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相关论文: Cosmic String Cusps with Small-Scale Structure: Th…

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We analyze the shapes of cosmic string loops found in large-scale simulations of an expanding-universe string network. The simulation does not include gravitational back reaction, but we model that process by smoothing the loop using…

宇宙学与河外天体物理 · 物理学 2015-09-30 Jose J. Blanco-Pillado , Ken D. Olum , Benjamin Shlaer

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

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

We present the results of computational gravitational backreaction on simple models of cosmic string loops. These results give us insight into the general behavior of cusps and kinks on loops, in addition to other features of evolution.…

广义相对论与量子宇宙学 · 物理学 2019-07-29 Jose J. Blanco-Pillado , Ken D. Olum , Jeremy M. Wachter

We extend our earlier model of the small scale structure of cosmic string networks through an improved treatment of the separation of long and short scales. We find that the production of small loops (at the gravitational radiation scale)…

天体物理学 · 物理学 2008-11-26 Florian Dubath , Joseph Polchinski , Jorge V. Rocha

We present an analytic model specifically designed to address the long standing issue of small scale structure on cosmic string networks. The model is derived from the microscopic string equations, together with a few motivated assumptions.…

广义相对论与量子宇宙学 · 物理学 2008-12-23 Jorge V. Rocha

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 analyze the effect of gravitational back reaction on cosmic string loops with kinks, which is an important determinant of the shape, and thus the potential observability, of string loops which may exist in the universe today. Kinks are…

广义相对论与量子宇宙学 · 物理学 2018-08-31 Jeremy M. Wachter , Ken D. Olum

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 consider an alternative approach for the computation of the stochastic gravitational wave background generated by small loops produced throughout the cosmological evolution of cosmic string networks and use it to derive an analytical…

宇宙学与河外天体物理 · 物理学 2016-10-05 L. Sousa , P. P. Avelino

We obtain general formulae for the plus- and cross- polarized waveforms of gravitational radiation emitted by a cosmic string loop in transverse, traceless (synchronous, harmonic) gauge. These equations are then specialized to the case of…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Bruce Allen , Adrian C. Ottewill

We classify the possible shapes of cosmic string cusps and how they transform under Lorentz boosts. A generic cusp can be brought into a form in which the motion of the cusp tip lies in the plane of the cusp. The cusp whose motion is…

广义相对论与量子宇宙学 · 物理学 2021-01-06 J. J. Blanco-Pillado , Ken D. Olum

If cosmic strings are formed in the early universe, their associated loops emit gravitational waves during the whole cosmic history and contribute to the stochastic gravitational wave background at all frequencies. We provide a new estimate…

宇宙学与河外天体物理 · 物理学 2018-01-15 Christophe Ringeval , Teruaki Suyama

We explore the kinematical effect of having extra dimensions on the gravity wave emission from cosmic strings. Additional dimensions both round off cusps, and reduce the probability of their formation. We recompute the gravity wave burst,…

高能物理 - 理论 · 物理学 2014-11-21 Eimear O'Callaghan , Sarah Chadburn , Ghazal Geshnizjani , Ruth Gregory , Ivonne Zavala

Numerical simulations and analytical models suggest that infinite cosmic strings produce cosmic string loops of all sizes with a given power-law. Precise estimations of the power-law exponent are still matter of debate while numerical…

宇宙学与河外天体物理 · 物理学 2020-11-26 Pierre G. Auclair

Complicated cosmic string loops will fragment until they reach simple, non-intersecting ("stable") configurations. Through extensive numerical study we characterize these attractor loop shapes including their length, velocity, kink, and…

高能物理 - 理论 · 物理学 2015-03-17 Craig J Copi , Tanmay Vachaspati

The formation of cusps on long cosmic strings is discussed and the probability of cusp formation is estimated. The energy distribution of the gamma-ray background due to cusp annihilation on long strings is calculated and compared to…

高能物理 - 唯象学 · 物理学 2009-10-22 M. Mohazzab , R. H. Brandenberger

The mean spectrum and burst statistics of gravitational waves produced by a cosmological population of cosmic string loops are estimated using analytic approximations, calibrated with earlier simulations. Formulas are derived showing the…

天体物理学 · 物理学 2009-11-11 Craig J. Hogan

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 investigate the contribution made by small loops from a cosmic string network as seeds for large-scale structure formation. We show that cosmic string loops are highly correlated with the long-string network on large scales and therefore…

天体物理学 · 物理学 2008-11-26 P. P. Avelino , E. P. S. Shellard , J. H. P. Wu , B. Allen
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