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NSR database version of April 11, 2024.

Search: Author = H.B.Prosper

Found 3 matches.

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2016UT01      Phys.Rev. C 93, 014311 (2016)

R.Utama, J.Piekarewicz, H.B.Prosper

Nuclear mass predictions for the crustal composition of neutron stars: A Bayesian neural network approach

ATOMIC MASSES A=40-240, Z=20-92; analyzed experimental masses from AME-2012 to deduce liquid-drop-model parameters and uncertainties, analyzed theoretical predictions of masses from different models such as Duflo and Zuker (DZ), Moller and Nix (MN), finite range droplet model (FRDM), HFB19 and HFB21 microscopic models using a novel Bayesian neural network (BNN) formalism; deduced a mass model that is used to predict the composition of the outer crust of a neutron star. 96,97,98,99,100,101,102,103,104,105,106,107,108,109,110,111,112Kr; analyzed mass predictions from five mass models, and from the BNN-improved formalism with comparison to AME-2012 evaluation. Relevance to prediction of composition of outer crust of a neutron star.

doi: 10.1103/PhysRevC.93.014311
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1990SM01      Phys.Lett. 234B, 191 (1990)

K.F.Smith, N.Crampin, J.M.Pendlebury, D.J.Richardson, D.Shiers, K.Green, A.I.Kilvington, J.Moir, H.B.Prosper, D.Thompson, N.F.Ramsey, B.R.Heckel, S.K.Lamoreaux, P.Ageron, W.Mampe, A.Steyerl

A Search for the Electric Dipole Moment of the Neutron

NUCLEAR MOMENTS 1n; measured electric dipole moment. Stored ultra cold neutrons, magnetic resonance technique.

doi: 10.1016/0370-2693(90)92027-G
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1987BA21      Nucl.Phys. A466, 473 (1987)

C.J.Batty, M.Fidecaro, H.B.Prosper

Neutron-Antineutron Oscillations in 16O

NUCLEAR STRUCTURE 16O; calculated n, n-bar average single particle densities. Antiproton-12C potential input.

NUCLEAR REACTIONS 12C(p-bar, p-bar), E=47 MeV; analyzed data; deduced neutron-antineutron mixing time.

doi: 10.1016/0375-9474(87)90453-2
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