Manual
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- Introduction
- General remarks on notation
- ac: Accelerator bounds
- an: Annihilation cross sections (general, 0 and )
- an1l: Annihilation cross sections (1-loop)
- Annihilation cross sections at 1-loop -- general
- Routine headers -- fortran files
- dsanggim.f
- dsanggimpar.f
- dsanggre.f
- dsanggrepar.f
- dsanglglim.f
- dsanglglre.f
- dsanzg.f
- dsanzgpar.f
- dsdilog.f
- dsdilogp.f
- dsfl1c1.f
- dsfl1c2.f
- dsfl2c1.f
- dsfl2c2.f
- dsfl3c1.f
- dsfl3c2.f
- dsfl4c1.f
- dsfl4c2.f
- dsi_12.f
- dsi_13.f
- dsi_14.f
- dsi_22.f
- dsi_23.f
- dsi_24.f
- dsi_32.f
- dsi_33.f
- dsi_34.f
- dsi_41.f
- dsi_42.f
- dsilp2.f
- dsj_1.f
- dsj_2.f
- dsj_3.f
- dslp2.f
- dspi1.f
- dspiw2.f
- dspiw2i.f
- dspiw3.f
- dspiw3i.f
- dsrepfbox.f
- dsrepgh.f
- dsrepw.f
- dsslc1.f
- dsslc2.f
- dssubka.f
- dssubkb.f
- dssubkc.f
- dsti_214.f
- dsti_224.f
- dsti_23.f
- dsti_33.f
- dsti_5.f
- anstu: t, u and s diagrams for ff-annihilation
- Annihilation amplitudes for fermion-fermion annihilation
- Routine headers -- fortran files
- dsansffsff.f
- dsansffsss.f
- dsansffssv.f
- dsansffsvs.f
- dsansffsvv.f
- dsansffvff.f
- dsansffvss.f
- dsansffvsv.f
- dsansffvvs.f
- dsansffvvv.f
- dsantfffss.f
- dsantfffssex.f
- dsantfffssin.f
- dsantfffsv.f
- dsantfffsvin.f
- dsantfffvs.f
- dsantfffvsex.f
- dsantfffvv.f
- dsantfffvvex.f
- dsantfffvvin.f
- dsantffsff.f
- dsanufffss.f
- dsanufffssin.f
- dsanufffsv.f
- dsanufffsvin.f
- dsanufffvs.f
- dsanufffvv.f
- dsanufffvvex.f
- dsanufffvvin.f
- dsanuffsff.f
- as: Annihilation cross sections (with sfermions)
- Annihilation cross sections with sfermions -- general
- Routine headers -- fortran files
- dsaschicasea.f
- dsaschicaseb.f
- dsaschicasec.f
- dsaschicased.f
- dsaschizero.f
- dsascolset.f
- dsasdepro.f
- dsasdwdcossfchi.f
- dsasdwdcossfsf.f
- dsasfer.f
- dsasfercode.f
- dsasfercol.f
- dsasfere.f
- dsasferecol.f
- dsasff.f
- dsasffcol.f
- dsasgbgb.f
- dsasgbgb1exp.f
- dsasgbgb2exp.f
- dsasgbhb.f
- dsashbhb.f
- dsaskinset.f
- dsaskinset1.f
- dsaskinset2.f
- dsaskinset3.f
- dsasphghb.f
- dsasscscsSHffb.f
- dsasscscsSHffbcol.f
- dsasscscsSVffb.f
- dsasscscsSVffbcol.f
- dsasscscsTCffb.f
- dsasscscsTCffbcol.f
- dsasscscTCff.f
- dsasscscTCffcol.f
- dsasscscUCff.f
- dsasscscUCffcol.f
- dsassfercode.f
- dsaswcomp.f
- bsg: b s
- b s -- theory
- b s -- routines
- Routine headers -- fortran files
- dsbsgalpha3.f
