Solar Neutrino References
- Standard Solar Model
-
J. N. Bahcall,
Neutrino Astrophysics, (Cambridge University Press, Cambridge, 1989).
-
J. N. Bahcall and M. H. Pinsonneault,
Rev. Mod. Phys. 64, 885 (1992).
-
S. Turck-Chieze and I. Lopes,
Astrophys. J. 408, 347 (1993).
S. Turck-Chieze, S. Cahen, M. Casse, and C. Doom,
Astrophys. J. 335, 415 (1988).
-
J. N. Bahcall and R. N. Ulrich,
Rev. Mod. Phys. 60, 297 (1988).
- Current Experiments
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Homestake:
R. Davis, Jr. et al.,
in Proceedings of the 21th International Cosmic Ray Conference, Vol. 12,
edited by R. J. Protheroe (University of Adelaide Press, Adelaide, 1990),
p. 143;
R. Davis, Jr., in Frontiers of Neutrino Astrophysics,
edited by Y. Suzuki and K. Nakamura (Universal Academy Press, Tokyo, 1993),
P. 47;
K. Lande, in Neutrino 94, Eilat, Israel, May 1994.
-
Kamiokande II: K. S. Hirata et al.,
Phys. Rev. Lett. 65, 1297, 1301 (1990);
66, 9 (1991);
Phys. Rev. D44, 2241 (1991).
Kamiokande III: Y. Suzuki,
in Neutrino 94, Eilat, Israel, May 1994.
-
SAGE: A. I. Abazov, et al.,
Phys. Rev. Lett. 67, 3332 (1991);
J. N. Abdurashitov et al.,
Phys. Lett. B 328, 234 (1994);
J. Nico, in ICHEP, Glasgow, July 1994.
-
GALLEX: P. Anselmann et al.,
Phys. Lett. B285, 376, 390 (1992);
B314, 445 (1993); B327, 377 (1994);
calibration: P. Anselmann et al.,
Phys. Lett. B342, 440 (1995).
- Astrophysical Solutions?
- Be-7 Suppression
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W. K. Kwong and S. P. Rosen, Phys. Rev. Lett. 73, 369 (1994).
-
N. Hata, S. Bludman, and P. Langacker,
Phys. Rev. D49, 3622 (1994).
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N. Hata and P. Langacker, Pennsylvania UPR-0625T.
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J. Bahcall, Institute for Advanced Study, IASSNS-AST 94/37.
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V. Castellani et al, ASTROPH-9405018;
Astron. Astrophys. 271, 601 (1993); Astrophys. J 402, 574 (1993);
Phys. Lett. B303, 68 (1993), B324, 425 (1994), B329, 525 (1994);
Phys. Rev. D50, 4749 (1994).
-
S. Degl'Innocenti, and G. Fiorentini, and M. Lissia, INFNFE-10-94.
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X. Shi and D. N. Schramm,
Particle World 3, 109 (1994);
X. Shi, D. N. Schramm, and D. Dearborn Phys. Rev. D50, 2414 (1994).
- Explicit Nonstandard Solar Models
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Low S17 (experiment): T. Motobayashi et al.,
Phys. Rev. Lett. 73, 2680 (1994).
-
Low opacity: D. Dearborn, private communications.
WIMP: J. Faulkner and R. L. Gilliland,
Ap. J. 299, 994 (1985);
R. L. Gilliland, J. Faulkner, W. H. Press, and D. N. Spergel,
Ap. J. 306, 703 (1986).
Large S11: V. Castellani, S. Degl'Innocenti, and G. Fiorentini,
Phys. Lett. B303, 68 (1993).
Small S34 or large S33:
[ref] .
Mixing models: R. Sienkiewicz, J. N. Bahcall, and B. Paczynski,
Astrophys. J. 349, 641 (1990).
Low Z or high Y:
[ref] and
[ref].
A. Dar and G. Shaviv, TECHNION-PH-94-5.
- Cool Sun Models
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S. Bludman, D. Kennedy, and P. Langacker,
Nucl. Phys. B374, 373 (1992). These results are
updated in
S. Bludman, N. Hata, D. Kennedy, and P. Langacker,
Phys. Rev. D47, 2220 (1993);
N. Hata and P. Langacker, Pennsylvania UPR-0625T.
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Relation to explicit models:
N. Hata, S. Bludman, and P. Langacker,
Phys. Rev.
D49, 3622 (1994).
