PaperPanorama

HEP Phenomenology·hep-ph

Tue·Sep 1, 2026

60 papers37 primary·23 cross-listed

  1. 01

    Constrained functional priors for Bayesian inference of hot QCD matter

    G. Guimarães🇧🇷 · L. Perin🇧🇷 · M. Luzum🇧🇷

    Bayesian analyses of heavy-ion collisions rely on functional inputs, such as temperature-dependent transport coefficients and the equation of state, whose prior specification remains a significant source of uncertainty. Standard approaches employ low-dimensional parametrizations that can impose artificial correlations and leave the resulting inference sensitive to the assumed functional form. We develop a nonparametric framework for constructing priors over such functions using Gaussian processes, tailored to emulator-based inference in heavy-ion phenomenology. Truncated Karhunen--Loève expansions yield optimized finite-dimensional representations suitable for use as emulator inputs. We investigate how physical constraints can be incorporated into these priors, demonstrating that rejection-based methods produce non-Gaussian measures and induce nontrivial correlations in the expansion coefficients. By contrast, pushforward constructions enforce the constraints while preserving a tractable Gaussian measure in a latent space. These results provide a systematic framework for incorporating physical constraints into functional priors and clarify their effects on the statistical structure of the finite-dimensional representations used in Bayesian inference.

    hep-phnucl-th0 citations
  2. 02

    First Evidence for an Unambiguous Triangle Singularity from

    Qi Huang🇨🇳 · Yi-Jia Zeng🇨🇳 · Xiao-Rui Lyu🇨🇳 · Rong-Gang Ping🇨🇳 · Jia-Jun Wu🇨🇳

    Triangle singularities, predicted by Landau in 1959, are purely kinematic enhancements arising from hadronic rescattering loops. Despite their proposed role in various anomalous decay processes and exotic hadron candidates, a direct experimental confirmation has remained elusive for more than six decades. We analyze the invariant mass spectrum in measured by the BESIII Collaboration. The data exhibit a clear cusp-like structure around 1.564~GeV in the region, in precise agreement with the kinematic position predicted for the triangle singularity. Including the triangle singularity loop in the fit substantially improves the description of the data, with decreasing from 1.22 to 0.90, corresponding to a significance of for the triangle singularity contribution. The precise alignment of the observed excess with the predicted kinematic position provides the first compelling evidence for the triangle singularity effect.

    hep-ph0 citations
  3. 03

    Towards power corrections in the factorization of baryon quasi-distribution amplitudes in LaMET

    Yu-Ji Shi🇨🇳 · Jun Zeng🇨🇳

    Light-cone distribution amplitudes (LCDAs) are essential to precision phenomenological studies. They can be accessed from lattice QCD through the large-momentum effective theory (LaMET) via quasi-distribution amplitudes (quasi-DAs). Factorization of quasi-DAs receive power corrections in inverse powers of the hadron momentum, including target-mass and higher-twist corrections. In this work, we present the first systematic analysis of such power corrections for the leading-twist baryon quasi-DA. Establishing the moment relation between the quasi-DA and the LCDA, we derive an exact closed-form relation that resums target-mass correction to all orders at leading twist. This result also applies to heavy baryons and to quasi-transverse-momentum-dependent distributions. We numerically assess these corrections for the baryon quasi-DA using existing lattice data, finding that the target-mass correction decreases rapidly with increasing baryon momentum and is almost negligible in the endpoint regions. In addition, we explicitly construct the next-to-leading-twist operators entering the quasi-DA factorization. Our results are a first step toward quantifying the power corrections in future lattice determinations of light or heavy baryon LCDAs.

    hep-phhep-lat0 citations
  4. 04

    Taming lepton portal dark matter by a non-invertible selection rule

    Junichiro Kawamura🇯🇵

    We point out that a non-invertible selection rule can control the flavor violation inherent in lepton portal dark matter, a weakly interacting massive particle candidate that can evade severe constraints from direct detection experiments. We show that ordinary invertible symmetries cannot suppress flavor-violating portal couplings while accommodating the large mixing angles in the PMNS matrix. We then present a simple construction based on the gauging of a symmetry, which realizes one-flavor dominance of the portal couplings consistently with the PMNS mixing matrix. We also discuss possible flavor leakage in a type-I seesaw completion and study experimental probes of the model through lepton observables, especially lepton flavor non-universality in boson decays.

    hep-phhep-th0 citations
  5. 05

    Higgs boson pair production in SMEFT: shape and truncation studies

    Manosch Bär🇩🇪 · Bakar Chargeishvili🇩🇪 · Ramona Gröber🇮🇹 · Gudrun Heinrich🇩🇪 · Konstantin Schmid🇮🇹

    We present a comparative study of the influence of Wilson coefficients on Higgs boson pair production cross sections in SMEFT up to dimension-6, also including loop-suppressed operators. Our study accounts for NLO QCD corrections, and is based on updated parametrizations of the cross section as a polynomial in the Wilson coefficients. We focus on differential distributions for the Higgs boson pair invariant mass, as well as the transverse momenta of the leading Higgs bosons, identifying benchmark scenarios exhibiting pronounced shape distortions in the and distributions. While some of these scenarios remain physically meaningful under a purely linear truncation of the SMEFT expansion, others yield unphysical differential cross sections when quadratic dimension-6 contributions are omitted, exposing the breakdown of the linear approximation for large anomalous couplings.

    hep-phhep-ex0 citations
  6. 06

    Probing strange-sector flavor-changing neutral currents at DUNE-like facilities

    Xin-Shuai Yan🇨🇳 · Miao Liu🇺🇸 · Qin Chang🇨🇳 · Ya-Dong Yang🇨🇳

    We investigate the sensitivity of DUNE-like facilities to flavor-changing neutral-current interactions between down and strange quarks through inclusive deep-inelastic neutrino scattering. In the framework of a general low-energy effective Lagrangian for Dirac and Majorana neutrinos, we evaluate projected sensitivities for CP- and -optimized beam configurations. The strongest bounds on the dimensionless Wilson coefficients, defined relative to the Fermi constant , reach at the near detector, whereas far-detector limits are roughly one order of magnitude weaker. When systematic uncertainties are included, the near-detector sensitivity is dominated by the background-rate uncertainty, while the far-detector sensitivity is limited primarily by the signal-rate uncertainty. At the far detector, the dependence of the projected bounds on the neutrino mass ordering and the Dirac CP-violating phase is largely confined to coefficients involving the electron flavor.

    hep-ph0 citations
  7. 07

    Embedding dependence of fermion mass hierarchies in -symmetric Yukawa sectors

    Ye Zhou🇺🇸

    When irreducible representations occur with multiplicity, a family symmetry fixes the representation content of a Yukawa sector but need not fix its embedding in the space of generation tensors. We study the spectral consequences of this additional embedding data for complex-symmetric three-family tensors with the assignment . Since , three-dimensional invariant Yukawa subspaces of type form a continuous family, denoted on a finite affine chart. On the branch, we solve the inverse singular-value problem and obtain necessary and sufficient conditions for any prescribed ordered positive mass spectrum. A fixed singlet embedding imposes a finite hierarchy bound, whereas varying the embedding accommodates every positive three-family spectrum. For general embeddings, contains a nonzero rank-one matrix if and only if ; equivalently, these are precisely the finite-chart embeddings for which is unbounded. In a conventional complex-symmetric three-Higgs sector, the same condition becomes , so order-one Yukawa coupling ratios can support arbitrarily large mass hierarchies. We then apply the result to a recent Clifford-algebraic construction and show that its family-resolved Yukawa tensors span , whose singular values obey . This excludes the observed charged-lepton hierarchy for arbitrary complex vacuum alignment within the existing Higgs directions. The resulting obstruction is therefore tied to the fixed multiplicity embedding rather than to the representation content alone.

    hep-phhep-th0 citations
  8. 08

    Probing Ultra-Compressed Scotogenic Dark Matter at the HL-LHC via 4D Spacetime Tracking

    Renjie Wang🇨🇳

    The ultra-compressed scotogenic regime, in which a 2\,GeV mass splitting between the charged inert scalar and the dark-matter fermion is motivated by and compatible with co-annihilation to the observed relic density for suitable choices of the remaining model parameters, produces decay leptons for which existing LHC displaced-lepton and disappearing-track searches retain only partial, unoptimised acceptance, leaving room for a dedicated timing-assisted strategy. We propose exploiting the 30\,ps timing resolution of the HL-LHC precision timing detectors as a fourth observable, converting the macroscopic scalar decay length of 100--1000\,mm into an arrival-time delay of 70--700\,ps---more than three orders of magnitude above the sub-picosecond delays of all prompt Standard Model backgrounds. Operating at the level of a low- disappearing-track stub matched to a delayed timing hit, without requiring full lepton reconstruction, our 4D timing strategy achieves signal efficiencies of 12--36\% across the probed mass range (14\% at the 200\,GeV benchmark) and zero background across simulated prompt SM events, projecting 95\%\,C.L.\ exclusion up to scalar masses of \,GeV at 3000\,fb under conservative background assumptions. The scalar lifetime is set by the Yukawa coupling through , while sub-eV neutrino masses constrain only the product ; the small couplings that place the charged scalar in the optimal timing window are therefore compatible with, though not uniquely fixed by, the radiative neutrino-mass mechanism, making the co-annihilation corridor---conventionally the most elusive regime---an accessible target for 4D spacetime tracking at the HL-LHC.

