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相关论文: Chirality production during axion inflation

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We study the generation of primeval magnetic fields during inflation era in nonlinear theories of electrodynamics. Although the intensity of the produced fields strongly depends on characteristics of inflation and on the form of…

天体物理学 · 物理学 2008-11-26 L. Campanelli , P. Cea , G. L. Fogli , L. Tedesco

The interrelation between the generation of large-scale electric fields and that of large-scale magnetic fields due to the breaking of the conformal invariance of the electromagnetic field in inflationary cosmology is studied. It is shown…

天体物理学 · 物理学 2009-06-23 Kazuharu Bamba

The spectrum of curvature perturbation generated during inflation is studied in the case the inflation-driving scalar field (inflaton) $\phi$ crosses over its potential extremum. It is shown that the nondecaying mode of perturbation has a…

高能物理 - 唯象学 · 物理学 2009-11-07 Jun'ichi Yokoyama , Shogo Inoue

Erickcek, Kamionkowski and Carroll proposed in 2008 that the dipole modulation of the CMB could be due to a very large scale perturbation of the field $\phi$ causing the primordial curvature perturbation. We repeat their calculation using…

宇宙学与河外天体物理 · 物理学 2015-06-15 David H. Lyth

A numerical study of a pseudoscalar inflation having an axion-photon-like coupling is performed by solving numerically the coupled differential equations of motion for inflaton and photon mode functions from the onset of inflation to the…

宇宙学与河外天体物理 · 物理学 2016-03-23 Shu-Lin Cheng , Wolung Lee , Kin-Wang Ng

We propose a large class of supergravity models in terms of a single chiral matter superfield, leading to (almost) arbitrary single-field inflationary scalar potentials similar to the F-term in rigid supersymmetry. Those scalar potentials…

高能物理 - 理论 · 物理学 2015-02-25 Sergei V. Ketov , Takahiro Terada

We show how short inflation naturally arises in a non-minimal gravity theory with a scalar field without any potential terms. This field drives inflation solely by its derivatives, which couple to the matter only through the combination…

高能物理 - 唯象学 · 物理学 2010-04-05 Nemanja Kaloper

We consider, in the context of axion-inflation, the \textit{Pure Natural Inflation} (PNI) model coupled with an SU(2) gauge sector via a Chern-Simons term. As the axion rolls down its potential, it dissipates energy in the gauge sector thus…

宇宙学与河外天体物理 · 物理学 2025-04-25 Ema Dimastrogiovanni , Matteo Fasiello , Alexandros Papageorgiou , Cristóbal Zenteno Gatica

We study the onset of the reheating epoch at the end of axion-driven inflation where the axion is coupled to an Abelian, $U(1)$, gauge field via a Chern-Simons interaction term. We focus primarily on $m^2\phi^2$ inflation and explore the…

宇宙学与河外天体物理 · 物理学 2016-12-26 Peter Adshead , John T. Giblin , Timothy R. Scully , Evangelos I. Sfakianakis

We study a variant of the Chromo-Natural Inflation (CNI) mechanism in which the inflaton interacts only gravitationally with the CNI fields. Integrating out all the non-dynamical scalar fields of the model results in a coupling between the…

宇宙学与河外天体物理 · 物理学 2019-09-04 Alexandros Papageorgiou , Marco Peloso , Caner Unal

The generation of magnetic fields during inflation in an electromagnetic model with a non-local form factor in Maxwell`s action is studied. The equations of motion for the electromagnetic field are derived and solved. It is found that the…

广义相对论与量子宇宙学 · 物理学 2023-11-28 E. V. Gorbar , T. V. Gorkavenko , V. M. Gorkavenko , O. M. Teslyk

We study the dynamics of a plasma of charged relativistic fermions at very high temperature $T\gg m$, where $m$ is the fermion mass, coupled to the electromagnetic field. In particular, we derive a magneto-hydrodynamical description of the…

高能物理 - 唯象学 · 物理学 2015-08-19 Alexey Boyarsky , Jurg Frohlich , Oleg Ruchayskiy

We calculate the rate of collisional decay of the axial charge in an ultrarelativistic electron-positron plasma, also known as the chirality flipping rate. We find that contrary to the existing estimates, the chirality flipping rate appears…

高能物理 - 唯象学 · 物理学 2021-01-20 A. Boyarsky , V. Cheianov , O. Ruchayskiy , O. Sobol

A primordial magnetic field may be generated during an inflationary period if conformal invariance is broken. We reexamine and generalize previous results about the magnetic field produced by couplings of the form $R^n…

天体物理学 · 物理学 2009-10-28 F. D. Mazzitelli , F. M. Spedalieri

We propose a novel scenario to generate primordial magnetic fields during inflation induced by an oscillating coupling of the electromagnetic field to the inflaton. This resonant mechanism has two key advantages over previous proposals.…

宇宙学与河外天体物理 · 物理学 2012-06-22 Christian T. Byrnes , Lukas Hollenstein , Rajeev Kumar Jain , Federico R. Urban

This paper concerns the generation and evolution of the cosmological (large-scale $\sim Mpc$) magnetic fields in an inflationary universe. The universe during inflation is represented by de Sitter space-time. We started with the Maxwell…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Zuxiang Dai

Chromo-natural inflation is a novel model of inflation which relies on the existence of non-abelian gauge fields interacting with an axion. In its simplest realization, an SU(2) gauge field is assumed to begin inflation in a rotationally…

高能物理 - 理论 · 物理学 2015-06-12 Emanuela Dimastrogiovanni , Matteo Fasiello , Andrew J. Tolley

We derive a nonlocal effective Lagrangian for the chiral magnetic effect. An electric field is generated by winding number fluctuations of the nonabelian gauge field in the presence of a strong magnetic field. We estimate the magnitude of…

高能物理 - 唯象学 · 物理学 2010-12-23 Berndt Müller , Andreas Schäfer

We revisit the study of the phenomenology associated to a burst of particle production of a field whose mass is controlled by the inflaton field and vanishes at one given instance during inflation. This generates a bump in the correlators…

宇宙学与河外天体物理 · 物理学 2017-06-14 Lauren Pearce , Marco Peloso , Lorenzo Sorbo

We study the generation of helical magnetic fields in a model of inflationary magnetogenesis which is free from the strong coupling and back-reaction problems. To generate helical magnetic fields, we add an $f^2 \tilde{F}^{\mu\nu}…

宇宙学与河外天体物理 · 物理学 2018-04-11 Ramkishor Sharma , Kandaswamy Subramanian , T. R. Seshadri