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Gamow-Teller Strength in the Exotic Odd-Odd Nuclei La138 and Ta180 and Its Relevance for Neutrino Nucleosynthesis

A. Byelikov, T. Adachi, H. Fujita, K. Fujita, Y. Fujita, K. Hatanaka, A. Heger, Y. Kalmykov, K. Kawase, K. Langanke, G. Martínez-Pinedo, K. Nakanishi, P. von Neumann-Cosel, R. Neveling, A. Richter, N. Sakamoto, Y. Sakemi, A. Shevchenko, Y. Shimbara, Y. Shimizu, F. D. Smit, Y. Tameshige, A. Tamii, S. E. Woosley, and M. Yosoi
Phys. Rev. Lett. 98, 082501 – Published 23 February 2007

Abstract

The Gamow-Teller strength distributions below the particle threshold in La138 and Ta180, deduced from high-resolution measurements of the (He3,t) reaction at 0°, allow us to evaluate the role of charged-current reactions for the production of these extremely rare nuclides in neutrino-nucleosynthesis models. The analysis suggests that essentially all La138 in the Universe can be made that way. Neutrino nucleosynthesis also contributes significantly to the abundance of Ta180 but the magnitude depends on the unknown branching ratio for population of the long-lived isomer.

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  • Received 28 October 2006

DOI:https://doi.org/10.1103/PhysRevLett.98.082501

©2007 American Physical Society

Authors & Affiliations

A. Byelikov1, T. Adachi2, H. Fujita3,4, K. Fujita5, Y. Fujita2, K. Hatanaka5, A. Heger6,7, Y. Kalmykov1, K. Kawase5, K. Langanke1,8, G. Martínez-Pinedo8, K. Nakanishi5, P. von Neumann-Cosel1,*, R. Neveling4, A. Richter1, N. Sakamoto5, Y. Sakemi5, A. Shevchenko1, Y. Shimbara2,†, Y. Shimizu5, F. D. Smit4, Y. Tameshige5, A. Tamii5, S. E. Woosley7, and M. Yosoi5

  • 1Institut für Kernphysik, Technische Universität Darmstadt, D-64289 Darmstadt, Germany
  • 2Department of Physics, Osaka University, Toyonaka, Osaka 560-0043, Japan
  • 3School of Physics, University of the Witwatersrand, PO Wits, Johannesburg 2050, South Africa
  • 4iThemba LABS, PO Box 722, Somerset West 7129, South Africa
  • 5Research Center for Nuclear Physics, Osaka University, Ibaraki, Osaka 567-0047, Japan
  • 6Theoretical Astrophysics Group, MS B227, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
  • 7Department of Astronomy and Astrophysics, University of California, Santa Cruz, California 95064, USA
  • 8Gesellschaft für Schwerionenforschung, D-64291 Darmstadt, Germany

  • *Email address: vnc@ikp.tu-darmstadt.de
  • Present address: NSCL, Michigan State University, East Lansing, MI 48824, USA.

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Issue

Vol. 98, Iss. 8 — 23 February 2007

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