directly from the ProcessCatalog [NB: this assumes no coannihilating particles!].

function RD_spectrum_ordered_func #

void RD_spectrum_ordered_func(
    RD_spectrum_type & result
)

Order RD_spectrum object and derive coannihilation thresholds.

function RD_annrate_DS5prep_func #

void RD_annrate_DS5prep_func(
    int & result
)

Some helper function to prepare evaluation of Weff from DarkSUSY 5.

function RD_annrate_DSprep_MSSM_func #

void RD_annrate_DSprep_MSSM_func(
    int & result
)

Some helper function to prepare evaluation of Weff from DarkSUSY 6.

function RD_eff_annrate_DS_MSSM #

void RD_eff_annrate_DS_MSSM(
    double(*&)(double &) result
)

Get Weff directly from initialized DarkSUSY. Note that these functions do not (and should not) correct Weff for non-self-conjugate dark matter.

function RD_eff_annrate_DS5_MSSM #

void RD_eff_annrate_DS5_MSSM(
    double(*&)(double &) result
)

function RD_eff_annrate_from_ProcessCatalog #

void RD_eff_annrate_from_ProcessCatalog(
    double(*&)(double &) result
)

Infer Weff from process catalog.

function RD_oh2_DS6pre4_ini_func #

void RD_oh2_DS6pre4_ini_func(
    int & result
)

Some helper function to prepare evaluation of RD_oh2_DS_general from DarkSUSY 6., up to version 6.2.5.

Option timeout: Maximum core time to allow for relic density calculation, in seconds (default: 600s)

Option fast: Numerical performance of Boltzmann solver in DS (default: 1) [NB: accurate is fast = 0 !]

function RD_oh2_DS6_ini_func #

void RD_oh2_DS6_ini_func(
    int & result
)

Some helper function to prepare evaluation of RD_oh2_DS_general from DarkSUSY 6., starting from version 6.4.0.

Option timeout: Maximum core time to allow for relic density calculation, in seconds (default: 600s)

Option fast: Numerical performance of Boltzmann solver in DS (default: 1) [NB: accurate is fast = 0 !]

function RD_oh2_DS_general #

void RD_oh2_DS_general(
    double & result
)

General routine for calculation of relic density, using DarkSUSY 6+ Boltzmann solver.

Requires:

• RD_thresholds_resonances from RD_spectrum_ordered
• RD_eff_annrate (Weff)

function RD_oh2_DS5_general #

void RD_oh2_DS5_general(
    double & result
)

General routine for calculation of relic density, using DarkSUSY 5 Boltzmann solver.

Requires:

• RD_thresholds_resonances
• RD_eff_annrate (Weff)

Option timeout: Maximum core time to allow for relic density calculation, in seconds (default: 600s)

Option fast: Numerical performance of Boltzmann solver in DS (default: 1) [NB: accurate is fast = 0 !]

function RD_oh2_Xf_MicrOmegas #

void RD_oh2_Xf_MicrOmegas(
    ddpair & result
)

Relic density directly from a call of initialized MicrOmegas.

function RD_oh2_DarkSUSY_DS5 #

void RD_oh2_DarkSUSY_DS5(
    double & result
)

Relic density directly from a call of initialized DarkSUSY 5.

Option omtype: 0 no coann, 1 all coann (default 1)

Option fast: 0 standard, 1 fast, 2 dirty (default 0)

Option timeout: Maximum core time to allow for relic density calculation, in seconds (default: 600s)

function RD_oh2_MicrOmegas #

void RD_oh2_MicrOmegas(
    double & result
)

function Xf_MicrOmegas #

void Xf_MicrOmegas(
    double & result
)

function RD_from_postprocessor #

void RD_from_postprocessor(
    double & result
)

function print_channel_contributions_MicrOmegas #

void print_channel_contributions_MicrOmegas(
    double & result
)

function get_semi_ann_MicrOmegas #

void get_semi_ann_MicrOmegas(
    double & result
)

function vSigma_freezeout_MicrOmegas #

void vSigma_freezeout_MicrOmegas(
    double & result
)

Return the thermally averaged cross-section at T_freezeout.

function RD_fraction_one #

void RD_fraction_one(
    double & result
)

function RD_fraction_leq_one #

void RD_fraction_leq_one(
    double & result
)

