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We consider stationary, non-extremal black holes in 11-dimensional supergravity having isometry group $\mathbb{R} \times U(1)^8$. We prove that such a black hole is uniquely specified by its angular momenta, its electric charges associated…

General Relativity and Quantum Cosmology · Physics 2015-06-04 Stefan Hollands

We derive and solve the black hole attractor conditions of N=8 supergravity by finding the critical points of the corresponding black hole potential. This is achieved by a simple generalization of the symplectic structure of the special…

High Energy Physics - Theory · Physics 2016-09-06 Sergio Ferrara , Renata Kallosh

We study four dimensional non-supersymmetric attractors in type IIA string theory in the presence of sub-leading corrections to the prepotential. For a given Calabi-Yau manifold, the D0-D4 system admits an attractor point in the moduli…

High Energy Physics - Theory · Physics 2015-05-28 Pramod Dominic , Prasanta K. Tripathy

In four dimensional string theories with N=4 and N=8 supersymmetries one can often define twisted index in a subspace of the moduli space which captures additional information on the partition function than the ones contained in the usual…

High Energy Physics - Theory · Physics 2010-05-25 Ashoke Sen

Solutions to low energy string theory describing black holes and black strings are reviewed. Many of these solutions can be obtained by applying simple solution generating transformations to the Schwarzschild metric. In a few cases, the…

High Energy Physics - Theory · Physics 2007-05-23 Gary T. Horowitz

In this work, we follow the recently revisited f(R) theory of gravity for studying the interaction between quantum scalar particles and the gravitational field of a generalized black hole with an f(R) global monopole. This background has a…

General Relativity and Quantum Cosmology · Physics 2022-01-04 H. S. Vieira

We report on the Parallel Session BH4 "Gravitational fields with sources: From compact objects to black holes" of the 14th Marcel Grossmann Meeting held at Sapienza University of Rome in 2015.

General Relativity and Quantum Cosmology · Physics 2016-09-06 José P. S. Lemos , Paolo Pani

These notes are the written version of two lectures delivered at the VIII Mexican School on Particles and Fields on November 1998. The level of the notes is basic assuming only some knowledge on Statistical Mechanics, General Relativity and…

High Energy Physics - Theory · Physics 2010-12-13 Maximo Banados

We show that the second order field equations characterizing extremal solutions for spherically symmetric, stationary black holes are in fact implied by a system of first order equations given in terms of a prepotential W. This confirms and…

High Energy Physics - Theory · Physics 2009-04-17 Laura Andrianopoli , Riccardo D'Auria , Emanuele Orazi , Mario Trigiante

This is a short summary of my lectures given at the Fourth Mexican School on Gravitation and Mathematical Physics. These lectures gave a brief introduction to black holes in string theory, in which I primarily focussed on describing some of…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Robert C. Myers

Scaling black holes are solutions of supergravity with multiple black hole singularities, which can be adiabatically connected to a single center black hole solution. We develop techniques to determine partition functions for such scaling…

High Energy Physics - Theory · Physics 2022-03-14 Aradhita Chattopadhyaya , Jan Manschot , Swapnamay Mondal

The type IIA superstring partition function Z_IIA on the euclidean attractor geometry AdS_2 x S^2 x CY_3, computes the modified elliptic genus Z_BH of the associated black hole. The hybrid formalism of superstrings defined as a conformally…

High Energy Physics - Theory · Physics 2011-08-09 B. Chandrasekhar

Black holes are the hydrogen atoms of quantum gravity. For instance solving the information loss paradox will likely require a deep understanding of how the long-sought quantum gravity theory works. In this thesis we explore how black holes…

High Energy Physics - Theory · Physics 2019-11-27 Lorenzo Pieri

We derive the Bekenstein-Hawking entropy for a class of BPS black holes in the massive type IIA supergravity background AdS$_4 \times S^6$ from a microscopic counting of supersymmetric ground states in a holographically dual field theory.…

High Energy Physics - Theory · Physics 2017-11-02 Seyed Morteza Hosseini , Kiril Hristov , Achilleas Passias

We consider theories with gravity, gauge fields and scalars in four-dimensional asymptotically flat space-time. By studying the equations of motion directly we show that the attractor mechanism can work for non-supersymmetric extremal black…

High Energy Physics - Theory · Physics 2009-11-11 Kevin Goldstein , Norihiro Iizuka , Rudra P. Jena , Sandip P. Trivedi

In two-derivative theories of gravity coupled to matter, charged black holes are self-attractive at large distances, with the force vanishing at zero temperature. However, in the presence of massless scalar fields and four-derivative…

High Energy Physics - Theory · Physics 2022-03-23 Sera Cremonini , Callum R. T. Jones , James T. Liu , Brian McPeak , Yuezhang Tang

These notes, based on lectures given at the summer school on Asymptotic Analysis in General Relativity, collect material on the Einstein equations, the geometry of black hole spacetimes, and the analysis of fields on black hole backgrounds.…

General Relativity and Quantum Cosmology · Physics 2016-10-13 Lars Andersson , Thomas Bäckdahl , Pieter Blue

These are lecture notes for two lectures delivered at the Les Houches workshop on Number Theory, Physics, and Geometry, March 2003. They review two examples of interesting interactions between number theory and string compactification, and…

High Energy Physics - Theory · Physics 2007-12-08 Gregory W. Moore

The study of regular black holes and black hole mimickers as alternatives to standard black holes has recently gained significant attention, driven both by the need to extend general relativity to describe black hole interiors, and by…

We consider Matrix theory compactified on T^3 and show that it correctly describes the properties of Schwarzschild black holes in 7+1 dimensions, including the energy-entropy relation, the Hawking temperature and the physical size, up to…

High Energy Physics - Theory · Physics 2008-11-26 T. Banks , W. Fischler , I. R. Klebanov , L. Susskind