Cococubed.com National Nuclear Physics Summer School 2009
Home Astronomy Research    2024 Radiative Opacity    2024 Neutrino Emission from Stars    2023 White Dwarfs & 12C(α,γ)16O    2023 MESA VI    2022 Earendel, A Highly Magnified Star    2022 Black Hole Mass Spectrum    2021 Skye Equation of State    2021 White Dwarf Pulsations & 22Ne    Software Instruments AAS Journals    2024 AAS YouTube    2024 AAS Peer Review Workshops 2024 ASU Energy in Everyday Life 2024 MESA Classroom Outreach and Education Materials Other Stuff:    Bicycle Adventures    Illustrations    Presentations      Equation of State      Stellar Neutrino Emission      The MESA Project      Stellar Neutrinos      Low Energy Nuclear Astrophysics      Celebration of Margaret Burbidge      The MESA Project      Rise of the Elements      White Dwarf Cocktails      Stars and Explosion Models      High Energy Astrophysics      Bonanza of Frontiers      Four Vignettes      Smashing White Dwarfs      Unstable isotopes & Burning      Customizing MESA's pgstar      Hunting SNIa Progenitors      Silicon ejecta from SNIa      NucAstro & Astrobiology      HIPACC SS EOS      NNPSS Lectures      Double degenerate SNIa      Peak Luminosity of SNIa      26Al and 60Fe      A Celebration of Willy Fowler Contact: F.X.Timmes my one page vitae, full vitae, research statement, and teaching statement.	Nuclear Astrophysics Lectures The 2009 school continues the tradition of past NNPSSs The NNPSS is distinctively different from many other schools in that it provides lectures and activities that cover the entire field of contemporary nuclear physics, ranging from QCD and the structure of the nucleon, over the reactions and structure of nuclei, to astrophysics. Particular attention is being paid to fostering interactions between students and lecturers as well as among the students that tend to come from all areas of nuclear science. This not only helps to broaden the perspective of the new generation but also aids in the formation of a community spirit within the field. The school can accommodate 50 students typically within 1-2 years either side of earning a PhD. Goals, nomenclature, forming a network, pp-chains, June 29 CNO cycles, time integration, jacobian formation, June 30 Energy generation, thermodynamic trajectories, big bang nucleosynthesis, July 1 A general network, radioactive isotopes, and the case of 60Fe and 26Al, July 02