Publications

REFEREED JOURNALS:

Sensitivity of the neutron star r-mode instability window to the density dependence of the nuclear symmetry energy

Wen, De-Hua, Newton, W. G. and Li, Bao-An; submitted to Physical Review C (2011)

How well do we know the composition of the neutron star crust?

Newton, W. G.Gearheart, M. and Li, Bao-An; submitted to Physical Review C (2011)

Upper limits on the observational effects of nuclear pasta in neutron stars 

Gearheart, M., Newton, W. G., Hooker, J. and Li, Bao-An; accepted for publication in MNRAS (2011)

Constraining the gravitational binding energy of PSR J0737-3039B using terrestrial nuclear data

Newton, W. G. and Li, Bao-An; Physical Review C80, 065809  (2009)

Modeling nuclear “pasta” and the transition to uniform nuclear matter with the 3D Skyrme-Hartree-Fock method at finite temperature: Core-collapse supernovae

Newton, W.G. and Stone, J.R.; Physical Review C79, 055801 (2009)

The double pulsar J0737-3039:Testing the neutron star equation of state

Podsiadlowski, Ph., Dewi, J. D. M., Lesaffre, P., Miller, J. C., Newton, W. G., Stone, J. R.; MNRAS, Volume 361, Issue 4, pp. 1243-1249 (2005)

Giant resonances from TDHF

Stevenson, P. D., Strayer, M. R., Rikovska-Stone, J., Newton, W. G.; International Journal of Modern Physics E, Volume 13, Issue 1, pp. 181-185 (2004)

CONFERENCE PROCEEDINGS:

Imprints of Nuclear Symmetry Energy on Properties of Neutron Stars

Li, Bao-An; Chen, Lie-Wen; Gearheart, M; Hooker, J; Ko, Che Ming; Krastev, P. G., Lin, Wei-Kang; Newton, W. G.; Wen, De-Hua; Xu, Chang; Xu, Jun; INPC2010, July 4-9, 2010, Vancouver, Canada; Journal of Physics: Conference Series; arxiv 1103.4652 (2011)

Modeling Nuclear Pasta and the Transition to Uniform Nuclear Matter with the 3D-Skyrme-Hartree-Fock Method

Newton, W.G.; Proceedings of the 5th FRIB Workshop on Bulk Nuclear Properties, arxiv 0903.1464 (2009)

A new study of the transition to uniform nuclear matter in neutron stars and supernovae

Newton, W.G.; Participant Contribution at the “Dense Matter in Heavy Ion Collisions and Astrophysics” Summer School, JINR, Dubna, Aug. 21 – Sept. 1, 2006. Published in PEPAN letters

From microscales to macroscales in 3D: Self-consistent equation of state for supernova and neutron star models

Newton, W.G., Stone, J.R. and  Mezzacappa, A; Journal of Physics Conference Series 46, pp. 408-412, (2006)

Sub-nuclear matter in neutron stars and supernovae: nuclear pasta and beyond

Newton, W.G.; Proceedings of RAGtime 6/7: Workshop on Black Holes and Neutron Stars, S. Hledík and Z. Stuchlík, editors, Silesian University in Opava, Czech Republic, 12/2005, ISBN 80-7248-334-X, pp. 119-135, (2006)

Self-Consistent 3D Equations of State at Finite Temperatures for Supernovae and Neutron Stars

Stone, J.R., Newton, W.G., Mezzacappa, A; American Astronomical Society Meeting 207, #17.07; Bulletin of the American Astronomical Society, Vol. 37, p.1182, (2005)

THESES:

The Phase Transition to Uniform Nuclear Matter in Supernovae and Neutron Stars

W.G. Newton, DPhil Thesis, University of Oxford, 2007

Giant resonances in argon isotopes

W.G. Newton, MSc Thesis, University of Tennessee, 2002

·Refereed journals:

Constraining the gravitational binding energy of PSR J0737-3039B using terrestrial nuclear data

Newton, W. G. and Li, Bao-An

To be published in Physical Review C80, (2009)

Modeling nuclear “pasta” and the transition to uniform nuclear matter with the 3D Skyrme-Hartree-Fock method at finite temperature: Core-collapse supernovae

Newton, W.G. and Stone, J.R.;

Physical Review C79, 055801 (2009)

The double pulsar J0737-3039:Testing the neutron star equation of state
Podsiadlowski, Ph.; Dewi, J. D. M.; Lesaffre, P.; Miller, J. C.; Newton, W. G.; Stone, J. R.;

Monthly Notices of the Royal Astronomical Society, Volume 361, Issue 4, pp. 1243-1249 (2005)

Giant resonances from TDHF

Stevenson, P. D.; Strayer, M. R.; Rikovska-Stone, J.; Newton, W. G.; International Journal of Modern Physics E, Volume 13, Issue 1, pp. 181-185 (2004)

·Conference Proceedings:

Modeling nuclear pasta and the phase transition to uniform nuclear matter with the 3D-Skyrme-Hartree-Fock method

Newton, W.G.;

Proceedings of the 5th FRIB Workshop on Bulk Nuclear Properties, arxiv0903.1464 (2009)

A new study of the transition to uniform nuclear matter in neutron stars and supernovae

Newton, W.G.;

Participant Contribution at the “Dense Matter in Heavy Ion Collisions and Astrophysics” Summer School, JINR, Dubna, Aug. 21 – Sept. 1, 2006. To be published in PEPAN letters

From microscales to macroscales in 3D: Self-consistent equation of state for supernova and neutron star models

Newton, W.G., Stone, J.R. and  Mezzacappa, A;

Journal of Physics Conference Series 46, pp. 408-412, (2006)

Sub-nuclear matter in neutron stars and supernovae: nuclear pasta and beyond Newton, W.G.;

Proceedings of RAGtime 6/7: Workshop on Black Holes and Neutron Stars,

S. Hledík and Z. Stuchlík, editors, Silesian University in Opava, Czech Republic, 12/2005, ISBN 80-7248-334-X, pp. 119-135, (2006)

Self-consistent 3D equations of state at finite temperature for supernovae and neutronsStars

Stone, J.R.; Newton, W.G.; Mezzacappa, A.

American Astronomical Society Meeting 207, #17.07; Bulletin of the American Astronomical Society, Vol. 37, p.1182, (2005)

·Theses:

W.G. Newton, DPhil Thesis, University of Oxford, 2007

Giant resonances in argon isotopes

W.G. Newton, MSc Thesis, University of Tennessee, 2002

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