Hunting for a Quantum Whirlwind in Heavy-Ion Collisions
![In heavy-ion collisions of lead nuclei at [latex]\sqrt{s_{NN}} = 5.02 \text{TeV}[/latex], the centrality dependence of the correlated two-particle flow coefficient, [latex]f_{CME}[/latex],-extracted via correlations relative to the spectator and participant planes as defined by Eq. 7-reveals a consistent trend across varying degrees of collision centrality, as indicated by the statistical and systematic uncertainties represented by vertical bars and boxes, respectively, and further validated by a constant fit within a 95% confidence level band.](https://arxiv.org/html/2602.22900v1/2602.22900v1/x6.png)
New results from the Large Hadron Collider constrain the search for the chiral magnetic effect-a fleeting quantum phenomenon predicted to arise in the ultra-hot matter created by colliding lead ions.
![The study demonstrates a correlation between the strength parameter α and the dimensionless decay constant [latex]\tilde{\beta}[/latex], with observed minor dependencies on the [latex]M\_B[/latex] mass and a relationship to both the inverse of the initial time [latex]1/\sqrt{t\_0}[/latex] and the Hubble parameter [latex]H[/latex], further influenced by temperature [latex]T[/latex] within the Standard Model’s effective degrees of freedom [latex]g\_{\rm eff,SM}(T)[/latex].](https://arxiv.org/html/2602.23002v1/2602.23002v1/x15.png)
![The study demonstrates a decomposition and weighting of spin-[latex]\frac{1}{2}[/latex] U(1) gauge links interacting with a matter Hamiltonian, revealing the intricate relationships within the system described by the inequality [latex]\tilde{1}[/latex].](https://arxiv.org/html/2602.22332v1/2602.22332v1/x4.png)
![This work establishes upper limits on the kinetic-mixing parameter ε as a function of dark-photon mass [latex]m_{A^{\prime}}[/latex], derived from [latex]B_{x}B_{y}[/latex] and [latex]B_{y}B_{x}[/latex] channels and enhanced through noise subtraction utilizing [latex]B_{z}[/latex] as a coherent reference, demonstrating a sensitivity reaching over [latex]10^{7}[/latex] scanned masses and providing constraints complementary to those from astrophysical observations and existing bounds such as the Coulomb-law limit and projections for future implementations with sensitivities of [latex]0.1\,\mathrm{fT}/\sqrt{\mathrm{Hz}}[/latex].](https://arxiv.org/html/2602.22308v1/2602.22308v1/x2.png)
![The emergence of superconductivity hinges on a delicate balance, where the transition temperature [latex] T_c(p) \sim E_{\rm pair}\rho_0(p) [/latex] peaks near a correlated critical point [latex] p_c [/latex], governed not by complex interactions, but by the finite infrared extent of collective relaxation modes-a principle demonstrated by the linear scaling between transition temperature and superfluid stiffness [latex] T_c \propto \rho_s [/latex] across diverse material families.](https://arxiv.org/html/2602.22626v1/2602.22626v1/x3.png)

![The spatial behavior of correlation functions-specifically [latex]g_{ss^{\prime}}(\delta{\bf r})[/latex] and [latex]g_{nn}(\delta{\bf r})[/latex]-reveals distinct characteristics of translationally and rotationally invariant systems dependent on interaction parameters, exhibiting behavior consistent with either a deep BCS regime ([latex]\ln k_{\rm F}a=2.15[/latex]) or a crossover region ([latex]\ln k_{\rm F}a=0.36[/latex]), as modulated by the level of approximation detailed in Table 1.](https://arxiv.org/html/2602.23019v1/2602.23019v1/x1.png)
![The study demonstrates that highly energetic photons observed by LHAASO can be explained through the mixing of axion-like particles and photons within strong, non-Gaussian magnetic fields, with survival probability [latex]\mathcal{P}\_{\gamma\rightarrow\gamma}[/latex] dependent on parameters κ and [latex]\lambda\_{\rho}[/latex] but independent of axion-like particle mass, suggesting a mechanism where even established theoretical frameworks are vulnerable beyond certain thresholds.](https://arxiv.org/html/2602.23249v1/2602.23249v1/FigNGCase3.png)