Table of Contents

Frontiers in Physics — Editor’s Foreword — Preface to the 2002 Paperback Edition — Standard Model Expectations — Introduction — Standard Model Expectations — Solar Neutrinos. I. Theoretical* — Calcium-37† — New Delayed-Proton Emitters: Ti44, Ca37, AND Ar33 † — Neutrino Opacity I. Neutrino-Lepton Scattering* — Absorption Of Solar Neutrinos In Deuterium* — Solar Neutrinos* — Prediction For Neutrino-Electron Cross-Sections In Weinberg’s Model Of Weak Interactions — Solar neutrino experiments — Solar Neutrino Flux* — Helium Content And Neutrino Fluxes In Solar Models* — A Study Of Solar Evolution — On the Problem of Detecting Solar Neutrinos — Present Status of the Theoretical Predictions for the 36Cl Solar-Neutrino Experiment * — Solar Neutrinos and the Solar Helium Abundance * — Sensitivity of the Solar-Neutrino Fluxes * — More Solar Models and Neutrino Fluxes * † — Standard solar models and the uncertainties in predicted capture rates of solar neutrinos — Solar models, neutrino experiments, and helioseismology — Our Sun. I. The Standard Model — Standard solar models, with and without helium diffusion, and the solor neutrino problem — On the depletion of lithium in the Sun — Standard solar models with CESAM code — Toward a Unified Classical model of the Sun: on the Sensitivity of Neutrinos and Helioseismology to the Microscopic Physics — Solar neutrinos and nuclear reactions in the solar interior — Do solar-neutrino experiments imply new physics? — Effects of Heavy-Element Settling on Solar Neutrino Fluxes and Interior Structure — Solar Neutrino Experiments — Introduction — Solar Neutrino Experiments — National Research Council of Canada division of atomic energy — Solar Neutrinos. II. Experimental* — Limits on Solar Neutrino Flux and Elastic Scattering* — Neutrino-Spectroscopy of Tee Solar Interior * — Detection of Solar Neutrinos by Means of the Ga71(v,e~)Ge71 Reaction — Proposed Solar-Neutrino Experiment Using 7lGa — Direct Approach to Resolve the Solar-Neutrino Problem — Predictions For a Liquid Argon Solar Neutrino Detector — New Tools for Solving the Solar-Neutrino Problem — Radiochemical Neutrino Detection via l27I(ve, e −)l27 Xe — The Superkamiokande — Sudbury Neutrino Observatory — Search for Neutrinos from the Sun* — Solar Neutrinos — The Chlorine Solar Neutrino Experiment — Results from One Thousand Days of Real-Time, Directional Solar-Neutrino Data — Search for Neutrinos from the Sun Using the Reaction 71Ga(v e ,e –)71 Ge — Solar neutrinos observed by GALLEX at Gran Sasso — GALLEX results from the first 30 solar neutrino runs — Results from SAGE — Solar Neutrinos: Proposal for a New Test — Inverse β Decay of 115In → 115Sn*: A New Possibility for Detecting Solar Neutrinos from the Proton-Proton Reaction — Solar Neutrino Production of Technetium-97 and Technetium-98 — Feasibility of a 81Br(v,e –)81Kr Solar Neutrino Experiment — Detection of Solar Neutrinos in Superfluid Helium — Nuclear Fusion Reactions — Introduction — Nuclear Fusion Reactions - Parker — H3(α, γ)Li7 and He3(α,γ)Be7 Reactions — Completion of The Proton-Proton Reaction Chain and The Possibility of Energetic Neutrino Emission by Hot Stars* — Session XA — γ Rays from an Extranuclear Direct Capture Process — Electron Capture and Nuclear Matrix Elements of Be7 † — The Reaction D(p, γ)He3 Below 50 Kev — He3(α, γ)Be7 Reaction* — Termination of The Proton-Proton Chain in Stellar Interiors* — The Effect of Be7 K-Capture on the Solar Neutrino Flux* — The Rate of the Proton-Proton Reaction* — The 7Be Electron-Capture Rate — 3He,(3He, 2p)4He Total Cross-Section Measurements Below the Coulomb Barrier* — Reaction Rates in the Proton-Proton Chain* — Low-Energy 3He(α, γ)7Be Cross-Section Measurements — Proton capture cross section of 7Be and the flux of high energy solar neutrinos — Astrophysical S(E) Factor of 3He(3He, 2p)4He at Solar Energies* — The Fate of 7Be in the Sun — Physics Beyond the Standard Model — Introduction — Physics Beyond the Standard Model - Smirnov — Neutrino Astronomy and Lepton Charge — Lepton Non-Conservation and Solar Neutrinos * — Realistic calculations of solar-neutrino oscillations — “Just So” Neutrino Oscillations — Are Neutrinos Stable Particles?* — Neutrino Decay in Matter — Neutrino Mixing, Decays and Supernova 1987A * — Neutrino oscillations in matter — Matter effects on three-neutrino oscillations — On the detection of cosmological neutrinos by coherent scattering — Resonance enhancement of oscillations in matter and solar neutrino spectroscopy — Neutrino oscillations in a variable-density medium and v-bursts due to the gravitational collapse of stars — Treatment of v ⊙-Oscillations in Solar Matter the MSW Effect — Mikheyev-Smirnov-Wolfenstein enhancement of oscillations as a possible solution to the solar-neutrino problem — Possible Explanation of the Solar-Neutrino Puzzle — Nonadiabatic Level Crossing in Resonant Neutrino Oscillations — Adiabatic Conversion of Solar Neutrinos — Effect Of Neutrino Magnetic Moment On Solar Neutrino Observations — Neutrino electrodynamics and possible consequences for solar neutrinos — Resonant spin-flavor precession of solar and supernova neutrinos — Resonant Amplification of Neutrino Spin Rotation in Matter and the Solar-Neutrino Problem — Testing the principle of equivalence with neutrino oscillations — Mikheyev-Smirnov-Wolfenstein effect with flavor-changing neutrino interactions — On the MSW effect with massless neutrinos and no mixing in the vacuum — Helioseismology — Introduction — Velocity Fields in the Solar Atmosphere — The Five-Minute Oscillations on the Solar Surface* — A New Description of the Solar Five-Minute Oscillation — Observations of Low Wavenumber Nonradial Eigenmodes of the Sun* — Solar structure from global studies of the 5-minute oscillation — Solar oscillations — Internal rotation of the Sun — Seismology of the Sun — The Depth of the Solar Convection Zone — Advances in Helioseismology — Transition from “Problem” to Opportunity” — Introduction — How uncertain are solar neutrino predictions? — Solar 8B and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data — Measurement of the Rate of ve + d→p + p + e- Interactions Produced by 8B Solar Neutrinos at the Sudbury Neutrino Observatory