ASTROPHYSICAL S(E) FACTOR OF B-13(P,ALPHA(1))BE-7 AT LOW ENERGIES

Authors
ANGULO C SCHULTE WH ZAHNOW D RAIMANN G ROLFS C
Citation
C. Angulo et al., ASTROPHYSICAL S(E) FACTOR OF B-13(P,ALPHA(1))BE-7 AT LOW ENERGIES, ZEITSCHRIFT FUR PHYSIK A-HADRONS AND NUCLEI, 345(3), 1993, pp. 333-334
Citations number
2
Categorie Soggetti
Physics, Nuclear","Physics, Particles & Fields
Journal title
ZEITSCHRIFT FUR PHYSIK A-HADRONS AND NUCLEI → ACNP
ISSN journal
09397922
Volume
345
Issue
3
Year of publication
1993
Pages
333 - 334
Database
ISI
SICI code
0939-7922(1993)345:3<333:ASFOBA>2.0.ZU;2-T
Abstract
The absolute cross section of the fusion reaction B-10(p,alpha1gamma)B e-7 has been measured at the c.m. energy range E = 48 to 159 keV via t he 429 keV secondary gamma-ray transition. The studies involved high p roton currents and thick solid B-10 targets. The resulting cross secti ons have the same energy dependence as those of the B-10(p,alpha0)Be-7 reaction but they are lower by a factor 600.