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Title: Neutron capture and total cross sections for /sup 48/Ca: astrophysical implications

Conference ·
OSTI ID:6395745

Attempts to understand abundance anomalies of the Ca isotopes in the Allende meteorite via the n..beta..-process require 30-keV Maxwellian averaged capture cross sections. Experimental data on /sup 48/Ca in this energy region of astrophysical significance is important since a single resonance in this vicinity could dominate the capture cross section. Neutron capture and total cross section measurements have been performed at ORELA on a 9.97-g sample of CaCO/sub 3/, enriched to 96% /sup 48/Ca, over the energy ranges 10 eV to 500 keV (sigma/sub ..gamma../) and 10 keV to 4MeV (sigma/sub T/). Only two small resonances were found for /sup 48/ Ca in the 30-keV energy region (at 19.3 and 106.9 keV) and those only in capture. Their contribution to the 30-keV-averaged cross section is only 50 ..mu..b compared to 1.0 mb calculated from direct capture. The p-wave strength and large d/sub 5/2/ strength observed above 150 keV do not contribute significantly to the 30 keV capture.

Research Organization:
Middle Tennessee State Univ., Murfreesboro (USA); Oak Ridge National Lab., TN (USA)
DOE Contract Number:
AC05-84OR21400; AS05-80ER10710
OSTI ID:
6395745
Report Number(s):
CONF-840906-2; ON: DE85001759
Resource Relation:
Conference: Capture gamma-ray spectroscopy conference, Knoxville, TN, USA, 10 Sep 1984
Country of Publication:
United States
Language:
English