William G. Newton - Concepedia

Author

William G. Newton

Also Known As

Newton, W. G., Newton, William, Newton, William G., W G Newton, W. G. NEWTON, W. G. Newton, W. Newton, William G Newton, William G. Newton, William Newton

Publications

1.7K

Citations

H-Index

Concepts

All Affiliations

East Texas A&M University Shanghai Jiao Tong University University of Tennessee at Knoxville University of California, Berkeley South China University of Technology

About

William G. Newton is an author at East Texas A&M University specializing in physics, natural sciences, and nuclear physics.

Top Concepts

#	Concept	H-Index	Publications	Citations
1	Natural Sciences	14	15	858
2	Engineering	10	10	525
3	Medicine	1	1	20
4	Applied Physics	1	1	13
5	Comparative Literature	1	1	15

William G. Newton

Publications

1.6K

Citations

H-Index

Page 1

	Year	Citations
Modeling nuclear “pasta” and the transition to uniform nuclear matter with the 3D Skyrme-Hartree-Fock method at finite temperature: Core-collapse supernovae William G. Newton, J. R. Stone Physical Review C Uniform Nuclear MatterEngineeringNuclear PhysicsPhysicsNuclear Structure	2009	170
Using neutron star observations to determine crust thicknesses, moments of inertia, and tidal deformabilities Andrew W. Steiner, Stefano Gandolfi, F. J. Fattoyev, Physical Review C Relativistic AstrophysicsNeutron Star PhysicsCrustal DeformationEngineeringMagnetar	2015	161
Dense nuclear matter equation of state from heavy-ion collisions Agnieszka Sorensen, Kshitij Agarwal, K. W. Brown, Progress in Particle and Nuclear Physics Heavy Ion PhysicHigh-energy Nuclear ReactionNuclear PhysicsPhysicsHeavy-ion Physics	2023	153
Constraining the high-density behavior of the nuclear symmetry energy with the tidal polarizability of neutron stars F. J. Fattoyev, J. Carvajal, William G. Newton, Physical Review C	2013	148
A SURVEY OF THE PARAMETER SPACE OF THE COMPRESSIBLE LIQUID DROP MODEL AS APPLIED TO THE NEUTRON STAR INNER CRUST William G. Newton, Michael Gearheart, Bao-An Li The Astrophysical Journal Supplement Series	2012	111
Upper limits on the observational effects of nuclear pasta in neutron stars Michael Gearheart, William G. Newton, J. Hooker, Monthly Notices of the Royal Astronomical Society	2011	98
Neutron–proton effective mass splitting in neutron-rich matter at normal density from analyzing nucleon–nucleus scattering data within an isospin dependent optical model Xiao‐Hua Li, Guo Wen-Jun, Bao-An Li, Physics Letters B	2015	73
How tightly is the nuclear symmetry energy constrained by a unitary Fermi gas? Naibo Zhang, Bao-Jun Cai, Bao-An Li, Nuclear Science and Techniques Nuclear PhysicsPhysicsNatural SciencesNuclear Symmetry EnergyUnitary Fermi Gas	2017	59
Generic constraints on the relativistic mean-field and Skyrme-Hartree-Fock models from the pure neutron matter equation of state F. J. Fattoyev, William G. Newton, Jun Xu, Physical Review C	2012	57
Constraints on the symmetry energy from observational probes of the neutron star crust William G. Newton, J. Hooker, Michael Gearheart, The European Physical Journal A Relativistic AstrophysicsPhysicsObservational ProbesNatural SciencesNuclear Theory	2014	49

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