Cold Nuclear Matter In Holographic QCD
arXiv:0708.1322 · doi:10.1088/1126-6708/2008/01/053
Abstract
We study the Sakai-Sugimoto model of holographic QCD at zero temperature and finite chemical potential. We find that as the baryon chemical potential is increased above a critical value, there is a phase transition to a nuclear matter phase characterized by a condensate of instantons on the probe D-branes in the string theory dual. As a result of electrostatic interactions between the instantons, this condensate expands towards the UV when the chemical potential is increased, giving a holographic version of the expansion of the Fermi surface. We argue based on properties of instantons that the nuclear matter phase is necessarily inhomogeneous to arbitrarily high density. This suggests an explanation of the "chiral density wave" instability of the quark Fermi surface in large N_c QCD at asymptotically large chemical potential. We study properties of the nuclear matter phase as a function of chemical potential beyond the transition and argue in particular that the model can be used to make a semi-quantitative prediction of the binding energy per nucleon for nuclear matter in ordinary QCD.
31 pages, LaTeX, 1 figure, v2: some formulae corrected, qualitative results unchanged
References in corpus (7)
- Viscosity, Black Holes, and Quantum Field Theory
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- Baryon Number-Induced Chern-Simons Couplings of Vector and Axial-Vector Mesons in Holographic QCD
- Stringy NJL and Gross-Neveu models at finite density and temperature
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- Quark Soup al dente: Applied Superstring Theory
- Sound Modes in Holographic Hydrodynamics for Charged AdS Black Hole
- Holographic Magnetic Phase Transition
- Baryonic Response of Dense Holographic QCD
- Chiral Condensates in Finite Density Holographic NJL Model from String Worldsheets
- On the Baryonic Density and Susceptibilities in a Holographic Model of QCD