- dsbsgalpha3int.f
- dsbsgammafull.f
- dsbsgat0.f
- dsbsgat1.f
- dsbsgbofe.f
- dsbsgc41h2.f
- dsbsgc41susy.f
- dsbsgc70h2.f
- dsbsgc70susy.f
- dsbsgc71chisusy.f
- dsbsgc71h2.f
- dsbsgc71phi1susy.f
- dsbsgc71phi2susy.f
- dsbsgc71wsusy.f
- dsbsgc80h2.f
- dsbsgc80susy.f
- dsbsgc81chisusy.f
- dsbsgc81h2.f
- dsbsgc81phi1susy.f
- dsbsgc81phi2susy.f
- dsbsgc81wsusy.f
- dsbsgckm.f
- dsbsgd1td.f
- dsbsgd2d.f
- dsbsgd2td.f
- dsbsgd7chi1.f
- dsbsgd7chi2.f
- dsbsgd7h.f
- dsbsgd8chi1.f
- dsbsgd8chi2.f
- dsbsgd8h.f
- dsbsgeb.f
- dsbsgechi.f
- dsbsgeh.f
- dsbsget0.f
- dsbsgf71.f
- dsbsgf72.f
- dsbsgf73.f
- dsbsgf81.f
- dsbsgf82.f
- dsbsgf83.f
- dsbsgft0.f
- dsbsgft1.f
- dsbsgfxy.f
- dsbsgg.f
- dsbsgg7chi2.f
- dsbsgg7chij1.f
- dsbsgg7h.f
- dsbsgg7w.f
- dsbsgg8chi2.f
- dsbsgg8chij1.f
- dsbsgg8h.f
- dsbsgg8w.f
- dsbsggxy.f
- dsbsgh1x.f
- dsbsgh2xy.f
- dsbsgh3x.f
- dsbsghd.f
- dsbsghtd.f
- dsbsgkc.f
- dsbsgkt.f
- dsbsgmtmuw.f
- dsbsgmtmuwint.f
- dsbsgri.f
- dsbsgud.f
- dsbsgutd.f
- dsbsgwud.f
- dsbsgwxy.f
- dsbsgyt.f
- dsphi22a.f
- dsphi22b.f
- dsphi27a.f
- dsphi27b.f
- db: Anti-deuteron fluxes from the halo
- dd: Direct detection
- ep: Positron fluxes from the halo
- Positrons from the halo -- theory
- Positrons from the halo -- routines
- Routine headers -- fortran files
- dsembg.f
- dsepbg.f
- dsepdiff.f
- dsepdsigv_de.f
- dsepeecut.f
- dsepeeuncut.f
- dsepf.f
- dsepfrsm.f
- dsepgalpropdiff.f
- dsepgalpropig.f
- dsepgalpropig2.f
- dsepgalpropline.f
- dsephalodens2.f
- dsepideltavint.f
- dsepimage_sum.f
- dsepipol.f
- dsepkt.f
- dsepktdiff.f
- dsepktig.f
- dsepktig2.f
- dsepktline.f
- dseploghalodens2.f
- dsepmake_tables.f
- dsepmake_tables2.f
- dsepmsdiff.f
- dsepmsig.f
- dsepmsig2.f
- dsepmsline.f
- dsepmstable.f
- dseprsm.f
- dsepset.f
- dsepsigvdnde.f
- dsepspec.f
- dseptab.f
- dsepvvcut.f
- dsepvvuncut.f
- dsepwcut.f
- dsepwuncut.f
- dsgalpropig.f
- dsgalpropig2.f
- dsgalpropset.f
- ep2: Positron fluxes from the halo (alternative solution)
- ge: General routines
- ha: Halo annihilation yields
- hm: Halo models
- Halo models -- theory
- Halo model -- routines
- Routine headers -- fortran files
- dshmabgrho.f
- dshmaxiprob.f
- dshmaxirho.f
- dshmboerrho.f
- dshmboerrhoaxi.f
- dshmburrho.f
- dshmdfisotr.f
- dshmdfisotrnum.f
- dshmhaloprof.f
- dshmj.f
- dshmjave.f
- dshmjavegc.f
- dshmjavepar1.f
- dshmjavepar2.f
- dshmjavepar3.f
- dshmjavepar4.f
- dshmjavepar5.f
