PaperPanorama

HEP Phenomenology·hep-ph

Tue·Jun 10, 2025

47 papers34 primary·13 cross-listed·reconstructed*

  1. 01*

    Flavour and cosmological probes of Diracon models

    Salvador Centelles Chuliá🇪🇸 · Tim Herbermann🇩🇪 · Antonio Herrero-Brocal🇪🇸 · Avelino Vicente🇪🇸

    We present and analyze two minimal extensions of the Standard Model featuring a spontaneously broken global, chiral, and anomaly-free symmetry. This breaking generates naturally small Dirac neutrino masses via a seesaw mechanism and yields a physical massless Goldstone boson, the Diracon. Although both models share the same particle content and scalar potential, their distinct symmetry breaking pattern leads to remarkably different phenomenological and cosmological signatures. In the first model, the Diracon couples weakly to charged leptons but right-handed neutrinos can be efficiently produced in the early Universe, resulting in stringent constraints from the effective number of relativistic species, . Conversely, in the second one, right-handed neutrino production is suppressed, and flavour-violating processes such as provide the most promising probes. These simple but elegant models showcase the complementarity between cosmological observations and low-energy flavour experiments in the search for physics beyond the Standard Model.

    hep-phJHEP(2025)·5 citations
  2. 02*

    Universal Mass Equation for Equal-Quantum Excited-States Sets II

    L. David Roper (VTech)🇺🇸 · Igor Strakovsky (GWU)🇺🇸

    We extend our recent study of the universal mass equation for equal-quantum excited-states sets reported by Roper and Strakovsky~\cite{Roper:2024ovj}. The masses of twelve baryon sets and sixteen meson sets, with only two equal-quantum excited states in each set, using Breit-Wigner PDG2024 masses and their uncertainties at fixed for baryons and for mesons, are fitted by a simple one-parameter logarithmic function, , where is the level of radial excitation. Two accurate masses that start a set are used to calculate four higher masses in the set accurately. It is noted that values for equal-quantum excited-states sets accurately lie on a straight line, whose line parameters can be used to calculate and predict higher mass states for sets that have only one known member.

    hep-phhep-exnucl-exnucl-thEPJA(2025)·0 citations
  3. 03*

    Semileptonic decays: hadronic dynamics and the determination of

    J. L. Gutiérrez Santiago🇲🇽 · G. López Castro🇲🇽

    The four-body decays () and () are studied in a model where the momentum-dependence of the hadronic matrix elements are described in terms of and pole contributions. From fits to the recent data of the BESIII collaboration we find that the -pole can mimic the effect of the -wave contribution of the system to the branching fraction. Implications for the determination of the quark mixing matrix element are discussed.

    hep-phEPJC(2026)·1 citation
  4. 04*

    Understanding the medium-like effects in the jet-like yield in pp and p-Pb collisions using event generators

    Dushmanta Sahu🇲🇽 · Antonio Ortiz🇲🇽 · Victor Campos🇲🇽

    To understand the dynamics of jet-medium interaction in small systems such as proton-proton (pp) and proton-lead (p-Pb) collisions at = 5.02 TeV, particle production is studied in three distinct topological regions defined with respect to the charged particle with the highest transverse momentum in the event (). The jet-like yield is defined by the particle density in the toward region () after subtracting that in the transverse region (). The activity on the transverse side is used as a proxy for medium-like effects. Three different Monte Carlo event generators -- \textsc{Pythia8}, a multiphase transport (AMPT) model, and EPOS4 -- are employed to investigate particle yields as a function of in the interval 0.5-20\,GeV/. Calculations are performed for the threshold of 0.5 GeV/ at mid-rapidity (). The jet-like yield in the toward region for pp collisions show interesting dynamics; they are significantly affected by the medium-like effects in the low to intermediate (\,GeV/) which is studied through color reconnection and hydrodynamics in \textsc{Pythia8} and EPOS4, respectively. However, the results from AMPT show that the jet-like yield is medium-like modified throughout the entire range. The jet-like yield in p-Pb collisions using AMPT is also studied. Notably, a dip structure that is observed in the jet-like signal ratio of pp to p-Pb at low in ALICE data, is reproduced by AMPT model with string melting on, pointing to possible medium-like behavior in small systems. The results of this article also underscore the importance of high- ( 8 GeV/) for minimizing underlying event biases in jet-related studies.

    hep-phJ.Phys.G(2025)·1 citation
  5. 05*

    Investigating the most active pp collisions (top 0.1%) using the tools developed by experiments at the LHC

    Jesús Eduardo Muñoz Méndez🇲🇽 · Antonio Ortiz🇲🇽

    The LHC data have unveiled unexpected features in proton-proton (pp) collisions, namely, collective-like behavior and strangeness enhancement. Originally, these new effects were discovered only in high-multiplicity pp collisions. However, recently the ALICE Collaboration has shown that even low-multiplicity pp collisions yield a non-zero elliptic flow (). Moreover, analyses as functions of the event structure, such as transverse spherocity, suggest that multiplicity might not be the main driver of the new effects. Therefore, new ways of analyzing the data have to be explored in order to understand the origin of the new phenomena. In this paper, pp collisions simulated with PYTHIA 8 are analyzed using different event estimators (mid-pseudorapidity multiplicity, spherocity, sphericity, , forward multiplicity and flattenicity). The features of the selected events for the top 0.1% using the different estimators are discussed. The transverse momentum spectrum of primary particles and the recoil jet distributions are analyzed. The results suggest that flattenicity is the estimator with the least bias on the neutral-to-charged particle ratio, and on the bias towards harder-than-average pp collisions.

    hep-phJ.Phys.G(2025)·4 citations
  6. 06*

    Spectroscopy and Decay Properties of Excited Charmonium States

    Zi-Yue Cui🇨🇳 · Hao Chen🇨🇳 · Cheng-Qun Pang🇨🇳 · Zhi-Feng Sun🇨🇳

    In this work, we investigate the mass spectra of excited charmonia employing a nonrelativistic potential model with screening effect, and analyze their two-body strong decay, two-photon decay, leptonic decay, and hadronic transitions. Especially, we find that the newly observed resonances , , and can be identified as , , and states, respectively. We also predict the masses and the widths of higher excited states in the charmonia family.

