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相关论文: Do Global String Loops Collapse to Form Black Hole…

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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

We present the first fully general relativistic dynamical simulations of Abelian Higgs cosmic strings using 3+1D numerical relativity. Focusing on cosmic string loops, we show that they collapse due to their tension and can either (i)…

广义相对论与量子宇宙学 · 物理学 2019-05-22 Thomas Helfer , Josu C. Aurrekoetxea , Eugene A. Lim

In this paper, we study the equation of circular loops with time-dependant tension in the BTZ black hole background. We obtain various cases where cosmic string loops finally collapse to form black holes. Also, we study effect of the BTZ…

高能物理 - 理论 · 物理学 2011-08-24 J. Sadeghi , H. M. Farahani , B. Pourhassan , S. M. Noorbakhsh

The fraction of cosmic string loops which collapse to form black holes is estimated using a set of realistic loops generated by loop fragmentation. The smallest radius sphere into which each cosmic string loop may fit is obtained by…

广义相对论与量子宇宙学 · 物理学 2009-10-28 R. R. Caldwell , Paul Casper

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

Recent work by Jenkins and Sakellariadou claims that cusps on cosmic strings lead to black hole production. To derive this conclusion they use the hoop conjecture in the rest frame of the string loop, rather than in the rest frame of the…

宇宙学与河外天体物理 · 物理学 2021-01-14 Jose J. Blanco-Pillado , Ken D. Olum , Alexander Vilenkin

In this work the equation of circular loops of cosmic string possessing time-dependent tension is studied in the de Sitter spacetime. We find that the cosmic string loops with initial radius $r(t_{0})>0.707L$, L de Sitter radius, should not…

高能物理 - 理论 · 物理学 2009-03-24 Yunqi Liu , Hongbo Cheng

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

The equation of circular loops of cosmic string with time-dependent tension is studied in the Minkowski spacetime and Robertson-Walker universe. We find that, in the case where the tension depends on some power of the cosmic time, cosmic…

高能物理 - 理论 · 物理学 2008-12-25 Hongbo Cheng , Yunqi Liu

The leading classical low-energy effective actions for two-dimensional string theories have solutions describing the gravitational collapse of shells of matter into a black hole. It is shown that string loop corrections can be made…

高能物理 - 理论 · 物理学 2009-11-10 Joanna L. Karczmarek , Juan Maldacena , Andrew Strominger

The cosmological features of primordial black holes formed from collapsed cosmic string loops are studied. Observational restrictions on a population of primordial black holes are used to restrict $f$, the fraction of cosmic string loops…

高能物理 - 唯象学 · 物理学 2008-11-26 R. R. Caldwell , E. Gates

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

In a recent essay, we discussed the possibility of using polymer sizing to model the collapse of a single, long excited string to a black hole. In this letter, we apply this idea to bring further support to string/black hole correspondence.…

高能物理 - 理论 · 物理学 2009-10-31 Ramzi R. Khuri

It is conventionally believed that if a ball of matter of mass $M$ has a radius close to $2GM$ then it must collapse to a black hole. But string theory microstates (fuzzballs) have no horizon or singularity, and they do {\it not} collapse.…

高能物理 - 理论 · 物理学 2016-11-15 Samir D. Mathur

A small fraction, $f$, of cosmic string loops can collapse to form Primordial Black Holes (PBHs). Constraints on the abundance of PBHs can therefore be used to constrain $f$. We update these calculations, taking into account the PBH…

宇宙学与河外天体物理 · 物理学 2020-07-01 Chloe James-Turner , Danton P. B. Weil , Anne M. Green , Edmund J. Copeland

We examine the question of collapse of Turok's two-parameter family of cosmic strings. We first perform a classification of the strings according to the specific time(s) at which the minimal string size is reached during one period. We then…

广义相对论与量子宇宙学 · 物理学 2016-12-28 R. N. Hansen , M. Christensen , A. L. Larsen

In this paper the equation of circular loops of cosmic string with periodic tension is investigated in the Minkowski spacetime and Robertson-Walker universe respectively. We find that the cosmic string loops possessing this kind of…

高能物理 - 理论 · 物理学 2015-06-05 Leilin Wang , Hongbo Cheng

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

This paper discusses the gravitational scattering of a straight, infinitely long test cosmic string by a black hole. We present numerical results that probe the two-dimensional parameter space of impact parameter and initial velocity and…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Jean-Pierre De Villiers , Valeri Frolov

This paper puts forward a conjecture that there are no black holes in M theory. We will show that a mechanism to prevent black hole formation is needed in 4 dimensions to make string theory a viable high energy model of quantum gravity.…

高能物理 - 理论 · 物理学 2016-06-07 Michael Hewitt
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