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Presentations from the
Workshop of the RIA Theory Working Group
2-3 November 2003, Westwardlook Resort, Tucson, AZ
From NN to finite Nuclei and Nuclear Matter
Coordinators: A. Brown, J. Dobaczewski, and R. Wiringa
EFT for Nuclei - R. Furnstahl
NN & NNN Interaction and Applications to Light Nuclei - S. Pieper
Modern Shell Model - E. Ormand
Mean Field Applications - J. Dobaczewski
Weak Interaction - A. Brown
Collective Modes - J. Engel
Nuclear Matter & Neutron Stars - M. Hjorth-Jensen
Nuclear Reaction Theory
Coordinators: H. Esbensen and F. Nunes
Reivie on Nuclear Reactions - J. Al-Khalili
Semiclassical Methods and Dynamic Polarization - H. Esbensen
Central Collisions and RIA - Bao-An Li
Numerical Methods for the Continuum - A. Moro
Getting More Structure into Reaction Models - P. Navratil
The Future of Reaction Theory - F. Nunes
Nuclear Astrophysics and Fundamental Symmetries
Coordinators: M. Wiescher and S. Woosley
Nuclear Data far off Stability in Nuclear Astrophysics - M. Wiescher
Nuclear Gross Properties in Nuclear Astrophysics - P. Moller
Statistical Approaches for Nuclei far from Stability - T. Rauscher
Surrogate Reactions for Astrophysics - J. Escher
Shell Structure Signatures in Nuclear Astrophysics - A. Brown
Multi-disciplinary Aspects of RIA Science
Coordinators: A. Bulgac and D. Dean
Testing Dilute Systems - R. Furnstahl
Stockpile Stewardship and RIA - E. Hartouni
Quantum Dots and Chaos - Y. Alhassid