Holographic superfluids and the Landau criterion
We revisit the question of stability of holographic superfluids with finite super-fluid velocity. Our method is based on applying the Landau criterion to the Quasinormal Mode (QNM) spectrum. In particular we study the QNMs related to the Goldstone modes of spontaneous symmetry breaking with linear a...
| Autores: | , , , , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2014 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/96562 |
| Acceso en línea: | http://hdl.handle.net/10261/96562 |
| Access Level: | acceso abierto |
| Palabra clave: | AdS-CFT correspondence Holography and quark-gluon plasmas Holography and condensed matter physics (AdS/CMT) |
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Holographic superfluids and the Landau criterionAmado, IreneAreán, DanielJiménez-Alba, AmadeoLandsteiner, KarlMelgar, LuisSalazar, I.AdS-CFT correspondenceHolography and quark-gluon plasmasHolography and condensed matter physics (AdS/CMT)We revisit the question of stability of holographic superfluids with finite super-fluid velocity. Our method is based on applying the Landau criterion to the Quasinormal Mode (QNM) spectrum. In particular we study the QNMs related to the Goldstone modes of spontaneous symmetry breaking with linear and quadratic dispersions. In the linear case we show that the sound velocity becomes negative for large enough superfluid velocity and that the imaginary part of the quasinormal frequency moves to the upper half plane. Since the instability is strongest at finite wavelength, we take this as an indication for the existence of an inhomogeneous or striped condensed phase for large superfluid velocity. In the quadratic case the instability is present for arbitrarily small superfluid velocity.This work has been supported by MEC and FEDER grant FPA2012-32828, Consolider Ingenio Programme CPAN (CSD2007-00042), Comunidad de Madrid HEP-HACOS S2009/ESP-1473 and MINECO Centro de excelencia Severo Ochoa Program under grant SEV-2012-0249. I.A. is supported by the Israel Science Foundation under grants no. 392/09 and 495/11. L.M. has been supported by FPI-fellowship BES- 2010-041571. A.J. is supported by FPU fellowship AP2010-5686.Peer reviewedSpringer NatureSCOAP201420142014info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/96562reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)Ingléshttp://dx.doi.org/10.1007/JHEP02(2014)063info:eu-repo/semantics/openAccessoai:digital.csic.es:10261/965622026-05-22T06:33:51Z |
| dc.title.none.fl_str_mv |
Holographic superfluids and the Landau criterion |
| title |
Holographic superfluids and the Landau criterion |
| spellingShingle |
Holographic superfluids and the Landau criterion Amado, Irene AdS-CFT correspondence Holography and quark-gluon plasmas Holography and condensed matter physics (AdS/CMT) |
| title_short |
Holographic superfluids and the Landau criterion |
| title_full |
Holographic superfluids and the Landau criterion |
| title_fullStr |
Holographic superfluids and the Landau criterion |
| title_full_unstemmed |
Holographic superfluids and the Landau criterion |
| title_sort |
Holographic superfluids and the Landau criterion |
| dc.creator.none.fl_str_mv |
Amado, Irene Areán, Daniel Jiménez-Alba, Amadeo Landsteiner, Karl Melgar, Luis Salazar, I. |
| author |
Amado, Irene |
| author_facet |
Amado, Irene Areán, Daniel Jiménez-Alba, Amadeo Landsteiner, Karl Melgar, Luis Salazar, I. |
| author_role |
author |
| author2 |
Areán, Daniel Jiménez-Alba, Amadeo Landsteiner, Karl Melgar, Luis Salazar, I. |
| author2_role |
author author author author author |
| dc.contributor.none.fl_str_mv |
SCOAP |
| dc.subject.none.fl_str_mv |
AdS-CFT correspondence Holography and quark-gluon plasmas Holography and condensed matter physics (AdS/CMT) |
| topic |
AdS-CFT correspondence Holography and quark-gluon plasmas Holography and condensed matter physics (AdS/CMT) |
| description |
We revisit the question of stability of holographic superfluids with finite super-fluid velocity. Our method is based on applying the Landau criterion to the Quasinormal Mode (QNM) spectrum. In particular we study the QNMs related to the Goldstone modes of spontaneous symmetry breaking with linear and quadratic dispersions. In the linear case we show that the sound velocity becomes negative for large enough superfluid velocity and that the imaginary part of the quasinormal frequency moves to the upper half plane. Since the instability is strongest at finite wavelength, we take this as an indication for the existence of an inhomogeneous or striped condensed phase for large superfluid velocity. In the quadratic case the instability is present for arbitrarily small superfluid velocity. |
| publishDate |
2014 |
| dc.date.none.fl_str_mv |
2014 2014 2014 |
| dc.type.none.fl_str_mv |
info:eu-repo/semantics/article http://purl.org/coar/resource_type/c_6501 Publisher's version info:eu-repo/semantics/publishedVersion |
| format |
article |
| status_str |
publishedVersion |
| dc.identifier.none.fl_str_mv |
http://hdl.handle.net/10261/96562 |
| url |
http://hdl.handle.net/10261/96562 |
| dc.language.none.fl_str_mv |
Inglés |
| language_invalid_str_mv |
Inglés |
| dc.relation.none.fl_str_mv |
http://dx.doi.org/10.1007/JHEP02(2014)063 |
| dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess |
| eu_rights_str_mv |
openAccess |
| dc.publisher.none.fl_str_mv |
Springer Nature |
| publisher.none.fl_str_mv |
Springer Nature |
| dc.source.none.fl_str_mv |
reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC instname:Consejo Superior de Investigaciones Científicas (CSIC) |
| instname_str |
Consejo Superior de Investigaciones Científicas (CSIC) |
| reponame_str |
DIGITAL.CSIC. Repositorio Institucional del CSIC |
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DIGITAL.CSIC. Repositorio Institucional del CSIC |
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1869418396063367168 |
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15.812429 |