Bahcall, John - Institute for Advanced Study, Princeton University

• Solar Neutrinos: Solved and Unsolved Problems John N. Bahcall
• A&A 383, 291295 (2002) DOI: 10.1051/0004-6361:20011715
• What can we learn from neutrinoless double beta decay experiments? John N. Bahcall,* Hitoshi Murayama,
• Solar fusion cross sections Eric G. Adelberger
• JHEP11(2003)004 Published by Institute of Physics Publishing for SISSA/ISAS
• AN INTRODUCTION TO SOLAR NEUTRINO RESEARCH
• Does the Sun Shine by pp or CNO Fusion Reactions? John N. Bahcall *
• LOCALIZED HELIOSEISMIC CONSTRAINTS ON SOLAR STRUCTURE JOHN N. BAHCALL
• Correlations of solar neutrino observables for SNO John N. Bahcall*
• Disk M Dwarf Luminosity Function From HST Star Counts Andrew Gould ?
• What can we learn from neutrinoless double beta decay experiments? John N. Bahcall,* Hitoshi Murayama, + and C. Pen aGaray #
• JHEPJHEP08(2004)016 Published by Institute of Physics Publishing for SISSA/ISAS
• Electron-screening correction for the proton-proton reaction John N. Bahcall*
• the astrophysical journal, Vol. 144, No. 2, 847--852, May 1966 Copyright 1966 by the University of Chicago, Printed in U.S.A.
• OBSERVATIONAL NEUTRINO ASTROPHYSICS J. N. BAHCALL
• JHEP11(2003)004 Published by Institute of Physics Publishing for SISSA/ISAS
• arXiv:astroph/0412096 How Do Uncertainties in the Surface Chemical Composition of
• HST Images of Twenty Nearby Luminous John N. Bahcall 1 , Sofia Kirhakos 1 , and Donald P. Schneider 2
• JHEP02(2003)009 Published by Institute of Physics Publishing for SISSA/ISAS
• OBSERVATIONAL SEARCHES FOR SOLAR g-MODES: SOME THEORETICAL CONSIDERATIONS PAWAN KUMAR
• JHEP04(2002)007 Published by Institute of Physics Publishing for SISSA/ISAS
• arXiv:astroph/0407060 Helioseismological Implications of Recent Solar Abundance
• THE ASTROPHYSICAL JOURNAL, 542:542547, 2000 October 20 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• Where do we stand with solar neutrino oscillations? J. N. Bahcall
• How well do we ,,and will we... know solar neutrino fluxes and oscillation parameters? J. N. Bahcall and P. I. Krastev
• JHEP07(2002)054 Published by Institute of Physics Publishing for SISSA/ISAS
• The luminosity constraint on solar neutrino fluxes John N. Bahcall*
• 6 August 1998 Z .Physics Letters B 433 1998 18
• THE ASTROPHYSICAL JOURNAL, 504:9961001, 1998 September 10 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• 10,000 STANDARD SOLAR MODELS: A MONTE CARLO SIMULATION John N. Bahcall1
• What DoWe (Not) Know Theoretically about Solar Neutrino Fluxes? John N. Bahcall*
• HOW ACCURATELY CAN WE CALCULATE THE DEPTH OF THE SOLAR CONVECTIVE ZONE? John N. Bahcall and Aldo M. Serenelli
• Solar models and solar neutrino oscillations John N Bahcall and Carlos Pea-Garay
• THE ASTROPHYSICAL JOURNAL, 529:10841100, 2000 February 1 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• VOLUME 78, NUMBER 2 P H Y S I C A L R E V I E W L E T T E R S 13 JANUARY 1997 Are Standard Solar Models Reliable?
• LOCALIZED HELIOSEISMIC CONSTRAINTS ON SOLAR STRUCTURE JOHN N. BAHCALL
• Gallium solar neutrino experiments: Absorption cross sections, neutrino spectra, and predicted event rates
• If sterile neutrinos exist, how can one determine the total solar neutrino fluxes? John N. Bahcall,1,
• Correlations of solar neutrino observables for SNO John N. Bahcall*
• Is a large mixing angle MSW effect the solution of the solar neutrino problems? J. N. Bahcall
• Tests of electron flavor conservation with the Sudbury Neutrino Observatory John N. Bahcall
• What can be learned by measuring the fluxes of the 7 Be and the pep solar neutrino lines?
