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441“…We provide a general strategy to obtain the superpotential W for both BPS and non-BPS extremal black holes in N=2 four dimensional supergravities based on symmetric spaces. …”
Enlace del recurso
Enlace del recurso
info:eu-repo/semantics/article -
442“…We study the effects of N=4 topological string amplitudes on the entropy of black holes. We analyse the leading contribution associated to six-derivative terms and find one particular operator which can correct the entropy of N=4 black holes. …”
Enlace del recurso
Enlace del recurso
info:eu-repo/semantics/article -
443
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444
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445
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446
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447
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448
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449“…In particular the W function for small non-BPS black holes can always be computed analytically, unlike for the large black-hole case.…”
Enlace del recurso
Enlace del recurso
info:eu-repo/semantics/article -
450por Marrani, Alessio“…We report on the theory of "large" U-duality charge orbits and related "moduli spaces" of extremal black hole attractors in N = 2, d = 4 Maxwell-Einstein supergravity theories with symmetric scalar manifolds, as well as in N > 3-extended, d = 4 supergravities.…”
Publicado 2010
Enlace del recurso
Enlace del recurso
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451“…We also speculate on N=1 theories displaying "large" extremal black hole solutions.…”
Enlace del recurso
Enlace del recurso
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452
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453por Botta Cantcheff, Marcelo“…We also argue that, in this context, gravitational collapse and formation of a black hole may be described by unitary evolution of the dual non-perturbative degrees of freedom.…”
Publicado 2012
Enlace del recurso
Enlace del recurso
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454“…We reformulate the quantum black hole portrait in the language of modern condensed matter physics. …”
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Enlace del recurso
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455“…After a brief introduction to the Attractor Mechanism, we review the appearance of groups of type E7 as generalized electric-magnetic duality symmetries in locally supersymmetric theories of gravity, with particular emphasis on the symplectic structure of fluxes in the background of extremal black hole solutions, with one or two centers. In the latter case, the role of an "horizontal" symmetry SL(2,R) is elucidated by presenting a set of two-centered relations governing the structure of two-centered invariant polynomials.…”
Enlace del recurso
Enlace del recurso
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456
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457por Damour, Thibault Marie Alban Guillaume“…Experimental tests. Black Holes: extensions of the Schwarzschild solution; Kerr-Newman holes; no-hair theorems; energtics of black holes; the membrane approach; quantum mechanics of black holes; Bekenstein entropy; Hawking temperature; black holes and string theory.…”
Publicado 2001
Enlace del recurso
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458por Damour, Thibault Marie Alban Guillaume“…Experimental tests. Black Holes: extensions of the Schwarzschild solution; Kerr-Newman holes; no-hair theorems; energtics of black holes; the membrane approach; quantum mechanics of black holes; Bekenstein entropy; Hawking temperature; black holes and string theory.…”
Publicado 2001
Enlace del recurso
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459por Damour, Thibault Marie Alban Guillaume“…Experimental tests. Black Holes: extensions of the Schwarzschild solution; Kerr-Newman holes; no-hair theorems; energtics of black holes; the membrane approach; quantum mechanics of black holes; Bekenstein entropy; Hawking temperature; black holes and string theory.…”
Publicado 2001
Enlace del recurso
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460por Damour, Thibault Marie Alban Guillaume“…Experimental tests. Black Holes: extensions of the Schwarzschild solution; Kerr-Newman holes; no-hair theorems; energtics of black holes; the membrane approach; quantum mechanics of black holes; Bekenstein entropy; Hawking temperature; black holes and string theory.…”
Publicado 2001
Enlace del recurso