PaperPanorama

HEP Phenomenology·hep-ph

Wed·May 28, 2025

40 papers25 primary·15 cross-listed·reconstructed*

  1. 01*

    The role of unitarisation on dark-matter freeze-out via metastable bound states

    Kalliopi Petraki🇫🇷 · Anna Socha🇫🇷 · Christiana Vasilaki🇫🇷

    In many Abelian and non-Abelian theories, standard calculations of radiative bound-state formation violate partial-wave unitarity - even at arbitrarily small couplings - when capture into excited states is considered. Recent work demonstrated that unitarity can be restored by the proper resummation of squared inelastic processes in the self-energy of the incoming state. We examine how unitarisation affects dark-matter thermal decoupling, given that the formation and decay of metastable dark-matter bound states are critical in determining the relic abundance, especially for multi-TeV dark matter. We consider an Abelian model featuring bound-state formation via emission of a light scalar that carries a conserved charge, whose dynamics also emulates relevant aspects of non-Abelian theories. Incorporating capture into excited states, we show that, without proper treatment, unitarity violation is so severe as to prevent freeze-out. Resumming the squared bound-state formation processes restores unitarity and ensures freeze-out, while capture into excited levels still significantly depletes dark matter. We further discuss the impact of higher partial waves, both within and beyond the present model. Finally, we point out the intriguing possibility of late dark-matter decoupling that can affect structure formation.

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

    Searching for Axion Dark Matter Near Relaxing Magnetars

    Sandip Roy🇺🇸 · Anirudh Prabhu🇺🇸 · Christopher Thompson🇨🇦 · Samuel J. Witte🇬🇧 · Carlos Blanco🇺🇸 · Jonathan Zhang🇨🇦

    Axion dark matter passing through the magnetospheres of magnetars can undergo hyper-efficient resonant mixing with low-energy photons, leading to the production of narrow spectral lines that could be detectable on Earth. Since this is a resonant process triggered by the spatial variation in the photon dispersion relation, the luminosity and spectral properties of the emission are highly sensitive to the charge and current densities permeating the magnetosphere. To date, a majority of the studies investigating this phenomenon have assumed a perfectly dipolar magnetic field structure with a near-field plasma distribution fixed to the minimal charge-separated force-free configuration. While this {may} be a reasonable treatment for the closed field lines of conventional radio pulsars, the strong magnetic fields around magnetars are believed to host processes that drive strong deviations from this minimal configuration. In this work, we study how realistic magnetar magnetospheres impact the electromagnetic emission produced from axion dark matter. Specifically, we construct charge and current distributions that are consistent with magnetar observations, and use these to recompute the prospective sensitivity of radio and sub-mm telescopes to axion dark matter. We demonstrate that the two leading models yield vastly different predictions for the frequency and amplitude of the spectral line, indicating systematic uncertainties in the plasma structure are significant. Finally, we discuss various observational signatures that can be used to differentiate the local plasma loading mechanism of an individual magnetar, which will be necessary if there is hope of using such objects to search for axions.

    hep-phastro-ph.HEPRD(2026)·11 citations
  3. 03*

    A new probe of the quartic Higgs self-coupling

    Ulrich Haisch🇩🇪 · Aparna Sankar🇩🇪 · Giulia Zanderighi🇩🇪

    We calculate the corrections to the Higgs wave-function renormalization constant arising from modified cubic, quartic, and quintic Higgs self-couplings up to the two-loop level. Using our analytic results, we derive two-dimensional constraints on the modifications of the considered Higgs self-interactions that could potentially be set from precision measurements of single-Higgs production processes at the high-luminosity Large Hadron Collider (LHC) and a Future Circular Collider. Our novel constraints are compared to those that might be set by searches for multi-Higgs production at the same facilities. In view of the first LHC results on triple-Higgs production, we also review the current status of Higgs self-coupling determinations after LHC Run 2.

    hep-phhep-ex10 citations
  4. 04*

    One-loop renormalization of quark TMD in the light-cone gauge: CSS evolution

    Tolga Altinoluk🇵🇱 · Guillaume Beuf🇵🇱 · Jamal Jalilian-Marian🇺🇸

    We calculate the one-loop corrections to the quark TMD in the light-cone gauge using the background field formalism, with the Mandelstam-Leibbrandt (ML) prescription for the extra singularity present in the light-cone gauge propagator. We use the pure rapidity regulator for rapidity divergences. The Collins-Soper-Sterman (CSS) evolution equations are indeed obtained from the one loop renormalization of the quark TMD. In this setup, the double log contribution to the CSS resummation is found to come from the ghost-like zero-mode from the ML prescription, in the diagrams with a gluon propagator ending on the transverse part of the gauge link at infinity.

