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Black Holes in String Theory

Ansari, Saeid
  

(2011):


	Microscopic Calabi-Yau Black Holes in String Theory.


Dissertation, LMU München: Fakultät für Physik

Ansari, Saeid (2011): Microscopic Calabi-Yau Black Holes in String Theory. Dissertation, LMU München: Fakultät für Physik

... Calabi-Yau black hole, we then address the entropy of black hole in string ...use string theory to reproduce the macroscopic entropy law by counting the states of the underlay- ing ...

103

Subtracted Geometry

Subtracted Geometry

... of black holes in string ...four-charge black holes in the STU model, a con- sistent truncation of maximally supersymmetric supergravity with four types of electromag- netic ...

161

Six Dimensional Schwarzschild Brane Universe Sourced By Torsion

Six Dimensional Schwarzschild Brane Universe Sourced By Torsion

... describes black holes. In string theory, black holes have been obtained in a low energy limit of string effective action 12–15 ...superstring theory in a strong ...

9

Infinitely coloured black holes

Infinitely coloured black holes

... hairy black hole structures in Einstein theories coupled to non-Abelian gauge fields ...concerning black hole solutions in SU( ∞ ) gauge ...by string theory considerations. String ...

24

Black Holes in the Light of Field Theory and Quantum Mechanics

Black Holes in the Light of Field Theory and Quantum Mechanics

... in string theory is the study of the solution of a black hole in two ...4-dimensional black holes. With the hope that string theory provides a natural framework for ...

11

Hagedorn temperature and physics of black holes

Hagedorn temperature and physics of black holes

... We considered a kind of mean field approximation, when a thin shell of matter of mass δ M falls into the black hole of mass M. The gravitational field of the mass M is taken into account while the self-interaction ...

9

Schneider, Marc
  

(2018):


	Black holes are quantum complete.


Dissertation, LMU München: Fakultät für Physik

Schneider, Marc (2018): Black holes are quantum complete. Dissertation, LMU München: Fakultät für Physik

... in string theory a passing through a singular region is not ...Although string theo- ry has some candidate for black holes [Horowitz and Strominger, 1991], it is beyond the scope of ...

174

Effect of the Hair on Deflection Angle by Asymptotically Flat Black Holes in Einstein-Maxwell-Dilaton Theory

Effect of the Hair on Deflection Angle by Asymptotically Flat Black Holes in Einstein-Maxwell-Dilaton Theory

... flat black holes in Einstein-Maxwell-dilaton (EMD) theory, where is derived from a string theory at low energy limits ...EMD black holes have a scalar hair, in addition to ...

9

Perz, Jan
  

(2007):


	Black hole attractors and the entropy function in four- and five-dimensional N=2 supergravity.


Dissertation, LMU München: Fakultät für Physik

Perz, Jan (2007): Black hole attractors and the entropy function in four- and five-dimensional N=2 supergravity. Dissertation, LMU München: Fakultät für Physik

... Extremal black holes in theories of gravity coupled to abelian gauge fields and neutral scalars, such as those arising in the low-energy description of compactifications of string theory on ...

137

Dilatonic black holes in higher curvature string gravity. II. Linear stability

Dilatonic black holes in higher curvature string gravity. II. Linear stability

... dilatonic black holes are indeed stable under linear time-dependent perturbations of the classical ...hairy black hole structure that appears to be, at least linearly, ...of string ...

27

Dilatonic black holes in higher curvature string gravity. II. Linear stability

Dilatonic black holes in higher curvature string gravity. II. Linear stability

... of black holes are mod- ified when the theory of matter fields has sufficient ...of String Theory [1], ...have black holes with hair [2] ...Explicit black hole ...

24

Testing Generalized Einstein-Cartan-Kibble-Sciama Gravity using Weak Deflection Angle and Shadow Cast

Testing Generalized Einstein-Cartan-Kibble-Sciama Gravity using Weak Deflection Angle and Shadow Cast

... ECSK theory, the torsion field is not dynamic, because the torsion equation is an algebraic constraint rather than a partial differential equation, showing that the torsion field outside the distribution of matter ...

14

Frontiers of Astronomy, Astrophysics and Cosmology

Frontiers of Astronomy, Astrophysics and Cosmology

... H is spherical and the density of s-matter is uniform in the θ and ϕ angular directions. It is obvious that the temperature T sC in the centre of the s − black hole is the highest in the s-black hole. The ...

5

Topological black holes in su(N) Einstein Yang Mills theory with a negative cosmological constant

Topological black holes in su(N) Einstein Yang Mills theory with a negative cosmological constant

... of black holes with nontrivial matter field hair in asymptotically adS space-time also differ from the properties of their asymptotically flat ...(EYM) theory, spherically symmetric, asymptotically ...

8

Topology of Black Holes’ Horizons

Topology of Black Holes’ Horizons

... a black hole tends to deform the space around it, creating a vortex that captures nearby chunks of ...of black holes can be represented by a Schwarzschild Spacetime Embedding Diagram ...a ...

6

Binary Black Holes Algorithm

Binary Black Holes Algorithm

... The black hole algorithm proposed in the paper [12] by Nemati et ...random black holes as initial solution. Each of this black holes has own position, mass and electrical ...of ...

7

THE CASE STUDY OF  BLACK HOLES?

THE CASE STUDY OF BLACK HOLES?

... At the point when a question falls into a dark opening, any data about the state of the protest or dissemination of charge on it is uniformly dispersed along the skyline of the dark gap, and is lost to outside onlookers. ...

6

Elasticity of Cylindrical Black Holes

Elasticity of Cylindrical Black Holes

... and black cylinders have known instabilities that act to change the energy of the cylinder by changing the surface area, as in equation ...perturbed black cylinder, the final evolved shape (after the ...

9

Topological black holes in su(N) Einstein-Yang-Mills theory with a negative cosmological constant

Topological black holes in su(N) Einstein-Yang-Mills theory with a negative cosmological constant

... Topological black holes with Ricci-flat (k = 0) event horizons have attracted a great deal of attention recently as models of holo- graphic superconductors (see, for example, [28] for a recent re- ...EYM ...

6

Properties of particles in the ergosphere of black holes

Properties of particles in the ergosphere of black holes

... As it is known special geodesics on which particles with negative and zero energy (with nonzero angular momentum projection) can move are existing in the ergosphere of rotating black holes [1]– [3]. Such ...

12

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