دورية أكاديمية

micrOMEGAs 6.0: N-component dark matter

التفاصيل البيبلوغرافية
العنوان: micrOMEGAs 6.0: N-component dark matter
المؤلفون: Alguero, G, Belanger, G, Boudjema, F, Chakraborti, S, Goudelis, A, Kraml, S, Mjallal, A, Pukhov, A
المساهمون: Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Laboratoire d'Annecy-le-Vieux de Physique Théorique (LAPTH), Université Savoie Mont Blanc (USMB Université de Savoie Université de Chambéry )-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique de Clermont (LPC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Clermont Auvergne (UCA)
المصدر: Comput.Phys.Commun. ; https://hal.science/hal-04385542Test ; Comput.Phys.Commun., 2024, 299, pp.109133. ⟨10.1016/j.cpc.2024.109133⟩
بيانات النشر: HAL CCSD
سنة النشر: 2024
المجموعة: Université Grenoble Alpes: HAL
مصطلحات موضوعية: dark matter, production, effect, thermal, photon, spectrum, mass, particle, interaction, relic density, annihilation, meson, Boltzmann equation, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]
الوصف: International audience ; 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. Finally, the tables for the DM self-annihilation - induced photon spectra have been extended down to DM masses of 110 MeV, and they now include annihilation channels into light mesons.
نوع الوثيقة: article in journal/newspaper
اللغة: English
العلاقة: info:eu-repo/semantics/altIdentifier/arxiv/2312.14894; hal-04385542; https://hal.science/hal-04385542Test; ARXIV: 2312.14894; INSPIRE: 2740358
DOI: 10.1016/j.cpc.2024.109133
الإتاحة: https://doi.org/10.1016/j.cpc.2024.109133Test
https://hal.science/hal-04385542Test
رقم الانضمام: edsbas.63BC51E8
قاعدة البيانات: BASE