    hep-ph5 citations
  5. 05*

    Mapping the transverse spin sum rule in position space

    Cédric Lorcé🇫🇷 · Asmita Mukherjee🇮🇳 · Ravi Singh🇮🇳 · Ho-Yeon Won🇫🇷

    We discuss in detail the relativistic spatial distribution of transverse angular momentum, including both orbital and intrinsic spin contributions. Using the quantum phase-space formalism, we begin with the definition of the three-dimensional spatial distributions of transverse orbital angular momentum and intrinsic spin in a generic Lorentz frame. By integrating these three-dimensional spatial distributions over the longitudinal axis, we derive for the first time the relativistic spatial distributions of transverse orbital angular momentum, intrinsic spin, and total angular momentum for spin-0 and spin-1/2 targets in the transverse plane. We verify the transverse spin sum rule about the relativistic center of spin for spin-0 and spin-1/2 systems, and find that the transverse total angular momentum distribution is non-trivial, even for spin-0 targets. We also show how the distributions of transverse orbital angular momentum, intrinsic spin, and total angular momentum change with the target momentum.

    hep-phhep-thnucl-thPLB(2025)·5 citations
  6. 06*

    Factorial growth in perturbation theory, power corrections: precise extraction of quark masses and

    Andreas S. Kronfeld🇺🇸

    These proceedings summarize a newly found connection between the factorial growth of coefficients in perturbative QCD and power corrections to the perturbation series, discussed in refs. [1-4]. The improved convergence is shown for three quantities four which four terms in the series are available: the static energy, the quark pole mass, and the polarized Bjorken sum rule. Prospects for determinations of with controlled truncation uncertainties are discussed, as was found earlier in quark-mass determinations [3,5].

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

    Study of decays in the improved perturbative QCD formalism

    Xin Liu🇨🇳 · Hsiang-nan Li🇹🇼 · Zhen-Jun Xiao🇨🇳

    Motivated by the recent LHCb measurements of the ratios between the branching ratios (BRs), and , we analyze the decays in the improved perturbative QCD (iPQCD) formalism, where denotes the -wave charmonia with , and denotes the pseudoscalars and (the vectors and ). Our results and at leading order in the strong coupling agree well with the data within uncertainties. The result is lower than inferred by the measurement. The large longitudinal polarization fractions imply that these components dominate the BRs. A peculiar constructive (destructive) interference between the twist-2 and twist-3 contributions is identified in the () mode, but not in the corresponding ones with mesons. Inputting the BRs of the strong decays and reported by the BESIII Collaboration, we obtain those of followed by secondary decay chains under the narrow-width approximation. All the above iPQCD predictions can be confronted by more precise experiments in the future to deepen our understanding of QCD dynamics in transitions.

    hep-phhep-exPRD(2025)·4 citations
  8. 08*

    Form Factors for at NLO in QCD

    Wei Tao🇨🇳 · Ya-Hui Zhao🇨🇳 · Li-Ting Wang🇨🇳 · Qin Chang🇨🇳 · Zhen-Jun Xiao🇨🇳

    We present the Non-Relativistic QCD (NRQCD) calculations at the next-to-leading order (NLO) of for vector, axial-vector, tensor and axial-tensor form factors, and obtain complete analytical expressions for the form factors, along with their asymptotic forms in the hierarchical heavy quark limit. Our results show that the NLO corrections are both sizable and well-behaved in the low squared transfer momentum region. Using the NRQCD + lattice + -series method, we further provide theoretical predictions for form factors across the full physical range. Based on these predicted form factors, we finally compute the decay widths and branching fractions for the semileptonic decays .

    hep-phPRD(2026)·0 citations
  9. 09*

    Electromagnetic tomography of radial flow in the quark-gluon plasma

    Lipei Du🇺🇸 · Ulrich Heinz🇺🇸

    We present a novel multimessenger approach to extract the effective radial flow of the quark-gluon plasma (QGP) by jointly analyzing thermal photon and dilepton spectra in heavy-ion collisions. A key feature of this method is that it circumvents the need for a directly unmeasurable reference -- the photon temperature in the absence of flow -- by establishing, within a calibrated model framework, a stable, approximately linear correlation with the dilepton-inferred temperature. This construction defines an experimentally constructible quantity, , which reflects early-time collectivity and exhibits a strong correlation with the spacetime-averaged radial velocity of the QGP. Together with previous results linking dilepton slopes to the initial QGP temperature, our work establishes a consistent framework for electromagnetic tomography of the QGP. Our framework quantifies the experimental precision target, thereby providing a concrete roadmap for future measurements at RHIC and the LHC and opening a new avenue to probe the early-time dynamics of hot QCD matter.

