The paradigm of warm quintessential inflation and spontaneous baryogenesis
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Publication:5099228
DOI10.1088/1475-7516/2022/03/063zbMath1504.83027arXiv2110.00607OpenAlexW3202597676MaRDI QIDQ5099228
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Publication date: 31 August 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2110.00607
Relativistic cosmology (83F05) Nuclear physics (81V35) Geometrodynamics and the holographic principle (83E05) Weak interaction in quantum theory (81V15) Gravitational waves (83C35) Dark matter and dark energy (83C56)
Cites Work
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- The importance of being warm (during inflation)
- \(f(R)\) theories
- Curvaton reheating in non-oscillatory inflationary models
- Preheating in quintessential inflation
- Towards a reliable effective field theory of inflation
- Warm quintessential inflation
- A new type of isotropic cosmological models without singularity
- DYNAMICS OF DARK ENERGY
- Non-minimal gravitational reheating during kination
- Ricci reheating
- Warm-assisted natural inflation
- Gravity waves and primordial black holes in scalar warm little inflation
- Spontaneous symmetry breaking in the late Universe and glimpses of the early Universe phase transitions à la baryogenesis
- Inflationary universe: A possible solution to the horizon and flatness problems
- Hubble-induced phase transitions on the lattice with applications to Ricci reheating
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