Option oh2_obs: Set reference dark matter density (Oh2) for this module function (default 0.1188)

function RD_fraction_rescaled #

void RD_fraction_rescaled(
    double & result
)

Option oh2_obs: Set reference dark matter density (Oh2) for this module function (default 0.1188)

function RD_fraction_rescaled_LCDM #

void RD_fraction_rescaled_LCDM(
    double & result
)

function DarkMatter_ID_ScalarSingletDM #

void DarkMatter_ID_ScalarSingletDM(
    std::string & result
)

function DarkMatterConj_ID_ScalarSingletDM #

void DarkMatterConj_ID_ScalarSingletDM(
    std::string & result
)

function get_ScalarSingletDM_DD_couplings #

void get_ScalarSingletDM_DD_couplings(
    const Spectrum & spec,
    DM_nucleon_couplings & result,
    Models::safe_param_map< safe_ptr< const double > > & Param
)

Common code for different scalar singlet direct detection coupling routines.

function DD_couplings_ScalarSingletDM_Z2 #

void DD_couplings_ScalarSingletDM_Z2(
    DM_nucleon_couplings & result
)

Direct detection couplings for Z2 scalar singlet DM.

function DD_couplings_ScalarSingletDM_Z3 #

void DD_couplings_ScalarSingletDM_Z3(
    DM_nucleon_couplings & result
)

Direct detection couplings for Z3 scalar singlet DM.

function TH_ProcessCatalog_ScalarSingletDM_Z2 #

void TH_ProcessCatalog_ScalarSingletDM_Z2(
    DarkBit::TH_ProcessCatalog & result
)

Set up process catalog for Z2 scalar singlet DM.

function TH_ProcessCatalog_ScalarSingletDM_Z3 #

void TH_ProcessCatalog_ScalarSingletDM_Z3(
    DarkBit::TH_ProcessCatalog & result
)

Set up process catalog for Z3 scalar singlet DM.

function lnL_FermiLATdwarfs_gamLike #

void lnL_FermiLATdwarfs_gamLike(
    double & result
)

