TY - JOUR
T1 - Energy-broadened proton beam for production of quasi-stellar neutrons from the 7Li(p,n)7Be reaction
AU - Feinberg, G.
AU - Shor, A.
AU - Berkovits, D.
AU - Eisen, Y.
AU - Friedman, M.
AU - Giorginis, G.
AU - Hirsh, T.
AU - Krása, A.
AU - Paul, M.
AU - Plompen, A.
AU - Tsuk, E.
PY - 2012
Y1 - 2012
N2 - Production of quasi-stellar neutrons by the 7Li(p,n) 7Be reaction has been used for measuring s-process cross sections and efforts to upgrade the proton beam intensity with RF linear accelerators are presently ongoing. We investigated the effect of an energy-broadened proton beam, as is expected for a RF linear accelerator, on the produced 25-keV quasi-Maxwellian neutron spectrum and compared it to that of a Van de Graaff accelerator with well-defined proton energy. Neutron spectrum measurements from 0° to 80° were carried out with a pulsed proton beam at the IRMM Van de Graaff accelerator using time-of-flight techniques, both with a narrow energy spread (σ≈1.5 keV) proton beam and with an energy-broadened beam (σ≈20 keV) obtained by straggling through a Au-foil degrader. In the latter case, the neutron spectrum is closer to the Maxwellian flux distribution in the high neutron energy region.
AB - Production of quasi-stellar neutrons by the 7Li(p,n) 7Be reaction has been used for measuring s-process cross sections and efforts to upgrade the proton beam intensity with RF linear accelerators are presently ongoing. We investigated the effect of an energy-broadened proton beam, as is expected for a RF linear accelerator, on the produced 25-keV quasi-Maxwellian neutron spectrum and compared it to that of a Van de Graaff accelerator with well-defined proton energy. Neutron spectrum measurements from 0° to 80° were carried out with a pulsed proton beam at the IRMM Van de Graaff accelerator using time-of-flight techniques, both with a narrow energy spread (σ≈1.5 keV) proton beam and with an energy-broadened beam (σ≈20 keV) obtained by straggling through a Au-foil degrader. In the latter case, the neutron spectrum is closer to the Maxwellian flux distribution in the high neutron energy region.
UR - http://www.scopus.com/inward/record.url?scp=84857943995&partnerID=8YFLogxK
U2 - 10.1088/1742-6596/337/1/012044
DO - 10.1088/1742-6596/337/1/012044
M3 - ???researchoutput.researchoutputtypes.contributiontojournal.conferencearticle???
AN - SCOPUS:84857943995
SN - 1742-6588
VL - 337
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
IS - 1
M1 - 012044
T2 - 5th Bi-Annual Nuclear Physics in Astrophysics, NPA5
Y2 - 3 April 2011 through 8 April 2011
ER -