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Solar Neutrinos
A. A. Shikhin
A. Bevilacqua
A. Claverie
A. G. W. Cameron
A. I. Abazov
A. J. Elwyn+
A. J. Howard
A. K. Mann
A. Krauss
A. M. Poskanzer
A. M. Pshukov
A. Masiero
A. Suzuki
A. V. Kalikhov
A. V. Ostrinsky
A. Yu. Smirnov
A.M. Shalagin
A.O. Gusev
A01=Jr. Davis
A01=Peter Parker
A01=Raymond Davis
A01=Roger Ulrich
Albert Messiah
Alexei Smirnov
Amos Yahill
Arnold I. Boothroyd
Arturo Cisneros
astrophysical modeling
Author_Jr. Davis
Author_Peter Parker
Author_Raymond Davis
Author_Roger Ulrich
B. A. Brown
B. Abreus
B. Pontecorvo
B. T. Cleveland
B. W. Filippone*
C. A. Barnes
C. Bacci
C. Cattadori
C. D. Scarfe
C. H. Chen
C. N. Davids
C. P. McLeod
C. Rolfs
C. Rubbia
C. Schlosser
C. Tao
C. W. Johnson
C.K. Lee
Category=PHP
Category=PHVB
chain
Charles P. Moeller
Charles R. Proffitt
Chong-Sa Lim
convective
Convective Zone
Cross-section Factor
D. D. Koetke
D. Ezer
D. L. Wark
D. O. Gough ?
D. Vignaud
D.B. Cline
Don S. Harmer
E. Bellotti
E. D. Frank
E. Fiorini
E. Henrich
E. Kodera
E. Kolbe
E. L. Faizov
E. P. Veretenkin
E. Pernicka
E. Schatzman
E. W. Bcicr
E.Kh. Akhmedov
Electron Neutrino
eq_bestseller
eq_isMigrated=1
eq_isMigrated=2
eq_nobargain
eq_non-fiction
eq_science
Eric Fossat +
Esteban Roulet
experiment
F. J. Schima
F. M. Newcomer
F. Reines
F. v. Feilitzsch
F. von Feilitzsch
F. Weirich
F. Weyrich
F.X. Hartmann
Fletcher Gabbard
flux
Francis J. Kelly
Franz-Ludwig Deubner
G. 't Hooft
G. A. Cowan
G. Berthomieu
G. Dupont
G. Fiorentini
G. Friedlander
G. Heusser
G. J. Mathews
G. M. Griffiths
G. M. Seidel
G. R. Isaak
G. S. Hurst
G. T. Zalscpin
G.T. Ewan
G.T. Zatsepin
Gallium Experiment
George W. Simon
Gerard Grec*
Giora Shaviv
H. A. Bethe
H. A. O'Brien
H. B. van der Raay
H. D. Holmgren
H. J. Maris
H. Lalla
H. Miyata
H. Takei
H. Uberall
H. Winkler
H.P. Trautvetter
H.W. Becker
heavy element abundance
helioseismic analysis
Herbert H. Chen
Howard E. Haber
hydrogen fusion process
I. Carmi
I. Dostrovsky
I. N. Mirmov
I.-Juliana Sackmann
I.I. Knyshenko
Ian Duck
Icko Iben
Icko Jr. Iben
Ilidio Lopes
interior
J. C. Evans
J. C. Hardy
J. Christensen-Dalsgaard
J. F. Wilkerson
J. K. Rowley
J. Kiko
J. L. Osborne
J. L. Zyskind
J. Leibacher
J. M. Gelb
J. N. Bahcall
J. Provost
J. Rich
J. W. Harvey ||
J. W. Leibacher||
J. Weneser
J.N. Abdurashitov
J.S. Nico
Jacques P. Leveille
John Bahcall
John Bahcalld
John N. Bahcall
John N. Bancall
Jon Sheiman
Joshua A. Frieman
Jr.
Judah Schwartz
K. G. Libbrecht
K. Hellriegel
K. Inoue
K. Kaneyuki
K. Kihara
K. Lande
K. Langanke
K. Miyano
K. Nakamura
K. S. Hirata
K. Takahashi
K. Whisnant
K. Winter
K.H. Ebert
Katherine Freese
Kenneth C. Hoffman
Kenneth Kalata
L. B. Okun
L. Dostrovsky
L. Gosset
L. Paoluzi
L. R. Feldscher
L. Stieglitz
L. Wolfenstein
L. Zanotti
Lawrence M. Krauss
Lower Energy Neutrinos
M. Altmann
M. B. Voloshin
M. Balata
M. Baldo-Ceolin
M. Cribier
M. F. Woodard
M. Gasperini
M. H. Pinsonneault
M. I. Vysotsku
M. J. Thompson
M. Koshiba
M. L. Cherry
M. Lal
M. Laubenstein
M. Mori
M. Nakahata
M. R. Dwarakanath
M. Sann
M. Spiro
M. Stix
M. Takita
M. Thorn
M. Wjcik
M. Wojcik
M. Yamada
M.I. Vysotsky
M.M. Guzzo
Martin Pomerantz ?
