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Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New MgAl Reaction Rate Determined at Gamow Energy
J. Hu, H. Yamaguchi, Y. H. Lam +34
We report the first (in)elastic scattering measurement of with the capability to select and measure in a broad energy range the proton resonances in Si…
Resonances in 19Ne with relevance to the astrophysically important 18F(p,α)15O reaction
D. J. Mountford, A. St J. Murphy, N. L. Achouri +11
The most intense gamma-ray line observable from novae is likely to be from positron annihilation associated with the decay of 18F. The uncertainty in the destruction rate of this n…
Quenching Factor for Low Energy Nuclear Recoils in a Plastic Scintillator
L. Reichhart, D. Yu. Akimov, H. M. Araujo +34
Plastic scintillators are widely used in industry, medicine and scientific research, including nuclear and particle physics. Although one of their most common applications is in ne…
Optimization of the design of OMNIS, the observatory of multiflavor neutrinos from supernovae
J. J. Zach, A. StJ. Murphy, D. Marriott +1
A Monte Carlo code has been developed to simulate the operation of the planned detectors in OMNIS, a supernova neutrino observatory. OMNIS will detect neutrinos originating from a…