<p>We study the Ising <i>p</i>-spin glass model for large <i>p</i>. We show that for any inverse temperature <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="440_2025_1414_Article_IEq1.gif" Format="GIF" Height="20" Rendition="HTML" Resolution="72" Type="Linedraw" Width="149" /> </InlineMediaObject> <EquationSource Format="TEX">\(\sqrt{\ln 2}&lt;\beta &lt;\sqrt{2\ln 2}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <msqrt> <mrow> <mo>ln</mo> <mn>2</mn> </mrow> </msqrt> <mo>&lt;</mo> <mi>β</mi> <mo>&lt;</mo> <msqrt> <mrow> <mn>2</mn> <mo>ln</mo> <mn>2</mn> </mrow> </msqrt> </mrow> </math></EquationSource> </InlineEquation> and any large <i>p</i>, the model exhibits <i>shattering</i>: w.h.p.&#xa0;as <InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="440_2025_1414_Article_IEq2.gif" Format="GIF" Height="10" Rendition="HTML" Resolution="72" Type="Linedraw" Width="58" /> </InlineMediaObject> <EquationSource Format="TEX">\(n\rightarrow \infty \)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>n</mi> <mo stretchy="false">→</mo> <mi>∞</mi> </mrow> </math></EquationSource> </InlineEquation>, there exists exponentially many well-separated clusters such that (a) each cluster has exponentially small Gibbs mass, and (b) the clusters collectively contain all but a vanishing fraction of Gibbs mass. Moreover, these clusters consist of configurations with energy near <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="440_2025_1414_Article_IEq3.gif" Format="GIF" Height="17" Rendition="HTML" Resolution="72" Type="Linedraw" Width="15" /> </InlineMediaObject> <EquationSource Format="TEX">\(\beta \)</EquationSource> <EquationSource Format="MATHML"><math> <mi>β</mi> </math></EquationSource> </InlineEquation>. Range of temperatures for which shattering occurs is within the <i>replica symmetric</i> region. To the best of our knowledge, this is the first shattering result regarding the Ising <i>p</i>-spin glass models. Furthermore, we show that for any <InlineEquation ID="IEq4"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="440_2025_1414_Article_IEq4.gif" Format="GIF" Height="16" Rendition="HTML" Resolution="72" Type="Linedraw" Width="43" /> </InlineMediaObject> <EquationSource Format="TEX">\(\gamma &gt;0\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>γ</mi> <mo>&gt;</mo> <mn>0</mn> </mrow> </math></EquationSource> </InlineEquation> and any large enough <i>p</i>, the model exhibits an intricate geometrical property known as the multi Overlap Gap Property above the energy value <InlineEquation ID="IEq5"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="440_2025_1414_Article_IEq5.gif" Format="GIF" Height="20" Rendition="HTML" Resolution="72" Type="Linedraw" Width="61" /> </InlineMediaObject> <EquationSource Format="TEX">\(\gamma \sqrt{2\ln 2}\)</EquationSource> <EquationSource Format="MATHML"><math> <mrow> <mi>γ</mi> <msqrt> <mrow> <mn>2</mn> <mo>ln</mo> <mn>2</mn> </mrow> </msqrt> </mrow> </math></EquationSource> </InlineEquation>. Our proofs are elementary, and in particular based on simple applications of the first and the second moment methods.</p>

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Shattering in the Ising p-spin glass model

  • David Gamarnik,
  • Aukosh Jagannath,
  • Eren C. Kızıldağ

摘要

We study the Ising p-spin glass model for large p. We show that for any inverse temperature \(\sqrt{\ln 2}<\beta <\sqrt{2\ln 2}\) ln 2 < β < 2 ln 2 and any large p, the model exhibits shattering: w.h.p. as \(n\rightarrow \infty \) n , there exists exponentially many well-separated clusters such that (a) each cluster has exponentially small Gibbs mass, and (b) the clusters collectively contain all but a vanishing fraction of Gibbs mass. Moreover, these clusters consist of configurations with energy near \(\beta \) β . Range of temperatures for which shattering occurs is within the replica symmetric region. To the best of our knowledge, this is the first shattering result regarding the Ising p-spin glass models. Furthermore, we show that for any \(\gamma >0\) γ > 0 and any large enough p, the model exhibits an intricate geometrical property known as the multi Overlap Gap Property above the energy value \(\gamma \sqrt{2\ln 2}\) γ 2 ln 2 . Our proofs are elementary, and in particular based on simple applications of the first and the second moment methods.