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Complexity of Shapiro steps
dc.creator | Mali, Petar | |
dc.creator | Šakota, Anđela | |
dc.creator | Tekić, Jasmina | |
dc.creator | Radošević, Slobodan | |
dc.creator | Pantić, Milan | |
dc.creator | Pavkov-Hrvojević, Milica | |
dc.date.accessioned | 2021-02-09T11:25:43Z | |
dc.date.available | 2021-02-09T11:25:43Z | |
dc.date.issued | 2020 | |
dc.identifier.issn | 2470-0045 | |
dc.identifier.uri | https://vinar.vin.bg.ac.rs/handle/123456789/8931 | |
dc.description.abstract | We demonstrate, using the example of the dc+ac driven overdamped Frenkel-Kontorova model, that an easily calculable measure of complexity can be used for the examination of Shapiro steps in the presence of thermal noise. In real systems, thermal noise causes melting or even disappearance of Shapiro steps, which makes their analysis in the standard way from the response function difficult. Unlike in the conventional approach, here, by calculating the Kolmogorov complexity of certain areas in the response function, we were able to detect Shapiro steps, measure their size with the desired precision, and examine their temperature dependence. The aim of this work is to provide scientists, particularly experimentalists, with an unconventional, but practical and easy tool for examination of Shapiro steps in real systems. | en |
dc.language.iso | en | |
dc.relation | info:eu-repo/grantAgreement/MESTD/Basic Research (BR or ON)/171009/RS// | |
dc.relation | info:eu-repo/grantAgreement/MESTD/Integrated and Interdisciplinary Research (IIR or III)/45010/RS// | |
dc.relation | Provincial Secretariat for High Education and Scientific Research of Vojvodina [APV 114-451-2201] | |
dc.relation | info:eu-repo/grantAgreement/MESTD/inst-2020/200125/RS// | |
dc.rights | restrictedAccess | |
dc.source | Physical Review E | |
dc.title | Complexity of Shapiro steps | en |
dc.type | article | en |
dc.rights.license | ARR | |
dcterms.abstract | Радошевић, Слободан; Пантић, Милан; Павков-Хрвојевић, Милица; Текић, Јасмина; Мали, Петар; Шакота, Aнђела; | |
dc.rights.holder | © 2020 American Physical Society | |
dc.citation.volume | 101 | |
dc.citation.issue | 3 | |
dc.citation.spage | 032203 | |
dc.identifier.wos | 000517967700003 | |
dc.identifier.doi | 10.1103/PhysRevE.101.032203 | |
dc.citation.rank | M21 | |
dc.identifier.pmid | 32289931 | |
dc.type.version | publishedVersion | |
dc.identifier.scopus | 2-s2.0-85082722520 |
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