PIRSA:06050027

Video URL

https://pirsa.org/06050027

String Cosmology in the Hagedorn Phase

Patil, S. (2006). String Cosmology in the Hagedorn Phase. Perimeter Institute for Theoretical Physics. https://pirsa.org/06050027

Patil, Subodh. String Cosmology in the Hagedorn Phase. Perimeter Institute for Theoretical Physics, May. 30, 2006, https://pirsa.org/06050027 

          @misc{ scivideos_PIRSA:06050027,
            doi = {10.48660/06050027},
            url = {https://pirsa.org/06050027},
            author = {Patil, Subodh},
            keywords = {Cosmology},
            language = {en},
            title = {String Cosmology in the Hagedorn Phase},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2006},
            month = {may},
            note = {PIRSA:06050027 see, \url{https://scivideos.org/pirsa/06050027}}
          }

Subodh Patil Université de Genève

Talk numberPIRSA:06050027
DOI10.48660/06050027
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

It has recently been proposed by Nayeri, Brandenberger and Vafa, that the thermodynamics of strings in the early universe can provide us with a causal mechanism to generate a scale invariant spectrum of primordial density fluctuations, without requiring an intervening epoch of inflation. We will review this mechanism, and report on more recent work which has uncovered several observational consequences of the NBV mechanism, some of which in principle, will be distinguishable from the generic predictions of inflation.