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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 present new generation mechanisms of magnetic fields in supernova remnant shocks propagating to partially ionized plasmas in the early universe. Upstream plasmas are dissipated at the collisionless shock, but hydrogen atoms are not…

高能天体物理现象 · 物理学 2022-09-08 Shuhei Kashiwamura , Yutaka Ohira

It was recently shown that the vanishing of the Coulomb field related to the electric charge of a black hole by virtue of a tiny but non-vanishing photon mass can produce an electric asymmetry in the universe. This process can have place…

高能物理 - 唯象学 · 物理学 2007-05-23 Diego N. Pelliccia

We give a pedagogical introduction to two aspects of magnetic fields in the early universe. We first focus on how to formulate electrodynamics in curved space time, defining appropriate magnetic and electric fields and writing Maxwell…

宇宙学与河外天体物理 · 物理学 2014-11-20 Kandaswamy Subramanian

Large scale primordial magnetic fields (PMFs) threading the intergalactic medium are observed ubiquitously in the Universe playing a key role in the cosmic evolution. Their origin is still debated constituting a very active field of…

宇宙学与河外天体物理 · 物理学 2023-06-14 Theodoros Papanikolaou , Konstantinos N. Gourgouliatos

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 second order.…

天体物理学 · 物理学 2007-05-23 Keitaro Takahashi , Kiyotomo Ichiki , Hiroshi Ohno , Hidekazu Hanayama , Naoshi Sugiyama

There is strong observational evidence for the presence of large-scale magnetic fields MF in galaxies and clusters, with strength $\sim \mu$G and coherence lenght on the order of Kpc. However its origin remains as an outstanding problem.…

宇宙学与河外天体物理 · 物理学 2014-09-08 Eduard F. Piratova , Edilson A. Reyes , Héctor J. Hortúa

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

We describe the generation of the electric current flowing along the external magnetic field in the system of massive charged fermions, possessing anomalous magnetic moments and electroweakly interacting with background matter. This current…

高能物理 - 唯象学 · 物理学 2019-06-07 Maxim Dvornikov

We analyze the generation of helical magnetic fields during preheating in a model of low-scale electroweak (EW) hybrid inflation. We show how the inhomogeneities in the Higgs field, resulting from tachyonic preheating after inflation, seed…

高能物理 - 唯象学 · 物理学 2008-12-18 Andres Diaz-Gil , Juan Garcia-Bellido , Margarita Garcia Perez , Antonio Gonzalez-Arroyo

The existence of magnetic fields in the universe is unmistakable. They are observed at all scales from stars to galaxy clusters. However, the origin of these fields remains enigmatic. It is believed that magnetic field seeds may have…

广义相对论与量子宇宙学 · 物理学 2022-08-17 Orfeu Bertolami , Maria Margarida Lima , Filipe C. Mena

Strongly supercooled first order phase transitions (FOPTs) can produce primordial black hole (PBH) dark matter (DM) along with observable gravitational waves (GWs) from bubble collisions. Such FOPTs may also produce coherent magnetic fields…

高能物理 - 唯象学 · 物理学 2025-03-24 Shyam Balaji , Malcolm Fairbairn , Maria Olalla Olea-Romacho

We study the magnetic fields produced in the early Universe during the electroweak symmetry breaking by considering random configurations of an inhomogeneous Higgs field. By exploiting the inherent randomness of the initial configurations…

高能物理 - 唯象学 · 物理学 2026-04-28 Károly Seller , Günter Sigl

Magnetic fields appear to be ubiquitous in astrophysical environments. Their existence in the intracluster medium is established through observations of synchrotron emission and Faraday rotation. On the other hand, the nature of magnetic…

宇宙学与河外天体物理 · 物理学 2015-05-30 Dongsu Ryu , Dominik R. G. Schleicher , Rudolf A. Treumann , Christos G. Tsagas , Lawrence M. Widrow

In this thesis, we have studied the generation and evolution of the magnetic field in the early Universe. We investigated the generation of magnetic fields in the presence of chiral symmetry and gravitational anomaly. We have used modified…

宇宙学与河外天体物理 · 物理学 2017-12-20 Arun Kumar Pandey

A primordial magnetic field may be generated during an inflationary period if conformal invariance is broken. We reexamine and generalize previous results about the magnetic field produced by couplings of the form $R^n…

天体物理学 · 物理学 2009-10-28 F. D. Mazzitelli , F. M. Spedalieri

We review the creation mechanism of primordial black holes from first order phase transitions. We discuss various model-dependent and independent mechanisms and relate the properties of these mechanisms to the properties of primordial black…

高能物理 - 唯象学 · 物理学 2025-12-30 Indra Kumar Banerjee , Ujjal Kumar Dey , Shaaban Khalil

Magnetic fields have been observed in galaxies, clusters of galaxies and probably in superclusters. While mechanisms exist to generate these in the late universe, it is possible that magnetic fields have existed since very early times. This…

天体物理学 · 物理学 2009-12-07 Iain A. Brown

It is usually assumed that when Weyl invariance is unbroken in the electromagnetic sector, the energy density of primordial magnetic fields will redshift as radiation. Here we show that primordial magnetic fields do not exhibit…

宇宙学与河外天体物理 · 物理学 2019-07-22 Takeshi Kobayashi , Martin S. Sloth

The origin of galactic and extra-galactic magnetic fields is an unsolved problem in modern cosmology. A possible scenario comes from the idea of these fields emerged from a small field, a seed, which was produced in the early universe…

宇宙学与河外天体物理 · 物理学 2013-06-14 Hector J. Hortua , Leonardo Castaneda , Juan M. Tejeiro