Prediction of Observable Polarization-Analyzing-Power Differences in <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mmultiscripts><mrow><mi mathvariant="normal">B</mi></mrow><mprescripts></mprescripts><mrow></mrow><mrow><mn>11</mn></mrow><mrow></mrow><mrow></mrow></mmultiscripts></mrow></math>(<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>p</mi></math>,<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mi>n</mi></math>)<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mmultiscripts><mrow><mi mathvariant="normal">C</mi></mrow><mprescripts></mprescripts><mrow></mrow><mrow><mn>11</mn></mrow><mrow></mrow><mrow></mrow></mmultiscripts></mrow></math>

R. J. Philpott; Dean Halderson

doi:10.1103/PhysRevLett.43.1785

Prediction of Observable Polarization-Analyzing-Power Differences in ${}^{11}B$ ( $p$ , $n$ ) ${}^{11}C$

R. J. Philpott and Dean Halderson

Phys. Rev. Lett. 43, 1785 – Published 10 December 1979

Abstract

Polarization-analyzing-power differences in ${}^{11}B$ ( $p$ , $n$ ) ${}^{11}C$ are predicted to be observable at selected energies below $E_{p} \sim 10$ MeV at the level of $| P - A | ≳ 0.1$ . This result is derived from recoil-corrected continuum shell-model calculations in the one-particle, one-hole approximation, using a realistic $g$ -matrix interaction.