    hep-phhep-exPRD(2025)·1 citation
  7. 07*

    Composite Hybrid Inflation : Primordial Black Holes and Stochastic Gravitational Waves

    Giacomo Cacciapaglia🇫🇷 · Dhong Yeon Cheong🇰🇷 · Aldo Deandrea🇫🇷 · Wanda Isnard🇫🇷 · Seong Chan Park🇰🇷 · Xinpeng Wang🇨🇳 · Ying-li Zhang🇯🇵

    We investigate the production of primordial black holes and gravitational waves in composite hybrid inflation. Starting from an effective chiral Lagrangian with a dilaton and pions, we identify inflation occurring due to the walking dynamics of the theory. A symmetry-breaking term in the pion sector induces a shift in the inflaton's trajectory, which leads to a tachyonic instability phase. Curvature perturbations grow exponentially, producing copious primordial black holes and a stochastic gravitational wave background. We show that the primordial black hole mass and the gravitational wave frequency are strongly restricted by the anomalous dimensions of the pion operators, with larger anomalous dimensions giving lighter primordial black holes and higher frequency gravitational waves. In both cases, the associated signatures lie within reach of future gravitational wave observatories.

    hep-phastro-ph.COJCAP(2026)·8 citations
  8. 08*

    production in the decays process

    Zhuo Yu🇨🇳 · Qi Wu🇨🇳 · Dian-Yong Chen🇨🇳

    In the present work, we studied the exotic state production in the meson decays through the meson loop mechanism, where the meson decays into an anti-charmed meson and a charmed-strange meson pair, and consequently couples to and a light meson (, and ) via exchanging a proper charmed or charmed-strange meson. Using the effective Lagrangian approach, we estimated the branching fractions of different channels find them to be on the order of and their ratios are almost independent of the model parameter. The fit fractions of in different decay processes are also estimated, and we propose searching for in the process, which should be accessible to both Belle II and LHCb Collaborations.

    hep-phPRD(2025)·2 citations
  9. 09*

    New Types of Hydrogenlike matter Composed of Electron(s) and Meson(s)

    Jun-Feng Wang🇨🇳 · Zi-Yue Cui🇨🇳 · Cheng-Qun Pang🇨🇳 · Zhi-Feng Sun🇨🇳

    In the present work, we predict the existence of new types of hydrogenlike matter, including hydrogenlike atoms (, , ), hydrogenlike molecular ions (, , ) and hydrogenlike molecules (, , ). By solving the Schrödinger equation, the binding energy of hydrogenlike atoms is obtained as . For hydrogenlike molecular ions and molecules, the variational method is employed to calculate the binding energies, i.e., and for hydrogenlike molecular ions and molecules, respectively. And the bond lengths for hydrogenlike molecular ions and molecules are also calculated, whose values are and , respectively. Here all the quantities are in atomic units for convenience. In addition, the strong interaction between the two constituent mesons is considered in our calculations, where we find that its influence on the hydrogenlike molecular ions and molecules can be neglected. Comparisons of hydrogenlike molecular ion and molecule with the systems governed by the strong interaction are made, which suggests the possible existence of doubly heavy triquark, hidden heavy-flavor tetraquarks and doubly heavy tetraquarks. Hopefully, these types of matter would be observed in the future with the improvement of accuracy in the high energy physical experiments.

    hep-phhep-exnucl-exnucl-thFew Body Syst.(2026)·0 citations
  10. 10*

    Dense matter in a holographic hard-wall model of QCD

    Daisuke Fujii🇯🇵 · Atsushi Hosaka🇯🇵 · Akihiro Iwanaka🇯🇵 · Tadakatsu Sakai🇯🇵 · Motoi Tachibana🇯🇵

    A deeper understanding of QCD matter at strong coupling remains challenging due to its non-perturbative nature. To this end, we study a two-flavor holographic hard-wall model to investigate the properties of QCD at finite-density and zero temperature with a nonvanishing quark mass. A dense matter phase is described by a classical solution of the equations of motion in a homogeneous Ansatz. We apply holographic renormalization to formulate the holographic dictionary that relates UV boundary data in the bulk with the physical quantities in QCD. We emphasize a role played by an IR boundary action on the hard-wall when analyzing the QCD phase structures in this holographic setup. It is found that a baryonic matter phase is manifested in this model with a high baryon number density and a nearly vanishing chiral condensate. We derive the equation of state for the resulting phase and use it to work out the mass-radius relation for neutron stars. We find that the maximum mass of neutron stars can exceed two solar masses for a wide range of free parameters in this model. We also comment on an alternative scenario about the phase structure such that the baryonic matter phase arises at a baryon number chemical potential greater than a critical value.

    hep-phhep-thnucl-thPRD(2026)·3 citations
  11. 11*

    Indirect Detection of Dark Matter Around a Supermassive Black Hole with High Energy-Resolution Gamma-Ray Telescopes

    Yu Watanabe🇯🇵 · Alexander Kusenko🇺🇸 · Shigeki Matsumoto🇯🇵

    We explore whether the unprecedented energy resolution of upcoming gamma-ray telescopes can uncover relativistic effects in photon spectra resulting from dark matter (DM) annihilation or decay near the supermassive black hole (SMBH) at the Galactic Center (GC), specifically, gravitational redshift, Doppler broadening due to Lorentz boosts, and kinetic energy enhancements arising from high DM velocities. By modeling DM density and velocity profiles under various SMBH formation scenarios and DM properties, we calculate the corresponding gamma-ray spectra and identify the conditions under which SMBH-induced spectral distortions become observable. We find that, in favorable cases, the observed spectra encode the DM velocity distribution near the SMBH, enabling potential discrimination among annihilation mechanisms with different velocity dependencies. Even when SMBH-induced effects are modest, the upcoming COSI mission, with sub-percent energy resolution surpassing the typical DM velocity dispersion at the GC, , may still be able to detect subtle Doppler broadening. These results highlight a promising pathway for determining the origin of gamma-ray signals and probing DM properties through high-resolution spectral measurements.

