Fate of \(Z_{2}\) symmetric scalar field
From MaRDI portal
Publication:737859
DOI10.1007/JHEP12(2013)053zbMath1342.83542arXiv1308.4394MaRDI QIDQ737859
Masahiro Takimoto, Kazunori Nakayama, Kyohei Mukaida
Publication date: 12 August 2016
Published in: Journal of High Energy Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1308.4394
Related Items (9)
Weyl scaling invariant \(R^2\) gravity for inflation and dark matter ⋮ Effective action for cosmological scalar fields at finite temperature ⋮ General Markovian equation for scalar fields in a slowly evolving background ⋮ Weyl symmetry inspired inflation and dark matter ⋮ Inflation and dark matter in the Z 5 model ⋮ CMB constraints on the inflaton couplings and reheating temperature in \(\alpha\)-attractor inflation ⋮ Oscillating scalar dissipating in a medium ⋮ Hidden inflaton dark matter ⋮ Moduli oscillation induced by reheating
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