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Anthony W. Thomas
Researcher at University of Adelaide
Publications - 982
Citations - 22196
Anthony W. Thomas is an academic researcher from University of Adelaide. The author has contributed to research in topics: Nucleon & Quark. The author has an hindex of 69, co-authored 955 publications receiving 20694 citations. Previous affiliations of Anthony W. Thomas include University of Bonn & University of Mainz.
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Quark-hadron duality and the nuclear EMC effect
TL;DR: In this paper, the authors used model independent relations derived on the basis of quark-hadron duality to relate the medium modification of the form factors to the modification at large x of the deep-inelastic structure function of a bound proton.
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Charge symmetry breaking in mirror nuclei from quarks
TL;DR: In this article, the binding energy differences of the valence proton and neutron of the mirror nuclei were calculated using the quark-meson coupling (QMC) model, and the origin of these differences may be ascribed to the charge symmetry breaking effects set in the strong interaction through the u and d current quark mass difference.
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The strangeness magnetic moment of the nucleon from FLIC fermions
Derek B. Leinweber,S. Boinepalli,Anthony W. Thomas,Anthony G. Williams,Ross D. Young,James Zanotti,Jian-Bo Zhang +6 more
TL;DR: In this paper, the strangeness magnetic moment of the nucleon can be expressed in terms of empirical magnetic moments and ratios of valence quark magnetic moments using modern chiral extrapolation techniques and recent low mass lattice QCD simulations of the individual quark contributions to the magnetic moments of the nucleus octet.
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Novel neutron decay mode inside neutron stars
Wasif Husain,Anthony W. Thomas +1 more
TL;DR: In this paper , the authors explored the possibility of neutrons decaying into dark matter through the process, n → χχ χ, with χ having a mass one third of that of the neutron, and examined the consequences of such a decay mode for the properties of neutron stars.
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Neutron Star Properties from an NJL Model Modified to Simulate Confinement
TL;DR: In this article, the authors use the model to investigate the equation of state of asymmetric nuclear matter and then use it to compute the properties of neutron stars, which leads in mean field approximation to a natural mechanism for the saturation of nuclear matter.