<p>This paper deals with the initial-boundary value problem for the rotational chemotaxis system with two species and two chemicals with zero-flux boundary condition for <i>u</i>,&#xa0;<i>w</i> and zero-Neumann boundary condition for <i>v</i>,&#xa0;<i>z</i>, where <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(\Omega \)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="normal">Ω</mi> </math></EquationSource> </InlineEquation> is a bounded domain in <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(\mathbb {R}^2\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mn>2</mn> </msup> </math></EquationSource> </InlineEquation> with smooth boundary <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(\partial \Omega \)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>∂</mi> <mi mathvariant="normal">Ω</mi> </mrow> </math></EquationSource> </InlineEquation>, <Equation ID="Equ67"> <EquationSource Format="TEX">\(\begin{aligned} S_{\theta } = \Big [ \begin{array}{cc} \cos \theta &amp; -\sin \theta \\ \sin \theta &amp; \cos \theta \end{array} \Big ] \end{aligned}\)</EquationSource> <EquationSource Format="MATHML"><math display="block"> <mrow> <mtable> <mtr> <mtd columnalign="right"> <mrow> <msub> <mi>S</mi> <mi>θ</mi> </msub> <mo>=</mo> <mrow> <mo maxsize="1.623em" minsize="1.623em" stretchy="true">[</mo> </mrow> <mrow> <mtable> <mtr> <mtd> <mrow> <mo>cos</mo> <mi>θ</mi> </mrow> </mtd> <mtd> <mrow> <mo>-</mo> <mo>sin</mo> <mi>θ</mi> </mrow> </mtd> </mtr> <mtr> <mtd> <mrow> <mrow /> <mo>sin</mo> <mi>θ</mi> </mrow> </mtd> <mtd> <mrow> <mo>cos</mo> <mi>θ</mi> </mrow> </mtd> </mtr> </mtable> </mrow> <mrow> <mo maxsize="1.623em" minsize="1.623em" stretchy="true">]</mo> </mrow> </mrow> </mtd> </mtr> </mtable> </mrow> </math></EquationSource> </Equation>is a rotation matrix with <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(\theta \in (-\frac{\pi }{2}, \frac{\pi }{2})\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>θ</mi> <mo>∈</mo> <mo stretchy="false">(</mo> <mo>-</mo> <mfrac> <mi>π</mi> <mn>2</mn> </mfrac> <mo>,</mo> <mfrac> <mi>π</mi> <mn>2</mn> </mfrac> <mo stretchy="false">)</mo> </mrow> </math></EquationSource> </InlineEquation> and <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\(\chi ,\xi ,\alpha ,\beta ,\gamma ,\delta &gt;0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>χ</mi> <mo>,</mo> <mi>ξ</mi> <mo>,</mo> <mi>α</mi> <mo>,</mo> <mi>β</mi> <mo>,</mo> <mi>γ</mi> <mo>,</mo> <mi>δ</mi> <mo>&gt;</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation>. Let <InlineEquation ID="IEq6"> <EquationSource Format="TEX">\(m_1,m_2\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mi>m</mi> <mn>1</mn> </msub> <mo>,</mo> <msub> <mi>m</mi> <mn>2</mn> </msub> </mrow> </math></EquationSource> </InlineEquation> be the initial mass for <i>u</i> and <i>w</i> respectively. We show that:<UnorderedList Mark="Bullet"> <ItemContent> <p>If <InlineEquation ID="IEq7"> <EquationSource Format="TEX">\(m_1m_2- \frac{4\pi }{\cos \theta }(\frac{m_1}{\chi \beta }+\frac{m_2}{\xi \delta })&gt;0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mi>m</mi> <mn>1</mn> </msub> <msub> <mi>m</mi> <mn>2</mn> </msub> <mo>-</mo> <mfrac> <mrow> <mn>4</mn> <mi>π</mi> </mrow> <mrow> <mo>cos</mo> <mi>θ</mi> </mrow> </mfrac> <mrow> <mo stretchy="false">(</mo> <mfrac> <msub> <mi>m</mi> <mn>1</mn> </msub> <mrow> <mi>χ</mi> <mi>β</mi> </mrow> </mfrac> <mo>+</mo> <mfrac> <msub> <mi>m</mi> <mn>2</mn> </msub> <mrow> <mi>ξ</mi> <mi>δ</mi> </mrow> </mfrac> <mo stretchy="false">)</mo> </mrow> <mo>&gt;</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation>, then there exists finite-time blow-up