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NSR database version of May 3, 2024.

Search: Author = D.Neill

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2023NE03      Phys.Rev.Lett. 130, 112701 (2023)

D.Neill, R.Preston, W.G.Newton, D.Tsang

Constraining the Nuclear Symmetry Energy with Multimessenger Resonant Shattering Flares

doi: 10.1103/PhysRevLett.130.112701
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2020PA11      Phys.Rev. C 101, 035804 (2020)

A.Pastore, D.Neill, H.Powell, K.Medler, C.Barton

Impact of statistical uncertainties on the composition of the outer crust of a neutron star

ATOMIC MASSES A=20-260; analyzed masses by Monte Carlo methods with full error analysis on the Duflo-Zucker (DZ) mass model; deduced correlations in the residuals. Z=28, A=58-80; Z=29, A=59-82; analyzed binding energy differences between the theoretical and the experimental values obtained using a DZ10 model and a DZ10 plus NN model ⁵⁶Fe, ^62,64,66,78Ni, ⁸⁰Zn, ⁸²Ge, ⁸⁴Se, ^86,118Kr, ¹²⁰Sr, ¹²²Zr, ¹²⁴Mo; calculated pressure and baryonic density at which the nucleus is found, and existence probability within the outer crust of non-accreting neutron star as a function of the pressure using DZ10+NN mass model. Investigated the use of neural networks to reduce the discrepancy between the DZ10 model and the experimental masses in AME2016.

doi: 10.1103/PhysRevC.101.035804
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