講演会のお知らせ （10/19：Prof. Omar Benhar (Roma, Sapienza))

演題：中性子星核物質の熱平衡・非平衡状態の統一的な記述とその結果について
講師：Prof. Omar Benhar (Roma, Sapienza)
日時：１０月１９日（水）　１６：２０〜
場所：コラボレーション棟３階　コラボレーション室
Abstract: The CBF (Correlated-Basis-Functions) effective interaction approach, whose accuracy was extensively tested studying the properties of the fermion hard-sphere system at T=0, has been extended to describe hot nuclear matter. I will report the results of this effort, and discuss their relevance to the understanding of neutron star structure and dynamics.
Ref. O.Benharet al., Phys. Rev. Lett. 99, 232501 (2007), Phys. Rev. C 81, 024305 (2010); 87, 014601 (2013); 89, 025804 (2014); 91, 034325 (2015); 93, 035802 (2016).

Leaflet    Benhar16Oct19-f.pdf

連絡先：作田　誠（7822）