منابع مشابه
Rotating Rotated Branes
We present a class of spacetime rotations that preserve a proportion of spacetime supersymmetry. We then give the rules for superposing these rotations with various branes to construct rotating brane solutions which preserve exotic fractions of supersymmetry. We also investigate the superposition of rotations with intersecting branes at angles and we find new rotating intersecting branes at ang...
متن کاملSupersymmetry of Rotating Branes
We present a new 1/8 supersymmetric intersecting M-brane solution of D=11 supergravity with two independent rotation parameters. The metric has a non-singular event horizon and the near-horizon geometry is adS3×S×S×E (just as in the non-rotating case). We also present a method of determining the isometry supergroup of supergravity solutions from the Killing spinors and use it to show that for t...
متن کاملRotating Intersecting M-Branes
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 rot...
متن کاملRotated Branes and N = 1 Duality
We consider configurations of rotated N S-branes leading to a family of four-dimensional N = 1 super-QCD theories, interpolating between four-dimensional analogues of the Hanany-Witten vacua, and the Elitzur-Giveon-Kutasov configuration for N = 1 duality. The rotation angle is the N = 2 breaking parameter, the mass of the adjoint scalar in the N = 2 vector multiplet. We add some comments on the...
متن کاملLocalization instability in the rotating D-branes
In the microcanonical ensemble for string theory on AdSm × Sn, there is a phase transition between a black hole solution extended over the Sn and a solution localized on the Sn if the AdSm has the topology R 2 × Sm−2. The phase transition will not appear if the AdSm has the topology R 2 × Tm−2, that is, when the AdSm × Sn geometry is regarded as arising from the nearhorizon limit of a black m −...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Journal of High Energy Physics
سال: 1999
ISSN: 1029-8479
DOI: 10.1088/1126-6708/1999/04/014