    hep-phJHEP(2026)·3 citations
  12. 12*

    Decays and in the chiral quark NJL model

    M.K. Volkov🇷🇺 · A.A. Pivovarov🇷🇺 · K. Nurlan🇷🇺

    The branching fractions of the axial vector meson decays , and are calculated in the standard quark NJL model. The intermediate channels with the states and are taken into account in the decay . In the case of the scalar mesons, the representation as a chiral symmetric partners of the pseudoscalar mesons is used. It is shown that the decays and occur due to the mass difference of the and quarks. All the results are obtained without using any additional arbitrary parameters and are in satisfactory agreement with the known experimental data.

    hep-ph0 citations
  13. 13*

    Open-Flavor Heavy Hadron Production in Heavy-Ion Collisions

    C.E. Fontoura🇧🇷 · G. Krein🇧🇷 · A. Valcarce🇪🇸 · J. Vijande🇪🇸

    We study the production of open-flavor heavy hadrons in relativistic heavy-ion collisions. The hadronization in the quark-gluon plasma is described in the quark coalescence model. We evaluated yields and transverse momentum distributions. A simultaneous study of conventional and exotic hadrons is carried out. The Wigner functions are evaluated using hadron wave functions obtained from a single realistic quark model. Thus, results are presented in a single framework for the production of open-flavor heavy mesons, baryons, and exotic tetraquarks, in particular: , , , , , , and ( or ). The consequences of a partial restoration of chiral symmetry at the hadronization temperature are studied in detail.

    hep-phPRD(2025)·2 citations
  14. 14*

    Squeezing effect on three-dimensional Hanbury Brown-Twiss radii

    Yong Zhang🇨🇳 · Peng Ru🇨🇳

    This paper examines the impacts of the squeezing effect caused by the particle's in-medium mass modification on the three-dimensional Hanbury Brown-Twiss (HBT) radii. An analysis is conducted on how the squeezing effect impacts the three-dimensional HBT radii of , , and . The squeezing effect suppresses the impacts of transverse flow on the transverse source distribution and broadens the space-time rapidity distribution of the particle-emitting source, leading to an increase in the HBT radii, notably in out and longitudinal direction. This phenomenon becomes more significant for higher transverse pair momentum, resulting in a non-monotonic decrease in the HBT radii with increasing transverse pair momentum. The impact of the squeezing effect on the HBT radii is more pronounced for than for . Furthermore, this effect is also more significant for than for . The findings presented in this paper could offer fresh perspectives on investigating the squeezing effect.

    hep-phnucl-thCPC(2025)·0 citations
  15. 15*

    Gravitational Wave Signals in a Promising Realization of SO(10) Unification

    Injun Jeong (1 and 2)🇰🇷 · Jörn Kersten (3 and 4)🇳🇴 · Stefano Scopel (1 and 2)🇰🇷 · Liliana Velasco-Sevilla (1 and 2) ((1) Center for Quantum Spacetime, Sogang University, (2) Department of Physics, Sogang University, (3) Department of Physics and Technology, University of Bergen, (4) Department of Physics and IPAP, Yonsei University)🇰🇷

    We investigate gravitational wave signals in a non-supersymmetric grand unified model where the group is broken in two steps to the Standard Model gauge group. We calculate the analytical form of the one-loop effective potential responsible for the first step of symmetry breaking and show that it can lead to a first-order phase transition with gravitational wave production. We also determine the gravitational wave background produced by the primordial plasma of relativistic particles. The present experimental sensitivity is still far from the expected signals, but could be in reach of novel detector concepts.

    hep-phgr-qcPRD(2026)·1 citation
  16. 16*

    violation in two-body hadronic decays in the PQCD approach

    Jia-Jie Han🇨🇳 · Ji-Xin Yu🇨🇳 · Ya Li🇨🇳 · Hsiang-nan Li🇹🇼 · Jian-Peng Wang🇨🇳 · Zhen-Jun Xiao🇨🇳 · Fu-Sheng Yu

    We systematically investigate the -averaged branching ratios and violations (CPVs) for the two-body hadronic decays , where runs through the mesons , , , , , and , in the perturbative QCD approach to order in the strong coupling. Various topological amplitudes are obtained by incorporating subleading-twist hadron distribution amplitudes, which exhibit reasonable hierarchical patterns, sizable strong phases, and non-negligible higher-power corrections. The predicted direct CPVs in , different from those in similar meson decays, are as small as the current data. The low CPV in results from the cancellation between the - and -wave CPVs, while the one in is determined by the tiny -wave CPV. However, individual partial-wave CPVs can exceed , consistent with direct CPVs in meson decays. The CPVs in the channels are relatively larger. In particular, CPVs above appear in the up-down asymmetries associated with the final-state angular distributions of , followed by the secondary decays. These observables offer promising prospects for firmly establishing baryon CPVs. The decay asymmetry parameters of are also predicted for future experimental confrontations.

    hep-phhep-exPRD(2025)·14 citations
  17. 17*

    Towards numerical two-loop integrand reduction

    Giuseppe Bevilacqua🇬🇷 · Dhimiter Canko🇮🇹 · Costas Papadopoulos🇬🇷 · Aris Spourdalakis🇬🇷

    We present a method for the integrand-level reduction of two-loop helicity amplitudes in both and dimensions. The amplitude is expressed in terms of a set of Feynman integrals and their coefficients that depend on the external kinematics. The analysis presented in this paper, in conjunction with the ongoing development of the computational framework , paves the road for the construction of an automated program for two-loop amplitude calculations for arbitrary scattering processes.

    hep-phhep-thJHEP(2025)·3 citations
  18. 18*

    Propagation and Dynamics of Oscillating Tetraquark Systems

    Sh. Janjan🇮🇷 · G.R.Boroun🇮🇷

    We have presented a theoretical investigation into the behavior of tetraquark states. These states are modeled as a non-relativistic four-body quantum system governed by harmonic interactions. Our goal is to capture the fundamental dynamics of quark-antiquark interactions in the tetraquark configuration. Within this framework, we have derived an analytical expression for the quantum propagator. This expression was then used to compute the time evolution of the wave function and the associated probability density. We examined the time evolution and oscillation patterns to gain a better understanding of the wave function and its probability of presence in space. This approach offers valuable insights into the dynamics of the tetraquark system. This model can serve as a basis for predicting complex structures such as entanglement and multipartite dependence of quarks.

