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We present a mechanism that allows to describe any nonlinear theory of Electrodynamics as a consequence of the coupling of the electromagnetic field to gravity in the presence of a vacuum represented by the cosmological constant. We…

广义相对论与量子宇宙学 · 物理学 2017-06-21 M. Novello , C. E. L. Ducap

It is argued that static electromagnetic sources induce Weyl-Majumdar-Papapetrou solutions for the spacetime metric. The acceleration in such fields has a term many orders of magnitude stronger than usual perturbative terms. Two…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Boyko V. Ivanov

Within the scope of a spherically symmetric space-time we study the role of different types of matter in the formation of different configurations with spherical symmetries. Here we have considered matter with barotropic equation of state,…

广义相对论与量子宇宙学 · 物理学 2021-11-22 Bijan Saha

A spacetime consisting of parallel electric/magnetic fields held together by its own gravity in the presence of a cosmological constant $\Lambda$ is derived as a limit of the de Sitter/anti-de Sitter C-metric. The limiting procedure is…

广义相对论与量子宇宙学 · 物理学 2018-10-17 Yen-Kheng Lim

Cylindrically symmetric inhomogeneous cosmological model for bulk viscous fluid distribution with electromagnetic field is obtained. The source of the magnetic field is due to an electric current produced along the z-axis. $F_{12}$ is the…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Anirudh Pradhan , Vandana Rai , Kanti Jotania

Earlier Enqvist and Olesen have shown that formation of ferromagnetic planar walls in vacuum at GUT scales in comoving plasmas may generate a large scale magnetic field of $B_{now}\simeq{10^{-14}G}$. In this paper we show that starting from…

广义相对论与量子宇宙学 · 物理学 2015-06-18 L. C. Garcia de Andrade

It is argued that static electric or magnetic fields induce Weyl-Majumdar-Papapetrou solutions for the metric of spacetime. Their gravitational acceleration includes a term many orders of magnitude stronger than usual perturbative terms. It…

广义相对论与量子宇宙学 · 物理学 2007-05-23 B. V. Ivanov

It is shown that the standard cosmological model predicts {\it ab initio} generation of large-scale but very small-amplitude cosmic magnetic fields at the epoch of recombination of the primeval plasma. Matter velocities dominated by…

天体物理学 · 物理学 2007-05-23 Craig J. Hogan

We observe that the standard homogeneous cosmologies, those of Minkowski, de Sitter, and anti-de Sitter, which form the matrix for the Robertson--Walker scale factor, live naturally as isolated points inside a larger family of conformally…

广义相对论与量子宇宙学 · 物理学 2014-11-19 Jonathan Holland , George Sparling

We investigate the magnetic field which is generated by turbulent motions of a weakly ionized gas. Galactic molecular clouds give us an example of such a medium. As in the Kazantsev-Kraichnan model we assume a medium to be homogeneous and a…

星系天体物理 · 物理学 2013-09-25 Ya. N. Istomin , A. M. Kiselev

We consider the process of magnetogenesis in the context of nonsingular bounce cosmology. We show that large primordial magnetic fields can be generated during contraction without encountering strong coupling and backreaction issues. The…

广义相对论与量子宇宙学 · 物理学 2016-11-02 Peng Qian , Yi-Fu Cai , Damien A. Easson , Zong-Kuan Guo

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

We study a spatial-temporal structure of quantum fluctuations in the stress-energy tensor of zero-point modes for a scalar field in order to formulate a covariant model. The model describes an invariant vacuum contribution to the…

高能物理 - 理论 · 物理学 2025-05-06 A. Aynbund , V. V. Kiselev

Cosmological phase transitions accompanied by some kind of symmetry breaking would cause the creation of topological defects and the resulting production of primordial magnetic field. Moreover, such a procedure inevitably affects the cosmic…

高能物理 - 唯象学 · 物理学 2014-11-21 Michiyasu Nagasawa

We study the inflationary generation of helical cosmological magnetic fields in a higher-dimensional generalization of the electromagnetic theory. For this purpose, we also include a parity breaking piece to the electromagnetic action. The…

宇宙学与河外天体物理 · 物理学 2015-06-17 Kumar Atmjeet , T. R. Seshadri , Kandaswamy Subramanian

In this paper we show that noncommutativity in spatial coordinates can generate magnetic field in the early Universe on a horizon scale. The strength of such a magnetic field depends on the number density of massive charged particles…

高能物理 - 唯象学 · 物理学 2009-10-07 Anupam Mazumdar , Mohammad M. Sheikh-Jabbari

It is suggested that the exact value of the cosmological constant could be derived from first principles, based on entanglement of the Standard Model field vacuum with emergent holographic quantum geometry. For the observed value of the…

广义相对论与量子宇宙学 · 物理学 2018-04-03 Craig Hogan

In the present article we find a new class of solutions of Einstein's field equations. It describes stationary, cylindrically symmetric spacetimes with closed timelike geodesics everywhere outside the symmetry axis. These spacetimes contain…

广义相对论与量子宇宙学 · 物理学 2010-04-20 Oyvind Gron , Steinar Johannesen

In this study we advocate the view that the cosmological constant is of electromagnetic (em) origin, which can be generated from the collision of em shock waves coupled with gravitational shock waves. The wave profiles that participate in…

综合物理 · 物理学 2014-11-12 M. Halilsoy , S. Habib Mazharimousavi , O. Gurtug

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