Reheating in quintessential inflation via gravitational production of heavy massive particles: a detailed analysis
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Publication:5862440
DOI10.1088/1475-7516/2019/01/023OpenAlexW3103036205WikidataQ128625442 ScholiaQ128625442MaRDI QIDQ5862440
Jaume Haro, Supriya Pan, Wei-Qiang Yang
Publication date: 9 March 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1811.07371
Related Items (10)
Understanding gravitational particle production in quintessential inflation ⋮ Palatini R 2 quintessential inflation ⋮ Palatini approach and large-scale magnetogenesis ⋮ Gravitational reheating and superheavy Dark Matter creation after inflation with non-minimal coupling ⋮ Freeze-in from preheating ⋮ Post-inflationary phases stiffer than radiation and Palatini formulation ⋮ Gravitational production of superheavy dark matter and associated cosmological signatures ⋮ Ability of LIGO and LISA to probe the equation of state of the early Universe ⋮ Non-oscillatory no-scale inflation ⋮ Quintessential α-attractor inflation: forecasts for Stage IV galaxy surveys
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