What can we learn from the stochastic gravitational wave background produced by oscillons?
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Publication:5022253
DOI10.1088/1475-7516/2018/03/032OpenAlexW2772570327MaRDI QIDQ5022253
Stefan Antusch, Francesco Cefalà, Stefano Orani
Publication date: 18 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1712.03231
Related Items (18)
Oscillons during Dirac-Born-Infeld preheating ⋮ Properties of oscillons in hilltop potentials: energies, shapes, and lifetimes ⋮ GFiRe—Gauge Field integrator for Reheating ⋮ Finite temperature effects in modular cosmology ⋮ The linear regime of tachyonic preheating ⋮ Quantum decay of scalar and vector boson stars and oscillons into gravitons ⋮ Oscillon spectroscopy ⋮ Detection of early-universe gravitational-wave signatures and fundamental physics ⋮ Constraints on the non-minimally coupled Witten-O'Raifeartaigh inflation ⋮ Transient acceleration after non-minimal M-flation preheating ⋮ Oscillon preheating in full general relativity ⋮ Cosmological backgrounds of gravitational waves ⋮ Gravitational wave forest from string axiverse ⋮ The fate of dense scalar stars ⋮ Probing primordial features with the stochastic gravitational wave background ⋮ Gravitational waves from dark sectors, oscillating inflatons, and mass boosted dark matter ⋮ Can axion clumps be formed in a pre-inflationary scenario? ⋮ Oscillon collapse to black holes
Uses Software
Cites Work
- \texttt{LATTICEEASY}: A program for lattice simulations of scalar fields in an expanding universe
- Gravitational waves from oscillon preheating
- Oscillons from string moduli
- de Sitter vacua in string theory
- Semiclassicality and decoherence of cosmological perturbations
- Detecting the cosmic gravitational wave background with the Big Bang Observer
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