Line versus continuum solar neutrinos

John N. Bahcall

doi:10.1103/PhysRevD.41.2964

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Line versus continuum solar neutrinos

John N. Bahcall

Institute for Advanced Study, Princeton, New Jersey 08540

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Phys. Rev. D 41, 2964 – Published 15 May, 1990

DOI: https://doi.org/10.1103/PhysRevD.41.2964

Abstract

The rate of neutrino line emission is calculated for nuclei that are usually assumed to produce only continuum neutrino emission. A convenient formula is derived that gives for solar interior conditions the ratio of the rates of neutrino line emission to continuum neutrino emission. The only significant line emission from the solar interior is expected from the $pep$ and ${}^{7}{Be}$ -electron capture reactions.

References (6)

J. N. Bahcall, Phys. Rev. 135, B137 (1964)
J. N. Bahcall, Neutrino Astrophysics (Cambridge University Press, Cambridge, England, 1989)
P. Cheeseman, report, 1989 (unpublished)
P. E. Tegner and C. Bargholtz, Astrophys. J. 272, 311 (1983)
J. N. Bahcall and R. M. May, Astrophys. J. 155, 501 (1969)
S. F. Mughabghab and D. I. Garber, Neutron Cross Sections, Vol. 1, Resonance Parameters (BNL Report No. 325) (National Neutron Cross Section Center, Brookhaven National Laboratory, Upton, New York, 1973)

[c1] J. N. Bahcall, Phys. Rev. 135, B137 (1964)

[c2] J. N. Bahcall, Neutrino Astrophysics (Cambridge University Press, Cambridge, England, 1989)

[c3] P. Cheeseman, report, 1989 (unpublished)

[c4] P. E. Tegner and C. Bargholtz, Astrophys. J. 272, 311 (1983)

[c5] J. N. Bahcall and R. M. May, Astrophys. J. 155, 501 (1969)

[c6] S. F. Mughabghab and D. I. Garber, Neutron Cross Sections, Vol. 1, Resonance Parameters (BNL Report No. 325) (National Neutron Cross Section Center, Brookhaven National Laboratory, Upton, New York, 1973)

Physical Review D

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Line versus continuum solar neutrinos

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