Third Gravitational Wave Detection Offers New Insight into Black Holes

Credit: LSC/OzGrav

The research is published in Physical Review Letters.

ANU is one of the leading Australian institutions supporting the Laser Interferometer Gravitational-wave Observatory (LIGO) project.

Professor Susan Scott from the ANU Research School of Physics and Engineering (RSPE) said the discovery provided the first evidence that black holes in binary systems may not be aligned.

“This means that the two black holes could be spinning in opposite directions, which provides a tantalising clue as to how the binary system may have formed,” said Professor Scott, who is also a Chief Investigator of the ARC Centre of Excellence for Gravitational Wave Discovery (OzGrav).

“It’s possible this is a binary system of black holes that formed in the early Universe and contributes significantly to the dark matter in the cosmos.

“This heavy stellar-mass binary black hole system was at a much greater distance than the first two gravitational wave events, at some three billion light years away.

“This discovery highlights the need to continue improving the sensitivity of our detectors to see further and further out into the Universe.”

ANU scientists designed systems to improve the duty cycle of the LIGO detectors so that more time can be spent searching for gravitational waves.

Credit: SXS

Researchers Dr Bram Slagmolen and Dr Robert Ward from RSPE are working on further improvements to the instruments so the team will be able to detect other types of events such as gravitational waves radiated by neutron stars, which are made when giant stars explode and their cores collapse.

“We hope to detect continuous gravitational waves from neutron stars, which is good motivation to develop advanced technologies including quantum-squeezing optical devices to search for these fainter sources of gravitational waves,” said Dr Ward, who is also a member of OzGrav.

ANU and the University of Melbourne are leading OzGrav’s search for gravitational waves from neutron stars using LIGO data.

 

 

Citation: GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2
B. P. Abbott et al. (LIGO Scientific and Virgo Collaboration)
Phys. Rev. Lett. 118, 221101 – Published 1 June 2017
http://dx.doi.org/10.1103/PhysRevLett.118.221101