V. Castellani et al, ASTROPH-9405018;
INFN preprint INFNFE-3-94, 1994;
Astron. Astrophys. 271, 601 (1993); Astrophys. J 402, 574 (1993);
Phys. Lett. B303, 68 (1993), B324, 425 (1994), B329, 525 (1994);
Phys. Rev. D50, 4749 (1994).
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Nonstandard T and cross sections:
X. Shi, D. N. Schramm, and D. Dearborn,
Phys. Rev. D50, 2414 (1994).
V. Berezinsky, G. Fiorentini, and M. Lissia, Phys. Lett. B341,
38 (1994).
- Model-Independent Analyses
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Present: N. Hata, S. Bludman, and P. Langacker,
Phys. Rev. D49, 3622 (1994).
-
Future (with MSW):
N. Hata and P. Langacker, Pennsylvania UPR-0625T.
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M. Spiro and D. Vignaud, Phys. Lett. B242, 279 (1990).
V. Castellani et al., [ref];
S. Parke, Phys. Rev. Lett. 74, 839 (1994).
-
No spectral distortion: J. N. Bahcall,
Phys. Rev. D44, 1644 (1991).
- Neutrino Oscillations
- MSW
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L. Wolfenstein,
Phys. Rev. D17, 2369 (1978); D20, 2634 (1979);
S. P. Mikheyev and A. Yu. Smirnov,
Yad. Fiz. 42, 1441 (1985)
[Sov. J. Nucl. Phys. 42, 913 (1986)];
Nuovo Cimento 9C, 17 (1986).
- Recent MSW Calculations
-
N. Hata and P. Langacker,
Phys. Rev. D50, 632 (1994).
-
S. Bludman, N. Hata, D. Kennedy, and P. Langacker,
Phys. Rev. D47, 2220 (1993).
-
X. Shi, D. N. Schramm, and J. Bahcall,
Phys. Rev. Lett. 69, 717 (1992).
-
J. M. Gelb, W. Kwong, and S. P. Rosen,
Phys. Rev. Lett. 69, 1864 (1992).
-
G. L. Fogli, E. Lisi, and D. Montanino,
Phys. Rev. D49, 3626 (1994).
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G. Fiorentini et al., Phys. Rev. D49, 6298 (1994).
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P. I. Krastev and S. T. Petcov, SISSA-41-94-EP;
Phys. Lett. B299, 99 (1993).
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J. N. Bahcall and W. C. Haxton,
Phys. Rev. D40, 931 (1989).
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L. Krauss, E. Gates, and M. White,
Phys. Lett. B299, 94 (1993).
-
V. Berezinsky, G. Fiorentini, and M. Lissia,
Phys. Lett. B341,
38 (1994).
- Earth Effect
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A. J. Baltz and J. Weneser,
Phys. Rev. D35, 528 (1987), D37, 3364, (1988),
D50, 5971, (1994);
E. D. Carlson,
Phys. Rev. D34, 1454 (1986);
J. Bouchez, M. Cribier, W. Hampel, J. Rich, M. Spiro, and D. Vignaud,
Z. Phys. C32, 499 (1986);
M. Cribier, W. Hampel, J. Rich, and D. Vignaud,
Phys. Lett. B182, 89 (1986).
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Kamiokande:
K. S. Hirata et al., Phys. Rev. Lett. 66, 9 (1991).
-
N. Hata and P. Langacker,
Phys. Rev. D48, 2937 (1993);
Phys. Rev. D50, 632 (1994).
- Three Flavor MSW
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X. Shi and D. N. Schramm, Phys. Lett. B283, 305 (1992);
J. Pantaleone, Phys. Rev. D49, 2152 (1994); D. Harley, T. K. Kuo, and J. Pantaleone,
Phys. Rev. D47, 4059 (1993).
- Vacuum Oscillations
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S. L. Glashow and L. M. Krauss,
Phys. Lett. B190, 199 (1988).
-
V. Barger, R. J. N. Phillips, and K. Whisnant,
Phys. Rev. D43, 1110 (1991);
Phys. Ref. Lett. 69, 3135 (1992).
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A. Acker, S. Pakvasa, and J. Pantaleone,
Phys. Rev. D43, 1754 (1991).
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P. I. Krastev and S. T. Petcov,
Phys. Rev. Lett. 72, 1960 (1994), SISSA-41-94-EP;
Phys. Lett. B285, 85 (1992), B299, 99 (1993).
-
A. Acker, A. B. Balantekin, and F. Loreti,
Phys. Rev. D49, 328 (1994).
