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Jason Kumar (Texas A&M University)30/07/2007, 16:30Theoretical Models (String Theory and Formal Aspects of SUSY)Parallel TalkWe introduce a novel mechanism for baryogenesis, in which mixed anomalies between the hidden sector and $U(1)_{baryon}$ drive the baryon asymmetry. We demonstrate that this mechanism occurs quite naturally in intersecting- brane constructions of the Standard Model, and show that it solves some of the theoretical difficulties faced in matching baryogenesis to experimental bounds. We...Go to contribution page
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Louis Clavelli (University of Alabama)30/07/2007, 16:50Theoretical Models (String Theory and Formal Aspects of SUSY)Parallel TalkString landscape ideas and the observation of a positive vacuum energy in the current universe suggest that there could be a future transition to an exactly supersymmetric world. Atomic and molecular binding in this susy background probably require that electroweak symmetry breaking survives the transition. Among several susy higgs models that have been discussed, one stands out in this...Go to contribution page
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Dr Ivonne Zavala (Durham University)30/07/2007, 17:10Theoretical Models (String Theory and Formal Aspects of SUSY)Parallel TalkI will discuss the dynamics of a probe D3-brane propagating in a warped string compactification. I will focus in the exploration of the trajectories obtained from giving the brane angular momentum in the extra dimensions. I will show that, in general, angular momentum creates a centrifugal barrier, causing bouncing as well as cyclic cosmologies from a "mirage" point of view. I will also...Go to contribution page
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Dr Xavier Calmet (Université Libre de Bruxelles)30/07/2007, 17:30Theoretical Models (String Theory and Formal Aspects of SUSY)Parallel TalkWe propose a new mechanism to generate the mass of a scalar field in an expanding universe. The mass of this field turns out to be generated by the cosmological constant and can be naturally small if protected by a conformal symmetry which is however broken in the gravitational sector. The mass is comparable today to the Hubble time. This scalar field could thus impact our universe today...Go to contribution page
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Prof. Teruki Kamon (Texas A&M University)30/07/2007, 17:50Theoretical Models (String Theory and Formal Aspects of SUSY)Parallel TalkRecently, it is shown that the modifications of the Boltzmann equation describing the evolution of relic abundances due to dilaton dissipative-source and non-critical-string terms change the cosmologically allowed parameter space of SUSY model. In this talk, we will investigate the allowed parameter space in the context of minimal SUGRA boundary condition at the LHC. We will...Go to contribution page
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Dr Axel Krause (Arnold Sommerfeld Center, LMU Muenchen)30/07/2007, 18:10Theoretical Models (String Theory and Formal Aspects of SUSY)Parallel TalkThe potential detection of gravitational waves from string inflation would provide essential complementary information to measurements of the scalar spectral index. E.g.~it can tell us directly the size of the inflationary potential. It is, however, clear that warped brane inflation (in case it can be tuned to give inflation) cannot lead to measurable gravitational waves. We will discuss...Go to contribution page
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