Measuring α-FPUT Cores and Tails
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Flach Sergej | - |
dc.date.accessioned | 2022-07-29T08:10:26Z | - |
dc.date.available | 2022-07-29T08:10:26Z | - |
dc.date.created | 2021-12-17 | - |
dc.date.issued | 2021-12 | - |
dc.identifier.issn | 2624-8174 | - |
dc.identifier.uri | https://pr.ibs.re.kr/handle/8788114/12080 | - |
dc.description.abstract | Almost 70 years ago, the Fermi–Pasta–Ulam–Tsingou (FPUT) paradox was formulated in, observed in, and reported using normal modes of a nonlinear, one-dimensional, non-integrable string. Let us recap the paradox. One normal mode is excited, which drives three or four more normal modes in the core. Then, that is it for quite a long time. So why are many normal modes staying weakly excited in the tail? Furthermore, how many? A quantitative, analytical answer to the latter question is given here using resonances and secular avalanches A comparison with the previous numerical data is made and extremely good agreement is found. | - |
dc.publisher | MDPI AG | - |
dc.title | Measuring α-FPUT Cores and Tails | - |
dc.type | Article | - |
dc.type.rims | ART | - |
dc.identifier.scopusid | 2-s2.0-85124937723 | - |
dc.identifier.rimsid | 76913 | - |
dc.contributor.affiliatedAuthor | Flach Sergej | - |
dc.identifier.doi | 10.3390/physics3040054 | - |
dc.identifier.bibliographicCitation | Physics, v.3, no.4, pp.879 - 887 | - |
dc.relation.isPartOf | Physics | - |
dc.citation.title | Physics | - |
dc.citation.volume | 3 | - |
dc.citation.number | 4 | - |
dc.citation.startPage | 879 | - |
dc.citation.endPage | 887 | - |
dc.description.journalClass | 1 | - |
dc.description.journalClass | 1 | - |
dc.description.isOpenAccess | N | - |
dc.description.journalRegisteredClass | scopus | - |
dc.description.journalRegisteredClass | other | - |
dc.subject.keywordAuthor | Fermi–Pasta–Ulam–Tsingou (FPUT) problem | - |
dc.subject.keywordAuthor | normal modes | - |
dc.subject.keywordAuthor | resonances | - |
dc.subject.keywordAuthor | secular avalanche | - |