PPT-Invariant-mass spectroscopy of neutron-rich Be isotopes

Contents Breakup reactions of 14 Be on a proton target Inelastic scattering 14 Be Oneneutron removal reaction 13 Be Y Kondo RIKEN Nishina Center 2 Collaborators Y Kondo. Mahata for the S287 LANDFRS Collaboration Gesellschaft f ur Schwerionenforschung GSI D64291 Darmstadt Germany In previous experiments at GSI the LAND collaboration has observed a sizeable fraction of lowlying E1 strength below the giant dipole reson Wolfram KORTEN. CEA . Saclay. DSM/IRFU/. SPhN. Shapes and shells in exotic nuclei. Prolate. Oblate. Quadrupole . deformation. . of. the nuclear ground states. M. Girod, CEA Bruy. ères-le-Châtel. Dominance of . Visit our Exhibitors:. Special Canberra demonstration during poster session Tuesday evening. Session M1. Session M1 (Chair: . Petr. . Navrátil. ).  . 08:45 Jonathan Bagger, . Director of . TRIUMF. What is it?. Isotopes are different versions of atoms having the same number of protons but different numbers of neutrons.. Atomic Mass. The mass of each isotope is different due to the different number of neutrons.. Farrukh. J. . Fattoyev. My TAMUC collaborators: . B.-A. Li, W. G. Newton . My outside collaborators: . C. J. Horowitz, J. . Piekarewicz. , G. . Shen. , J. . Xu. Texas A&M University-Commerce. International Workshop on Nuclear Dynamics and Thermodynamics. Neutrons. Electrons. Charge. 1. 0. -1. Mass . 1 . amu. 1 . amu. 0. Location. nucleus. nucleus. Electron cloud. Isotopes. Atoms that have the same number of protons, but have different numbers of neutrons. Mass measurements on very neutron-rich isotopes with a new Penning trap phase detection technique Guy Savard Argonne National Laboratory & University of Chicago Nuclear Structure 2016 Knoxville, Tennessee, July 25-29, 2016 III. How atoms differ. . A. Atomic Number. Equal to the number of protons – never changes; equals the number of electrons if AND ONLY IF the atom is . neutral. ; Moseley discovered . each atom has a unique number of protons in the nucleus. Piet Van Duppen. ISOLDE CERN, Switzerland. IKS-. K.U.Leuven. , Belgium. K.U. Leuven. University of Western Scotland, U.K. - . K.U.Leuven. , Belgium - SCK-CEN-Mol, Belgium - . U.Gent. , Belgium - . Commenius. 実験. （. J-PARC E15. 実験. ）. の. 解析. 状況. 佐田優太. (. 京都大学、理研. ). Y.SADA for the E15 collaboration. RCNP. 研究会「核子・ハイペロン多体系におけるクラスター現象」 . Part I. . Unstable. vs. . stable. nuclei: . neutron-rich. and . proton-rich. . systems. Limit of . nuclear. . stability. and . definition. of . drip. . lines. From: Exotic Nuclei, J. Enders, TU Darmstadt, Summer 2003. Big Bang . Nucleosynthesis. takes place when the universe is a few minutes old. makes . 2. H, . 3. He, . 4. He and . 7. Li. Fusion in stars. in stars like the Sun, makes . 4. He and C, N, O . in massive stars, makes elements up to iron-56. in neutron . star mergers through . mass measurements . with . the CPT. July 16-27. , . 2018. Jason . clark. FRIB and the GW170817 . kilonova. outline. 2. Role of mass measurements in r-process calculations. Frederick Seward. ABSTRACT. Neutron stars are predicted to be stable over the mass range ≈ 0.1 to ≈ 3M. ⊙. . At 1.4 M. ⊙. , 98% of the mass is in a core with . supernuclear. density and 1-2 % forms a thin crust and atmosphere . As mass...