薩德伯里微中子觀測站 (Chinese Wikipedia)
Analysis of information sources in references of the Wikipedia article "薩德伯里微中子觀測站" in Chinese language version.
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aip.org
scitation.aip.org
- Day, Charles. Takaaki Kajita and Arthur McDonald share 2015 Physics Nobel Prize. Physics Today. 2015-10-07 [2015-10-19]. （原始内容存档于2016-11-12）.
Established in 1984 in an abandoned nickel mine, the Sudbury Neutrino Observatory was conceived to resolve the solar neutrino problem.
arxiv.org
- SNO Collaboration. Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory. Phys. REv. Lett. 2001-07-25, 87 (7): 071301 [2015-10-08]. doi:10.1103/PhysRevLett.87.071301. （原始内容存档于2021-05-09）.
CC electrons are expected to have a distribution which is (1-0.340 cos θ), before accounting for detector response.
-
Ahmad, QR; et al. Measurement of the Rate of νe + d → p + p + e− Interactions Produced by 8B Solar Neutrinos at the Sudbury Neutrino Observatory. Physical Review Letters. 2001, 87 (7): 071301. Bibcode:2001PhRvL..87g1301A. arXiv:nucl-ex/0106015
. doi:10.1103/PhysRevLett.87.071301.
cerncourier.com
- The Sudbury Neutrino Observatory – Canada's eye on the universe. CERN Courier. CERN. 2001-12-04 [2008-06-04]. （原始内容存档于2016-06-25）.
doi.org
- SNO Collaboration. Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory. Phys. REv. Lett. 2001-07-25, 87 (7): 071301 [2015-10-08]. doi:10.1103/PhysRevLett.87.071301. （原始内容存档于2021-05-09）.
CC electrons are expected to have a distribution which is (1-0.340 cos θ), before accounting for detector response.
-
Ahmad, QR; et al. Measurement of the Rate of νe + d → p + p + e− Interactions Produced by 8B Solar Neutrinos at the Sudbury Neutrino Observatory. Physical Review Letters. 2001, 87 (7): 071301. Bibcode:2001PhRvL..87g1301A. arXiv:nucl-ex/0106015 . doi:10.1103/PhysRevLett.87.071301.
fi.edu
- Arthur B. McDonald, Ph.D.. Franklin Laureate Database. Franklin Institute. [2008-06-04]. （原始内容存档于2008-10-04）.
harvard.edu
ui.adsabs.harvard.edu
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Ahmad, QR; et al. Measurement of the Rate of νe + d → p + p + e− Interactions Produced by 8B Solar Neutrinos at the Sudbury Neutrino Observatory. Physical Review Letters. 2001, 87 (7): 071301. Bibcode:2001PhRvL..87g1301A. arXiv:nucl-ex/0106015 . doi:10.1103/PhysRevLett.87.071301.
ieee.ca
- Brewer, Robert. Deep Sphere: The unique structural design of the Sudbury Neutrinos Observatory buried within the earth. Canadian Consulting Engineer. [2016-01-14]. （原始内容存档于2016-03-04）.
nobelprize.org
- Bahcall, John. Solving the Mystery of the Missing Neutrinos. Nobelprize.org. Nobel Media. 2015 [2015-10-07]. （原始内容存档于2018-06-24）.
- The Nobel Prize in Physics 2015. [2015-10-06]. （原始内容存档于2016-05-15）.
queensu.ca
sno.phy.queensu.ca
- The SNO Detector. Sudbury Neutrino Observatory. 2015 [2015-10-07]. （原始内容存档于2021-05-07）.
- First Results from the Sudbury Neutrino Observatory Explain the Missing Solar Neutrinos and Reveal New Neutrino Properties. Sudbury Neutrino Observatory. 2001-06-18 [2015-10-08]. （原始内容存档于2015-12-12）.
- Thornewell, Peter. Neutral Current Detectors for the Sudbury Neutrino Observatory (PDF) (学位论文). Oxford University. 1997 [2015-10-16]. （原始内容 (PDF)存档于2020-02-03）.
- Sudbury Neutrino Observatory First Scientific Results. 2001-07-03 [2008-06-04]. （原始内容存档于2015-12-12）.
web.archive.org
- Day, Charles. Takaaki Kajita and Arthur McDonald share 2015 Physics Nobel Prize. Physics Today. 2015-10-07 [2015-10-19]. （原始内容存档于2016-11-12）.
Established in 1984 in an abandoned nickel mine, the Sudbury Neutrino Observatory was conceived to resolve the solar neutrino problem.
- Bahcall, John. Solving the Mystery of the Missing Neutrinos. Nobelprize.org. Nobel Media. 2015 [2015-10-07]. （原始内容存档于2018-06-24）.
- The Sudbury Neutrino Observatory – Canada's eye on the universe. CERN Courier. CERN. 2001-12-04 [2008-06-04]. （原始内容存档于2016-06-25）.
- The SNO Detector. Sudbury Neutrino Observatory. 2015 [2015-10-07]. （原始内容存档于2021-05-07）.
- Brewer, Robert. Deep Sphere: The unique structural design of the Sudbury Neutrinos Observatory buried within the earth. Canadian Consulting Engineer. [2016-01-14]. （原始内容存档于2016-03-04）.
- First Results from the Sudbury Neutrino Observatory Explain the Missing Solar Neutrinos and Reveal New Neutrino Properties. Sudbury Neutrino Observatory. 2001-06-18 [2015-10-08]. （原始内容存档于2015-12-12）.
- SNO Collaboration. Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory. Phys. REv. Lett. 2001-07-25, 87 (7): 071301 [2015-10-08]. doi:10.1103/PhysRevLett.87.071301. （原始内容存档于2021-05-09）.
CC electrons are expected to have a distribution which is (1-0.340 cos θ), before accounting for detector response.
- Thornewell, Peter. Neutral Current Detectors for the Sudbury Neutrino Observatory (PDF) (学位论文). Oxford University. 1997 [2015-10-16]. （原始内容 (PDF)存档于2020-02-03）.
- Sudbury Neutrino Observatory First Scientific Results. 2001-07-03 [2008-06-04]. （原始内容存档于2015-12-12）.
- SPIRES HEP Results. SPIRES. SLAC. [2009-10-06]. （原始内容存档于2020-01-29）.
- Arthur B. McDonald, Ph.D.. Franklin Laureate Database. Franklin Institute. [2008-06-04]. （原始内容存档于2008-10-04）.
- The Nobel Prize in Physics 2015. [2015-10-06]. （原始内容存档于2016-05-15）.