Healing the cosmological constant problem during inflation through a unified quasi-quintessence matter field

DOI10.1088/1361-6382/AC8AF2OpenAlexW4293068049WikidataQ114096911 ScholiaQ114096911MaRDI QIDQ5867542

Rocco D'Agostino, Marco Muccino, Orlando Luongo

Publication date: 14 September 2022

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2204.02190

zbMATH Keywords

inflationcosmologyvacuum energy

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Geometrodynamics and the holographic principle (83E05) Phase transitions (general) in equilibrium statistical mechanics (82B26) Gravitational energy and conservation laws; groups of motions (83C40) Classical and relativistic thermodynamics (80A10) Dark matter and dark energy (83C56)

Related Items (4)

Tadpole cosmology: Milne solution as a cosmological constant hideout ⋮ Entanglement area law violation from field-curvature coupling ⋮ Late-time constraints on modified Gauss-Bonnet cosmology ⋮ Observational constraints on modified CPL models for dark energy

Cites Work

• An expanding universe with constant pressure and no cosmological constant
• Cosmological constant -- the weight of the vacuum
• A new type of isotropic cosmological models without singularity
• The cosmological constant and dark energy
• DYNAMICS OF DARK ENERGY
• Inflation without Slow Roll
• The cosmological constant problem and quintessence
• Extended gravity cosmography
• Dark Energy, Dark Matter and baryogenesis from a model of a complex axion field
• Inflationary universe: A possible solution to the horizon and flatness problems
• A UNIFIED DARK ENERGY MODEL FROM A VANISHING SPEED OF SOUND WITH EMERGENT COSMOLOGICAL CONSTANT
• The cosmological constant problem
• The cosmological constant
• Brane inflation.
• \(k\)-inflation
• \(F\)-term inflation in superstring theories
• An alternative to quintessence

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