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相关论文: Formation of Cosmic String network from black hole…

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The Pulsar timing data from NANOGrav Collaboration has regenerated interest in the possibility of observing stochastic gravitational wave background arising from cosmic strings. In the standard theory, the cosmic string network forms during…

广义相对论与量子宇宙学 · 物理学 2024-05-08 Ajit M. Srivastava

Cosmic strings and primordial black holes (PBHs) commonly and naturally form in many scenarios describing the early universe. Here we show that if both cosmic strings and PBHs are present, their interaction leads to a range of interesting…

宇宙学与河外天体物理 · 物理学 2018-11-14 Alexander Vilenkin , Yuri Levin , Andrei Gruzinov

Recent discoveries of super-massive black holes at high redshifts indicate a possible tension with the standard Lambda CDM paradigm of early universe cosmology which has difficulties in explaining the origin of the required nonlinear…

宇宙学与河外天体物理 · 物理学 2015-07-24 Sebastian F. Bramberger , Robert H. Brandenberger , Paul Jreidini , Jerome Quintin

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

We describe a new mechanism, whose ingredients are realised in string compactifications, for the formation of cosmic (super)string networks. Oscillating string loops grow when their tension $\mu$ decreases with time. If $2H + \dot{\mu}/\mu…

高能物理 - 唯象学 · 物理学 2024-06-19 Joseph P. Conlon , Edmund J. Copeland , Edward Hardy , Noelia Sánchez González

We study the formation of cosmic strings by confining a stochastic magnetic field into flux tubes in a numerical simulation. We use overdamped evolution in a potential that is minimized when the flux through each face in the simulation…

高能物理 - 理论 · 物理学 2008-11-26 Jose J. Blanco-Pillado , Ken D. Olum , Alexander Vilenkin

Cosmic strings can be created in the early universe during symmetry-breaking phase transitions, such as might arise if the gauge structure of the standard model is extended by additional U(1) factors at high energies. Cosmic strings present…

高能物理 - 唯象学 · 物理学 2009-10-29 Yanou Cui , David E. Morrissey

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

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

Large-scale coherent magnetic fields are observed in galaxies and clusters, but their ultimate origin remains a mystery. We reconsider the prospects for primordial magnetogenesis by a cosmic string network. We show that the magnetic flux…

天体物理学 · 物理学 2008-11-26 Diana Battefeld , Thorsten Battefeld , Daniel H. Wesley , Mark Wyman

We study the deformation of a long cosmic string by a nearby rotating black hole. We examine whether the deformation of a cosmic string, induced by the gravitational field of a Kerr black hole, may lead to the formation of a loop of cosmic…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Florian Dubath , Mairi Sakellariadou , Claude Michel Viallet

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

The existence of a scaling evolution for cosmic string loops in an expanding universe is demonstrated for the first time by means of numerical simulations. In contrast with what is usually assumed, this result does not rely on any…

天体物理学 · 物理学 2009-11-13 Christophe Ringeval , Mairi Sakellariadou , Francois Bouchet

Primordial black hole formation by cosmic string collapse is reconsidered when the winding number of the string is larger than the unity. The line energy density of the multiple winding string becomes greater than that of the single winding…

天体物理学 · 物理学 2007-05-23 Nagasawa Michiyasu

In this paper the collision of two cosmic string loops is studied. After collision junctions are formed and the loops are entangled. We show that after their formation the junctions start to unzip and the loops disentangle. This analysis…

高能物理 - 理论 · 物理学 2009-11-06 Hassan Firouzjahi , Johanna Karouby , Shahram Khosravi , Robert Brandenberger

We develop the general formalism for joining, splitting and interconnection of closed and open strings. As an application, we study examples of fundamental cosmic string collisions leading to gravitational collapse. We find that the…

高能物理 - 理论 · 物理学 2009-11-11 R. Iengo , J. Russo

Cosmic strings are topological defects which can be formed as a result of phase transitions with a spontaneous symmetry breaking in the early Universe. The possibility of the generation of a magnetic field around a cosmic string on the…

宇宙学与河外天体物理 · 物理学 2013-05-02 L. V. Zadorozhna , B. I. Hnatyk , Yu. A. Sitenko

Cosmic strings are stable topological defects that may have been created at a phase transition in the early universe. It is a growing belief that, for a wide range of theoretical models, such strings may be superconducting and carry…

高能物理 - 唯象学 · 物理学 2010-11-19 Konstantinos Dimopoulos

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 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
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