Super-heavy dark matter -- Towards predictive scenarios from inflation

DOI10.1016/j.nuclphysb.2017.02.019zbMath1360.83090arXiv1605.09378OpenAlexW2409422413WikidataQ62372312 ScholiaQ62372312MaRDI QIDQ523824

Kristjan Kannike, Antonio Racioppi, Martti Raidal

Publication date: 24 April 2017

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1605.09378

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Methods of quantum field theory in general relativity and gravitational theory (83C47)

Related Items

Dynamically induced Planck scale and inflation in the Palatini formulation, The inflaton portal to dark matter, Higher spin dark matter, Super-heavy dark matter -- Towards predictive scenarios from inflation, Non-minimal (self-)running inflation: metric vs. Palatini formulation, Gravitational production of superheavy dark matter and associated cosmological signatures, Computation of gravitational particle production using adiabatic invariants, Multiple point criticality principle and Coleman-Weinberg inflation, Nonminimal Coleman-Weinberg inflation with an R² term, Despicable dark relics: generated by gravity with unconstrained masses, Coleman-Weinberg linear inflation: metric vs. Palatini formulation, Palatini inflation in models with an R² term, Scalar-tensor linear inflation, Gravitational dark matter production in Palatini preheating

Cites Work

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