Nuclear Structure and Dynamics from Light Nuclei to Neutron Stars

Statistics – Computation

Scientific paper

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Scientific paper

Significant progress has been achieved recently in microscopic studies light nuclei and their reactions. The strong interactions between nucleons depend crucially both upon the spatial coordinates of the nucleons and the orientation of spins and isospins. Electron scattering and hadronic probes have been used to determine many properties of these nuclei, and new studies are underway in parity-violating processes and neutrino scattering. Theoretical models of these processes are rapidly advancing, as are the computational algorithms used to predict their properties. Low energy reactions of astrophysical importance are receiving significant attention. Dramatic recent advances may make it possible to study much larger systems using related Quantum Monte Carlo algorithms, including the dense matter of importance in supernovae and neutron stars. In this talk I will describe our present understanding and abilities, and highlight some of the intriguing problems presently under study.

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