    hep-ph0 citations
  9. 09

    Finite-Width Dissolution of Radial Spectroscopy in Single-Top Mesonic Correlations

    Bing-Dong Wan🇨🇳 · Shuo Yang🇨🇳

    Within the heavy-mass expansion, the pole width of a system containing one unstable heavy constituent inherits the constituent width up to corrections, while radial splittings remain . The top quark is an extreme realization of this hierarchy. We implement the complex top pole mass in an instantaneous Bethe--Salpeter framework, where a biorthogonal Hellmann--Feynman relation realizes width inheritance at the operator level and an artificial heavy-mass scan confirms the predicted suppression. The low-pole source-projected response has a single broad maximum at the physical top width in the , , and channels. Full width-dependent non-Hermitian re-diagonalization and a direct full-matrix resolvent evaluation confirm the progressive dissolution of the small-width radial maxima. Thus stable-top eigenvalues survive as reference poles but not as a resolvable multi-peak spectrum; they may instead leave qualitative, process-dependent signatures, such as a broad threshold enhancement or modified color flow.

    hep-ph0 citations
  10. 10

    Probability-based Estimates of the Uncalculated NLO QCD Contribution to the Hadronic -Boson Decay Width

    Shu-Heng Yang🇨🇳 · Jiang Yan🇨🇳 · Xing-Gang Wu🇨🇳 · Zhi-Fei Wu🇨🇳

    The perturbative QCD corrections to the hadronic decay width of the boson are currently known up to next-to-next-to-next-to-next-to-leading order (), whereas the exact correction remains unavailable owing to its formidable computational complexity. In this work, we estimate the contributions by adopting Bayesian analysis (BA). Before performing the estimation, the Principle of Maximum Conformality (PMC) is employed to improve the precision of the initial scale-dependent perturbative series. Through recursive application of the renormalization group equation, non-conformal terms are absorbed into the strong running coupling, yielding a scheme-independent, scale-invariant perturbative series with improved convergence. The PMC procedure determines an effective coupling , with the PMC scale fixed as at next-to-next-to-leading logarithmic accuracy. Based on the improved and more precise series, the BA credible interval yields an uncertainty of . The resulting hadronic branching ratio is , which is consistent with experimental data within reasonable errors.

    hep-ph0 citations
  11. 11

    On-shell renormalization in NREFT: a simplified description of resonances, bound states, and coupled channel effects

    Guo-Ying Chen🇨🇳

    We discuss several issues regarding the modern generalization of Weinberg's compositeness criterion. In particular, we demonstrate that the on-shell renormalization in NREFT reproduces Weinberg's result and provides a simple description of resonances, bound states, and coupled channel effects. Additionally, we present the complete propagator, including the charged channel for the near-threshold p-wave states.

    hep-phhep-exnucl-th0 citations
  12. 12

    and LFV decays in a left-right model with inverse seesaw neutrinos

    L. T. Hue🇻🇳 · Vo Quoc Phong🇻🇳 · T.D. Tham🇻🇳 · N.H.T. Nha🇻🇳

    In the framework of a left-right model with inverse seesaw neutrinos recently proposed, we show that one-loop contributions from heavy singly charged Higgs bosons to the anomalous magnetic moments of charged leptons can accommodate the observed discrepancies, of and for the muon and electron, respectively. Meanwhile, all lepton-flavor violating decay rates for , , and are found to be highly suppressed as a consequence of the gauged symmetry.

    hep-ph0 citations
  13. 13

    X(2370) as the pseudoscalar glueball: Another clue from a constituent approach

    F. Buisseret🇧🇪

    The pseudoscalar state X(2370) is the clearest glueball candidate experimentally identified so far. From a phenomenological point of view, constituent approaches, in which the lightest glueballs are modelled as bound states of two transverse constituent gluons linked by an adjoint flux tube, reach a good agreement with quenched lattice QCD pure gauge spectrum. Based on the assumption that the total decay width of glueballs or light unflavoured mesons is proportional to the energy stored in the flux tube, a model is developed that linearly correlates the hadron decay width to its mass. The model is first fitted on light unflavoured mesons and then extended to glueballs. Both the mass and decay width of the X(2370) are compatible with the results of the constituent approach. Other experimental glueball candidates in the scalar and tensor channels are also reviewed to show the ability of the developed approach to identify glueballs: The f(2150) and f(2300) states appear as promising tensor glueball candidates.

    hep-ph0 citations
  14. 14

    Seesaw and Axion in No-Scale Gravity

    Anamaria Hell🇯🇵 · Lincoln da S. Pereira🇧🇷 · Tsutomu T. Yanagida🇯🇵

    The No-Scale gravity is a compelling framework to describe particle physics, gravity and cosmology, in which all mass scales are an illusion given by the value of a scalar field . This theory, however, falls under the umbrella of more general scalar-tensor theories, which propagate different modes depending on the scalar field, and faces the extensive debate regarding the equivalence between its Jordan and Einstein frame descriptions. In this work we advocate that by excluding the singular point in the transformation between the two frames (e.g., ) we can have the classical equivalence between them. To show the merit of removing this singular point, we argue the Jordan frame makes the symmetries of the model manifest, which creates a suitable playground for the particle-physics model building which we illustrate by showing the emergence of discrete symmetries which leads to a high-quality axion and also naturally incorporate the seesaw mechanism.

    hep-phastro-ph.COgr-qc0 citations
  15. 15

    Debye screening mass in hot QCD at three loops: Canonical form of the integrand

    York Schröder🇨🇱 · Miguel Váez

    The Debye screening mass is a fundamental parameter characterizing the screening of chromo-electric fields in a hot quark-gluon plasma. It plays an important role in thermal field theory, entering the description of screening lengths, transport phenomena, heavy-particle interactions in the early Universe, and the dimensional reduction program that connects thermal QCD to effective three-dimensional theories. In this contribution, we revisit the reduction strategy that serves to organize the large number of terms that contribute to the screening mass at the three-loop level, applying recent advances based on canonical forms of thermal (sum-) integrands. We emphasize the role of integration variable shifts, and discuss how canonical representations of thermal integrands may simplify future high-order calculations in hot QCD.

    hep-ph0 citations
  16. 16

    Kaon gravitational form factors and mechanical structure in a three-flavor NJL model

    Zhibo Liu🇯🇵 · Hiroaki Abuki🇯🇵

    We investigate the gravitational form factors (GFFs) of the kaon in a proper-time-regularized three-flavor Nambu--Jona-Lasinio model. We treat the kaon as a light--strange pseudoscalar bound state and evaluate its energy--momentum-tensor matrix element using a dressed quark--graviton vertex. By retaining the interaction-induced contact contribution alongside the quark triangle diagrams, we preserve the gravitational Ward--Takahashi identity and ensure the conservation of the total energy--momentum tensor. We determine the light- and strange-quark contributions to the kaon GFFs, contrast them with the corresponding pion results, and extract the associated pressure and shear-force distributions, together with the Breit-frame and transverse light-front mass radii. Explicit flavor-symmetry breaking dictates that the strange sector carries a larger share of the kaon momentum and mechanical response. Consequently, compared to the pion, the kaon exhibits a less negative -term and more compact mechanical distributions, featuring enhanced central pressure and shear. We further show that a Ward--Takahashi-identity-preserving reduction of the -term projection is essential for maintaining the pion low-energy theorem in proper-time regularization.

    hep-ph0 citations
  17. 17

    In-Medium Modification of Meson Mass over Temperature and Momentum

    Hidefumi Matsuda🇨🇳 · Philipp Gubler🇯🇵 · Koichi Hattori🇨🇳

    We analyze the in-medium modification of the meson mass below the pseudo-critical temperature at vanishing baryon chemical potential using QCD sum rules. The sum rules are applied separately to the transverse and longitudinal polarization modes of the meson defined relative to the spatial momentum in the medium rest frame. We map out the temperature and momentum dependence of the mass in each mode and quantify the resulting transverse--longitudinal mass splitting. The splitting develops with increasing temperature and momentum.

