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相关论文: Cosmic String Loops, Large and Small

200 篇论文

Cosmic superstrings of string theory differ from conventional cosmic strings of field theory. We review how the physical and cosmological properties of the macroscopic string loops influence experimental searches for these relics from the…

宇宙学与河外天体物理 · 物理学 2018-05-16 David F. Chernoff , S. -H. Henry Tye

We extend and develop our previous work on the evolution of a network of cosmic strings. The new treatment is based on an analysis of the probability distribution of the end-to-end distance of a randomly chosen segment of left-moving string…

高能物理 - 唯象学 · 物理学 2016-09-01 Daren Austin , E. J. Copeland , T. W. B. Kibble

At early stages the dynamics of cosmic string networks is expected to be influenced by an excessive production of small loops at the scales of initial conditions l_{min}. To understand the late time behavior we propose a very simple…

高能物理 - 理论 · 物理学 2014-11-21 Vitaly Vanchurin

Cosmic (super)strings offer promising ways to test ideas about the early universe and physics at high energies. While in field theory constructions their tension is usually assumed to be constant (or at most slowly-varying), this is often…

高能物理 - 唯象学 · 物理学 2025-05-08 Filippo Revello , Gonzalo Villa

We investigate the evolution of the global string network in the radiation dominated universe by use of numerical simulations in 3+1 dimensions. We find that the global string network settles down to the scaling regime where the energy…

高能物理 - 唯象学 · 物理学 2016-09-06 Masahide Yamaguchi

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

Cosmic superstrings are produced towards the end of the brane inflation. If the string tension is low enough, loops tend to be relatively long-lived. The resultant string network is expected to contain many loops which are smaller than…

天体物理学 · 物理学 2007-09-10 David F. Chernoff , S. -H. Henry Tye

In this paper we present the results of numerical simulations intended to study the behavior of non-Abelian cosmic strings networks. In particular we are interested in discussing the variations in the asymptotic behavior of the system as we…

宇宙学与河外天体物理 · 物理学 2016-06-17 G. Cella , M. Pieroni

We consider the gravitational lensing produced by long cosmic strings formed in a GUT scale phase transition. We derive a formula for the deflection of photons which pass near the strings that reduces to an integral over the light cone…

天体物理学 · 物理学 2009-10-30 Andrew A. de Laix

We solve numerically the Boltzmann equation describing the evolution of a cosmic string network which contains only loops. In Minkowski space time the equilibrium solution predicted by statistical mechanics is recovered, and we prove that…

天体物理学 · 物理学 2009-10-31 Joao Magueijo , Haavard Sandvik , Daniele Steer

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

We develop a semi-analytical model to describe the cosmological evolution of networks of cosmic strings with small-scale structure, by extending the velocity-dependent one-scale model to include an additional lengthscale describing the…

宇宙学与河外天体物理 · 物理学 2026-03-26 Teresa O. Miranda , Lara Sousa

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

When moduli roll in the early universe, all physical scales - including string tensions - simultaneously evolve. The dynamics of cosmic string loops with time-varying tension can produce cosmic string loop trackers in which most of the…

高能物理 - 唯象学 · 物理学 2025-11-21 Joseph P. Conlon , Edmund J. Copeland , Edward Hardy , Noelia Sánchez González

We derive a full analytical approximation to the stochastic gravitational wave background generated by the loops that are produced throughout the cosmological evolution of cosmic string networks. We show that this approximation not only…

宇宙学与河外天体物理 · 物理学 2020-05-13 Lara Sousa , Pedro P. Avelino , Guilherme S. F. Guedes

In supersymmetric theories, cosmic strings produced in the early Universe often have a width of TeV scale, while the tension is much larger. In a scaling regime, an infinite cosmic string releases significant fraction of its energy in the…

高能物理 - 唯象学 · 物理学 2015-03-19 Masahiro Kawasaki , Koichi Miyamoto , Kazunori Nakayama

We present a method for the calculation of the gravitational back reaction cutoff on the smallest scales of cosmic string networks taking into account that not all modes on strings interact with all other modes. This results in a small…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Xavier Siemens , Ken D. Olum , Alexander Vilenkin

We report on the results of performing computational gravitational backreaction on cosmic string loops taken from a network simulation. The principal effect of backreaction is to smooth out small-scale structure on loops, which we…

广义相对论与量子宇宙学 · 物理学 2025-11-14 Jeremy M. Wachter , Ken D. Olum , Jose J. Blanco-Pillado , Vishnu R. Gade , Kirthivarsha Sivakumar

The fragmentation of horizon crossing superstrings creates loops that accrete and bind to collapsing matter perturbations if the string tension is less than a critical value and if the loops are large-scale. For typical model parameters…

宇宙学与河外天体物理 · 物理学 2009-09-01 David F. Chernoff

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