Rotating intersecting M-branes
Dec, 199626 pages
Published in:
- Nucl.Phys.B 499 (1997) 253-282
e-Print:
- hep-th/9612229 [hep-th]
Report number:
- IASSNS-HEP-96-123,
- UPR-0728-T
View in:
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Abstract:
We present intersecting p-brane solutions of eleven-dimensional supergravity (M-branes) which upon toroidal compactification reduce to non-extreme ``rotating'' black holes. We identify harmonic functions, associated with each M-brane, and non-extremality functions, specifying a deviation from the BPS limit. These functions are modified due to the angular momentum parameters, which specify the rotation along the transverse directions of the M-branes. We spell out the intersection rules for the eleven-dimensional space-time metric for intersecting (up to three) rotating M-brane configurations (and a boost along the common intersecting direction).Note:
- 28 pages, uses RevTex, the revised version to appear in Nuclear Physics B Report-no: IASSNS-HEP-96/123,UPR-728-T
- 04.50.+h
- 04.20.Jb
- 04.70.Bw
- 11.25.Mj
- 11.27.+d
- Extended classical solutions
- p -branes
- Exact solutions
- Classical black holes
- Gravity in more than four dimensions
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