    hep-ph0 citations
  19. 19*

    Tracing the Evolution of Nuclear Excitation at the Electron-Ion Collider

    Niseem Magdy🇺🇸

    We investigate the evolution of nuclear excitation in electron-nucleus (e+A) collisions at the upcoming Electron-Ion Collider (EIC) using the BeAGLE event generator. Leveraging the EIC's unique collider kinematics, we demonstrate the remarkable capability to separate distinct nuclear reaction stages, hard scattering, intranuclear cascade, and nuclear de-excitation, in the laboratory frame. Our systematic analysis reveals that event-by-event fluctuations in the mean transverse momentum (k) are highly sensitive to the intranuclear cascade formation time and nuclear geometry, while minimally affected by variations in electron beam energy. These findings establish k as a robust observable for constraining nuclear excitation mechanisms, providing critical benchmarks for future EIC experiments and guiding theoretical advancements in nuclear transport modeling.

    hep-phnucl-exnucl-thPRC(2026)·1 citation
  20. 20*

    Three-loop QCD Mass Relation between the and Symmetric-momentum Subtraction Scheme Away from the Chiral Limit

    Long Chen🇨🇳 · Marco Niggetiedt🇩🇪

    The perturbative result for the quark-mass conversion factor between the and regularization-independent symmetric-momentum subtraction scheme (RI/SMOM) away from the chiral limit, i.e. at non-zero quark masses (RI/mSMOM), is derived up to three loops in QCD, extending the existing result by two additional orders. We further explore an illuminating possibility that in Dimensional Regularization, the original RI/(m)SMOM renormalization conditions may be interpreted merely in a weaker sense, namely as equations holding just in the 4-dimensional limit rather than exactly in dimensions: they result in different, albeit simpler, renormalization constants but still the same finite conversion factor. This novel observation has the added benefit of reducing computational effort, particularly at high orders. Our high-order results for the conversion factor exhibit rich behaviors, and in particular a window is observed in the subtraction scale and mass where it receives less perturbative corrections than the RI/SMOM counterpart up to three loops; this finding may help to further improve the accuracy of quark-mass determinations with Lattice QCD.

    hep-phhep-lathep-thPLB(2025)·2 citations
  21. 21*

    First Constraint on Axion-Photon Coupling from Neutron Star Observations

    Jun-Chen Wang🇨🇳 · Shunshun Cao🇨🇳 · Jinchen Jiang🇩🇪 · Yandong Liu🇨🇳 · Qing-Hong Cao🇨🇳 · Lijing Shao🇨🇳

    We propose a novel method to detect axions which uniquely depends on the dimensionless axion-photon coupling , independent of the suppressive axion decay constant . Using neutron star PSR B1919+21 data from the Five-hundred-meter Aperture Spherical Telescope, we derive the first constraint at confidence level for ultra-light axions ( eV).

    hep-phastro-ph.HE0 citations
  22. 22*

    Proton Gravitational Structure and Mass Decomposition on the Light Front

    Sreeraj Nair🇨🇳 · Chandan Mondal🇨🇳 · Siqi Xu🇨🇳 · Xingbo Zhao🇨🇳 · James P. Vary🇺🇸

    Gravitational form factors (GFFs) of hadrons encode essential information about the internal distributions of mass, spin, pressure, and shear among their quark and gluon constituents. We compute the quark and gluon GFFs of the proton using a fully relativistic, nonperturbative framework based on a light-front quantized Hamiltonian with quantum chromodynamics (QCD) input. This allows us to quantify the impact of a dynamical gluon on the proton's mechanical properties, such as pressure and shear distributions. Our predictions agree well with recent lattice QCD results and experimental extractions. We also determine the proton's mass and mechanical radii and address the long-standing puzzle of its mass decomposition. At the scale , we find that quark energy, gluon field energy, the quark condensate, and the QCD trace anomaly contribute , , , and , respectively, which are consistent with lattice QCD findings.

    hep-phPRD(2025)·14 citations
  23. 24*

    Probing Planck scale effects on absolute mass limit in neutrino flavor evolution

    Kartik Joshi🇮🇳 · Sanjib Dey🇮🇳 · Satyajit Jena🇮🇳

    This work explores how the generalized uncertainty principle, a theoretical modification of the Heisenberg uncertainty principle inspired by quantum gravity, affects neutrino flavor oscillations. By extending the standard two-flavor neutrino model, we show that the oscillation probability acquires an additional phase term that depends on the {square roots of the individual neutrino masses}, introducing new features beyond the conventional mass-squared differences. To account for the non-Hermitian nature of the resulting dynamics, we employ parity-time () symmetric quantum mechanics, which allows for consistent descriptions of systems with {balanced gain and loss mechanisms}. We analyze the feasibility of observing these effects in current and future neutrino experiments, such as DUNE, JUNO, IceCube, ORCA--KM3NeT, MINOS, Daya Bay, Hyper-Kamiokande, and KATRIN, and find that the predicted modifications could fall within the sensitivity of current experiments. Moreover, we propose that analog quantum simulation platforms, such as cold atoms, trapped ions, and photonic systems, offer a promising route to test these predictions under controlled conditions. Our findings suggest that neutrino oscillations may serve as an effective probe of quantum gravity effects, providing a novel connection between fundamental theory and experimental observables.

    hep-phhep-thNPB(2025)·1 citation
  24. 25*

    Thermal corrections to dark matter annihilation with real photon emission/absorption

    Prabhat Butola (IMSc, HBNI)🇮🇳 · D. Indumathi (IMSc, HBNI)🇮🇳 · Pritam Sen (TIFR)🇮🇳

