Advancing Along the N = Z Line: A 30 Year Odyssey

Details Advancing Along the N = Z Line: A 30 Year Odyssey Advancing Along the N = Z Line: A 30 Year Odyssey

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1012..128l&link_type=abstract

FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2. AIP Conference Proceedings, Volume 1012, pp. 128-133 (

Astronomy and Astrophysics

Astrophysics

Properties Of Nuclei, Nuclear Energy Levels, Shell Model, 59<=A<=89

Scientific paper

N = Z nuclei have always had a special role in nuclear physics due to the symmetry of their wavefunctions, and their anomalously high binding energy. Beyond 56Ni they gain new significance, as they lie close to the proton dripline, and approaching 100Sn, they define the dripline. They are interesting for their structure, for rp-process nucleosynthesis, and as laboratories for weak interaction physics. In this paper I review some currently interesting topics and open questions.

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