solution to the system (<InlineEquation ID="IEq8"> <EquationSource Format="TEX">\(\star \)</EquationSource> <EquationSource Format="MATHML"><math> <mo>⋆</mo> </math></EquationSource> </InlineEquation>);</p> </ItemContent> <ItemContent> <p>If <InlineEquation ID="IEq9"> <EquationSource Format="TEX">\(m_1m_2- \frac{2\pi }{\cos \theta }(\frac{m_1}{\chi \beta }+\frac{m_2}{\xi \delta })&gt;0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mi>m</mi> <mn>1</mn> </msub> <msub> <mi>m</mi> <mn>2</mn> </msub> <mo>-</mo> <mfrac> <mrow> <mn>2</mn> <mi>π</mi> </mrow> <mrow> <mo>cos</mo> <mi>θ</mi> </mrow> </mfrac> <mrow> <mo stretchy="false">(</mo> <mfrac> <msub> <mi>m</mi> <mn>1</mn> </msub> <mrow> <mi>χ</mi> <mi>β</mi> </mrow> </mfrac> <mo>+</mo> <mfrac> <msub> <mi>m</mi> <mn>2</mn> </msub> <mrow> <mi>ξ</mi> <mi>δ</mi> </mrow> </mfrac> <mo stretchy="false">)</mo> </mrow> <mo>&gt;</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation> and <InlineEquation ID="IEq10"> <EquationSource Format="TEX">\(\partial \Omega \)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>∂</mi> <mi mathvariant="normal">Ω</mi> </mrow> </math></EquationSource> </InlineEquation> contains a line segment, then there exists finite-time blow-up solution to the system (<InlineEquation ID="IEq11"> <EquationSource Format="TEX">\(\star \)</EquationSource> <EquationSource Format="MATHML"><math> <mo>⋆</mo> </math></EquationSource> </InlineEquation>).</p> </ItemContent> </UnorderedList> We point out that if <InlineEquation ID="IEq12"> <EquationSource Format="TEX">\(\Omega \)</EquationSource> <EquationSource Format="MATHML"><math> <mi mathvariant="normal">Ω</mi> </math></EquationSource> </InlineEquation> is a disc in <InlineEquation ID="IEq13"> <EquationSource Format="TEX">\(\mathbb {R}^2\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mn>2</mn> </msup> </math></EquationSource> </InlineEquation> and <InlineEquation ID="IEq14"> <EquationSource Format="TEX">\(m_1m_2- \frac{2\pi }{\cos \theta }(\frac{m_1}{\chi \beta }+\frac{m_2}{\xi \delta })&lt;0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mi>m</mi> <mn>1</mn> </msub> <msub> <mi>m</mi> <mn>2</mn> </msub> <mo>-</mo> <mfrac> <mrow> <mn>2</mn> <mi>π</mi> </mrow> <mrow> <mo>cos</mo> <mi>θ</mi> </mrow> </mfrac> <mrow> <mo stretchy="false">(</mo> <mfrac> <msub> <mi>m</mi> <mn>1</mn> </msub> <mrow> <mi>χ</mi> <mi>β</mi> </mrow> </mfrac> <mo>+</mo> <mfrac> <msub> <mi>m</mi> <mn>2</mn> </msub> <mrow> <mi>ξ</mi> <mi>δ</mi> </mrow> </mfrac> <mo stretchy="false">)</mo> </mrow> <mo>&lt;</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation>, it is easy to show that the global existence of the solution to the system (<InlineEquation ID="IEq15"> <EquationSource Format="TEX">\(\star \)</EquationSource> <EquationSource Format="MATHML"><math> <mo>⋆</mo> </math></EquationSource> </InlineEquation>) using the energy functional method. Therefore, the line <InlineEquation ID="IEq16"> <EquationSource Format="TEX">\(m_1m_2- \frac{2\pi }{\cos \theta }(\frac{m_1}{\chi \beta }+\frac{m_2}{\xi \delta })=0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msub> <mi>m</mi> <mn>1</mn> </msub> <msub> <mi>m</mi> <mn>2</mn> </msub> <mo>-</mo> <mfrac> <mrow> <mn>2</mn> <mi>π</mi> </mrow> <mrow> <mo>cos</mo> <mi>θ</mi> </mrow> </mfrac> <mrow> <mo stretchy="false">(</mo> <mfrac> <msub> <mi>m</mi> <mn>1</mn> </msub> <mrow> <mi>χ</mi> <mi>β</mi> </mrow> </mfrac> <mo>+</mo> <mfrac> <msub> <mi>m</mi> <mn>2</mn> </msub> <mrow> <mi>ξ</mi> <mi>δ</mi> </mrow> </mfrac> <mo stretchy="false">)</mo> </mrow> <mo>=</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation> is critical in this sense.</p>

