A-term inflation

          @misc{ scivideos_PIRSA:06100001,
            doi = {10.48660/06100001},
            url = {https://pirsa.org/06100001},
            author = {Allahverdi, Rouzbeh},
            keywords = {Particle Physics, Cosmology},
            language = {en},
            title = {A-term inflation},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2006},
            month = {oct},
            note = {PIRSA:06100001 see, \url{https://scivideos.org/index.php/pirsa/06100001}}
          }
          

Abstract

I argue that all necessary ingredients for successful inflation are present in the minimal supersymmetric standard model (MSSM). The potential for the supersymmetric flat directions (which can be viewed as moduli near points of enhanced symmetry) generically has metastable minima at large field values. An adjustment of soft supersymemtry breaking parameters results in a point where the first two derivatives of the potential vanish. One can then have more than 10^3 e-foldings of slow roll inflation with a Hubble rate ~ O(1-10) GeV in the vicinity of this point. The model has a robust prediction for the scalar spectral index: n_s \leq 0.93, which agrees with the current WMAP and LSS data within 2\sigma. It can be implemented purely within MSSM, or MSSM plus Dirac neutrinos. It has the unique feature of having a concrete and real connection to physics that can be observed in earthbound laboratories.