    The dark matter relic density is being increasingly precisely measured. This relic density is theoretically determined by a Boltzmann equation which computes the dark matter distribution according to the (thermally averaged) cross section for annihilation/production of dark matter within a given model. We present here the complete higher order thermal corrections, calculated using real time thermal field theory, to the cross section for the annihilation of dark matter into Standard Model fermions via charged scalars: and . The latter process includes real photon emission into, and absorption from, the heat bath at temperature . We use the Grammer and Yennie technique to separate the soft infra-red divergences, which greatly simplifies the calculation. We show explicitly the cancellation of both soft and collinear divergences between real and virtual contributions at next-to-leading order (NLO) in the thermal field theory and remark on the non-trivial nature of the collinear divergences when the thermal contribution from fermions is considered. We present the leading thermal contributions to order for the case when the dark matter particle is a Majorana or Dirac type fermion. In the former case, both the leading order (LO) and NLO cross sections are helicity suppressed, while neither is suppressed in the Dirac case. It is interesting that the ratio of NLO to LO cross sections is the same for both Majorana and Dirac type dark matter.

    hep-phhep-th1 citation
  25. 26*

    Determining from the Heavy Jet Mass distribution

    Miguel A. Benitez🇪🇸

    We present a state-of-the-art analysis on determining the strong coupling constant from available data for the Heavy Jet Mass (HJM) distribution. Dijet resummation is supplemented with additional resummation of shoulder logarithms appearing around the symmetric 3-jet configuration of the HJM spectrum. In addition to we further obtain numerical results for two non-perturbative parameters, and , encompassing effects from dijet and trijet hadronization effects, respectively.

    hep-ph1 citation
  26. 27*

    Torsion Balance Experiments Enable Direct Detection of Sub-eV Dark Matter

    Shigeki Matsumoto🇯🇵 · Jie Sheng🇨🇳 · Chuan-Yang Xing🇨🇳 · Lin Zhu🇨🇳

    Light dark matter with sub-eV masses has a high number density in our galaxy, and its scattering cross section with macroscopic objects can be significantly enhanced by coherence effects. Repeated scattering with a target object can induce a measurable acceleration. Torsion balance experiments with geometric asymmetry are, in principle, capable of detecting such signals. Our analysis shows that existing torsion balances designed to test the Equivalence Principle already place the most stringent constraints on DM-nucleon scattering in the eV mass range.

    hep-phhep-exPRL(2026)·4 citations
  27. 28*

    Level order of quark systems: The puzzle of the Roper resonance, and related questions

    Jean-Marc Richard🇫🇷

    The problem of ordering of radial vs.\ orbital excitations is reviewed. It is shown that the current quark models cannot explain the location of the Roper resonance which is slightly lower than the lowest negative-parity excitations. We also study some related spectral problems, such as the dependence of the energies on the quark masses, and the possibility of bound states in simple chromelectric models.

    hep-phnucl-thActa Phys.Polon.B(2026)·1 citation
  28. 29*

    Radially Excited Bottom Mesons in Heavy Quark Effective Theory

    Ritu Garg · Preeti Bhall · K.K Vishwakarma

    In this paper, Heavy Quark Effective Theory (HQET) is employed to investigate experimentally missing radially excited bottom-meson states. It is an extension of our previous work, in which we had applied HQET for the calculation of charm mesons. By incorporating both theoretical insights and available experimental data on charmed mesons with flavor-symmetry parameters, we computed masses of radially excited bottom-meson states with their strange partners. In addition, decay widths are calculated in the form of hadronic coupling constants , , . By comparing our decay width predictions with available total decay widths, we calculated upper bounds on the corresponding couplings. Regge trajectories are also constructed for our predicted data in planes (, ) and (, ), and estimate higher masses () by fixing Regge slopes and intercepts. Future experimental findings can validate the results obtained in this work.

    hep-phPTEP(2025)·0 citations
  29. 30*

    Towards AI-assisted Neutrino Flavor Theory Design

    Jason Benjamin Baretz🇺🇸 · Max Fieg🇺🇸 · Vijay Ganesh🇺🇸 · Aishik Ghosh🇺🇸 · V. Knapp-Perez🇺🇸 · Jake Rudolph🇺🇸 · Daniel Whiteson🇺🇸

    Particle physics theories, such as those which explain neutrino flavor mixing, arise from a vast landscape of model-building possibilities. A model's construction typically relies on the intuition of theorists. It also requires considerable effort to identify appropriate symmetry groups, assign field representations, and extract predictions for comparison with experimental data. We develop an Autonomous Model Builder (AMBer), a framework in which a reinforcement learning agent interacts with a streamlined physics software pipeline to search these spaces efficiently. AMBer selects symmetry groups, particle content, and group representation assignments to construct viable models while minimizing the number of free parameters introduced. We validate our approach in well-studied regions of theory space and extend the exploration to a novel, previously unexamined symmetry group. While demonstrated in the context of neutrino flavor theories, this approach of reinforcement learning with physics software feedback may be extended to other theoretical model-building problems in the future.

    hep-phcs.LGphysics.comp-phstat.MLCommun.Phys.(2026)·8 citations
  30. 31*

    Discovering the Higgsino at CTAO-North within the Decade

    Shotaro Abe🇯🇵 · Tomohiro Inada🇯🇵 · Emmanuel Moulin🇫🇷 · Nicholas L. Rodd🇺🇸 · Benjamin R. Safdi🇺🇸 · Weishuang Linda Xu🇺🇸

    We demonstrate that higgsino dark matter (DM) could be discovered within the next few years using the Cherenkov Telescope Array Observatory's soon-to-be-operational northern site (CTAO-North). A 1.1 TeV thermal higgsino is a highly motivated yet untested model of DM. Despite its strong theoretical motivation in supersymmetry and beyond, the higgsino is notoriously difficult to detect; it lies deep within the neutrino fog of direct detection experiments and could pose a challenge even for a future muon collider. We show that, in contrast, higgsino detection could be possible within this decade with CTAO-North in La Palma, Spain. The Galactic Center is the region where the dominant DM annihilation signature emerges, but it only barely rises above the horizon at the CTAO-North site. However, we project that this challenge can be overcome with large-zenith-angle observations at the northern site, enabling the conclusive detection of a higgsino signal by 2030 for a range of DM density profiles in the inner Galaxy.

