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相关论文: Charged Stringy Black Holes With Non-Abelian Hair

200 篇论文

Static spherically symmetric asymptotically flat particle-like and black hole solutions are constructed within the SU(2) sector of 4-dimensional heterotic string effective action. They separate topologically distinct Yang-Mills vacua and…

高能物理 - 理论 · 物理学 2010-11-19 E. E. Donets , D. V. Gal'Tsov

We construct finite mass, asymptotically flat black hole solutions in d=4 Einstein-Yang-Mills theory augmented with higher order curvature terms of the gauge field. They possess non-Abelian hair in addition to Coulomb electric charge, and,…

广义相对论与量子宇宙学 · 物理学 2013-05-30 Eugen Radu , D. H. Tchrakian

We construct rotating hairy black holes in SU(2) Einstein-Yang-Mills theory. These stationary axially symmetric black holes are asymptotically flat. They possess non-trivial non-Abelian gauge fields outside their regular event horizon, and…

广义相对论与量子宇宙学 · 物理学 2009-11-07 B. Kleihaus , J. Kunz , F. Navarro-Lerida

We construct static axially symmetric black holes in SU(2) Einstein-Yang-Mills-Higgs theory. Located in between a monopole-antimonopole pair, these black holes possess magnetic dipole hair. The difference of their mass and their horizon…

高能物理 - 理论 · 物理学 2009-10-31 B. Kleihaus , J. Kunz

We consider stationary rotating black holes in SU(2) Einstein-Yang-Mills theory, coupled to a dilaton. The black holes possess non-trivial non-Abelian electric and magnetic fields outside their regular event horizon. While generic solutions…

广义相对论与量子宇宙学 · 物理学 2009-11-10 B. Kleihaus , J. Kunz , F. Navarro-Lerida

We here review asymptotically flat rotating black holes in the presence of non-Abelian gauge fields. Like their static counterparts these black holes are no longer uniquely determined by their global charges. In the case of pure SU(2)…

高能物理 - 理论 · 物理学 2016-12-07 Burkhard Kleihaus , Jutta Kunz , Francisco Navarro-Lerida

In the light of the "no-hair" conjecture, we revisit stable black holes in su(N) Einstein-Yang-Mills theory with a negative cosmological constant. These black holes are endowed with copious amounts of gauge field hair, and we address the…

广义相对论与量子宇宙学 · 物理学 2015-06-04 Ben L. Shepherd , Elizabeth Winstanley

We construct charged soliton solutions around spherical charged black holes with no angular momentum in asymptotically flat spacetime. These solutions are non-linear generalizations of charged scalar clouds, dubbed Q-ball hair or Q-clouds,…

广义相对论与量子宇宙学 · 物理学 2020-03-18 Jeong-Pyong Hong , Motoo Suzuki , Masaki Yamada

We review the properties of static, higher dimensional black hole solutions in theories where non-abelian gauge fields are minimally coupled to gravity. It is shown that black holes with hyperspherically symmetric horizon topology do not…

广义相对论与量子宇宙学 · 物理学 2009-07-24 Betti Hartmann

An exact hairy asymptotically locally AdS black hole solution with a flat horizon in the Einstein-nonlinear sigma model system in (3+1) dimensions is constructed. The ansatz for the nonlinear $SU(2)$ field is regular everywhere and depends…

广义相对论与量子宇宙学 · 物理学 2017-12-08 Marco Astorino , Fabrizio Canfora , Alex Giacomini , Marcello Ortaggio

An electrically charged black hole solution with scalar hair in four dimensions is presented. The self-interacting scalar field is real and it is minimally coupled to gravity and electromagnetism. The event horizon is a surface of negative…

高能物理 - 理论 · 物理学 2008-11-26 Cristian Martinez , Ricardo Troncoso

Exact static spherically symmetric charged black holes in four dimensions are presented. One of them has only electric charge and another electric and magnetic charges. In these solutions the metric is asymptotically flat, has two horizons,…

广义相对论与量子宇宙学 · 物理学 2009-11-11 E. Kyriakopoulos

We construct stationary black holes in SU(2) Einstein-Yang-Mills theory, which carry angular momentum and electric charge. Possessing non-trivial non-abelian magnetic fields outside their regular event horizon, they represent…

广义相对论与量子宇宙学 · 物理学 2009-10-31 B. Kleihaus , J. Kunz

We construct static, asymptotically flat black hole solutions with scalar hair. They evade the no-hair theorems by having a scalar potential which is not strictly positive. By including an azimuthal winding number in the scalar field…

广义相对论与量子宇宙学 · 物理学 2015-06-16 Burkhard Kleihaus , Jutta Kunz , Eugen Radu , Bintoro Subagyo

In these lectures the properties of magnetically charged black holes are described. In addition to the standard Reissner-N\"ordstrom solution, there are new types of static black holes that arise in theories containing electrically charged…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Erick J. Weinberg

We present novel analytic hairy black holes with a flat base manifold in the (3+1)-dimensional Einstein SU(2)-Skyrme system with negative cosmological constant. We also construct (3+1)-dimensional black strings in the Einstein $SU(2)$-non…

高能物理 - 理论 · 物理学 2018-08-01 Marco Astorino , Fabrizio Canfora , Marcela Lagos , Aldo Vera

Previous studies showed that, in the presence of a simple and well-motivated self-interaction scalar potential, asymptotically flat and spherical black holes can carry minimally coupled and charged scalar cloud/hair in Einstein-Maxwell…

广义相对论与量子宇宙学 · 物理学 2022-06-09 Shao-Jun Zhang

We obtain charged spherically symmetric black holes in the two-component scalar Einstein-Maxwell-Friedberg-Lee-Sirlin model with a symmetry breaking potential. These asymptotically flat black holes carry resonant scalar Q-hair. As expected,…

高能物理 - 理论 · 物理学 2023-06-14 Jutta Kunz , Yakov Shnir

We investigate black hole solutions in the mimetic extension of the Einstein-Yang-Mills system, in which the Yang-Mills term is constrained to be constant. In the Abelian U(1) case, we find a static spherically symmetric solution that…

广义相对论与量子宇宙学 · 物理学 2025-12-01 Mohammad Ali Gorji , Susmita Jana , Pavel Petrov

Extreme magnetic dilaton black holes are promoted to exact solutions of heterotic string theory with unbroken supersymmetry. With account taken of alpha' corrections this is accomplished by supplementing the known solutions with SU(2)…

高能物理 - 理论 · 物理学 2009-12-30 R. Kallosh , T. Ortin
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