Constraining the non-Einsteinian polarizations of gravitational waves by pulsar timing array
- 27 March 2019
- journal article
- research article
- Published by Springer Science and Business Media LLC in Science China Physics Mechanics and Astronomy
- Vol. 62 (7), 970411
- https://doi.org/10.1007/s11433-018-9340-6
Abstract
No abstract availableKeywords
This publication has 23 references indexed in Scilit:
- Detection and localization of continuous gravitational waves with pulsar timing arrays: the role of pulsar termsMonthly Notices of the Royal Astronomical Society, 2016
- Observation of Gravitational Waves from a Binary Black Hole MergerPhysical Review Letters, 2016
- Projected constraints on Lorentz-violating gravity with gravitational wavesPhysical Review D, 2015
- GRAVITATIONAL WAVE HOTSPOTS: RANKING POTENTIAL LOCATIONS OF SINGLE-SOURCE GRAVITATIONAL WAVE EMISSIONThe Astrophysical Journal, 2014
- Optimal strategies for gravitational wave stochastic background searches in pulsar timing dataPhysical Review D, 2009
- Pulsar searches and timing with the square kilometre arrayAstronomy & Astrophysics, 2008
- Pulsar Timing as a Probe of Non‐Einsteinian Polarizations of Gravitational WavesThe Astrophysical Journal, 2008
- The Confrontation between General Relativity and ExperimentLiving Reviews in Relativity, 2006
- Pulsar timing measurements and the search for gravitational wavesThe Astrophysical Journal, 1979