{"title":"A Research Note on a Solution of Stefan Problem with Fractional Time and Space Derivatives","authors":"R. Meĭlanov, M. Shabanova, É. Akhmedov","doi":"10.15866/IREPHY.V11I2.12593","DOIUrl":null,"url":null,"abstract":"Stefan problem based on nonlocal heat conduction equation with fractional-time derivatives has been solved. The approach suggests a generalized time-dependent Stefan boundary condition defined by expression ϑ(α, β, τ) = σ(α, β)τ^(α/β). The solution developed shows that the phase change boundary co-ordinate ϑ depends on time τ and the parameters α (0<α≤1) and β (1<β≤2) which are the fractional orders with respect to the time and the space co-ordinate , respectively. A practical example with ice-water system was used to exemplify the solution with both α and β near to α = 1 and β = 1 (the classical problem).","PeriodicalId":448231,"journal":{"name":"International Review of Physics","volume":"84 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2017-04-30","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"International Review of Physics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.15866/IREPHY.V11I2.12593","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 2
Abstract
Stefan problem based on nonlocal heat conduction equation with fractional-time derivatives has been solved. The approach suggests a generalized time-dependent Stefan boundary condition defined by expression ϑ(α, β, τ) = σ(α, β)τ^(α/β). The solution developed shows that the phase change boundary co-ordinate ϑ depends on time τ and the parameters α (0<α≤1) and β (1<β≤2) which are the fractional orders with respect to the time and the space co-ordinate , respectively. A practical example with ice-water system was used to exemplify the solution with both α and β near to α = 1 and β = 1 (the classical problem).