Gravitational wave detector response in terms of spacetime Riemann curvature
, 2013 Gravitational wave detectors are typically described as responding to gravitational wave metric perturbations, which are gauge-dependent and --- correspondingly --- unphysical quantities.
Finn, Lee Samuel, Koop, Michael J.
core +1 more source
Compact Binaries in Star Clusters II - Escapers and Detection Rates [PDF]
, 2010 We use a self-consistent Monte Carlo treatment of stellar dynamics to investigate black hole binaries that are dynamically ejected from globular clusters to determine if they will be gravitational wave sources.
Benacquista, M. J. +3 more
core +3 more sources
Data Transmission Analysis and Communication Scheme Design for TianQin Mission
IEEE AccessCompared with ground-based gravitational wave detection, space-based gravitational wave detection has become a research hotspot because of its abundant wave sources.
Zhaoxiang Yi, Lin Sun, Meng Jiang
doaj +1 more source
Application of the Hilbert-Huang Transform to the Search for Gravitational Waves [PDF]
, 2007 We present the application of a novel method of time-series analysis, the Hilbert-Huang Transform, to the search for gravitational waves. This algorithm is adaptive and does not impose a basis set on the data, and thus the time-frequency decomposition it
Camp, Jordan B. +2 more
core +3 more sources
Can the Gravitational Wave Background from Inflation be Detected Locally?
, 1993 The Cosmic Background Explorer (COBE) detection of microwave background anisotropies may contain a component due to gravitational waves generated by inflation.
A. D. Linde +32 more
core +2 more sources
Detection methods for non-Gaussian gravitational wave stochastic backgrounds [PDF]
, 2002 We address the issue of finding an optimal detection method for a discontinuous or intermittent gravitational wave stochastic background. Such a signal might sound something like popcorn popping. We derive an appropriate version of the maximum likelihood
A. Abramovici +26 more
core +2 more sources
Detecting a gravitational-wave background with next-generation space interferometers [PDF]
Physical Review D, 2006 19 pages, 6 figures, references added, typos ...
Kudoh, Hideaki +3 more
openaire +2 more sources
Temperature stability in the sub-milliHertz band with LISA Pathfinder [PDF]
, 2019 This article has been accepted for publication in "Monthly notices of the royal astronomical society" published by Oxford University Press.LISA Pathfinder (LPF) was a technology pioneering mission designed to test key technologies required for ...
Armano, M. +6 more
core +2 more sources
Correlation analysis of stochastic gravitational wave background around 0.1-1Hz [PDF]
, 2006 We discuss prospects for direct measurement of stochastic gravitational wave background around 0.1-1Hz with future space missions. It is assumed to use correlation analysis technique with the optimal TDI variables for two sets of LISA-type ...
A. A. Starobinsky +3 more
core +2 more sources
Gravitational Wave Detection and Fundamental Physics in Space: Foreword
, 2020 This article is a foreword for the special issue on Gravitational Wave Detection and Fundamental Physics in Space for International Journal of Physics D. In the foreword, we review briefly the history of the development of mission concepts and projects for the gravitational wave detection in space together with fundamental physics missions.
Iyer, Bala, Ni, Wei-Tou
openaire +2 more sources