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Cold uniform matter and neutron stars in the quark-meson-coupling model

Abstract:: A new density dependent effective baryon-baryon interaction has been recently derived from the quark-meson-coupling (QMC) model, offering impressive results in application to finite nuclei and dense baryon matter. This self-consistent, relativistic, quark-level approach is used to construct the Equation of State (EoS) and to calculate key properties of high density matter and cold, slowly rotating neutron stars. The results include predictions for the maximum mass of neutron-star models, toge...
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Publication status:: Published

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APA Style

Stone, J. R., Guichon, P., Matevosyan, H., & Thomas, A. (2007). Cold uniform matter and neutron stars in the quark-meson-coupling model. NUCLEAR PHYSICS A, 792(3-4), 341–369.

MLA Style

Stone, J. R., et al. “Cold Uniform Matter and Neutron Stars in the Quark-Meson-Coupling Model.” NUCLEAR PHYSICS A, vol. 792, no. 3-4, 2007, pp. 341–69.

Chicago Style

Stone, JR, P Guichon, H Matevosyan, and A Thomas. 2007. “Cold Uniform Matter and Neutron Stars in the Quark-Meson-Coupling Model.” NUCLEAR PHYSICS A 792 (3-4): 341–69.
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Publisher copy:: 10.1016/j.nuclphysa.2007.05.011

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+ Stone, JR More by this author

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+ Guichon, P More by this author

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+ Matevosyan, H More by this author

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+ Thomas, A More by this author

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Bibliographic Details

Journal:: NUCLEAR PHYSICS A
Volume:: 792
Issue:: 3-4
Pages:: 341-369
Publication date:: 2007-08-15
DOI:: 10.1016/j.nuclphysa.2007.05.011
ISSN:: 0375-9474

Item Description

Language:: English
Pubs id:: pubs:164979
UUID:: uuid:c6eb2513-e090-4071-aa0e-411830fd5e1d
Local pid:: pubs:164979
Source identifiers:: 164979
Deposit date:: 2013-11-16

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Copyright date:: 2007

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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