Large Scale Structure: Our last chance to discover the hidden scenario of Early Universe

محمد انصاری (دانشکده فیزیک دانشگاه صنعتی شریف)

Abstract: The inflationary models solve several problems of cosmology, such as horizon problem and the flatness of the Universe. But however there are lots of inflationary models which Cosmic Microwave Background (CMB) can’t rule out them now. Non-Gaussianity and tensor perturbation are two complementary probes for inflationary models. This is because the inflationary models have different predictions for these two observables, however they are not detected yet. The deviation of the scale invariance of the primordial power spectrum is another opportunity which is detected by CMB data but with low statistical significance. In this presentation I will talk about the last opportunity and justify how Large Scale Structure will help us to rule out more inflationary models or the inflation scenario itself (through some idea about clock signal models which is developed recently).

یکشنبه 3 بهمن ماه 1395، ساعت 15:00

    دانشکده فیزیک، تالار پرتوی