    hep-phnucl-exnucl-thPRL(2026)·6 citations
  10. 10*

    Probing lepton number violating SMEFT operators at the same-sign muon collider

    Subhaditya Bhattacharya🇮🇳 · Soumyajit Datta🇮🇳 · Abhik Sarkar🇮🇳

    We investigate lepton number violation (LNV) induced by dimension-seven Standard Model Effective Field Theory (SMEFT) operators in the context of same-sign muon colliders. Specifically, we study production at the TRISTAN at 2 TeV with an integrated luminosity of 1 ab, using the final-state signature comprising two fat jets. This process is sensitive to eight distinct SMEFT operators, providing a unique avenue for testing LNV beyond the Standard Model. We determine the maximal sensitivity to these operators and compare our results with existing LHC constraints and future projections from the FCC. Our findings highlight the potential of same-sign muon colliders to serve as powerful probes of LNV and New Physics (NP) at the TeV scale.

    hep-phhep-exPRD(2026)·7 citations
  11. 11*

    Semileptonic decay of double strangeness heavy flavor baryons

    Hui-Hui Duan🇨🇳 · Yong-Lu Liu🇨🇳 · Qin Chang🇨🇳 · Ming-Qiu Huang🇨🇳

    This paper investigates the double strangeness heavy flavor baryons and , which contain two strange quarks. Using QCD light-cone sum rules (LCSRs), we calculate the form factors for the Cabibbo-suppressed processes and , corresponding to the heavy-quark transitions and , respectively. Combining these with the helicity amplitude formalism for semileptonic decay differential widths, we computed the branching fractions of their corresponding semileptonic decay processes. Our analysis reveals significant discrepancies between two versions of QCD LCSRs: one using the light-cone distribution amplitudes (LCDAs) of the final-state baryon and the other using the LCDAs of the initial-state double strangeness heavy flavor baryons. The results obtained with the baryon's LCDAs show excellent agreement with other theoretical calculations. However, when using the LCDAs of the double strangeness heavy flavor baryons, the results differ by orders of magnitude, warranting further investigation.

    hep-phPRD(2025)·2 citations
  12. 12*

    On chirality and chiral neutrino oscillations

    Evgeny Akhmedov🇩🇪

    It has been claimed in a number of publications that neutrinos can exhibit chirality oscillations. In this note we discuss the notion of chirality and show that chiral neutrino oscillations in vacuum do not occur. We argue that the incorrect claims to the contrary resulted from a failure to clearly discriminate between quantum fields, states and wave functions. We also emphasize the role played in the erroneous claims on the possibility of chirality oscillations by the widely spread misconceptions about negative energies.

    hep-phhep-exnucl-ex4 citations
  13. 13*

    Entanglement Negativity of Spin-Orbit Correlations in a general Qubit-Qudit Setup

    Sanskriti Agrawal🇮🇳 · Raktim Abir🇮🇳

    We present the complete eigenvalue spectrum of the partially transposed density matrix for a pure bipartite quantum state acting on a generic Hilbert space. The spectrum contains four non-zero eigenvalues, as, \begin{eqnarray} \lambda_{1,2}=\pm \sqrt{A}, ~~~ \lambda_{3,4}= \frac{1}{2}(1\pm\sqrt{1-4 A}), \nonumber \end{eqnarray} where is the determinant of the reduced density matrix (traced over the larger subspace). As , only one is negative among the four non-trivial eigenvalues. Within this qubit-qudit framework, we further studied the negativity as a measure of entanglement for the case of spin-orbit correlation of partons inside a proton. The entanglement negativity for spin-orbit correlations is found to be related to the gluon helicity PDF and the Hermitian angle of the associated Hilbert space for linearly polarized protons.

    hep-phnucl-thquant-phPLB(2025)·6 citations
  14. 14*

    Portraits of Charmoniumlike States

    Qingyang Liu🇨🇳 · Xiangyu Jiang🇨🇳 · Ying Chen🇨🇳 · Chunjiang Shi🇨🇳 · Wei Sun🇨🇳

    The charm quark density-density correlation is calculated for and conventional charmonia and charmoniumlike states from lattice QCD and are interpreted as spatial wave functions of these states with some approximations. The angular distributions of in conventional charmonia are found to be in accordance with the expectation of two-body systems, while that of the state exhibits an -wave feature. However, the radial distributions turn out to be strikingly different from the non-relativistic quark model and can be understood by the Dirac theory of two-body bound states. These results provide the first gauge invariant and model-independent three-dimensional portraits of charmonium(like) states.

    hep-phhep-lat1 citation
  15. 15*

    Some identities which involve Stirling numbers

    Stefano Frixione🇮🇹

    During the course of an ongoing work on the small- behaviour of parton distribution functions, some identities have been found which involve Stirling numbers of the first and the second kind, as well as binomial coefficients. Without any claim of originality I report them in this note.