-
N. Hata,
University of Pennsylvania Report No. UPR-0605T.
- Oscillations to Sterile Neutrinos
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Second class (sterile) oscillations:
V. Barger, P. Langacker, J. P. Leveille, and S. Pakvasa,
Phys. Rev. Lett. 45, 692 (1980).
-
Nucleosynthesis bounds:
P. Langacker, UPR-0401T; R. Barbieri and A. Dolgov,
Phys. Lett. B237, 440 (1990); Nucl. Phys. B349, 743 (1991); K. Kainulainen,
Phys. Lett. B244, 191 (1990); K. Enqvist, K. Kainulainen, and J. Maalampi,
Phys. Lett. B244, 186 (1990); B249, 531 (1990); M.J. Thomson and B.H.J.
McKellar, Phys. Lett. B259, 113 (1991); X. Shi, D. Schramm, and B. Fields,
Phys. Rev. D48, 2563 (1993).
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Solar neutrinos: V. Barger, N. Deshpande, R. J. N. Phillips, and
K. Whisnant, Phys. Rev. D43, 1759 (1991), and the papers in
[ref].
- Massless Nonorthogonal Neutrinos
- Other Nonstandard Neutrino Properties
- Large Magnetic Moment
-
M. B. Voloshin, M. I. Vysotskii, and L. B. Okun,
Yad Fiz. 44, 677 (1986)
(SJNP 44, 440 (1986)); C. S. Lim and W. J. Marciano, Phys. Rev. D37, 1368 (1988).
Recent treatments and reviews include E. Kh. Akhmedov, HEPPH-9405293;
E. Kh Akhmedov, A. Lanza, and S. T. Petcov, Phys. Lett. B303, 85 (1994);
X. Shi et al., Comm. Nucl. Part. Phys. 21, 151 (1993);
P. Vogel and J. Engel, Phys. Rev. D39, 3378 (1989).
- Neutrino Decay
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A. Acker and S. Pakvasa, Phys. Lett. B320, 320 (1994);
A. Acker, S. Pakvasa, and J. Pantaleone, Phys. Rev. D45, 1 (1992) and
[ref]; A. Acker, A. Joshipura, and
S. Pakvasa, Phys. Lett. B285, 371 (1992);
J. A. Frieman, H. E. Haber, and K. Freese, Phys. Lett. B200, 115 (1988).
- Violation of Equivalence Principle
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M. Gasperini,
Phys. Rev. D38, 2635 (1988), D39, 3606 (1989);
J. Pantaleone, A. Halprin, C.N. Leung, Phys. Rev. D47, 4199 (1993);
J. N. Bahcall, P. I. Krastev, and C. N. Leung, IASSNS-AST 95/54.
- Penn and OSU Articles
on Neutrino Mass, Solar Neutrinos, Nucleosynthesis
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Solutions to Solar Neutrino Anomaly
by N. Hata and P. Langacker,
UPR-0751T.
hep-ph/9705339
(36 pp with 21 figures, 5/97)
gzipped postscript file.
Figures, HTML file.
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Cosmological Implications of Two Conflicting Deuterium Abundances,
By N. Hata, G. Steigman, (Ohio State U.), S. Bludman, P.
Langacker (Penn U.), Phys. Rev. D55, 540 (1997),
astro-ph/9603087
(29 pp with 12 figures, 3/96).
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Big Bang Nucleosynthesis in Crisis,
By N. Hata, R.J. Scherrer, G. Steigman,
D. Thomas, T.P. Walker (Ohio State U.), S. Bludman, P.
Langacker (Penn U.), Phys. Rev. Lett. 75, 3977 (1995).
hep-ph/9505319
(15 pp with 5 figures, 5/95)
compressed postscript file.
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Implications of the GALLEX source experiment for the solar
neutrino problem,
by N. Hata and W. Haxton, Phys. Lett. B353, 422 (1995),
nucl-th/9503017
(26 pages with 5 figures, 3/95)
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DPF Long Range Planning Study:
Neutrino Mass Working Group,
P. Langacker, R. Rameika, H. Robertson, conveners,
files
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Review:
Neutrino Physics, by P. Langacker,
from Beyond the Standard Model IV,
Lake Tahoe, 1994,
UPR-0652T,
hep-ph/9503327.
(16 pages with 2 embedded figures, 3/14/95)
postscript file.
Updated version: Implications of Neutrino Mass,
from Pascos/Hopkins-95, Baltimore, 3/95,
postscript file.
