Non-mean-field quantum critical points from holography
Non-mean-field quantum critical points from holography
We construct a class of quantum critical points with non-mean-field critical exponents via holography. Our approach is phenomenological. Beginning with the D3/D5 system at nonzero density and magnetic field which has a chiral phase transition, we simulate the addition of a third control parameter. We then identify a line of quantum critical points in the phase diagram of this theory, provided that the simulated control parameter has dimension less than two. This line smoothly interpolates between a second-order transition with mean-field exponents at zero magnetic field to a holographic Berezinskii-Kosterlitz-Thouless transition at larger magnetic fields. The critical exponents of these transitions only depend upon the parameters of an emergent infrared theory. Moreover, the non-mean-field scaling is destroyed at any nonzero temperature. We discuss how generic these transitions are.
105012-[15pp]
Evans, Nick
33dfbb52-64dd-4c1f-9cd1-074faf2be4b3
Jensen, Kristan
1aa6bec5-5b04-4014-b008-ace89ed2884c
Kim, Keun-Young
45194302-dffc-4cf6-85f2-55bec8f574fb
15 November 2010
Evans, Nick
33dfbb52-64dd-4c1f-9cd1-074faf2be4b3
Jensen, Kristan
1aa6bec5-5b04-4014-b008-ace89ed2884c
Kim, Keun-Young
45194302-dffc-4cf6-85f2-55bec8f574fb
Evans, Nick, Jensen, Kristan and Kim, Keun-Young
(2010)
Non-mean-field quantum critical points from holography.
Physical Review D, 82 (10), .
(doi:10.1103/PhysRevD.82.105012).
Abstract
We construct a class of quantum critical points with non-mean-field critical exponents via holography. Our approach is phenomenological. Beginning with the D3/D5 system at nonzero density and magnetic field which has a chiral phase transition, we simulate the addition of a third control parameter. We then identify a line of quantum critical points in the phase diagram of this theory, provided that the simulated control parameter has dimension less than two. This line smoothly interpolates between a second-order transition with mean-field exponents at zero magnetic field to a holographic Berezinskii-Kosterlitz-Thouless transition at larger magnetic fields. The critical exponents of these transitions only depend upon the parameters of an emergent infrared theory. Moreover, the non-mean-field scaling is destroyed at any nonzero temperature. We discuss how generic these transitions are.
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Published date: 15 November 2010
Organisations:
Physics & Astronomy
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Local EPrints ID: 337320
URI: http://eprints.soton.ac.uk/id/eprint/337320
ISSN: 1550-7998
PURE UUID: 864d20f7-00ee-4728-99c3-b8ae61367121
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Date deposited: 24 Apr 2012 10:27
Last modified: 14 Mar 2024 10:52
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Author:
Kristan Jensen
Author:
Keun-Young Kim
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