• Nuclear Physics B (Proc. Suppl.) 77 (1999) 6472 Standard Solar Models
• Solar Neutrinos: Solved and Unsolved Problems John N. Bahcall
• OBSERVATIONAL NEUTRINO ASTROPHYSICS J. N. BAHCALL
• J. Bahcall/Nuclear Physics B (Proc. Suppl.) 48 (1996) 281283 281 Ray Davis: The Scientist and the Man
• Physics Letters B 556 (2003) 16 www.elsevier.com/locate/npe
• VOLUME 78, NUMBER 12 P H Y S I C A L R E V I E W L E T T E R S 24 MARCH 1997 High Energy Neutrinos from Cosmological Gamma-Ray Burst Fireballs
• THE ASTROPHYSICAL JOURNAL, 541:707711, 2000 October 1 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• HST Images of Twenty Nearby Luminous John N. Bahcall1
• JHEP07(2002)054 Published by Institute of Physics Publishing for SISSA/ISAS
• THE ASTROPHYSICAL JOURNAL, 529 : 10841100, 2000 February 1 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• THE ASTROPHYSICAL JOURNAL, 479 : 642658, 1997 April 20 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• THE ASTROPHYSICAL JOURNAL, 541 : 707711, 2000 October 1 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• High energy neutrinos from astrophysical sources: An upper bound Eli Waxman* and John Bahcall +
• JHEPJHEP08(2004)016 Published by Institute of Physics Publishing for SISSA/ISAS
• THE ASTROPHYSICAL JOURNAL, 520 : 6777, 1999 July 20 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• STATUS OF SOLAR MODELS a JOHN BAHCALL
• THE ASTROPHYSICAL JOURNAL, 490 : 437441, 1997 November 20 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• ASTROPHYSICAL JOURNAL, : 9901012, 2001
• THE ASTROPHYSICAL JOURNAL, 479:642658, 1997 April 20 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• Solar models and solar neutrino oscillations John N Bahcall and Carlos PeaGaray
• DOES THE FINESTRUCTURE CONSTANT VARY WITH COSMOLOGICAL EPOCH? John N. Bahcall
• SOLAR NEUTRINOS: WHERE WE ARE JOHN BAHCALL
• Is a large mixing angle MSW effect the solution of the solar neutrino problems? J. N. Bahcall
• Neutrino oscillations and moments of electron spectra J. N. Bahcall and P. I. Krastev
• arXiv:astro-ph/0407060v14Jul2004 Helioseismological Implications of Recent Solar Abundance
• M Dwarfs From Hubble Space Telescope Star Counts III: The Groth Strip
• VOLUME 85, NUMBER 7 P HY S I CA L R E V I E W L E T T E R S 14 AUGUST 2000 5 --10 GeV Neutrinos from GammaRay Burst Fireballs
• 10,000 STANDARD SOLAR MODELS: A MONTE CARLO SIMULATION John N. Bahcall 1
• WHY DO SOLAR NEUTRINO EXPERIMENTS BELOW J. N. BAHCALL
• J.N. Bahcall/Nuclear Physics B (Proc. Suppl.) 91 (2001) 917 9 ASTROPHYSICAL NEUTRINOS: 20th CENTURY AND BEYOND
• ABSORPTION LINES IN THE SPECTRA OF DISTANT OBJECTS 1 John N. Bahcall
• How many #'s is the solar neutrino effect? John N. Bahcall*
• What DoWe (Not) Know Theoretically about Solar Neutrino Fluxes? John N. Bahcall *
• J. Bahcall/Nuclear Physics B (Proc. Suppl.) 48 (1996) 281--283 281 Ray Davis: The Scientist and the Man
• J.N. Bahcall/Nuclear Physics B (Proc. Suppl.) 91 (2001) 9--17 9 ASTROPHYSICAL NEUTRINOS: 20th CENTURY AND BEYOND
• Globular Cluster Photometry with the Hubble Space Telescope. VI. WF/PCI Observations of the Stellar Populations
• If sterile neutrinos exist, how can one determine the total solar neutrino fluxes? John N. Bahcall, 1, * M. C. GonzalezGarcia, 2,3,4,+ and C. Pen aGaray 3,#
• JHEP05(2001)015 Received: March 23, 2001, Accepted: May 7, 2001
• Does the Sun appear brighter at night in neutrinos? J. N. Bahcall and P. I. Krastev
• STATUS OF SOLAR MODELS a JOHN BAHCALL
• AN INTRODUCTION TO SOLAR NEUTRINO RESEARCH
