The primordial perturbations will inevitably generate higher order
perturbations. We study the second order scalar perturbations generated by the
primordial curvature and tensor perturbations in the radiation-dominated era.
After presenting all the possible second-order source terms, we obtain the
explicit expressions of the kernel functions and the power spectra of the
second order scalar perturbations. The contributions from the initial
second-order perturbations are considered. We calculate the power spectra of
second order scalar perturbations for different tensor-to-scalar ratio $r$.
Description
Second order scalar perturbations induced by primordial curvature and tensor perturbations
%0 Generic
%1 changa2022second
%A Changa, Zhe
%A Tinga, Kung-Yu
%A Zhang, Xukun
%A Zhou, Jing-Zhi
%D 2022
%K library
%T Second order scalar perturbations induced by primordial curvature and
tensor perturbations
%U http://arxiv.org/abs/2211.11948
%X The primordial perturbations will inevitably generate higher order
perturbations. We study the second order scalar perturbations generated by the
primordial curvature and tensor perturbations in the radiation-dominated era.
After presenting all the possible second-order source terms, we obtain the
explicit expressions of the kernel functions and the power spectra of the
second order scalar perturbations. The contributions from the initial
second-order perturbations are considered. We calculate the power spectra of
second order scalar perturbations for different tensor-to-scalar ratio $r$.
@misc{changa2022second,
abstract = {The primordial perturbations will inevitably generate higher order
perturbations. We study the second order scalar perturbations generated by the
primordial curvature and tensor perturbations in the radiation-dominated era.
After presenting all the possible second-order source terms, we obtain the
explicit expressions of the kernel functions and the power spectra of the
second order scalar perturbations. The contributions from the initial
second-order perturbations are considered. We calculate the power spectra of
second order scalar perturbations for different tensor-to-scalar ratio $r$.},
added-at = {2022-11-23T06:59:09.000+0100},
author = {Changa, Zhe and Tinga, Kung-Yu and Zhang, Xukun and Zhou, Jing-Zhi},
biburl = {https://www.bibsonomy.org/bibtex/22aa3d08c50dd37f8e0e4170454615c40/gpkulkarni},
description = {Second order scalar perturbations induced by primordial curvature and tensor perturbations},
interhash = {90c0d578820b6d6a687c5895cbd0184c},
intrahash = {2aa3d08c50dd37f8e0e4170454615c40},
keywords = {library},
note = {cite arxiv:2211.11948},
timestamp = {2022-11-23T06:59:09.000+0100},
title = {Second order scalar perturbations induced by primordial curvature and
tensor perturbations},
url = {http://arxiv.org/abs/2211.11948},
year = 2022
}