CERN-TH/96-153 hep-th/9611205
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CERN-TH/96-32 IP-BBSR/96-9 hep-th/9602087 GRACEFUL EXIT IN QUANTUM STRING COSMOLOGY
We write an O(d, d)-covariant Wheeler-De Witt equation in the (d + 1)-dimensional minisuperspace of low-energy cosmological string backgrounds. We discuss explicit examples of transitions between two duality-related cosmological phases, and we find a finite quantum transition probability even when the two phases are classically separated by a curvature singularity. This quantum approach is comp...
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The Beckenstein-Hawking black hole entropy in string theory and its generalizations , as expressed in terms of charges that correspond to central extensions of the supersymmetry algebra, has more symmetries than U-duality. It is invariant under transformations of the charges, involving a 12th (or 13th) " dimension ". This is an indication that the secret theory behind string theory has a supera...
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The stability of the standard vacuum imposes constraints on flavor violating trilinear soft terms which are stronger than the laboratory bounds coming from the absence of neutral flavor violations (FCNC). Furthermore, contrary to the FCNC bounds, these constraints persist even if the scale of supersymmetry breaking is arbitrarily large. CERN-TH-96/116 SCIPP-96-22 SU-ITP 96/16 IEM-FT-131/96 May ...
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Theoretical Aspects of Dark Matter Detection
Direct and indirect dark matter detection relies on the scattering of the dark matter candidate on nucleons or nuclei. Here, attention is focused on dark matter candidates (neutralinos) predicted in the minimal supersymmetric standard model and its constrained version with universal input soft supersymmetry-breaking masses. Current expectations for elastic scattering cross sections for neutrali...
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