- dshmjpar1.f
- dshmn03rho.f
- dshmnumrho.f
- dshmrescale_rho.f
- dshmrho.f
- dshmrho2cylint.f
- dshmset.f
- dshmsphrho.f
- dshmudf.f
- dshmudfearth.f
- dshmudfearthtab.f
- dshmudfgauss.f
- dshmudfiso.f
- dshmudfnum.f
- dshmudfnumc.f
- dshmudftab.f
- dshmvelearth.f
- hr: Halo rates from annihilation
- ini: Initialization routines
- mu: Muon neutrino yields from annihilation in the Sun/Earth
- nt: Neutrino and muon rates from annihilation in the Sun/Earth
- Neutrinos from the Sun and Earth -- theory
- Neutrino yield from annihilations
- Evolution of the number density in the Earth/Sun
- Approximate capture rate expressions
- Earth and Sun composition
- More accurate capture rate expressions
- Accurate capture rates in the Earth for general velocity distributions
- Accurate capture rates for the Earth for a Maxwell-Boltzmann velocity distribution
- A possible new population of neutralinos
- Effects of WIMP diffusion in the solar system
- Neutrinos from Sun and Earth -- routines
- Routine headers -- fortran files
- dsai.f
- dsaip.f
- dsatm_mu.f
- dsbi.f
- dsbip.f
- dsff.f
- dsff2.f
- dsff3.f
- dsfff2.f
- dsfff3.f
- dsgauss1.f
- dshiprecint.f
- dshiprecint2.f
- dshonda.f
- dslnff.f
- dsntannrate.f
- dsntcapcom.f
- dsntcapearth.f
- dsntcapearth2.f
- dsntcapearthfull.f
- dsntcapearthnum.f
- dsntcapearthnumi.f
- dsntcapearthtab.f
- dsntcapsun.f
- dsntcapsunnum.f
- dsntcapsunnumi.f
- dsntcapsuntab.f
- dsntceint.f
- dsntceint2.f
- dsntcsint.f
- dsntcsint2.f
- dsntctabcreate.f
- dsntctabget.f
- dsntctabread.f
- dsntctabwrite.f
- dsntdiffrates.f
- dsntdkannrate.f
- dsntdkcapea.f
- dsntdkcapeafull.f
- dsntdkcapearth.f
- dsntdkcom.f
- dsntdkfbigu.f
- dsntdkfoveru.f
- dsntdkgtot10.f
- dsntdkka.f
- dsntdkyf.f
- dsntdqagse.f
- dsntdqagseb.f
- dsntdqk21.f
- dsntdqk21b.f
- dsntearthdens.f
- dsntearthdenscomp.f
- dsntearthmass.f
- dsntearthmassint.f
- dsntearthne.f
- dsntearthpot.f
- dsntearthpotint.f
- dsntearthvesc.f
- dsntedfunc.f
- dsntepfunc.f
- dsntfoveru.f
- dsntfoveruearth.f
- dsntismbkg.f
- dsntismrd.f
- dsntlitlf_e.f
- dsntlitlf_s.f
- dsntmoderf.f
- dsntmuonyield.f
- dsntnuism.f
- dsntnusun.f
- dsntrates.f
- dsntse.f
- dsntsefull.f
- dsntset.f
- dsntspfunc.f
- dsntss.f
- dsntsunbkg.f
- dsntsuncdens.f
- dsntsuncdensint.f
- dsntsuncdfunc.f
- dsntsundens.f
- dsntsundenscomp.f
- dsntsunmass.f
- dsntsunmfrac.f
- dsntsunne.f
- dsntsunne2x.f
- dsntsunpot.f
- dsntsunpotint.f
