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相关论文: Comment on `Critical scalar field collapse in AdS$…

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In the quest of the critical solution for scalar field collapse in 2+1 gravity with a negative cosmological constant, we present a one parameter family of solutions with continuous self similar (CSS) behaviour near the central singularity.…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Gerard Clement , Alessandro Fabbri

In the context of gravitational collapse and black hole formation, we reconsider the problem to describe analytically the critical collapse of a massless and minimally coupled scalar field in $2+1$ gravity.

广义相对论与量子宇宙学 · 物理学 2014-10-14 G. Clement , A. Fabbri

We report a new critical solution found at the threshold of axisymmetric gravitational collapse of a complex scalar field with angular momentum. To carry angular momentum the scalar field cannot be axisymmetric; however, its azimuthal…

广义相对论与量子宇宙学 · 物理学 2009-11-10 M. W. Choptuik , E. W. Hirschmann , S. L. Liebling , F. Pretorius

We present an analytical solution of a massless scalar field collapsing in a three dimensional space-time with a negative cosmological constant, i.e. asymptotically AdS_3. The Einstein and scalar field equations are formulated using double…

广义相对论与量子宇宙学 · 物理学 2015-06-17 Rudolf Baier , Stefan Stricker , Olli Taanila

We present a family of exact solutions, depending on two parameters $\alpha$ and $b$ (related to the scalar field strength), to the three-dimensional Einstein-scalar field equations with negative cosmological constant $\Lambda$. For $b=0$…

广义相对论与量子宇宙学 · 物理学 2016-02-25 Gérard Clément , Alessandro Fabbri

We consider the problem of critical gravitational collapse of a scalar field in 2+1 dimensions with spherical (circular) symmetry. After surveying all the analytic, continuously self-similar solutions and considering their global structure,…

广义相对论与量子宇宙学 · 物理学 2009-07-07 Eric W. Hirschmann , Anzhong Wang , Yumei Wu

We present results from the first study of critical behavior in 3-d gravitational collapse. The source of the gravitational field is a massless scalar field. This is a well-studied case for spherically symmetric gravitational collapse,…

广义相对论与量子宇宙学 · 物理学 2019-01-16 Nils Deppe , Lawrence E. Kidder , Mark A. Scheel , Saul A. Teukolsky

We study the spherically symmetric collapse of a scalar field in anti-de Sitter spacetime using a newly constructed, open-source code which parallelizes over heterogeneous architectures using the open standard OpenCL. An open question for…

广义相对论与量子宇宙学 · 物理学 2017-10-03 Steven L. Liebling , Gaurav Khanna

We study the dynamics of the critical collapse of a spherically symmetric scalar field. Approximate analytic expressions for the metric functions and matter field in the large-radius region are obtained. In the central region, owing to the…

广义相对论与量子宇宙学 · 物理学 2024-05-13 Jun-Qi Guo , Yu Hu , Pan-Pan Wang , Cheng-Gang Shao

We construct a one-parameter family of exact time-dependent solutions to 2+1 gravity with a negative cosmological constant and a massless minimally coupled scalar field as source. These solutions present a continuously self-similar (CSS)…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Gerard Clement , Alessandro Fabbri

We investigate non-spherically symmetric, scalar field collapse of a family of initial data consisting of a spherically symmetric profile with a deformation proportional to the real part of the spherical harmonic $Y_{21}(\theta,\varphi)$.…

广义相对论与量子宇宙学 · 物理学 2014-03-31 James Healy , Pablo Laguna

Critical collapse of a massless scalar field in spherical symmetry is systematically studied. We combine numerical simulations and asymptotic analysis, and synthesize critical collapse, spacetime singularities, and complex science. First…

广义相对论与量子宇宙学 · 物理学 2019-07-30 Jun-Qi Guo , Hongsheng Zhang

We describe results of a numerical calculation of circularly symmetric scalar field collapse in three spacetime dimensions with negative cosmological constant. The procedure uses a double null formulation of the Einstein-scalar equations.…

广义相对论与量子宇宙学 · 物理学 2010-04-06 Viqar Husain , Michel Olivier

We comment on Z. D. Zhang's Response [arXiv:0812.2330] to our recent Comment [arXiv:0811.3876] addressing the conjectured solution of the three-dimensional Ising model reported in [arXiv:0705.1045].

统计力学 · 物理学 2009-11-13 F. Y. Wu , B. M. McCoy , M. E. Fisher , L. Chayes

Critical phenomena in gravitational collapse exhibit the universal features of self-similarity, critical scaling, and the appearance of a naked singularity. We study critical collapse in AdS, focusing on holographic field theory…

高能物理 - 理论 · 物理学 2019-07-12 Paul M. Chesler , Benson Way

We examine the gravitational collapse of a non-linear sigma model in spherical symmetry. There exists a family of continuously self-similar solutions parameterized by the coupling constant of the theory. These solutions are calculated…

广义相对论与量子宇宙学 · 物理学 2011-09-09 Eric W. Hirschmann , Douglas M. Eardley

We perform numerical simulations of the critical gravitational collapse of a massive vector field. The result is that there are two critical solutions. One is equivalent to the Choptuik critical solution for a massless scalar field. The…

广义相对论与量子宇宙学 · 物理学 2009-11-10 David Garfinkle , Robert Mann , Chris Vuille

We present results from a numerical study of critical gravitational collapse of axisymmetric distributions of massless scalar field energy. We find threshold behavior that can be described by the spherically symmetric critical solution with…

广义相对论与量子宇宙学 · 物理学 2009-11-10 M. W. Choptuik , E. W. Hirschmann , S. L. Liebling , F. Pretorius

This paper studies near-critical evolution of the spherically symmetric scalar field configurations close to the continuously self-similar solution. Using analytic perturbative methods, it is shown that a generic growing perturbation…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Andrei V. Frolov

We report on a new behavior found in numerical simulations of spherically symmetric gravitational collapse in self-gravitating SU(2) sigma models at intermediate gravitational coupling constants: The critical solution (between black hole…

广义相对论与量子宇宙学 · 物理学 2007-05-23 J. Thornburg , Ch. Lechner , M. Purrer , P. C. Aichelburg , S. Husa
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