1999/05/24 by T. Asaka, Masahiro Kawasaki, M. Kawasaki · 5 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Dilaton #Gravitino #Hidden sector #Inflation (cosmology) #Moduli #Order (exchange) #Particle physics #Particle physics theoretical and experimental studies #Physics #Quantum mechanics #Supergravity #Superstring theory #Supersymmetry #Supersymmetry breaking #Theoretical physics #hep-ph
paper · pdf · doi:10.1103/physrevd.60.123509
published as Phys.Rev. D60 (1999) 123509 · 49 pages, 17 figures
arxiv created 1999/05/24 · openalex publication_date 1999/11/24 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
In superstring theories, there exist various dilaton and modulus fields whose masses are expected to be of the order of the gravitino mass m3/2. These fields lead to serious cosmological difficulties, the so called ``cosmological moduli problem,'' because a large number of moduli particles are produced as the coherent oscillations after primordial inflation. We make a comprehensive study of whether the thermal inflation can solve the cosmological moduli problem in the whole modulus mass region m_\ensuremathφ\ensuremath∼10eV--104GeV predicted by both hidden sector supersymmetry (SUSY) breaking and gauge-mediated SUSY breaking models. In particular, we take into account the primordial inflation model whose reheating temperature is so low that its reheating process finishes after the thermal inflation ends. We find that the above mass region m_\ensuremathφ(\ensuremath≃m3/2)\ensuremath∼10eV--104GeV survives from various cosmological constraints in the presence of thermal inflation.