    hep-phastro-ph.COastro-ph.HEPRD(2026)·17 citations
  31. 32*

    Impostor Among s: Dark Radiation Masquerading as Self-Interacting Neutrinos

    Anirban Das🇮🇳 · P. S. Bhupal Dev🇺🇸 · Christina Gao🇨🇳 · Subhajit Ghosh🇺🇸 · Taegyun Kim🇰🇷

    Multiple cosmological observations hint at neutrino self-interactions beyond the Standard Model, yet such interactions face severe constraints from terrestrial experiments. We resolve this tension by introducing a model where active neutrinos resonantly convert to self-interacting dark radiation after BBN but before CMB epoch. This exploits the fact that cosmological observables cannot distinguish between neutrinos and dark radiation with the same abundance and free-streaming properties. Our mechanism, based on a simple type-I seesaw framework along with a keV-scale scalar mediator, achieves two objectives: (i) it produces strongly self-interacting dark radiation that imitates neutrino self-interactions favored by cosmological data, and (ii) it depletes the active neutrino energy density, relaxing cosmological neutrino mass bounds and easing the tension with neutrino oscillation data. The model naturally evades laboratory constraints through suppression of the neutrino-mediator coupling by the squared mass ratio of active and sterile neutrinos. We show that this scenario is favored over CDM by the combined Planck and DESI data, while being consistent with all other constraints. Our mechanism is testable in future laboratory probes of absolute neutrino mass and searches for sterile neutrinos.

    hep-phastro-ph.COPRL(2026)·19 citations
  32. 33*

    Time-Dependent Precision Measurement of Decay at FCC-

    Tsz Hong Kwok🇨🇭 · Zachary Polonsky🇨🇭 · Valeriia Lukashenko🇨🇭 · Jason Aebischer🇨🇭 · Ben Kilminster🇨🇭

    We study the feasibility of measuring time-dependent violation in the rare flavor-changing neutral current (FCNC) decay at the FCC-. In the Standard Model (SM), violation in this mode arises only at higher orders and is highly suppressed. Extensions of the SM, collectively referred to as New Physics (NP), can introduce additional -violating phases that enhance such effects. The decay , mediated by the transition, is therefore a promising probe of NP. The FCC-, operating as a high-luminosity -factory, offers an optimal environment for this measurement due to its large event yield, clean conditions, efficient particle identification, and excellent vertex resolution. We perform a Monte Carlo study using Pythia and Delphes with the IDEA detector concept. A relative precision better than on the branching ratio and on the time-integrated asymmetry is found to be achievable. We determine the projected sensitivities to the observables , , and , which parameterize time-dependent violation. In the untagged analysis, a precision of on can be reached. With flavor tagging, sensitivities to and improve to . These measurements remain inaccessible to current flavor experiments. Interpreting the results within the Weak Effective Theory provides model-independent constraints on -violating NP. This study demonstrates that FCC- enables first-time access to -sensitive observables previously beyond experimental reach.

    hep-phhep-exEPJC(2026)·6 citations
  33. 34*

    Nucleon Decays into Light New Particles in Neutrino Detectors

    Julian Heeck🇺🇸 · Ian M. Shoemaker🇺🇸

    Proton and neutron decays into light new particles can drastically change the experimental signatures and benefit from the complementarity of large water-Cherenkov neutrino detectors such as Super/Hyper-Kamiokande and tracking detectors such as JUNO and DUNE. The proton decays and with near phase-space closure lead to charged particles below Cherenkov threshold, rendering them practically invisible in Super- and Hyper-Kamiokande but not in JUNO and DUNE, which are therefore uniquely positioned for these baryon-number-violating signatures despite their smaller size. As an additional signature, such nucleon decays in Earth can produce a sizable flux of particles in underground detectors. We present a simple model in which nucleons decay into sub-GeV sterile neutrinos that subsequently decay through active-sterile neutrino mixing, with a promisingly large number of events in Super-Kamiokande even in the seesaw-motivated parameter space.

    hep-phhep-exPRL(2025)·10 citations
  34. 35*

    Perturbative QCD reveals the softening of matter in the cores of massive neutron stars

    Oleg Komoltsev🇳🇴

    The cores of neutron stars (NSs) contain the densest matter in the universe. Rapid advancements in neutron-star observations allow unprecedented empirical access to cold, ultra-dense Quantum Chromodynamics (QCD) matter. The combination of these observations with theoretical calculations has revealed previously inaccessible features of the equation of state (EoS) and the QCD phase diagram. In this thesis, I demonstrate how perturbative-QCD calculations at asymptotically high baryon densities provide robust constraints on the EoS at neutron-star densities. The method for constraint propagation is based solely on thermodynamical causality, stability, and consistency of the EoS. By constructing a large ensemble of EoSs using Gaussian processes regression and incorporating it into a Bayesian inference of EoS, I demonstrate that the novel pQCD constraints go beyond those obtained from current astrophysical observations alone, forcing the EoS to soften at the maximum densities of stable neutron stars. This softening of the EoS can be interpreted as an indication of approximate conformal symmetry restoration, a sign of a first-order phase transition (FOPT), or potentially both. I show that the conformal symmetry restoration is consistent with the hypothesis of quark matter cores inside the most massive NSs. Although current astrophysical data and theoretical inputs cannot definitively distinguish between the two scenarios, they slightly favor the occurrence of a phase transition of some kind - whether a crossover to quark matter or a destabilizing FOPT - in the cores of the most massive neutron stars.

    astro-ph.HEhep-phnucl-th2 citations
  35. 36*

    The -Attractor E-Model in Warm Inflation: Observational Viability from Planck 2018