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Predicting Big Bang Deuterium,
by N. Hata, R.J. Scherrer, G. Steigman, D. Thomas, T.P. Walker, Ohio State
U., OSU-TA-26-94,
astro-ph/9412087.
(12 pages with 3 figures, 12/22/94).
- Review:
Solar Neutrinos, by P. Langacker,
from 32nd International School of Subnuclear Physics,
Erice, 1994,
UPR-0640T,
hep-ph/9411339.
(33 pages with 15 embedded figures, 11/18/94)
postscript file.
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Neutrino flux extraction:
Model Independent Determination of the Solar Neutrino Spectrum
with and without MSW,
by N. Hata and P. Langacker,
Phys. Rev. D52, 420 (1995),
hep-ph/9409372.
(61 pages with 23 figures, 9/21/94)
compressed postscript file.
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Uncertainties and correlations, MSW analysis:
Solar Model Uncertainties, MSW Analysis, and Future Solar
Neutrino Experiments (N. Hata and P. Langacker), Phys. Rev. D50, 632 (1994).
-
Vacuum Oscillations and Future Solar Neutrino Experiments,
by N. Hata, UPR-0605-T,
hep-ph/9402311.
(19 pages with 8 figures, 2/17/94).
-
Review:
Solar Neutrinos: Hint for Neutrino Mass,
by N. Hata, UPR-0612-T. Talk given at Solar
Modeling Workshop, Seattle, WA, 24 Mar 1994,
hep-ph/9404329.
(40 pages with 20 figures, 4/23/94).
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Model independent analysis:
Astrophysical Solutions are Incompatible with the
Solar Neutrino Data (N. Hata, S. Bludman, and P. Langacker),
Phys. Rev. D49, 3622 (1994).
-
Scenarios for Neutrino Mass (P. Langacker),
in Beyond the Standard Model III, ed. S. Godfrey and P. Kalyniak
(World, Singapore, 1993), p. 91.
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The Earth Effect in the MSW Analysis of the Solar
Neutrino Experiments
(N. Hata and P. Langacker), Phys. Rev. D48, 2937 (1993).
-
MSW analysis (no earth effect):
Implications of Combined Solar Neutrino Observations and Their Theoretical
Uncertainties (S. Bludman, N. Hata, D. Kennedy, and P. Langacker),
Phys. Rev. D47, 2220 (1993).
-
Theoretical Implications of Combined Solar Neutrino Observations
(S. Bludman, N. Hata, D. Kennedy, and P. Langacker), Proceedings of the
XVth International Conference on Neutrino Physics and Astrophysics,
Nucl. Phys. B31 (Proc. Suppl.) 156 (1993).
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Atmospheric Neutrino Data and Neutrino Oscillations
(W. Frati, T.K. Gaisser, A.K. Mann, and T. Stanev), Phys. Rev. D48, 1140 (1993).
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String-inspired models:
Neutrino Masses within the Minimal Supersymmetric Standard Model
(M. Cvetic and P. Langacker), Phys. Rev. D46, R2759 (1992).
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Improved Cosmological and Radiative Decay Constraints on Neutrino
Masses and Lifetimes (S.A. Bludman), Phys. Rev. D45, 4720 (1992).
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Seesaw Model Predictions for the tau Neutrino Mass
(S. Bludman, D. Kennedy, and P. Langacker), Phys. Rev. D45, 1810 (1992).
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Cool sun models: Solutions of the Solar Neutrino Problem
(S. Bludman, D. Kennedy, and P. Langacker), Nucl. Phys. B374, 373 (1992).
-
Review of models and constraints:
Neutrino Mass (P. Langacker)
in Testing the Standard Model, ed. M. Cvetic
and P. Langacker (World, Singapore, 1991), p. 863.
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Review: Status of Solar Neutrino Experiments
(E. W. Beier, R. Davis, S. B. Kim, S. R. Elliott, and N. Jelley),
Nucl. Phys. A527, 653c (1991).
-
On The Cosmological Production of Light Sterile Neutrinos,
by P. Langacker,
unpublished , UPR-0401T,
(12 pages with 1 figure, 9/20/89)
postscript paper, or
GIF figure, or
abstract .
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older papers on neutrino mass
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FTP index
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Papers on other subjects
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Standard Solar Model Predictions
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Current data and comparison with standard
solar model predictions
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Astrophysical/nuclear physics explanations
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MSW interpretation
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Main window
Naoya Hata (hata@pacific.mps.ohio-state.edu);
Paul Langacker (pgl@langacker.hep.upenn.edu)