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相关论文: Magnetogenesis from Rotating Cosmic String Loops

200 篇论文

We propose that strong magnetic fields should be generated at shock waves associated with formation of galaxies or clusters of galaxies by the Weibel instability, an instability in collisionless plasmas. The strength of the magnetic fields…

天体物理学 · 物理学 2009-11-13 Yutaka Fujita , Tsunehiko N. Kato

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

Magnetic fields of cosmic bodies are generated by the hydromagnetic dynamo effect in moving electrically conducting fluids, such as liquid metals or plasmas. Once produced, cosmic magnetic fields are able to act back on moving fluids. This…

物理学史与哲学 · 物理学 2014-03-17 Frank Stefani

The origin of large scale cosmological magnetic fields remains a mystery, despite the continuous efforts devoted to that problem. We present a new model of magnetic field generation, based on local charge separation provided by an…

天体物理学 · 物理学 2009-04-16 Mathieu Langer , Jean-Loup Puget , Nabila Aghanim

We reinvestigate the generation and accumulation of magnetic flux in optically thin accretion flows around active gravitating objects. The source of the magnetic field is the azimuthal electric current associated with the Poynting-Robertson…

Structure formation heralds the era of deviation of the matter content of the Universe away from thermal equilibrium, so the gravitational contribution to entropy, in the form of Weyl curvature, must become active in order for the overall…

宇宙学与河外天体物理 · 物理学 2024-01-03 Fan Zhang

We investigate an efficient mechanism for generating magnetic fields in turbulent, collisionless plasmas. By using fully kinetic, particle-in-cell simulations of an initially non-magnetized plasma, we inspect the genesis of magnetization,…

等离子体物理 · 物理学 2021-12-01 F. Pucci , M. Viviani , F. Valentini , G. Lapenta , W. H. Matthaeus , S. Servidio

It is argued that large scale cosmic magnetic field could be generated in the primeval plasma slightly before hydrogen recombination. Non-zero vorticity, necessary for that, might be created by the photon diffusion in the second order in…

天体物理学 · 物理学 2016-08-30 Z. Berezhiani , A. D. Dolgov

The origin and the magnitude of the inter-galactic magnetic field is of primordial importance in the global picture of magnetic field evolution, as it is considered to be the missing link between galactic magnetic fields and cluster…

宇宙学与河外天体物理 · 物理学 2015-05-14 Yohan Dubois , Romain Teyssier

In this work we consider an extended electromagnetic theory in which the scalar state which is usually eliminated by means of the Lorenz condition is allowed to propagate. This state has been shown to generate a small cosmological constant…

宇宙学与河外天体物理 · 物理学 2011-02-01 Jose Beltran Jimenez , Antonio L. Maroto

Magnetic fields are ubiquitous in the Universe. Extragalactic disks, halos and clusters have consistently been shown, via diffuse radio-synchrotron emission and Faraday rotation measurements, to exhibit magnetic field strengths ranging from…

A mechanism of generation of a toroidal component of large scale magnetic field, leading to the reconstruction of the pulsar magnetospheres is presented. In order to understand twisting of magnetic field lines, we investigate kinematics of…

天体物理学 · 物理学 2008-11-26 Z. Osmanov , G. Dalakishvili , G. Machabeli

We do a detailed study on vortex formation in a magnetized plasma within the spacetime of a moving cosmic string using analytical and numerical methods. The conical spacetime around the cosmic string causes the frozen-in magnetic field to…

宇宙学与河外天体物理 · 物理学 2025-12-02 Deepanshu Bisht , Dilip Kumar , Soumen Nayak , Soma Sanyal

Magnetic fields in rotating and radiating astrophysical plasma can be produced due to a radiative interaction between plasma layers moving relative to each other. The efficiency of current drive, and with it the associated dynamo effect, is…

等离子体物理 · 物理学 2017-09-22 Vadim R. Munirov , Nathaniel J. Fisch

This paper considers a possibility of magnetic-field generation by local turbulent flows at the bottom of convective zone. The cycle of magnetic-field generation in this model can be represented in the form of sequency of processes. There…

太阳与恒星天体物理 · 物理学 2013-10-18 Andrey G. Tlatov

The electromagnetic field near a rotating black hole is being explored in educational style here. By employing analytic solutions for electrovacuum fields, we plot the surfaces of constant flux and we show how the field is dragged around…

天体物理学 · 物理学 2007-05-23 Z. Budinova , M. Dovciak , V. Karas , A. Lanza

Using the generally covariant magnetofluid formalism for a hot plasma, a new spacetime curvature driven mechanism for generating seed vorticity/magnetic field is presented. The ``battery'' owes its origin to the interaction between gravity…

等离子体物理 · 物理学 2015-06-11 Felipe A. Asenjo , Swadesh M. Mahajan , Asghar Qadir

The nature and origin of turbulence and magnetic fields in the intergalactic space are important problems that are yet to be understood. We propose a scenario in which turbulent flow motions are induced via the cascade of the vorticity…

天体物理学 · 物理学 2009-11-13 Dongsu Ryu , Hyesung Kang , Jungyeon Cho , Santabrata Das

We introduce a new mechanism for generating magnetic fields in the recombination era. This Harrison-like mechanism utilizes vorticity in baryons that is sourced through the Bose-Einstein condensate of axions via gravitational interactions.…

宇宙学与河外天体物理 · 物理学 2016-03-23 Nilanjan Banik , Adam J. Christopherson

Using a generally covariant Electro-Vortic (magnetofluid) formalism for relativistic plasmas, the dynamical evolution of a generalized vorticity (a combination of the magnetic and kinematic parts) is studied in a cosmological context. We…

等离子体物理 · 物理学 2019-05-22 Felipe A. Asenjo , Swadesh M. Mahajan