Implications of 151Sm(n,γ) Cross Section at n_TOF

Details Implications of 151Sm(n,γ) Cross Section at n_TOF Implications of 151Sm(n,γ) Cross Section at n_TOF

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..831..502m&link_type=abstract

FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS - FINUSTAR. AIP Conference Proceedings, Volume 831, pp. 502-504 (20

Astronomy and Astrophysics

Astrophysics

Radiative Capture, 150<=A<=189, Spectrometers And Spectroscopic Techniques

Scientific paper

The accurate knowledge of the 151Sm(n,γ) cross section has important implications for the nuclear technologies as well as for fundamental studies. Due to its radioactivity, the only experimental data available on 151Sm were derived from a transmission measurement. Nowadays thanks to the innovative features of neutron time-of-flight facility (n_TOF), it was possible to measure 151Sm(n,γ) cross section in a wide energy range and with good accuracy. We present, here, the main experimental results together with the implications concerning the nuclear astrophysical part.

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