activity
20092011
most citedConstraining Galileon gravity from observational data with growth rate

15 citations · 43 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.CO2011★ 15 cited

Constraining Galileon gravity from observational data with growth rate

Koichi Hirano, Zen Komiya, Hisato Shirai

We studied the cosmological constraints on the Galileon gravity obtained from observational data of the growth rate of matter density perturbations, the supernovae Ia (SN Ia), the…

astro-ph.CO2011

Galaxy N-z Relation and CMB Spectrum Based on Cosmological Model with Scalar Field Having Modified Potential Form

Koichi Hirano, Kiyoshi Kawabata, Zen Komiya +1

We have succeeded in establishing a cosmological model with a non-minimally coupled scalar field that can account not only for the spatial periodicity or the picket-fence struc…

astro-ph.CO2010★ 12 cited

Observational tests for oscillating expansion rate of the Universe

Koichi Hirano, Zen Komiya

We investigate the observational constraints on the oscillating scalar field model using data from type Ia supernovae, cosmic microwave background anisotropies, and baryon acoustic…

astro-ph.CO2010★ 1 cited

N-z Relation and CMB Anisotropies in the Universe with an Oscillating Scalar Field Having a Null Field State

Koichi Hirano, Kiyoshi Kawabata, Zen Komiya +1

We investigate whether or nor it is possible to find a scalar field model or models that are capable of explaining simultaneously the observed - relation given by the 2dF Gal…

astro-ph.CO2010★ 4 cited

Observational Constraints on Phantom Crossing DGP Gravity

Koichi Hirano, Zen Komiya

We study the observational constraints on the Phantom Crossing DGP model. We demonstrate that the crossing of the phantom divide does not occur within the framework of the original…

astro-ph.CO2010

Phantom Crossing DGP Gravity

Koichi Hirano, Zen Komiya

We propose a phantom crossing Dvali--Gabadadze--Porrati (DGP) model. In our model, the effective equation of state of the DGP gravity crosses the phantom divide line. We demonstrat…