activity
19952009
most citedMeasurement of the Kerr Spin Parameter by Observation of a Compact Object's Shadow

457 citations · 2.2k across the 35 of their papers we have counts for

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Showing 2006Show all

6 papers · 1 filter

hep-th200630 cited

Supersymmetric Intersecting Branes in Time-dependent Backgrounds

Nobuyoshi Ohta, Kamal L. Panigrahi

We construct a family of supersymmetric solutions in time-dependent backgrounds in supergravity theories. One class of the solutions are intersecting brane solutions and another cl…

hep-th200640 cited

Fermions on Colliding Branes

Gary Gibbons, Kei-ichi Maeda, Yu-ichi Takamizu

We study the behaviour of five-dimensional fermions localized on branes, which we describe by domain walls, when two parallel branes collide in a five-dimensional Minkowski backgro…

hep-th20068 cited

Supersymmetric Rotating Black Hole in a Compactified Spacetime

Kei-ichi Maeda, Nobuyoshi Ohta, Makoto Tanabe

We construct a supersymmetric rotating black hole with asymptotically flat four-dimensional spacetime times a circle, by superposing an infinite number of BMPV black hole solutions…

astro-ph2006147 cited

Models for the Type Ic Hypernova SN 2003lw associated with GRB 031203

Paolo A. Mazzali, Jinsong Deng, Elena Pian +10

The Gamma-Ray Burst 031203 at a redshift z=0.1055 revealed a highly reddened Type Ic Supernova, SN 2003lw, in its afterglow light. This is the third well established case of a link…

hep-th200627 cited

Collision of Domain Walls in asymptotically Anti de Sitter spacetime

Yu-ichi Takamizu, Kei-ichi Maeda

We study collision of two domain walls in 5-dimensional asymptotically Anti de Sitter spacetime. This may provide the reheating mechanism of an ekpyrotic (or cyclic) brane universe…

astro-ph2006313 cited

A neutron-star-driven X-ray flash associated with supernova SN 2006aj

Paolo A. Mazzali, Jinsong Deng, Ken'ichi Nomoto +6

Supernovae connected with long-duration gamma-ray bursts (GRBs) are hyper-energetic explosion resulting from the collapse of very massive stars (about 40Mo, where Mo is the mass of…