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19942023
most citedThe Einstein Equations on the 3-Brane World

1.4k citations · 17k across the 291 of their papers we have counts for

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Showing 2002Show all

6 papers · 1 filter

gr-qc2002★ 61 cited

Five-dimensional Black Hole and Particle Solution with Non-Abelian Gauge Field

Naoya Okuyama, Kei-ichi Maeda

We study the 5-dimensional Einstein-Yang-Mills system with a cosmological constant. Assuming a spherically symmetric spacetime, we find a new analytic black hole solution, which ap…

astro-ph2002

Hypernovae and their Nucleosynthesis

Ken'ichi Nomoto, Keiichi Maeda, Hideyuki Umeda +3

We review the characteristics of nucleosynthesis in 'Hypernovae', i.e., core-collapse supernovae with very large explosion energies ($ \gsim 10^{52} $ ergs). The hypernova yields s…

astro-ph2002★ 47 cited

Carbon Monoxide in the Type Ic SN 2000ew

Christopher L. Gerardy, Robert A. Fesen, Ken'ichi Nomoto +3

We present K-band (1.9 -- 2.5 micron) spectra of the Type Ic SN 2000ew observed with IRCS on the Subaru Telescope. These data show the first detection of carbon monoxide (CO) emiss…

hep-ph2002★ 30 cited

Dynamics of Scalar field in a Brane World

Shuntaro Mizuno, Kei-ichi Maeda, Kohta Yamamoto

We study the dynamics of a scalar field in the brane cosmology. We assume that a scalar field is confined in our 4-dimensional world. As for the potential of the scalar field, we d…

astro-ph2002★ 20 cited

Perturbation theory in Lagrangian hydrodynamics for a cosmological fluid with velocity dispersion

Takayuki Tatekawa, Momoko Suda, Kei-ichi Maeda +2

We extensively develop a perturbation theory for nonlinear cosmological dynamics, based on the Lagrangian description of hydrodynamics. We solve hydrodynamic equations for a self-g…

gr-qc2002★ 10 cited

Uniqueness of Self-Similar Asymptotically Friedmann-Robertson-Walker Spacetime in Brans-Dicke theory

Hideki Maeda, Jun-ichirou Koga, Kei-ichi Maeda

We investigate spherically symmetric self-similar solutions in Brans-Dicke theory. Assuming a perfect fluid with the equation of state , we show that there are…