Phenomenology of self-interacting dark matter in a matter-dominated universe
Open Access
- 31 January 2019
- journal article
- research article
- Published by Springer Nature in The European Physical Journal C
- Vol. 79 (2) , 1-19
Abstract
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Funding Information
- Universidad Antonio Narino (2017239, 2018204)
- Consejo Superior de Investigaciones Científicas (FPA2017-84543-P)
- H2020 Marie Sklodowska-Curie Actions (674896, 690575)
- Simons Foundation
- Fundação para a Ciência e a Tecnologia (PD/BD/114453/2016)
- Science and Technology Facilities Council (ST/J001546/1)
This publication has 129 references indexed in Scilit:
- Cosmological simulations with self-interacting dark matter – II. Halo shapes versus observationsMonthly Notices of the Royal Astronomical Society, 2013
- Cosmological simulations with self-interacting dark matter – I. Constant-density cores and substructureMonthly Notices of the Royal Astronomical Society, 2013
- New constraints on the reheating temperature of the universe after WMAP-5Astroparticle Physics, 2008
- Oscillation effects on thermalization of the neutrinos in the universe with low reheating temperaturePhysical Review D, 2005
- What is the lowest possible reheating temperature?Physical Review D, 2004
- Direct Constraints on the Dark Matter Self‐Interaction Cross Section from the Merging Galaxy Cluster 1E 0657−56The Astrophysical Journal, 2004
- Thermally Generated Gauge Singlet Scalars as Self-Interacting Dark MatterPhysical Review Letters, 2002
- Equilibrium state of a self-interacting scalar field in the de Sitter backgroundPhysical Review D, 1994
- Observational and theoretical constraints on singular dark matter halosThe Astrophysical Journal, 1994
- Self-interacting dark matterThe Astrophysical Journal, 1992