The following sections are included:Physics of Gravitational Wave GenerationIn the Footsteps of Heinrich Hertz?Observation of Gravitational Wave EmissionAstronomical Sources of Gravitational Waves Physics of Gravitational Wave Generation In the Footsteps of Heinrich Hertz? Observation of Gravitational Wave ...
China has launched a pair of satellites which will watch for the electromagnetic counterparts that are emitted along with gravitational waves. These signals will be relayed quickly to the ground, helping narrow the area of sky scientists need to search t
Gravitational wave detectors in space, particularly the LISA project, can study a rich variety of astronomical systems whose gravitational radiation is not detectable from the ground, because it is emitted in the low-frequency gravitational wave band (0.1 mHz to 1 Hz) that is inaccessible to groun...
Sources of Gravitational Waves and their detectability Published in print B Schutz 被引量: 0发表: 1993年 Short‐period AM CVn systems as optical, X‐ray and gravitational‐wave sources We model the population of AM CVn systems in the Galaxy and discuss the detectability of these systems with ...
gravitational collapsereviewsNo Abstract available for this article.doi:10.1038/328204a0HunsuckerRobert D.Nature Publishing Group UKNatureHunsuker R.D., 1987. The sources of gravity waves. Nature , 328 , 204-205.Hunsucker, R. D.: The Sources of gravity waves, Nature, 328, 204- 205, 1987....
Computer calculations model the gravitational waves, which LIGO measured in the two observation runs O1 and O2, as well as the black holes, which radiate the waves. The film shows the event horizons of the black holes and the corresponding gravitational wave signal below. ...
C. Lousto and N. G. Sanchez, "Gravitational shock waves generated by extended sources: ultrarelativistic cosmic strings, monopoles and domain walls," Nuclear Physics B, vol. 355, pp. 231-249, 1991.C. O. Lousto´, N. Sa´nchez, "Gravitational shock waves generated by extended sources...
LISA is a spaceborne laser interferometer for the detection and observation of gravitational waves, currently under study by ESA. A brief introduction of the main features of this detector, concentrating on its one-year orbital motion around the Sun is given. The amplitude as well as the phase ...
Several scenarios were suggested for the origins of gravitational-wave (GW) sources from mergers of stellar binary black holes (BBHs). Here we propose a novel origin through catalyzed formation of GW sources from ultra-wide binaries in the field. Such binaries experience perturbations from random ...
the frequency evolution of a source in a targetted search. PACS numbers: 03.70.+k, 98.80.Cq I. INTRODUCTION The detection of periodic sources of gravitational waves using the LIGO, or similar, gravitational-wave detectors, is seemingly the most straightforward data analysis prob- lem facing gravi...