Formation and decay of oscillons after inflation in the presence of an external coupling. Part I. Lattice simulations

Abstract We investigate the formation and decay of oscillons during the post-inflationary reheating epoch from inflaton oscillations around asymptotically flat potentials V ( φ ) in the presence of an external coupling of the form 1/2 g 2 φ 2 χ 2 . It is well-known that in the absence of such an external coupling, the attractive self-interaction term in the potential leads to the formation of copious amounts of long-lived oscillons both for symmetric and asymmetric plateau potentials. We perform a detailed numerical analysis to study the formation of oscillons in the α -attractor E- and T-model potentials using the publicly available lattice simulation code C osmo L attice. We observe the formation of nonlinear oscillon-like structures with the average equation of state ⟨ w φ ⟩ ≃ 0 for a range of values of the inflaton self-coupling λ and the external coupling g 2 . Our results demonstrate that oscillons form even in the presence of an external coupling and we determine the upper bound on g 2 which facilitates oscillon formation. We also find that eventually, these oscillons decay into the scalar inflaton radiation as well as into the quanta of the offspring field χ . Thus, we establish the possibility that reheating could have proceeded through the channel of oscillon decay, along with the usual decay of the oscillating inflaton condensate into χ particles. For a given value of the self-coupling λ , we notice that the lifetime of a population of oscillons decreases with an increase in the strength of the external coupling, following an (approximately) inverse power-law dependence on g 2 .

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2024-10-01
DOI
https://doi.org/10.1088/1475-7516/2024/10/082
Citations
11
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
3.65

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article

Formation and decay of oscillons after inflation in the presence of an external coupling. Part I. Lattice simulations

Rafid Mahbub, Swagat S. Mishra, S. Basak, Edmund J. Copeland et al.
11 citations
Journal of Cosmology and Astroparticle Physics
Cosmology and Gravitation Theories
3.65
article

Formation and decay of oscillons after inflation in the presence of an external coupling. Part I. Lattice simulations

Rafid Mahbub, Swagat S. Mishra, S. Basak, Edmund J. Copeland, Mohammed Shafi
article en
11 citations

Abstract

Abstract We investigate the formation and decay of oscillons during the post-inflationary reheating epoch from inflaton oscillations around asymptotically flat potentials V ( φ ) in the presence of an external coupling of the form 1/2 g 2 φ 2 χ 2 . It is well-known that in the absence of such an external coupling, the attractive self-interaction term in the potential leads to the formation of copious amounts of long-lived oscillons both for symmetric and asymmetric plateau potentials. We perform a detailed numerical analysis to study the formation of oscillons in the α -attractor E- and T-model potentials using the publicly available lattice simulation code C osmo L attice. We observe the formation of nonlinear oscillon-like structures with the average equation of state ⟨ w φ ⟩ ≃ 0 for a range of values of the inflaton self-coupling λ and the external coupling g 2 . Our results demonstrate that oscillons form even in the presence of an external coupling and we determine the upper bound on g 2 which facilitates oscillon formation. We also find that eventually, these oscillons decay into the scalar inflaton radiation as well as into the quanta of the offspring field χ . Thus, we establish the possibility that reheating could have proceeded through the channel of oscillon decay, along with the usual decay of the oscillating inflaton condensate into χ particles. For a given value of the self-coupling λ , we notice that the lifetime of a population of oscillons decreases with an increase in the strength of the external coupling, following an (approximately) inverse power-law dependence on g 2 .

Journal of Cosmology and Astroparticle PhysicsVol. 2024(10)
Gustavus Adolphus College (US), University of Nottingham (GB), Indian Institute of Science Education and Research Thiruvananthapuram (IN)
Science and Technology Facilities Council
Openalex Percentile: Top 7%
Cosmology and Gravitation Theories
3.65
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