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The origin of the matter-antimatter asymmetry of the universe remains one of the outstanding questions yet to be answered by modern cosmology and also one of only a handful of problems where the need of a larger number of degrees of freedom…

高能物理 - 唯象学 · 物理学 2017-08-23 Gabriella Piccinelli , Alejandro Ayala

The chiral magnetic effect is a phenomenon where an electromagnetic current is generated along a magnetic field. Recently, in nonequilibrium systems, negative longitudinal magnetoresistance has been observed experimentally in Dirac/Weyl…

介观与纳米尺度物理 · 物理学 2017-04-18 Yohei Ibe , Hiroaki Sumiyoshi

The model for the generation of magnetic fields in a neutron star, based on the magnetic field instability caused by the electroweak interaction between electrons and nucleons, is developed. Using the methods of the quantum field theory,…

高能物理 - 唯象学 · 物理学 2017-01-12 Maxim Dvornikov

Generating axion dark matter through the kinetic misalignment mechanism implies the generation of large asymmetries for Standard Model fermions in the early universe. Even if these asymmetries are washed out at later times, they can trigger…

高能物理 - 唯象学 · 物理学 2023-08-09 Raymond T. Co , Valerie Domcke , Keisuke Harigaya

We study chiral symmetry structure at finite density and temperature in the presence of external magnetic field and gravity, a situation relevant in the early Universe and in the core of compact stars. We then investigate the dynamical…

高能物理 - 唯象学 · 物理学 2008-11-26 Ashok Goyal , Meenu Dahiya , Deepak Chandra

We study the generation of magnetic field in the primordial plasma of the standard model (SM) particles at temperature $T>80$~TeV much higher than the electroweak scale. It is assumed that there is an excess number of right-handed electrons…

宇宙学与河外天体物理 · 物理学 2016-09-07 Jitesh R. Bhatt , Arun Kumar Pandey

We study a matter turbulence caused by strong random hypermagnetic fields (HMFs ) that influence the baryon asymmetry evolution due to the Abelian anomalies in the symmetric phase in the early Universe. Such a matter turbulence is…

宇宙学与河外天体物理 · 物理学 2021-11-17 Maxim Dvornikov , Victor B. Semikoz

It is known that cosmic magnetic field, if present, can generate anisotropic stress in the plasma and hence, can act as a source of gravitational waves. These cosmic magnetic fields can be generated at very high temperature, much above…

宇宙学与河外天体物理 · 物理学 2019-01-25 Sampurn Anand , Jitesh R. Bhatt , Arun Kumar Pandey

The generation of helical magnetic fields during single field inflation due to an axial coupling of the electromagnetic field to the inflaton is discussed. We find that such a coupling always leads to a blue spectrum of magnetic fields…

宇宙学与河外天体物理 · 物理学 2014-03-12 Rajeev Kumar Jain , Ruth Durrer , Lukas Hollenstein

We study the generation of magnetic fields during preheating within an scenario of hybrid inflation at the electroweak (EW) scale. We find that the non-perturbative and strongly out-of-equilibrium process of magnetic field production occurs…

高能物理 - 唯象学 · 物理学 2008-11-26 Andres Diaz-Gil , Juan Garcia-Bellido , Margarita Garcia Perez , Antonio Gonzalez-Arroyo

We suggest a new mechanism for generation of large-scale magnetic field in the hot plasma of early universe which is based on the parity violation in weak interactions and depends neither on helicity of matter turbulence resulting in the…

天体物理学 · 物理学 2009-11-10 V. B. Semikoz , D. D. Sokoloff

Non-perturbative effect of the formation of a chiral symmetry breaking condensate <\bar\psi\psi> and of a dynamically generated fermion mass in QED in the presence of an external magnetic field is considered. The dynamical mass of a fermion…

高能物理 - 理论 · 物理学 2007-05-23 V. P. Gusynin

We report on an exploratory lattice study on the phenomenon of chiral instabilities in non-Abelian gauge theories at high temperature. It is based on a recently constructed anomalous Langevin-type effective theory of classical soft gauge…

高能物理 - 唯象学 · 物理学 2016-05-04 Yukinao Akamatsu , Alexander Rothkopf , Naoki Yamamoto

In our conventional understanding, large-scale magnetic fields are thought to originate from an inverse cascade in the presence of magnetic helicity, differential rotation, or a magneto-rotational instability. However, as recent simulations…

等离子体物理 · 物理学 2017-09-20 Kiwan Park

We study the generation of large scale primordial magnetic fields by a cosmological phase transition during the radiation dominated era. The setting is a theory of N charged scalar fields coupled to an abelian gauge field, that undergoes a…

天体物理学 · 物理学 2007-05-23 D. Boyanovsky , H. J. de Vega , M. Simionato

We show that the baryon asymmetry of the universe can be explained in models where the Higgs couples to the Chern-Simons term of the hypercharge group and is away from the late-time minimum of its potential during inflation. The Higgs then…

高能物理 - 唯象学 · 物理学 2021-09-07 Yann Cado , Benedict von Harling , Eduard Masso , Mariano Quiros

We extend our recent derivation of the time evolution equations for the energy content of magnetic fields and turbulent motions for incompressible, homogeneous, and isotropic turbulence to include the case of nonvanishing helicity. These…

宇宙学与河外天体物理 · 物理学 2013-06-14 Andrey Saveliev , Karsten Jedamzik , Guenter Sigl

We investigate analytically the amplification of a weak magnetic field in a homogeneous and isotropic turbulent flow lacking reflectional symmetry (helical turbulence). We propose that the spectral distributions of magnetic energy and…

天体物理学 · 物理学 2007-05-23 Stanislav Boldyrev , Fausto Cattaneo , Robert Rosner

We study the magnetohydrodynamics of relativistic plasmas accounting for the chiral magnetic effect (CME). To take into account the evolution of the plasma velocity, obeying the Navier-Stokes equation, we approximate it by the Lorentz force…

宇宙学与河外天体物理 · 物理学 2017-03-01 Maxim Dvornikov , Victor B. Semikoz

Conventional Leptogenesis mechanism, which provides compelling explanation to the origin of the baryon asymmetry of the universe (BAU), assumes the absence of hypermagnetic field in the early universe, thereby disregard the implications of…

高能物理 - 唯象学 · 物理学 2025-11-18 Wei Chao