<p>We prove existence of martingale solutions to a class of stochastic thin-film equations for mobility exponents <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(n \in (2,3)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>n</mi> <mo>∈</mo> <mo stretchy="false">(</mo> <mn>2</mn> <mo>,</mo> <mn>3</mn> <mo stretchy="false">)</mo> </mrow> </math></EquationSource> </InlineEquation> and compactly supported initial data. With the perspective to study free-boundary problems related to stochastic thin-film equations in Grün and Klein (SIAM J Math Anal), we start from the surface-tension driven stochastic thin-film equation with Stratonovich noise and exploit the regime of coefficients in front of the Stratonovich correction term (which—under natural assumptions on the spatially colored noise—is of porous-media-type) for which energy dissipation can be established. By Bernis inequalities, third order spatial derivatives of appropriate powers of the solution are controlled. Analytically, we rely on approximation with <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\({\mathbb {P}}\)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="double-struck">P</mi> </math></EquationSource> </InlineEquation>-almost surely strictly positive solutions and compactness methods based on energy-entropy estimates as well as martingale identification techniques.</p>

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Existence of nonnegative energy-dissipating solutions to a class of stochastic thin-film equations under weak slippage: part II—compactly supported initial data

  • Günther Grün,
  • Lorenz Klein

摘要

We prove existence of martingale solutions to a class of stochastic thin-film equations for mobility exponents \(n \in (2,3)\) n ( 2 , 3 ) and compactly supported initial data. With the perspective to study free-boundary problems related to stochastic thin-film equations in Grün and Klein (SIAM J Math Anal), we start from the surface-tension driven stochastic thin-film equation with Stratonovich noise and exploit the regime of coefficients in front of the Stratonovich correction term (which—under natural assumptions on the spatially colored noise—is of porous-media-type) for which energy dissipation can be established. By Bernis inequalities, third order spatial derivatives of appropriate powers of the solution are controlled. Analytically, we rely on approximation with \({\mathbb {P}}\) P -almost surely strictly positive solutions and compactness methods based on energy-entropy estimates as well as martingale identification techniques.