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Relic abundance of MeV millicharged particles. / Dolgov, A. D.; Rudenko, A. S.

в: Journal of Experimental and Theoretical Physics, Том 124, № 4, 01.04.2017, стр. 564-569.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Dolgov, AD & Rudenko, AS 2017, 'Relic abundance of MeV millicharged particles', Journal of Experimental and Theoretical Physics, Том. 124, № 4, стр. 564-569. https://doi.org/10.1134/S1063776117030116

APA

Vancouver

Dolgov AD, Rudenko AS. Relic abundance of MeV millicharged particles. Journal of Experimental and Theoretical Physics. 2017 апр. 1;124(4):564-569. doi: 10.1134/S1063776117030116

Author

Dolgov, A. D. ; Rudenko, A. S. / Relic abundance of MeV millicharged particles. в: Journal of Experimental and Theoretical Physics. 2017 ; Том 124, № 4. стр. 564-569.

BibTeX

@article{dcca3765095d4b998b7846776cd8cce6,
title = "Relic abundance of MeV millicharged particles",
abstract = "The relic abundance of light millicharged particles (MCPs) with the electric charge e′ = 5 × 10–5e and with the mass slightly below or above the electron mass is calculated. The abundance depends on the mass ratio η = mX/me and for η < 1 can be high enough to allow MCPs to be the cosmological dark matter or to make a noticeable contribution to it. On the other hand, for η ≳ 1 the cosmological energy density of MCPs can be quite low, ΩXh0 2 ≈ 0.02 for scalar MCPs, and ΩXh0 2 ≈ 0.001 for spin 1/2 fermions. But even the lowest value of ΩXh0 2 is in tension with several existing limits on the MCP abundances and parameters. However, these limits have been derived under some natural or reasonable assumptions on the properties of MCPs. If these assumptions are relaxed, a patch in the mass–charge plot of MCPs may appear, permitting them to be dark matter particles.",
keywords = "DARK-MATTER, BOUNDS, LIMITS",
author = "Dolgov, {A. D.} and Rudenko, {A. S.}",
year = "2017",
month = apr,
day = "1",
doi = "10.1134/S1063776117030116",
language = "English",
volume = "124",
pages = "564--569",
journal = "Journal of Experimental and Theoretical Physics",
issn = "1063-7761",
publisher = "Maik Nauka-Interperiodica Publishing",
number = "4",

}

RIS

TY - JOUR

T1 - Relic abundance of MeV millicharged particles

AU - Dolgov, A. D.

AU - Rudenko, A. S.

PY - 2017/4/1

Y1 - 2017/4/1

N2 - The relic abundance of light millicharged particles (MCPs) with the electric charge e′ = 5 × 10–5e and with the mass slightly below or above the electron mass is calculated. The abundance depends on the mass ratio η = mX/me and for η < 1 can be high enough to allow MCPs to be the cosmological dark matter or to make a noticeable contribution to it. On the other hand, for η ≳ 1 the cosmological energy density of MCPs can be quite low, ΩXh0 2 ≈ 0.02 for scalar MCPs, and ΩXh0 2 ≈ 0.001 for spin 1/2 fermions. But even the lowest value of ΩXh0 2 is in tension with several existing limits on the MCP abundances and parameters. However, these limits have been derived under some natural or reasonable assumptions on the properties of MCPs. If these assumptions are relaxed, a patch in the mass–charge plot of MCPs may appear, permitting them to be dark matter particles.

AB - The relic abundance of light millicharged particles (MCPs) with the electric charge e′ = 5 × 10–5e and with the mass slightly below or above the electron mass is calculated. The abundance depends on the mass ratio η = mX/me and for η < 1 can be high enough to allow MCPs to be the cosmological dark matter or to make a noticeable contribution to it. On the other hand, for η ≳ 1 the cosmological energy density of MCPs can be quite low, ΩXh0 2 ≈ 0.02 for scalar MCPs, and ΩXh0 2 ≈ 0.001 for spin 1/2 fermions. But even the lowest value of ΩXh0 2 is in tension with several existing limits on the MCP abundances and parameters. However, these limits have been derived under some natural or reasonable assumptions on the properties of MCPs. If these assumptions are relaxed, a patch in the mass–charge plot of MCPs may appear, permitting them to be dark matter particles.

KW - DARK-MATTER

KW - BOUNDS

KW - LIMITS

UR - http://www.scopus.com/inward/record.url?scp=85019653722&partnerID=8YFLogxK

U2 - 10.1134/S1063776117030116

DO - 10.1134/S1063776117030116

M3 - Article

AN - SCOPUS:85019653722

VL - 124

SP - 564

EP - 569

JO - Journal of Experimental and Theoretical Physics

JF - Journal of Experimental and Theoretical Physics

SN - 1063-7761

IS - 4

ER -

ID: 9053564