Fermi LAT dwarf likelihoods, based on arXiv:1108.2914. / void lnL_FermiLATdwarfsSimple(double &result) { using namespace Pipes::lnL_FermiLATdwarfsSimple; // Koushiappas’ limits [arXiv:1108.2914] // // This is the tabulated Phi-Likelihood function from Koushiappas et al. // Above L = 36, we use linear extrapolation up to L = 360000 // // phi (defined as phi = sigmav/mDM**2*Ntot/8/pi * 1e26) double xgridArray [101] = { 0. , 6.74308086122e-05 , 0.000123192463137 , 0.000171713798503 , 0.000215245918518 , 0.000255093268618 , 0.00029207805123 , 0.000326751732695 , 0.000359503469472 , 0.000390620122006 , 0.000420321264006, 0.00044878042576 , 0.000476138421008 , 0.000502511975672 , 0.000527999496499, 0.000552685056887 , 0.000576641243501 , 0.000599931255273 , 0.000622610497068 , 0.000644727821172 , 0.000666326515638 , 0.000687445105269, 0.000708118010141 , 0.000728376093388 , 0.000748247120993 , 0.00076775615078, 0.000786925863514 , 0.000805776846231 , 0.000824327835809 , 0.00084259592922, 0.000860596765645 , 0.000878344684789 , 0.000895852864914 , 0.000913133443547 , 0.000930197623331 , 0.0009470557651 , 0.000963717469925 , 0.00098019165163 , 0.000996486601006 , 0.00101261004288 , 0.00102856918685 , 0.00104437077256 , 0.00106002111016 , 0.00107552611658 , 0.00109089134805 , 0.00110612202935 , 0.00112122308019 , 0.00113619913897 , 0.00115105458439 , 0.00116579355487 , 0.00118041996631 , 0.00119493752815 , 0.00120934975806 , 0.00122365999528 , 0.00123787141289 , 0.00125198702892 , 0.00126600971667 , 0.00127994221404 , 0.00129378713223 , 0.00130754696367 , 0.00132122408935 , 0.00133482078559 , 0.00134833923028 , 0.00136178150869 , 0.0013751496188 , 0.00138844547626 , 0.00140167091906 , 0.00141482771173 , 0.00142791754942 , 0.00144094206154 , 0.0014539028153 , 0.00146680131887 , 0.00147963902447 , 0.00149241733116 , 0.00150513758749 , 0.00151780109399 , 0.00153040910553 , 0.00154296283341 , 0.00155546344754 , 0.00156791207827 , 0.00158030981824 , 0.00159265772411 , 0.00160495681814 , 0.00161720808976 , 0.00162941249692 , 0.00164157096757 , 0.00165368440081 , 0.00166575366823 , 0.00167777961494 , 0.00168976306076 , 0.00170170480119 , 0.00171360560841 , 0.00172546623219 , 0.00173728740083 , 0.00174906982191 , 0.00176081418314 , 0.00177252115315 , 0.00178419138212 , 0.00179582550256 , 0.00180742412988 , 18.0 }; // // Normalization w.r.t. p-value of phi=0 // // chi^2 double ygridArray [101] = { 0.0, 0.0513551, 0.177438, 0.35228, 0.561353, 0.795726, 1.04953, 1.3187, 1.60032, 1.89222, 2.19274, 2.50059, 2.81476, 3.13441, 3.45887, 3.78757, 4.12006, 4.45594, 4.79486, 5.13653, 5.48072, 5.82719, 6.17576, 6.52625, 6.87853, 7.23244, 7.58789, 7.94475, 8.30294, 8.66236, 9.02294, 9.38462, 9.74731, 10.111, 10.4755, 10.841, 11.2072, 11.5742, 11.9419, 12.3104, 12.6795, 13.0492, 13.4195, 13.7904, 14.1619, 14.5339, 14.9063, 15.2793, 15.6527, 16.0266, 16.4008, 16.7755, 17.1506, 17.5261, 17.9019, 18.2781, 18.6546, 19.0315, 19.4087, 19.7861, 20.1639, 20.542, 20.9203, 21.2989, 21.6778, 22.0569, 22.4362, 22.8158, 23.1957, 23.5757, 23.956, 24.3365, 24.7171, 25.098, 25.4791, 25.8604, 26.2418, 26.6235, 27.0053, 27.3872, 27.7694, 28.1517, 28.5342, 28.9168, 29.2996, 29.6825, 30.0655, 30.4487, 30.8321, 31.2155, 31.5992, 31.9829, 32.3667, 32.7507, 33.1348, 33.519, 33.9034, 34.2878, 34.6724, 35.0571, 350000.0 }; // Convert arrays to vectors. std::vector xgrid(xgridArray, xgridArray + sizeof xgridArray / sizeof xgridArray[0]); std::vector ygrid(ygridArray, ygridArray + sizeof ygridArray / sizeof ygridArray[0]); // Construct interpolated function, using GAMBIT base functions. auto dwarf_likelihood = daFunk::interp(“phi”, xgrid, ygrid);.

double fraction = *Dep::RD_fraction;

// Integate spectrum // (the zero velocity limit of the differential annihilation // cross-section as function of individual final state photons) double AnnYieldint = (*Dep::GA_Yield)-> set(“v”, 0.)->gsl_integration(“E”, 1, 100)->set_epsabs(0)->set_epsrel(1e-3)->bind()->eval(); logger() « “AnnYieldInt (1-100 GeV): " « AnnYieldint « EOM;

// Calculate phi-value double phi = AnnYieldint / 8. / M_PI * 1e26 * fraction * fraction;

// And return final likelihood result = 0.5*dwarf_likelihood->bind(“phi”)->eval(phi); logger() « “dwarf_likelihood: " « result « EOM; logger() « “phi: " « phi « EOM; }

module function which sets the Milky Way halo profile for the gamlike backend void set_gamLike_GC_halo(bool &result) { using namespace Pipes::set_gamLike_GC_halo;

daFunk::Funk profile = (Dep::GalacticHalo)->DensityProfile; auto r = daFunk::logspace(-3, 2, 100); auto rho = daFunk::logspace(-3, 2, 100); double dist = (Dep::GalacticHalo)->r_sun; for ( size_t i = 0; i<r.size(); i++ ) { rho[i] = profile->bind(“r”)->eval(r[i]); } BEreq::set_halo_profile(0, r, rho, byVal(dist)); result = true; }

/*! \brief Fermi LAT dwarf likelihoods, using gamLike backend.

