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Dr Anupam Mazumdar (NORDITA)30/07/2007, 16:30Cosmology and AstrophysicsParallel TalkMinimal Supersymmetric Standard Model has all the ingredients to provide a successful inflation. The inflaton is a gauge invariant flat direction which carries the Standard Model charges. I will discuss how such a model predicts the CMB observations and provides hope for its detectability at LHC. I will also discuss how a thermal production of neutalino in conjunction with MSSM inflation...Go to contribution page
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Dr Motoi Endo (DESY)30/07/2007, 16:50Cosmology and AstrophysicsParallel TalkWe will discuss the gravitino production in early universe from scalar field which reheats the universe. Such production is pointed out to be rather generic and modify usual cosmological scenarios significantly. To be concrete, we will analyze several inflation models.Go to contribution page
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Dr Fuminobu Takahashi (DESY)30/07/2007, 17:10Cosmology and AstrophysicsParallel TalkI will discuss the recently discovered gravitino overproduction from inflaton decay, particualrly focusing on its implication for the SUSY breaking and inflation models. Importantly, since the inflaton generically produces the gravitinos, those constraints will turn out to be quite useful to know which models are realized in nature, especially when the upcoming collider experimental data...Go to contribution page
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Dr Krzysztof Turzynski (University of Michigan)30/07/2007, 17:30Cosmology and AstrophysicsParallel TalkWe study cosmological perturbations in two-field inflation, allowing for non-standard kinetic terms. We calculate analytically the spectra of curvature and isocurvature modes at Hubble crossing, up to first order in the slow-roll parameters. We also compute numerically the evolution of the curvature and isocurvature modes from well within the Hubble radius until the end of inflation. We...Go to contribution page
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Mr Tomohiro Matsuda (Saitama Institute of Technology)30/07/2007, 17:50Cosmology and AstrophysicsParallel TalkWe consider an inhomogeneous preheating scenario in multi-field inflationary models. There are at least two fields trapped at the ESP after preheating, one is the inflaton and the other is a ``trapped field'' that plays important role in generating the curvature perturbation. We consider several kinds of the potential for the trapped field, which mimics thermal or quintessential inflation.Go to contribution page
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Mr Masahide Yamaguchi (Aoyama Gakuin University)30/07/2007, 18:10Cosmology and AstrophysicsParallel TalkWe present a chaotic inflation model dominated by the D-term in supergravity. Our model opens a new branch of model building for inflation.Go to contribution page
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