ADDENDUM on the mass neutrino oscillation in a gravitational field

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dc.creatorPereira, J. G.
dc.creatorZhang, C. M.
dc.date2002-05-08
dc.date.accessioned2026-07-07T03:26:51Z
dc.date.available2026-07-07T03:26:51Z
dc.descriptionIn the article {\it Gen. Rel. Grav.} {\bf 32}, 1633 (2000), by J. G. Pereira and C. M. Zhang, the special relativity energy-momentum tensor was used to discuss the neutrino phase-splitting in a weak gravitational field. However, it would be more appropriate to use the general relativity energy-momentum tensor. When we do that, as we are going to see, some results change, but the basic conclusion remains the same.
dc.description2 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0205030
dc.identifierhttp://arxiv.org/abs/gr-qc/0205030
dc.identifierGen.Rel.Grav. 33 (2001) 2801-2802
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34209
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleADDENDUM on the mass neutrino oscillation in a gravitational field
dc.typetext

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