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We calculate the equation of state of nuclear matter for arbitrary isospin-asymmetry up to three loop order in the free energy density in the framework of in-medium chiral perturbation theory.
J. Gasser, H. Leutwyler, M.E. Sainio, Phys. Lett. B 253
1991
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N. Kaiser, Phys. Rev. C 59
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J.B. Natowitz, R. Wada, K. Hagel, T. Keygen, M. Murray, A. Makeev, L. Qin, P. Smith, C. Hamilton, Phys. Rev. C 65
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N. Kaiser, S. Fritsch, W. Weise, Nucl. Phys. A 697
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S. Fritsch, N. Kaiser, W. Weise, Physics Letters B 545
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Cited alongside, same era.
S. Fritsch, N. Kaiser, W. Weise, Nucl. Phys. A 750
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N. Kaiser, P. de Homont, W. Weise, Phys. Rev. C 77
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Cited alongside, same era.
P.B. Demorest, T. Pennucci, S.M. Ransom, M.S.E. Roberts, J.W.T. Hessels, Nature 467
2010
Later among the works it cites.
S. Fiorilla, N. Kaiser, W. Weise, arXiv :1104.2819v1 (2011)
2011
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S. Fiorilla, N. Kaiser, W. Weise, preprint (2011)
2011
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