48 citations · 150 across the 6 of their papers we have counts for
6 papers
Confirmation of the isomeric state in 26P
D. Pérez-Loureiro, C. Wrede, M. B. Bennett +20
We report the independent experimental confirmation of an isomeric state in the proton drip-line nucleus P. The -ray energy and half-life determined are 164.4 0.3 (…
Isobaric multiplet mass equation in the quartets
M. B. Bennett, C. Wrede, B. A. Brown +20
The observed mass excesses of analog nuclear states with the same mass number and isospin can be used to test the isobaric multiplet mass equation (IMME), which has, in mos…
Beta-delayed gamma decay of 26P: Possible evidence of a proton halo
D. Pérez-Loureiro, C. Wrede, M. B. Bennett +23
Background: Measurements of decay provide important nuclear structure information that can be used to probe isospin asymmetries and inform nuclear astrophysics studies. Purpose…
Isospin Mixing Reveals P()S Resonance Influencing Nova Nucleosynthesis
M. B. Bennett, C. Wrede, B. A. Brown +21
The thermonuclear P()S reaction rate is critical for modeling the final elemental and isotopic abundances of ONe nova nucleosynthesis, which affect the calibrati…
Observation of Doppler broadening in -delayed proton- decay
S. B. Schwartz, C. Wrede, M. B. Bennett +22
Background: The Doppler broadening of -ray peaks due to nuclear recoil from -delayed nucleon emission can be used to measure the energies of the nucleons. This method has nev…
Classical-Nova Contribution to the Milky Way's Al Abundance: Exit Channel of the Key Al()Si Resonance
M. B. Bennett, C. Wrede, K. A. Chipps +21
Classical novae are expected to contribute to the 1809-keV Galactic -ray emission by producing its precursor Al, but the yield depends on the thermonuclear rate of the un…