    hep-ph0 citations
  18. 18

    The inclusive decay rate with higher precision

    M. Misiak🇵🇱 · H. M. Asatrian🇦🇲 · K. Brune🇩🇪 · M. Czaja🇩🇪 · M. Czakon🇩🇪 · M. Fael🇮🇹 · C. Greub🇨🇭 · T. Huber🇩🇪 · F. Lange🇨🇭 · L. T. Moos🇩🇪 · M. Niggetiedt🇨🇭 · A. Rehman🇨🇦 · K. Schönwald🇨🇭 · M. Steinhauser🇩🇪

    We present a new and upgraded analysis of the inclusive weak radiative decay of the meson in the standard model and beyond. The perturbative corrections are included in a formally complete manner. At the order , exact dependence on the charm quark mass is calculated for the dominant corrections, which removes a sizeable uncertainty that was present in all the previous analyses. The global normalization factor and many of the non-perturbative contributions are expressed in terms of the kinetic-scheme mass of the -quark and the heavy-quark-expansion matrix elements. These parameters are adopted from the most recent semileptonic fits that include corrections and up-to-date experimental results. We find for the CP- and isospin-averaged branching ratio of the considered decay in the standard model, with a lower cut on the photon energy . It agrees with the current experimental average , which provides constraints on beyond standard model physics. In particular, we find at for the charged Higgs boson mass in the two-Higgs-doublet model~II.

    hep-phhep-ex2 citations
  19. 19

    NNLO QCD corrections to the weak radiative -meson decay with exact dependence on

    M. Czaja🇩🇪 · M. Czakon🇩🇪 · T. Huber🇩🇪 · M. Misiak🇵🇱 · M. Niggetiedt🇨🇭 · A. Rehman🇨🇦 · K. Schönwald🇨🇭 · M. Steinhauser🇩🇪

    The inclusive weak radiative -meson decay provides important constraints on many popular extensions of the Standard Model. Some of the numerically relevant Next-to-Next-to-Leading-Order QCD corrections to its branching ratio have so far been evaluated using an interpolation in the charm quark mass between the and limits. In the current paper, we present their determination for the physical value of , which required calculating hundreds of four-loop propagator diagrams with unitarity cuts and two mass scales. Our final result for the CP- and isospin-averaged branching ratio reads for in the decaying meson rest frame. It is in good agreement with the current Particle Data Group average .

    hep-ph1 citation
  20. 20

    Quantum-statistical effects of bosonic warm dark matter in microscopic interacting dark sectors

    Zhijian Zhang🇨🇳

    We investigate the impact of the quantum statistical properties of bosonic warm dark matter (BWDM) on a microscopic interacting dark-sector model mediated by a Yukawa coupling. We consider a BWDM scenario containing a Bose--Einstein condensed (BEC) component. By separating the BWDM phase-space distribution into thermal and condensate components, we derive the thermally averaged annihilation cross sections for the thermal--thermal, thermal--condensate, and condensate--condensate channels. The long-range scalar interaction and its Sommerfeld enhancement are included in the annihilation processes. We find that the condensate fraction provides an additional quantum-statistical degree of freedom controlling the microscopic dark-sector energy transfer. In particular, the transition between the thermal--thermal dominated regime and the condensate--condensate dominated regime is characterized by a critical condensate fraction r_c, which is mainly determined by the BWDM mass and the dark energy scalar field mass. For condensate fractions above this critical value, the condensate--condensate channel dominates the present-day interaction rate. By imposing the condition that the present-day interaction rate does not exceed the Hubble expansion rate, we determine the corresponding region of the dark-sector parameter space satisfying this condition.

    hep-ph0 citations
  21. 21

    Quantum Steering Geometry at High Energy Particle Colliders

    Juan J. Mejia Alvarez🇺🇸 · Andrew J. Wildridge🇺🇸 · Angelo Arisi🇺🇸 · Juan M. Duarte-Quiros🇺🇸 · Santosh Bhandari🇺🇸 · Jingyan Li🇺🇸 · Giulia Negro🇺🇸 · Andreas W. Jung🇺🇸

    We formulate collider observables based on quantum steering ellipsoids (QSEs) for reconstructed bipartite systems of spin- particles. A collider spin density matrix defines a two-qubit state, while its QSE gives the geometry of conditional states accessible through local measurements. This makes the ellipsoid a direct probe of the quantum properties of fundamental particles, encoding polarization, spin correlation anisotropy, accessible-state volume, and the orientation of the dominant correlation axes. Using top-quark pair production as a benchmark process, we show how QSE observables organize the Standard Model spin state, probe entanglement, steerability, and Bell-nonlocality criteria, and use an expected precision metric to assess sensitivity to non-local correlations in the boosted central region. We show that different dimension-six operators generate distinctive QSE deformations, and provide a geometric interpretation of quantum information observables in high-energy particle physics. Quantum steering geometry therefore provides a unified framework for particle collider tomography, quantum information diagnostics, and precision searches for physics beyond the Standard Model with applications spanning the HL--LHC and future lepton, muon, flavor, and electron-ion collider programs.

    hep-phquant-ph0 citations
  22. 22

    Building a Better Beta: Nucleation and Timescales in Cosmological Phase Transitions

    William Searle🇦🇺 · Csaba Balázs🇦🇺

    First-order phase transitions in the early universe can generate a stochastic background of gravitational waves, offering a unique probe of high-energy physics. In this work, we investigate aspects of bubble nucleation and transition timescales, which play a central role in shaping the resulting gravitational wave spectrum. Many common approaches characterise the transition rate via a Taylor expansion of the false vacuum decay rate. We argue that a more fundamental description is instead given by the distribution of bubble lifetimes, and define a new timescale, , as the first moment of this distribution. We show that reproduces the behaviour of previous timescale definitions in the appropriate limits, while avoiding their pathologies, and offers a more natural description of the ensemble of nucleated bubbles. We then quantify the impact of this improved timescale on the predicted gravitational wave spectrum, finding that it shifts the peak amplitude by up to an order of magnitude relative to previous definitions. As next-generation gravitational wave detectors come online, robust theoretical predictions will be essential; we hope this work represents a step in that direction.

    hep-phastro-ph.CO0 citations
  23. 23

    Spin-dependent fermion potentials from mixed tensor couplings of massive spin-1 and spin-2 bosons

    D. Khadka🇦🇺 · V.V. Flambaum🇦🇺

    Searches for weak spin-dependent forces are commonly interpreted in terms of a basis of sixteen rotationally invariant two-fermion potentials , including potentials which violate parity (P) and time-reversal (T) invariance. We derive finite-range coordinate-space potentials generated by a massive spin-1 boson with vector, axial-vector, tensor, and pseudotensor couplings to Dirac fermions. In addition to the familiar vector--vector, vector--axial-vector, and axial-vector--axial-vector interactions, we obtain the mixed vector--tensor, vector--pseudotensor, axial-vector--tensor, and axial-vector--pseudotensor potentials, together with tensor--tensor, tensor--pseudotensor, and pseudotensor--pseudotensor terms. We retain the contact terms needed in atomic-scale applications and give compact expressions that include both orderings of inequivalent fermion vertices. We then extend the analysis to a massive spin-2 mediator described by a symmetric Fierz--Pauli field. Besides the conventional coupling to the conserved fermion energy--momentum tensor, we consider a symmetric axial-tensor current. Its nonconservation for massive fermions makes the longitudinal spin-2 helicities contribute to axial-tensor--axial-tensor exchange. The leading minimal spin-2 interactions are either even or odd and even; in particular, they do not generate a -odd potential. Heavy-mediator contact limits and the distinction between the massive-spin-2 limit and a genuine massless graviton are also discussed. We map the new interactions onto the sixteen-potential Dobrescu--Mocioiu basis and use this mapping to obtain numerical translations of existing limits for both spin-1 and spin-2 coupling products in the small- and large-mediator-mass regimes, together with representative limits at finite mediator masses.

    hep-phnucl-thphysics.atom-ph0 citations
  24. 24

    High energy thermal photons from chirally imbalanced QGP

    Sourav Duari🇮🇳 · Nilanjan Chaudhuri🇮🇳 · Pradip Roy🇮🇳 · Sourav Sarkar🇮🇳

    We compute the thermal photon production rate from a chirally asymmetric quark gluon plasma. We estimate the hard part from scattering of chiral quarks and demonstrate the cut-off independence of the total thermal photon emission rate. This is achieved by combining the hard with the soft contribution evaluated in our previous work using the Braaten-Pisarski method of hard thermal loop perturbation theory. It is observed that the presence of chiral imbalance leads to an overall enhancement in the emission rate of thermal photons.

    hep-ph0 citations
  25. 25

    First-principle predictions of fragmentation functions via quantum computing

    Juan J. Gálvez-Viruet🇪🇸 · Felipe J. Llanes-Estrada🇪🇸 · Nicolas M. Arenaza🇪🇸 · María Gómez-Rocha🇪🇸 · T. J. Hobbs🇺🇸

