Cosmological imprints of non-thermalized dark matter

Quentin Decant; Jan Heisig; Deanna C. Hooper; Laura Lopez-Honorez

doi:10.22323/1.398.0171

Cosmological imprints of non-thermalized dark matter

Quentin Decant, Jan Heisig, Deanna C. Hooper, Laura Lopez-Honorez

Fysiikan tutkimuslaitos

Tutkimustuotos: Artikkelijulkaisu › Konferenssiartikkeli › Tieteellinen › vertaisarvioitu

Abstrakti

Non-thermalized dark matter is a cosmologically viable alternative to the widely studied weakly interacting massive particle. We study the evolution of the dark matter phase-space distributions arising from freeze-in and superWIMP production as well as the combination of both. Utilizing our implementation in class, we investigate the cosmological imprints on the matter power spectrum, constrained by Lyman-a forest observations. For the explicit example of a colored t-channel mediator model, we explore the cosmologically allowed parameter space highlighting the interplay of Lyman-a constraints with those from Big Bang Nucleosynthesis and the LHC.

Alkuperäiskieli	englanti
Artikkeli	171
Lehti	Proceedings of Science
Vuosikerta	398
Sivumäärä	6
ISSN	1824-8039
DOI - pysyväislinkit	https://doi.org/10.22323/1.398.0171
Tila	Julkaistu - 2022
OKM-julkaisutyyppi	A4 Artikkeli konferenssijulkaisuussa
Tapahtuma	2021 European Physical Society Conference on High Energy Physics, EPS-HEP 2021 - Virtual, Online Kesto: 26 heinäk. 2021 → 30 heinäk. 2021

Lisätietoja

Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)

Tieteenalat

114 Fysiikka

Pääsy asiakirjaan

10.22323/1.398.0171Lisenssi: CC BY-NC-ND

EPS-HEP2021_171Lopullinen julkaistu versio, 758 KBLisenssi: CC BY-NC-ND

Siteeraa tätä

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abstract = "Non-thermalized dark matter is a cosmologically viable alternative to the widely studied weakly interacting massive particle. We study the evolution of the dark matter phase-space distributions arising from freeze-in and superWIMP production as well as the combination of both. Utilizing our implementation in class, we investigate the cosmological imprints on the matter power spectrum, constrained by Lyman-a forest observations. For the explicit example of a colored t-channel mediator model, we explore the cosmologically allowed parameter space highlighting the interplay of Lyman-a constraints with those from Big Bang Nucleosynthesis and the LHC.",

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author = "Quentin Decant and Jan Heisig and Hooper, {Deanna C.} and Laura Lopez-Honorez",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0); 2021 European Physical Society Conference on High Energy Physics, EPS-HEP 2021 ; Conference date: 26-07-2021 Through 30-07-2021",

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TY - JOUR

T1 - Cosmological imprints of non-thermalized dark matter

AU - Decant, Quentin

AU - Heisig, Jan

AU - Hooper, Deanna C.

AU - Lopez-Honorez, Laura

N1 - Publisher Copyright: © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)

PY - 2022

Y1 - 2022

N2 - Non-thermalized dark matter is a cosmologically viable alternative to the widely studied weakly interacting massive particle. We study the evolution of the dark matter phase-space distributions arising from freeze-in and superWIMP production as well as the combination of both. Utilizing our implementation in class, we investigate the cosmological imprints on the matter power spectrum, constrained by Lyman-a forest observations. For the explicit example of a colored t-channel mediator model, we explore the cosmologically allowed parameter space highlighting the interplay of Lyman-a constraints with those from Big Bang Nucleosynthesis and the LHC.

AB - Non-thermalized dark matter is a cosmologically viable alternative to the widely studied weakly interacting massive particle. We study the evolution of the dark matter phase-space distributions arising from freeze-in and superWIMP production as well as the combination of both. Utilizing our implementation in class, we investigate the cosmological imprints on the matter power spectrum, constrained by Lyman-a forest observations. For the explicit example of a colored t-channel mediator model, we explore the cosmologically allowed parameter space highlighting the interplay of Lyman-a constraints with those from Big Bang Nucleosynthesis and the LHC.

KW - 114 Physical sciences

U2 - 10.22323/1.398.0171

DO - 10.22323/1.398.0171

M3 - Conference article

AN - SCOPUS:85129437769

SN - 1824-8039

VL - 398

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 171

T2 - 2021 European Physical Society Conference on High Energy Physics, EPS-HEP 2021

Y2 - 26 July 2021 through 30 July 2021

ER -