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相关论文: Primordial magnetic fields induced by cosmological…

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As one of the prime contributors to the interstellar medium energy budget, magnetic fields naturally play a part in shaping the evolution of galaxies. Galactic magnetic fields can originate from strong primordial magnetic fields provided…

星系天体物理 · 物理学 2020-06-03 Sergio Martin-Alvarez , Adrianne Slyz , Julien Devriendt , Carlos Gómez-Guijarro

We investigate the generation of magnetic field by the Biermann battery in cosmological ionization fronts, using new simulations of the reionization of the universe by stars in protogalaxies. Two mechanisms are primarily responsible for…

天体物理学 · 物理学 2009-10-31 Nickolay Y. Gnedin , Andrea Ferrara , Ellen G. Zweibel

We review the possible mechanisms for the generation of cosmological magnetic fields, discuss their evolution in an expanding Universe filled with the cosmic plasma and provide a critical review of the literature on the subject. We put…

宇宙学与河外天体物理 · 物理学 2015-06-15 R. Durrer , A. Neronov

Magnetic fields are observed not only in stars, but in galaxies, clusters, and even high redshift Lyman-alpha systems. In principle, these fields could play an important role in structure formation and also affect the anisotropies in the…

天体物理学 · 物理学 2009-10-31 Roy Maartens

The hot plasma above the electroweak scale contains (hyper) charged scalar particles which are coupled to Abelian gauge fields. Scalars may interact with gravity in a non-conformally invariant way and thus their fluctuations can be…

高能物理 - 唯象学 · 物理学 2009-10-31 M. Giovannini , M. Shaposhnikov

In this work we investigate the possibility of generation of primordial magnetic field in the early universe near the QCD phase transition epoch via the collapse of $Z(3)$ domains. The $Z(3)$ domain walls arise in the deconfined phase of…

高能物理 - 唯象学 · 物理学 2018-12-18 Abhishek Atreya , Soma Sanyal

A primordial stochastic magnetic field will induce temperature and polarization fluctuations in the cosmic microwave background. We outline a calculation of the resulting fluctuation power spectra and present numerical results.

天体物理学 · 物理学 2009-10-31 Tina Kahniashvili , Arthur Kosowsky , Andrew Mack , Ruth Durrer

We show that coherent magnetic field is generated spontaneously when a large domain wall is created in the early universe. It is caused by two dimensional massless fermions bounded to the domain wall soliton. We point out that the magnetic…

高能物理 - 唯象学 · 物理学 2009-10-28 Aiichi Iwazaki

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. Implications for…

天体物理学 · 物理学 2016-11-03 Ola Tornkvist

Magnetic fields are generated in ionized objects rotating with respect to a radiation background. Based on conservation of canonical ion momentum, it has been previously suggested that even if the radiation intensity is unrestricted the…

天体物理学 · 物理学 2009-11-10 L. Chuzhoy

While magnetic fields are important in contemporary star formation, their role in primordial star formation is unknown. Magnetic fields of order 10^-16 G are produced by the Biermann battery due to the curved shocks and turbulence…

星系天体物理 · 物理学 2020-07-15 Christopher F. McKee , Athena Stacy , Pak Shing Li

Most early Universe scenarios predict negligible magnetic fields on cosmological scales if they are unprocessed during subsequent expansion of the Universe. We present a new numerical treatment of the evolution of primordial fields and…

天体物理学 · 物理学 2009-11-07 Guenter Sigl

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

The origin of magnetic fields in clusters of galaxies is still an unsolved problem, which is largely due to our poor understanding of initial seed magnetic fields. If the seed magnetic fields have primordial origins, it is likely that…

宇宙学与河外天体物理 · 物理学 2015-06-23 Jungyeon Cho

Sufficiently large seeds for generating the observed (inter)galactic magnetic fields emerge naturally in string cosmology from the amplification of electromagnetic vacuum fluctuations due to a dynamical dilaton background. The success of…

高能物理 - 理论 · 物理学 2009-10-28 M. GasperinI , M. Giovannini , G. Veneziano

The generation of a magnetic field in the Early Universe is considered, due to the gravitational production of the Z-boson field during inflation. Scaled to the epoch of galaxy formation this magnetic field suffices to trigger the galactic…

天体物理学 · 物理学 2017-01-25 Konstantinos Dimopoulos

The creation of large scale magnetic fields is studied in an inflationary universe where electrodynamics is assumed to be nonlinear. After inflation ends electrodynamics becomes linear and thus the description of reheating and the…

天体物理学 · 物理学 2008-11-26 Kerstin E. Kunze

We explore cosmological magnetogenesis in the post-inflationary universe, when the inflaton oscillates around its potential minimum and the universe is effectively dominated by cold matter. During this epoch prior to reheating, large-scale…

宇宙学与河外天体物理 · 物理学 2014-05-29 Takeshi Kobayashi

The origin of intergalactic magnetic fields is still a mystery and several scenarios have been proposed so far: among them, primordial phase transitions, structure formation shocks and galactic outflows. In this work we investigate how…

天体物理学 · 物理学 2009-11-11 Serena Bertone , Corina Vogt , Torsten Ensslin

We argue that ultra-high energy cosmic rays emitted by galaxy clusters result in electric currents in filaments of the large-scale structure that are sufficient to generate magnetic fields in voids of the magnitude of ~1e-12 G and the…

高能天体物理现象 · 物理学 2012-02-03 M. S. Pshirkov , P. G. Tinyakov