    We report on an algorithm to compute fragmentation functions from the first principles Quantum Chromodynamics (QCD) Hamiltonian quantized in Light-Front Gauge, opening a path for digital quantum computers to calculate these longitudinal jet-structure observables. Simulating the behaviour of such computers on a classical cluster (which is memory-limited to about 30 qubits, given the expansive Hilbert spaces of actual quantum computers), we run a demonstration of a heavy-quark leading parton fragmenting into quarkonium, which we benchmark against NRQCD computations. Future quantum computers, perhaps concurrently running with HL-LHC, would have ample opportunity to extract arbitrary parton-hadron combinations.

    hep-phquant-ph0 citations
  26. 26

    Meson gravitational D-form factors and symmetry breaking in low-energy QCD

    Mamiya Kawaguchi🇺🇸 · Kazuhiro Tanaka🇯🇵 · Mitsuru Tanaka🇯🇵

    We investigate meson gravitational D-form factors in the three-flavor linear sigma model and their connection to symmetry breaking in low-energy QCD. Within the scalar meson dominance picture, we examine the scalar meson exchange contributions and their relation to meson masses through scalar-meson couplings. In the three-flavor symmetric limit, we first derive analytical expressions for the D-form factors of pseudoscalar and scalar mesons. In the chiral limit, the forward-limit value of the octet pseudoscalar D-form factor is fixed to , whereas the anomaly generates additional contributions to the singlet pseudoscalar and scalar-meson D-form factors. For realistic flavor breaking, the interaction introduced to reproduce the scalar-meson mass hierarchy below GeV significantly affects the scalar-meson D-form factors. We further compare the linear sigma model results with those obtained from a chiral perturbation theory Lagrangian including a dilatonic scalar field and show that their differences are governed by the canonical mass dimensions of the interaction terms contributing to meson mass generation. These results indicate that meson D-form factors provide sensitive probes of symmetry-breaking structures in low-energy hadron physics.

    hep-phhep-latnucl-th0 citations
  27. 27

    Two-loop QCD corrections to -even Higgs boson decays into in the Type-I Two-Higgs-Doublet Model

    Lin-Qiao Qu🇨🇳 · Zhong-Yuan Liu🇨🇳 · Peng-Fei Duan🇨🇳 · Yu Zhang🇨🇳 · Wei-Long Duan🇨🇳

    We investigate the QCD corrections to the loop-induced decays of the heavy -even Higgs boson, (), within the framework of the Type-I Two-Higgs-Doublet Model (THDM). Owing to the similarity of the underlying loop topologies, the two decay channels exhibit closely correlated behaviour. After imposing relevant phenomenological constraints, we evaluate the decay widths for 5000 viable parameter points at next-to-leading order (NLO) in QCD under the alignment limit. The width exceeds that of by roughly a factor of four. Both are dominated by the top-quark loop: the contribution vanishes in the alignment limit, and the charged-Higgs loop is suppressed throughout most of the viable parameter region. The corrections exhibit a pronounced dependence on the heavy Higgs boson mass , attaining a maximum in the vicinity of the production threshold. To elucidate the individual parameter dependences, dedicated benchmark scenarios are analysed, revealing that the decay widths diminish monotonically with increasing while growing with . The QCD corrections for both decay modes typically span approximately to , with larger corrections in the non-alignment scenario: in the channel they reach up to at large , and in the channel they cross zero to become positive. The selection rule forces the pair into a -wave configuration at threshold, which strongly suppresses the Coulomb corrections and secures the perturbative stability of the fixed-order prediction. A comparison with ATLAS limits shows that current data do not yet constrain the parameter space, whereas the NLO corrections may become relevant for interpreting exclusion bounds at the HL-LHC.

    hep-ph0 citations
  28. 28

    Polarized jet anisotropy at the Electron-Ion Collider

    Zhong-Bo Kang🇺🇸 · Hongxi Xing🇨🇳 · Fanyi Zhao🇺🇸 · Yiyu Zhou🇨🇳

    Jets provide a powerful probe of the three-dimensional spin structure of the nucleon, a central goal of the Electron-Ion Collider. Yet the observed jet defines an axis that breaks the azimuthal isotropy of soft-gluon radiation, thereby reshaping the very asymmetries used to extract that structure. Using transverse-momentum-dependent (TMD) QCD factorization, we show for the first time that this jet-induced anisotropy imposes a parity selection rule on polarized asymmetries. Expanding the transversely polarized structure functions in harmonics , where is the angle between the jet and the lepton-jet momentum imbalance, makes this rule explicit: the symmetry of each harmonic is fixed by the parity of , independently of the magnitudes of the harmonic coefficients. For the Sivers function, the canonical left-right asymmetry about the proton spin survives for even but is replaced by a counterintuitive left-right symmetry for odd . The worm-gear function retains its up-down asymmetry at every harmonic while being left-right symmetric for even and asymmetric for odd . At EIC kinematics, the higher harmonics studied here are predicted to be individually measurable, providing new observables for the azimuthal dynamics of soft radiation and an essential ingredient in precision extractions of nucleon structure.

    hep-phhep-exnucl-th0 citations
  29. 29

    Exploring possible bound states through femtoscopic correlations

    Ye Yan🇨🇳 · Qi Huang🇨🇳 · Qian Wu🇨🇳 · Hongxia Huang🇨🇳 · Jialun Ping🇨🇳

    The femtoscopic correlation technique in relativistic heavy-ion collisions provides a unique opportunity to investigate hadron-hadron interactions and possible exotic states. In this work, we study the correlation function and its sensitivity to the low-energy interaction related to possible bound states. Based on the quark delocalization color screening model, three interaction scenarios with different strengths are constructed, and the corresponding spin-averaged correlation functions are calculated within the Koonin--Pratt formalism. The results demonstrate that the correlation function is sensitive to the interaction strength, with coupled-channel effects and - wave mixing producing additional enhancements in the correlation signal. These findings suggest that future femtoscopic measurements at relativistic heavy-ion collision experiments can provide valuable constraints on the interaction between charmed baryons and nucleons and offer guidance for exploring possible heavy-flavor hypernuclei.

    hep-phnucl-th0 citations
  30. 30

    Charmonium production in p+A collisions at SPS and FAIR energies

    Taesoo Song🇩🇪 · Jiaxing Zhao🇩🇪 · Joerg Aichelin🇫🇷 · Elena Bratkovskaya🇩🇪

    We employ the Parton-Hadron-String Dynamics (PHSD) transport approach to investigate the influence of baryon-rich matter on charmonium production and dissociation. The Remler formalism is implemented to dynamically model charmonium formation from charm-anticharm pairs. As a validation step, the formalism is first benchmarked against experimental data from elementary pp collisions and then extended to pA systems to extract the effective nuclear absorption cross section of charmonium. This extracted cross section can subsequently be applied in heavy-ion collisions to quantify medium-induced effects. Our results demonstrate that the Remler formalism provides a quantitatively consistent description of charmonium production in pp and pA collisions at SPS energies. The approach is then extrapolated to GSI/FAIR energies, where predictions for charmonium yields and survival probabilities are presented. These findings highlight the relevance of the Remler formalism as a dynamical framework for studying heavy-quark bound-state formation in baryon-rich matter and offer theoretical guidance for future experimental programs at SPS, FAIR and NICA aimed at mapping the QCD phase structure.

    hep-phnucl-th0 citations
  31. 31

    Hadron interactions in the U-70 energy range: results and problems

    V. A. Petrov🇷🇺 · N. P. Tkachenko🇷🇺

    From late 1967 until the early 1970s, the Soviet proton synchrotron (better known as the Serpukhov accelerator or U-70), with a nominal laboratory energy of up to 76 GeV, was the world leader. During these few years, several results of fundamental significance were obtained (partially in collaboration with physicists from CERN, France, and other countries). Let us briefly outline the main provisions of the paradigm that reigned at that time in the field of strong interaction theory.

    hep-ph0 citations
  32. 32

    Small-x TMD distributions: JIMWLK evolution and the Gaussian truncation

    Florian Cougoulic🇵🇱 · Piotr Korcyl🇵🇱

    We extend the systematic study of small- Transverse Momentum Dependent (TMD) distributions, initiated in [Cougoulic:2026drr], by including the energy evolution. We use the JIMWLK evolution equation to study the energy dependence of three distributions in the quark-gluon sector, , and seven distributions in the gluon-gluon sector, . The initial conditions are provided by the McLerran-Venugopalan model. We study these TMD distributions in position space and with fixed. We then compare these results to the Gaussian truncation of the Balitsky hierarchy. Although the Gaussian truncation worked very well for the TMD distributions at the initial condition, now we identify some cases where the Gaussian truncation provides a reasonably good description, but in the majority of cases it fails to fully reproduce numerical data. Using the fixed representation building blocks, , we are able to partially explain the outcomes. This work constitutes the next step with the goal of understanding the interplays between the large- limit and Gaussian truncation as well as the BK/JIMWLK evolution equations for phenomenologically relevant observables.