Masato Takita
Mixing Angles
model
N. E. Revzin
N. Ferrari
N. Sato
NA Bahcall
NA Davis
Neta A. Bahcall
Neta A. Bahcallt
Neutrino Capture
Neutrino Capture Rate
Neutrino Decay
Neutrino Flux
Neutrino Masses
Neutrino Oscillations
Nicola Cabibbo
O. Cremonesi
O. L. Anosov
Oscillation Length
oscillations
P. Anselmann
P. Belli
P. D. Pajuces
P. D. Parker
P. L. Reeder
P. Morel
P. R. Goode ?
P. V. Timofeyev
P.W. Wildenhain
particle physics theory
Paul Langacker
Peter D. Parker
Peter Parker
Predicted Capture Rates
problem
proton
Proton Proton Chain
R. A. Esterlund
R. Bernabei
R. Davis
R. E. Lanou
R. F. Christy
R. F. Stein
R. I. Verrall
R. J. N. Phillips
R. K. Rowley
R. L. Johnston
R. L. Sears
R. M. Kremer
R. Mossbauer
R. Plaga
R. S. Raghavan
R. T. Kouzes
R. v. Ammon
R. Van Berg
R. von Ammon
R. W. Kavanagh
R. W. Stoenner
R. Wink
R.L. Hahn
Ralph W. Kavanagh
Raymond Davis
Robert B. Leighton
Robert M. May
Robert W. Noyes
Roger K. Ulrich
Roger Ulrich
S. A. Mezentseva
S. B. Kim
S. C. Frautschi
S. Charbit
S. d'Angelo
S. D. Kramer
S. Degl'Innocenti
S. E. Koontn
S. Ohara
S. P. Mikheev
S. P. Rosen
S. Pakvasa
S. Pezzoni
S. R. Elliott
S.T. Petcov
Sandip Pakvasa
Sarbani Basu
Sheldon L. Glashow
Solar Interior
Solar Model
Solar Model Calculations
Solar Neutrino
Solar Neutrino Detectors
Solar Neutrino Experiment
Solar Neutrino Flux
solar neutrino flux uncertainty
Solar Neutrino Problem
Solar Neutrino Units
standard
Standard Solar Model
stellar nucleosynthesis
Stephen H. Lubow
Stephen J. Parke
Sylvaine Turck-Chieze
T. Daily
T. Fritsch
T. J. Bowles
T. Kajita
T. Kifune
T. Kirsten
T. L. Duvall
T. Roca Cortes
T. Stolarczyk
T. Suda
T. Tajima
T. Tanimori
T. V. Knodel
U. Ronn
U. Schanda
V. A. Kuz'min
V. Bargcr
V. Barger
V. Castellani
V. Gribov
V. M. Vermul
V. N. Gavrin
V. N. Kornoukhov
W. A. Dziembowsk +
W. C. Haxton
W. Frati
W. Hampel
W. R. Kropp
W. Zhang
W.A. Teasdale
Walter F. Huebner
William A. Fowler
William J. Marciano
Y. Fukuda
Y. Lebreton
Y. Nagashima
Y. Oyama
Y. Suzuki
Y. Totsuka
Y. Yaginuma
Z.G. Berezhiani
Zulema Abraham
Product details
- ISBN 9780813340371
- Weight: 453g
- Dimensions: 152 x 229mm
- Publication Date: 05 Sep 2002
- Publisher: Taylor & Francis Inc
- Publication City/Country: US
- Product Form: Paperback
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A variety of evolutionary sequences of models for the solar interior has been computed, corresponding to variations in input data, to obtain some idea of the uncertainties involved in predicting a solar neutrino flux. It is concluded that the neutrino flux can be estimated to within a factor of 2, the primary uncertainty being the initial homogeneous solar composition; detailed results are given. With a preferred value of the heavy-element-to-hydrogen ratio Z/X = 0.028, the helium content necessary to fit a model to the observed solar luminosity is found to be Y = 0.27.
John Bahcall has held positions at Indiana University, Caltech, and the Institute for Advanced Study. He is currently the Richard Black Professor of Natural Sciences at the Institute for Advanced Study and Visiting Lecturer with rank of Professor at Princeton University. He has received numerous awards, including the National Medal of Science and the Hans Bethe Prize from the American Physical Society in 1998. He has written several books, including Unsolved Problems in Astrophysics and The Decade of Discovery in Astronomy and Astrophysics He was recently awarded the Dan David prize for his wide-ranging contributions, given by the Tel Aviv-based Dan David Foundation. Peter Parker is Professor of Physics and Astronomy at Yale University in the Wright Nuclear Structure labouratory. Since his graduate student days, Parker has performed labouratory experiments to study nuclear reactions that are important in stars. Roger Ulrich is professor of Astronomy at the University of California, Los Angeles, and is active in the study of the solar interior using theoretical and observational methods. He first interpreted the periodic fluctuations observed on the solar surface as the solar analogue of terrestrial seismic waves. Raymond Davis, Jr. retired from a prestigious career at Brookhaven Lab, a multi-program national labouratory operated for the U.S. Dept. of Energy, to become a research professor at the University of Pennsylvania in 1984. A member of the National Academy of Sciences, Davis has won numerous scientific awards, including the Tom W. Bonner Prize in 1988 and the W.K.H. Panofsky Prize in 1992. Alexei Smirnov is senior research scientist at the International centre for Theoretical Physics (Trieste, Italy), and is also a leading research scientist at the Institute for nuclear research of the Russian Academy of Sciences in Moscow. Smirnov is a co-discoverer of the MSW (Mikhayev-Smirnov-Wolfenstein) effect, which describes how matter can enhance the flavor conversion of neutrinos, and is a leading particle phenomenologist.
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