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Title: Exploring dark matter microphysics with galaxy surveys

Abstract

We use present cosmological observations and forecasts of future experiments to illustrate the power of large-scale structure (LSS) surveys in probing dark matter (DM) microphysics and unveiling potential deviations from the standard ΛCDM scenario. To quantify this statement, we focus on an extension of ΛCDM with DM-neutrino scattering, which leaves a distinctive imprint on the angular and matter power spectra. After finding that future CMB experiments (such as COrE+) will not significantly improve the constraints set by the Planck satellite, we show that the next generation of galaxy clustering surveys (such as DESI) could play a leading role in constraining alternative cosmologies and even have the potential to make a discovery. Typically we find that DESI would be an order of magnitude more sensitive to DM interactions than Planck, thus probing effects that until now have only been accessible via N-body simulations.

Authors:
;  [1]; ; ;  [2]
  1. Instituto de Física Corpuscular (IFIC), CSIC-Universitat de València, Apartado de Correos 22085, E-46071 Valencia (Spain)
  2. Institute for Particle Physics Phenomenology (IPPP), Durham University, South Road, Durham DH1 3LE (United Kingdom)
Publication Date:
OSTI Identifier:
22525388
Resource Type:
Journal Article
Resource Relation:
Journal Name: Journal of Cosmology and Astroparticle Physics; Journal Volume: 2015; Journal Issue: 09; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; COMPUTERIZED SIMULATION; COSMOLOGICAL CONSTANT; COSMOLOGY; ENERGY SPECTRA; GALAXIES; LIMITING VALUES; NEUTRINOS; NONLUMINOUS MATTER; POTENTIALS; PROBES; SATELLITES; SCATTERING

Citation Formats

Escudero, Miguel, Mena, Olga, Vincent, Aaron C., Wilkinson, Ryan J., and Boehm, Céline, E-mail: miguel.Escudero@uv.es, E-mail: omena@ific.uv.es, E-mail: aaron.vincent@durham.ac.uk, E-mail: ryan.wilkinson@durham.ac.uk, E-mail: c.m.boehm@durham.ac.uk. Exploring dark matter microphysics with galaxy surveys. United States: N. p., 2015. Web. doi:10.1088/1475-7516/2015/09/034.
Escudero, Miguel, Mena, Olga, Vincent, Aaron C., Wilkinson, Ryan J., & Boehm, Céline, E-mail: miguel.Escudero@uv.es, E-mail: omena@ific.uv.es, E-mail: aaron.vincent@durham.ac.uk, E-mail: ryan.wilkinson@durham.ac.uk, E-mail: c.m.boehm@durham.ac.uk. Exploring dark matter microphysics with galaxy surveys. United States. doi:10.1088/1475-7516/2015/09/034.
Escudero, Miguel, Mena, Olga, Vincent, Aaron C., Wilkinson, Ryan J., and Boehm, Céline, E-mail: miguel.Escudero@uv.es, E-mail: omena@ific.uv.es, E-mail: aaron.vincent@durham.ac.uk, E-mail: ryan.wilkinson@durham.ac.uk, E-mail: c.m.boehm@durham.ac.uk. 2015. "Exploring dark matter microphysics with galaxy surveys". United States. doi:10.1088/1475-7516/2015/09/034.
@article{osti_22525388,
title = {Exploring dark matter microphysics with galaxy surveys},
author = {Escudero, Miguel and Mena, Olga and Vincent, Aaron C. and Wilkinson, Ryan J. and Boehm, Céline, E-mail: miguel.Escudero@uv.es, E-mail: omena@ific.uv.es, E-mail: aaron.vincent@durham.ac.uk, E-mail: ryan.wilkinson@durham.ac.uk, E-mail: c.m.boehm@durham.ac.uk},
abstractNote = {We use present cosmological observations and forecasts of future experiments to illustrate the power of large-scale structure (LSS) surveys in probing dark matter (DM) microphysics and unveiling potential deviations from the standard ΛCDM scenario. To quantify this statement, we focus on an extension of ΛCDM with DM-neutrino scattering, which leaves a distinctive imprint on the angular and matter power spectra. After finding that future CMB experiments (such as COrE+) will not significantly improve the constraints set by the Planck satellite, we show that the next generation of galaxy clustering surveys (such as DESI) could play a leading role in constraining alternative cosmologies and even have the potential to make a discovery. Typically we find that DESI would be an order of magnitude more sensitive to DM interactions than Planck, thus probing effects that until now have only been accessible via N-body simulations.},
doi = {10.1088/1475-7516/2015/09/034},
journal = {Journal of Cosmology and Astroparticle Physics},
number = 09,
volume = 2015,
place = {United States},
year = 2015,
month = 9
}
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