Zero-degree differential cross sections and D{sub NN} values for the {sup 17,18}O({rvec p},{rvec n}){sup 17,18}F reactions at E{sub p}=118 MeV

Journal Article · Mon Mar 01 04:00:00 EST 1999 · Physical Review, C

DOI:https://doi.org/10.1103/PhysRevC.59.1488· OSTI ID:322008

van Heerden, I J; Goodman, C D; Foster, C C ^[1]; Palarczyk, M; Dehnhard, D; ODonnell, J M ^[2]; Wang, X; Rapaport, J; Hicks, K; Wang, L; Yang, X ^[3]; Prout, D L; Sugarbaker, E ^[4]; Luther, B A ^[5]; Taddeucci, T N ^[6]; Ohnuma, H ^[7]; Park, B K; Burleson, G R; Blanchard, S ^[8]

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1. Indiana University Cyclotron Facility, Bloomington, Indiana 47405 (United States)
2. University of Minnesota, Minneapolis, Minnesota 55455 (United States)
3. Ohio University, Athens, Ohio 45701 (United States)
4. The Ohio State University, Columbus, Ohio 43210 (United States)
5. Concordia College, Moorhead, Minnesota 56562 (United States)
6. Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States)
7. Chiba Institute of Technology, Narashino 275-0023, Chiba (Japan)
8. New Mexico State University, Las Cruces, New Mexico 88003 (United States)

We present zero-degree differential cross sections and transverse spin-transfer coefficients D{sub NN}(0{degree}) for the {sup 17,18}O({rvec p},{rvec n}){sup 17,18}F reactions at E{sub p}=118 MeV. For the transition to the {sup 17}F(g.s.) to which several multipoles contribute, the measured D{sub NN}(0{degree})={minus}0.13{plus_minus}0.05 is used to separate the Fermi and Gamow-Teller contributions at 0{degree}. The empirical Gamow-Teller strengths and the Fermi strengths are employed to estimate the solar neutrino absorption cross section in {sup 17}O and {sup 18}O. {copyright} {ital 1999} {ital The American Physical Society}

• OSTI ID: 322008
• Journal Information: Physical Review, C, Journal Name: Physical Review, C Journal Issue: 3 Vol. 59; ISSN 0556-2813; ISSN PRVCAN
• Country of Publication: United States
• Language: English

Related Subjects

66 PHYSICS
DIFFERENTIAL CROSS SECTIONS
FLUORINE 17
FLUORINE 18
GAMOW-TELLER RULES
OXYGEN 17 TARGET
OXYGEN 18 TARGET
PROTON REACTIONS
SOLAR NEUTRINOS
SPIN