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相关论文: Evolution of cosmic string configurations

200 篇论文

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

We provide a general overview of the velocity-dependent one-scale model for cosmic string evolution and discuss two further extensions to it. We introduce and justify a new ansatz for the momentum parameter $k$, and also incorporate the…

高能物理 - 唯象学 · 物理学 2014-11-17 C. J. A. P. Martins , E. P. S. Shellard

We set up and analyse a model for the non-equilibrium evolution of a network of cosmic strings initially containing only loops and no infinite strings. Due to this particular initial condition, our analytical approach differs significantly…

高能物理 - 唯象学 · 物理学 2009-10-31 E. J. Copeland , T. W. B. Kibble , D. A. Steer

We discuss the cosmological evolution of cosmic strings with time-dependent tension. We show that, in the case that the tension changes as a power of time, the cosmic string network obeys the scaling solution: the characteristic scale of…

高能物理 - 唯象学 · 物理学 2009-11-11 Masahide Yamaguchi

Understanding of the signatures of cosmic string networks is limited by a large uncertainty in the sizes at which cosmic string loops form. We review cosmic string network evolution, and the gravitational signatures, with emphasis on this…

天体物理学 · 物理学 2007-11-07 Joseph Polchinski

We study the effects of friction on the scaling evolution of string networks in condensed matter and cosmological contexts. We derive a generalized `one-scale' model with the string correlation length $L$ and velocity $v$ as dynamical…

高能物理 - 唯象学 · 物理学 2016-09-01 C. J. A. P. Martins , E. P. S. Shellard

We present results of new field-theoretic simulation of cosmological axion strings, which are eight times longer than previous ones. We have upgraded our simulation of physical strings in Hiramatsu et al. (2011) in terms of the number of…

高能物理 - 唯象学 · 物理学 2019-12-06 Masahiro Kawasaki , Toyokazu Sekiguchi , Masahide Yamaguchi , Jun'ichi Yokoyama

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

An analytic model of long string network evolution, recently developed by the authors, is presented in detail, and modified to describe string loop evolution. By treating the average string velocity, as well as the characteristic…

高能物理 - 唯象学 · 物理学 2011-05-05 C. J. A. P. Martins , E. P. S. Shellard

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

We describe the detailed study and results of high-resolution numerical simulations of string-induced structure formation in open universes and those with a non-zero cosmological constant. The effect from small loops generated from the…

天体物理学 · 物理学 2009-09-25 J. H. P. Wu , P. P. Avelino , E. P. S. Shellard , B. Allen

It has recently been realised that strings with time-dependent tensions exhibit interesting dynamics; in particular, when the tension decreases loops of string can grow and possibly percolate. We extend previous analytic studies of strings…

高能物理 - 理论 · 物理学 2026-01-09 Hubert Lau Sze Chun , Joseph Conlon

We analyze all individual cosmic strings of various lengths in a large ensemble of the global cosmic string networks in the post-inflationary scenario, obtained from numerical simulations on a discrete lattice with $N^3 = 4096^3$. A strong…

高能物理 - 唯象学 · 物理学 2025-09-19 Heejoo Kim , Minho Son

We study the formation and evolution of an interconnected string network in large-scale field-theory numerical simulations, both in flat spacetime and in expanding universe. The network consists of gauge U(1) strings of two different kinds…

高能物理 - 理论 · 物理学 2008-11-26 Jon Urrestilla , Alexander Vilenkin

We describe a numerical simulation of the evolution of an $S_3$ cosmic string network which takes fully into account the non-commutative nature of the cosmic string fluxes and the topological obstructions which hinder strings from moving…

天体物理学 · 物理学 2009-10-30 Patrick N. McGraw

We investigate the evolution of infinite strings as a part of a complete cosmic string network in flat space. We perform a simulation of the network which uses functional forms for the string position and thus is exact to the limits of…

广义相对论与量子宇宙学 · 物理学 2013-05-29 Vitaly Vanchurin , Ken Olum , Alexander Vilenkin

The evolution of cosmic string networks is an interesting dynamical problem. The equations governing these networks are classical and fully specified, but the length scale at which cosmic string loops form has been uncertain to tens of…

天体物理学 · 物理学 2009-06-23 Joseph Polchinski

We examine the scaling properties of an evolving network of strings in Minkowski spacetime and study the evolution of length scales in terms of a 3-scale model proposed by Austin, Copeland and Kibble (ACK). We find good qualitative and some…

天体物理学 · 物理学 2008-11-26 Graham R. Vincent , Mark Hindmarsh , Mairi Sakellariadou

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

The dynamics of string junctions and their influence on the evolution of cosmic superstring networks are studied in full detail. We review kinematic constraints for colliding strings in a Friedmann-Lema\^itre-Robertson-Walker background and…

宇宙学与河外天体物理 · 物理学 2019-03-27 I. Yu. Rybak , A. Avgoustidis , C. J. A. P. Martins
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