Journal article

Determining the Low Energy Backgrounds at the Sudbury Neutrino Observatory

Abstract:: Naturally occurring radioisotopes can produce neutrons by photodisintegration and Cherenkov events via beta/gamma decays. The techniques used to measure the radioisotopes in the heavy water target and light water shield in the third phase of SNO is discussed. © 2011 Elsevier B.V.

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APA Style

O'Keeffe, H., Aharmim, B., Ford, R., Farine, J., Jelley, N., Goon, J., & Seibert, S. R. (2011). Determining the Low Energy Backgrounds at the Sudbury Neutrino Observatory. Nuclear Physics B - Proceedings Supplements, 221, 381–381.

MLA Style

O'Keeffe, H., et al. “Determining the Low Energy Backgrounds at the Sudbury Neutrino Observatory.” Nuclear Physics B - Proceedings Supplements, vol. 221, 2011, pp. 381–81.

Chicago Style

O'Keeffe, H, B Aharmim, R Ford, J Farine, N Jelley, J Goon, and SR Seibert. 2011. “Determining the Low Energy Backgrounds at the Sudbury Neutrino Observatory.” Nuclear Physics B - Proceedings Supplements 221: 381–81.
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Publisher copy:: 10.1016/j.nuclphysbps.2011.10.031

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+ O'Keeffe, H More by this author

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+ Aharmim, B More by this author

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+ Ford, R More by this author

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+ Farine, J More by this author

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+ Jelley, N More by this author

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Journal:: Nuclear Physics B - Proceedings Supplements More from this journal
Volume:: 221
Pages:: 381-381
Publication date:: 2011-12-01
DOI:: 10.1016/j.nuclphysbps.2011.10.031
ISSN:: 0920-5632

Language:: English
Pubs id:: pubs:325353
UUID:: uuid:b226ca6b-f292-483c-8281-caa6ba0c10be
Local pid:: pubs:325353
Source identifiers:: 325353
Deposit date:: 2012-12-19

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Copyright date:: 2011

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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