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Title: The effect of dark matter and dark energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect

Abstract

The interaction between Dark Matter and Dark Energy has been proposed as a mechanism to alleviate the coincidence problem. We analyze its effects on the evolution of the gravitational and the peculiar velocity fields. We find that for different model parameters peculiar velocities vary from a factor five times smaller to two times larger than in the ΛCDM cosmological model at the same scales. We propose two new observables sensitive to such interactions based on their effect on the velocity field. We compare the effects on peculiar velocities with those on the Integrated Sachs-Wolfe effect demonstrating that velocities are more sensitive to the interaction. We show that the current upper limits on the amplitude of the kinetic Sunyaev-Zel'dovich power spectrum of temperature anisotropies provide constraints on the coupling within the dark sectors that are consistent with those obtained previously from the Cosmic Microwave Background and galaxy clusters. In particular, we show that Atacama Cosmology Telescope and South Pole Telescope data favor the decay of Dark Energy into Dark Matter, as required to solve the coincidence problem.

Authors:
; ;  [1];  [2]
  1. Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240 (China)
  2. Física Teórica, Universidad de Salamanca, 37008 Salamanca (Spain)
Publication Date:
OSTI Identifier:
22369882
Resource Type:
Journal Article
Resource Relation:
Journal Name: Journal of Cosmology and Astroparticle Physics; Journal Volume: 2013; Journal Issue: 12; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; AMPLITUDES; ANISOTROPY; COSMOLOGICAL MODELS; COSMOLOGY; COUPLING; LIMITING VALUES; NONLUMINOUS MATTER; RELICT RADIATION; TELESCOPES; VELOCITY

Citation Formats

Xu, Xiao-Dong, Wang, Bin, Zhang, Pengjie, and Atrio-Barandela, Fernando, E-mail: ammonitex@163.com, E-mail: wang_b@sjtu.edu.cn, E-mail: zhangpengjie@gmail.com, E-mail: atrio@usal.es. The effect of dark matter and dark energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect. United States: N. p., 2013. Web. doi:10.1088/1475-7516/2013/12/001.
Xu, Xiao-Dong, Wang, Bin, Zhang, Pengjie, & Atrio-Barandela, Fernando, E-mail: ammonitex@163.com, E-mail: wang_b@sjtu.edu.cn, E-mail: zhangpengjie@gmail.com, E-mail: atrio@usal.es. The effect of dark matter and dark energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect. United States. doi:10.1088/1475-7516/2013/12/001.
Xu, Xiao-Dong, Wang, Bin, Zhang, Pengjie, and Atrio-Barandela, Fernando, E-mail: ammonitex@163.com, E-mail: wang_b@sjtu.edu.cn, E-mail: zhangpengjie@gmail.com, E-mail: atrio@usal.es. 2013. "The effect of dark matter and dark energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect". United States. doi:10.1088/1475-7516/2013/12/001.
@article{osti_22369882,
title = {The effect of dark matter and dark energy interactions on the peculiar velocity field and the kinetic Sunyaev-Zel'dovich effect},
author = {Xu, Xiao-Dong and Wang, Bin and Zhang, Pengjie and Atrio-Barandela, Fernando, E-mail: ammonitex@163.com, E-mail: wang_b@sjtu.edu.cn, E-mail: zhangpengjie@gmail.com, E-mail: atrio@usal.es},
abstractNote = {The interaction between Dark Matter and Dark Energy has been proposed as a mechanism to alleviate the coincidence problem. We analyze its effects on the evolution of the gravitational and the peculiar velocity fields. We find that for different model parameters peculiar velocities vary from a factor five times smaller to two times larger than in the ΛCDM cosmological model at the same scales. We propose two new observables sensitive to such interactions based on their effect on the velocity field. We compare the effects on peculiar velocities with those on the Integrated Sachs-Wolfe effect demonstrating that velocities are more sensitive to the interaction. We show that the current upper limits on the amplitude of the kinetic Sunyaev-Zel'dovich power spectrum of temperature anisotropies provide constraints on the coupling within the dark sectors that are consistent with those obtained previously from the Cosmic Microwave Background and galaxy clusters. In particular, we show that Atacama Cosmology Telescope and South Pole Telescope data favor the decay of Dark Energy into Dark Matter, as required to solve the coincidence problem.},
doi = {10.1088/1475-7516/2013/12/001},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 12,
volume = 2013,
place = {United States},
year = 2013,
month =
}
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