    hep-phmath.NT0 citations
  16. 16*

    Prominent enhancement of axion thermalization rate from axion-kaon interactions

    Jin-Bao Wang🇨🇳 · Zhi-Hui Guo🇨🇳 · Hai-Qing Zhou🇨🇳

    The axion thermalization rate is a crucial input to determine the hot dark matter bound of axions, resulting from the scattering processes in the thermal bath of early Universe. We demonstrate that the commonly employed axion thermalization rate by including the channel alone is significantly underestimated for the temperature above 100 MeV. This is obtained through the systematical calculation of the axion-light flavor meson scattering amplitudes within the framework of the chiral unitarization approach, paying special attention to the reaction. Hadron resonances appearing in amplitudes significantly enlarge the cross sections, which turn out to be much bigger than that of . The axion thermalization rate is then substantially enhanced by the channel for MeV. Especially at MeV, the contribution from the reaction to the axion thermalization rate exceeds the one. Obviously more stringent constraints on the axion parameters are obtained, when confronting the number of extra relativistic degrees of freedom from Planck18.

    hep-phPRD(2025)·2 citations
  17. 17*

    On the equivalence of Flavor SU(3) analyses of decays

    Yu-Ji Shi🇨🇳 · Wei Wang🇨🇳 · Ji Xu🇨🇳

    We conduct an SU(3) analysis of decays based on reduced matrix elements (RMEs), with being a light pseudoscalar meson excluding . We show that a complete basis for the decays consists of ten RMEs, where the three RMEs arise from the electroweak penguin operators . In the Standard Model, the relevant Wilson coefficients are small and thus can be neglected. We further demonstrate the equivalence of the RME approach with the irreducible representation amplitude (IRA) and topological diagram amplitude (TDA) methods, and derive relations between the ten RME amplitudes and corresponding IRA/TDA amplitudes. These relations lay a foundation for consistent SU(3) analyses of heavy meson decays.

    hep-phEPJC(2025)·5 citations
  18. 18*

    Hyperbolic recoil and the Unruh effect at CERN-NA63

    Morgan H. Lynch🇩🇪

    In this manuscript we examine the high energy channeling radiation data sets from the CERN-NA63 experiment using ultra relativistic synchrotron emission. To incorporate recoil, we examine the standard quasi-classical formalism as well as develop a formalism which includes the Unruh effect by utilizing a hyperbolic recoil acceleration, based on conservation of momentum, in the classical synchrotron trajectory. We also perform an asymptotic radiation time scale analysis which predicts a photon energy threshold, beyond which the Unruh effect dominates. We then compare the classical, quasi-classical, and Unruh synchrotron theories to the data. We find that above threshold, the Unruh effect saturates the spectrum of all data sets.

    hep-phgr-qcPRD(2025)·2 citations
  19. 19*

    Concurrent Exploration of Axion-Like Particle Interactions with Gauge Bosons at the LHC

    Shirin Chenarani🇮🇷 · Mojtaba Mohammadi Najafabadi🇮🇷

    Axion-like particles (ALPs) are pseudo Nambu-Goldstone bosons associated with spontaneously broken global symmetries incorporated in the Standard Model (SM) Lagrangian in many models beyond the SM. The existence of a light ALP is plausible due to the long-standing problems that the SM has not been able to address, such as the dark matter (DM) problem and the observed matter-antimatter asymmetry. There are many proposals in recent decades considering the ALP as a solution to some of these shortcomings. Motivated by such potential, we search for ALPs with a mass of 1 MeV at the LHC in a model-independent fashion. We explore two complementary production modes: ALP production in association with a pair of electroweak gauge bosons ( or ) and ALP production in association with a single gauge boson ( or ) plus jets. For the final state, signal and dominant SM backgrounds are generated, and a realistic detector response simulation is performed. A multivariate analysis is employed to discriminate the signal from background processes, and the expected confidence level (CL) exclusion limits in two-dimensional parameter spaces involving the ALP couplings are subsequently derived. The +jets channel is interpreted using LHC measurements in regimes where the ALP escapes detection, appearing as missing energy. The two analyses are complementary: both the and the +jets channels probe simultaneously the ALP couplings to gluons and to electroweak gauge bosons. While the channel offers clean multi-lepton final states and direct reconstruction of the or system, the +jets channel benefits from larger production cross sections, enabling stronger constraints in certain regions of the parameter space.

    hep-phNPB(2025)·3 citations
  20. 20*

    Charmed baryon decays into light scalar mesons in the topological framework

    Y. L. Wang🇨🇳 · Y. K. Hsiao🇨🇳

    Using the topological-diagram approach based on flavor symmetry, we investigate two-body decays, where denotes the final-state baryon and refers to a light scalar meson, such as , , , or . Our analysis indicates that interpreting the light scalar mesons as tetraquark states provides a more consistent description of the currently available experimental data. In particular, this framework naturally accommodates the experimentally observed branching fraction , which exceeds predictions based solely on long-distance effects by an order of magnitude. Within the tetraquark scenario, we predict and . Owing to mixing, and are suppressed to the levels of and , respectively. These modes therefore provide sensitive probes of the internal structure of the light scalar mesons. More generally, the remaining branching ratios of are found to be comparable to those of , where denotes a pseudoscalar meson. Their predicted sizes suggest that these decay modes should be accessible to ongoing and near-future experimental studies at BESIII, Belle II, and LHCb.

