This volume contains the proceedings of a workshop on Solar Modeling held at the Institute for Nuclear Theory, University of Washington, Seattle during the Spring of 1994.

This workshop was part of a program which concentrated on the nuclear, particle, and astrophysics of the solar neutrino problem, with particular emphasis on the experimental goals and opportunities.

The workshop covered the physics of the standard and alternative solar models, the present status of the solar neutrino problem, the existing uncertainties in the nuclear and atomic physics (opacity) of the standard solar model, and constraints from helioseismology. Among the topics discussed were: the evolution of the rotating sun; solar model independent neutrino observables; the role of convective overshoot and diffusion; and turbulence in the solar interior and the role of g-modes. It was unique in bringing together nuclear, particle, atomic physicists and astrophysicists working on this problem.Contents:

• Grand Unified Theories of Neutrino Mass (L Wolfenstein)
• Nuclear Input for Solar Models — From a Theoretical Viewpoint (K Langanke)
• Solar Neutrinos: Hint for Neutrino Mass (N Hata)
• Clues for Non-Standard Processes in Stellar Interion (C Charbonnel)
• Solar Neutrinos Almost Independently of Solar Models (V Castellani et al.)
• The Combined Effects of Rotation and Diffusion on the Standard Solar Model (P Demarque et al.)
• Solar Models with Convective Overshoot (M Stix)
• Transport Processes Due to Internal Waves (E Schatzman & J Montalbán)
• Measurement of the 3-Neutrino Mixing Matrix Using Long Baseline and Other Neutrino Sources (D B Cline)
• and other papers

Readership: Researchers in nuclear physics, particle physicists and astrophysicists.