Spatiotemporal buildup of the Kondo screening cloud
We investigate how the Kondo screening cloud builds up as a function of space and time. Starting from an impurity spin decoupled from the conduction band, the Kondo coupling is switched on at time t = 0. We work at the Toulouse point where one can obtain exact analytical results for the ensuing spin...
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Veröffentlicht in: | Physical review. B, Condensed matter and materials physics Condensed matter and materials physics, 2013-09, Vol.88 (9), Article 094306 |
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creator | Medvedyeva, M. Hoffmann, A. Kehrein, S. |
description | We investigate how the Kondo screening cloud builds up as a function of space and time. Starting from an impurity spin decoupled from the conduction band, the Kondo coupling is switched on at time t = 0. We work at the Toulouse point where one can obtain exact analytical results for the ensuing spin dynamics at both zero and nonzero temperature T. For t > 0 the Kondo screening cloud starts building up in the wake of the impurity spin being transported to infinity. In this buildup process the impurity spin-conduction band spin susceptibility shows a sharp light cone due to causality, while the corresponding correlation function has a tail outside the light cone. At T = 0 this tail has a power-law decay as a function of distance from the impurity, which we interpret as due to initial entanglement in the Fermi sea. |
doi_str_mv | 10.1103/PhysRevB.88.094306 |
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At T = 0 this tail has a power-law decay as a function of distance from the impurity, which we interpret as due to initial entanglement in the Fermi sea.</description><identifier>ISSN: 1098-0121</identifier><identifier>EISSN: 1550-235X</identifier><identifier>DOI: 10.1103/PhysRevB.88.094306</identifier><language>eng</language><subject>Clouds ; Condensed matter ; Construction ; Decay ; Impurities ; Mathematical analysis ; Screening ; Wakes</subject><ispartof>Physical review. 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Starting from an impurity spin decoupled from the conduction band, the Kondo coupling is switched on at time t = 0. We work at the Toulouse point where one can obtain exact analytical results for the ensuing spin dynamics at both zero and nonzero temperature T. For t > 0 the Kondo screening cloud starts building up in the wake of the impurity spin being transported to infinity. In this buildup process the impurity spin-conduction band spin susceptibility shows a sharp light cone due to causality, while the corresponding correlation function has a tail outside the light cone. At T = 0 this tail has a power-law decay as a function of distance from the impurity, which we interpret as due to initial entanglement in the Fermi sea.</description><subject>Clouds</subject><subject>Condensed matter</subject><subject>Construction</subject><subject>Decay</subject><subject>Impurities</subject><subject>Mathematical analysis</subject><subject>Screening</subject><subject>Wakes</subject><issn>1098-0121</issn><issn>1550-235X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNo1kL1OwzAURi0EEqXwAkwZWRLutePGGaGCgqgE4kdisxznmgYlcbATpL49RYXp-4ajMxzGzhEyRBCXT5ttfKbv60ypDMpcwOKAzVBKSLmQ74e7D6VKATkes5MYPwEwL3M-Y-JlMGPjR-oGH0ybVFPT1tOQeJeMG0oefF_7JNpA1Df9R2JbP9Wn7MiZNtLZ387Z2-3N6_IuXT-u7pdX69RyBWNacKMIcmUNQC65tIZqWFiQJRWVkyiM4FKglSJ3TlFVOwGVqxRUUCB3CzFnF3vvEPzXRHHUXRMtta3pyU9RY4GqlLIAvkP5HrXBxxjI6SE0nQlbjaB_C-n_QlopvS8kfgAZelr0</recordid><startdate>20130917</startdate><enddate>20130917</enddate><creator>Medvedyeva, M.</creator><creator>Hoffmann, A.</creator><creator>Kehrein, S.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20130917</creationdate><title>Spatiotemporal buildup of the Kondo screening cloud</title><author>Medvedyeva, M. ; Hoffmann, A. ; Kehrein, S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c280t-72a8e048ca004525caed06c059e7bf513a32531c534ff8ebdf30bfb80b0712f63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Clouds</topic><topic>Condensed matter</topic><topic>Construction</topic><topic>Decay</topic><topic>Impurities</topic><topic>Mathematical analysis</topic><topic>Screening</topic><topic>Wakes</topic><toplevel>online_resources</toplevel><creatorcontrib>Medvedyeva, M.</creatorcontrib><creatorcontrib>Hoffmann, A.</creatorcontrib><creatorcontrib>Kehrein, S.</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physical review. B, Condensed matter and materials physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Medvedyeva, M.</au><au>Hoffmann, A.</au><au>Kehrein, S.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Spatiotemporal buildup of the Kondo screening cloud</atitle><jtitle>Physical review. B, Condensed matter and materials physics</jtitle><date>2013-09-17</date><risdate>2013</risdate><volume>88</volume><issue>9</issue><artnum>094306</artnum><issn>1098-0121</issn><eissn>1550-235X</eissn><abstract>We investigate how the Kondo screening cloud builds up as a function of space and time. Starting from an impurity spin decoupled from the conduction band, the Kondo coupling is switched on at time t = 0. We work at the Toulouse point where one can obtain exact analytical results for the ensuing spin dynamics at both zero and nonzero temperature T. For t > 0 the Kondo screening cloud starts building up in the wake of the impurity spin being transported to infinity. In this buildup process the impurity spin-conduction band spin susceptibility shows a sharp light cone due to causality, while the corresponding correlation function has a tail outside the light cone. At T = 0 this tail has a power-law decay as a function of distance from the impurity, which we interpret as due to initial entanglement in the Fermi sea.</abstract><doi>10.1103/PhysRevB.88.094306</doi></addata></record> |
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subjects | Clouds Condensed matter Construction Decay Impurities Mathematical analysis Screening Wakes |
title | Spatiotemporal buildup of the Kondo screening cloud |
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