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Second-order tensor modes induced by nonlinear gravity are a key component of the cosmological background of gravitational waves. A detection of this background would allow us to probe the primordial power spectrum at otherwise inaccessible…

广义相对论与量子宇宙学 · 物理学 2022-10-05 Atsuhisa Ota , Hayley J. Macpherson , William R. Coulton

The transverse-traceless gauge condition is an important concept in the theory of gravitational wave. It is well known that vacuum is one of the key conditions to guarantee the existence of the transverse-traceless gauge. Although it is…

广义相对论与量子宇宙学 · 物理学 2024-10-08 Yadong Xue , Xiaokai He , Zhoujian Cao

In this paper, we investigate gravitational waves beyond the linear approximation, focusing on second-order contributions sourced by linearized waves in the transverse-traceless (TT) gauge. A general spacetime metric is constructed, and…

广义相对论与量子宇宙学 · 物理学 2025-05-06 M. A. Misyura

To simplify a number of considerations in the weak field approximation, including the determination of the response of interferometric gravitational wave detectors, the "transverse traceless" (TT) gauge is often used. While the…

广义相对论与量子宇宙学 · 物理学 2009-12-02 Istvan Racz

A tensor-type cosmological perturbation, defined as a transverse and traceless spatial fluctuation, is often interpreted as the gravitational waves. While decoupled from the scalar-type perturbations in linear order, the tensor…

宇宙学与河外天体物理 · 物理学 2017-06-28 Jai-chan Hwang , Donghui Jeong , Hyerim Noh

There is currently no rigorous definition of gravitational wave strain at second order in cosmological perturbation theory. The usual association of gravitational waves with transverse and traceless fluctuations of the metric on spatial…

广义相对论与量子宇宙学 · 物理学 2026-01-05 Guillem Domènech , Shi Pi , Ao Wang

We compute the second-order matching conditions for tensor metric perturbations at an abrupt change in the equation of state. For adiabatic perturbations on large scales the matching hypersurface coincides with a uniform-density…

宇宙学与河外天体物理 · 物理学 2013-05-29 Frederico Arroja , Hooshyar Assadullahi , Kazuya Koyama , David Wands

We consider in detail the problem of gauge dependence that exists in relativistic perturbation theory, going beyond the linear approximation and treating second and higher order perturbations. We first derive some mathematical results…

广义相对论与量子宇宙学 · 物理学 2009-10-28 Marco Bruni , Sabino Matarrese , Silvia Mollerach , Sebastiano Sonego

Gauge invariant treatments of the second order cosmological perturbation in a four dimensional homogeneous isotropic universe filled with the perfect fluid are completely formulated without any gauge fixing. We derive all components of the…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Kouji Nakamura

We consider the evolution of relativistic perturbations in the Einstein-de Sitter cosmological model, including second-order effects. The perturbations are considered in two different settings: the widely used synchronous gauge and the…

天体物理学 · 物理学 2009-10-30 S. Matarrese , S. Mollerach , M. Bruni

The investigation of the transverse effect of gravitational waves (GWs) could constitute a further tool to discriminate among several relativistic theories of gravity on the ground. After a review of the TT gauge, the transverse effect of…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Christian Corda

This paper discusses the gauge issue touching the gravitational waves induced at the second order by the scalar modes of cosmological perturbations. These waves are known to depend on the gauge used for their calculation. In this paper, we…

广义相对论与量子宇宙学 · 物理学 2023-09-27 Vincent Comeau

Except for the presence of gravitational wave source term, the relativistic perturbation equations of a zero-pressure irrotational fluid in a flat Friedmann world model coincide exactly with the Newtonian ones to the second order in…

天体物理学 · 物理学 2009-11-11 J. Hwang , H. Noh

The cosmological stochastic gravitational-wave background produced by the mildly non-linear evolution of density fluctuations is analyzed, in the frame of an Einstein-de Sitter model, by means of a fully relativistic perturbation expansion…

天体物理学 · 物理学 2007-05-23 Sabino Matarrese , Silvia Mollerach

Along the general framework of the gauge invariant perturbation theory developed in the papers [K. Nakamura, Prog. Theor. Phys. {\bf 110} (2003), 723; {\it ibid}, {\bf 113} (2005), 481.], we formulate the second order gauge invariant…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Kouji Nakamura

We investigate the gauge invariance of the second order gravitational waves induced by the first order scalar perturbations by following the Lie derivative method. It is shown explicitly that the second order gravitational waves are gauge…

广义相对论与量子宇宙学 · 物理学 2020-09-30 Zhe Chang , Sai Wang , Qing-Hua Zhu

Gauge-invariant treatments of the second-order cosmological perturbation in a four dimensional homogeneous isotropic universe are formulated without any gauge fixing. We have derived the Einstein equations in the case of the single perfect…

广义相对论与量子宇宙学 · 物理学 2009-01-27 Kouji Nakamura

We study cosmological gravitational waves generated during inflation under the influence of a decaying cosmological "constant", in the Transverse-Traceless (TT) gauge. In our approach we consider a non-perturbative contribution of the…

广义相对论与量子宇宙学 · 物理学 2012-02-27 Reyes Luz Marina , Moreno Claudia , Madriz Aguilar Jose Edgar

In this review we look into the gauge-dependence of scalar-induced gravitational waves (SIGWs) that are second-order tensors produced by first-order scalar-modes. The method includes deriving the background, first- and second-order Einstein…

广义相对论与量子宇宙学 · 物理学 2025-06-27 Anjali Abirami Kugarajh

The aim of this paper is to show the gauge-invariance on the response of interferometers to gravitational waves (GWs). In this process, after a review of results on the Tranverse-Traceless (TT) gauge, where, in general, the theoretical…

广义相对论与量子宇宙学 · 物理学 2011-03-25 Christian Corda
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