We report the first evidence of breakup dominance at deep sub-barrier energies for the proton halo nucleus B8 on a heavy target. Angular distribution measurements of the B8 breakup fragment, Be7, on lead were performed at the TwinSol facility of the University of Notre Dame at a beam energy of 30 MeV, 58% of the Coulomb barrier and corresponding to a distance of closest approach of 20.5 fm. The Be7 yield was observed in two double sided silicon strip detector telescopes symmetrical to the radioactive beam and normalized using the B8 Rutherford scattering. The results are in excellent agreement with continuum discretized coupled channel calculations with a total breakup cross section (326±84)mb. This is found to exhaust all of the total reaction cross section for the system B8+Pb208, possibly prohibiting a fusion enhancement. This finding is expected to give more insight to the puzzle of fusion suppression at deep sub-barrier energies with possible major consequences on nuclear astrophysics.

Dominance of direct reaction channels at deep sub-barrier energies for weakly bound nuclei on heavy targets: The case B 8 + Pb 208

Cappuzzello F.;Sgouros O.;Soukeras V.;
2020-01-01

Abstract

We report the first evidence of breakup dominance at deep sub-barrier energies for the proton halo nucleus B8 on a heavy target. Angular distribution measurements of the B8 breakup fragment, Be7, on lead were performed at the TwinSol facility of the University of Notre Dame at a beam energy of 30 MeV, 58% of the Coulomb barrier and corresponding to a distance of closest approach of 20.5 fm. The Be7 yield was observed in two double sided silicon strip detector telescopes symmetrical to the radioactive beam and normalized using the B8 Rutherford scattering. The results are in excellent agreement with continuum discretized coupled channel calculations with a total breakup cross section (326±84)mb. This is found to exhaust all of the total reaction cross section for the system B8+Pb208, possibly prohibiting a fusion enhancement. This finding is expected to give more insight to the puzzle of fusion suppression at deep sub-barrier energies with possible major consequences on nuclear astrophysics.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11769/501343
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