Dark radiation and dark matter in supersymmetric axion models with high reheating temperature

Peter Graf; Frank Daniel Steffen

doi:10.1088/1475-7516/2013/12/047

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arXiv · 1302.2143

Dark radiation and dark matter in supersymmetric axion models with high reheating temperature

Peter Graf·Frank Daniel Steffen

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Abstract

Recent studies of the cosmic microwave background, large scale structure, and big bang nucleosynthesis (BBN) show trends towards extra radiation. Within the framework of supersymmetric hadronic axion models, we explore two high-reheating-temperature scenarios that can explain consistently extra radiation and cold dark matter (CDM), with the latter residing either in gravitinos or in axions. In the gravitino CDM case, axions from decays of thermal saxions provide extra radiation already prior to BBN and decays of axinos with a cosmologically required TeV-scale mass can produce extra entropy. In the axion CDM case, cosmological constraints are respected with light eV-scale axinos and weak-scale gravitinos that decay into axions and axinos. These decays lead to late extra radiation which can coexist with the early contributions from saxion decays. Recent results of the Planck satellite probe extra radiation at late times and thereby both scenarios. Further tests are the searches for axions at ADMX and for supersymmetric particles at the LHC.

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Peter Graf, Frank Daniel Steffen. 2013-10-04. Dark radiation and dark matter in supersymmetric axion models with high reheating temperature. https://doi.org/10.1088/1475-7516%2F2013%2F12%2F047

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