5–7 May 2014
University of Pittsburgh
US/Eastern timezone

Constraints on Supersymmetric Cosmological Inflation Model

5 May 2014, 15:15
15m
Benedum Hall G26 (University of Pittsburgh)

Benedum Hall G26

University of Pittsburgh

Speaker

Mayukh Gangopadhyay (University of Notre Dame du Lac)

Description

Cosmological Inflation is a theory ad hoc from Particle Physics in Cosmology. It is a very important inclusion in early universe study and became one of the very important and open topic of research in last three decades. In my talk I will go through some of the well known models of cosmological inflation and what is the chance of survival of these models as we test them with observational results. With the recent data from Planck project, we get better idea about the CMB and thus can study these models in details. On the other hand different experimental bounds from different particle physics experiment effects this models too. In this presentation my special emphasis will be on those models which depend on SUSY when built and how they can be affected by the recent developments in observations.

Author

Mayukh Gangopadhyay (University of Notre Dame du Lac)

Presentation materials