    hep-phnucl-th0 citations
  33. 33

    Exclusive Leptonium Electroproduction

    Hao-ye Deng🇨🇳 · Qi-Ming Feng🇨🇳 · Qi-Wei Hu🇨🇳 · Si-Qin Huang🇨🇳 · Cong-Feng Qiao🇨🇳 · Jia-Xuan Shen🇨🇳 · Ting-Ting Wang🇨🇳 · Shun-Yan Yu🇨🇳 · Hao Zhang🇨🇳 · Xuan-Heng Zhang🇨🇳 · Yi-Nan Zhao🇨🇳

    Purely leptonic bound states provide precision probes of QED. Positronium and muonium have long been observed, whereas dimuonium and tauonium remain undiscovered. We study exclusive vector-leptonium electroproduction in collisions within nonrelativistic QED. We include the Bethe--Heitler and double deeply virtual Compton scattering contributions and their interference, and calculate the NLO QCD hard-scattering kernels entering the dominant Compton form factor within collinear GPD factorization. The NLO QCD correction to the DDVCS contribution changes from a strong suppression at low photon virtuality to a sizable enhancement as the lower virtuality cut is raised, with the gluon channel providing the dominant contribution. Bethe--Heitler production dominates the exclusive rate, supporting dedicated dimuonium searches at the EIC and JLab, with larger samples expected at higher-energy electron--proton colliders. The much larger positronium samples provide a high-statistics environment for precision QED studies, whereas tauonium production remains strongly suppressed.

    hep-ph0 citations
  34. 34

    Medium effect on spin alignment of strange and charm vector mesons

    Ruixiang Chen🇨🇳 · Hiwa A. Ahmed🇷🇴 · Yidian Chen🇨🇳 · Mei Huang🇨🇳

    Understanding the spin alignment of vector mesons in relativistic heavy-ion collisions requires a nonperturbative description of their spin-dependent in-medium properties. We investigate this problem within a unified four-flavor soft-wall holographic framework that combines an anisotropic Einstein--Maxwell--dilaton background at finite temperature, baryon chemical potential, and angular velocity. Spin alignment is determined from the medium-induced splitting of the spin-resolved vector-current spectral functions through an instantaneous freeze-out prescription. We systematically study the strange and charm vector mesons , , , , and and the dependence of their spin alignment on transverse momentum, rapidity, temperature, baryon chemical potential, and angular velocity. We find that the heavy charm vector mesons , , and mesons exhibit at low transverse momentum, whereas the light strange vector mesons and exhibit the opposite low-momentum behavior and angular distributions with . We trace this flavor-dependent separation to the different locations of the vacuum mass shell relative to the thermally shifted longitudinal and transverse spectral peaks. The results qualitatively reproduce several trends observed at low and intermediate transverse momentum. Spin alignment is insensitive to baryon chemical potential and only weakly affected by angular velocity. These results establish an equilibrium holographic baseline for vector-meson spin alignment across flavor sectors and help delineate the regimes in which additional mechanisms, such as nonequilibrium evolution, fluctuations, and hard production, become important.

    hep-ph0 citations
  35. 35

    Columnar Recasting and High-Luminosity LHC Projections for a Light Gauge Boson in the Four-Muon Channel

    Cesar Rendon

    We present an independent recasting of light vector gauge boson () searches at the LHC within the leptophilic framework. A simplified Standard Model extension is implemented in FeynRules, enforcing symmetric chiral leptonic currents while suppressing hadronic couplings. Signal generation for the four-muon () final state is performed using MadGraph5_aMC@NLO, Pythia8, and a tuned Delphes3 detector emulation, covering the mass range 5-62 GeV under a reference coupling g=0.01. The analysis employs a vectorized columnar pipeline in Coffea with Awkward Array masks, enabling parallelized kinematic selections and the recovery of boosted muon topologies. Signal yields are statistically extracted via pyhf against digitized CMS Run 2 backgrounds (77.3 fb). The resulting expected median limit profile tracks the absolute experimental sensitivity morphology within a factor of , a discrepancy successfully quantified as a systematic consequence of fast-simulation detector limitations and the mass-window binned counting strategy relative to experimental unbinned multivariate profiling, thereby establishing a rigorous and conservative baseline sensitivity floor. Furthermore, we project the discovery potential for the future High-Luminosity LHC (HL-LHC) phase at fb under the official CERN Scenario II recommendations. We demonstrate quantitatively that the HL-LHC will achieve exceptional expected local statistical discovery significances between 10.22 and 16.61 within the 5-28 GeV mass window, comfortably clearing the discovery threshold and establishing the multi-muon channel as a primary probe for lightweight vector portals in upcoming collider phases.

    hep-ph0 citations
  36. 36

    From Threshold Crossing to Wave-function Renormalization: Defining the Pion Mott Temperature in a Magnetic Field

    Sidney S. Avancini🇧🇷 · Maximo Coppola🇦🇷 · Dyana C. Duarte🇧🇷 · Ricardo L. S. Farias🇧🇷 · Norberto N. Scoccola🇦🇷 · William R. Tavares🇵🇹

    We investigate the dissociation of the neutral pion in hot magnetized quark matter within the two-flavor Nambu--Jona-Lasinio model. At zero magnetic field, the Mott temperature is conventionally determined by , above which a real pole ceases to exist. At finite magnetic field, Landau quantization replaces this single threshold by a hierarchy of quark--antiquark continua and generates multiple solutions of the pion pole equation, rendering a direct threshold-crossing criterion ambiguous since a real pion solution below the lowest nominal threshold always exists. We therefore propose to define the magnetic Mott temperature through the inflection point of the pion wave-function renormalization factor of that lowest pole, corresponding to the fastest loss of its spectral function strength. The prescription reproduces the conventional Mott temperature as and tracks the chiral pseudocritical temperature for both constant and magnetic-field-dependent couplings. Our results characterize pion dissociation in a magnetic field as a spectral crossover rather than a simple threshold crossing.

    hep-phhep-lat0 citations
  37. 37

    Quantum Simulation of Markovian and Non-Markovian Open Quantum Dynamics in Heavy-Ion Collisions

    Doojin Kim🇺🇸 · Balbeer Singh🇺🇸

    We present a quantum computing framework for simulating open-quantum-system approaches based on Markovian and non-Markovian dynamics, which is relevant to heavy-ion collisions. To simulate the non-Markovian evolution on quantum computers, we introduce an auxiliary two-level pseudomode that carries the memory forward and couples to both the subsystem and the residual Markovian bath. We explicitly show that tracing out the pseudomode reproduces the non-Markovian evolution with the exact memory kernel. Moreover, in the relevant time scale hierarchy, the quantum circuit construction of the pseudomode smoothly converges to the Markovian limit. For a given bath memory kernel, our results demonstrate the feasibility of quantum simulations of both Markovian and non-Markovian dynamics, establishing a framework for future studies of hard probes such as jets, heavy quarks, and quarkonia in heavy-ion collisions.

    hep-phquant-ph0 citations
  38. 38

    Characterizing Single-Signal Events from Atmospheric-Neutrino Neutral-Current Interactions in Large Liquid Scintillator Detectors

    Zhenning Qu🇨🇳 · Jie Cheng🇨🇳 · Wan-lei Guo🇨🇳 · Gaosong Li🇨🇳 · Yu-Feng Li🇨🇳 · Liang-jian Wen🇨🇳

    Neutral-current interactions of atmospheric neutrinos in large liquid scintillator detectors offer a new opportunity to study single-signal events (hereafter singles), characterized by a prompt energy deposition on the MeV-to-GeV scale and no identified delayed signal. In this work, we systematically investigate the model dependence of atmospheric-neutrino singles due to the primary neutrino-nucleus interaction, residual-nucleus de-excitation, and secondary interactions in the scintillator. Our results show that the dominant model dependence originates from the primary neutrino-nucleus interaction, especially for neutral-current processes on carbon, whereas de-excitation is essential for the singles selection yet leads to relatively small spectral variations among realistic models. Secondary-interaction effects are also subdominant overall. We further present the predicted event rates and prompt-energy spectra for neutral-current singles, along with the charged-current contribution. Separately, we estimate the low-energy contribution from elastic scattering of sub-\SI{100}{\MeV} atmospheric neutrinos on free protons. These results highlight the physics potential of current and future large liquid scintillator detectors, such as the Jiangmen Underground Neutrino Observatory, to study atmospheric-neutrino singles, probe neutrino-nucleus interaction models, and improve background estimates for rare-event searches.

    hep-exhep-ph0 citations
  39. 39

    Machine Learning Unveils Finite-volume Energy Shifts in Three-body System

    Wei-Jie Zhang🇨🇳 · Zhenyu Zhang🇨🇳 · Jifeng Hu🇨🇳 · Bing-Nan Lu🇨🇳 · Jin-Yi Pang🇨🇳 · Qian Wang🇨🇳

