Inverse Anisotropic Catalysis in Holographic QCD

Publication date

2019-04-09

Authors

Gursoy, U.ISNI 0000000392717860
Järvinen, MattiISNI 0000000506769475
Nijs, GovertISNI 000000049252269X
Pedraza, Juan F.

Editors

Advisors

Supervisors

Document Type

Article
Open Access logo

License

Abstract

We investigate the effects of anisotropy on the chiral condensate in a holographic model of QCD with a fully backreacted quark sector at vanishing chemical potential. The high temperature deconfined phase is therefore a neutral and anisotropic plasma showing different pressure gradients along different spatial directions, similar to the state produced in noncentral heavy-ion collisions. We find that the chiral transition occurs at a lower temperature in the presence of anisotropy. Equivalently, we find that anisotropy acts destructively on the chiral condensate near the transition temperature. These are precisely the same footprints as the "inverse magnetic catalysis" i.e. the destruction of the condensate with increasing magnetic field observed earlier on the lattice, in effective field theory models and in holography. Based on our findings we suggest, in accordance with the conjecture of [1], that the cause for the inverse magnetic catalysis may be the anisotropy caused by the presence of the magnetic field instead of the charge dynamics created by it. We conclude that the weakening of the chiral condensate due to anisotropy is more general than that due to a magnetic field and we coin the former "inverse anisotropic catalysis". Finally, we observe that any amount of anisotropy changes the IR physics substantially: the geometry is $\text{AdS}_4 \times \mathbb{R}$ up to small corrections, confinement is present only up to a certain scale, and the particles acquire finite widths.

Keywords

hep-th, hep-lat, hep-ph, Gauge-gravity correspondence, Holography and quark-gluon plasmas, Phase Diagram of QCD

Citation

Gursoy, U, Jarvinen, M, Nijs, G & Pedraza, J F 2019, 'Inverse Anisotropic Catalysis in Holographic QCD', Journal of High Energy Physics, no. 4, 71. https://doi.org/10.1007/JHEP04(2019)071