On large lepton number asymmetries of the Universe

Abstract

A large lepton number asymmetry of $\mathcal{O}(0.1-1)$ at present universe might not only be allowed but also necessary for consistency among cosmological data. We show that, if a sizeable lepton number asymmetry were produced before the electroweak phase transition, the requirement for not producing too much baryon number asymmetry through sphalerons processes, forces the high scale lepton number asymmetry to be larger than about $30$. Therefore a mild entropy release causing $\mathcal{O}(10-100)$ suppression of pre-existing particle density should take place, when the background temperature of the universe is around $T=\mathcal{O}(10^{-2}-10^2)\mathrm{GeV}$ for a large but experimentally consistent asymmetry to be present today. We also show that such a mild entropy production can be obtained by the late-time decays of the saxion, constraining the parameters of the Peccei-Quinn sector such as the mass and the vacuum expectation value of the saxion field to be $m_{\varphi }\gtrsim \mathcal{O}(10)\mathrm{TeV}$ and ${\varphi }_0\gtrsim \mathcal{O}(10^{14})\mathrm{GeV}$, respectively.

6 pages, 2 figures

References in corpus (4)

• Cosmological lepton asymmetry with a nonzero mixing angle θ_{13}
• Resurrection of large lepton number asymmetries from neutrino flavor oscillations
• Thermal inflation, baryogenesis and axions
• Neutrino flavor transformation in the lepton-asymmetric universe

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• Quarks to Cosmos: Particles and Plasma in Cosmological evolution