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 2007Show all

11 papers · 1 filter

hep-th200722 cited

Entropy Function and Universality of Entropy-Area Relation for Small Black Holes

Rong-Gen Cai, Chiang-Mei Chen, Kei-ichi Maeda +2

We discuss the entropy-area relation for the small black holes with higher curvature corrections by using the entropy function formalism and field redefinition method. We show that…

hep-th200730 cited

Cosmological Density Fluctuations in Stochastic Gravity -- Formalism and Linear Analysis --

Yuko Urakawa, Kei-ichi Maeda

We study primordial perturbations generated from quantum fluctuations of an inflaton based on the formalism of stochastic gravity. Integrating out the degree of freedom of the infl…

astro-ph2007101 cited

The evolution of the peculiar Type Ia supernova SN 2005hk over 400 days

D. K. Sahu, Masaomi Tanaka, G. C. Anupama +6

photometry and medium resolution optical spectroscopy of peculiar Type Ia supernova SN 2005hk are presented and analysed, covering the pre-maximum phase to around 400 days…

astro-ph200734 cited

Multi-Dimensional Simulations for Early Phase Spectra of Aspherical Hypernovae: SN 1998bw and Off-Axis Hypernovae

Masaomi Tanaka, Keiichi Maeda, Paolo A. Mazzali +1

Early phase optical spectra of aspherical jet-like supernovae (SNe) are presented. We focus on energetic core-collapse SNe, or hypernovae. Based on hydrodynamic and nucleosynthetic…

astro-ph2007

Probing the Explosion Mechanism of Supernovae by Radioactive Decay Gamma- and X-Rays

Keiichi Maeda

Gamma- and X-rays resulting from radioactive decays provide a potentially powerful tool to investigate the explosion physics of supernovae, since the distribution and the amount of…

astro-ph2007

Supernovae in Three-Dimension: A Link to Gamma-Ray Bursts

Keiichi Maeda

Observational consequences of a jet-driven supernova (SN) explosion model are presented. The results are compared in detail with optical observations of SN 1998bw associated with a…