We study unphysical features of the BMPV black hole and how each can be resolved using the enhancon mechanism. We begin by reviewing how the enhancon mechanism resolves a class of repulson singularities which arise in the BMPV geometry when D--branes are wrapped on K3. In the process, we show that the interior of an enhancon shell can be a time machine due to non-vanishing rotation. We link the resolution of the time machine to the recently proposed resolution of the BMPV naked singularity / "over-rotating" geometry through the expansion of strings in the presence of RR flux. We extend the analysis to include a general class of BMPV black hole configurations, showing that any attempt to "over-rotate" a causally sound BMPV black hole will be...
We revisit here a recent work on regular rotating black holes. We introduce a new mass function gene...
We present a Kerr-Newman type stationary and axisymmetric solution that describes rotating black hol...
We employ the formalism of the Horizon Quantum Mechanics to describe the gravitational radius of com...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.Includes bibliographi...
This thesis is divided into two parts. The first part studies the response of Unruh DeWitt detectors...
Rotating black holes in Einstein-Maxwell-Chern-Simons theory possess remarkable features when the Ch...
Blandford and Znajek discovered a process by which a spinning black hole can transfer rotational ene...
Recently, two of us have argued that non-Kerr black holes in gravity theories different from General...
We construct spinning black holes (BHs) in shift-symmetric Horndeski theory. This is an Einstein-sca...
We consider black holes generically sourced by quantum matter described by regular wavefunctions. Th...
Understanding the microscopic structure of black holes remains one of the most important tasks of th...
We study collisions of boosted rotating black holes in $D=6$ and 7 spacetime dimensions with a non-...
Singly-spinning Myers-Perry black holes in d ≥ 6 spacetime dimensions are unstable for sufficiently ...
Abstract We study collisions of boosted rotating black holes in D = 6 and 7 spa...
We study slowly rotating, asymptotically flat black holes in Einstein-aether theory and show that so...
We revisit here a recent work on regular rotating black holes. We introduce a new mass function gene...
We present a Kerr-Newman type stationary and axisymmetric solution that describes rotating black hol...
We employ the formalism of the Horizon Quantum Mechanics to describe the gravitational radius of com...
Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.Includes bibliographi...
This thesis is divided into two parts. The first part studies the response of Unruh DeWitt detectors...
Rotating black holes in Einstein-Maxwell-Chern-Simons theory possess remarkable features when the Ch...
Blandford and Znajek discovered a process by which a spinning black hole can transfer rotational ene...
Recently, two of us have argued that non-Kerr black holes in gravity theories different from General...
We construct spinning black holes (BHs) in shift-symmetric Horndeski theory. This is an Einstein-sca...
We consider black holes generically sourced by quantum matter described by regular wavefunctions. Th...
Understanding the microscopic structure of black holes remains one of the most important tasks of th...
We study collisions of boosted rotating black holes in $D=6$ and 7 spacetime dimensions with a non-...
Singly-spinning Myers-Perry black holes in d ≥ 6 spacetime dimensions are unstable for sufficiently ...
Abstract We study collisions of boosted rotating black holes in D = 6 and 7 spa...
We study slowly rotating, asymptotically flat black holes in Einstein-aether theory and show that so...
We revisit here a recent work on regular rotating black holes. We introduce a new mass function gene...
We present a Kerr-Newman type stationary and axisymmetric solution that describes rotating black hol...
We employ the formalism of the Horizon Quantum Mechanics to describe the gravitational radius of com...