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Cosmology, high-energy physics and astrophysics are converging on the study of large-scale magnetic fields. While the experimental evidence for the existence of large-scale magnetization in galaxies, clusters and superclusters is rather…

天体物理学 · 物理学 2009-11-10 Massimo Giovannini

We consider the possibility of inflationary magnetogenesis due to dynamical couplings of the electromagnetic fields to gravity. We find that large primordial magnetic fields can be generated during inflation without the strong coupling…

宇宙学与河外天体物理 · 物理学 2016-02-26 Peng Qian , Zong-Kuan Guo

A possible explanation for the origin of the magnetic fields observed today in matter structures is that they were generated in the primordial universe. After briefly revising the model of a primordial stochastic magnetic field and…

宇宙学与河外天体物理 · 物理学 2015-03-19 Chiara Caprini

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 detection of magnetic fields at high redshifts, and in empty intergalactic space, support the idea that cosmic magnetism has a primordial origin. Assuming that Maxwellian electromagnetism and general relativity hold, and without…

广义相对论与量子宇宙学 · 物理学 2015-06-11 J. D. Barrow , C. G. Tsagas , K. Yamamoto

This paper concerns the generation and evolution of the cosmological (large-scale $\sim Mpc$) magnetic fields in an inflationary universe. The universe during inflation is represented by de Sitter space-time. We started with the Maxwell…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Zuxiang Dai

We compute the contribution to the scalar metric perturbations from large-scale magnetic fields which are generated during inflation. We show that apart from the usual passive and compensated modes, the magnetic fields also contribute to…

宇宙学与河外天体物理 · 物理学 2012-11-01 Camille Bonvin , Chiara Caprini , Ruth Durrer

Recently observational lower bounds on the strength of cosmic magnetic fields were reported, based on gamma-ray flux from distant blazars. If inflation is responsible for the generation of such magnetic fields then the inflation energy…

宇宙学与河外天体物理 · 物理学 2012-10-23 Tomohiro Fujita , Shinji Mukohyama

The interrelation between the generation of large-scale electric fields and that of large-scale magnetic fields due to the breaking of the conformal invariance of the electromagnetic field in inflationary cosmology is studied. It is shown…

天体物理学 · 物理学 2009-06-23 Kazuharu Bamba

The origin of the $\mu$G magnetic fields observed in galaxies is unknown. One promising scenario is that magnetic fields generated during inflation, larger than 0.1 nG on Mpc scales, were adiabatically compressed to $\mu$G strengths in…

宇宙学与河外天体物理 · 物理学 2022-04-06 Sayan Mandal , Neelima Sehgal , Toshiya Namikawa

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

We propose a new mechanism for magnetic field generation from inflation, by which strong magnetic fields can be generated on cosmological scales. These fields may be observable by cosmic microwave background radition measurements, and may…

天体物理学 · 物理学 2009-11-10 Tomislav Prokopec , Ewald Puchwein

We present a five dimensional unified theory of gravity and electromagnetism which leads to modified Maxwell equations, suggesting a new origin for galactic magnetic fields. It is shown that a region with nonzero scalar curvature would…

广义相对论与量子宇宙学 · 物理学 2009-11-19 A. Borzou , H. R. Sepangi , R. Yousefi , A. H. Ziaie

The origin of our universe's cosmological magnetic fields remains a mystery. In this study, we consider whether these magnetic fields could have been generated in the early universe by a population of charged, spinning primordial black…

宇宙学与河外天体物理 · 物理学 2023-05-31 Dan Hooper , Aurora Ireland , Gordan Krnjaic

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

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

Models of cosmic inflation posit an early phase of accelerated expansion of the universe, driven by the dynamics of one or more scalar fields in curved spacetime. Though detailed assumptions about fields and couplings vary across models,…

宇宙学与河外天体物理 · 物理学 2014-05-09 Alan H. Guth , David I. Kaiser , Yasunori Nomura

We discuss the evolution of cosmological magnetic fields from the early universe to the present. We review different scenarios for magnetogenesis in the early universe and follow the subsequent evolution of these fields as the universe…

天体物理学 · 物理学 2007-05-23 Angela V. Olinto

We investigate the generation of primordial magnetic fields from stochastic currents created by the cosmological transition from inflation to reheating. We consider N charged scalar fields coupled to the electromagnetic field in a curved…

天体物理学 · 物理学 2009-11-07 Esteban Calzetta , Alejandra Kandus

In this letter, we discuss generation of magnetic field from cosmological perturbations. We consider the evolution of three component plasma (electron, proton and photon) evaluating the collision term between elecrons and photons up to the…

天体物理学 · 物理学 2009-11-10 Keitaro Takahashi , Kiyotomo Ichiki , Hiroshi Ohno , Hidekazu Hanayama