activity
19942017
most citedEvolution of cosmological perturbations in a stage dominated by an oscillatory scalar field

73 citations · 172 across the 9 of their papers we have counts for

collaborators

9 papers

gr-qc2017

Construction and applications of the manifestly gauge invariant expressions of the solutions of the cosmological perturbation theory

Takashi Hamazaki

After giving how to construct the gauge invariant perturbation variable in an arbitrarily high order and in the arbitrary background spacetime, we consider the manifestly gauge inv…

astro-ph.CO2011★ 4 cited

Manifestly gauge invariant theory of the nonlinear cosmological perturbations in the leading order of the gradient expansion

Takashi Hamazaki

In the full nonlinear cosmological perturbation theory in the leading order of the gradient expansion, all the types of the gauge invariant perturbation variables are defined. The…

astro-ph2008★ 14 cited

Long wavelength limit of evolution of nonlinear cosmological perturbations

Takashi Hamazaki

In the general matter composition where the multiple scalar fields and the multiple perfect fluids coexist, in the leading order of the gradient expansion, we construct all of the…

astro-ph2007★ 5 cited

Long wavelength limit of evolution of cosmological perturbations in the universe where scalar fields and fluids coexist

Takashi Hamazaki

We present the LWL formula which represents the long wavelengh limit of the solutions of evolution equations of cosmological perturbations in terms of the exactly homogeneous solut…

gr-qc2004★ 5 cited

Evolution of Cosmological Perturbations in the Universe dominated by Resonant Scalar Fields

Takashi Hamazaki

Recently a Hamiltonian formulation for the evolution of the universe dominated by multiple oscillatory scalar fields was developed by the present author and was applied to the inve…

gr-qc2003★ 5 cited

Evolution of Cosmological Perturbations in the Universe dominated by Multiple Scalar Fields

Takashi Hamazaki

By efforts of several authors, it is recently established that the dynamical behavior of the cosmological perturbation on superhorizon scales is well approximated in terms of that…