Estimating the sensitivity of pulsar timing arrays

DOI10.1088/0264-9381/32/5/055004zbMath1309.83041arXiv1406.5199OpenAlexW3102350337WikidataQ59756474 ScholiaQ59756474MaRDI QIDQ5245659

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Publication date: 14 April 2015

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1406.5199

zbMATH Keywords

black holesgravitational wavespulsar timing

Mathematics Subject Classification ID

Black holes (83C57) Applications of statistics to physics (62P35) Gravitational waves (83C35)

Related Items (5)

Gravitational shine of dark domain walls ⋮ Primordial scalar gravitational waves produced at the QCD phase transition due to the trace anomaly ⋮ Quasinormal modes of Dirac field in \(2 + 1\) dimensional gravitational wave background ⋮ Cosmological phase transitions in warped space: gravitational waves and collider signatures ⋮ Scalar gravitational wave signals from core collapse in massive scalar–tensor gravity with triple-scalar interactions

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