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相关论文: Relic gravitational waves from the chiral magnetic…

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The authority of J. A. Wheeler in many areas of gravitational physics is immense, and there is a connection with the study of relic gravitational waves as well. I begin with a brief description of Wheeler's influence on this study. One part…

广义相对论与量子宇宙学 · 物理学 2010-03-09 L. P. Grishchuk

The chiral magnetic effect (CME) -- a macroscopic manifestation of the quantum chiral anomaly -- induces currents along magnetic field lines, facilitating mutual conversion between chiral asymmetry and magnetic helicity. Although the finite…

高能天体物理现象 · 物理学 2025-09-16 Clara Dehman , José A. Pons

We consider a relativistic plasma containing charged chiral fermions in an external magnetic field, e.g a chirally symmetric quark-gluon plasma created in relativistic heavy ion collisions. We show that triangle anomalies imply the…

高能物理 - 理论 · 物理学 2011-04-22 Dmitri E. Kharzeev , Ho-Ung Yee

The production of a stochastic background of relic gravitational waves is well known in various works in the literature, where, using the so called adiabatically-amplified zero-point fluctuations process it has been shown how the standard…

广义相对论与量子宇宙学 · 物理学 2008-12-18 Christian Corda

We reexamine generation of the primordial magnetic fields, at temperature $T>80$TeV, by applying a consistent kinetic theory framework which is suitably modified to take the quantum anomaly into account. The modified kinetic equation can…

广义相对论与量子宇宙学 · 物理学 2016-09-01 Arun Kumar Pandey , Jitesh R. Bhatt

Turbulence may have been produced in the early universe during several kind of non-equilibrium processes. Periods of cosmic turbulence may have left a detectable relic in the form of stochastic backgrounds of gravitational waves. In this…

天体物理学 · 物理学 2009-11-07 Alexander D. Dolgov , Dario Grasso , Alberto Nicolis

Here, we consider a classically scale-invariant extension of the Standard Model (SM) with two-component dark matter (DM) candidates, including a Dirac spinor and a scalar DM. We probe the parameter space of the model, constrained by relic…

高能物理 - 唯象学 · 物理学 2024-12-20 Seyed Yaser Ayazi , Mojtaba Hosseini , Rouzbeh Rouzbehi

First order phase transitions in the early universe can give rise to a stochastic background of gravitational waves. A hypothetical first order electroweak phase transition is particularly interesting in this respect, since the signal is in…

宇宙学与河外天体物理 · 物理学 2015-03-17 Chiara Caprini

The chiral magnetic effect (CME), arising from the chiral anomaly and enabling a mutual conversion between magnetic topology and fermionic chirality, is a key mechanism in magnetar field evolution. Previous work by Dehman & Pons (2025)…

高能天体物理现象 · 物理学 2026-05-11 Clara Dehman

The General Relativity affirms that any field is a source of gravitational field, thus one should affirm that the energy of Cosmic Microwave Background (CMB) generated primordial gravitational waves. The present article shows that a…

广义相对论与量子宇宙学 · 物理学 2012-05-15 Wytler Cordeiro dos Santos

A stochastic background of relic gravitational waves is achieved by the so called adiabatically-amplified zero-point fluctuations process derived from early inflation. In principle, it provides a distinctive spectrum of relic gravitational…

广义相对论与量子宇宙学 · 物理学 2008-11-26 S. Capozziello , Ch. Corda , M De Laurentis

The presence of asymmetry between fermions of opposite handedness in plasmas of relativistic particles can lead to exponential growth of a helical magnetic field via a small-scale chiral dynamo instability known as the chiral magnetic…

Primordial magnetic fields may account for all or part of the fields observed in galaxies. We consider the evolution of the magnetic fields created by pseudoscalar effects in the early universe. Such processes can create force-free fields…

天体物理学 · 物理学 2009-10-31 George B. Field , Sean M. Carroll

During a strongly first-order phase transition gravitational waves are produced by bubble collisions and turbulent plasma motion. We analyze the relevant characteristics of the electroweak phase transition in the nMSSM to determine the…

高能物理 - 唯象学 · 物理学 2008-11-26 Stephan J. Huber , Thomas Konstandin

The chirality imbalance in QCD is spontaneously induced by a repulsive axial-vector interaction from the instanton anti-instanton pairing at high temperature above the chiral phase transition, and vanishes at low temperature. The chiral…

高能物理 - 唯象学 · 物理学 2023-02-22 Jingdong Shao , Mei Huang

Gravitational waves (GW) can constitute a unique probe of the primordial universe. In many cases, the characteristic frequency of the emitted GW is directly related to the energy scale at which the GW source is operating in the early…

广义相对论与量子宇宙学 · 物理学 2015-06-11 Chiara Caprini

Cosmological phase transitions in the early Universe may produce relics in the form of a network of cosmic defects. Independently of the order of a phase transition, topology of the defects, and their global or gauge nature, the defects are…

宇宙学与河外天体物理 · 物理学 2020-11-18 Daniel G. Figueroa , Mark Hindmarsh , Joanes Lizarraga , Jon Urrestilla

We investigate the influence of cosmic magnetic fields on gravitational wave perturbations, and find exact solutions on large scales. We show that a large-scale magnetic field can generate large-scale non-decaying gravitational waves. In…

天体物理学 · 物理学 2009-11-06 Roy Maartens , Christos Tsagas , Carlo Ungarelli

The chiral magnetic effect (CME) is a phenomenon in which an electric current is induced parallel to an external magnetic field in the presence of chiral asymmetry in a fermionic system. In this paper, we show that the electric current…

高能物理 - 唯象学 · 物理学 2020-05-20 Kohei Kamada , Chang Sub Shin

Hydrodynamic and magnetohydrodynamic turbulence in the early Universe can drive gravitational waves (GWs) and imprint their spectrum onto that of GWs, which might still be observable today. We study the production of the GW background from…

宇宙学与河外天体物理 · 物理学 2022-12-02 Ramkishor Sharma , Axel Brandenburg