The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where G. D. Hammond sits on this spectrum.
This scientist: 381 publications — 34th percentile
34% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 1,469 publications or more.
The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where G. D. Hammond sits on this spectrum.
This scientist: 124 D-Index — 82nd percentile
82% of scientists in this discipline score the same or lower.
The last bar groups every scientist with 185 D-Index or more.
His main research concerns Astrophysics, LIGO, Gravitational wave, Binary black hole and Astronomy. Astrophysics and General relativity are commonly linked in his work. His LIGO research incorporates themes from Stars, Galaxy, Mass distribution and Neutron star.
His research in Gravitational wave intersects with topics in Observatory and Detector. His study looks at the relationship between Binary black hole and topics such as Gravitational wave background, which overlap with Cosmic background radiation, De Sitter universe and Age of the universe. His Kilonova study combines topics in areas such as Gravastar and Primordial black hole.
The scientist’s investigation covers issues in Gravitational wave, LIGO, Astrophysics, Astronomy and Neutron star. His Gravitational wave study incorporates themes from Amplitude, Pulsar, Detector and Sky. His work on GW151226 and Gravitational-wave astronomy as part of general LIGO study is frequently connected to Population, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them.
Binary black hole, Gamma-ray burst, Black hole, Redshift and Gravitational-wave observatory are among the areas of Astrophysics where the researcher is concentrating his efforts. His Binary black hole study combines topics from a wide range of disciplines, such as General relativity and Mass distribution. His Neutron star research incorporates elements of Stars, Supernova and Dimensionless quantity.
His primary scientific interests are in LIGO, Gravitational wave, Astrophysics, Neutron star and Binary black hole. His LIGO study contributes to a more complete understanding of Astronomy. The Gravitational wave study combines topics in areas such as Detector, Sky, Magnetar, Pulsar and Coincident.
The concepts of his Astrophysics study are interwoven with issues in Amplitude and General relativity. His Neutron star study integrates concerns from other disciplines, such as Coalescence, Cosmology, Mass ratio and LIGO Scientific Collaboration. His work in Binary black hole is not limited to one particular discipline; it also encompasses Gravitational wave background.
His primary areas of study are LIGO, Astrophysics, Gravitational wave, Neutron star and Binary black hole. His studies in LIGO integrate themes in fields like Amplitude, Galaxy, Cosmic string and Superposition principle. His work on Black hole, Stars and Mass distribution as part of general Astrophysics research is frequently linked to Population, thereby connecting diverse disciplines of science.
His Gravitational wave study is concerned with the field of Astronomy as a whole. His research integrates issues of Coalescence, Gamma-ray burst, Tests of general relativity and LIGO Scientific Collaboration in his study of Neutron star. His study explores the link between Binary black hole and topics such as Redshift that cross with problems in Supernova.
B. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott
B. P. Abbott;R. Abbott
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
M. Punturo;M. Abernathy;F. Acernese;B. Allen
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy
B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy
B. P. Abbott;R. Abbott
J. Abadie;B. P. Abbott;R. Abbott;M. Abernathy
J. Abadie;B. P. Abbott
B. P. Abbott;R. Abbott
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese
B. P. Abbott;R. Abbott
J. Aasi;J. Abadie;B. P. Abbott;R. Abbott
J. Aasi;J. Abadie;B. P. Abbott;R. Abbott
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