Well-posedness of non-isentropic Euler equations with physical vacuum
We consider the local well-posedness of the one-dimensional non-isentropic compressible Euler equations with moving physical vacuum boundary condition. The physical vacuum singularity requires the sound speed to be scaled as the square root of the distance to the vacuum boundary. The main difficulty...
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Veröffentlicht in: | Interfaces and free boundaries 2019-01, Vol.21 (2), p.231-266 |
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description | We consider the local well-posedness of the one-dimensional non-isentropic compressible Euler equations with moving physical vacuum boundary condition. The physical vacuum singularity requires the sound speed to be scaled as the square root of the distance to the vacuum boundary. The main difficulty lies in the fact that the system of hyperbolic conservation laws becomes characteristic and degenerate at the vacuum boundary. Our proof is based on an approximation of the Euler equations by a degenerate parabolic regularization obtained from a specific choice of a degenerate artificial viscosity term. Then we construct the solutions to this degenerate parabolic problem and establish the estimates that are uniform with respect to the artificial viscosity parameter. Solutions to the compressible Euler equations are obtained as the limit of the vanishing artificial viscosity. Different from the isentropic case [7, 12], our momentum equation of conservation laws has an extra term $p_{S}S_\eta$ that leads to some extra terms in the energy function and causes more difficulties even for the case of $\gamma=2$. Moreover, we deal with this free boundary problem starting from the general cases of $2\leq\gamma |
doi_str_mv | 10.4171/IFB/422 |
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The physical vacuum singularity requires the sound speed to be scaled as the square root of the distance to the vacuum boundary. The main difficulty lies in the fact that the system of hyperbolic conservation laws becomes characteristic and degenerate at the vacuum boundary. Our proof is based on an approximation of the Euler equations by a degenerate parabolic regularization obtained from a specific choice of a degenerate artificial viscosity term. Then we construct the solutions to this degenerate parabolic problem and establish the estimates that are uniform with respect to the artificial viscosity parameter. Solutions to the compressible Euler equations are obtained as the limit of the vanishing artificial viscosity. Different from the isentropic case [7, 12], our momentum equation of conservation laws has an extra term $p_{S}S_\eta$ that leads to some extra terms in the energy function and causes more difficulties even for the case of $\gamma=2$. Moreover, we deal with this free boundary problem starting from the general cases of $2\leq\gamma</description><identifier>ISSN: 1463-9963</identifier><identifier>EISSN: 1463-9971</identifier><identifier>DOI: 10.4171/IFB/422</identifier><language>eng</language><publisher>Zuerich, Switzerland: European Mathematical Society Publishing House</publisher><subject>Environmental law ; Fluid mechanics ; Partial differential equations</subject><ispartof>Interfaces and free boundaries, 2019-01, Vol.21 (2), p.231-266</ispartof><rights>European Mathematical Society</rights><rights>COPYRIGHT 2019 European Mathematical Society Publishing House</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c320t-e11f77957089fb3198c527a989f9145823656057f11f3835908b9137146553873</citedby></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,24032,27901,27902</link.rule.ids></links><search><creatorcontrib>Geng, Yongcai</creatorcontrib><creatorcontrib>Li, Yachun</creatorcontrib><creatorcontrib>Wang, Dehua</creatorcontrib><creatorcontrib>Xu, Runzhang</creatorcontrib><title>Well-posedness of non-isentropic Euler equations with physical vacuum</title><title>Interfaces and free boundaries</title><addtitle>Interfaces Free Bound</addtitle><description>We consider the local well-posedness of the one-dimensional non-isentropic compressible Euler equations with moving physical vacuum boundary condition. The physical vacuum singularity requires the sound speed to be scaled as the square root of the distance to the vacuum boundary. The main difficulty lies in the fact that the system of hyperbolic conservation laws becomes characteristic and degenerate at the vacuum boundary. Our proof is based on an approximation of the Euler equations by a degenerate parabolic regularization obtained from a specific choice of a degenerate artificial viscosity term. Then we construct the solutions to this degenerate parabolic problem and establish the estimates that are uniform with respect to the artificial viscosity parameter. Solutions to the compressible Euler equations are obtained as the limit of the vanishing artificial viscosity. Different from the isentropic case [7, 12], our momentum equation of conservation laws has an extra term $p_{S}S_\eta$ that leads to some extra terms in the energy function and causes more difficulties even for the case of $\gamma=2$. 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The physical vacuum singularity requires the sound speed to be scaled as the square root of the distance to the vacuum boundary. The main difficulty lies in the fact that the system of hyperbolic conservation laws becomes characteristic and degenerate at the vacuum boundary. Our proof is based on an approximation of the Euler equations by a degenerate parabolic regularization obtained from a specific choice of a degenerate artificial viscosity term. Then we construct the solutions to this degenerate parabolic problem and establish the estimates that are uniform with respect to the artificial viscosity parameter. Solutions to the compressible Euler equations are obtained as the limit of the vanishing artificial viscosity. Different from the isentropic case [7, 12], our momentum equation of conservation laws has an extra term $p_{S}S_\eta$ that leads to some extra terms in the energy function and causes more difficulties even for the case of $\gamma=2$. 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title | Well-posedness of non-isentropic Euler equations with physical vacuum |
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