Holographic superfluids and the Landau criterion
A bstract 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 wit...
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Veröffentlicht in: | The journal of high energy physics 2014-02, Vol.2014 (2), p.1-24, Article 63 |
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container_title | The journal of high energy physics |
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creator | Amado, Irene Areán, Daniel Jiménez-Alba, Amadeo Landsteiner, Karl Melgar, Luis Landea, Ignacio Salazar |
description | A
bstract
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. |
doi_str_mv | 10.1007/JHEP02(2014)063 |
format | Article |
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bstract
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.</description><identifier>ISSN: 1029-8479</identifier><identifier>EISSN: 1029-8479</identifier><identifier>DOI: 10.1007/JHEP02(2014)063</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Broken symmetry ; Classical and Quantum Gravitation ; Criteria ; Dispersions ; Elementary Particles ; Fluids ; High energy physics ; Instability ; Mathematical analysis ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Quantum Physics ; Relativity Theory ; Stability ; String Theory ; Superfluidity</subject><ispartof>The journal of high energy physics, 2014-02, Vol.2014 (2), p.1-24, Article 63</ispartof><rights>The Author(s) 2014</rights><rights>SISSA, Trieste, Italy 2014</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c384t-7bac68742d197fbf7908b3c48dbfb0c346dfb55203b27bfb51fbac67a174d21d3</citedby><cites>FETCH-LOGICAL-c384t-7bac68742d197fbf7908b3c48dbfb0c346dfb55203b27bfb51fbac67a174d21d3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/JHEP02(2014)063$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://doi.org/10.1007/JHEP02(2014)063$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,864,27922,27923,41118,41486,42187,42555,51317,51574</link.rule.ids></links><search><creatorcontrib>Amado, Irene</creatorcontrib><creatorcontrib>Areán, Daniel</creatorcontrib><creatorcontrib>Jiménez-Alba, Amadeo</creatorcontrib><creatorcontrib>Landsteiner, Karl</creatorcontrib><creatorcontrib>Melgar, Luis</creatorcontrib><creatorcontrib>Landea, Ignacio Salazar</creatorcontrib><title>Holographic superfluids and the Landau criterion</title><title>The journal of high energy physics</title><addtitle>J. High Energ. Phys</addtitle><description>A
bstract
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.</description><subject>Broken symmetry</subject><subject>Classical and Quantum Gravitation</subject><subject>Criteria</subject><subject>Dispersions</subject><subject>Elementary Particles</subject><subject>Fluids</subject><subject>High energy physics</subject><subject>Instability</subject><subject>Mathematical analysis</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Relativity Theory</subject><subject>Stability</subject><subject>String Theory</subject><subject>Superfluidity</subject><issn>1029-8479</issn><issn>1029-8479</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNp1kMFLwzAUh4MoOKdnrwUv81D3kqZNepQxnTLQg55DkiZbR9fUpD3435tSD0Pw9H48vt_j8SF0i-EBA7Dl62b9DmRBANN7KLIzNMNAypRTVp6f5Et0FcIBAOe4hBmCjWvczstuX-skDJ3xthnqKiSyrZJ-b5JtDHJItK9742vXXqMLK5tgbn7nHH0-rT9Wm3T79vyyetymOuO0T5mSuuCMkgqXzCrLSuAq05RXyirQGS0qq_KcQKYIi6sc27HBJGa0IrjK5mgx3e28-xpM6MWxDto0jWyNG4LAjAFhHBhE9O4PenCDb-N3Ahc54UVBCY_UcqK0dyF4Y0Xn66P03wKDGA2KyaAYDYpoMDZgaoRItjvjT-7-U_kBAwlxsQ</recordid><startdate>20140201</startdate><enddate>20140201</enddate><creator>Amado, Irene</creator><creator>Areán, Daniel</creator><creator>Jiménez-Alba, Amadeo</creator><creator>Landsteiner, Karl</creator><creator>Melgar, Luis</creator><creator>Landea, Ignacio Salazar</creator><general>Springer Berlin Heidelberg</general><general>Springer Nature B.V</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20140201</creationdate><title>Holographic superfluids and the Landau criterion</title><author>Amado, Irene ; 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High Energ. Phys</stitle><date>2014-02-01</date><risdate>2014</risdate><volume>2014</volume><issue>2</issue><spage>1</spage><epage>24</epage><pages>1-24</pages><artnum>63</artnum><issn>1029-8479</issn><eissn>1029-8479</eissn><abstract>A
bstract
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.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1007/JHEP02(2014)063</doi><tpages>24</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Broken symmetry Classical and Quantum Gravitation Criteria Dispersions Elementary Particles Fluids High energy physics Instability Mathematical analysis Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Quantum Physics Relativity Theory Stability String Theory Superfluidity |
title | Holographic superfluids and the Landau criterion |
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