    Bhargabi Saha🇮🇳 · Malay K. Nandy🇮🇳

    We explore the inflationary evolution and observational viability of the -attractor E-model in the framework of warm inflation, focusing on both weak and strong dissipative regimes, with a dissipation coefficient linear in temperature. In the strong regime, we account for the growth of inflaton fluctuations due to coupling with the radiation bath via two different forms for the dissipation enhancement function: one associated with plateau-like potentials, and another motivated by the warm little inflation scenario. Employing slow roll conditions, we analytically derive the expressions for the key inflationary observables, the spectral index and the tensor-to-scalar ratio , in both dissipative regimes. The resulting theoretical trajectories on the -- plane are then juxtaposed with the contour plots obtained from Planck 2018 data in order to constrain the model parameter. Our analysis shows that the warm -attractor E-model remains compatible with observations in both dissipative regimes, with dissipation playing a crucial role in shifting the predictions and enlarging the viable parameter space, highlighting observational robustness of the model when extended to warm inflation.

    astro-ph.COgr-qchep-phJCAP(2025)·3 citations
  36. 37*

    Primordial black holes save inflation

    Xinpeng Wang🇨🇳 · Kazunori Kohri🇯🇵 · Tsutomu T. Yanagida🇯🇵

    In light of the latest Planck and Atacama Cosmology Telescope (P-ACT) joint results on the primordial scalar power spectrum, we show that the inflation model extended with a non-minimally coupled scalar field --namely the -extended inflation model--can naturally accommodate a larger spectral index and a small positive running at cosmic microwave background (CMB) scales, both of which are consistent with the latest P-ACT constraints. This is because the field contributes a blue-tilted component to the primordial power spectrum, which both modifies the large-scale power and, as a result, significantly enhances power on small scales. The deviation of the and from the single field inflation is related to the non-minimal coupling constant . The consequent enhancement in the primordial power spectrum can be large enough to lead to the formation of primordial black holes (PBHs) of mass as dark matter candidates. Furthermore, future observations of the small-scale power spectrum, CMB spectral distortions, and stochastic gravitational waves will provide decisive tests of this model and its predictions for PBHs. We stress its strong connection to the seesaw mechanism for the generation of the observed small masses.

    astro-ph.COgr-qchep-phJCAP(2026)·25 citations
  37. 38*

    Supersymmetry searches at ATLAS and CMS

    Hyejin Kwon (on behalf of the ATLAS and CMS Collaborations)🇧🇪

    This document presents recent results from the ATLAS and CMS experiments at the CERN Large Hadron Collider (LHC) on supersymmetry (SUSY) searches. These searches provide results with some non-conventional SUSY search assumptions such as with compressed mass scenario or with long-lived particle scenario. Some of the recent results covers the unexplored SUSY phase space from prior results, brings a new insight to the SUSY landscape. Sensitivity on SUSY upper limits are enhanced with newly added LHC data, enhanced trigger algorithm or advanced event selection with machine learning (ML).

    hep-exhep-ph2 citations
  38. 39*

    Unveiling the role of vector potential in the Aharonov-Bohm effect

    Masashi Wakamatsu🇯🇵

    The most popular interpretation of the Aharonov-Bohm (AB) effect is that the electromagnetic potential locally affects the complex phase of a charged particle's wave function in the magnetic field free region. However, since the vector potential is a gauge-variant quantity, not a few researchers suspect that it is just a convenient tool for calculating the force field. This motivates them to explain the AB effect without using the vector potential, which inevitably leads to some sort of non-locality. This frustrating situation is shortly summarized by the statement of Aharonov et al. that the AB effect may be due to a local gauge potential or due to non-local gauge-invariant fields. In the present paper, we shall give several convincing arguments, which support the viewpoint that the vector potential is not just a convenient mathematical tool with little physical entity. Despite its gauge arbitrariness, the vector potential certainly contains a gauge-invariant piece, which solely explains the observed AB phase shift. Importantly, this component has a property such that it is basically unique and cannot be eliminated by any regular gauge transformations. To make the discussion complete, we also discuss the role of remaining gauge arbitrariness still contained in the entire vector potential.

    quant-phhep-phnucl-thphysics.ed-phSymmetry(2025)·0 citations
  39. 40*

    What is the Quark-Gluon Plasma made of?

    Berndt Müller🇺🇸

    This article surveys our present understanding of the internal structure of the fully developed quark-gluon plasma at temperatures outside the crossover region. The theoretical part of the review covers perturbative and nonperturbative approaches to quark-gluon plasma structure, in particular, hard-thermal loop effective theory, lattice QCD and the functional renormalization group. The phenomenological part of the review scrutinizes the information that has been derived from bulk observables and hard probes in relativistic heavy ion collisions in terms of how it informs our knowledge about the structure of the quark-gluon plasma. The final section lists possible avenues for future progress.

    nucl-thhep-ph3 citations
  40. 41*

    Towards a Global Search for New Physics with Isotope Shifts

    Elina Fuchs🇩🇪 · Fiona Kirk🇩🇪 · Agnese Mariotti🇩🇪 · Jan Richter🇩🇪 · Matteo Robbiati🇮🇹

    Isotope shifts have emerged as a sensitive probe of new bosons that couple to electrons and neutrons, and of nuclear structure. The recent Hz- or even sub-Hz-level isotope shift measurements across different elements call for a global assessment of all available data. In this work, we present the fit framework kifit that for the first time enables a combined analysis of isotope shift data from several elements, taking into account correlations. We provide a thorough comparison of analytical methods and the fit to analyse linear and nonlinear King plots and quantify their uncertainties. Finally, we provide recommendations for future measurements that could enhance the sensitivity to new physics and offer new insights into nuclear structure.

    physics.atom-phhep-phnucl-exnucl-thPRA(2025)·2 citations
  41. 42*

    Measurement of Downward-going Milli-charged particles beyond GZK cutoff at the Pierre Auger Observatory

    Ye Xu🇨🇳

    It is assumed that superheavy dark matter particles (SHDM, ) with (ZeV) mass may decay to relativistic milli-charged particles (MCPs, ) via a channel . The downward-going MCPs passing through the atmosphere can be searched for at the Pierre Auger observatory (Auger). The massless hidden photon model is taken for MCPs to interact with nuclei, so that we evaluated the numbers and fluxes of expected MCPs at Auger assuming 14 years of Auger data. The hybrid data of Auger was fitted with the flux of UHE MCPs exceeding GZK-cutoff energy. Then the corresponding upper limits on are calculated at 90\% C. L.. These results indicate that MCPs can be searched for with at Auger, when eV and s. And a new region of 10 eV < < 10 eV and > is ruled out in the - plane with 14 years of Auger data. These results indicate potential existence of MCPs and SHDM in the Universe.

