Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование
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 изданиях › статья › Рецензирование
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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