Built on

J. Ghiglieri and U. A. Wiedemann, “Thermal width of the Higgs boson in hot QCD matter,” Phys. Rev. D
Original
1901
Earlier work this paper cites.
R. T. D’Agnolo, D. Pappadopulo, J. T. Ruderman, and P.-J. Wang, “Thermal Relic Targets with Exponentially Small Couplings,” Phys. Rev. Lett
Original
1906
Earlier work this paper cites.
A. Coogan, L. Morrison, and S. Profumo, “Hazma: A Python Toolkit for Studying Indirect Detection of Sub-GeV Dark Matter,” JCAP
Original
1907
Earlier work this paper cites.
M. Archidiacono, D. C. Hooper, R. Murgia, S. Bohr, J. Lesgourgues, and M. Viel, “Constraining Dark Matter-Dark Radiation interactions with CMB, BAO, and Lyman- α \alpha ,” JCAP
Original
1907
Earlier work this paper cites.
F. Brümmer, “Coscattering in next-to-minimal dark matter and split supersymmetry,” JHEP
Original
1910
Earlier work this paper cites.
S. Baumholzer, V. Brdar, P. Schwaller, and A. Segner, “Shining Light on the Scotogenic Model: Interplay of Colliders and Cosmology,” JHEP
Original
1912
Earlier work this paper cites.
H. A. Weldon, “Covariant Calculations at Finite Temperature: The Relativistic Plasma,” Phys. Rev. D
1982
Earlier work this paper cites.
M. Srednicki, R. Watkins, and K. A. Olive, “Calculations of Relic Densities in the Early Universe,” Nucl. Phys. B
1988
Earlier work this paper cites.
P. Gondolo and G. Gelmini, “Cosmic abundances of stable particles: Improved analysis,” Nucl. Phys. B
1991
Earlier work this paper cites.
J. Edsjo and P. Gondolo, “Neutralino relic density including coannihilations,” Phys. Rev. D
1997
Earlier work this paper cites.
J. McDonald, “Thermally generated gauge singlet scalars as selfinteracting dark matter,” Phys. Rev. Lett
2002
Earlier work this paper cites.
G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, “MicrOMEGAs: A Program for calculating the relic density in the MSSM,” Comput. Phys. Commun
2002
Earlier work this paper cites.
J. L. Feng, A. Rajaraman, and F. Takayama, “Superweakly interacting massive particles,” Phys. Rev. Lett
2003
Earlier work this paper cites.
K. Melnikov and V. G. Serbo, “Processes with the T channel singularity in the physical region: Finite beam sizes make cross-sections finite,” Nucl. Phys. B
2003
Earlier work this paper cites.
P. Agrawal, A. Parikh, and M. Reece, “Systematizing the Effective Theory of Self-Interacting Dark Matter,” JHEP
Original
2003
Earlier work this paper cites.
G. Belanger, A. Mjallal, and A. Pukhov, “Recasting direct detection limits within micrOMEGAs and implication for non-standard Dark Matter scenarios,” Eur. Phys. J. C
Original
2003
Earlier work this paper cites.
P. Gondolo, J. Edsjo, P. Ullio, L. Bergstrom, M. Schelke, and E. A. Baltz, “DarkSUSY: Computing supersymmetric dark matter properties numerically,” JCAP
2004
Earlier work this paper cites.
M. Hindmarsh and O. Philipsen, “WIMP dark matter and the QCD equation of state,” Phys. Rev. D
2005
Earlier work this paper cites.
D. Boyanovsky, K. Davey, and C. M. Ho, “Particle abundance in a thermal plasma: Quantum kinetics vs. Boltzmann equation,” Phys. Rev. D
2005
Earlier work this paper cites.
J. Hisano, S. Matsumoto, M. M. Nojiri, and O. Saito, “Non-perturbative effect on dark matter annihilation and gamma ray signature from galactic center,” Phys. Rev. D
2005
Earlier work this paper cites.
J. A. R. Cembranos, J. L. Feng, A. Rajaraman, and F. Takayama, “SuperWIMP solutions to small scale structure problems,” Phys. Rev. Lett
2005
Earlier work this paper cites.
G. Bélanger, A. Pukhov, C. E. Yaguna, and O. Zapata, “The Z 5
Original
2006
Earlier work this paper cites.
G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, “micrOMEGAs: Version 1.3,” Comput. Phys. Commun
2006
Earlier work this paper cites.
G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, “MicrOMEGAs 2.0: A Program to calculate the relic density of dark matter in a generic model,” Comput. Phys. Commun
2007
Earlier work this paper cites.
V. S. Rychkov and A. Strumia, “Thermal production of gravitinos,” Phys. Rev. D
2007
Earlier work this paper cites.

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2023

micrOMEGAs 6.0: N-component dark matter

Alguero, G., Belanger, G., Boudjema, F. et al.

Understand

micrOMEGAs is a numerical code to compute dark matter (DM) observables in generic extensions of the Standard Model of particle physics.

