Validating dark energy models using the polarized Sunyaev-Zel'dovich effect with large-angle CMB temperature and E-mode polarization anisotropies

被引：0
|
作者：
Kondo, Hiroto [1 ]
Ichiki, Kiyotomo [1 ,2 ,3 ]
Tashiro, Hiroyuki [1 ,4 ]
Hasegawa, Kenji [1 ]
机构：
[1] Nagoya Univ, Grad Sch Sci, Div Particle & Astrophys Sci, Chikusa Ku, Nagoya, Aichi 4648602, Japan
[2] Nagoya Univ, Kobayashi Maskawa Inst Origin Particles & Universe, Chikusa Ku, Nagoya, Aichi 4648602, Japan
[3] Nagoya Univ, Inst Adv Res, Chikusa Ku, Nagoya, Aichi 4648602, Japan
[4] Sojo Univ, Ctr Educ & Innovat, Nishi Ku, Ikeda, Kumamoto 8600082, Japan
来源：
PHYSICAL REVIEW D | 2023年 / 107卷 / 10期
关键词：
PROBE;
D O I：
10.1103/PhysRevD.107.103508
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The tomography of the polarized Sunyaev-Zeldvich effect due to free electrons of galaxy clusters can be used to constrain the nature of dark energy because Cosmic Microwave Background quadrupoles at different redshifts as the polarization source are sensitive to the Integrated Sachs-Wolfe effect. Here we show that the low multipoles of the temperature and E-mode polarization anisotropies from the all-sky CMB can improve the constraint further through the correlation between them and the CMB quadrupoles viewed from the galaxy clusters. Using a Monte Carlo simulation, we find that low multipoles of the temperature and E-mode polarization anisotropies potentially improve the constraint on the equation of state of dark energy parameter by about 17 percent.
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页数：7
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