OPERA experiment (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "OPERA experiment" in English language version.

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4arxiv.org

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arxiv.org

Agafonova, N.; et al. (OPERA Collaboration) (2010). "Observation of a first ν_τ candidate event in the OPERA experiment in the CNGS beam". Physics Letters B. 691 (3): 138–145. arXiv:1006.1623. Bibcode:2010PhLB..691..138A. doi:10.1016/j.physletb.2010.06.022. S2CID 119256958.
Adam, T.; et al. (OPERA collaboration) (17 November 2011). "Measurement of the neutrino velocity with the OPERA detector in the CNGS beam". arXiv:1109.4897v1 [hep-ex].
Adam, T.; et al. (OPERA collaboration) (2012). "Measurement of the neutrino velocity with the OPERA detector in the CNGS beam". Journal of High Energy Physics. 2012 (10): 93. arXiv:1109.4897. Bibcode:2012JHEP...10..093A. doi:10.1007/JHEP10(2012)093. S2CID 17652398.
Adam, T.; et al. (OPERA collaboration) (2013). "Measurement of the neutrino velocity with the OPERA detector in the CNGS beam using the 2012 dedicated data". Journal of High Energy Physics. 1: 153. arXiv:1212.1276. Bibcode:2013JHEP...01..153A. doi:10.1007/JHEP01(2013)153. S2CID 119258343.

cern.ch

press-archived.web.cern.ch

"Neutrinos sent from CERN to Gran Sasso respect the cosmic speed limit" (Press release). CERN. 8 June 2012. Archived from the original on 22 February 2014. Retrieved 8 June 2012.

doi.org

Agafonova, N.; et al. (OPERA Collaboration) (2010). "Observation of a first ν_τ candidate event in the OPERA experiment in the CNGS beam". Physics Letters B. 691 (3): 138–145. arXiv:1006.1623. Bibcode:2010PhLB..691..138A. doi:10.1016/j.physletb.2010.06.022. S2CID 119256958.
Brumfiel, G. (16 March 2012). "Neutrinos not faster than light". Nature News. doi:10.1038/nature.2012.10249. S2CID 119620081. Retrieved 12 March 2013.
Adam, T.; et al. (OPERA collaboration) (2012). "Measurement of the neutrino velocity with the OPERA detector in the CNGS beam". Journal of High Energy Physics. 2012 (10): 93. arXiv:1109.4897. Bibcode:2012JHEP...10..093A. doi:10.1007/JHEP10(2012)093. S2CID 17652398.
Adam, T.; et al. (OPERA collaboration) (2013). "Measurement of the neutrino velocity with the OPERA detector in the CNGS beam using the 2012 dedicated data". Journal of High Energy Physics. 1: 153. arXiv:1212.1276. Bibcode:2013JHEP...01..153A. doi:10.1007/JHEP01(2013)153. S2CID 119258343.

harvard.edu

ui.adsabs.harvard.edu

Agafonova, N.; et al. (OPERA Collaboration) (2010). "Observation of a first ν_τ candidate event in the OPERA experiment in the CNGS beam". Physics Letters B. 691 (3): 138–145. arXiv:1006.1623. Bibcode:2010PhLB..691..138A. doi:10.1016/j.physletb.2010.06.022. S2CID 119256958.
Adam, T.; et al. (OPERA collaboration) (2012). "Measurement of the neutrino velocity with the OPERA detector in the CNGS beam". Journal of High Energy Physics. 2012 (10): 93. arXiv:1109.4897. Bibcode:2012JHEP...10..093A. doi:10.1007/JHEP10(2012)093. S2CID 17652398.
Adam, T.; et al. (OPERA collaboration) (2013). "Measurement of the neutrino velocity with the OPERA detector in the CNGS beam using the 2012 dedicated data". Journal of High Energy Physics. 1: 153. arXiv:1212.1276. Bibcode:2013JHEP...01..153A. doi:10.1007/JHEP01(2013)153. S2CID 119258343.

home.cern

O'Luanaigh, C. (6 October 2015). "OPERA detects its fifth tau neutrino". Retrieved 8 February 2017.

infn.it

operaweb.lngs.infn.it

"[OPERA]: News and Updates". 21 May 2018. Archived from the original on 25 January 2021. Retrieved 25 September 2011. 3 December 2012 After 5 years of operation the CNGS beam was stopped. In total it was 17.97×10¹⁹ protons on target provided by the CNGS.
"The Opera Detector". OPERA. Archived from the original on 11 February 2019. Retrieved 25 September 2011.

interactions.org

"OPERA Observes the Second Tau Neutrino" (Press release). Istituto Nazionale di Fisica Nucleare. 6 June 2012. Retrieved 8 June 2012.

jimal-khalili.com

Al-Khalili, J. (18 November 2011). "Faster than the speed of light?". Jim's Blog. Archived from the original on 1 February 2014. Retrieved 31 August 2013.

nature.com

Brumfiel, G. (16 March 2012). "Neutrinos not faster than light". Nature News. doi:10.1038/nature.2012.10249. S2CID 119620081. Retrieved 12 March 2013.

semanticscholar.org

api.semanticscholar.org

Agafonova, N.; et al. (OPERA Collaboration) (2010). "Observation of a first ν_τ candidate event in the OPERA experiment in the CNGS beam". Physics Letters B. 691 (3): 138–145. arXiv:1006.1623. Bibcode:2010PhLB..691..138A. doi:10.1016/j.physletb.2010.06.022. S2CID 119256958.
Brumfiel, G. (16 March 2012). "Neutrinos not faster than light". Nature News. doi:10.1038/nature.2012.10249. S2CID 119620081. Retrieved 12 March 2013.
Adam, T.; et al. (OPERA collaboration) (2012). "Measurement of the neutrino velocity with the OPERA detector in the CNGS beam". Journal of High Energy Physics. 2012 (10): 93. arXiv:1109.4897. Bibcode:2012JHEP...10..093A. doi:10.1007/JHEP10(2012)093. S2CID 17652398.
Adam, T.; et al. (OPERA collaboration) (2013). "Measurement of the neutrino velocity with the OPERA detector in the CNGS beam using the 2012 dedicated data". Journal of High Energy Physics. 1: 153. arXiv:1212.1276. Bibcode:2013JHEP...01..153A. doi:10.1007/JHEP01(2013)153. S2CID 119258343.

symmetrymagazine.org

Jepsen, K. (26 March 2013). "OPERA snags third tau neutrino". Symmetry Magazine. Retrieved 27 March 2013.

web.archive.org

Al-Khalili, J. (18 November 2011). "Faster than the speed of light?". Jim's Blog. Archived from the original on 1 February 2014. Retrieved 31 August 2013.
"[OPERA]: News and Updates". 21 May 2018. Archived from the original on 25 January 2021. Retrieved 25 September 2011. 3 December 2012 After 5 years of operation the CNGS beam was stopped. In total it was 17.97×10¹⁹ protons on target provided by the CNGS.
"The Opera Detector". OPERA. Archived from the original on 11 February 2019. Retrieved 25 September 2011.
"Neutrinos sent from CERN to Gran Sasso respect the cosmic speed limit" (Press release). CERN. 8 June 2012. Archived from the original on 22 February 2014. Retrieved 8 June 2012.