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Observation of the Isovector Giant Monopole Resonance via the
Scott, M; Zegers, R G T; Almus, R; Austin, Sam M; Bazin, D; Brown, B A; Campbell, C; Gade, A; Bowry, M; Galès, S; Garg, U; Harakeh, M N; Kwan, E; Langer, C; Loelius, C; Lipschutz, S; Litvinova, E; Lunderberg, E; Morse, C; Noji, S; Perdikakis, G; Redpath, T; Robin, C; Sakai, H; Sasamoto, Y; Sasano, M; Sullivan, C; Tostevin, J A; Uesaka, T; Weisshaar, D.
Afiliação
  • Scott M; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Zegers RGT; Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA.
  • Almus R; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
  • Austin SM; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Bazin D; Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA.
  • Brown BA; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
  • Campbell C; Department of Physics, Central Michigan University, Mount Pleasant, Michigan 48859, USA.
  • Gade A; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Bowry M; Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA.
  • Galès S; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
  • Garg U; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Harakeh MN; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Kwan E; Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA.
  • Langer C; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
  • Loelius C; Lawrence Berkeley National Laboratory, Berkeley, California 94720, USA.
  • Lipschutz S; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Litvinova E; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
  • Lunderberg E; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Morse C; IPN Orsay, CNRS-IN2P3, Université Paris-Sud, Université Paris-Saclay, 91406 Orsay Cedex, France.
  • Noji S; Horia Hulubei National Institute of Physics and Nuclear Engineering, P.O. Box MG6, Bucharest, Romania.
  • Perdikakis G; Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA.
  • Redpath T; Kernfysisch Versneller Instituut-Center for Advanced Radiation Technology, University of Groningen, Groningen, 9747 AA, Netherlands.
  • Robin C; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Sakai H; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Sasamoto Y; Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA.
  • Sasano M; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Sullivan C; Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA.
  • Tostevin JA; Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824, USA.
  • Uesaka T; National Superconducting Cyclotron Laboratory, Michigan State University, East Lansing, Michigan 48824, USA.
  • Weisshaar D; Joint Institute for Nuclear Astrophysics, Michigan State University, East Lansing, Michigan 48824, USA.
Phys Rev Lett ; 118(17): 172501, 2017 Apr 28.
Article em En | MEDLINE | ID: mdl-28498679
The (^{10}Be,^{10}B^{*}[1.74 MeV]) charge-exchange reaction at 100 AMeV is presented as a new probe for isolating the isovector (ΔT=1) nonspin-transfer (ΔS=0) response of nuclei, with ^{28}Si being the first nucleus studied. By using a secondary ^{10}Be beam produced by fast fragmentation of ^{18}O nuclei at the NSCL Coupled Cyclotron Facility, applying the dispersion-matching technique with the S800 magnetic spectrometer to determine the excitation energy in ^{28}Al, and performing high-resolution γ-ray tracking with the Gamma-Ray Energy Tracking In-beam Nuclear Array (GRETINA) to identify the 1022-keV γ ray associated with the decay from the 1.74-MeV T=1 isobaric analog state in ^{10}B, a ΔS=0 excitation-energy spectrum in ^{28}Al was extracted. Monopole and dipole contributions were determined through a multipole-decomposition analysis, and the isovector giant dipole resonance and isovector giant monopole resonance (IVGMR) were identified. The results show that this probe is a powerful tool for studying the elusive IVGMR, which is of interest for performing stringent tests of modern density functional theories at high excitation energies and for constraining the bulk properties of nuclei and nuclear matter. The extracted distributions were compared with theoretical calculations based on the normal-modes formalism and the proton-neutron relativistic time-blocking approximation. Calculated cross sections based on these strengths underestimate the data by about a factor of 2, which likely indicates deficiencies in the reaction calculations based on the distorted wave Born approximation.

Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2017 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2017 Tipo de documento: Article