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相关论文: Kinetic approach to the Schwinger effect during in…

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By using the first-principles approach, we derive a system of three quantum kinetic equations governing the production and evolution of charged scalar particles by an electric field in an expanding universe. Analyzing the ultraviolet…

广义相对论与量子宇宙学 · 物理学 2020-08-04 O. O. Sobol , E. V. Gorbar , A. I. Momot , S. I. Vilchinskii

We study the generation of electromagnetic fields during inflation when the conformal invariance of Maxwell's action is broken by the kinetic coupling $f^{2}(\phi)F_{\mu\nu}F^{\mu\nu}$ of the electromagnetic field to the inflaton field…

高能物理 - 唯象学 · 物理学 2018-10-03 O. O. Sobol , E. V. Gorbar , M. Kamarpour , S. I. Vilchinskii

In a four dimensional inflation theory, a persistent electric field can be established by making the inflaton coupled to the gauge field like a dilaton. We investigate the pair production of scalar particles in the inflaton-driven electric…

高能物理 - 理论 · 物理学 2018-11-14 Hiroyuki Kitamoto

We revisit the efficiency of Schwinger mechanism in creating charged pairs during inflation. We consider a minimal setup of inflation in which the inflaton field is a complex scalar field charged under a $U(1)$ gauge field. There is a time…

高能物理 - 理论 · 物理学 2019-05-29 Soroush Shakeri , Mohammad Ali Gorji , Hassan Firouzjahi

In this work we study the effects of the electromagnetic coupling in natural inflation in a systematic manner using the Schwinger-Keldysh formalism. The corresponding influence functional is evaluated to one-loop level. It can be…

广义相对论与量子宇宙学 · 物理学 2020-08-26 Hing-Tong Cho , Kin-Wang Ng

A quantum kinetic equation has been derived for the description of pair production in a time-dependent homogeneous electric field $E(t)$. As a source term, the Schwinger mechanism for particle creation is incorporated. Possible particle…

高能物理 - 唯象学 · 物理学 2007-05-23 S. A. Smolyansky , G. Roepke , S. Schmidt , D. Blaschke , V. D. Toneev , A. V. Prozorkevich

When the inflaton couples to photons and amplifies electric fields, charged particles produced via the Schwinger effect can dominate the universe after inflation, which is dubbed as the Schwinger preheating. Using the hydrodynamic approach…

高能物理 - 唯象学 · 物理学 2022-03-30 So Okano , Tomohiro Fujita

A quantum kinetic equation is derived for the description of pair production in a time-dependent homogeneous electric field $E(t)$. As a source term, the Schwinger mechanism for particle creation is incorporated. Possible particle…

高能物理 - 唯象学 · 物理学 2015-06-25 S. Schmidt , D. Blaschke , G. Röpke , S. A. Smolyansky , A. V. Prozorkevich , V. D. Toneev

We investigate the process of the Schwinger effect by axial coupling in the natural single-field inflation model in two parts. First we consider the Schwinger effect when the conformal invariance of Maxwell action should be broken by axial…

广义相对论与量子宇宙学 · 物理学 2023-07-04 Mehran Kamarpour

In the framework of Higgs inflation, we consider the electromagnetic field nonminimally coupled to gravity via the parity-preserving $\propto RF^{2}$ and parity-violating $\propto RF\tilde{F}$ terms. Using the perturbation theory to the…

广义相对论与量子宇宙学 · 物理学 2021-08-11 O. O. Sobol , E. V. Gorbar , O. M. Teslyk , S. I. Vilchinskii

Pair-creation of charged particles in a strong gauge-field background - the renowned Schwinger effect - can strongly alter the efficiency of gauge-field production during axion inflation. It is therefore crucial to have a clear…

高能物理 - 唯象学 · 物理学 2025-04-14 Richard von Eckardstein , Kai Schmitz , Oleksandr Sobol

In these lecture notes we give an introduction to the kinetic equation approach to pair production form the vacuum in strong, time-dependent external fields (dynamical Schwinger process). We first give a derivation of the kinetic equation…

高能物理 - 唯象学 · 物理学 2017-04-14 D. B. Blaschke , S. A. Smolyansky , A. Panferov , L. Juchnowski

In the presence of a dilatonic coupling between an inflaton and a $U(1)$ gauge field, a persistent electric field (i.e., an anisotropic inflation) is obtained as a solution of the classical field equations. We introduce charged, massive,…

高能物理 - 理论 · 物理学 2021-03-22 Hiroyuki Kitamoto

A field kinetic coupling with the Einstein tensor leads to a gravitationally enhanced friction during inflation, by which even steep potentials with theoretically natural model parameters can drive cosmic acceleration. In the presence of…

宇宙学与河外天体物理 · 物理学 2015-06-03 Shinji Tsujikawa

We consider the classical evolution of the inflaton field $\phi(t)$ and the Hubble parameter $H(t)$ in homogeneous and isotropic single-field inflation models. Under an extremely broad assumption, we show that the universe generically…

宇宙学与河外天体物理 · 物理学 2018-09-19 W. J. Handley , S. D. Brechet , A. N. Lasenby , M. P. Hobson

Recently, a novel class of models for inflation has been found in which the inflationary dynamics is driven solely by (non-canonical) kinetic terms rather than by potential terms. As an obvious extension, we show that a scalar field with…

天体物理学 · 物理学 2008-11-26 Takeshi Chiba , Takahiro Okabe , Masahide Yamaguchi

A continuous process of creation of particles is investigated as a possible connection between the inflationary stage with late cosmic acceleration. In this model, the inflationary era occurs due to a continuous and fast process of creation…

广义相对论与量子宇宙学 · 物理学 2016-04-27 Rafael C. Nunes

We analytically investigate the Schwinger pair production in the de Sitter background by using {\em the uniform asymptotic approximation method}, and show that the equation of motion in general has two turning points, and the nature of…

广义相对论与量子宇宙学 · 物理学 2018-02-12 Jia-Jia Geng , Bao-Fei Li , Jiro Soda , Anzhong Wang , Qiang Wu , Tao Zhu

We show that upon applying Palatini $f(R)$, characterized by an $\a R^2$-term, within a scenario motivated by a temporal variation of strong coupling constant, then one gets a quadratic kinetic energy. We do not drop this term, but rather…

宇宙学与河外天体物理 · 物理学 2022-02-15 M. AlHallak , A. AlRakik , N. Chamoun , M. S. El-Daher

We study a recently proposed running kinetic inflation model in which the inflaton potential becomes flat due to rapid growth of the kinetic term at large inflaton field values. As concrete examples, we build a variety of chaotic inflation…

高能物理 - 唯象学 · 物理学 2010-12-09 Kazunori Nakayama , Fuminobu Takahashi
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