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相关论文: Evolution of cosmic string configurations

200 篇论文

We develop an analytical model to study the production spectrum of loops in the cosmic string network. In the scaling regime, we find two different scales corresponding to large (one order below horizon) and small (few orders below horizon)…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Vitaly Vanchurin

Cosmic strings with degrees of freedom beyond the standard Abrikosov-Nielsen-Olesen or Nambu-Goto strings are ubiquitous in field theory as well as in models with extra dimensions, such as string theoretic brane inflation scenarios. Here we…

高能物理 - 唯象学 · 物理学 2015-06-03 M. F. Oliveira , A. Avgoustidis , C. J. A. P. Martins

We study the spectrum of loops as a part of a complete network of cosmic strings in flat spacetime. After a long transient regime, characterized by production of small loops at the scale of the initial conditions, it appears that a true…

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

We present results from a detailed numerical study of the small-scale and loop production properties of cosmic string networks, based on the largest and highest resolution string simulations to date. We investigate the non-trivial fractal…

天体物理学 · 物理学 2008-11-26 C. J. A. P. Martins , E. P. S. Shellard

We discuss and summarise the predictions of a model for the non-equilibrium evolution of a network of cosmic strings initially containing {\em only loops} and {\em no infinite strings}. The results are of interest given recent work…

高能物理 - 唯象学 · 物理学 2007-05-23 D. A. Steer

We study the production of loops in the cosmic string network in the expanding background by means of a numerical simulation exact in the flat-spacetime limit and first-order in the expansion rate. We find an initial regime characterized by…

天体物理学 · 物理学 2008-11-26 Ken D. Olum , Vitaly Vanchurin

We develop a model of string dynamics with back-reaction from both scaling and non-scaling loops taken into account. The evolution of a string network is described by the distribution functions of coherence segments and kinks. We derive two…

高能物理 - 理论 · 物理学 2010-11-19 Vitaly Vanchurin

Cosmic string loops are non-linear density fluctuations which form in the early universe and could play an important role in explaining many phenomena which are in tension with the standard $\Lambda$CDM model. Hence, the details of the…

宇宙学与河外天体物理 · 物理学 2023-09-11 Hao Jiao , Bryce Cyr , Robert Brandenberger

We present an extension of the velocity-dependent one-scale model for cosmic string evolution, which is suitable for describing the evolution of local and global monopole networks. We discuss the key dynamical features that need to be…

高能物理 - 唯象学 · 物理学 2009-11-13 C. J. A. P. Martins , A. Achucarro

We calculate the gravitational radiation emitted by an infinite cosmic string with two oppositely moving wave-trains, in the small amplitude approximation. After comparing our result to the previously studied cases we extend the results to…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Xavier Siemens , Ken D. Olum

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 obtain the equations of motion for cosmic strings in extensions of the 3+1 FRW model with extra dimensions. From these we derive a generalisation of the Velocity-dependent One-Scale (VOS) model for cosmic string network evolution which…

高能物理 - 唯象学 · 物理学 2009-11-10 A. Avgoustidis , E. P. S. Shellard

We study the impact of fragmentation on the cosmic string loop number density, using an approach inspired by the three-scale model and a Boltzmann equation. We build a new formulation designed to be more amenable to numerical resolution and…

宇宙学与河外天体物理 · 物理学 2025-12-12 Pierre Auclair

Classical lattice simulations of the Abelian Higgs model are used to investigate small scale structure and loop distributions in cosmic string networks. Use of the field theory ensures that the small-scale physics is captured correctly. The…

高能物理 - 理论 · 物理学 2011-06-02 Mark Hindmarsh , Stephanie Stuckey , Neil Bevis

We have studied the cosmological evolution of domain wall networks in two, three and four spatial dimensions using high-resolution field theory simulations. The dynamical range and number of our simulations is larger than in previous works,…

高能物理 - 唯象学 · 物理学 2009-11-10 J. C. R. E. Oliveira , C. J. A. P. Martins , P. P. Avelino

The velocity-dependent `one-scale' model of Martins and Shellard is used to study the evolution of a cosmic string network (and the corresponding loop population) in open universes. It is shown that in this case there is no linear scaling…

天体物理学 · 物理学 2009-10-30 C. J. A. P. Martins

We report on a study of axion string networks using fixed-grid simulations of up to $16384$ points per side. The length of string can be characterised in terms of standard dimensionless parameters $\zeta_\text{w}$ and $\zeta_\text{r}$, the…

高能物理 - 唯象学 · 物理学 2025-01-08 José Correia , Mark Hindmarsh , Joanes Lizarraga , Asier Lopez-Eiguren , Kari Rummukainen , Jon Urrestilla

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 study the evolution of cosmic strings taking into account the frictional force due to the surrounding radiation. We consider small perturbations on straight strings, oscillation of circular loops and small perturbations on circular…

高能物理 - 理论 · 物理学 2009-10-22 J. Garriga , M. Sakellariadou

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