Impact of the vector dark matter on polarization of the CMB photon

被引：4
作者：
Vamegh, S. Al Modares [1 ]
Haghighat, M. [1 ,2 ]
Mahmoudi, S. [1 ]
Mohammadi, R. [3 ,4 ]
机构：
[1] Shiraz Univ, Dept Phys, Shiraz 71454, Iran
[2] Islamic World Sci Citat Ctr, Shiraz 7194694173, Iran
[3] Iranian Natl Sci & Technol Museum INMOST, Tehran 1136914611, Iran
[4] Inst Res Fundamental Sci IPM, Sch Astron, Tehran 193955531, Iran
来源：
PHYSICAL REVIEW D | 2019年 / 100卷 / 10期
关键词：
MASSIVE PARTICLES; CONSTRAINTS; LINE;
D O I：
10.1103/PhysRevD.100.103024
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We consider a vector dark matter (VDM) with a direct coupling with photon. We examine the effect of such an interaction on the CMB polarization to put new constrains on the properties of the DM particles. We show that a partially polarized VDM of the order of temperature fluctuation with a quadrupole distribution leads to a valuable circular polarization (CP) for the CMB. In different DM-models the DM-masses range from few eV to a few TeV. We show that the CP angular power spectrum depends on the mass of VDM as Co-Vl(S) proportional to 1/m(V)(6) such that for m(V) = 10 eV-1 keV, the CP angular power spectrum is Co-Vl(S) similar or equal to 10(3)-10(-11) nK(2). Therefore, the light VDM with masses less than 10 eV leads to an unexpected very large CP which can be excluded from the acceptable range of the VDM masses.
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页数：21
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