    hep-phhep-exJHEP(2026)·3 citations
  21. 21*

    Automation of a Matching On-Shell Calculator

    Javier López Miras🇪🇸 · Fuensanta Vilches🇪🇸

    We introduce , a package designed to facilitate on-shell calculations in effective field theories (EFTs). This initial release focuses on the reduction of Green's bases to physical bases, as well as transformations between arbitrary operator bases. The core of the package is based on a diagrammatic on-shell matching procedure, grounded in the equivalence of physical observables derived from both redundant and non-redundant Lagrangians. offers a complete set of tools for performing basis transformations, diagram isomorphism detection, numerical substitution of kinematic configurations, and symbolic manipulation of algebraic expressions. Planned future developments include extension to one-loop computations, thus providing support for EFT renormalization directly in a physical basis and automated computation of one-loop finite matching, including contributions from evanescent operators. The package, along with example notebooks and documentation, is available at: https://gitlab.com/matchingonshell/mosca.

    hep-phhep-thComput.Phys.Commun.(2026)·13 citations
  22. 22*

    decays assisted by QCD light-cone sum rules

    Anshika Bansal🇩🇪 · Alexander Khodjamirian🇩🇪 · Thomas Mannel🇩🇪

    We suggest a new method to analyse the rare decays (), combining QCD light-cone sum rules (LCSR) with hadronic dispersion relations. As our main study case, we consider the mode which attracts much of interest from the point of view of GIM cancellation and potential new sources of the FCNC transitions. The hadronic amplitude of this decay is dominated by the combination of weak annihilation with the emission of a virtual photon. This amplitude is calculated at spacelike photon virtualities, , using LCSR with pion distribution amplitudes. The LCSR results are then fitted to the hadronic dispersion relation in the variable . The fit allows us to determine relative phases of the -,- and -meson terms and to estimate the contributions of heavier hadronic states. The latter are parameterized in two different ways: first, with a -expansion and second, using a model with excited vector-meson resonances. The resulting width obtained from the LCSR-assisted dispersion relation is not much smaller than the current upper bound measured by LHCb collaboration. In comparison with our result for the dominant transition, the contribution induced by the short distance quark transition generated by the effective operator in Standard Model turns out to be practically invisible. To detect its effect, one readily needs a enhancement of the coefficient from non-standard effects by many orders of magnitude. We also establish new -spin symmetry relations between the amplitudes of decays and apply our method to the Cabibbo-favoured modes and which proceed via the same weak annihilation mechanism.

    hep-phhep-exJHEP(2025)·3 citations
  23. 23*

    The reaction, and a triangle singularity producing the state

    Yi-Yao Li🇨🇳 · Jing Song🇨🇳 · Eulogio Oset🇪🇸 · Wei-Hong Liang🇨🇳 · Raquel Molina🇪🇸

    We study the decay , focusing on the production of the resonance observed by the Belle Collaboration. Interpreted as a dynamically generated state from meson-baryon interactions in the chiral unitary approach, the signal is shown to be enhanced by a triangle singularity involving intermediate , , and states. This mechanism leads to a sharp peak near 1434 MeV in the invariant mass distribution, in agreement with the experimental observations, and predicts a secondary peak around 1875 MeV in the spectrum tied to the triangle singularity. We also estimate the branching ratio of to be about . The results for the branching ratio and the mass distributions are predictions of the theoretical approach, which could be tested with reanalysis of existing data.

    hep-phEPJC(2025)·5 citations
  24. 24*

    Modular-symmetry-protected seesaw

    A. Granelli🇮🇹 · D. Meloni🇮🇹 · M. Parriciatu🇮🇹 · J. T. Penedo🇮🇹 · S. T. Petcov🇮🇹

    In the presence of a finite modular flavour symmetry, fermion mass hierarchies may be generated by a slight deviation of the modulus from a symmetric point. We point out that this small parameter governing charged-lepton mass hierarchies may also be responsible for the breaking of lepton number in a symmetry-protected low-scale seesaw, sourcing active neutrino masses and the mass splitting of a pseudo-Dirac pair of heavy neutrinos. We discuss the phenomenological implications of this mechanism, including the possibility to test the considered models at future planned and proposed heavy neutral lepton searches.

    hep-phJHEP(2025)·10 citations
  25. 25*

    The anomalous magnetic moment of the muon in the Standard Model: an update

    R. Aliberti🇩🇪 · T. Aoyama🇯🇵 · E. Balzani🇮🇹 · A. Bashir🇲🇽 · G. Benton🇺🇸 · J. Bijnens🇸🇪 · V. Biloshytskyi🇩🇪 · T. Blum🇺🇸 · D. Boito🇧🇷 · M. Bruno🇮🇹 · E. Budassi🇮🇹 · S. Burri🇨🇭 and 223 other authors

