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We revisit the non-thermal dark matter (DM) production during the thermalization and reheating era after inflation.
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A. Kurkela and U. A. Wiedemann, “Picturing perturbative parton cascades in QCD matter,”
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2003
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P. Jaikumar and A. Mazumdar, “Postinflationary thermalization and hadronization: QCD based approach,”
2004
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G. B. Gelmini and P. Gondolo, “Neutralino with the right cold dark matter abundance in (almost) any supersymmetric model,”
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2010
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A. Kurkela and G. D. Moore, “Thermalization in Weakly Coupled Nonabelian Plasmas,”
2011
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2012
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K. Mukaida and K. Nakayama, “Dynamics of oscillating scalar field in thermal environment,”
2013
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2015
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2015
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2016
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A. Soni and Y. Zhang, “Hidden SU(N) Glueball Dark Matter,”
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K. Benakli, Y. Chen, E. Dudas, and Y. Mambrini, “Minimal model of gravitino dark matter,”
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E. Dudas, Y. Mambrini, and K. Olive, “Case for an EeV Gravitino,”
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M. Drees and F. Hajkarim, “Dark Matter Production in an Early Matter Dominated Era,”
2018
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M. A. G. Garcia and M. A. Amin, “Prethermalization production of dark matter,”
2018
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