    astro-ph.HEhep-ph0 citations
  42. 43*

    Polymer Geodesic Motion in Schwarzschild Spacetime

    Lorenzo Boldorini🇮🇹 · Corrado Marzano🇮🇹 · Giovanni Montani🇮🇹

    In this paper we will study the geodesic motion of massive particles, in a Schwarzschild background, with a semi-classical quantum framework called "Polymer Quantum Mechanics" (PQM) in order to investigate the black hole phenomenology resulting from this formulation, which accounts for Planckian scale physics. In particular we studied two main scenarios, being the radial in-fall and circular orbits and their stability. In this framework, we built an effective Hamiltonian taking into account the polymer quantum effects, altering the classical equations of motion with Planckian scale corrections. As a main result, we obtained the existence of a classically forbidden region surrounding the event horizon, preventing particles from crossing it. Additionally, we discovered the presence of stable circular orbits below both the classical Innermost Stable Circular Orbit (ISCO) and the horizon (corresponding to closed time-like geodesics).

    gr-qchep-ph1 citation
  43. 44*

    Model Comparisons of Transverse Energy and Charged-Particle Multiplicity in A+A Collisions at Midrapidity from 7.7 to 200~GeV

    Niseem Magdy🇺🇸 · Antonio Silva🇺🇸 · Christal Martin🇺🇸 · Josie Hakanson🇺🇸 · Olivia Bartoshesky🇺🇸 · Aidan Hill🇺🇸 · Christine Nattrass🇺🇸

    We present a comprehensive comparison of PHENIX measurements of transverse energy production () and charged-particle multiplicity () at midrapidity to simulations from PYTHIA-8, AMPT, HIJING, and SMASH. These comparisons span both small systems (d+Au, He+Au) and large systems (Cu+Cu, Cu+Au, Au+Au, and U+U) at 200~GeV and Au+Au over a range of beam energies --200~GeV. Using the Rivet framework, we assess the performance of these models. While general trends are captured, significant deviations persist, particularly in low-energy and peripheral collisions, underscoring the need for improved modeling of baryon stopping and energy deposition mechanisms.

    nucl-exhep-phnucl-thJ.Phys.G(2025)·0 citations
  44. 45*

    Resonant neutrino self-interactions: Insights from the full shape galaxy power spectrum

    Hernán E. Noriega🇲🇽 · Josue De-Santiago🇲🇽 · Gabriela Garcia-Arroyo🇲🇽 · Jorge Venzor🇲🇽 · Abdel Pérez-Lorenzana🇲🇽

    This paper investigates resonant neutrino self-interactions in cosmology by employing, for the first time, the effective field theory of large-scale structure to model their impact on the matter distribution up to mildly nonlinear scales. We explore a broad range of mediator masses in two main analyses: one combining BOSS Full Shape (FS) galaxy clustering with Big Bang Nucleosynthesis (BBN), and another combining FS with Planck Cosmic Microwave Background (CMB) data. Our results place the strongest cosmological constraints to date on the resonant self interactions when using FS+Planck data, reaching up to at confidence for the 1 eV mediator. Notably, FS+BBN can constrain the interaction for the 10 eV mediator independently of CMB data, yielding at confidence. Our results suggest that resonant neutrino self-interactions are unlikely to resolve existing cosmological tensions within the standard CDM framework.

    astro-ph.COhep-phPRD(2025)·9 citations
  45. 46*

    Kinetically Coupled Dark Matter Condensates

    Michael W. Toomey🇺🇸 · Savvas M. Koushiappas🇺🇸 · Stephon Alexander🇺🇸

    Dark matter consisting of ultralight bosons can form a macroscopic Bose-Einstein condensate with distinctive observational signatures. While this possibility has been extensively studied for axions and axion-like particles pseudoscalars with masses protected by shift symmetry realistic models from string theory and other higher-dimensional theories predict more complex structures. Here we investigate a two-field generalization where an axion couples to a moduli field through its kinetic term, representing the phase and radial modes of a complex scalar field. We demonstrate that when this system forms a gravitationally bound Bose-Einstein condensate, the kinetic coupling produces dramatic modifications to cosmological evolution compared to the canonical single-field case. Most notably, the axion Jeans scale becomes dynamically dependent on the moduli field's evolution, fundamentally altering structure formation. By mapping existing observational constraints from canonical axion models to our two-field scenario, we identify regions of parameter space that are already excluded by current observations. In particular, consistency with observations requires that the moduli field must take on small field values, , throughout most of cosmic history for this class of axions to remain a viable description of all dark matter.

    astro-ph.COhep-ph5 citations
  46. 47*

    Perturbative Kähler Moduli Inflation

    Mishaal Hai🇮🇹 · Ahmed Rakin Kamal🇨🇿 · Noshin Ferdous Shamma🇮🇹 · Md Shaikot Jahan Shuvo🇺🇸

    In this work, we present two classes of inflationary models in the framework of type IIB string theory. The inflatons correspond to blow-up Kähler modulus arising from compactifying type IIB string theory on a Calabi-Yau. Using perturbative corrections, we first highlight a procedure for stabilising more than one Kähler modulus. For the case of two Kähler moduli, we explicitly construct two classes of inflationary potentials within the Kähler cone which satisfy both EFT and cosmological constraints. The first class of models, arising from moduli redefinition of the blow-up mode, garners a potential of the form align with CMB data with scalar-to-tensor ratio . The second class of models, which have been recently proposed as loop blow-up inflation, have a form , also agrees with CMB data with scalar-to tensor-ratio . Our work differs from the original loop blow-up inflation in terms of stabilization mechanism and subsequently the scalar-to tensor ratio.

    hep-thastro-ph.COgr-qchep-ph29 citations

* Reconstructed cohort: no mailing for this day survives in the archive. Papers are grouped by their submission times and arXiv's announcement cut-off, assuming announcement without delay; positions follow identifier order. Validated at ~91% exact-day agreement against the archived era.