<p>This paper is concerned with a critical mass phenomenon in the following nonlinear Keller–Segel system with indirect signal production <Equation ID="Equ238"> <MediaObject ID="MO1"> <ImageObject Color="BlackWhite" FileRef="MediaObjects/28_2026_1214_Equ238_HTML.png" Format="PNG" Height="200" Rendition="HTML" Resolution="300" Type="Linedraw" Width="1187" /> </MediaObject> </Equation>proposed on <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(\Omega :=B_R(0) \subset \mathbb {R}^n(n\geqslant 2) \)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi mathvariant="normal">Ω</mi> <mo>:</mo> <mo>=</mo> <msub> <mi>B</mi> <mi>R</mi> </msub> <mrow> <mo stretchy="false">(</mo> <mn>0</mn> <mo stretchy="false">)</mo> </mrow> <mo>⊂</mo> <msup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mi>n</mi> </msup> <mrow> <mo stretchy="false">(</mo> <mi>n</mi> <mo>⩾</mo> <mn>2</mn> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation> and subjected to homogeneous Neumann boundary conditions. According to the paper (Jin and Li in Nonlinear Anal 89, Paper No. 104523, 2026), the system (<InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(\star \)</EquationSource> <EquationSource Format="MATHML"><math> <mo>⋆</mo> </math></EquationSource> </InlineEquation>) in radial setting admits <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(\frac{2}{n}\)</EquationSource> <EquationSource Format="MATHML"><math> <mfrac> <mn>2</mn> <mi>n</mi> </mfrac> </math></EquationSource> </InlineEquation> as a critical exponent in the sense that if <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(\alpha &lt; \frac{2}{n}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>α</mi> <mo>&lt;</mo> <mfrac> <mn>2</mn> <mi>n</mi> </mfrac> </mrow> </math></EquationSource> </InlineEquation>, all solutions exist globally and if <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\(\alpha &gt; \frac{2}{n}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>α</mi> <mo>&gt;</mo> <mfrac> <mn>2</mn> <mi>n</mi> </mfrac> </mrow> </math></EquationSource> </InlineEquation>, there exist finite-time blowup solutions. In this paper, we further demonstrate a critical mass phenomenon in the supercritical case <InlineEquation ID="IEq6"> <EquationSource Format="TEX">\( \alpha \geqslant \frac{2}{n}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>α</mi> <mo>⩾</mo> <mfrac> <mn>2</mn> <mi>n</mi> </mfrac> </mrow> </math></EquationSource> </InlineEquation>. More precisely, there exists a critical mass <InlineEquation ID="IEq7"> <EquationSource Format="TEX">\(m_c:= m_c(n, R, \alpha )\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mi>m</mi> <mi>c</mi> </msub> <mo>:</mo> <mo>=</mo> <msub> <mi>m</mi> <mi>c</mi> </msub> <mrow> <mo stretchy="false">(</mo> <mi>n</mi> <mo>,</mo> <mi>R</mi> <mo>,</mo> <mi>α</mi> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation> such that<UnorderedList Mark="Bullet"> <ItemContent> <p>for arbitrary nonconstant radial initial data <InlineEquation ID="IEq8"> <EquationSource Format="TEX">\((u_0, w_0)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mo stretchy="false">(</mo> <msub> <mi>u</mi> <mn>0</mn> </msub> <mo>,</mo> <msub> <mi>w</mi> <mn>0</mn> </msub> <mo stretchy="false">)</mo> </mrow> </math></EquationSource> </InlineEquation> satisfying <InlineEquation ID="IEq9"> <EquationSource Format="TEX">\(\int _{\Omega } u_0&gt;m_c\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mo>∫</mo> <mi mathvariant="normal">Ω</mi> </msub> <msub> <mi>u</mi> <mn>0</mn> </msub> <mo>&gt;</mo> <msub> <mi>m</mi> <mi>c</mi> </msub> </mrow> </math></EquationSource> </InlineEquation>, <InlineEquation ID="IEq10"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="MediaObjects/28_2026_1214_IEq10_HTML.gif" Format="GIF" Height="23" Rendition="HTML" Resolution="120" Type="Linedraw" Width="104" /> </InlineMediaObject> </InlineEquation> and <InlineEquation ID="IEq11"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="MediaObjects/28_2026_1214_IEq11_HTML.gif" Format="GIF" Height="23" Rendition="HTML" Resolution="120" Type="Linedraw" Width="110" /> </InlineMediaObject> </InlineEquation> for all <InlineEquation ID="IEq12"> <EquationSource Format="TEX">\(r \in (0,R)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>r</mi> <mo>∈</mo> <mo stretchy="false">(</mo> <mn>0</mn> <mo>,</mo> <mi>R</mi> <mo stretchy="false">)</mo> </mrow> </math></EquationSource> </InlineEquation>, if <InlineEquation ID="IEq13"> <EquationSource Format="TEX">\(\alpha &gt;\frac{2}{n}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>α</mi> <mo>&gt;</mo> <mfrac> <mn>2</mn> <mi>n</mi> </mfrac> </mrow> </math></EquationSource> </InlineEquation>, the corresponding solution blows up in finite time; if <InlineEquation ID="IEq14"> <EquationSource Format="TEX">\(\alpha =\frac{2}{n}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>α</mi> <mo>=</mo> <mfrac> <mn>2</mn> <mi>n</mi> </mfrac> </mrow> </math></EquationSource> </InlineEquation>, the corresponding solution blows up in infinite time and forms a Dirac-type distribution as times goes to infinity.</p> </ItemContent> <ItemContent> <p>there exist nonconstant, regular, and radial initial data <InlineEquation ID="IEq15"> <EquationSource Format="TEX">\((u_0, w_0)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mo stretchy="false">(</mo> <msub> <mi>u</mi> <mn>0</mn> </msub> <mo>,</mo> <msub> <mi>w</mi> <mn>0</mn> </msub> <mo stretchy="false">)</mo> </mrow> </math></EquationSource> </InlineEquation> with <InlineEquation ID="IEq16"> <EquationSource Format="TEX">\(\int _{\Omega } u_0&lt;m_c\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mo>∫</mo> <mi mathvariant="normal">Ω</mi> </msub> <msub> <mi>u</mi> <mn>0</mn> </msub> <mo>&lt;</mo> <msub> <mi>m</mi> <mi>c</mi> </msub> </mrow> </math></EquationSource> </InlineEquation> such that the corresponding solution is global.</p> </ItemContent> </UnorderedList></p>

