LIGO Scientific Collaboration
 | |
| Formation | 1997[1] |
|---|---|
| Headquarters | California Institute of Technology and Massachusetts Institute of Technology, United States |
Membership | 991 scientists[2] |
LSC Spokesperson | Gabriela González |
Executive Director of LIGO | David Reitze |
| Award(s) |
Special Breakthrough Prize in Fundamental Physics (2016) Gruber Prize in Cosmology (2016) Enrico Fermi Prize (2016) |
| Website | www.ligo.org |
The LIGO Scientific Collaboration (LSC) is a scientific collaboration of international physics institutes and research groups dedicated to the search for gravitational waves. The LSC was established in 1997, under the leadership of Barry Barish.[3] Its mission is to ensure equal scientific opportunity for individual participants and institutions by organizing research, publications, and all other scientific activities, and it includes scientists from both LIGO Laboratory and collaborating institutions. Barish appointed Rainer Weiss as the first spokesperson.
LSC members have access to the US-based Advanced LIGO detectors in Hanford, Washington and in Livingston, Louisiana, as well as the GEO 600 detector in Sarstedt, Germany. Under an agreement with the European Gravitational Observatory (EGO), LSC members also have access to data from the Virgo detector in Pisa, Italy. While the LSC and the Virgo Collaboration are separate organizations, they cooperate closely and are referred to collectively as "LVC".[4]
The current LSC Spokesperson is Gabriela González from Louisiana State University. The Executive Director of the LIGO Laboratory is David Reitze from the University of Florida.
On 11 February 2016, the LIGO and Virgo collaborations[lower-alpha 1] announced that they succeeded in making the first direct gravitational wave observation on 14 September 2015.[5][6][7][8]
In 2016, Barish received the Enrico Fermi Prize "for his fundamental contributions to the formation of the LIGO and LIGO-Virgo scientific collaborations and for his role in addressing challenging technological and scientific aspects whose solution led to the first detection of gravitational waves". [9]
Collaboration members
Membership of LIGO Scientific Collaboration as of November 2015 is detailed in the table below.[2]
.svg.png){kind=small}
Notes
- ↑ The 11 February 2016 announcement team were Kip Thorne, David Reitze, Gabriela González, and Rainer Weiss.
References
- ↑ "About the LSC". LIGO Scientific Collaboration. Retrieved 5 May 2014.
- 1 2 "LSC/Virgo Census". myLIGO. Retrieved 28 November 2015.
- ↑ Committee on Setting Priorities for NSF-Sponsored Large Research Facility Projects, Committee on Science, Engineering, and Public Policy, Policy and Global Affairs, Board on Physics and Astronomy, Division on Engineering and Physical Sciences, National Research Council. (2004). Setting Priorities for Large Research Facility Projects Supported by the National Science Foundation. National Academies Press. pp. 129–136.
- ↑ Gabriela González, Fulvio Ricci, LIGO Scientific Collaboration, Virgo Collaboration (2015-12-06). "Open call for partnership for the EM identification and follow-up of GW candidate events" (PDF). Retrieved 25 May 2016.
- ↑ Twilley, Nicola. "Gravitational Waves Exist: The Inside Story of How Scientists Finally Found Them". The New Yorker. ISSN 0028-792X. Retrieved 2016-02-11.
- ↑ Abbott, B.P.; et al. (2016). "Observation of Gravitational Waves from a Binary Black Hole Merger". Phys. Rev. Lett. 116: 061102. doi:10.1103/PhysRevLett.116.061102.
- ↑ Naeye, Robert (11 February 2016). "Gravitational Wave Detection Heralds New Era of Science". Sky and Telescope. Retrieved 11 February 2016.
- ↑ Castelvecchi, Davide; Witze, Alexandra (11 February 2016). "Einstein's gravitational waves found at last". Nature News. doi:10.1038/nature.2016.19361. Retrieved 11 February 2016.
- ↑ "2016 Enrico Fermi Prize". Società Italiana di Fisica.
External links
- Official website (English) (Spanish) (Hungarian)
- LIGO Magazine
| Detectors |
| 
 | ||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Pulsar timing arrays | ||||||||||||||||
| Data analysis | ||||||||||||||||
| Observations |
| |||||||||||||||
| Theory | ||||||||||||||||