Gravitational waves from dark sectors, oscillating inflatons, and mass boosted dark matter

DOI10.1088/1475-7516/2021/04/043zbMath1485.83035arXiv2008.12306OpenAlexW3153128298MaRDI QIDQ5026127

Joseph Bramante, Amit Bhoonah, Simran Nerval, Ningqiang Song

Publication date: 7 February 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2008.12306

zbMATH Keywords

inflationdark matter theorycosmological phase transitionsprimordial gravitational waves (theory)

Mathematics Subject Classification ID

Geometric probability and stochastic geometry (60D05) Relativistic cosmology (83F05) Oscillation, zeros of solutions, mean value theorems, etc. in context of PDEs (35B05) Phase transitions (general) in equilibrium statistical mechanics (82B26) Gravitational waves (83C35) Dark matter and dark energy (83C56)

Related Items (2)

Tachyonic preheating in plateau inflation ⋮ The linear regime of tachyonic preheating

Cites Work

• Unnamed Item
• Unnamed Item
• Freeze-in production of FIMP dark matter
• The dark side of the electroweak phase transition
• Baryon washout, electroweak phase transition, and perturbation theory
• Gravitational waves from oscillon preheating
• Superheavy thermal dark matter and primordial asymmetries
• Oscillons from string moduli
• A new type of isotropic cosmological models without singularity
• \(\alpha\)-attractors: Planck, LHC and dark energy
• What can we learn from the stochastic gravitational wave background produced by oscillons?
• Phase transitions in an expanding universe: stochastic gravitational waves in standard and non-standard histories
• The Primordial Density Perturbation
• Generating the curvature perturbation without an inflaton

This page was built for publication: Gravitational waves from dark sectors, oscillating inflatons, and mass boosted dark matter