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We calculate the number density and the energy density of a massive scalar particle conformally coupled to gravity produced by gravitational particle creation in the case the kination stage follows inflation. In this model, mode functions…

广义相对论与量子宇宙学 · 物理学 2019-01-16 Soichiro Hashiba , Jun'ichi Yokoyama

During cosmological inflation, it has been suggested that fields coupled to the inflaton can be excited by the slow-rolling inflaton into a quasi-stable non-vacuum state. Within this scenario of ``warm inflation'', this could allow for a…

高能物理 - 唯象学 · 物理学 2008-11-26 Gert Aarts , Anders Tranberg

Analytic and numerical techniques are presented for computing gravitational production of scalar particles in the limit that the inflaton mass is much larger than the Hubble expansion rate at the end of inflation. These techniques rely upon…

高能物理 - 唯象学 · 物理学 2021-12-08 Edward E. Basso , Daniel J. H. Chung

We investigate the gravitational production of scalar dark matter particles during the inflationary and reheating epochs. The oscillatory behavior of the curvature scalar $R$ during the reheating phase generates two different enhancement…

高能物理 - 唯象学 · 物理学 2020-06-16 Jose A. R. Cembranos , Luis J. Garay , Jose M. Sánchez Velázquez

Gravitational production of decoupled scalars during inflationary and post-inflationary phases is efficient and can lead to over-production. We study this production with various reheating scenarios such as a generic power-law inflaton…

高能物理 - 唯象学 · 物理学 2026-05-11 Francesco Costa , Jinsu Kim

In this article we calculate the reheating temperature in the cosmological scenarios where heavy scalar particles are gravitationally produced, due to a conformally coupled interaction between a massive scalar quantum field and the Ricci…

广义相对论与量子宇宙学 · 物理学 2024-11-05 Jaume de Haro , Llibert Aresté Saló , Supriya Pan

Gravitational particle production of spectator fields due to the expansion universe during the inflationary and reheating phases of the early universe is of particular interest in the context of dark matter, since it allows to constrain the…

广义相对论与量子宇宙学 · 物理学 2023-10-12 Jose A. R. Cembranos , Luis J. Garay , Álvaro Parra-López , Jose M. Sánchez Velázquez

We analyze cosmological particle production driven by spacetime expansion in the early universe for homogeneous and isotropic cosmologies with positive, negative, and zero spatial curvature. We prioritize analytical results to gain a deeper…

广义相对论与量子宇宙学 · 物理学 2026-02-06 Jose A. R. Cembranos , Luis J. Garay , Álvaro Parra-López

We investigate the gravitational production of a scalar field $\chi$ with a mass exceeding the Hubble scale during inflation $m_\chi \gtrsim H_I$, employing both analytical and numerical approaches. We demonstrate that the steepest descent…

高能物理 - 唯象学 · 物理学 2024-05-24 Davide Racco , Sarunas Verner , Wei Xue

We study the problem of scalar particle production after inflation by a rapidly oscillating inflaton field. We use the framework of the chaotic inflation scenario with quartic and quadratic inflaton potentials. Particular attention is paid…

高能物理 - 唯象学 · 物理学 2009-10-28 Y. Shtanov , J. Traschen , R. Brandenberger

We propose a new mechanism of non-thermal particle production during inflation based on a narrow parametric resonance, akin to the dynamics of post-inflationary preheating. The mechanism is based on the production of scalar particles with a…

高能物理 - 唯象学 · 物理学 2025-07-18 Diogo S. Gorgulho , João G. Rosa

In this paper we analyze scalar gravitational perturbations on a Robertson-Walker background in the presence of multiple scalar fields that take values on a (geometrically non-trivial) field manifold during slow-roll inflation. For this…

高能物理 - 唯象学 · 物理学 2007-05-23 S. Groot Nibbelink , B. J. W. van Tent

A curved space-time is known to act as a source for particle production in environments where gravity plays a significant role. We explore this effect in a minimal setup of cosmic inflation on the production of a scalar dark matter…

高能物理 - 唯象学 · 物理学 2023-09-18 Mathias Pierre

We study the phenomenon of gravitational particle production as applied to a scalar spectator field in the context of $\alpha$-attractor inflation. Assuming that the scalar has a minimal coupling to gravity, we calculate the abundance of…

宇宙学与河外天体物理 · 物理学 2021-05-26 Siyang Ling , Andrew J. Long

A theory of gravitational production of light scalar particles during and after inflation is investigated. We show that in the most interesting cases where long-wavelength fluctuations of light scalar fields can be generated during…

高能物理 - 唯象学 · 物理学 2009-10-31 Gary Felder , Lev Kofman , Andrei Linde

We investigate gravitational reheating in the Starobinsky model in the Jordan frame, where inflation is driven by an $R^2$ modification of gravity with no explicit inflaton field. In this description, reheating proceeds exclusively through…

广义相对论与量子宇宙学 · 物理学 2026-03-06 Gláuber C. Dorsch , Luiz Carlos Miranda , Nelson Yokomizo

Adiabatic (curvature) perturbations are produced during a period of cosmological inflation that is driven by a single scalar field, the inflaton. On particle physics grounds -- though -- it is natural to expect that this scalar field is…

天体物理学 · 物理学 2009-11-06 N. Bartolo , S. Matarrese , A. Riotto

We investigate the gravitational particle production from vacuum for a minimally coupled fermionic spectator field during a single-field inflationary phase. We observe that metric perturbations arising from the quantum fluctuations of a…

广义相对论与量子宇宙学 · 物理学 2025-12-04 Alessio Belfiglio , Orlando Luongo

We study the prescriptions for the coupling constant of a scalar field to the Ricci curvature of spacetime in specific gravity and scalar field theories. The results are applied to the most popular inflationary scenarios of the universe;…

天体物理学 · 物理学 2014-10-13 Valerio Faraoni

We discuss the gravitational creation of superheavy particles $\chi$ in an inflationary scenario with a quartic potential and a non-minimal coupling between the inflaton $\varphi$ and the Ricci curvature: $\xi \varphi^2 R/2$. We show that…

高能物理 - 唯象学 · 物理学 2020-10-14 E. Babichev , D. Gorbunov , S. Ramazanov , L. Reverberi
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