TY - JOUR
T1 - Stationary spacetime from intersecting M-branes
AU - Tanabe, Makoto
AU - Maeda, Kei Ichi
N1 - Funding Information:
We would like to thank Valeri Frolov, Dmitri Gal'tsov, Gary Gibbons, James Isenberg, Renata Kallosh, Tatsuhiko Koike, Robert Mann, Shuntaro Mizuno, Hidefumi Nomura, Masato Nozawa, Nobuyoshi Ohta, and Takashi Torii for useful discussions. K.M. also acknowledges Nobuyoshi Ohta for his especially helpful comments and M.T. expresses his heartfelt thanks to Hiroyuki Hyuga for encouragement. This work was partially supported by the Grant-in-Aid for Scientific Research Fund of the JSPS (No. 17540268) and another for the Japan–UK Research Cooperative Program, and by the Waseda University Grants for Special Research Projects and for The 21st Century COE Program (Holistic Research and Education Center for Physics Self-organization Systems) at Waseda University.
PY - 2006/3/22
Y1 - 2006/3/22
N2 - We study a stationary "black" brane in M/superstring theory. Assuming BPS-type relations between the first-order derivatives of metric functions, we present general stationary black brane solutions with a traveling wave for the Einstein equations in D-dimensions. The solutions are given by a few independent harmonic equations (and plus the Poisson equation). General solutions are constructed by superposition of a complete set of those harmonic functions. We prove that the solutions preserve the 1/8 supersymmetry if the gravi-electromagnetic field ℱij, which is a rotational part of gravity, is self-dual.
AB - We study a stationary "black" brane in M/superstring theory. Assuming BPS-type relations between the first-order derivatives of metric functions, we present general stationary black brane solutions with a traveling wave for the Einstein equations in D-dimensions. The solutions are given by a few independent harmonic equations (and plus the Poisson equation). General solutions are constructed by superposition of a complete set of those harmonic functions. We prove that the solutions preserve the 1/8 supersymmetry if the gravi-electromagnetic field ℱij, which is a rotational part of gravity, is self-dual.
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U2 - 10.1088/1742-6596/31/1/060
DO - 10.1088/1742-6596/31/1/060
M3 - Article
AN - SCOPUS:33645413412
SN - 1742-6588
VL - 31
SP - 215
EP - 216
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
IS - 1
ER -