activity
20062010
most citedReheating Temperature after Inflation in No-Scale Supergravity

1 citations · 3 across the 6 of their papers we have counts for

collaborators

6 papers

hep-ph2010★ 1 cited

Dilatonic Inflation, Gravitino and Reheating in Modified Modular invariant Supergravity

Yuta Koshimizu, Toyokazu Fukuoka, Kenji Takagi +2

A new modified string-inspired modular invariant supergravity model is proposed and is applied to realize the slow roll inflation in Einstein frame, so that the model explains WMAP…

hep-ph2010

Inflation, Gravitino and Reheating in Modified Modular invariant Supergravity

Mitsuo J. Hayashi, Yuta Koshimizu, Toyokazu Fukuoka +2

A new modified string-inspired modular invariant supergravity model is proposed and is applied to realize the slow roll inflation in Einstein frame. Because inflation deals with Pl…

hep-ph2010

Supersymmetry Breaking and Gravitino Production after Inflation in Modular Invariant Supergravity

Kenji Takagi, Yuta Koshimizu, Toyokazu Fukuoka +2

By using a string-inspired modular invariant supergravity, which was proved well to explain WMAP observations appropriately, a mechanism of supersymmetry breaking (SSB) and Graviti…

hep-ph2010★ 1 cited

Reheating Temperature after Inflation in No-Scale Supergravity

Yuta Koshimizu, Toyokazu Fukuoka, Kenji Takagi +2

By using a No-Scale Supergravity model, which was proved well to explain WMAP observations appropriately, a mechanism of preheating just after the end of inflation is investigated.…

hep-ph2009

Gravitino Production after Inflation in No-Scale Supergravity

Kenji Takagi, Yuta Koshimizu, Toyokazu Fukuoka +3

By using a No-Scale Supergravity model, which was proved to explain WMAP observations appropriately, a mechanism of supersymmetry breaking and a preheating just after the end of in…

astro-ph2006★ 1 cited

Angular Power Spectrum in Modular Invariant Inflation Model

Mitsuo J. Hayashi, Shiro Hirai, Tomoyuki Takami +3

We propose a scalar potential of inflation, motivated by modular invariant supergravity, and compute the angular power spectra of the adiabatic density perturbations that result fr…