    We present the current Standard Model (SM) prediction for the muon anomalous magnetic moment, , updating the first White Paper (WP20) [1]. The pure QED and electroweak contributions have been further consolidated, while hadronic contributions continue to be responsible for the bulk of the uncertainty of the SM prediction. Significant progress has been achieved in the hadronic light-by-light scattering contribution using both the data-driven dispersive approach as well as lattice-QCD calculations, leading to a reduction of the uncertainty by almost a factor of two. The most important development since WP20 is the change in the estimate of the leading-order hadronic-vacuum-polarization (LO HVP) contribution. A new measurement of the cross section by CMD-3 has increased the tensions among data-driven dispersive evaluations of the LO HVP contribution to a level that makes it impossible to combine the results in a meaningful way. At the same time, the attainable precision of lattice-QCD calculations has increased substantially and allows for a consolidated lattice-QCD average of the LO HVP contribution with a precision of about 0.9%. Adopting the latter in this update has resulted in a major upward shift of the total SM prediction, which now reads (530 ppb). When compared against the current experimental average based on the E821 experiment and runs 1-6 of E989 at Fermilab, one finds , which implies that there is no tension between the SM and experiment at the current level of precision. The final precision of E989 (127 ppb) is the target of future efforts by the Theory Initiative. The resolution of the tensions among data-driven dispersive evaluations of the LO HVP contribution will be a key element in this endeavor.

    hep-phhep-exhep-latnucl-ex+1Phys.Rept.(2025)·354 citations
  26. 26*

    Constraints on the symmetric mass generation paradigm for lattice chiral gauge theories

    Maarten Golterman🇺🇸 · Yigal Shamir🇮🇱

    Within the symmetric mass generation (SMG) approach to the construction of lattice chiral gauge theories, one attempts to use interactions to render mirror fermions massive without symmetry breaking, thus obtaining the desired chiral massless spectrum. If successful, the gauge field can be turned on, and thus a chiral gauge theory can be constructed in the phase in which SMG takes place. In this paper we argue that the zeros that often replace the mirror poles of fermion two-point functions in an SMG phase should be ``kinematical'' singularities. We conjecture that the SMG interactions generate opposite-chirality bound states, which combine with the gapped elementary mirror states to form massive Dirac fermions. The propagator zeros can then be avoided by choosing an appropriate set of interpolating fields that contains both elementary and composite fields. This allows us to apply general constraints on the existence of a chiral fermion spectrum which are valid in the presence of (non-gauge) interactions of arbitrary strength, including in any SMG phase. Using a suitably constructed one-particle lattice hamiltonian describing the fermion spectrum, we formulate a generalized no-go theorem which establishes the conditions for the applicability of the Nielsen-Ninomiya theorem to this hamiltonian. If these conditions are satisfied, the massless fermion spectrum must be vector-like. We add some general observations on the strong coupling limit of SMG models. We also elaborate on the qualitative differences between four-dimensional and two-dimensional theories that limit the lessons that can be drawn from two-dimensional models. Finally, we compile a list of open questions which must be addressed in any SMG model in order to determine whether or not it is subject to the generalized no-go theorem.

    hep-latcond-mat.str-elhep-phhep-thPRD(2026)·7 citations
  27. 27*

    Exploring the Structural Properties of Anisotropic Dark Matter-Admixed Quark Stars

    G. Panotopoulos🇨🇱 · A. Rincón🇪🇸 · I. Lopes🇵🇹

    We investigate anisotropic compact stars comprising two non-interacting fluids: quark matter and condensed dark matter. Using the MIT Bag model equation of state for quark matter and Bose-Einstein Condensate equation of state for dark matter, we numerically compute interior solutions for those two-fluid component spherical configurations. Varying the initial central density ratio of dark matter to quark matter, we examine how different proportions of these components influence the mass-radius profile, the factor of compactness as well as the quark mass fraction. Recent studies suggest that quark matter may exist in the cores of massive neutron stars, significantly affecting their structure and stability. We calculate the factor of compactness for both negative and positive anisotropy cases explored in this article. Our findings demonstrate that dark matter-admixed quark stars are more compact yet less massive compared to pure quark matter stars, aligning with recent theoretical predictions and gravitational wave observations.

    gr-qcastro-ph.HEastro-ph.SRhep-phPhys.Dark Univ.(2025)·9 citations
  28. 28*

    Strong coupling and instabilities in singularity-free inflation from an infinite sum of curvature corrections

