<p>We first show that any 4-dimensional non-Ricci-flat steady gradient Ricci soliton singularity model must satisfy <InlineEquation ID="IEq1"> <EquationSource Format="TEX">\(|{{{\,\textrm{Rm}\,}}}|\le cR\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mo stretchy="false">|</mo> <mrow> <mspace width="0.166667em" /> <mtext>Rm</mtext> <mspace width="0.166667em" /> </mrow> <mo stretchy="false">|</mo> <mo>≤</mo> <mi>c</mi> <mi>R</mi> </mrow> </math></EquationSource> </InlineEquation> for some positive constant <i>c</i>. Then, we apply the Hamilton-Ivey estimate to prove a quantitative lower bound of the curvature operator for 4-dimensional steady gradient solitons with linear scalar curvature decay and proper potential function. The technique is also used to establish a sufficient condition for a 3-dimensional expanding gradient Ricci soliton to have positive curvature. This sufficient condition is satisfied by a large class of conical expanders. As an application, we remove the positive curvature condition in a classification result by Math. Ann. 364(3–4), 777–792 (2014) in dimension three and show that any 3-dimensional gradient Ricci expander <InlineEquation ID="IEq2"> <EquationSource Format="TEX">\(C^2\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mi>C</mi> <mn>2</mn> </msup> </math></EquationSource> </InlineEquation> asymptotic to <InlineEquation ID="IEq3"> <EquationSource Format="TEX">\(\left( C(\mathbb S^2), dt^2+\alpha t^2 g_{\mathbb {S}^2}\right) \)</EquationSource> <EquationSource Format="MATHML"><math> <mfenced close=")" open="("> <mi>C</mi> <mrow> <mo stretchy="false">(</mo> <msup> <mi mathvariant="double-struck">S</mi> <mn>2</mn> </msup> <mo stretchy="false">)</mo> </mrow> <mo>,</mo> <mi>d</mi> <msup> <mi>t</mi> <mn>2</mn> </msup> <mo>+</mo> <mi>α</mi> <msup> <mi>t</mi> <mn>2</mn> </msup> <msub> <mi>g</mi> <msup> <mrow> <mi mathvariant="double-struck">S</mi> </mrow> <mn>2</mn> </msup> </msub> </mfenced> </math></EquationSource> </InlineEquation> is rotationally symmetric, where <InlineEquation ID="IEq4"> <EquationSource Format="TEX">\(\alpha \in (0,1]\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>α</mi> <mo>∈</mo> <mo stretchy="false">(</mo> <mn>0</mn> <mo>,</mo> <mn>1</mn> <mo stretchy="false">]</mo> </mrow> </math></EquationSource> </InlineEquation> is a constant and <InlineEquation ID="IEq5"> <EquationSource Format="TEX">\(g_{\mathbb {S}^2}\)</EquationSource> <EquationSource Format="MATHML"><math> <msub> <mi>g</mi> <msup> <mrow> <mi mathvariant="double-struck">S</mi> </mrow> <mn>2</mn> </msup> </msub> </math></EquationSource> </InlineEquation> is the standard metric on <InlineEquation ID="IEq6"> <EquationSource Format="TEX">\(\mathbb {S}^2\)</EquationSource> <EquationSource Format="MATHML"><math> <msup> <mrow> <mi mathvariant="double-struck">S</mi> </mrow> <mn>2</mn> </msup> </math></EquationSource> </InlineEquation> with constant curvature 1.</p>

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Hamilton-Ivey estimates for gradient Ricci solitons

  • Pak-Yeung Chan,
  • Zilu Ma,
  • Yongjia Zhang

摘要

We first show that any 4-dimensional non-Ricci-flat steady gradient Ricci soliton singularity model must satisfy \(|{{{\,\textrm{Rm}\,}}}|\le cR\) | Rm | c R for some positive constant c. Then, we apply the Hamilton-Ivey estimate to prove a quantitative lower bound of the curvature operator for 4-dimensional steady gradient solitons with linear scalar curvature decay and proper potential function. The technique is also used to establish a sufficient condition for a 3-dimensional expanding gradient Ricci soliton to have positive curvature. This sufficient condition is satisfied by a large class of conical expanders. As an application, we remove the positive curvature condition in a classification result by Math. Ann. 364(3–4), 777–792 (2014) in dimension three and show that any 3-dimensional gradient Ricci expander \(C^2\) C 2 asymptotic to \(\left( C(\mathbb S^2), dt^2+\alpha t^2 g_{\mathbb {S}^2}\right) \) C ( S 2 ) , d t 2 + α t 2 g S 2 is rotationally symmetric, where \(\alpha \in (0,1]\) α ( 0 , 1 ] is a constant and \(g_{\mathbb {S}^2}\) g S 2 is the standard metric on \(\mathbb {S}^2\) S 2 with constant curvature 1.