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Critical mass phenomenon in a nonlinear Keller–Segel system with indirect signal production

  • Chaopeng Dai,
  • Yuxiang Li,
  • Jianlu Yan

摘要

This paper is concerned with a critical mass phenomenon in the following nonlinear Keller–Segel system with indirect signal production proposed on \(\Omega :=B_R(0) \subset \mathbb {R}^n(n\geqslant 2) \) Ω : = B R ( 0 ) R n ( n 2 ) and subjected to homogeneous Neumann boundary conditions. According to the paper (Jin and Li in Nonlinear Anal 89, Paper No. 104523, 2026), the system ( \(\star \) ) in radial setting admits \(\frac{2}{n}\) 2 n as a critical exponent in the sense that if \(\alpha < \frac{2}{n}\) α < 2 n , all solutions exist globally and if \(\alpha > \frac{2}{n}\) α > 2 n , there exist finite-time blowup solutions. In this paper, we further demonstrate a critical mass phenomenon in the supercritical case \( \alpha \geqslant \frac{2}{n}\) α 2 n . More precisely, there exists a critical mass \(m_c:= m_c(n, R, \alpha )\) m c : = m c ( n , R , α ) such that

for arbitrary nonconstant radial initial data \((u_0, w_0)\) ( u 0 , w 0 ) satisfying \(\int _{\Omega } u_0>m_c\) Ω u 0 > m c , and for all \(r \in (0,R)\) r ( 0 , R ) , if \(\alpha >\frac{2}{n}\) α > 2 n , the corresponding solution blows up in finite time; if \(\alpha =\frac{2}{n}\) α = 2 n , the corresponding solution blows up in infinite time and forms a Dirac-type distribution as times goes to infinity.

there exist nonconstant, regular, and radial initial data \((u_0, w_0)\) ( u 0 , w 0 ) with \(\int _{\Omega } u_0<m_c\) Ω u 0 < m c such that the corresponding solution is global.