<p>To address the longstanding tension between the Constrained Minimal Supersymmetric Standard Model (CMSSM) and recent experimental data, we investigate non-universal gaugino masses within an SU(5) Grand Unified Theory (GUT) framework, focusing on the <InlineEquation ID="IEq1"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_25863_Article_IEq1.gif" Format="GIF" Height="20" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mover accent="true"> <mi>g</mi> <mo stretchy="true">~</mo> </mover> </math></EquationSource> <EquationSource Format="TEX">\( \overset{\sim }{g} \)</EquationSource> </InlineEquation>-SUGRA scenario where |<i>M</i><sub>3</sub>| ≫ |<i>M</i><sub>1</sub>|<i>,</i> |<i>M</i><sub>2</sub>|. This hierarchy enables a heavier gluino, thereby evading current experimental bounds on supersymmetric particles. Our analysis reveals that precise Higgs measurements place stringent constraints on the model, requiring tan <i>β</i> ≳ 5 and <i>M</i><sub>0</sub> ≳ 20 tan <i>β</i> GeV<i>.</i> Although the <InlineEquation ID="IEq2"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_25863_Article_IEq2.gif" Format="GIF" Height="20" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mover accent="true"> <mi>g</mi> <mo stretchy="true">~</mo> </mover> </math></EquationSource> <EquationSource Format="TEX">\( \overset{\sim }{g} \)</EquationSource> </InlineEquation>-SUGRA scenario can help reconcile the persistent (<i>g −</i> 2)<sub><i>μ</i></sub> anomaly, the Higgs constraints significantly restrict its parameter space, making a large contribution to (<i>g −</i> 2)<sub><i>μ</i></sub> challenging. We also assess the discovery prospects in upcoming dark matter direct detection experiments, including PandaX-xT (200 t.y.), LZ (projected), and XENONnT (20 t.y.), which may not fully cover the viable parameter space. In contrast, future collider experiments — such as the High-Luminosity LHC at 3 ab<sup><i>−</i>1</sup> and CLIC<sub>1500</sub> at 2<i>.</i>5 ab<sup><i>−</i>1</sup> — can comprehensively probe the remaining regions. These findings highlight <InlineEquation ID="IEq3"> <InlineMediaObject> <ImageObject Color="BlackWhite" FileRef="13130_2025_25863_Article_IEq3.gif" Format="GIF" Height="20" Rendition="HTML" Resolution="72" Type="Linedraw" Width="13" /> </InlineMediaObject> <EquationSource Format="MATHML"><math display="inline"> <mover accent="true"> <mi>g</mi> <mo stretchy="true">~</mo> </mover> </math></EquationSource> <EquationSource Format="TEX">\( \overset{\sim }{g} \)</EquationSource> </InlineEquation>-SUGRA as a promising solution to the CMSSM tension and offer clear, testable predictions for upcoming collider searches.</p>

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Revisiting CMSSM with non-universal gaugino masses under current constraints

  • Yabo Dong,
  • Kun Wang,
  • Hailong Yuan,
  • Jingya Zhu,
  • Pengxuan Zhu

摘要

To address the longstanding tension between the Constrained Minimal Supersymmetric Standard Model (CMSSM) and recent experimental data, we investigate non-universal gaugino masses within an SU(5) Grand Unified Theory (GUT) framework, focusing on the g ~ \( \overset{\sim }{g} \) -SUGRA scenario where |M3| ≫ |M1|, |M2|. This hierarchy enables a heavier gluino, thereby evading current experimental bounds on supersymmetric particles. Our analysis reveals that precise Higgs measurements place stringent constraints on the model, requiring tan β ≳ 5 and M0 ≳ 20 tan β GeV. Although the g ~ \( \overset{\sim }{g} \) -SUGRA scenario can help reconcile the persistent (g − 2)μ anomaly, the Higgs constraints significantly restrict its parameter space, making a large contribution to (g − 2)μ challenging. We also assess the discovery prospects in upcoming dark matter direct detection experiments, including PandaX-xT (200 t.y.), LZ (projected), and XENONnT (20 t.y.), which may not fully cover the viable parameter space. In contrast, future collider experiments — such as the High-Luminosity LHC at 3 ab1 and CLIC1500 at 2.5 ab1 — can comprehensively probe the remaining regions. These findings highlight g ~ \( \overset{\sim }{g} \) -SUGRA as a promising solution to the CMSSM tension and offer clear, testable predictions for upcoming collider searches.