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相关论文: Semilocal Cosmic String Networks

200 篇论文

We study the cosmological constant problem in a three-dimensional N=2 supergravity theory with gauge group SU[2]_{global}xU[1]_{local}. The model we consider is known to admit string-like configurations, the so-called semi-local cosmic…

高能物理 - 理论 · 物理学 2009-10-30 Jose Daniel Edelstein

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

Cosmic string networks generate cosmological perturbations actively throughout the history of the universe. Thus, the string sourced anisotropy of the cosmic microwave background is not affected by Silk damping as much as the anisotropy…

天体物理学 · 物理学 2010-04-15 Levon Pogosian , S. -H. Henry Tye , Ira Wasserman , Mark Wyman

I report on recent numerical simulations of the simplest field theory with cosmic string solutions, the Abelian Higgs model. We find that random networks of string quickly converge to a scaling solution in which the network scale length…

高能物理 - 唯象学 · 物理学 2016-10-26 Mark Hindmarsh

We present the first ever calculation of cosmic microwave background CMB anisotropy power spectra from semilocal cosmic strings, obtained via simulations of a classical field theory. Semilocal strings are a type of non-topological defect…

天体物理学 · 物理学 2009-06-23 Jon Urrestilla , Neil Bevis , Mark Hindmarsh , Martin Kunz , Andrew R. Liddle

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

Cosmic strings, topological defects predicted by high-energy theories, may contribute to the late-time expansion of the Universe, effectively mimicking dynamical dark energy. We investigate four phenomenological extensions of the…

宇宙学与河外天体物理 · 物理学 2026-04-06 Hanyu Cheng , Eleonora Di Valentino , Luca Visinelli

We study cosmic strings in the complex symmetron model, a scalar-tensor theory with a spontaneously broken local $U(1)$ symmetry in low matter density regions. Using numerical simulations, we show that these strings preferentially attach to…

高能物理 - 唯象学 · 物理学 2025-08-19 Ali Nezhadsafavi , Levon Pogosian

We present a toy model for the investigation of the formation of semilocal strings, where a planar symmetry is employed to reduce the system to two dimensions. We approximate the symmetry breaking using an extension of the…

高能物理 - 唯象学 · 物理学 2009-10-30 Ana Achucarro , Julian Borrill , Andrew R Liddle

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 study how the presence of world-sheet currents affects the evolution of cosmic string networks, and their impact on predictions for the cosmic microwave background (CMB) anisotropies generated by these networks. We provide a general…

宇宙学与河外天体物理 · 物理学 2020-10-21 I. Yu. Rybak , A. Avgoustidis , C. J. A. P. Martins

I use a combination of state-of-the-art numerical simulations and analytic modelling to discuss the scaling properties of cosmic defect networks, including superstrings. Particular attention is given to the role of extra degrees of freedom…

高能物理 - 唯象学 · 物理学 2015-06-17 C. J. A. P. Martins

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

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

We present the first complete Markov chain Monte Carlo analysis of cosmological models with evolving cosmic (super)string networks, using the unconnected segment model in the unequal-time correlator formalism. For ordinary cosmic string…

宇宙学与河外天体物理 · 物理学 2016-06-08 Tom Charnock , Anastasios Avgoustidis , Edmund J. Copeland , Adam Moss

Motivated by recent developments in superstring theory in the cosmological context, we examine a field theory which contains string networks with 3-way junctions. We perform numerical simulations of this model, identify the length scales of…

高能物理 - 理论 · 物理学 2009-11-11 Mark Hindmarsh , P. M. Saffin

We use our model of the small scale structure on cosmic strings to develop further the result of Siemens, Olum, and Vilenkin that the gravitational radiation length scale on cosmic strings is smaller than the previously assumed $\Gamma G\mu…

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

We investigate scaling and correlations of the energy and momentum in an evolving network of cosmic strings in Minkowski space. These quantities are of great interest, as they must be understood before accurate predictions for the power…

天体物理学 · 物理学 2009-10-28 Graham R. Vincent , Mark Hindmarsh , Mairi Sakellariadou

We exploit the techniques of dynamical systems to study the cosmological evolution of cosmic fundamental strings and effective strings arising from branes wrapped on internal cycles. We also include the whole potential of the volume modulus…

高能物理 - 理论 · 物理学 2026-04-01 Luca Brunelli , Michele Cicoli , Francisco Gil Pedro

Cosmic strings, a hot subject in the 1980's and early 1990's, lost its appeal when it was found that it leads to inconsistencies in the power spectrum of the measured cosmic microwave background temperature anisotropies. However,…

高能物理 - 理论 · 物理学 2008-11-26 Mairi Sakellariadou