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Primordial black holes and their gravitational-wave signatures. [PDF]

open access: yesLiving Rev Relativ, 2023
In the recent years, primordial black holes (PBHs) have emerged as one of the most interesting and hotly debated topics in cosmology. Among other possibilities, PBHs could explain both some of the signals from binary black hole mergers observed in ...
Bagui E   +20 more
europepmc   +5 more sources

Correlation between birefringence and absorption mapping in large-size Sapphire substrates for gravitational-wave interferometry [PDF]

open access: yesScientific Reports, 2023
In high-sensitive laser interferometers, such as the gravitational-wave detector KAGRA, ultra-high-quality mirrors are essential. In the case of KAGRA, where cavity mirrors are cooled down to 20 K, large-size Sapphire crystals are used as the substrate ...
Simon Zeidler   +4 more
doaj   +2 more sources

Core Payload of the Space Gravitational Wave Observatory: Inertial Sensor and Its Critical Technologies [PDF]

open access: yesSensors
Since Einstein’s prediction regarding the existence of gravitational waves was directly verified by the ground-based detector Advanced LIGO, research on gravitational wave detection has garnered increasing attention.
Shaoxin Wang   +10 more
doaj   +2 more sources

Testing general relativity with gravitational-wave catalogs: The insidious nature of waveform systematics [PDF]

open access: yesiScience, 2021
Summary: Gravitational-wave observations of binary black holes allow new tests of general relativity (GR) to be performed on strong, dynamical gravitational fields.
Christopher J. Moore   +3 more
doaj   +2 more sources

Design method for the structure of a gravitational wave detection telescope with low TTL noise [PDF]

open access: yesScientific Reports
As a critical payload of the gravitational wave detection interferometry system, the tilt-to-length (TTL) noise has a significant influence on the detection accuracy of the interferometry system.
Sijun Fang   +8 more
doaj   +2 more sources

The NANOGrav 15 yr Data Set: Evidence for a Gravitational-wave Background [PDF]

open access: yesAstrophysical Journal Letters, 2023
We report multiple lines of evidence for a stochastic signal that is correlated among 67 pulsars from the 15 yr pulsar timing data set collected by the North American Nanohertz Observatory for Gravitational Waves.
G. Agazie   +113 more
semanticscholar   +1 more source

The second data release from the European Pulsar Timing Array. III. Search for gravitational wave signals [PDF]

open access: yesAstronomy & Astrophysics, 2023
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

Search for an Isotropic Gravitational-wave Background with the Parkes Pulsar Timing Array [PDF]

open access: yesAstrophysical Journal Letters, 2023
Pulsar timing arrays aim to detect nanohertz-frequency gravitational waves (GWs). A background of GWs modulates pulsar arrival times and manifests as a stochastic process, common to all pulsars, with a signature spatial correlation.
D. Reardon   +28 more
semanticscholar   +1 more source

Searching for the Nano-Hertz Stochastic Gravitational Wave Background with the Chinese Pulsar Timing Array Data Release I [PDF]

open access: yesResearch in Astronomy and Astrophysics, 2023
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 NANOGrav 15 yr Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational-wave Background [PDF]

open access: yesAstrophysical Journal Letters, 2023
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

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