- dsntsunread.f
- dsntsunvesc.f
- dsntsunx2z.f
- dsntsunz2x.f
- Neutrinos from the Sun and Earth -- theory
- pb: Antiproton fluxes from the halo
- Antiprotons -- theory
- Antiprotons from the halo -- routines
- Routine headers -- fortran files
- dspbaddterm.f
- dspbbeupargc.f
- dspbbeupargs.f
- dspbbeuparh.f
- dspbbeuparm.f
- dspbcharpar1.f
- dspbcharpar2.f
- dspbgalpropdiff.f
- dspbgalpropig.f
- dspbgalpropig2.f
- dspbkdiff.f
- dspbkdiffm.f
- dspbset.f
- dspbsigmavpbar.f
- dspbtd15.f
- dspbtd15beu.f
- dspbtd15beucl.f
- dspbtd15beuclsp.f
- dspbtd15beum.f
- dspbtd15char.f
- dspbtd15comp.f
- dspbtd15point.f
- dspbtd15x.f
- dspbtpb.f
- rd: Relic density routines (general)
- Relic density -- theoretical background
- Relic density -- numerical integration of the density equation
- Relic density -- routines
- Routine headers -- fortran files
- dsrdaddpt.f
- dsrdcom.f
- dsrddof150.f
- dsrddpmin.f
- dsrdens.f
- dsrdeqn.f
- dsrdfunc.f
- dsrdfuncs.f
- dsrdlny.f
- dsrdnormlz.f
- dsrdqad.f
- dsrdqrkck.f
- dsrdrhs.f
- dsrdspline.f
- dsrdstart.f
- dsrdtab.f
- dsrdthav.f
- dsrdthclose.f
- dsrdthlim.f
- dsrdthtest.f
- dsrdwdwdcos.f
- dsrdwfunc.f
- dsrdwintp.f
- dsrdwintpch.f
- dsrdwintprint.f
- dsrdwintrp.f
- dsrdwprint.f
- dsrdwres.f
- rge: mSUGRA interface (Isasugra) to DarkSUSY
- rn: Relic density of neutralinos (wrapper for rd routines)
- su: General SUSY model setup: masses, vertices etc
- Supersymmetric model
- General supersymmetry -- routines
- Routine headers -- fortran files
- dsb0loop.f
- dschasct.f
- dsfeynhiggsfast.f
- dsfindmtmt.f
- dsg0loop.f
- dsg4set.f
- dsg4set12.f
- dsg4set1234.f
- dsg4set13.f
- dsg4set23.f
- dsg4set34.f
- dsg4setc.f
- dsg4setc12.f
- dsg4setc1234.f
- dsg4setc13.f
- dsg4setc23.f
- dsg4setc34.f
- dsgive_model.f
- dshgfu.f
- dshigferqcd.f
- dshigsct.f
- dshigwid.f
- dshlf2.f
- dshlf3.f
- dsmodelsetup.f
- dsmqpole1loop.f
- dsneusct.f
- dspole.f
- dsprep.f
- dsqindx.f
- dsralph3.f
- dsralph31loop.f
- dsrghm.f
- dsrmq.f
- dsrmq1loop.f
- dssettopmass.f
- dssfesct.f
- dsspectrum.f
- dssuconst.f
- dssusy.f
- dsvertx.f
- dsvertx1.f
- dsvertx3.f
- dswhwarn.f
- dswspectrum.f
- dswunph.f
- dswvertx.f
- g4p.f
- suspect: mSUGRA interface (suspect) to DarkSUSY
- xcern: CERN routines needed by DarkSUSY
- xcmlib: CMLIB routines needed by DarkSUSY
- xfeynhiggs: FeynHiggs interface to DarkSUSY
- xhdecay: HDecay interface to DarkSUSY
- Acknowledgements
- Bibliography