    Finite-volume extrapolation (FVE) is essential for extracting physical observables in the lattice calculation. While rigorous FVE formulations are well established for short-range potentials in both two- and three-body systems, long-range interactions with force ranges comparable to the lattice size remain challenging. Extending a previous data-driven scheme for two-body systems, we apply symbolic regression (PySR) to uncover universal three-body FVE formulae. For short-range potentials, we reproduce the two limiting cases, i.e. and . For pure long-range potentials, we obtain a dedicated analytic expression, and after incorporating short-range contributions, we uncover a unified formula consistent with the original PySR solution, which performs excellently in the intermediate force range around 1 fm. This work demonstrates that combining machine learning with physical constraints can yield novel analytical results inaccessible to conventional theoretical tools, advancing data-driven methodologies in hadron physics.

    hep-lathep-phnucl-th0 citations
  40. 40

    Emergent hydrodynamic response and dynamical backreaction: Magnon bound-state propagation in a Bose-Hubbard fluid

    Andrés N. Cáliz🇪🇸 · Arnau Riera🇪🇸 · Enrique Rico🇨🇭 · João Barata🇨🇭 · Marcin Płodzień🇪🇸

    We study the nonequilibrium response of a one-dimensional Bose-Hubbard medium to a two-magnon bound state propagating along an attractive XXZ chain. A Holstein-type displacement coupling makes the magnon density act both as a local chemical-potential perturbation and as a source of bosons. We derive a long-wavelength hydrodynamic description of the density and phase fluctuations and test it against matrix-product-state simulations of the full coupled dynamics. The theory predicts a comoving near-field deformation together with retarded density waves confined to a sound cone. In the Mott regime, the deformation remains localized around the moving pair. In the compressible regime, two counterpropagating fronts detach and approach the semiclassical sound velocity, recovered from the equilibrium density with no fitted parameters. The coupling also induces a dynamical backreaction that slows the bound state and broadens its magnon-density profile. The comparison delimits where hydrodynamics stays quantitative once the probe reacts back on the medium.

    cond-mat.quant-gashep-phquant-ph0 citations
  41. 41

    AXIS Could Have Accessed Dark Matter Decays

    Joshua W. Foster🇺🇸 · Inci Karaaslan🇺🇸 · Gordan Krnjaic🇺🇸 · Nimrod Shapir🇺🇸

    The Advanced X-ray Imaging Satellite (AXIS) was a mission concept designed to improve upon the sensitivity and spatial resolution of the Chandra X-ray Observatory and XMM-Newton. Although AXIS was not selected for implementation, the concept study defined a mature instrument design with low-background, arcsecond imaging over the - keV energy range, a large effective area, and a wide field of view. These capabilities provide a useful benchmark for the dark matter decay sensitivity of future X-ray observatories. We estimate the reach of a future AXIS-like instrument for narrow photon lines from decaying keV-scale dark matter, including axion-like particles and sterile neutrinos. For Galactic center observations, we find projected lifetime sensitivities of order s, improving upon existing limits by up to an order of magnitude over part of the keV mass range.

    astro-ph.COastro-ph.GAastro-ph.HEhep-ex+10 citations
  42. 42

    Inspiralling Binary merger parameter reconstruction with lunar and satellite Laser Ranging

    Miguel Vanvlasselaer🇧🇪

    Precision tracking of Earth--Moon and Earth--satellite ranges offers a novel, low-frequency avenue for detecting gravitational waves from inspiralling massive black hole binaries, complementary to space-based interferometers. In this paper, we propose a first study of the reconstruction of the binary parameters from a synthetic set of range observations. \textit{Set-up}: Assuming an ideal unperturbed Keplerian motion for the earth-satellite binary, we develop a framework for reconstructing the chirp mass and luminosity distance of chirping sources from the perturbations they induce on ranging observables, using both Lunar Laser Ranging (LLR) and a two-satellite ranging configuration (GUEST) as concrete case studies. \textit{Result}: We find that chirp-mass recovery tightly converges as a power law in SNR (, to ) for both LLR and GUEST. In contrast, the luminosity distance suffers from a severe, SNR-independent degeneracy with the sky-orientation angles in the LLR configuration, yielding fractional biases and uncertainties of tens to over a hundred percent regardless of signal strength. The two-satellite GUEST configuration breaks this degeneracy and restores a convergent, SNR-dependent recovery of comparable in scaling to that of the chirp mass. These results demonstrate that multi-baseline ranging architectures are essential for extracting luminosity-distance information from ranging-based gravitational wave searches, while chirp-mass measurements remain reliably accessible even with a single ranging baseline such as the Earth--Moon system.

    gr-qcastro-ph.COhep-ph0 citations
  43. 43

    Decisive evidence for a global cosmic-ray feature in gamma-ray data

    Fernando Valenciano · Pedro De la Torre Luque🇪🇸 · Daniele Gaggero🇮🇹 · Jorge Martin Camalich🇪🇸

    We analyze 17 years of Fermi-LAT data to study the diffuse -ray emission along the Galactic plane and its connection to cosmic-ray (CR) propagation. Accounting for correlated instrumental systematics, we find decisive evidence for a spectral break at GeV, present across the inner Galactic disk, with a preference of ( global). The energy and amplitude of this feature are in striking agreement with the spectral feature observed in local CR nuclei, indicating that it is a global property of the Galactic disk rather than a local phenomenon. The measured slope change, , is consistent with local CR data and with expectations from a transition in the CR diffusion regime from Kolmogorov to Kraichnan turbulence. Our results provide strong evidence that diffuse -ray emission along the Galactic disk is dominated by decay emission up to a hundred GeV. These findings provide key insights into the origin of the CR spectral hardening and the propagation of CRs throughout the Galaxy, and illustrate how this multimessenger approach can be used to probe the origin of features in the CR spectra, such as the long-studied CR Knee.

    astro-ph.HEastro-ph.GAhep-ph0 citations
  44. 44

    Torsion and Nonmetricity Constraints From Neutron Spin Rotation in Polarized Matter

    Sepehr Samiei🇺🇸 · Ralf Lehnert🇺🇸 · W. Michael Snow🇺🇸

    Many modified-gravity frameworks employ non-Riemannian connection degrees of freedom, including torsion and nonmetricity. In Einstein-Cartan-type theories, torsion is associated with spin density, while more general metric-affine frameworks can be investigated through phenomenological searches for in-matter torsion and nonmetricity backgrounds. This work applies an effective field theory approach to characterize general couplings of electron and neutron operators to spacetime torsion and nonmetricity up to mass dimension six, predicting novel neutron-polarization signatures in the presence of an electron background. Neutron spin-rotation data from a polarized-electron ensemble inside a compensated ferrimagnet are used to constrain for the first time axially symmetric, direction-dependent in-matter torsion and nonmetricity combinations.

    gr-qchep-exhep-phnucl-ex0 citations
  45. 45

    Strongly coupled quark matter in neutron stars and their mergers

    Konstantin Maslov🇺🇸 · Ralf Rapp🇺🇸 · Joaquin Grefa🇺🇸 · Veronica Dexheimer🇺🇸 · Claudia Ratti🇺🇸

    The discovery of the strongly-coupled quark-gluon plasma (sQGP) in high-energy heavy-ion collisions has revealed remarkable properties of matter at high temperature, with transport coefficients close to conjectured bounds from quantum field theory at strong coupling. The high sQGP collision rates imply very large energy uncertainties and the melting of quasiparticle structures. Deploying quantum many-body theory based on the self-consistent -matrix approach for the sQGP at high temperature, we investigate its manifestation at high baryon density and low temperature, as present in neutron stars and their mergers. We constrain the chemical-potential dependence of the quark interaction kernel using first-principles information from Quantum Chromodynamics on baryon-number susceptibilities. Very large collisional widths persist at large density and are found to relegate superconducting phases to rather small temperatures. Instead, a strongly coupled diquark liquid prevails in the thermodynamics under the conditions relevant to neutron-star mergers. At lower densities, the diquarks take over from the single-quark contributions, suggesting a pathway toward hadronization. Our results are consistent with observational constraints on the equation of state of neutron stars, corroborating the presence of strongly coupled quark matter in the interior of these objects.

    nucl-thastro-ph.HEcond-mat.quant-gashep-ph0 citations
  46. 46

    Anomalous horizontal track-like events at the HAWC observatory: candidate neutrino-induced charged leptons from the Pico de Orizaba volcano

