Measurements with $^7$Be beams at the HRIBF

ORAL

Abstract

A $^7$Be beam has been used at the HRIBF to study important reactions in stellar burning. Precise knowledge of the $^7$Be($p,\gamma$)$^8$B rate is important for interpreting solar neutrino flux observations. A direct measurement of the $^7$Be($p,\gamma$)$^8$B cross section is being made by bombarding a H$_2$ gas target with a $^7$Be beam and counting $^8$B recoils at the focal plane of the DRS mass spectrometer. The $^3$He($^3$He,2$p$)$^4$He reaction also occurs in stellar burning, but interpretation of low energy measurements have been hindered by a surprisingly strong low-energy rise in the cross section. This rise could, in part, be due to broad $^6$Be resonances. We have studied $^2$H($^7$Be,$t$)$^6$Be to search for any such broad $^6$Be levels. Initial results from these measurements will be presented.

*ORNL is managed by UT-Battelle, LLC for the U.S. DOE under Contract No. DE-AC05-00OR22725.

Authors

  • D.W. Bardayan

  • J.C. Blackmon

  • J.J. Das

  • C.D. Nesaraja

  • M.S. Smith

  • D.W. Stracener

    • ORNL
  • K.Y. Chae

  • Z. Ma

    • U. Tenn.
  • A.E. Champagne

  • R. Fitzgerald

  • D.W. Visser

    • UNC
  • U. Greife

  • R.J. Livesay

    • Colorado School of Mines
  • V. Guimaraes

    • U. Sao Paulo
  • J. Howard

  • R.L. Kozub

    • Tenn. Tech. U.
  • M.S. Johnson

    • ORAU
  • K.L. Jones

  • S.D. Pain

  • J.S. Thomas

    • Rutgers
  • P.D. Parker

    • Yale