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相关论文: Limits on Black Hole Formation from Cosmic String …

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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

Primordial Black Holes (PBH) may have formed from the collapse of cosmic string loops. The spectral shape of the PBH mass spectrum can be determined by the scaling argument for string networks. Limits on the spectral amplitude derived from…

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

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

Hawking has shown that the emission of gravitational radiation cannot prevent circular loops of gauged cosmic strings from collapsing into black holes. Here we consider the corresponding question for global strings: can Goldstone boson…

高能物理 - 理论 · 物理学 2009-10-22 Joaquim Fort , Tanmay Vachaspati

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

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 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 evaluate the probability that a loop of string that has spontaneously nucleated during inflation will form a black hole upon collapse, after the end of inflation. We then use the observational bounds on the density of primordial black…

高能物理 - 唯象学 · 物理学 2009-10-22 Jaume Garriga , Alexander Vilenkin

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

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

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

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

Black holes can be produced in collapse of small-scale dark matter structures, which can happen at any time from the early to present-day universe. Microstructure black holes (MSBHs) can have a wide range of masses. Small MSBHs evaporate…

宇宙学与河外天体物理 · 物理学 2023-09-06 Zachary S. C. Picker , Alexander Kusenko

We review recent progress in our understanding of the physics of black holes. In particular, we discuss the ideas from string theory that explain the entropy of black holes from a counting of microstates of the hole, and the related…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Sumit R. Das , Samir D. Mathur

Primordial black holes may form in the early Universe, for example from the collapse of large amplitude density perturbations predicted in some inflationary models. Light black holes undergo Hawking evaporation, the energy injection from…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Andrew R Liddle , Anne M Green

Black holes are extreme outcomes of General Relativity, and can form through a variety of ways, including gravitational collapse of massive stars, or quantum fluctuations in the early universe. Here, we ask the question of whether they can…

广义相对论与量子宇宙学 · 物理学 2025-02-04 Diego Blas , Vitor Cardoso , Jose María Ezquiaga

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

We consider the possibility of formation of cosmic strings with black holes as beads. We focus on the simplest setup where two black holes are formed on a long cosmic string. It turns out the in absence of a background magnetic field and…

高能物理 - 理论 · 物理学 2014-11-06 Amjad Ashoorioon , Robert B. Mann

We give an elementary review of black holes in string theory. We discuss black hole entropy from string microstates and Hawking radiation from these states. We then review the structure of 2-charge microstates, and explore how…

高能物理 - 理论 · 物理学 2009-11-11 Samir D. Mathur
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