2020
DOI: 10.1007/jhep02(2020)007
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Brane nucleation instabilities in non-AdS/non-CFT

Abstract: We speculate that the weak gravity conjecture applied to theories with holographic duals bans the existence of disordered phases at zero temperature. We test this idea by introducing a nonzero baryon chemical potential in a deformation of the SU (N c ) × SU (N c ) Klebanov-Witten gauge theory with broken supersymmetry and conformal invariance. At low temperature, a disordered phase dual to a black brane geometry is unstable for low chemical potentials and metastable for high values. In the metastable phase, st… Show more

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Cited by 16 publications
(16 citation statements)
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“…Third, for planar horizons we have found an instability towards nucleation of spacetime filling M2 branes. This is of the same form as in [43], where five-dimensional black branes in the conifold T 11 theory were found to be unstable towards the emission of spacetime filling D3 branes. In both cases this phase transition is triggered not by the baryonic charges, but by the R-symmetry.…”
Section: Jhep02(2022)009supporting
confidence: 68%
See 3 more Smart Citations
“…Third, for planar horizons we have found an instability towards nucleation of spacetime filling M2 branes. This is of the same form as in [43], where five-dimensional black branes in the conifold T 11 theory were found to be unstable towards the emission of spacetime filling D3 branes. In both cases this phase transition is triggered not by the baryonic charges, but by the R-symmetry.…”
Section: Jhep02(2022)009supporting
confidence: 68%
“…First of all, one can notice that the hypermultiplets have dropped out from the expression of the mass, which depends solely on the vector multiplets scalars. Previous examples of probe computations (wrapped M2 branes on AdS 4 backgrounds of [29], and wrapped D3 branes on AdS 5 black branes discussed in [43]) also showed the same pattern. It is however surprising that this sector of the theory does not contribute to the mass term of the DBI action.…”
Section: Jhep02(2022)009supporting
confidence: 59%
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“…Therefore, the spacetimes that we will consider herein are taken to be asymptotically AdS 4 . At low temperature, the charged AdS 4 black hole may undergo a "brane nucleation" instability by ejecting its charge to reach an energetically more favorable ground state [81,82]; in AdS/CFT context this instability has also been called the Fermi seasickness [33]. In other words, when the backreaction of bulk fermions is taken into account, the AdS 4 -Reissner-Nordström black hole is quantum mechanically unstable towards the formation of an electron cloud.…”
Section: Review Of Electron Cloud Geometrymentioning
confidence: 99%