Searching for the Nano-Hertz Stochastic Gravitational Wave Background with the Chinese Pulsar Timing Array Data Release I [PDF]
Observing and timing a group of millisecond pulsars with high rotational stability enables the direct detection of gravitational waves (GWs). The GW signals can be identified from the spatial correlations encoded in the times-of-arrival of widely spaced ...
Heng Xu +26 more
semanticscholar +1 more source
The second data release from the European Pulsar Timing Array. III. Search for gravitational wave signals [PDF]
We present the results of the search for an isotropic stochastic gravitational wave background (GWB) at nanohertz frequencies using the second data release of the European Pulsar Timing Array (EPTA) for 25 millisecond pulsars and a combination with the ...
J. Antoniadis +97 more
semanticscholar +1 more source
The NANOGrav 15 yr Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational-wave Background [PDF]
The NANOGrav 15 yr data set shows evidence for the presence of a low-frequency gravitational-wave background (GWB). While many physical processes can source such low-frequency gravitational waves, here we analyze the signal as coming from a population of
G. Agazie +113 more
semanticscholar +1 more source
Scalar-induced gravitational wave interpretation of PTA data: the role of scalar fluctuation propagation speed [PDF]
Pulsar timing arrays gathered evidence of the presence of a gravitational wave background around nHz frequencies. If the gravitational wave background was induced by large and Gaussian primordial fluctuations, they would then produce too many sub-solar ...
S. Balaji +2 more
semanticscholar +1 more source
Tolerance Analysis of Test Mass Alignment Errors for Space-Based Gravitational Wave Detection. [PDF]
Ke J +6 more
europepmc +3 more sources
Gravitational Lensing of Continuous Gravitational Waves [PDF]
Continuous gravitational waves are analogous to monochromatic light and could therefore be used to detect wave effects such as interference or diffraction. This would be possible with strongly lensed gravitational waves. This article reviews and summarises the theory of gravitational lensing in the context of gravitational waves in two different ...
Marek Biesiada, Sreekanth Harikumar
openaire +3 more sources
Review of the Advanced LIGO Gravitational Wave Observatories Leading to Observing Run Four [PDF]
Gravitational waves from binary black hole and neutron star mergers are being regularly detected. As of 2021, 90 confident gravitational wave detections have been made by the LIGO and Virgo detectors.
C. Cahillane, G. Mansell
semanticscholar +1 more source
On the Evidence for a Common-spectrum Process in the Search for the Nanohertz Gravitational-wave Background with the Parkes Pulsar Timing Array [PDF]
A nanohertz-frequency stochastic gravitational-wave background can potentially be detected through the precise timing of an array of millisecond pulsars.
B. Goncharov +28 more
semanticscholar +1 more source
Gravitational Fields and Gravitational Waves [PDF]
Abstract For any object with finite velocity, the relative velocity between them will affect the effect between them. This effect can be called the chasing effect (general Doppler effect). LIGO discovered gravitational waves and measured the speed of gravitational waves equal to the speed of light c. Gravitational waves are generated due to the
openaire +14 more sources
The NANOGrav 12.5 yr Data Set: Search for an Isotropic Stochastic Gravitational-wave Background [PDF]
We search for an isotropic stochastic gravitational-wave background (GWB) in the 12.5 yr pulsar-timing data set collected by the North American Nanohertz Observatory for Gravitational Waves.
Z. Arzoumanian +60 more
semanticscholar +1 more source

