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TOF-Brho Mass Measurement of Neutron Rich Nuclei at the NSCL

AIP Conf. Proc. -- October 26, 2007 -- Volume 947, pp. 383-386
VII LATIN AMERICAN SYMPOSIUM ON NUCLEAR PHYSICS AND APPLICATIONS; doi:10.1063/1.2813835

Issue Date: 26 October 2007

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Alfredo Estradé,a,b Milan Matoš,a,c Matthew A. Amthor,a,b Daniel Bazin,a Ana D. Becerril,a,b Thom J. Elliot,a,b Alexandra Gade,a Daniel Galaviz,a,c Giuseppe Lorusso,a,b Jorge Pereira,a,c Mauricio Portillo,a Andrew Rogers,a,b Hendrik Schatz,a,b Dan Shapira,d Edward Smith,e Andreas Stolz,a and Mark S. Wallacef
aNational Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, MI, USA
bDepartment of Physics and Astronomy & Joint Institute for Nuclear Astrophysics, Michigan State University East Lansing, MI, USA
cJoint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, MI, USA
dPhysics Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee, USA
eDepartment of Physics, The Ohio State University, Columbus, OH, USA
fLos Alamos National Laboratory Los Alamos, NM, USA

Experimental knowledge of nuclear masses of exotic nuclei is important for understanding nuclear structure far from the valley of beta-stability, and as a direct input into astrophysical models. In the case of astrophysical processes involving neutron rich nuclei, such as nucleosynthesis during the r-process and the evolution of matter in the crust of an accreting neutron star, we are mostly limited to using theoretical mass models. The time of flight (TOF) mass measurement technique allows measuring very short-lived nuclei. It has been effectively applied using the fast fragment beams produced at the A1900 fragment separator at the National Superconducting Cyclotron Lab (NSCL) to reach masses very far from stability. We describe a recent mass measurement experiment in the neutron rich Fe region performed at the NSCL, and present preliminary results. ©2007 American Institute of Physics
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KEYWORDS and PACS

Keywords
PACS
  • 21.10.Dr
    Nuclear binding energies and masses
  • 21.60.Cs
    Nuclear shell model
  • 26.40.+r
    Cosmic ray nucleosynthesis
  • 26.60.+c
    Nuclear matter aspects of neutron stars
  • YEAR: 2007

PUBLICATION DATA

ISSN:
0094-243X (print)  
Publisher:
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