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Local Existence and Finite-Time Blow-up in a Rotational Chemotaxis System with Two Species and Two Chemicals

  • Hengling Wang,
  • Jianlu Yan

摘要

This paper deals with the initial-boundary value problem for the rotational chemotaxis system with two species and two chemicals with zero-flux boundary condition for uw and zero-Neumann boundary condition for vz, where \(\Omega \) Ω is a bounded domain in \(\mathbb {R}^2\) R 2 with smooth boundary \(\partial \Omega \) Ω , \(\begin{aligned} S_{\theta } = \Big [ \begin{array}{cc} \cos \theta & -\sin \theta \\ \sin \theta & \cos \theta \end{array} \Big ] \end{aligned}\) S θ = [ cos θ - sin θ sin θ cos θ ] is a rotation matrix with \(\theta \in (-\frac{\pi }{2}, \frac{\pi }{2})\) θ ( - π 2 , π 2 ) and \(\chi ,\xi ,\alpha ,\beta ,\gamma ,\delta >0\) χ , ξ , α , β , γ , δ > 0 . Let \(m_1,m_2\) m 1 , m 2 be the initial mass for u and w respectively. We show that:

If \(m_1m_2- \frac{4\pi }{\cos \theta }(\frac{m_1}{\chi \beta }+\frac{m_2}{\xi \delta })>0\) m 1 m 2 - 4 π cos θ ( m 1 χ β + m 2 ξ δ ) > 0 , then there exists finite-time blow-up solution to the system ( \(\star \) );

If \(m_1m_2- \frac{2\pi }{\cos \theta }(\frac{m_1}{\chi \beta }+\frac{m_2}{\xi \delta })>0\) m 1 m 2 - 2 π cos θ ( m 1 χ β + m 2 ξ δ ) > 0 and \(\partial \Omega \) Ω contains a line segment, then there exists finite-time blow-up solution to the system ( \(\star \) ).

We point out that if \(\Omega \) Ω is a disc in \(\mathbb {R}^2\) R 2 and \(m_1m_2- \frac{2\pi }{\cos \theta }(\frac{m_1}{\chi \beta }+\frac{m_2}{\xi \delta })<0\) m 1 m 2 - 2 π cos θ ( m 1 χ β + m 2 ξ δ ) < 0 , it is easy to show that the global existence of the solution to the system ( \(\star \) ) using the energy functional method. Therefore, the line \(m_1m_2- \frac{2\pi }{\cos \theta }(\frac{m_1}{\chi \beta }+\frac{m_2}{\xi \delta })=0\) m 1 m 2 - 2 π cos θ ( m 1 χ β + m 2 ξ δ ) = 0 is critical in this sense.