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相关论文: Primordial magnetic fields from pseudo-Goldstone b…

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Primordial magnetic fields seem to be a generic relic of phase transitions in the early universe. We consider a primordial electromagnetic field formed as a result of a second-order phase transition, and show that it is stable to thermal…

天体物理学 · 物理学 2016-08-30 A. P. Martin , A. C. Davis

It is argued that large scale cosmic magnetic field could be generated in the primeval plasma slightly before hydrogen recombination. Non-zero vorticity, necessary for that, might be created by the photon diffusion in the second order in…

天体物理学 · 物理学 2016-08-30 Z. Berezhiani , A. D. Dolgov

We study the backreaction problem in a mechanism of magnetogenesis from inflation. In usual analysis, it has been assumed that the backreaction due to electromagnetic fields spoils inflation once it becomes important. However, there exists…

宇宙学与河外天体物理 · 物理学 2014-12-09 Sugumi Kanno , Jiro Soda , Masa-aki Watanabe

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

Pseudo-Goldstone bosons (pGBs) can provide technically natural inflatons, as has been comparatively well-explored in the simplest axion examples. Although inflationary success requires trans-Planckian decay constants, f > Mp, several…

高能物理 - 理论 · 物理学 2015-09-01 C. P. Burgess , Diederik Roest

Any attempt to understand the ubiquitous nature of the magnetic field in the present universe seems to lead us towards its primordial origin. For large-scale magnetic fields, however, their strength and length scale may not necessarily…

宇宙学与河外天体物理 · 物理学 2025-09-01 Subhasis Maiti , Debaprasad Maity , Rohan Srikanth

We present preliminary results on the possible effects that primordial magnetic fields can have for a warm inflation scenario, based on global supersymmetry, with a new-inflation-type potential. This work is motivated by two considerations:…

宇宙学与河外天体物理 · 物理学 2015-06-17 Gabriella Piccinelli , Angel Sanchez , Alejandro Ayala , Ana Julia Mizher

Magnetic fields observed across cosmic scales are difficult to explain within conventional physics. A primordial origin is, thus, often assumed. While a nonminimal coupling of the inflaton with the electromagnetic field could theoretically…

宇宙学与河外天体物理 · 物理学 2026-05-22 Debottam Nandi , Debajyoti Choudhury

The role played by a primordial magnetic field during the pre-recombination epoch is analysed through the cyclotron radiation (due to the free electrons) it might produce in the primordial plasma. We discuss the constraint implied by the…

天体物理学 · 物理学 2009-10-30 Denis Puy , Patrick Peter

We explore the generation of large-scale magnetic fields in the so-called moduli inflation. The hypercharge electromagnetic fields couple to not only a scalar field but also a pseudoscalar one, so that the conformal invariance of the…

宇宙学与河外天体物理 · 物理学 2015-06-30 Kazuharu Bamba

We analyse the evolution of primordial magnetic fields in spatially flat Friedmann universes and reconsider the belief that, after inflation, these fields decay adiabatically on all scales. Without~abandoning classical electromagnetism or…

宇宙学与河外天体物理 · 物理学 2017-05-11 Christos G. Tsagas

The origin of interstellar and intergalactic magnetic fields remains largely unknown. One possibility is that they are related to the primordial magnetic fields (PMFs) produced by, for instance, the phase transitions of the early Universe.…

高能天体物理现象 · 物理学 2024-03-05 Yao-Yu Li , Chi Zhang , Ziwei Wang , Ming-Yang Cui , Yue-Lin Sming Tsai , Qiang Yuan , Yi-Zhong Fan

Generation of primordial magnetic fields during inflation typically requires the breaking of conformal invariance of the Electromagnetic action. In this paper this has been achieved naturally in a higher dimensional cosmological model with…

宇宙学与河外天体物理 · 物理学 2014-03-12 Kumar Atmjeet , Isha Pahwa , T. R. Seshadri , Kandaswamy Subramanian

Cosmic strings are stable topological defects that may have been created at a phase transition in the early universe. It is a growing belief that, for a wide range of theoretical models, such strings may be superconducting and carry…

高能物理 - 唯象学 · 物理学 2010-11-19 Konstantinos Dimopoulos

Large scale strong magnetic fields in galaxies are generally thought to have been generated by a mean field dynamo. In order to have generated the fields observed, the dynamo would have had to have operated for a sufficiently long period of…

天体物理学 · 物理学 2007-05-23 A. Kandus , R. Opher , S. R. M. Barros

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

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

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

Generation of large-scale magnetic fields in inflationary cosmology is studied in teleparallelism, where instead of the scalar curvature in general relativity, the torsion scalar describes the gravity theory. In particular, we investigate a…

宇宙学与河外天体物理 · 物理学 2014-03-26 Kazuharu Bamba , Chao-Qiang Geng , Ling-Wei Luo

We study the generation of primeval magnetic fields during inflation era in nonlinear theories of electrodynamics. Although the intensity of the produced fields strongly depends on characteristics of inflation and on the form of…

天体物理学 · 物理学 2008-11-26 L. Campanelli , P. Cea , G. L. Fogli , L. Tedesco