    Shinji Tsujikawa🇯🇵

    Four-dimensional gravitational theories derived from an infinite sum of Lovelock curvature invariants, combined with a conformal rescaling of the metric, are equivalent to a subclass of shift-symmetric Horndeski theories that possess a single scalar degree of freedom. Under the assumption of a homogeneous and isotropic cosmological background, the theory admits an inflationary solution that replaces the Big Bang singularity. This can be achieved by a solution where the Hubble expansion rate is equal to the time derivative of the scalar field . We show that the solution suffers from a strong coupling problem, characterized by the vanishing kinetic term of linear scalar perturbations at all times. Consequently, nonlinear scalar perturbations remain uncontrolled from the onset of inflation throughout the subsequent cosmological evolution. Moreover, tensor perturbations are generally subject to Laplacian instabilities during inflation. This instability in the tensor sector also persists under background initial conditions where . In the latter case, both the coefficient of the kinetic term for scalar perturbations and the scalar sound speed diverge at the onset of inflation. Thus, the dominance of inhomogeneities in this theory renders the homogeneous background solution illegitimate.

    gr-qcastro-ph.COhep-phhep-thPRD(2025)·4 citations
  29. 29*

    Inflationary power spectrum from the Lanczos algorithm

    Ke-Hong Zhai🇨🇳 · Lei-Hua Liu🇨🇳 · Hai-Qing Zhang🇨🇳

    The generalized Lanczos algorithm can provide a universal method for constructing the wave function under the group structure of Hamiltonian. Based on this fact, we obtain an open two-mode squeezed state as the quantum origin for the curvature perturbation. In light of this wave function in the open system, we successfully develop a new method to calculate its corresponding power spectrum by using the Bogoliubov transformation. Unlike traditional approaches, we explicitly retain the Bogoliubov coefficients in terms of the squeezing amplitude \( r_k \) and the squeezing rotation angle \( \phi_k \). As a result, the power spectrum of the open two-mode squeezed state will match that of the Bunch-Davies vacuum numerically. Furthermore, the derivation of the open two-mode squeezed state relies on the second kind Meixner polynomial (equivalent to the generalized Lanczos algorithm) and the symmetry of the Hamiltonian. Therefore, our research may offer a new insight into the calculation of the correlation functions through a group-theoretic perspective.

    quant-phastro-ph.COgr-qchep-ph+1EPJC(2025)·11 citations
  30. 30*

    Integrable Non-Holonomic Constraints and Gauge Fixing in Classical Field Theory

    Ben Bert🇿🇦 · William A. Horowitz🇿🇦

    We re-examine the derivation of the equations of motion from an action principle for classical field theories with non-holonomic constraints, \textit{i.e.}, constraints involving derivatives of the fields. We find that the usual method for gauge fixing in classical and quantum field theories is highly non-trivial for non-holonomic gauge constraints, such as the Coulomb and Lorenz gauges. The subtlety appears at the use of the so-called transposition rule, , which has been shown not to hold for general non-holonomic constraints in the point-particle context. We provide a sufficient definition of integrable non-holonomic constraints in classical field theory that allows us to prove that the transposition rule holds for all theories with these constraints; we are then able to recover the usual treatment of gauge fixing for gauges of this type.

    hep-thhep-phmath-phmath.MP+11 citation
  31. 31*

    Magnetically arrested transmutation of a compact star

    H. A. Adarsha (MCNS, India) · Chandrachur Chakraborty (MCNS, India)🇮🇳 · Sudip Bhattacharyya (TIFR, India)🇮🇳

    We introduce a novel mechanism -- Magnetically Arrested Transmutation (MAT) -- which could be a viable model to account for the observed over-representation of magnetic white dwarfs (WDs) near the Galactic centre (GC), and the presence of a magnetar as opposed to the absence of ordinary pulsars in the same region. In this scenario, compact stars accumulate asymmetric or non-self-annihilating dark matter particles, eventually forming an endoparasitic black hole (EBH) of initial mass at their core. Although such EBHs generally grow by accreting host matter, we show that sufficiently strong core magnetic fields can establish pressure equilibrium, thereby stalling further accretion and halting the star's transmutation into a black hole. We derive the conditions for this MAT to occur, identifying a critical parameter , that encapsulates the interplay between the magnetic field strength, host matter density, and EBH mass. For , the growth of the EBH is arrested, limiting its final mass () to , whereas for , full transmutation may ensue. We argue that highly magnetized WDs may survive near the GC due to the MAT mechanism, as do high-spin ordinary WDs, despite hosting a central EBH. We also speculate a possibility that the magnetar PSR J1745-2900 survives near the GC due to the MAT mechanism. Overall, the MAT framework may explain an elevated population of magnetic WDs in dense dark matter environments, and hence could be tested and should have implications for understanding dark matter and compact objects.

