The basic physics of the binary black hole merger GW150914

The basic physics of the binary black hole merger GW150914

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, features of the signal...

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Bibliographic Details
Main Authors: Aggarwal, Nancy, Barsotti, Lisa, Biscans, Sebastien, Brown, N. M., Buikema, Aaron, Donovan, Frederick J, Essick, Reed Clasey, Evans, M., Fritschel, Peter K, Gras, Slawomir, Isogai, Tomoki, Katsavounidis, Erotokritos, Kontos, Antonios, Krolak, A., Kutynia, A., Libson, Adam A., Lynch, Ryan Christopher, MacInnis, Myron E, Marchesoni, F., Martynov, D. V., Mason, Kenneth R, Matichard, Fabrice, Mavalvala, Nergis, Miller, John, Mittleman, Richard K, Mohapatra, S. R. P., Oelker, Eric Glenn, Shoemaker, David H, Tse, Maggie, Vaulin, Ruslan, Vitale, Salvatore, Weiss, Rainer, Yam, William, Yu, H., Zucker, Michael E
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Published: Wiley-Blackwell 2019
Online Access:https://hdl.handle.net/1721.1/121202

Internet

https://hdl.handle.net/1721.1/121202

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