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相关论文: Cosmological magnetic fields from nonlinear effect…

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We describe a scenario for large-scale magnetic field generation and particle acceleration in a collisionless collision of cold plasma clouds. A first-principle (i.e. using particles) numerical simulation of this process might be possible.…

天体物理学 · 物理学 2008-03-11 Andrei Gruzinov

We study the generation of primordial magnetic fields, coherent over cosmologically interesting scales, by gravitational creation of charged scalar particles during the reheating period. We show that magnetic fields consistent with those…

高能物理 - 唯象学 · 物理学 2009-10-07 Alejandra Kandus , Esteban A. Calzetta , Francisco D. Mazzitelli , Carlos E. M. Wagner

We find a class of cylindrically symmetric, static electrovacuum spacetimes generated by a non-homogeneous magnetic field and involving the cosmological constant and one additional parameter, which determine uniquely the strength of the…

广义相对论与量子宇宙学 · 物理学 2021-04-07 Jiří Veselý , Martin Žofka

The energy momentum tensor of a magnetic field always contains a spin-2 component in its anisotropic stress and therefore generates gravitational waves. It has been argued in the literature (Caprini & Durrer \cite{CD}) that this…

天体物理学 · 物理学 2010-08-13 Elisa Fenu , Ruth Durrer

Among primordial magnetogenesis models, inflation is a prime candidate to explain the current existence of cosmological magnetic fields. Assuming conformal invariance to be restored after inflation, their energy density decreases as…

宇宙学与河外天体物理 · 物理学 2012-05-11 Vittoria Demozzi , Christophe Ringeval

We propose a mechanism for the generation of a magnetic field in the early universe during the QCD crossover assuming that dark matter is made of axions. Thermoelectric fields arise at pressure gradients in the primordial plasma due to the…

宇宙学与河外天体物理 · 物理学 2018-07-18 Francesco Miniati , Gianluca Gregori , Brian Reville , Subir Sarkar

We present a mechanism for generating primordial magnetic fields with large correlation lengths on the order of 100 kpc today. The mechanism is based on recently conjectured QCD domain walls or similar CP violating domain walls with QCD…

高能物理 - 唯象学 · 物理学 2007-05-23 Michael McNeil Forbes , Ariel R. Zhitnitsky

In a rotation-dominated magnetosphere, there is a region where closed field lines rotate around the planet, and also a region where the open field lines stretch away from the planet, forming the lobes of the magnetotail. This paper shows…

地球与行星天体物理 · 物理学 2023-01-13 Zoltan Nemeth

We study the evolution of magnetic fields in turbulent hot plasma of the early Universe accounting for the chiral magnetic effect. The magnetohydrodynamic turbulence is modeled by replacing the matter velocity in the advection term in the…

宇宙学与河外天体物理 · 物理学 2018-01-17 Maxim Dvornikov

The $R^2$ term in the Starobinsky inflationary model can be regarded as a leading quantum correction to the gravitational effective action. We assume that parity-preserving and parity-violating (axial) non-minimal couplings between…

宇宙学与河外天体物理 · 物理学 2019-10-09 Oleg Savchenko , Yuri Shtanov

Magnetic fields are a dynamically important agent for regulating structure formation in the interstellar medium. The study of the relative orientation between the local magnetic field and gas (column-) density gradient has become a powerful…

星系天体物理 · 物理学 2020-10-14 Bastian Körtgen , Juan D. Soler

We revisit the mechanism of primordial magnetogenesis during inflation by taking into account the dynamics of the stochastic noises of the electromagnetic perturbations. We obtain the associated Langevin and Fokker-Planck equations for the…

广义相对论与量子宇宙学 · 物理学 2020-11-18 Alireza Talebian , Amin Nassiri-Rad , Hassan Firouzjahi

We show that at second order in cosmological perturbation theory vorticity generation is sourced by entropy gradients. This is an extension of Crocco's theorem to a cosmological setting.

宇宙学与河外天体物理 · 物理学 2011-11-10 Adam J. Christopherson , Karim A. Malik , David R. Matravers

In this talk, I review a number of particle-physics models that lead to the creation of magnetic fields in the early universe and address the complex problem of evolving such primordial magnetic fields into the fields observed today.…

天体物理学 · 物理学 2016-11-03 Ola Tornkvist

Basically the only existing theories for the creation of a magnetic field B in the Universe are the creation of a seed field of order 10^{-20} G in spiral galaxy which is subsequently supposedly amplified up to the observed 10^{-6} -…

天体物理学 · 物理学 2009-10-30 R. Opher , U. F. Wichoski

Magneto-curvature stresses could deform magnetic field lines and this would give rise to back reaction and restoring magnetic stresses [Tsagas, PRL (2001)]. Barrow et al [PRD (2008)] have shown in Friedman universe the expansion to be slow…

宇宙学与河外天体物理 · 物理学 2010-11-03 Garcia de Andrade

We investigate the second-order non-linear interaction as a means to generate entanglement between fields of differing wavelengths. And show that perfect entanglement can, in principle, be produced between the fundamental and second…

量子物理 · 物理学 2015-06-26 Nicolai B. Grosse , Warwick P. Bowen , Kirk McKenzie , Ping Koy Lam

It is shown that Einstein gravity tends to modify the electric and magnetic fields appreciably at distances of the order of the Compton wavelength. At that distance the gravitational field becomes spin dominated rather than mass dominated.…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Kjell Rosquist

Recently much controversy has been shed on BICEP 2 experiments for the concerning this validity or not and a possible set of new experiments to detect primordial inflation and gravitational waves. Since gravitational waves imply the…

广义相对论与量子宇宙学 · 物理学 2015-01-13 L. C. G. Andrade

A new scenario for creation of galactic magnetic fields is proposed which is operative at the cosmological epoch of the galaxy formation, and which relies on unconventional properties of dark matter. Namely, it requires existence of feeble…

宇宙学与河外天体物理 · 物理学 2013-12-09 Zurab Berezhiani , A. D. Dolgov , I. I. Tkachev
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