Neutrino-deuteron scattering in effective field theory at next-to-next-to-leading order

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dc.creator Butler, Malcolm
dc.creator Chen, Jiunn-Wei
dc.creator Kong, Xinwei
dc.date.accessioned 2015-07-29T13:08:52Z
dc.date.available 2015-07-29T13:08:52Z
dc.date.issued 2001-03
dc.identifier.issn 0556-2813
dc.identifier.uri http://library2.smu.ca/xmlui/handle/01/26266
dc.description Publisher's version/PDF en_CA
dc.description.abstract We study the four channels associated with neutrino-deuteron breakup reactions at next-to-next-to-leading order in effective field theory. We find that the total cross section is indeed converging for neutrino energies up to 20 MeV, and thus our calculations can provide constraints on theoretical uncertainties for the Sudbury Neutrino Observatory. We stress the importance of a direct experimental measurement to high precision in at least one channel, in order to fix an axial two-body counterterm. en_CA
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dc.language.iso en en_CA
dc.publisher American Physical Society en_CA
dc.relation.uri http://dx.doi.org/10.1103/PhysRevC.63.035501
dc.rights Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.
dc.subject.lcsh Neutrinos -- Scattering
dc.subject.lcsh Deuterons -- Scattering
dc.subject.lcsh Field theory (Physics)
dc.title Neutrino-deuteron scattering in effective field theory at next-to-next-to-leading order en_CA
dc.type Text en_CA
dcterms.bibliographicCitation Physical Review C 63(3), 035501. (2001) en_CA
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Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.
 
Published Version: http://dx.doi.org/10.1103/PhysRevC.63.035501
 
 

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