• The luminosity constraint on solar neutrino fluxes John N. Bahcall*
• THE ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 118 1125, 1998 September 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• arXiv:astro-ph/0412096v13Dec2004 How Do Uncertainties in the Surface Chemical Composition of
• Temperature dependence of solar neutrino fluxes John N. Bahcall
• THE ASTROPHYSICAL JOURNAL, 503 : 798808, 1998 August 20 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• HOW ACCURATELY CAN WE CALCULATE THE DEPTH OF THE SOLAR CONVECTIVE ZONE? John N. Bahcall and Aldo M. Serenelli
• JHEP04(2002)007 Published by Institute of Physics Publishing for SISSA/ISAS
• THE ASTROPHYSICAL JOURNAL, 555:9901012, 2001 July 10 V ( 2001. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• The Astrophysical Journal, 621:L85--L88, 2005 March The American Astronomical Society. reserved. Printed
• 24 September 1998 Z .Physics Letters B 436 1998 243250
• How many 's is the solar neutrino effect? John N. Bahcall*
• the astrophysical journal, Vol. 142, No. 4, 1677--1681, November 15, 1965 Copyright 1965 by the University of Chicago, Printed in U.S.A.
• SOLAR NEUTRINOS: WHERE WE ARE JOHN BAHCALL
• Does the Sun Shine by pp or CNO Fusion Reactions? John N. Bahcall*
• SNO: Predictions for ten measurable quantities John N. Bahcall*
• JHEP05(2001)015 Received: March 23, 2001, Accepted: May 7, 2001
• A&A 383, 291--295 (2002) DOI: 10.1051/00046361:20011715
• THE ASTROPHYSICAL JOURNAL, 520:6777, 1999 July 20 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• THE ASTROPHYSICAL JOURNAL, 503:798808, 1998 August 20 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• Where do we stand with solar neutrino oscillations? J. N. Bahcall
• JHEP02(2003)009 Published by Institute of Physics Publishing for SISSA/ISAS
• SNO: Predictions for ten measurable quantities John N. Bahcall*
• High energy neutrinos from astrophysical sources: An upper bound Eli Waxman* and John Bahcall
• High energy astrophysical neutrinos: The upper bound is robust John Bahcall*
• THE ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 118:1125, 1998 September 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• Hubble Deep Field Constraint on Baryonic Dark Matter Chris Flynn
• Standard neutrino spectrum from 8 John N. Bahcall and E. Lisi*
• THE ASTROPHYSICAL JOURNAL, 504 : 9961001, 1998 September 10 1998. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• The Astrophysical Journal, 621:L85L88, 2005 March 1 2005. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• THE ASTROPHYSICAL JOURNAL, 542 : 542547, 2000 October 20 2000. The American Astronomical Society. All rights reserved. Printed in U.S.A.
• Physics Letters (2003) 1--6 www.elsevier.com/locate/npe Has the GZK suppression been discovered?
• JHEP08(2001)014 Received: July 4, 2001, Accepted: August 6, 2001
• THE ASTROPHYSICAL JOURNAL, 490:437441, 1997 November 20 1997. The American Astronomical Society. All rights reserved. Printed in U.S.A.(
• JHEP08(2001)014 Received: July 4, 2001, Accepted: August 6, 2001
• DOES THE FINE-STRUCTURE CONSTANT VARY WITH COSMOLOGICAL EPOCH? John N. Bahcall
• Nuclear Physics B (Proc. Suppl.) 77 (1999) 64--72 Standard Solar Models
• OBSERVATIONAL SEARCHES FOR SOLAR gMODES: SOME THEORETICAL CONSIDERATIONS PAWAN KUMAR 1 AND ELIOT J. QUATAERT
• VOLUME 85, NUMBER 7 P H Y S I C A L R E V I E W L E T T E R S 14 AUGUST 2000 510 GeV Neutrinos from Gamma-Ray Burst Fireballs
• WHY DO SOLAR NEUTRINO EXPERIMENTS BELOW J. N. BAHCALL
• High energy astrophysical neutrinos: The upper bound is robust John Bahcall*