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相关论文: Cosmic Strings are Current-Carrying

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We investigate the standard model in a cosmic string background and show that the electroweak symmetry is partially restored. For a range of parameters the electroweak Higgs field can wind in this region, producing an electroweak string…

高能物理 - 唯象学 · 物理学 2009-10-28 Anne-Christine Davis , Warren B. Perkins

We show that stable local cosmic strings are a generic prediction of supersymmetric models where supersymmetry is broken at scales within a few orders of magnitude of the weak scale and is fed down to the observable sector by gauge…

高能物理 - 唯象学 · 物理学 2009-10-30 Antonio Riotto

Cosmic strings are predicted by many Standard Model extensions involving the cosmological breaking of a symmetry with nontrivial first homotopy group and represent a potential source of primordial gravitational waves (GWs). Present efforts…

宇宙学与河外天体物理 · 物理学 2023-04-07 Pierre Auclair , Simone Blasi , Vedran Brdar , Kai Schmitz

We investigate the cosmological consequences of particle physics theories that admit stable loops of superconducting cosmic string - {\it vortons}. General symmetry breaking schemes are considered, in which strings are formed at one energy…

高能物理 - 唯象学 · 物理学 2009-10-28 R. Brandenberger , B. Carter , A. -C. Davis , M. Trodden

We consider the cosmological consequences of a network of superconducting cosmic strings. For strong enough current the period of friction domination never ends. Instead a plasma scaling solution is reached. We demonstrate that this gives…

高能物理 - 唯象学 · 物理学 2009-10-31 K. Dimopoulos , A. C. Davis

It has been speculated that cosmic string networks could produce ultra-high energy cosmic rays as a by-product of their evolution. By making use of recent work on the evolution of such networks, it will be shown that the flux of cosmic rays…

高能物理 - 唯象学 · 物理学 2014-11-17 A. J. Gill , T. W. B. Kibble

Many symmetry breaking patterns in grand unified theories (GUTs) give rise to cosmic strings that eventually decay when pairs of GUT monopoles spontaneously nucleate along the string cores. These strings are known as metastable cosmic…

高能物理 - 唯象学 · 物理学 2024-01-23 Wilfried Buchmuller , Valerie Domcke , Kai Schmitz

The lensing properties of superconducting cosmic strings endowed with a time dependent pulse of lightlike current are investigated. The metric outside the core of the string belongs to the $pp$--wave class, with a deficit angle. We study…

广义相对论与量子宇宙学 · 物理学 2010-04-06 Jaume Garriga , Patrick Peter

The dynamical evolution of superconducting cosmic string loops with specific equations of state describing timelike and spacelike currents is studied numerically. This analysis extends previous work in two directions: first it shows results…

高能物理 - 唯象学 · 物理学 2009-11-07 Adriana Cordero-Cid , Xavier Martin , Patrick Peter

We investigate the stability of the electroweak Z-string at high temperatures. Our results show that while finite temperature corrections can improve the stability of the Z-string, their effect is not strong enough to stabilize the Z-string…

高能物理 - 唯象学 · 物理学 2011-07-19 R. Holman , S. D. H. Hsu , T. Vachaspati , R. Watkins

We consider the evolution of current-carrying cosmic string networks described by the charge-velocity-dependent one scale (CVOS) model beyond the linear equation of state regime, specifically focusing on the Witten superconducting model. We…

宇宙学与河外天体物理 · 物理学 2023-06-28 I. Yu. Rybak , C. J. A. P. Martins , Patrick Peter , E. P. S. Shellard

It is shown that in models including the standard electroweak theory and for some particular values of the underlying parameters, electric currents can be spontaneously generated in cosmic strings, without the need of any external field…

高能物理 - 唯象学 · 物理学 2010-11-01 Patrick PETER

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

It has been suggested that cosmological dark matter may include a population of vortons (meaning small centrifugally stabilised cosmic string loops) as an outcome of (non-standard) electroweak symmetry breaking. The implications for this…

高能物理 - 唯象学 · 物理学 2007-05-23 B. Carter

Cosmic strings are linear concentrations of energy that may be formed at phase transitions in the very early universe. At one time they were thought to provide a possible origin for the density inhomogeneities from which galaxies eventually…

高能物理 - 理论 · 物理学 2009-11-11 A. -C. Davis , T. W. B. Kibble

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 idea of GUT implies that the universe went through a series of phase transitions during which topological defects are expected to form. We investigate here the genericity of cosmic strings formation in realistic SUSY GUTs models. We…

高能物理 - 唯象学 · 物理学 2007-05-23 J. Rocher , R. Jeannerot , M. Sakellariadou

Classical solutions describing strings endowed with an electric charge and carrying a constant electromagnetic current are constructed within the bosonic sector of the Electroweak Theory. For any given ratio of the Higgs boson mass to W…

高能物理 - 理论 · 物理学 2008-11-26 Mikhail S. Volkov

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 string networks are expected to form in early Universe phase transitions via the Kibble mechanism and are unavoidable in several Beyond the Standard Model theories. While most predictions of observational signals of string networks…

高能物理 - 唯象学 · 物理学 2024-06-07 J. R. C. C. C. Correia , C. J. A. P. Martins , F. C. N. Q. Pimenta
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