<p>We introduce anisotropic Hölder spaces that are useful for studying the regularity theory for non-local kinetic operators <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="28_2025_1062_Article_IEq1.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="25" /> </InlineMediaObject> <EquationSource Format="TEX">\(\mathscr {L}\)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="script">L</mi> </math></EquationSource> </InlineEquation>, whose prototypical example is <Equation ID="Equ36"> <MediaObject> <ImageObject Color="BlackWhite" FileRef="28_2025_1062_Article_Equ36.gif" Format="GIF" Height="41" Rendition="HTML" Resolution="72" Type="Linedraw" Width="502" /> </MediaObject> <EquationSource Format="TEX">\(\begin{aligned} \mathscr {L}u (t,x,v) = \int _{{{\mathbb {R}}}^d} \frac{C_{d,s}}{|v - v'|^{d+2s}} (u(t,x,v') - u(t,x,v)) \textrm{d}v' + \langle v, \nabla _x \rangle + \partial _t, \end{aligned}\)</EquationSource> <EquationSource Format="MATHML"><math display="block"> <mrow> <mtable> <mtr> <mtd columnalign="right"> <mrow> <mi mathvariant="script">L</mi> <mi>u</mi> <mrow> <mo stretchy="false">(</mo> <mi>t</mi> <mo>,</mo> <mi>x</mi> <mo>,</mo> <mi>v</mi> <mo stretchy="false">)</mo> </mrow> <mo>=</mo> <msub> <mo>∫</mo> <msup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mi>d</mi> </msup> </msub> <mfrac> <msub> <mi>C</mi> <mrow> <mi>d</mi> <mo>,</mo> <mi>s</mi> </mrow> </msub> <mrow> <mrow> <mo stretchy="false">|</mo> <mi>v</mi> <mo>-</mo> </mrow> <msup> <mi>v</mi> <mo>′</mo> </msup> <msup> <mrow> <mo stretchy="false">|</mo> </mrow> <mrow> <mi>d</mi> <mo>+</mo> <mn>2</mn> <mi>s</mi> </mrow> </msup> </mrow> </mfrac> <mrow> <mo stretchy="false">(</mo> <mi>u</mi> <mrow> <mo stretchy="false">(</mo> <mi>t</mi> <mo>,</mo> <mi>x</mi> <mo>,</mo> <msup> <mi>v</mi> <mo>′</mo> </msup> <mo stretchy="false">)</mo> </mrow> <mo>-</mo> <mi>u</mi> <mrow> <mo stretchy="false">(</mo> <mi>t</mi> <mo>,</mo> <mi>x</mi> <mo>,</mo> <mi>v</mi> <mo stretchy="false">)</mo> </mrow> <mo stretchy="false">)</mo> </mrow> <mtext>d</mtext> <msup> <mi>v</mi> <mo>′</mo> </msup> <mo>+</mo> <mrow> <mo stretchy="false">⟨</mo> <mi>v</mi> <mo>,</mo> <msub> <mi mathvariant="normal">∇</mi> <mi>x</mi> </msub> <mo stretchy="false">⟩</mo> </mrow> <mo>+</mo> <msub> <mi>∂</mi> <mi>t</mi> </msub> <mo>,</mo> </mrow> </mtd> </mtr> </mtable> </mrow> </math></EquationSource> </Equation>with <InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="28_2025_1062_Article_IEq2.gif" Format="GIF" Height="21" Rendition="HTML" Resolution="72" Type="Linedraw" Width="130" /> </InlineMediaObject> <EquationSource Format="TEX">\((t,x,v)\in {{\mathbb {R}}}\times {{\mathbb {R}}}^{2d}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mrow> <mo stretchy="false">(</mo> <mi>t</mi> <mo>,</mo> <mi>x</mi> <mo>,</mo> <mi>v</mi> <mo stretchy="false">)</mo> </mrow> <mo>∈</mo> <mi mathvariant="double-struck">R</mi> <mo>×</mo> <msup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mrow> <mn>2</mn> <mi>d</mi> </mrow> </msup> </mrow> </math></EquationSource> </InlineEquation>. The Hölder spaces are defined in terms of an anisotropic distance relevant to the Galilean geometric structure on <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="28_2025_1062_Article_IEq3.gif" Format="GIF" Height="18" Rendition="HTML" Resolution="72" Type="Linedraw" Width="57" /> </InlineMediaObject> <EquationSource Format="TEX">\({{\mathbb {R}}}\times {{\mathbb {R}}}^{2d}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi mathvariant="double-struck">R</mi> <mo>×</mo> <msup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mrow> <mn>2</mn> <mi>d</mi> </mrow> </msup> </mrow> </math></EquationSource> </InlineEquation>, with respect to which the operator <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="28_2025_1062_Article_IEq1.gif" Format="GIF" Height="14" Rendition="HTML" Resolution="72" Type="Linedraw" Width="25" /> </InlineMediaObject> <EquationSource Format="TEX">\(\mathscr {L}\)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="script">L</mi> </math></EquationSource> </InlineEquation> is invariant. We prove an intrinsic Taylor-like formula, whose remainder is bounded in terms of the anisotropic distance of the Galilean structure. Our achievements naturally extend analogous known results for purely differential operators on Lie groups.</p>

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Intrinsic Hölder spaces for fractional kinetic operators

  • Maria Manfredini,
  • Stefano Pagliarani,
  • Sergio Polidoro

摘要

We introduce anisotropic Hölder spaces that are useful for studying the regularity theory for non-local kinetic operators \(\mathscr {L}\) L , whose prototypical example is \(\begin{aligned} \mathscr {L}u (t,x,v) = \int _{{{\mathbb {R}}}^d} \frac{C_{d,s}}{|v - v'|^{d+2s}} (u(t,x,v') - u(t,x,v)) \textrm{d}v' + \langle v, \nabla _x \rangle + \partial _t, \end{aligned}\) L u ( t , x , v ) = R d C d , s | v - v | d + 2 s ( u ( t , x , v ) - u ( t , x , v ) ) d v + v , x + t , with \((t,x,v)\in {{\mathbb {R}}}\times {{\mathbb {R}}}^{2d}\) ( t , x , v ) R × R 2 d . The Hölder spaces are defined in terms of an anisotropic distance relevant to the Galilean geometric structure on \({{\mathbb {R}}}\times {{\mathbb {R}}}^{2d}\) R × R 2 d , with respect to which the operator \(\mathscr {L}\) L is invariant. We prove an intrinsic Taylor-like formula, whose remainder is bounded in terms of the anisotropic distance of the Galilean structure. Our achievements naturally extend analogous known results for purely differential operators on Lie groups.