We simulate the formation and the evolution of global strings taking into account the expansion of the universe and the concomitant change of the effective potential, that is, the change from the restoration stage of the global {\it U}(1)-symmetry to the broken stage. Starting from the thermal equilibrium state, we run simulations for 100 sets of different initial conditions in 2+1 dimensions. As a result, we find deviation from scale invariance. This is because the energy loss mechanism is pair annihilation rather than intercommutation, so that a string and an anti-string attract each other under a logarithmic potential
We present a full characterization of the phase transition in U(1) scalar field theory and of the as...
Lattice-based string formation algorithms can, at least in principle, be reduced to the study of the...
Cosmic strings provide a radically different paradigm for the formation of structure to the prevaili...
We completely elucidate quantitative nature of cosmological evolution of global string network, that...
We present a toy model for the investigation of the formation of semilocal strings, where a planar s...
We present a toy model for the investigation of the formation of semilocal strings, where a planar s...
A system of intercommuting cosmic strings is numerically evolved in a homogeneous radiation-dominate...
We describe a numerical simulation of the evolution of an S3 cosmic string network which takes fully...
Results on cosmic strings are summarized including: (1) the application of non-equilibrium statistic...
We report on a detailed numerical study of the evolution of semilocal string networks, based on the ...
Many extensions to the Standard Model of particle physics feature a first-order phase transition in ...
We describe a numerical simulation of the evolution of an S 3 cosmic string network which takes full...
It was argued, and fought through numerical work that the results of non-dynamical Monte Carlo compu...
In this paper we investigate the dynamical properties of binary cosmic strings. We find extrinsic cu...
There has been recent interest in the evolution and cosmological consequences of global axionic stri...
We present a full characterization of the phase transition in U(1) scalar field theory and of the as...
Lattice-based string formation algorithms can, at least in principle, be reduced to the study of the...
Cosmic strings provide a radically different paradigm for the formation of structure to the prevaili...
We completely elucidate quantitative nature of cosmological evolution of global string network, that...
We present a toy model for the investigation of the formation of semilocal strings, where a planar s...
We present a toy model for the investigation of the formation of semilocal strings, where a planar s...
A system of intercommuting cosmic strings is numerically evolved in a homogeneous radiation-dominate...
We describe a numerical simulation of the evolution of an S3 cosmic string network which takes fully...
Results on cosmic strings are summarized including: (1) the application of non-equilibrium statistic...
We report on a detailed numerical study of the evolution of semilocal string networks, based on the ...
Many extensions to the Standard Model of particle physics feature a first-order phase transition in ...
We describe a numerical simulation of the evolution of an S 3 cosmic string network which takes full...
It was argued, and fought through numerical work that the results of non-dynamical Monte Carlo compu...
In this paper we investigate the dynamical properties of binary cosmic strings. We find extrinsic cu...
There has been recent interest in the evolution and cosmological consequences of global axionic stri...
We present a full characterization of the phase transition in U(1) scalar field theory and of the as...
Lattice-based string formation algorithms can, at least in principle, be reduced to the study of the...
Cosmic strings provide a radically different paradigm for the formation of structure to the prevaili...