Dynamical Formation and Evolution of Neutron Star and Black Hole Binaries in Globular Clusters

Colpi, M.; Devecchi, B.

doi:10.1007/978-1-4020-9264-0_5

Cited by 2 publications

(2 citation statements)

References 95 publications

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“…After its birth, GTR went to fertilize and seed, directly as well as indirectly, many branches of disparate sciences as mathematics [225][226][227][228][229][230], metrology [231][232][233][234], geodesy [236][237][238], geophysics [239][240][241], astronomy [242][243][244][245][246][247], astrophysics [248][249][250][251][252], cosmology [181,[253][254][255], not to say about the exquisite technological spin-off [256][257][258][259][260][261][262][263][264][265][266][267][268][269][270] due to the long-lasting efforts required to put to the test various key predictions of the theory…”

Section: Discussionmentioning

confidence: 99%

Editorial for the Special Issue 100 Years of Chronogeometrodynamics: The Status of the Einstein’s Theory of Gravitation in Its Centennial Year

Iorio

2015

Universe

133

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The present Editorial introduces the Special Issue dedicated by the journal Universe to the General Theory of Relativity, the beautiful theory of gravitation of Einstein, a century after its birth. It reviews some of its key features in a historical perspective, and, in welcoming distinguished researchers from all over the world to contribute it, some of the main topics at the forefront of the current research are outlined. general relativity and gravitation; classical general relativity; gravitational waves; quantum gravity; cosmology; experimental studies of gravity PACS classifications: 04.; 04.20.-q; 04.30.-w; 04.60.-m; 98.80.-k; 04.80.-y

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Section: Discussionmentioning

confidence: 99%

Editorial for the Special Issue 100 Years of Chronogeometrodynamics: The Status of the Einstein’s Theory of Gravitation in Its Centennial Year

Iorio

2015

Universe

133

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“…In April 1973 (and therefore before the discovery of the first binary pulsar) G S Bisnovatyi-Koyan and B V Komberg had already suggested that some pulsating x-ray sources in binaries may later in their life, after their massive companion stars have exploded as supernovas, become observable as binary radio pulsars [89]. For an authoritative review of the formation and evolution of relativistic binaries, see the contribution of E P J van den Heuvel to the book [90].…”

Section: Binary Pulsars and Astrophysicsmentioning

confidence: 99%

1974: the discovery of the first binary pulsar

Damour

2015

Class. Quantum Grav.

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The 1974 discovery, by Russell A. Hulse and Joseph H. Taylor, of the first binary pulsar PSR B1913+16, opened up new possibilities for the study of relativistic gravity. PSR B1913+16, as well as several other binary pulsars, provided direct observational proofs that gravity propagates at the velocity of light and has a quadrupolar structure. Binary pulsars also provided accurate tests of the strong-field regime of relativistic gravity. General Relativity has passed all the binary pulsar tests with flying colors. The discovery of binary pulsars had also very important consequences for astrophysics: accurate measurement of neutron star masses, improved understanding of the possible evolution scenarios for the coevolution of binary stars, proof of the existence of binary neutron stars emitting gravitational waves for hundreds of millions of years, before coalescing in catastrophic events radiating intense gravitational-wave signals, and probably leading also to important emissions of electromagnetic radiation and neutrinos. This article reviews the history of the discovery of the first binary pulsar, and describes both its immediate impact, and its longer-term effect on theoretical and experimental studies of relativistic gravity.

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Dynamical Formation and Evolution of Neutron Star and Black Hole Binaries in Globular Clusters

Cited by 2 publications

References 95 publications

Editorial for the Special Issue 100 Years of Chronogeometrodynamics: The Status of the Einstein’s Theory of Gravitation in Its Centennial Year

Editorial for the Special Issue 100 Years of Chronogeometrodynamics: The Status of the Einstein’s Theory of Gravitation in Its Centennial Year

1974: the discovery of the first binary pulsar

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