    Hermes León Vargas🇲🇽 · Andrés Sandoval🇲🇽

    Two track-like events with exceptionally large charge deposits, pointing back to the region of maximum overburden ( km.w.e.) of the Pico de Orizaba volcano, were reported by the HAWC Collaboration in a search for Earth-skimming neutrinos. Using exclusively published information, including the published Monte Carlo charge distributions and the scattered-muon background model, we show that these events are kinematically inconsistent with all identified backgrounds. A conservative energy-conservation bound places the in-tank energy deposit of the candidates above 190--210~GeV, with a worst-case minimum of 122--136~GeV, in either case exceeding the 100~GeV maximum of the scattered-muon background model. Calibration systematics derived from the published simulations act unidirectionally, pushing the implied deposits into the multi-TeV regime. Direct atmospheric muons require ~PeV to penetrate the overburden and contribute expected events ( under the largest possible prompt-charm flux); collinear muon bundles are excluded by five independent arguments. Conversely, the neutrino hypothesis predicts identifiable events precisely in the observed charge window (-- photoelectrons) and in the highest-overburden analysis region, both observed. The two track-like events imply a rate that exceeds the conventional atmospheric neutrino flux expectation at the 2.1--2.5 level. The charges of the observed candidates require an emerging lepton above about 20~TeV; the published calibration does not bound the energy from above. These would constitute the first neutrino candidates detected in Mexico and the first obtained with the Earth-skimming volcano technique.

    astro-ph.HEhep-exhep-ph0 citations
  47. 47

    Primordial black holes and induced gravitational waves from localized features in DBI inflation

    Narges Rashidi🇮🇷

    We investigate primordial black hole formation in a Dirac-Born-Infeld inflationary framework in which the background dynamics are determined by explicit functional forms of the inflaton potential and the warp factor . The background equations are solved numerically to obtain the evolution of the slow-roll parameters. We show that a localized feature in the potential, accompanied by a correlated structure in the warp factor, dynamically induces a transient suppression of the slow-roll parameter, leading to a short-lived non-attractor phase. This behavior generates an enhancement of the curvature power spectrum on small scales, while preserving consistency with CMB-scale observables. The Mukhanov-Sasaki equation is then solved numerically to compute the resulting power spectrum, which exhibits narrow and localized peaks in the PBH abundance across different mass ranges. We also evaluate the associated stochastic background of induced gravitational waves and find that the predicted signal can fall within the sensitivity bands of future pulsar timing arrays and space-based interferometers, depending on the scale of the inflationary feature. A parameter scan in the plane shows that the large-scale predictions remain consistent with current observational constraints.

    astro-ph.COhep-phEPJC(2026)·1 citation
  48. 48

    A Pythia8 Tune for Open Charm and Beauty Production in Fixed-Target Collisions

    Matei Climescu🇧🇪 · Didar Dobur🇧🇪 · Kirill Skovpen🇧🇪

    We present FTFT (Fixed-Target Fragmentation Tune), a set of Pythia8 parameters optimised for the production of charm and beauty hadrons in fixed-target collisions at centre-of-mass energies GeV. Accurate heavy-flavour production in this regime is needed to predict neutrino fluxes and hidden-particle yields at beam-dump experiments such as SHiP. The tune is derived in two stages. First, differential distributions in Feynman- (), transverse momentum squared (), and charge or leading-particle production asymmetry of mesons are fitted to data from pion- and proton-beam fixed-target experiments. Second, -factors for each beam are extracted from inclusive charm cross-section measurements to scale the simulated cross section to the measured data. The fitted charm-fragmentation and multiparton-interaction parameters depart from standard LHC-tuned defaults, in line with earlier fixed-target studies.

    hep-exhep-ph0 citations
  49. 49

    The onset of the strong backreaction regime in axion inflation, an analytical study

    Aditya Kulkarni🇺🇸 · Lorenzo Sorbo🇺🇸

    Models where an axion-like inflaton is coupled to a gauge field are theoretically well motivated and can display a rich phenomenology. The regime in which the quanta of the gauge field strongly backreact on the rolling inflaton has been studied for well more than a decade, and yet we cannot say that it is fully understood. In this paper we present an analytical study of the onset of the strong backreaction regime. Our formalism relies on a Laplace transform to convert a complicated integro-differential equation into the search of the poles of an analytic function. We confirm the existence, previously observed using a completely different formalism, of a stable region of strong backreaction. Our work provides, for the first time, analytical formulae that allow to study the evolution of the system as it transitions from the weak to the strong backreaction regime.

    astro-ph.COhep-phhep-th0 citations
  50. 50

    Local-nuclear-density dependent calculation of nucleon electromagnetic form factor ratios in finite nuclei

    G. Ramalho🇰🇷 · K. Tsushima🇧🇷 · Myung-Ki Cheoun🇰🇷

    We calculate the electromagnetic form factors of nucleons bound in finite nuclei and make predictions to the ratio between the electric () and magnetic () form factors in terms of the square of the four-momentum transfer . We extend our previous constant-density calculations within the covariant spectator-QMC framework by incorporating the spatial nuclear density profiles of finite nuclei and quantify the deviations from the average-density approximation used in our previous applications. The impact of the medium effects can then be observed considering the ratio between and the ratio in free space , that define the proton electromagnetic double ratio associated with a given nucleus. The double ratio is expected to remove some systematic uncertainties. There is the expectation that ratios associated with the bound protons inside the nucleus will be measured in the near future in polarization-transfer experiments . Anticipating future measurements on the subject, we make predictions for the double ratios, to be compared with the average measurements on the energy states of protons bound to nuclei. We consider the nuclei C, O and Ca. We conclude that the form factors calculated using nuclear density profile function are less suppressed than in the case of the results calculated using the average nuclear density. The results indicate that the relative importance of the low-density surface region increases with , leading to a weaker suppression than that predicted by the average-density approximation. We also make predictions for the ratios associated with neutrons bound to nuclei.

    nucl-thhep-exhep-lathep-ph+10 citations
  51. 51

    Latent Geometry and the Emergence of Lorentzian Time in Matrix Quantum Mechanics

    Badis Ydri🇩🇿

    We introduce \emph{latent geometry} in BFSS/BMN models. Before an emergent geometry evaporates at the geometric transition, large- Gaussianization encodes its information in the exceptional sector selected by the baby fuzzy sphere, a single active spin- Pauli block. Dimensional reduction, finite- Gaussianization and exact Molien--Weyl projection transport this encoding to mass-deformed BFSS. At , the same stable BFSS oscillator admits inequivalent unitary and decodings, realizing spacetime transmutation and the emergence of Lorentzian time.

    hep-thgr-qchep-lathep-ph+20 citations
  52. 52

    Searching for Extra Dimensions and Copies of the Standard Model with IceCube

    R. Abbasi🇺🇸 · M. Ackermann🇩🇪 · J. Adams🇳🇿 · J. A. Aguilar🇧🇪 · M. Ahlers🇩🇰 · J.M. Alameddine🇩🇪 · S. Ali🇺🇸 · N. M. Amin🇺🇸 · K. Andeen🇺🇸 · C. Argüelles🇺🇸 · S. Athanasiadou🇩🇪 · S. N. Axani🇺🇸 and 409 other authors

    The hierarchy problem remains an open question in particle physics. A number of theories that address this problem lower the fundamental scale of gravity, resulting in observable consequences in the neutrino sector. In this work, we place constraints on low-scale gravity scenarios using high-energy neutrinos observed with the IceCube Neutrino Observatory. The analysis is based on 10.7 years of upward-going muon neutrino data in the energy range from 0.5 to 100 TeV. In this energy range, the theories predict characteristic spectral distortions arising from matter effects when neutrinos propagate through Earth. In the context of large extra dimension models, we constrain the compactification radius of the largest extra dimension to at confidence level for both normal and inverted neutrino mass ordering. For scenarios with multiple Standard Model copies, we obtain lower limits of up to , depending on the value of the lightest neutrino mass. In parts of the parameter space, these results constitute the strongest constraints in the literature to our knowledge, while in other regions they probe previously unexplored parameter space.

    hep-exhep-ph0 citations
  53. 53

    Examples of Gribov copies in the presence of planar boundaries, and an emergent boundary gauge invariance in Yang-Mills theory

    David Dudal🇧🇪 · Luigi Rosa🇮🇹 · Sebbe Stouten🇧🇪

    First, we explicitly construct zero-modes of the Yang-Mills Faddeev-Popov operator in the presence of two parallel plates, with either perfect electric (PEC) or perfect magnetic (PMC) boundary conditions imposed. This establishes the existence of Gribov copies with finite action, and even finite L_2-norm, in Yang-Mills theory with non-trivial interfaces. We adapt Henyey's construction, although the boundary configuration imposes extra restrictions on the ansatz for the gauge field. Second, we discuss the phenomenon of an emergent boundary gauge invariance for PEC and PMC plates in Yang-Mills theory. This shall be important when applying the Gribov-Zwanziger procedure to parallel plate setups, of relevance for non-perturbatively studying the non-Abelian Casimir effect in the future.

