Slide 1 1 SOHO, 171A Fe emission line The mass of a nucleus Energy generation in stars which nuclei are stable which nuclei exist in principle Slide 2 2 Nucleons MassSpinCharge…
Degenerate stars There is not a sharp transition between relativistically degenerate and non-relativistically degenerate gas. Similarly there is no sharp transition between…
Coherent p0 Photoproduction on Nuclei Claire Tarbert, University of Edinburgh Spokesperson: Dan Watts Crystal Ball Collaboration Meeting, Basel, October 2006 Claire Tarbert,…
Nucleon correlations and neutron star physics T.Takatsuka (Iwate) and R. Tamagaki (Kyoto) KEK Workshop on 「Short-range correlations and tensor structure…