Option version

<string> 

: Set Fermi LAT dwarf likelihood version (default: pass8)

function lnL_HESSGC_gamLike #

void lnL_HESSGC_gamLike(
    double & result
)

Option version

<string> 

: Set HESS GC likelihood version (default: spectral_externalJ)

function lnL_CTAGC_gamLike #

void lnL_CTAGC_gamLike(
    double & result
)

function lnL_FermiGC_gamLike #

void lnL_FermiGC_gamLike(
    double & result
)

Fermi LAT galactic center likelihoods, using gamLike backend.

Option version

<string> 

: Set Fermi LAT GC likelihood version (default: externalJ)

function lnL_oh2_Simple #

void lnL_oh2_Simple(
    double & result
)

Likelihood for cosmological relic density constraints. Default data: Omega_c h^2 = 0.11933 +/- 0.00091 (1 sigma), Gaussian. Planck TT,TE,EE+lowP+lensing+BAO 2018, arxiv:1807.06209 theory error: 5% S.B. 19/3/20 Updated with 2018 Planck results.

option oh2_fractional_theory_err: Relic density fractional 1 sigma theory error (default: 0.05)

option oh2_obs: Observed value of Omega h^2 (default: 0.11933)

option oh2_obserr: 1 sigma error on observed value of Omega h^2 (default: 0.00091)

Option profile_systematics: Use likelihood version that has been profiled over systematic errors (default false)

function lnL_oh2_upperlimit #

void lnL_oh2_upperlimit(
    double & result
)

Likelihood for cosmological relic density constraints, implemented as an upper limit only Default data: Omega_c h^2 = 0.11933 +/- 0.00091 (1 sigma), Gaussian. Planck TT,TE,EE+lowP+lensing+BAO 2018, arxiv:1807.06209 theory error: 5% S.B. 19/3/20 Updated with 2018 Planck results.

option oh2_fractional_theory_err: Relic density fractional 1 sigma theory error (default: 0.05)

option oh2_obs: Observed value of Omega h^2 (default: 0.11933)

option oh2_obserr: 1 sigma error on observed value of Omega h^2 (default: 0.00091)

Option profile_systematics: Use likelihood version that has been profiled over systematic errors (default false)

function lnL_sigmas_sigmal #

void lnL_sigmas_sigmal(
    double & result
)

Likelihoods for spin independent nuclear parameters. Follows treatment of Cline, et. al. Phys. Rev. D. 88, 055025 (2013) Default data: sigma_s = 43 +/- 8 MeV arXiv:1112.2435v1 sigma_l = 58 +/- 9 MeV.

Option sigmas_obs: Experimental value of sigma_s (default 43.)

Option sigmas_obserr: 1 sigma error on sigma_s (default 8.)

Option sigmal_obs: Experimental value of sigma_l (default 58.)

Option sigmal_obserr: 1 sigma error on sigma_l (default 9.)

Option profile_systematics: Use likelihood version that has been profiled over systematic errors (default false)

function lnL_deltaq #

void lnL_deltaq(
    double & result
)

Likelihoods for spin dependent nuclear parameters. Follows treatment of Akrami, et. al. JCAP04 (2011) 012. (Note that all deltaq are for proton.) Default data: a3 = deltau - deltad = 1.2723 +/- 0.0023 PDG 2015 lambda parameter from neutron beta decay a8 = deltau + deltad - 2*deltas = 0.585 +/- 0.025 http://arxiv.org/abs/hep-ph/0001046 deltas = -0.09 +/- 0.03 COMPASS: https://arxiv.org/abs/hep-ex/0609038.

