@article{6bebeac4e9c846ee8d72d619ca0a0f70,
title = "Strong Neutron- γ Competition above the Neutron Threshold in the Decay of Co 70",
abstract = "The β-decay intensity of Co70 was measured for the first time using the technique of total absorption spectroscopy. The large β-decay Q value [12.3(3) MeV] offers a rare opportunity to study β-decay properties in a broad energy range. Two surprising features were observed in the experimental results, namely, the large fragmentation of the β intensity at high energies, as well as the strong competition between γ rays and neutrons, up to more than 2 MeV above the neutron-separation energy. The data are compared to two theoretical calculations: the shell model and the quasiparticle random phase approximation (QRPA). Both models seem to be missing a significant strength at high excitation energies. Possible interpretations of this discrepancy are discussed. The shell model is used for a detailed nuclear structure interpretation and helps to explain the observed γ-neutron competition. The comparison to the QRPA calculations is done as a means to test a model that provides global β-decay properties for astrophysical calculations. Our work demonstrates the importance of performing detailed comparisons to experimental results, beyond the simple half-life comparisons. A realistic and robust description of the β-decay intensity is crucial for our understanding of nuclear structure as well as of r-process nucleosynthesis.",
author = "A. Spyrou and Liddick, {S. N.} and F. Naqvi and Crider, {B. P.} and Dombos, {A. C.} and Bleuel, {D. L.} and Brown, {B. A.} and A. Couture and {Crespo Campo}, L. and M. Guttormsen and Larsen, {A. C.} and R. Lewis and P. M{\"o}ller and S. Mosby and Mumpower, {M. R.} and G. Perdikakis and Prokop, {C. J.} and T. Renstr{\o}m and S. Siem and Quinn, {S. J.} and S. Valenta",
note = "Funding Information: We gratefully acknowledge the support of NSCL operations staff. Financial support from the Research Council of Norway, Project Grant No.{\^A} 205528 (A. C. L and M. G.) and Project Grant No.{\^A} 210007 (L. C. C., T. R., and S. S.) is gratefully acknowledged. A. C. L. acknowledges funding through the ERC-STG-2014 under Grant Agreement No.{\^A} 637686. D. L. B. acknowledges the support of LLNL under Contract No.{\^A} DE-AC52-07NA27344. The LANL work was carried out under the auspices of the NNSA of the U.S. Department of Energy at Los Alamos National Laboratory under Contract No.{\^A} DE-AC52-06NA25396. This work was supported by the National Science Foundation under Grants No.{\^A} PHY 1102511 (NSCL), No.{\^A} PHY 1404442, No.{\^A} PHY 0822648 (Joint Institute for Nuclear Astrophysics), and No.{\^A} PHY 1350234 (CAREER). This work was also supported by NNSA Grants No.{\^A} DE-NA-0000979 and No.{\^A} DE-NA-0002132. Publisher Copyright: {\textcopyright} 2016 American Physical Society.",
year = "2016",
month = sep,
day = "29",
doi = "10.1103/PhysRevLett.117.142701",
language = "English",
volume = "117",
journal = "Physical Review Letters",
issn = "0031-9007",
publisher = "Physical Review Letters",
number = "14",
}