<p>For a system in <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(\mathbb {R}^n\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mi>n</mi> </msup> </math></EquationSource> </InlineEquation> consisting of an unstable star node and homogeneous nonlinearity, i.e. <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(\dot{x}=\mu x+Q(x)\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mover accent="true"> <mi>x</mi> <mo>˙</mo> </mover> <mo>=</mo> <mi>μ</mi> <mi>x</mi> <mo>+</mo> <mi>Q</mi> <mrow> <mo stretchy="false">(</mo> <mi>x</mi> <mo stretchy="false">)</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation> with <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(\mu &gt;0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>μ</mi> <mo>&gt;</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation> and <i>Q</i>(<i>x</i>) a homogeneous polynomial satisfying <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(xQ(x)&lt;0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>x</mi> <mi>Q</mi> <mo stretchy="false">(</mo> <mi>x</mi> <mo stretchy="false">)</mo> <mo>&lt;</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation> for all <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\(x\ne 0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>x</mi> <mo>≠</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation>, Field in 1989 proved the existence of a unique topological invariant sphere. Here restricted to <InlineEquation ID="IEq6"> <EquationSource Format="TEX">\(n=2\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>n</mi> <mo>=</mo> <mn>2</mn> </mrow> </math></EquationSource> </InlineEquation>, we prove that the topological invariant circle is of star shape, and obtain the classification of all their phase portraits in the Poincaré disc when <i>Q</i> is of degree 5 and the invariant circle is the circle <InlineEquation ID="IEq7"> <EquationSource Format="TEX">\({\mathbb {S}}^1=\{(x,y,z) \in \mathbb {R}^3|\ x^2+y^2+z^2=1\}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msup> <mrow> <mi mathvariant="double-struck">S</mi> </mrow> <mn>1</mn> </msup> <mo>=</mo> <mrow> <mo stretchy="false">{</mo> <mrow> <mo stretchy="false">(</mo> <mi>x</mi> <mo>,</mo> <mi>y</mi> <mo>,</mo> <mi>z</mi> <mo stretchy="false">)</mo> </mrow> <mo>∈</mo> <msup> <mrow> <mi mathvariant="double-struck">R</mi> </mrow> <mn>3</mn> </msup> <mo stretchy="false">|</mo> <mspace width="4pt" /> <msup> <mi>x</mi> <mn>2</mn> </msup> <mo>+</mo> <msup> <mi>y</mi> <mn>2</mn> </msup> <mo>+</mo> <msup> <mi>z</mi> <mn>2</mn> </msup> <mo>=</mo> <mn>1</mn> <mo stretchy="false">}</mo> </mrow> </mrow> </math></EquationSource> </InlineEquation>. Moreover, without the restriction <InlineEquation ID="IEq8"> <EquationSource Format="TEX">\(xQ(x)&lt;0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>x</mi> <mi>Q</mi> <mo stretchy="false">(</mo> <mi>x</mi> <mo stretchy="false">)</mo> <mo>&lt;</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation> we characterize the relation between equilibria (both finite and infinite) and the invariant straight lines passing through the origin. These results extend and improve the previous results of other authors.</p>

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On the Invariant Sphere Theorem

  • Jaume Llibre,
  • Xiang Zhang

摘要

For a system in \(\mathbb {R}^n\) R n consisting of an unstable star node and homogeneous nonlinearity, i.e. \(\dot{x}=\mu x+Q(x)\) x ˙ = μ x + Q ( x ) with \(\mu >0\) μ > 0 and Q(x) a homogeneous polynomial satisfying \(xQ(x)<0\) x Q ( x ) < 0 for all \(x\ne 0\) x 0 , Field in 1989 proved the existence of a unique topological invariant sphere. Here restricted to \(n=2\) n = 2 , we prove that the topological invariant circle is of star shape, and obtain the classification of all their phase portraits in the Poincaré disc when Q is of degree 5 and the invariant circle is the circle \({\mathbb {S}}^1=\{(x,y,z) \in \mathbb {R}^3|\ x^2+y^2+z^2=1\}\) S 1 = { ( x , y , z ) R 3 | x 2 + y 2 + z 2 = 1 } . Moreover, without the restriction \(xQ(x)<0\) x Q ( x ) < 0 we characterize the relation between equilibria (both finite and infinite) and the invariant straight lines passing through the origin. These results extend and improve the previous results of other authors.