The basic physics of the binary black hole merger GW150914

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dc.contributor.author Abbott, B. P.
dc.contributor.author Davies, G. S.
dc.contributor.author LIGO Scientific Collaboration and Virgo Collaboration
dc.date.accessioned 2017-04-19T15:31:08Z
dc.date.available 2017-04-19T15:31:08Z
dc.date.issued 2016-10-04
dc.identifier.citation Abbott, BP., et al., (LIGO Scientific Collaboration and Virgo Collaboration). The basic physics of the binary black hole merger GW150914. Annalen Der Physik, Volume 529, Issue 1-2, 2017, Article number 1600209 en_UK
dc.identifier.uri http://dspace.lib.cranfield.ac.uk/handle/1826/11784
dc.identifier.uri http://dx.doi.org/10.1002/andp.201600209
dc.description.abstract The first direct gravitational-wave detection was made by the Advanced Laser Interferometer Gravitational Wave Observatory on September 14, 2015. The GW150914 signal was strong enough to be apparent, without using any waveform model, in the filtered detector strain data. Here those features of the signal visible in these data are used, along with only such concepts from Newtonian and General Relativity as are accessible to anyone with a general physics background. The simple analysis presented here is consistent with the fully general-relativistic analyses published elsewhere, in showing that the signal was produced by the inspiral and subsequent merger of two black holes. The black holes were each of approximately 35 Msun, still orbited each other as close as 350 km apart and subsequently merged to form a single black hole. Similar reasoning, directly from the data, is used to roughly estimate how far these black holes were from the Earth, and the energy that they radiated in gravitational waves. en_UK
dc.language.iso en en_UK
dc.publisher Wiley en_UK
dc.rights Attribution 4.0 International
dc.rights.uri http://creativecommons.org/licenses/by/4.0/
dc.title The basic physics of the binary black hole merger GW150914 en_UK
dc.type Article en_UK


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