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Split SIMPs with Decays

We discuss a minimal realization of the strongly interacting massive particle (SIMP) framework. The model includes a dark copy of QCD with three colors and three light flavors. A massive dark photon, kinetically mixed with the Standard Model hypercharge, maintains kinetic equilibrium between the dar...

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Detalles Bibliográficos
Autores principales: Katz, Andrey, Salvioni, Ennio, Shakya, Bibhushan
Lenguaje:eng
Publicado: 2020
Materias:
Acceso en línea:https://dx.doi.org/10.1007/JHEP10(2020)049
http://cds.cern.ch/record/2722411
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author Katz, Andrey
Salvioni, Ennio
Shakya, Bibhushan
author_facet Katz, Andrey
Salvioni, Ennio
Shakya, Bibhushan
author_sort Katz, Andrey
collection CERN
description We discuss a minimal realization of the strongly interacting massive particle (SIMP) framework. The model includes a dark copy of QCD with three colors and three light flavors. A massive dark photon, kinetically mixed with the Standard Model hypercharge, maintains kinetic equilibrium between the dark and visible sectors. One of the dark mesons is necessarily unstable but long-lived, with potential impact on CMB observables. We show that an approximate “isospin” symmetry acting on the down-type quarks is an essential ingredient of the model. This symmetry stabilizes the dark matter and allows to split sufficiently the masses of the other states to suppress strongly their relic abundances. We discuss for the first time the SIMP cosmology with sizable mass splittings between all meson multiplets. We demonstrate that the SIMP mechanism remains efficient in setting the dark matter relic density, while CMB constraints on unstable relics can be robustly avoided. We also consider the phenomenological consequences of isospin breaking, including dark matter decay. Cosmological, astrophysical, and terrestrial probes are combined into a global picture of the parameter space. In addition, we outline an ultraviolet completion in the context of neutral naturalness, where confinement at the GeV scale is generic. We emphasize the general applicability of several novel features of the SIMP mechanism that we discuss here.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2020
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spelling cern-27224112021-11-12T20:18:27Zdoi:10.1007/JHEP10(2020)049http://cds.cern.ch/record/2722411engKatz, AndreySalvioni, EnnioShakya, BibhushanSplit SIMPs with Decaysastro-ph.HEAstrophysics and Astronomyastro-ph.COAstrophysics and Astronomyhep-phParticle Physics - PhenomenologyWe discuss a minimal realization of the strongly interacting massive particle (SIMP) framework. The model includes a dark copy of QCD with three colors and three light flavors. A massive dark photon, kinetically mixed with the Standard Model hypercharge, maintains kinetic equilibrium between the dark and visible sectors. One of the dark mesons is necessarily unstable but long-lived, with potential impact on CMB observables. We show that an approximate “isospin” symmetry acting on the down-type quarks is an essential ingredient of the model. This symmetry stabilizes the dark matter and allows to split sufficiently the masses of the other states to suppress strongly their relic abundances. We discuss for the first time the SIMP cosmology with sizable mass splittings between all meson multiplets. We demonstrate that the SIMP mechanism remains efficient in setting the dark matter relic density, while CMB constraints on unstable relics can be robustly avoided. We also consider the phenomenological consequences of isospin breaking, including dark matter decay. Cosmological, astrophysical, and terrestrial probes are combined into a global picture of the parameter space. In addition, we outline an ultraviolet completion in the context of neutral naturalness, where confinement at the GeV scale is generic. We emphasize the general applicability of several novel features of the SIMP mechanism that we discuss here.We discuss a minimal realization of the strongly interacting massive particle (SIMP) framework. The model includes a dark copy of QCD with three colors and three light flavors. A massive dark photon, kinetically mixed with the Standard Model hypercharge, maintains kinetic equilibrium between the dark and visible sectors. One of the dark mesons is necessarily unstable but long-lived, with potential impact on CMB observables. We show that an approximate "isospin" symmetry acting on the down-type quarks is an essential ingredient of the model. This symmetry stabilizes the dark matter and allows to split sufficiently the masses of the other states to suppress strongly their relic abundances. We discuss for the first time the SIMP cosmology with sizable mass splittings between all meson multiplets. We demonstrate that the SIMP mechanism remains efficient in setting the dark matter relic density, while CMB constraints on unstable relics can be robustly avoided. We also consider the phenomenological consequences of isospin breaking, including dark matter decay. Cosmological, astrophysical, and terrestrial probes are combined into a global picture of the parameter space. In addition, we outline an ultraviolet completion in the context of neutral naturalness, where confinement at the GeV scale is generic. We emphasize the general applicability of several novel features of the SIMP mechanism that we discuss here.arXiv:2006.15148CERN-TH-2020-107oai:cds.cern.ch:27224112020-06-26
spellingShingle astro-ph.HE
Astrophysics and Astronomy
astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
Katz, Andrey
Salvioni, Ennio
Shakya, Bibhushan
Split SIMPs with Decays
title Split SIMPs with Decays
title_full Split SIMPs with Decays
title_fullStr Split SIMPs with Decays
title_full_unstemmed Split SIMPs with Decays
title_short Split SIMPs with Decays
title_sort split simps with decays
topic astro-ph.HE
Astrophysics and Astronomy
astro-ph.CO
Astrophysics and Astronomy
hep-ph
Particle Physics - Phenomenology
url https://dx.doi.org/10.1007/JHEP10(2020)049
http://cds.cern.ch/record/2722411
work_keys_str_mv AT katzandrey splitsimpswithdecays
AT salvioniennio splitsimpswithdecays
AT shakyabibhushan splitsimpswithdecays