Inflation and late-time acceleration from a double-well potential with cosmological constant
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🌀 gr-qc
astro-ph.CO
keywords
modeluniverseaccelerationbangbeforeconstantcosmologicaldeflationary
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A model of a universe without big bang singularity is presented, which displaysanearly inflationary period ending just before a phase transition to a deflationary epoch. The model produces enough heavy particles so as to reheat the universe at temperatures in the MeV regime. After the reheating, it smoothly matches the standard $\Lambda$CDM scenario.
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Cited by 1 Pith paper
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Modified Gravity Theories on a Nutshell: Inflation, Bounce and Late-time Evolution
Modified gravity theories supply viable mathematical frameworks for inflation, bounces, and dark energy eras that match observational data.
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