    hep-thhep-lathep-ph0 citations
  54. 54

    Cascades from ultra-high-energy neutrinos

    Gaetano Di Marco🇪🇸 · Rhorry Gauld🇩🇪 · Rafael Alves Batista🇫🇷 · Alfonso García-Soto🇪🇸 · Miguel Á. Sánchez-Conde🇪🇸

    Neutrinos produced at the highest energies can interact with cosmic neutrino and radiation backgrounds during their propagation to Earth. The many available , , and channels can lead to their absorption or energy redistribution, whilst the leptonic and hadronic final states may feed secondary fluxes of neutrinos, protons, and electromagnetic particles through the decay or hadronisation of the heavy leptons, bosons, and quarks produced. We present a framework to characterise these propagation effects in detail, \texttt{propa}, an extension of the CRPropa Monte Carlo code that interfaces with event generators and to dedicated computations of the relevant cross sections. It also treats flavour oscillations in vacuum. Using this code, we investigate sources at high redshifts (), and find a strong absorption of the prompt flux beyond~, although the copious secondary neutrinos partially compensate this depletion, also contributing to the spectrum at lower energies. The framework is designed to study scenarios of cosmological neutrino production beyond~EeV energies such as superheavy dark matter, cosmic strings, and primordial black holes, and to yield reliable predictions for the forthcoming neutrino observatories.

    astro-ph.HEhep-ph0 citations
  55. 55

    NS-UNO: Neutron Star EoS Inference from an Unconstrained Number of Observations

    Valéria Carvalho🇵🇹 · Márcio Ferreira🇵🇹 · Michał Bejger🇵🇱 · Constança Providência🇵🇹

    Future multimessenger observations of neutron stars (NS) are expected to substantially increase both the number and precision of astrophysical constraints on the equation of state (EoS) of dense matter. This motivates inference frameworks capable of accommodating a variable, non fixed number of observations while preserving the posterior information associated with each measurement. In this work, we introduce NS-UNO, a Neural Posterior Estimation framework for NS EoS inference designed to accommodate an Unconstrained Number of Observations (UNO). NS-UNO combines a hierarchical DeepSets model with a conditional normalising flow, enabling a single trained model to perform inference from mass-radius observation sets of varying size, with each observation represented by a set of posterior samples. We demonstrate accurate and well calibrated posterior reconstructions using a model trained jointly on piecewise polytropic and non-parametric Gaussian process EoS ensembles. The reconstruction improves as observations probe a broader range of NS masses, while remaining robust to variations in the number and precision of the observations. The model also generalises to EoSs outside the families used during training. Finally, we qualitatively demonstrate the framework on current multimessenger constraints from NICER and GW170817. NS-UNO provides a flexible and scalable approach to NS EoS inference, naturally suited to the increasingly diverse observational datasets expected from next generation multimessenger astronomy.

    nucl-thastro-ph.HEastro-ph.IMhep-ph0 citations
  56. 56

    at the SU(3)-flavour-symmetric point I: Methodology and strong phase determination

    Matthew Black🇬🇧 · Felix Erben🇨🇭 · Maxwell T. Hansen🇬🇧 · Fabian Joswig🇬🇧 · Nelson Pitanga Lachini🇬🇧 · Rajnandini Mukherjee🇬🇧 · Srijit Paul🇨🇾 · Antonin Portelli🇬🇧

    We present part one of an SU(3)-flavour-symmetric lattice QCD calculation of the amplitude for a -meson decaying to a final state in the 27-dimensional irreducible representation of the flavour symmetry group, denoted . The Wilson--clover gauge ensembles used in this work, generated by the OpenLat collaboration, are tuned such that . Using the distillation framework, we construct a matrix of Euclidean correlation functions from pairs of single-hadron operators projected to definite spatial momentum. Solving a generalised eigenvalue problem yields the finite-volume energy spectrum that is used to determine the scattering phase shift from threshold up to , which sits below but plausibly within reach of . The calculation is performed across three lattice spacings, and we apply two strategies in which the continuum limit is taken at different stages of the computation: (i) on the extracted scattering parameters and (ii) on the finite-volume energies at fixed physical volume before extracting the scattering parameters. We find consistent results across these methods for the scattering phase shift as a function of the centre-of-mass energy, . Taking a scattering-length-only parametrisation, we infer a value for the strong phase of the weak decay, . We further describe the methodology for using the same operator basis to compute three-point correlation functions to extract , for the tree-level effective weak Hamiltonian , and for relating such finite-volume matrix elements to the full decay amplitude. The complete analysis leading to the latter will be presented in a forthcoming manuscript.

    hep-lathep-ph0 citations
  57. 57

    Effects of isospin imbalance on the chiral phase transition within a Chiral Dual Partner Model

    R. M. Aguirre🇦🇷

    The chiral symmetry is a property of the fundamental theory of the strong interaction that is relevant for the hadronic physics. It is expected that at sufficiently high temperature and matter density, this symmetry becomes manifest. Within the Chiral Dual Partner Model the chiral transformation is implemented in such a way that a fermion mass term is allowed if the parity partner of each baryon is included in the framework. This model is used here to study possible manifestations of the chiral symmetry in dense nuclear matter, assuming constant isospin fraction. It is found that the onset of the odd parity baryons is associated with two branches of thermodynamical instabilities, one of them leads to a first order phase transition for temperatures below MeV. An analysis of these instabilities in the phase space is given, and neutron star matter is considered as a special case.

    nucl-thhep-ph0 citations
  58. 58

    Resonant Dynamics of Gravitational Wave and Chiral Alfvén wave in the Early Universe

    Arun Kumar Pandey🇮🇳 · Subalakshmi A · Sampurn Anand🇮🇳

    In this work, we investigate the resonant interaction between stochastic gravitational waves (GWs) and chiral Alfvén waves in a magnetized chiral plasma in the early Universe. Starting from covariant chiral magnetohydrodynamics coupled to linearized gravity, we derive a closed system of equations for the coupled chiral-Alfvén velocity and magnetic-field perturbations. Both analytics and numerics show a parametric resonance at the sum frequency of the two CVE-split branches, with an instability band that widens as the GW strain grows. This CVE-to-Alfvén ratio is not a free parameter. In the early Universe, it is fixed by the Standard Model's relativistic degrees of freedom. Including the plasma's backreaction on the GW makes the energy exchange nonlinear, breaking the usual single-frequency Manley-Rowe picture. For a self-consistent choice of parameters, where backreaction is only a small correction, the unsuppressed resonance still drives the system to a finite-time blow-up within a few Hubble times. We then work out the resonant frequencies and growth rates involved, mapping out what current and future gravitational-wave detectors could observe.

    astro-ph.COgr-qchep-ph0 citations
  59. 59

    First-principles determination of anomaly-induced pion decay beyond the chiral limit

    Tian Lin🇨🇳 · Xu Feng🇨🇳 · Lu-Chang Jin🇺🇸 · Chuan Liu🇨🇳 · Qi-Yuan Luo🇨🇳

    The two-photon decay of the neutral pion is fixed in the chiral limit by the Adler-Bell-Jackiw anomaly, while nonzero quark masses induce few-percent corrections that must be determined for precision tests of QCD beyond the chiral limit. Using the anomalous PCAC relation, we compute them in lattice QCD as deviations from the exact anomaly condition at , thereby avoiding both four-point functions and the cancellation of chiral logarithms that limits conventional approaches. Because the correction is proportional to the light-quark masses, both statistical and systematic uncertainties are correspondingly suppressed, making a precision calculation feasible. On two nearly-physical domain-wall ensembles we achieve statistical precision each for the decay width, obtaining after continuum extrapolation. The mass correction to the decay amplitude, positive and isospin-breaking dominated, provides the first ab initio confirmation of the -- mixing enhancement.

    hep-lathep-exhep-ph0 citations
  60. 60

    Evolution of Cosmic String Loops under Gravitational Backreaction

    Lasse Gerblich🇬🇧 · Richard A. Battye🇬🇧 · E.P.S. Shellard🇬🇧

    Nambu-Goto cosmic string loops generically develop cusps, points where the string momentarily reaches the speed of light. These cusps produce strong gravitational wave bursts with a characteristic strain spectrum , making them prime targets for gravitational wave searches, where is the string mass per unit length. However, this picture is modified when one accounts for gravitational backreaction. Using a convenient gauge, we reformulate the Nambu-Goto equations of motion for a loop moving in its own dynamically sourced gravitational field, enabling the first continuous numerical evolution of loops under this backreaction. A key finding is that locally cusps survive backreaction. Nevertheless, the gravitational waveform calculated in this formalism is significantly modified, weakening the cusp burst and introducing a high-frequency cutoff at . This suppression above reduces the expected signal-to-noise ratio in current and near-future detectors relative to unperturbed waveform predictions.

    gr-qcastro-ph.COhep-ph0 citations

Affiliations

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