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相关论文: Correlations in Cosmic String Networks

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Cosmic strings are topological defects possibly formed in the early Universe, which may be observable due to their gravitational effects on the cosmic microwave background radiation or gravitational wave experiments. To this effect it is…

宇宙学与河外天体物理 · 物理学 2017-03-01 R. P. L. Azevedo , C. J. A. P. Martins

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 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

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

Cosmic (super)strings offer promising ways to test ideas about the early universe and physics at high energies. While in field theory constructions their tension is usually assumed to be constant (or at most slowly-varying), this is often…

高能物理 - 唯象学 · 物理学 2025-05-08 Filippo Revello , Gonzalo Villa

We solve numerically the Boltzmann equation describing the evolution of a cosmic string network which contains only loops. In Minkowski space time the equilibrium solution predicted by statistical mechanics is recovered, and we prove that…

天体物理学 · 物理学 2009-10-31 Joao Magueijo , Haavard Sandvik , Daniele Steer

Appearance of cosmic strings in the early Universe is a common manifestation of new physics typically linked to some high energy scale. In this paper, we discuss a different situation, where a model underlying cosmic string formation is…

高能物理 - 唯象学 · 物理学 2022-02-02 William T. Emond , Sabir Ramazanov , Rome Samanta

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 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

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 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

Chiral cosmic strings are produced naturally at the end of inflation in supersymmetric models where the symmetry is broken via a D-term. Consequently in such theories, where both inflation and cosmic strings contribute to the density and…

天体物理学 · 物理学 2009-10-31 A. C. Davis , T. W. B. Kibble , M. Pickles , D. A. Steer

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 study the behaviour of a non-relativistic quantum particle interacting with different potentials, in the background spacetime generated by a cosmic string. We find the energy spectra for the quantum systems under consideration and…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Geusa de A. Marques , V. B. Bezerra

We derive analytic expressions for the interaction energy between two general $U(1)$ cosmic strings as the function of their relative orientation and the ratio of the coupling constants in the model. The results are relevant to the…

高能物理 - 唯象学 · 物理学 2009-10-28 L. M. A. Bettencourt , R. J. Rivers

We discuss some hitherto puzzling features of the small-scale structure of cosmic strings. We argue that kinks play a key role, and that an important quantity to study is their sharpness distribution. In particular we suggest that for very…

宇宙学与河外天体物理 · 物理学 2009-12-31 E. J. Copeland , T. W. B. Kibble

We investigate cosmological evolution and implications of cosmic strings with time-dependent tension. We derive basic equations of time development of the correlation length and the velocity of such strings, based on the one scale model.…

高能物理 - 唯象学 · 物理学 2008-11-26 Kazuhide Ichikawa , Tomo Takahashi , Masahide Yamaguchi

We consider F-strings with arbitrary configurations in the Minkowski directions of a higher-dimensional spacetime, which also wrap and spin around $S^1$ subcycles of constant radius in an arbitrary internal manifold, and determine the…

高能物理 - 唯象学 · 物理学 2015-09-29 Daisuke Yamauchi , Matthew J. Lake

We study the behaviour and consequences of cosmic string networks in contracting universes. They approximately behave during the collapse phase as a radiation fluids. Scaling solutions describing this are derived and tested against…

天体物理学 · 物理学 2015-06-24 P. P. Avelino , C. J. A. P. Martins , C. Santos , E. P. S. Shellard

In the context of a cosmological string model describing the propagation of strings in a time-dependent Robertson-Walker background space-time, we show that the asymptotic acceleration of the Universe can be identified with the square of…

高能物理 - 理论 · 物理学 2009-09-11 John Ellis , N. E. Mavromatos , D. V. Nanopoulos
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