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We analyze families of hybrid equations of state of cold QCD matter, which combine input from gauge/gravity duality and from various ab initio methods for nuclear matter at low density, and predict that all neutron stars are fully hadronic without quark matter cores.
1902
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T. Ishii, M. Järvinen and G. Nijs, Cool baryon and quark matter in holographic QCD , JHEP 07
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B. Friman and W. Weise, Neutron Star Matter as a Relativistic Fermi Liquid , Phys. Rev. C 100
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T. Sakai and S. Sugimoto, More on a Holographic Dual of QCD , Prog. Theor. Phys. 114
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Y.-L. Ma and M. Rho, What’s in the core of massive neutron stars? , 2006.14173
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2007
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U. Gürsoy and E. Kiritsis, Exploring improved holographic theories for QCD: Part I , JHEP 02
2008
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2008
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M. Rozali, H.-H. Shieh, M. Van Raamsdonk and J. Wu, Cold Nuclear Matter in Holographic QCD , JHEP 01
2016
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2016
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F. Preis and A. Schmitt, Layers of Deformed Instantons in Holographic Baryonic Matter , JHEP 07
2016
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M. Elliot-Ripley, P. Sutcliffe and M. Zamaklar, Phases of kinky holographic nuclear matter , JHEP 10
2016
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2008
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2010
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2010
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M. Järvinen and E. Kiritsis, Holographic Models for QCD in the Veneziano Limit , JHEP 03
2012
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2019
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N. Kovensky and A. Schmitt, Isospin asymmetry in holographic baryonic matter , SciPost Phys. 11
2021
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