Option a3_obs: Experimental value of a3 (default 1.2723)

Option a3_obserr: 1 sigma error on a3 (default 0.0023)

Option a8_obs: Experimental value of a8 (default 0.585)

Option a8_obserr: 1 sigma error on a8 (default 0.025)

Option deltas_obs: Experimental value of Delta_s (default -0.09)

Option deltas_obserr: 1 sigma error on Delta_s (default 0.03)

Option profile_systematics: Use likelihood version that has been profiled over systematic errors (default false)

function lnL_sigmapiN_Deltas_gTs_rs2 #

void lnL_sigmapiN_Deltas_gTs_rs2(
    double & result
)

Likelihoods for nuclear parameters (ChPT) as used in DirectDM v2.2.0 Default data: sigmapiN = 0.050 +/- 0.015 GeV Deltas = -0.035 +/- 0.009 gTs = -0.027 +/- 0.016 rs2 = -0.115 +/- 0.035 GeV^-2.

Use likelihood version that has been profiled over systematic errors (default false)

function lnL_rho0_lognormal #

void lnL_rho0_lognormal(
    double & result
)

Likelihoods for halo parameters. The likelihood for the local DM density follows a log normal distribution while for the velocities the distribution is Gaussian. For discussion of the default values for measured halo paramters and their errors, see JCAP04(2011)012.

Option rho0_obs: Best fit value for local dark matter density (default .4)

Option rho0_obserr: Error on local dark matter density (default .15)

Option profile_systematics: Use likelihood version that has been profiled over systematic errors (default false)

function lnL_vrot_gaussian #

void lnL_vrot_gaussian(
    double & result
)

Option vrot_obs: Best fit value for local disk rotational speed (default 235)

Option vrot_obserr: 1 sigma error on local disk rotational speed (default 20)

Option profile_systematics: Use likelihood version that has been profiled over systematic errors (default false)

function lnL_v0_gaussian #

void lnL_v0_gaussian(
    double & result
)

Option v0_obs: Best fit value for most-probable DM speed (default 235)

Option v0_obserr: 1 sigma error on most-probable DM speed (default 20)

Option profile_systematics: Use likelihood version that has been profiled over systematic errors (default false)

function lnL_vesc_gaussian #

void lnL_vesc_gaussian(
    double & result
)

Option vesc_obs: Best fit value for escape velocity (default 550)

Option vesc_obserr: 1 sigma error on escape velocity (default 35)

Option profile_systematics: Use likelihood version that has been profiled over systematic errors (default false)

function capture_rate_Sun_const_xsec_DS5 #

void capture_rate_Sun_const_xsec_DS5(
    double & result
)

Capture rate of regular dark matter in the Sun (no v-dependent or q-dependent cross-sections) (s^-1). DarkSUSY 5 version.

function capture_rate_Sun_const_xsec #

void capture_rate_Sun_const_xsec(
    double & result
)

Capture rate of regular dark matter in the Sun (no v-dependent or q-dependent cross-sections) (s^-1). DarkSUSY 6 version.

function capture_rate_Sun_const_xsec_capgen #

void capture_rate_Sun_const_xsec_capgen(
    double & result
)

Alternative to the darkSusy fct, using captn_specific from capgen instead.

function capture_rate_Sun_vnqn #

void capture_rate_Sun_vnqn(
    double & result
)

Capture rate for v^n and q^n-dependent cross sections. Isoscalar (same proton/neutron coupling) SD only couples to Hydrogen. See DirectDetection.cpp to see how to define the cross sections sigma_SD_p, sigma_SI_pi

function capture_rate_Sun_NREO #

void capture_rate_Sun_NREO(
    double & result
)

function equilibration_time_Sun #

void equilibration_time_Sun(
    double & result
)

Equilibration time for capture and annihilation of dark matter in the Sun (s)

function annihilation_rate_Sun #

void annihilation_rate_Sun(
    double & result
)

Annihilation rate of dark matter in the Sun (s^-1)

function nuyield_from_DS #

void nuyield_from_DS(
    nuyield_info & result
)

Neutrino yield function pointer and setup.

function IC79_loglike #

void IC79_loglike(
    double & result
)

Composite IceCube 79-string likelihood function.

function IC_loglike #

void IC_loglike(
    double & result
)

Complete composite IceCube likelihood function.

function DarkSUSY5_PointInit_LocalHalo_func #

void DarkSUSY5_PointInit_LocalHalo_func(
    bool & result
)

Function to set Local Halo Parameters in DarkSUSY (DS5 only)

Option v_earth: Keplerian velocity of the Earth around the Sun in km/s (default 29.78)

function DarkSUSY_PointInit_LocalHalo_func #

void DarkSUSY_PointInit_LocalHalo_func(
    bool & result
)

