Friedrich Schiller University Jena
Germany
Sebastiano Bernuzzi mainly investigates Astrophysics, Gravitational wave, Neutron star, LIGO and Kilonova. His work on Binary black hole, Mass ratio, Black hole and Supernova as part of general Astrophysics study is frequently linked to Cosmic string, bridging the gap between disciplines. His Gravitational wave study combines topics in areas such as General relativity, Magnetar, Order of magnitude and Gravitation.
His work on X-ray binary as part of general Neutron star study is frequently connected to Nuclear matter, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them. His X-ray binary research integrates issues from GW151226 and Stellar black hole. His LIGO research is multidisciplinary, relying on both Stars, Mass distribution, Dimensionless quantity and Coalescence.
Sebastiano Bernuzzi mainly focuses on Gravitational wave, Neutron star, Astrophysics, LIGO and Numerical relativity. In the field of Gravitational wave, his study on Binary black hole overlaps with subjects such as Waveform. Particularly relevant to X-ray binary is his body of work in Neutron star.
Astrophysics is a component of his Kilonova, Mass ratio, Ejecta, Redshift and Stars studies. Sebastiano Bernuzzi combines subjects such as Light curve and Equation of state with his study of Ejecta. Within one scientific family, he focuses on topics pertaining to Gamma-ray burst under LIGO, and may sometimes address concerns connected to Fermi Gamma-ray Space Telescope.
His primary scientific interests are in Gravitational wave, Astrophysics, Neutron star, LIGO and Binary black hole. His studies in Gravitational wave integrate themes in fields like Amplitude, Statistical physics and Detector. His Astrophysics research is multidisciplinary, incorporating elements of Coalescence and Dimensionless quantity.
His work carried out in the field of Neutron star brings together such families of science as Neutrino, Equation of state, Numerical relativity, Mass distribution and Kilonova. His LIGO research incorporates elements of Gamma-ray burst, Compact star, Pulsar and Sky. His Binary black hole study which covers Angular momentum that intersects with Rotating black hole, Computational physics and Test particle.
His main research concerns LIGO, Gravitational wave, Astrophysics, Neutron star and Black hole. His biological study spans a wide range of topics, including Stars and Mass ratio. His study in Mass ratio is interdisciplinary in nature, drawing from both Theory of relativity and Multipole expansion.
His research in Gravitational wave intersects with topics in Nuclear astrophysics and Observable. The Astrophysics study combines topics in areas such as General relativity and Radiation. His research on Neutron star also deals with topics like
This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.
GW170817: observation of gravitational waves from a binary neutron star inspiral
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese.
Physical Review Letters (2017)
GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
B. P. Abbott;R. Abbott.
Physical Review X (2019)
GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs
B. P. Abbott;R. Abbott.
arXiv: High Energy Astrophysical Phenomena (2018)
GW170817: Measurements of Neutron Star Radii and Equation of State.
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese.
Physical Review Letters (2018)
GW190814: Gravitational Waves from the Coalescence of a 23 M$_\odot$ Black Hole with a 2.6 M$_\odot$ Compact Object
R. Abbott;T. D. Abbott.
arXiv: High Energy Astrophysical Phenomena (2020)
GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim 3.4 M_{\odot}$
B. P. Abbott;R. Abbott.
arXiv: High Energy Astrophysical Phenomena (2020)
Binary Black Hole Population Properties Inferred from the First and Second Observing Runs of Advanced LIGO and Advanced Virgo
B. P. Abbott;R. Abbott.
arXiv: High Energy Astrophysical Phenomena (2018)
GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M O
B. P. Abbott;R. Abbott;T. D. Abbott;S. Abraham.
The Astrophysical Journal (2020)
Properties of the binary neutron star merger GW170817
B. P. Abbott;R. Abbott.
arXiv: General Relativity and Quantum Cosmology (2018)
Properties of the Binary Neutron Star Merger GW170817
B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese.
Physical Review X (2019)
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