Abstract
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 percent.
- Received 6 January 2023
- Accepted 17 April 2023
DOI:https://doi.org/10.1103/PhysRevD.107.103508
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