We present a new version of micrOMEGAs that includes a generalization of the Boltzmann equations governing the DM cosmic abundance evolution which can be solved to compute the relic density of N-component DM.
The direct and indirect detection rates in such scenarios take into account the relative contribution of each component such that constraints on the combined signal of all DM components can be imposed.
The co-scattering mechanism for DM production is also included, whereas the routines used to compute the relic density of feebly interacting particles have been improved in order to take into account the effect of thermal masses of t-channel particles.

Built on

J. Ghiglieri and U. A. Wiedemann, “Thermal width of the Higgs boson in hot QCD matter,” Phys. Rev. D
Original
1901
Earlier work this paper cites.
R. T. D’Agnolo, D. Pappadopulo, J. T. Ruderman, and P.-J. Wang, “Thermal Relic Targets with Exponentially Small Couplings,” Phys. Rev. Lett
Original
1906
Earlier work this paper cites.
A. Coogan, L. Morrison, and S. Profumo, “Hazma: A Python Toolkit for Studying Indirect Detection of Sub-GeV Dark Matter,” JCAP
Original
1907
Earlier work this paper cites.
M. Archidiacono, D. C. Hooper, R. Murgia, S. Bohr, J. Lesgourgues, and M. Viel, “Constraining Dark Matter-Dark Radiation interactions with CMB, BAO, and Lyman- α \alpha ,” JCAP
Original
1907
Earlier work this paper cites.
F. Brümmer, “Coscattering in next-to-minimal dark matter and split supersymmetry,” JHEP
Original
1910
Earlier work this paper cites.
S. Baumholzer, V. Brdar, P. Schwaller, and A. Segner, “Shining Light on the Scotogenic Model: Interplay of Colliders and Cosmology,” JHEP
Original
1912
Earlier work this paper cites.
H. A. Weldon, “Covariant Calculations at Finite Temperature: The Relativistic Plasma,” Phys. Rev. D
1982
Earlier work this paper cites.
M. Srednicki, R. Watkins, and K. A. Olive, “Calculations of Relic Densities in the Early Universe,” Nucl. Phys. B
1988
Earlier work this paper cites.
P. Gondolo and G. Gelmini, “Cosmic abundances of stable particles: Improved analysis,” Nucl. Phys. B
1991
Earlier work this paper cites.
J. Edsjo and P. Gondolo, “Neutralino relic density including coannihilations,” Phys. Rev. D
1997
Earlier work this paper cites.
J. McDonald, “Thermally generated gauge singlet scalars as selfinteracting dark matter,” Phys. Rev. Lett
2002
Earlier work this paper cites.
G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, “MicrOMEGAs: A Program for calculating the relic density in the MSSM,” Comput. Phys. Commun
2002
Earlier work this paper cites.
J. L. Feng, A. Rajaraman, and F. Takayama, “Superweakly interacting massive particles,” Phys. Rev. Lett
2003
Earlier work this paper cites.
K. Melnikov and V. G. Serbo, “Processes with the T channel singularity in the physical region: Finite beam sizes make cross-sections finite,” Nucl. Phys. B
2003
Earlier work this paper cites.
P. Agrawal, A. Parikh, and M. Reece, “Systematizing the Effective Theory of Self-Interacting Dark Matter,” JHEP
Original
2003
Earlier work this paper cites.
G. Belanger, A. Mjallal, and A. Pukhov, “Recasting direct detection limits within micrOMEGAs and implication for non-standard Dark Matter scenarios,” Eur. Phys. J. C
Original
2003
Earlier work this paper cites.
P. Gondolo, J. Edsjo, P. Ullio, L. Bergstrom, M. Schelke, and E. A. Baltz, “DarkSUSY: Computing supersymmetric dark matter properties numerically,” JCAP
2004
Earlier work this paper cites.
M. Hindmarsh and O. Philipsen, “WIMP dark matter and the QCD equation of state,” Phys. Rev. D
2005
Earlier work this paper cites.
D. Boyanovsky, K. Davey, and C. M. Ho, “Particle abundance in a thermal plasma: Quantum kinetics vs. Boltzmann equation,” Phys. Rev. D
2005
Earlier work this paper cites.
J. Hisano, S. Matsumoto, M. M. Nojiri, and O. Saito, “Non-perturbative effect on dark matter annihilation and gamma ray signature from galactic center,” Phys. Rev. D
2005
Earlier work this paper cites.
J. A. R. Cembranos, J. L. Feng, A. Rajaraman, and F. Takayama, “SuperWIMP solutions to small scale structure problems,” Phys. Rev. Lett
2005
Earlier work this paper cites.
G. Bélanger, A. Pukhov, C. E. Yaguna, and O. Zapata, “The Z 5
Original
2006
Earlier work this paper cites.
G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, “micrOMEGAs: Version 1.3,” Comput. Phys. Commun
2006
Earlier work this paper cites.
G. Belanger, F. Boudjema, A. Pukhov, and A. Semenov, “MicrOMEGAs 2.0: A Program to calculate the relic density of dark matter in a generic model,” Comput. Phys. Commun
2007
Earlier work this paper cites.
V. S. Rychkov and A. Strumia, “Thermal production of gravitinos,” Phys. Rev. D
2007
Earlier work this paper cites.