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Entry No. D1498

T.Motobayashi1, T.Takei1, S.Kox2, C.Perrin2, F.Merchez2, D.Rebreyend2, K.Ieki1, H.Murakami1, Y.Ando1, N.Iwasa1, M.Kurokawa1, S.Shirato1, J.Ruan1, T.Ichihara3, T.Kubo3, N.Inabe3, A.Goto3, S.Kubono4, S.Shimoura5, M.Ishihara3, 5
error1
Grenoble, Isere (CEA and Univ.2
Inst.of Physical and Chemical Res. (RIKEN3
Institute for Nuclear Study, Univ. of Tokyo, Tanashi4
Univ. of Tokyo, Tokyo5
Physics Letters,Section B264(1991)259

Determination of the astrophysical 13N(p,gamma)14O cross section through the Coulomb dissociation method

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DataFilePhysical quantitiesReaction(s)Energies
1 *ENGY-EMT-LAB COUNTS11)
COUNTS: Count number; ENGY-EMT-LAB: Energy of emitted particle in lab. system #5		 208PB(14O,14O)208PB; 87.5 MEV/A
2 *EXC-ENGY-INTRM COUNTS
COUNTS: Count number; EXC-ENGY-INTRM: Excitation energy of intermediate nucleus #2		 208PB(14O,14O)208PB; 87.5 MEV/A
3 *THTC DSIGMA/DOMEGA
DSIGMA/DOMEGA: dsigma/dOmega #1; THTC: Scattering angle theta in c.m. system #4		 208PB(14O,14O)208PB; 87.5 MEV/A
4 *THTC DSIGMA/DOMEGA
DSIGMA/DOMEGA: dsigma/dOmega #1; THTC: Scattering angle theta in c.m. system #4		 208PB(13N,13N)208PB; 78.1 MEV/A
5 *EXC-ENGY RESN-WDTH
EXC-ENGY: Excitation energy (of the final state) #2; RESN-WDTH: Resonance width		 13N(P,GAMMA)14O;
6 *EXC-ENGY RESN-WDTH
EXC-ENGY: Excitation energy (of the final state) #2; RESN-WDTH: Resonance width		 12C(P,GAMMA)13N;

11) Energy spectrum in counts
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