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相关论文: Primordial Magnetic Fields From String Cosmology

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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

Generation of large-scale magnetic fields is studied in dilaton electromagnetism in noncommutative inflationary cosmology, taking into account the effects of the spacetime uncertainty principle motivated by string theory. We show that it is…

高能物理 - 唯象学 · 物理学 2007-05-23 Kazuharu Bamba , J. Yokoyama

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

The generation of large-scale magnetic fields is studied in dilaton electromagnetism in noncommutative inflationary cosmology taking into account the effects of the spacetime uncertainty principle motivated by string theory. We show that it…

高能物理 - 唯象学 · 物理学 2009-11-10 Kazuharu Bamba , J. Yokoyama

After a discussion of the inflationary production of primordial magnetic seeds, and a short review of various possible mechanisms, we concentrate on the analysis of the photon-dilaton coupling typical of string theory models. Particular…

天体物理学 · 物理学 2009-11-11 M. Gasperini

The explanation of the observed galactic magnetic fields may require the existence of a primordial magnetic field. Such a field may arise during the early cosmological phase transitions, or because of other particle physics related…

天体物理学 · 物理学 2009-10-30 Kari Enqvist

The duality-type symmetries of string cosmology naturally lead to a pre-big-bang phase of accelerated evolution as dual counterpart of the decelerated expansion of standard cosmology. We discuss several properties of this scenario,…

高能物理 - 理论 · 物理学 2011-05-23 M. Gasperini , G. Veneziano

Large-scale magnetic fields are observed today to be coherent on galactic scales. While there exists an explanation for their amplification and their specific configuration in spiral galaxies -- the dynamo mechanism -- a satisfying…

高能物理 - 理论 · 物理学 2009-12-04 Rhiannon Gwyn , Stephon Alexander , Robert H. Brandenberger , Keshav Dasgupta

We present some phenomenological aspects of the pre-big-bang cosmological model inspired by the duality properties of string theory. In particular, assuming the spatial sections of the homogeneous background geometry to be isotropic, we…

天体物理学 · 物理学 2012-10-23 R. Durrer , K. E. Kunze , M. Sakellariadou

Mechanisms of generation of magnetic fields in the early universe which could seed the present-day large scale galactic magnetic fields, are briefly reviewed. Three possible ways to create large scale magnetic fields are discussed: breaking…

高能物理 - 唯象学 · 物理学 2016-11-23 A. D. Dolgov

The different couplings of the dilaton to the U(1) gauge field of heterotic and Type I superstrings may leave an imprint on the relics of the very early cosmological evolution. Working in the context of the pre-big bang scenario, we discuss…

高能物理 - 理论 · 物理学 2010-04-05 M. Gasperini , S. Nicotri

Cosmic strings are topological defects which can be formed as a result of phase transitions with a spontaneous symmetry breaking in the early Universe. The possibility of the generation of a magnetic field around a cosmic string on the…

宇宙学与河外天体物理 · 物理学 2013-05-02 L. V. Zadorozhna , B. I. Hnatyk , Yu. A. Sitenko

I report recent studies on the evolution of perturbations in the context of the ``pre-big-bang" scenario typical of string cosmology, with emphasis on the formation of a stochastic background of relic photons and gravitons, and its possible…

高能物理 - 理论 · 物理学 2009-09-25 M. Gasperini

The observed galactic magnetic fields may have a primordial origin. I briefly review the observations, their interpretation in terms of the dynamo theory, and the current limits on cosmological magnetic fields. Several possible mechanisms…

天体物理学 · 物理学 2007-05-23 Kari Enqvist

This paper examines the generation of seed magnetic fields due to the growth of cosmological perturbations. In the radiation era, different rates of scattering from photons induce local differences in the ion and electron density and…

天体物理学 · 物理学 2008-11-26 E. R. Siegel , J. N. Fry

Using lattice techniques we investigate the generation of long range cosmological magnetic fields during a cold electroweak transition. We will show how magnetic fields arise, during bubble collisions, in the form of magnetic strings. We…

高能物理 - 格点 · 物理学 2009-04-14 A. Diaz-Gil , J. Garcia-Bellido , M. Garcia Perez , A. Gonzalez-Arroyo

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

The origin of the substantial magnetic fields that are found in galaxies and on even larger scales, such as in clusters of galaxies, is yet unclear. If the second-order couplings between photons and electrons are considered, then…

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

Cosmic superstrings are produced at the end of brane inflation. Their properties are similar to cosmic strings arising in grand unified theories. Like cosmic strings they can give rise to a primordial magnetic field, as a result of vortical…

高能物理 - 唯象学 · 物理学 2009-11-11 Anne-Christine Davis , Konstantinos Dimopoulos

A string cosmology scenario ("pre-big-bang") postulates that the evolution of the Universe starts from a state of very small curvature and coupling, undergoes a long phase of dilaton-driven kinetic inflation and at some later time joins…

高能物理 - 理论 · 物理学 2016-10-26 Ram Brustein
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