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Primordial magnetic fields generated in the early universe are subject of considerable investigation, and observational limits on their strength are required to constrain the theory. Due to their impact on the reionization process, the…

宇宙学与河外天体物理 · 物理学 2015-05-30 Dominik R. G. Schleicher , Francesco Miniati

It is assumed that long range coherent magnetic fields in the universe were spontaneously generated at high temperature due to vacuum polarization of non-Abelian gauge fields, and resulted in the present intergalaxy magnetic field. The zero…

高能物理 - 唯象学 · 物理学 2011-06-27 E. Elizalde , V. Skalozub

Using a set of cosmological hydro-dynamical simulations, we constrained the properties of primordial magnetic fields by studying their impact on the formation and evolution of dwarf galaxies. We performed a large set of simulations (8 dark…

星系天体物理 · 物理学 2020-11-04 Mahsa Sanati , Yves Revaz , Jennifer Schober , Kerstin E. Kunze , Pascale Jablonka

We reanalyze the effect of magnetic fields in BBN, incorporating several features which were omitted in previous analyses. We find that the effects of coherent magnetic fields on the weak interaction rates and the electron thermodynamic…

天体物理学 · 物理学 2014-10-13 Peter. J. Kernan , Glenn D. Starkman , Tammay Vachaspati

Weak magnetic fields must have existed in the early Universe, as they were sourced by the cross product of electron density and temperature gradients through the Biermann-battery mechanism. In this paper we calculate the magnetic fields…

宇宙学与河外天体物理 · 物理学 2024-08-15 Nanoom Lee , Yacine Ali-Haimoud

Recently Cheng, Olinto, Schramm and Truran (COST) reexamined the constraints from big bang nucleosynthesis (BBN) on the strength of primordial magnetic fields. Their bottom line agreed with that of an earlier recent paper on the subject…

天体物理学 · 物理学 2016-08-30 Peter J. Kernan , Glenn D. Starkman , Tanmay Vachaspati

In view of several conflicting results, we reanalyze the effects of magnetic fields on the primordial nucleosynthesis. In the case the magnetic field is homogeneous over a horizon volume, we show that the main effects of the magnetic field…

天体物理学 · 物理学 2008-11-26 D. Grasso , H. R. Rubinstein

The effects of magnetic fields on Big Bang Nucleosynthesis(BBN) have been calculated, and the impact on the abundances of the light elements have been investigated numerically. An upper limit on the strength of primordial magnetic fields…

天体物理学 · 物理学 2009-12-30 Baolian Cheng , David N. Schramm , James W. Truran

We study primordial magnetic field effects on the matter perturbations in the Universe. We assume magnetic field generation prior to the big bang nucleosynthesis (BBN), i.e. during the radiation dominated epoch of the Universe expansion,…

宇宙学与河外天体物理 · 物理学 2015-06-12 Tina Kahniashvili , Yurii Maravin , Aravind Natarajan , Nicholas Battaglia , Alexander G. Tevzadze

Hydrogen recombination in the early Universe in the presence of a magnetic field is studied. An equation for the temperature of recombination in the presence of a magnetic field is derived. Limiting cases of weak and strong fields are…

高能物理 - 唯象学 · 物理学 2016-11-21 N. O. Agasian , S. M. Fedorov

We present generic bounds on magnetic fields produced from cosmic inflation. By investigating field bounds on the vector potential, we constrain both the quantum mechanical production of magnetic fields and their classical growth in a model…

宇宙学与河外天体物理 · 物理学 2016-03-10 Daniel Green , Takeshi Kobayashi

A variety of observations impose upper limits at the nano Gauss level on magnetic fields that are coherent on inter-galactic scales while blazar observations indicate a lower bound $\sim 10^{-16}$ Gauss. Such magnetic fields can play an…

宇宙学与河外天体物理 · 物理学 2021-06-15 Tanmay Vachaspati

In this paper, we revisit in detail the effects of primordial magnetic fields on big bang nucleosynthesis (BBN) including a discussion of the magnetic field geometry and the anomalous magnetic moment. The presence of magnetic fields affects…

天体物理学 · 物理学 2009-12-30 Baolian Cheng , Angela V. Olinto , David N. Schramm , James W. Truran

We study the impact of the extra density fluctuations induced by primordial magnetic fields on the reionization history in the redshift range: $6 < z < 10$. We perform a comprehensive MCMC physical analysis allowing the variation of…

宇宙学与河外天体物理 · 物理学 2015-05-13 Kanhaiya L. Pandey , T. Roy Choudhury , Shiv K. Sethi , Andrea Ferrara

We consider the possibility of generation of the seeds of primordial magnetic field on inflation and show that the effect of the back reaction of this field can be very important. Assuming that back reaction does not spoil inflation we find…

宇宙学与河外天体物理 · 物理学 2009-09-28 Vittoria Demozzi , Viatcheslav Mukhanov , Hector Rubinstein

We point out that the lower bound on the primordial magnetic field required to seed the galactic dynamo is significantly relaxed in an open universe or in a universe with a positive cosmological constant. It is shown that, for reasonable…

天体物理学 · 物理学 2008-11-26 Anne-Christine Davis , Matthew Lilley , Ola Tornkvist

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

Primordial magnetic fields possibly generated in the very early universe are one of the candidates for the origin of magnetic fields observed in many galaxies and galaxy clusters. After recombination, the dissipation process of the…

天体物理学 · 物理学 2009-11-11 Hiroyuki Tashiro , Naoshi Sugiyama

The presence of magnetic fields in the early universe affects the cosmological processes, leading to the distinct signature, which allows constraining their properties and the genesis mechanisms. In this study, we revisit the method to…

宇宙学与河外天体物理 · 物理学 2024-11-13 Ashu Kushwaha , Teruaki Suyama

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
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