Hunting Exotic Pentaquarks: A Decay Pathway for Hidden Charm
![The strong decay behavior of [latex]\Lambda_{c}\bar{K}^{<i>}[/latex] and [latex]\Sigma_{c}\bar{K}^{</i>}[/latex] molecules proceeds through S-wave interactions, with final states exhibiting negligible branching ratios excluded from analysis.](https://arxiv.org/html/2603.24998v1/x7.png)
Researchers are charting the predicted strong decay patterns of unusual pentaquark particles containing charmed baryons and strange mesons, offering a roadmap for their potential discovery.


![Fading ergodicity emerges within specific parameter regimes in both the Rosenzweig-Porter model-where it is observed for [latex] 1 < \gamma < 2 [/latex]-and the ultrametric model-where it is observed for [latex] 1/\sqrt{2} < \alpha < 1 [/latex]-indicating that, in both systems, the observable relaxation time, or Thouless time [latex] t_{Th} [/latex], consistently falls below the Heisenberg time [latex] t_{H} [/latex].](https://arxiv.org/html/2603.23616v1/fig_DYNAMICS/Fig_sketch.png)

![The shadow cast by a rotating black hole-its shape acutely sensitive to spin-exhibits quantifiable distortions when quantum gravitational parameters are introduced, as demonstrated by the deviation of shadow contours-for spin values of [latex]aM = 0[/latex], [latex]0.8[/latex], and [latex]0.95[/latex]-from those predicted by classical Kerr geometry ([latex]Q_{b}/M^{2} = 0 = Q_{c}/M^{6}[/latex]), revealing the influence of quantum gravity on spacetime geometry itself with parameters [latex]Q_{b}/M^{2} = 0.1 = Q_{c}/M^{6}[/latex] and a black hole mass of [latex]M = 1[/latex] at an inclination angle of [latex]\theta_{0} = \pi/2[/latex].](https://arxiv.org/html/2603.23680v1/x4.png)