Neutrino-Nucleus Reactions in Effective Field Theory

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Neutrino-nucleus reactions play important roles not only as a tool for probing nuclear structure and/or the structure of fundamental weak interactions but also as means of measuring various astrophysical neutrinos in laboratories. A prominent example of the latter case is the neutrino-deuterium reaction used in a very recent SNO experiment [1] which has given strong evidence for νe oscilations. The interpretation of the SNO data crucially depends on the reliability of theoretical estimates of the ν-d cross sections [2,3]. A recent development of nuclear effective field theory [4] is expected to shed much light on this issue. My talk will cover this and several other topics related to electroweak processes in light nuclei. References: [1] Q.R. Ahmad et al., nucl-ex/0106015; [2] S. Nakamura, T. Sato, V. Gudkov and K. Kubodera, Phys. Rev. C 63, 034617 (2001); [3] M. Butler, J.-W. Chen and X. Kong, Phys. Rev. C 63, 035501 (2001); [4] T.-S. Park, L.E. Marcucci, R. Sciavilla, M. Viviani, A. Kievsky, R. Rosati, K. Kubodera, D.-P. Min and M. Rho, nucl-th/0106025.

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