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Titlebook: Black Objects in Supergravity; Proceedings of the I Stefano Bellucci Conference proceedings 2013 Springer International Publishing Switzerl

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樓主: ARSON
31#
發(fā)表于 2025-3-26 22:31:56 | 只看該作者
On Symmetries of Extremal Black Holes with One and Two Centers,ic 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 “.” symmetry . is elucidated by presenting a set of two-centered relations governing the structure of two-centered invariant polynomials.
32#
發(fā)表于 2025-3-27 01:28:49 | 只看該作者
33#
發(fā)表于 2025-3-27 07:14:00 | 只看該作者
Non-supersymmetric Extremal Black Holes: First-Order Flows and Stabilisation Equations,We review the results of [1, 2] on reducing the second-order equations of motion for stationary extremal black holes in four-dimensional . supergravity to first-order flow equations and further to non-differential stabilisation equations.
34#
發(fā)表于 2025-3-27 11:23:05 | 只看該作者
Non-holomorphic Deformations of Special Geometry and Their Applications,was first introduced in the context of . BPS black holes, but has a wider range of applicability. A theorem is presented according to which an arbitrary point-particle Lagrangian can be formulated in terms of a complex function ., whose features are analogous to those of the holomorphic function of
35#
發(fā)表于 2025-3-27 14:36:39 | 只看該作者
36#
發(fā)表于 2025-3-27 19:44:31 | 只看該作者
37#
發(fā)表于 2025-3-27 22:13:49 | 只看該作者
Non-extremal Black-Hole Solutions of , Supergravity,rgravity theories that describe effectively the low-energy dynamics of different string compactifications. Being solutions of theories with local supersymmetry one can distinguish among them the particular class of those that preserve some unbroken supersymmetries (called supersymmetric or, less pre
38#
發(fā)表于 2025-3-28 05:59:37 | 只看該作者
39#
發(fā)表于 2025-3-28 08:59:12 | 只看該作者
40#
發(fā)表于 2025-3-28 11:29:01 | 只看該作者
,From Clock Synchronization to Dark Matter as?a Relativistic Inertial Effect,universe given by the standard .CDM cosmological model [1, 2] based on the cosmological principle (homogeneity and isotropy of the space-time), which selects the class of Friedmann-Robertson-Walker (FWR) space-times.
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