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Nuclear Physics of Core-Collapse Supernovae. (Report for August 15, 2000-August 14, 2004).

DE2005834073

Publication Date	2004
Page Count	18
Abstract	During the funding period from August 15, 2000 to August 14, 2004, the main foci of my research have been implications of abundances in metal-poor stars for nucleosynthetic yields of supernovae and chemical evolution of the universe, effects of neutrino oscillations and neutrino-nucleus interactions on r-process nucleosynthesis, physical conditions in neutrino-driven winds from proto-neutron stars, neutrino driven mechanism of supernova explosion, supernova neutrino signals in terrestrial detectors, and constraints on variations of fundamental couplings and astrophysical conditions from properties of nuclear reactions. Personnel (three graduate students and a postdoctoral research associate) involved in my research are listed in section 2. Completed research projects are discussed in section 3. Publications during the funding period are listed in section 4 and oral presentations in section 5. Remarks about the budget are given in section 6.
Keywords	Nuclear physics Neutrino oscillation Nuclear reactions Nucleosynthesis Personnel R process Stars Universe Supernovae Neutrinos Core-collapse supernovae
Source Agency	Technical Information Center Oak Ridge Tennessee
Corporate Authors	Minnesota Univ., Minneapolis. School of Physics and Astronomy.; Department of Energy, Washington, DC.
Supplemental Notes	Sponsored by Department of Energy, Washington, DC.
Document Type	Technical Report
NTIS Issue Number	200522

Nuclear Physics of Core-Collapse Supernovae. (Report for August 15, 2000-August 14, 2004).

Nuclear Physics of Core-Collapse Supernovae. (Report for August 15, 2000-August 14, 2004).
DE2005834073

Publication Date	2004
Page Count	18
Abstract	During the funding period from August 15, 2000 to August 14, 2004, the main foci of my research have been implications of abundances in metal-poor stars for nucleosynthetic yields of supernovae and chemical evolution of the universe, effects of neutrino oscillations and neutrino-nucleus interactions on r-process nucleosynthesis, physical conditions in neutrino-driven winds from proto-neutron stars, neutrino driven mechanism of supernova explosion, supernova neutrino signals in terrestrial detectors, and constraints on variations of fundamental couplings and astrophysical conditions from properties of nuclear reactions. Personnel (three graduate students and a postdoctoral research associate) involved in my research are listed in section 2. Completed research projects are discussed in section 3. Publications during the funding period are listed in section 4 and oral presentations in section 5. Remarks about the budget are given in section 6.
Keywords	Nuclear physics Neutrino oscillation Nuclear reactions Nucleosynthesis Personnel R process Stars Universe Supernovae Neutrinos Core-collapse supernovae
Source Agency	Technical Information Center Oak Ridge Tennessee
Corporate Authors	Minnesota Univ., Minneapolis. School of Physics and Astronomy.; Department of Energy, Washington, DC.
Supplemental Notes	Sponsored by Department of Energy, Washington, DC.
Document Type	Technical Report
NTIS Issue Number	200522