Function to set Local Halo Parameters in DarkSUSY (DS 6)

Option v_earth: Keplerian velocity of the Earth around the Sun in km/s (default 29.78)

function DarkMatter_ID_VectorSingletDM #

void DarkMatter_ID_VectorSingletDM(
    std::string & result
)

function DarkMatterConj_ID_VectorSingletDM #

void DarkMatterConj_ID_VectorSingletDM(
    std::string & result
)

function DD_couplings_VectorSingletDM_Z2 #

void DD_couplings_VectorSingletDM_Z2(
    DM_nucleon_couplings & result
)

Direct detection couplings for the VectorSingletDM_Z2 model.

function TH_ProcessCatalog_VectorSingletDM_Z2 #

void TH_ProcessCatalog_VectorSingletDM_Z2(
    DarkBit::TH_ProcessCatalog & result
)

Set up process catalog for the VectorSingletDM_Z2 model.

function DarkMatter_ID_EFT #

void DarkMatter_ID_EFT(
    std::string & result
)

DarkMatter_ID string for generic EFT dark matter.

function DarkMatterConj_ID_EFT #

void DarkMatterConj_ID_EFT(
    std::string & result
)

DarkMatterConj_ID string for generic EFT dark matter.

function NREO_couplings_from_parameters #

void NREO_couplings_from_parameters(
    NREO_DM_nucleon_couplings & NREO_couplings
)

function NREO_from_DD_couplings #

void NREO_from_DD_couplings(
    NREO_DM_nucleon_couplings & NREO_couplings
)

function DD_nonrel_WCs_flavscheme #

void DD_nonrel_WCs_flavscheme(
    NREO_DM_nucleon_couplings & result
)

Obtain the non-relativistic Wilson Coefficients from a set of model specific relativistic Wilson Coefficients from DirectDM in the flavour matching scheme (default 5 flavours). NR WCs defined at 2 GeV.

function ExtractDirectDMNuisanceParameters #

void ExtractDirectDMNuisanceParameters(
    map_str_dbl & result
)

Module function providing nuisance parameters for to be passed to DirectDM directly from the model parameters.

function TH_ProcessCatalog_WIMP_EFT #

void TH_ProcessCatalog_WIMP_EFT(
    DarkBit::TH_ProcessCatalog & result
)

Set up process catalog for a generic parameterisation of (two body) WIMP dark matter decays and annihilations.

Generic parameterisation of WIMP self-annihilation cross-section to various SM two-body final states

Attributes Documentation #

variable gagg_conversion #

const double gagg_conversion = 1.0E-9;

Supporting classes and functions for the axion module.

variable gaee_conversion #

const double gaee_conversion = 1.0E+13;

variable int_type_name #

const std::map< InterpolationOptions1D, std::string > int_type_name = { { InterpolationOptions1D::linear, "linear" }, { InterpolationOptions1D::cspline, "cspline"} };

variable int_2d_type_name #

const std::map< InterpolationOptions2D, std::string > int_2d_type_name = { { InterpolationOptions2D::bilinear, "bilinear" }, { InterpolationOptions2D::bicubic, "bicubic"} };

variable abs_prec #

const double abs_prec = 1.0E-1;

variable rel_prec #

const double rel_prec = 1.0E-6;

variable method #

const int method = 5;

variable colnames #

static std::vector< std::string > colnames {"mass", "log10x", 
                                             "e_L", "e_R", "e",
                                             "mu_L", "mu_R", "mu",
                                             "tau_L", "tau_R", "tau",
                                             "q", "c", "b", "t",
                                             "W_L", "W_T", "W",
                                             "Z_L", "Z_T", "Z",
                                             "g", "gamma", "h",
                                             "nu_e", "nu_mu", "nu_tau",
                                             "VV_to_4e", "VV_to_4mu", "VV_to_4tau"};

variable channels #

static std::vector< std::string > channels {"e", "mu", "tau",
                                              "q", "c", "b", "t",
                                              "W","Z", "g", "gamma", "h",
                                              "nu_e", "nu_mu", "nu_tau"};

Updated on 2023-06-26 at 21:36:52 +0000