R Allahverdi, MA Amin, A Berlin, N Bernal… - arXiv preprint arXiv …, 2020 - arxiv.org
It is commonly assumed that the energy density of the Universe was dominated by radiation between reheating after inflation and the onset of matter domination 54,000 years later …
L Visinelli - International Journal of Modern Physics D, 2021 - World Scientific
Compact objects occupy a pivotal role in the exploration of Nature. The interest spans from the role of compact objects in astrophysics to their detection through various methods …
Our understanding of the state of the universe between the end of inflation and big bang nucleosynthesis (BBN) is incomplete. The dynamics at the end of inflation are rich and a …
MAG Garcia, M Pierre - Journal of Cosmology and Astroparticle …, 2023 - iopscience.iop.org
In the presence of self-interactions, the post-inflationary evolution of the inflaton field is driven into the non-linear regime by the resonant growth of its fluctuations. The once …
Homogeneous oscillations of the inflaton after inflation can be unstable to small spatial perturbations even without coupling to other fields. We show that for inflaton potentials∝| ϕ …
Oscillons are massive, long-lived, localized excitations of a scalar field. We show that in a class of well-motivated single-field models, inflation is followed by self resonance, leading to …
MAG Garcia, M Gross, Y Mambrini… - … of Cosmology and …, 2023 - iopscience.iop.org
We consider the effects of fragmentation on the post-inflationary epoch of reheating. In simple single field models of inflation, an inflaton condensate undergoes an oscillatory …
T Helfer, DJE Marsh, K Clough… - … of Cosmology and …, 2017 - iopscience.iop.org
The classical equations of motion for an axion with potential V (ϕ)= ma 2 fa 2 [1− cos (ϕ/fa)] possess quasi-stable, localized, oscillating solutions, which we refer to as``axion stars''. We …
We show that fragmentation of the inflaton into long-lived spatially localized oscillon configurations can lead to copious production of black holes. In simple inflation models …