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相关论文: Radiation constraints from cosmic strings

200 篇论文

We discuss radiative backreaction for global strings described by the Kalb-Ramond action with an analogous derivation to that for the point electron in classical electrodynamics. We show how local corrections to the equations of motion…

天体物理学 · 物理学 2009-10-22 R. A. Battye , E. P. S. Shellard

We consider radiative backreaction for global strings using the Kalb-Ramond formalism. In analogy to the point electron in classical electrodynamics, we show how local radiative corrections to the equations of motion allow one to remove the…

高能物理 - 唯象学 · 物理学 2009-10-28 R. A. Battye , E. P. S. Shellard

We study Goldstone boson (or axion) radiation from global $U(1)$-strings making direct quantitative comparisons between numerical scalar field theory simulations and linearized analytic calculations in the dual antisymmetric tensor…

天体物理学 · 物理学 2009-10-22 R. A. Battye , E. P. S. Shellard

We discuss key aspects of the nature of radiation from global strings and its impact on the relic axion density. Using a simple model we demonstrate the dependence on the spectrum of radiation emitted by strings. We then study the radiation…

高能物理 - 唯象学 · 物理学 2026-02-02 Richard A. Battye , Lukasz P. Bunio , Steven J. Cotterill , Pranav B. Gangrekalve Manoj

We implement adaptive mesh refinement (AMR) simulations of global topological strings using the public numerical relativity code, GRChombo. We perform a quantitative investigation of the dynamics of single sinusoidally displaced string…

宇宙学与河外天体物理 · 物理学 2022-04-28 Amelia Drew , E. P. S. Shellard

We develop methods by which cosmic superstring interactions can be studied in detail. These include the reconnection probability and emission of radiation such as gravitons or small string loops. Loop corrections to these are discussed, as…

高能物理 - 理论 · 物理学 2009-11-18 Mark G. Jackson

Cosmic strings provide a radically different paradigm for the formation of structure to the prevailing inflationary one. They afford some extra technical complications: for example, the calculation of the power spectrum of matter and…

天体物理学 · 物理学 2007-05-23 Mark Hindmarsh , Mairi Sakellariadou , Graham R. Vincent

We study the production of cosmological axions in the standard scenario in which a global string network forms at the Peccei-Quinn phase transition. We make detailed calculations of the axions produced by string loops (a previously…

天体物理学 · 物理学 2009-10-22 R. A. Battye , E. P. S. Shellard

We consider aspects of the low energy description of global cosmic strings. In the non-relativistic limit, we study the extent to which these are described by the combination of the Nambu-Gotto and Kalb-Ramond actions. While in a formal…

高能物理 - 唯象学 · 物理学 2022-09-21 Michael Dine

In this paper, we obtain the three-dimensional regular extremal black string solution incorporating $\alpha'$ corrections and a non-trivial Kalb-Ramond field. The difficulty in considering the Kalb-Ramond field lies in the fact that it…

高能物理 - 理论 · 物理学 2023-07-04 Shuxuan Ying

The existence of a scaling evolution for cosmic string loops in an expanding universe is demonstrated for the first time by means of numerical simulations. In contrast with what is usually assumed, this result does not rely on any…

天体物理学 · 物理学 2009-11-13 Christophe Ringeval , Mairi Sakellariadou , Francois Bouchet

Using the formalism developed in a previous paper we analyze the cosmological implications of our conclusions concerning the scaling behaviour of a network of cosmic strings, in particular the idea that once gravitational back-reaction…

高能物理 - 唯象学 · 物理学 2010-01-06 Daren Austin , E. J. Copeland , T. W. B. Kibble

We study the radiation reaction on cosmic strings due to the emission of dilatonic, gravitational and axionic waves. After verifying the (on average) conservative nature of the time-symmetric self-interactions, we concentrate on the finite…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Alessandra Buonanno , Thibault Damour

We examine the leading order corrections to the Nambu effective action for the motion of a cosmic string, which appear at fourth order in the ratio of the width to radius of curvature of the string. We determine the numerical coefficients…

高能物理 - 唯象学 · 物理学 2009-10-30 Malcolm Anderson , Filipe Bonjour , Ruth Gregory , John Stewart

We study the behaviour and consequences of cosmic string networks in contracting universes. They approximately behave during the collapse phase as a radiation fluids. Scaling solutions describing this are derived and tested against…

天体物理学 · 物理学 2015-06-24 P. P. Avelino , C. J. A. P. Martins , C. Santos , E. P. S. Shellard

We have studied numerically the evolution and decay of axion strings. These global defects decay mainly by axion emission and thus contribute to the cosmological axion density. The relative importance of this source relative to misalignment…

高能物理 - 唯象学 · 物理学 2009-10-31 C. Hagmann , S. Chang , P. Sikivie

We consider the evolution of a network of strings in an expanding universe, allowing for the formation of junctions between strings of different tensions. By explicitly including, in the velocity-dependent evolution equations for the…

高能物理 - 唯象学 · 物理学 2010-04-06 A. Avgoustidis , E. J. Copeland

We examine the spectrum of gravitational radiation emitted by a network of cosmic strings, with emphasis on the observational constraints and the opportunities for detection. The analysis improves over past work, as we use a…

天体物理学 · 物理学 2009-12-30 R. R. Caldwell , R. A. Battye , E. P. S. Shellard

The equation governing the time evolution of the number density of loops in a cosmic string network is a detailed balance determined by energy conservation. We solve this equation with the inclusion of the gravitational radiation effect…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Jorge V. Rocha

We investigate the properties of global cosmic string networks as a function of the ratio of string tension to Goldstone-field coupling, and as a function of the Hubble damping strength. Our results show unambiguously that the string…

高能物理 - 唯象学 · 物理学 2020-06-17 Vincent B. Klaer , Guy D. Moore
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