activity
20002009
most citedBig-Bang Nucleosynthesis and Gravitino

462 citations · 2k across the 32 of their papers we have counts for

collaborators
Showing 2006Show all

13 papers · 1 filter

hep-ph20067 cited

The Gravitino-Overproduction Problem in Inflaton Decay

Masahiro Kawasaki, Fuminobu Takahashi, T. T. Yanagida

We show that the gravitino-overproduction problem is prevalent among inflation models in supergravity. An inflaton field generically acquires (effective) non-vanishing auxiliary fi…

astro-ph200658 cited

Constraint on the Effective Number of Neutrino Species from the WMAP and SDSS LRG Power Spectra

Kazuhide Ichikawa, Masahiro Kawasaki, Fuminobu Takahashi

We derive constraint on the effective number of neutrino species N_nu from the cosmic microwave background power spectrum of the WMAP and galaxy clustering power spectrum of the SD…

hep-ph200670 cited

Cosmological Constraints on Gravitino LSP Scenario with Sneutrino NLSP

Toru Kanzaki, Masahiro Kawasaki, Kazunori Kohri +1

We study the scenario where a sneutrino is the next lightest supersymmetric particle (NLSP) and decays into a gravitino and standard model particles. The daughter particles such as…

hep-ph200625 cited

Late-time Affleck-Dine baryogenesis after thermal inflation

Masahiro Kawasaki, Kazunori Nakayama

Thermal inflation can solve serious cosmological problems such as overproduction of gravitinos and moduli. However, it also dilutes the preexisting baryon asymmetry. We investigate…

hep-ph200691 cited

Inflaton Decay through Supergravity Effects

Motoi Endo, Masahiro Kawasaki, Fuminobu Takahashi +1

We point out that supergravity effects enable the inflaton to decay into all matter fields, including the visible and the supersymmetry breaking sectors, once the inflaton acquires…

hep-ph200627 cited

Towards the robustness of the Affleck-Dine baryogenesis

Shinta Kasuya, Masahiro Kawasaki

We study the Affleck-Dine mechanism with various types of the Kahler potential, and investigate whether or not the Affleck-Dine field could acquire a large VEV as an initial condit…