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  • Effective field theory description of light dilaton
    2026, 50(7): 073112-073112-24. doi: 10.1088/1674-1137/ae6da0
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    Dilatons, the CP-even pseudo-Nambu-Goldstone bosons arising from spontaneous scale symmetry breaking, offer a compelling alternative to axion-like particles (ALPs) yet lack a comprehensive low-energy framework. We address this by constructing a systematic effective field theory (EFT) for the dilaton based on a manifestly scale-invariant regularization scheme. This approach derives universal linear couplings to the trace anomaly while preserving consistent renormalization group evolution. We establish a hierarchical EFT tower connecting the ultraviolet conformal sector to the infrared, encompassing the dilaton-extended SMEFT, low-energy EFT up to dimension-7, and a chiral Lagrangian describing meson and baryon interactions. We perform a comprehensive phenomenological analysis across two distinct mass regimes, where the dilaton manifests as either a conventional particle or a wave-like particle. For MeV-scale dilatons behaving as conventional particles, we obtain constraints from LHC production, semi-invisible B- and K-meson decays, and supernova cooling. For ultralight dilatons acting as dark matter, we project sensitivities for atomic clocks and atom interferometers. This unified EFT framework would pave the way for extended phenomenological studies across the full mass spectrum of the light dilaton.
  • Research on the contribution of s-process to the abundance of 94Mo
    2026, 50(7): 074102-074102-7. doi: 10.1088/1674-1137/ae5ef4
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    This paper addresses a long-standing problem in astrophysics—the origin of the solar system abundance of the proton-rich isotope $ ^{94}\text{Mo} $ by proposing a valuable novel mechanism. The main contribution of this work is that it challenges the traditional view of "$ ^{94}\text{Mo} $ as a pure p-process nuclide". For the first time, it demonstrates that within the s-process environment of low-mass AGB stars, a new s-process path ($ ^{93}\text{Zr} \rightarrow $ $ ^{93}\text{Nb} $ $ \rightarrow ^{94}\text{Nb} \rightarrow ^{94}\text{Mo} $) for producing $ ^{94}\text{Mo} $ can be opened, enabled by the significant enhancement of the effective decay rates of $ ^{93}\text{Zr} $ and $ ^{94}\text{Nb} $ due to the high-temperature astrophysical environment. The results show that this s-process channel can contribute up to a maximum of approximately 10.6% to the solar system abundance of $ ^{94}\text{Mo} $. This work provides a new s-process perspective on the origin of $ ^{94}\text{Mo} $ and has implications for reevaluating the sources of other "shielded" p-nuclei.
  • The medium modification of the charge-weighted Energy-Energy Correlators in Pb+Pb collisions at ${\sqrt{{\boldsymbol s}_{\boldsymbol{NN}}}\bf =5.02}$ TeV
    2026, 50(7): 074103-074103-9. doi: 10.1088/1674-1137/ae62ff
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    We report a systematic study and predictions of medium-induced modifications in charge-dependent jet substructure using the charge-weighted Energy-Energy Correlators (EEC) in 0−10% central Pb+Pb collisions at $ \sqrt{s_{NN}} = 5.02\ {\rm{TeV}} $. Charged-hadron jets, as well as flavor-separated quark- and gluon-initiated jets with momenta of 40−60 GeV and R = 0.4, are analyzed. The ratio of the charge-weighted distribution to the inclusive EEC, which reflects the magnitude of charge correlations, is uniformly negative, demonstrating the dominance of opposite-charge pairs due to charge conservation. A clear flavor dependence is observed: gluon-initiated jets exhibit weaker opposite-charge correlations in the transition and small-RL regions than quark-initiated jets, but stronger opposite-charge correlations at larger RL. In Pb+Pb collisions, the A+A-to-p+p ratio for charge correlations exhibits a universal, flavor-independent pattern: jet quenching enhances opposite-charge correlations at small angles while suppressing them at large angles, leading to a steeper RL dependence of charge correlations in A+A and indicating more rapid decorrelation as RL increases. A distinctive V-shaped modification, together with a plateau-like enhancement, appears in the transition and small-RL regions, independent of jet flavor. By factorizing the EEC into the charged-hadron–pair multiplicity and the average energy-weighting distribution, we identify an enhanced but smeared energy weighting of opposite-charge pairs at small RL as the origin of this modification. These observations indicate that medium-induced broadening of parton-level splittings in the hot, dense medium dissociates the charged di-hadron pairs (such as $ \pi^+\pi^{-} $) present in p+p collisions. The plateau-like enhancement of charge correlations is also found to be unrelated to selection-bias effects.
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