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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 2009 · hep-thShow all

6 papers · 2 filters

hep-th2009★ 37 cited

Black Hole in the Expanding Universe from Intersecting Branes

Kei-ichi Maeda, Masato Nozawa

We study physical properties and global structures of a time-dependent, spherically symmetric solution obtained via the dimensional reduction of intersecting M-branes. We find that…

hep-th2009★ 7 cited

The Bernstein Conjecture, Minimal Cones, and Critical Dimensions

Gary W. Gibbons, Kei-ichi Maeda, Umpei Miyamoto

Minimal surfaces and domain walls play important roles in various contexts of spacetime physics as well as material science. In this paper, we first review the Bernstein conjecture…

hep-th2009★ 97 cited

Black Hole Solutions in String Theory with Gauss-Bonnet Curvature Correction

Kei-ichi Maeda, Nobuyoshi Ohta, Yukinori Sasagawa

We present the black hole solutions and analyse their properties in the superstring effective field theory with the Gauss-Bonnet curvature correction terms. We find qualitative dif…

hep-th2009★ 52 cited

Dynamics of intersecting brane systems -- Classification and their applications --

Kei-ichi Maeda, Nobuyoshi Ohta, Kunihito Uzawa

We present dynamical intersecting brane solutions in higher-dimensional gravitational theory coupled to dilaton and several forms. Assuming the forms of metric, form fields, and di…

hep-th2009★ 28 cited

Supersymmetric Intersecting Branes in Time-dependent Backgrounds

Kei-ichi Maeda, Nobuyoshi Ohta, Makoto Tanabe +1

We construct a fairy general family of supersymmetric solutions in time- and space-dependent backgrounds in general supergravity theories. One class of the solutions are intersecti…

hep-th2009★ 30 cited

Attractor Universe in the Scalar-Tensor Theory of Gravitation

Kei-ichi Maeda, Yasunori Fujii

In the scalar-tensor theory of gravitation it seems nontrivial to establish if solutions of the cosmological equations in the presence of a cosmological constant behave as attracto…