«We have observed — on the 4th of January, 2017 — another massive black hole - black hole
binary coalescence; the in - spiral and merging of black holes 20 and 30 times the mass of our sun,» Dave Shoemaker, a senior research scientist who works at Massachusetts Institute of Technology (MIT) and the spokesperson for the LIGO Scientific Collaboration, told reporters during a special news briefing on Wednesday (May 31).
In the last years he has focused in the emerging area of Gravitational Wave Astronomy, which consists in the detection and analysis of gravitational radiation emitted by cosmic sources (core collapse supernovae, compact
binary coalescence, etc.).
Hanna has served as co-chair of the Compact
Binary Coalescence Group of the Laser Interferometer Gravitational Wave Observatory (LIGO), and is one of the primary data analysts involved in this research.
Not exact matches
GW170814: A three - detector observation of gravitational waves from a
binary black hole
coalescence.
«They are the most complete and accurate models of
binary black - hole
coalescence.»
On July 6, Lazzati's team of theorists had published a paper predicting that, contrary to earlier estimates by the astrophysics community, short gamma - ray bursts associated with the gravitational emission of
binary neutron star
coalescence could be detected — whether or not the gamma - ray burst was pointing at Earth.
«All observations until the last one were from the
coalescence of
binary black hole systems,» Lazzati said.
These findings were published in Physical Review Letters the week of October 11 in a paper titled «Formation and
Coalescence of Cosmological Supermassive - Black - Hole
Binaries in Supermassive - Star Collapse.»
GW151226: Observation of Gravitational Waves from a 22 - Solar - mass
Binary Black Hole
Coalescence.
The research paper, «GW151226: Observation of Gravitational Waves from a 22 Solar - mass
Binary Black Hole
Coalescence,» by the LIGO Scientific Collaboration and the Virgo Collaboration, has been accepted for publication in the journal Physical Review Letters.
More information: GW170608: Observation of a 19 - solar - mass
Binary Black Hole
Coalescence, arXiv: 1711.05578 [astro - ph.
A paper describing the newly confirmed observation, «GW170608: Observation of a 19 - solar - mass
binary black hole
coalescence,» authored by the LIGO Scientific Collaboration and the Virgo Collaboration has been submitted to The Astrophysical Journal Letters and is available to read on the arXiv.
The inferred source of both events is the
coalescence of a stellar mass
binary black hole system at cosmological distances.