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相关论文: High Harmonic Configurations of Cosmic Strings: An…

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The collisions of cosmic strings loops and the dynamics of junctions formations in expanding backgrounds are studied. The key parameter controlling the dynamics of junctions formation, the cosmic strings zipping and unzipping is the…

高能物理 - 理论 · 物理学 2015-03-13 Hassan Firouzjahi , Salomeh Khoeini-Moghaddam , Shahram Khosravi

Low-harmonic formulas for closed relativistic strings are given. General parametrizations are presented for the addition of second- and third-harmonic waves to the fundamental wave. The method of determination of the parametrizations is…

高能物理 - 理论 · 物理学 2010-11-01 R. W. Brown , M. E. Convery , S. A. Hotes , M. G. Knepley , L. S. Petropoulos

Based on a binary tree model for the self intersection of cosmic string loops containing high harmonics we estimate the number of self-intersections of the parent and daughter loops and the associated cusp production to determine the most…

宇宙学与河外天体物理 · 物理学 2021-12-15 Despoina Pazouli , Konstantinos Palapanidis , Anastasios Avgoustidis , Edmund J. Copeland

Cosmic strings are linear concentrations of energy that form whenever phase transitions in the early universe break axial symmetries as originally shown by Kibble. They are the result of frustrated order in the quantum fields responsible…

天体物理学 · 物理学 2008-11-11 A. Achucarro , 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

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

A new candidate source of gravitational radiation is described: the nearly-perfect harmonic series from individual loops of cosmic string. It is argued that theories with light cosmic strings give rise to a population of numerous long-lived…

宇宙学与河外天体物理 · 物理学 2009-08-02 Matthew R DePies , Craig J Hogan

We argue that cosmic strings with high winding numbers generally form in first-order gauge symmetry breaking phase transitions, and we demonstrate this using computer simulations. These strings are heavier than single-winding strings and…

高能物理 - 唯象学 · 物理学 2007-05-23 M. Donaire , A. Rajantie

The topic of cosmic strings provides a bridge between the physics of the very small and the very large. They are predicted by some unified theories of particle interactions. If they exist, they may help to explain some of the largest-scale…

高能物理 - 唯象学 · 物理学 2010-11-01 M. B. Hindmarsh , T. W. B. Kibble

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

In this thesis we describe high-harmonic cosmic string loops in a general relativistic context, and study the implications of high-harmonic content for the predicted gravitational wave signal from cosmic string networks. Initially, we…

广义相对论与量子宇宙学 · 物理学 2021-08-19 Despoina Pazouli

In determining the gravitational signal of cusps from a network of cosmic strings loops, a number of key parameters have to be assumed. These include the typical number of cusps per period of string oscillation and the typical values of the…

高能物理 - 理论 · 物理学 2021-04-07 Despoina Pazouli , Anastasios Avgoustidis , Edmund J. Copeland

Cosmic strings are one-dimensional topological defects which could have been formed in the early stages of our Universe. They triggered a lot of interest, mainly for their cosmological implications: they could offer an alternative to…

高能物理 - 理论 · 物理学 2009-11-11 Mairi Sakellariadou

In theories with cosmic strings, a small fraction of string loops may collapse to form black holes. In this Letter, various constraints on such models involving black holes are considered. Hawking radiation from black holes, gamma and…

天体物理学 · 物理学 2009-10-30 Jane H. MacGibbon , Robert H. Brandenberger , U. F. Wichoski

Whilst standard field theoretic Cosmic Strings cannot end, Cosmic Superstrings can form three string junctions, at which each string ends. This opens up a new class of possible boundary conditions for such strings and we show that, at least…

广义相对论与量子宇宙学 · 物理学 2014-11-20 William Nelson

We develop methods by which cosmic superstring interactions can be studied in detail. These include the reconnection probability and emission of radiation such as gravitons or small string loops. Loop corrections to these are discussed, as…

高能物理 - 理论 · 物理学 2009-11-18 Mark G. Jackson

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

Cosmic strings are predicted by many field-theory models, and may have been formed at a symmetry-breaking transition early in the history of the universe, such as that associated with grand unification. They could have important…

高能物理 - 理论 · 物理学 2010-05-07 Edmund J. Copeland , T. W. B. Kibble

The time-dependent metric of a cosmic string leads to an effective interaction between the string and photons - the "gravitational Aharonov-Bohm" effect -- and causes cosmic strings to emit light. We evaluate the radiation of pairs of…

高能物理 - 理论 · 物理学 2011-03-23 Daniele A. Steer , Tanmay Vachaspati

Cosmic superstring loops generically contain strings of different tensions that meet at Y-junctions. These loops evolve non-periodically in time, and have cusps and kinks that interact with the junctions. We study the effect of junctions on…

高能物理 - 理论 · 物理学 2009-12-30 P. Binetruy , A. Bohe , T. Hertog , D. A. Steer
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