Built on

J. R. Oppenheimer and G. M. Volkoff, “On Massive neutron cores,” Phys. Rev. 55
1939
Earlier work this paper cites.
J. M. Luttinger, “Fermi Surface and Some Simple Equilibrium Properties of a System of Interacting Fermions,” Phys. Rev. 119
1960
Earlier work this paper cites.
A. A. Belavin, A. M. Polyakov, A. S. Schwartz and Yu. S. Tyupkin, “Pseudoparticle Solutions of the Yang-Mills Equations,” Phys. Lett. B 59
1975
Earlier work this paper cites.
S. de Haro, S. N. Solodukhin and K. Skenderis, “Holographic reconstruction of spacetime and renormalization in the AdS/CFT correspondence,” Commun. Math. Phys. 217
2001
Earlier work this paper cites.
K. Skenderis, “Holographic reconstruction of spacetime and renormalization in the AdS/CFT correspondence,” Class. Quant. Grav. 19
2002
Earlier work this paper cites.
T. Sakai and S. Sugimoto, “Low energy hadron physics in holographic QCD,” Prog. Theor. Phys. 113
2005
Earlier work this paper cites.
H. Hata, T. Sakai, S. Sugimoto and S. Yamato, “Baryons from instantons in holographic QCD,” Prog. Theor. Phys. 117
2007
Earlier work this paper cites.

Similar

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Original
2007
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2008
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Then

W. -y. Chuang, S. -H. Dai, S. Kawamoto, F. -L. Lin and C. -P. Yeh, “Dynamical Instability of Holographic QCD at Finite Density,” Phys. Rev. D 83
Original
2011
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Original
2011
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V. Kaplunovsky, D. Melnikov and J. Sonnenschein, “Baryonic Popcorn,” JHEP 1211
Original
2012
Later among the works it cites.
S. Seki and S. -J. Sin, “Chiral Condensate in Holographic QCD with Baryon Density,” JHEP 1208
Original
2012
Later among the works it cites.
J. de Boer, B. D. Chowdhury, M. P. Heller and J. Jankowski, “Towards a holographic realization of the Quarkyonic phase,” Phys. Rev. D 87

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2013

Holographic cold nuclear matter and neutron star

Ghoroku, Kazuo, Kubo, Kouki, Tachibana, Motoi et al.

Understand

We have previously found a new phase of cold nuclear matter based on a holographic gauge theory, where baryons are introduced as instanton gas in the probe D8/$\overline{\rm D8}$ branes.

In our model, we could obtain the equation of state (EOS) of our nuclear matter by introducing fermi momentum.
Then, here we apply this model to the neutron star and study its mass and radius by solving the Tolman-Oppenheimer-Volkoff (TOV) equations in terms of the EOS given here.
We give some comments for our holographic model from a viewpoint of the other field theoretical approaches.

Built on

J. R. Oppenheimer and G. M. Volkoff, “On Massive neutron cores,” Phys. Rev. 55
1939
Earlier work this paper cites.
J. M. Luttinger, “Fermi Surface and Some Simple Equilibrium Properties of a System of Interacting Fermions,” Phys. Rev. 119
1960
Earlier work this paper cites.
A. A. Belavin, A. M. Polyakov, A. S. Schwartz and Yu. S. Tyupkin, “Pseudoparticle Solutions of the Yang-Mills Equations,” Phys. Lett. B 59
1975
Earlier work this paper cites.
S. de Haro, S. N. Solodukhin and K. Skenderis, “Holographic reconstruction of spacetime and renormalization in the AdS/CFT correspondence,” Commun. Math. Phys. 217
2001
Earlier work this paper cites.
K. Skenderis, “Holographic reconstruction of spacetime and renormalization in the AdS/CFT correspondence,” Class. Quant. Grav. 19
2002
Earlier work this paper cites.
T. Sakai and S. Sugimoto, “Low energy hadron physics in holographic QCD,” Prog. Theor. Phys. 113
2005
Earlier work this paper cites.
H. Hata, T. Sakai, S. Sugimoto and S. Yamato, “Baryons from instantons in holographic QCD,” Prog. Theor. Phys. 117
2007
Earlier work this paper cites.