    astro-ph.HEastro-ph.COgr-qchep-ph+1EPJC(2026)·5 citations
  32. 32*

    Slowly Rotating and Tidal Deformation of Nonlocal Modified Tolman VII Star

    Byon N. Jayawiguna · Piyabut Burikham🇹🇭

    We investigate the moment of inertia, quadrupole deformation, and tidal deformation within the framework of nonlocal gravity, utilizing the exact modified Tolman-VII (NEMTVII) density model with an isotropic perfect fluid. The Love number~ is derived using standard even-parity perturbation theory. Additionally, we explore the observational implications by analyzing the tidal deformability parameter~ in comparison with the constraints from GW170817, GW190425, PSR J0348+0432, and PSR J0740+6620. We found that the results are consistent with the tidal constraint when with the small . For slowly rotating object, the dimensionless moment of inertia~, rotational Love parameter~, and quadrupole moment~ are fully determined by the perturbed metric. Our findings reveal that the nonlocal parameter~ significantly affects the star radius. For a fixed and varying , the -Love- relations are found to be universal. For varying , the -Love- relations become non-universal.

    gr-qchep-phJCAP(2025)·1 citation
  33. 33*

    Parameter inference of millilensed gravitational waves using neural spline flows

    Zheng Qin🇨🇳 · Tian-Yang Sun🇺🇸 · Bo-Yuan Li🇺🇸 · Jing-Fei Zhang🇺🇸 · Xiao Guo🇨🇳 · Xin Zhang🇺🇸

    When gravitational waves (GWs) propagate near massive objects, they undergo gravitational lensing that imprints lens model dependent modulations on the waveform. This effect provides a powerful tool for cosmological and astrophysical studies. Due to the added parameters of lenses and the uncertainty of lens models, parameter inference for lensed GW events using traditional methods is extremely time-consuming, thus requiring more efficient parameter inference methods. In this work, we explore the use of neural spline flows (NSFs) for posterior inference of millilensed GWs, and successfully apply NSFs to the inference of 11-dimensional lens parameters. Our results demonstrate that compared with traditional methods like Bilby dynesty that rely on Bayesian inference, the NSF network we built not only achieves inference accuracy comparable to traditional methods for most parameters, but also can reduce the inference time from approximately 3 days to 0.8 s on average. Additionally, the network exhibits strong generalization for the spin parameters of GW sources. It is anticipated to become a powerful tool for future low-latency searches for lensed GW signals.

    gr-qcastro-ph.COastro-ph.IMhep-ph+1PRD(2026)·10 citations
  34. 34*

    Polaron formation as the vertex function problem: From Dyck's paths to self-energy Feynman diagrams

    Tomislav Miškić🇭🇷 · Juraj Krsnik🇭🇷 · Stefano Ragni🇭🇷 · Andrey S. Mishchenko🇭🇷 · Osor S. Barišić🇭🇷

    We present an iterative method for generating the complete set of self-energy Feynman diagrams at arbitrary order for the single-polaron problem with arbitrary linear coupling to the lattice. The approach combines a combinatorial representation of noncrossing diagrams, based on Dyck paths associated with Stieltjes-Rogers polynomials, with the constraints of the Ward-Takahashi identity to systematically incorporate vertex corrections. This construction yields a one-to-one correspondence between terms in the expansion based on Stieltjes-Rogers polynomials and diagrammatic contributions, and provides, through a sequence of simple steps, a closed, algorithmic framework for generating all diagrams of a given order, together with their relative weights. The method enables efficient, unbiased evaluation of diagrammatic series and improves the convergence of diagrammatic Monte Carlo by eliminating the need for stochastic weighting between different topologies. We further outline how the construction can be generalized to finite-density electron systems.

    cond-mat.str-elhep-phSciPost Phys.(2026)·1 citation
  35. 35*

    Dyons in higher-dimensional gauge theories

    Yuki Adachi🇯🇵 · C.S. Lim🇯🇵 · Nobuhito Maru🇯🇵

    We discuss the 't Hooft-Polyakov (TP) monopole and then dyon in the framework of higher dimensional gauge theories, such as gauge-Higgs unification models. First, we point out that the Bogomol'nyi-Prasad-Sommerfield (BPS) monopole is nothing but a self-dual gauge field in the 4-dimensional (4D) space including the extra dimension, which is argued to lead to a consequence that the mass of the BPS monopole and therefore the vacuum expectation value (VEV) of the Higgs field are topologically quantized. In literatures, there exist related arguments on the calorons, which may be understood to be a composition of a pair of constituent monopole and anti-monopole, with each constituent carrying fractional topological charge, while the net topological charge carried by the caloron is unity. From the viewpoint of the caloron, our conclusion of the quantized monopole mass corresponds to the special case, where only a single monopole exists that carries the net topological charge. Next, the argument is generalized to the case of dyon. The mass of the BPS dyon, , is still proportional to the quantized Higgs VEV, though it also depends on a parameter , denoting the ratio of the electric and magnetic charges of the dyon. In the 5D gauge theories the Chern-Simons term is induced at the quantum level, which, after the extra space component of the gauge field is replaced by its VEV, produces the term. Then, through the Witten effect we reach to an interesting conclusion that the parameter and therefore are discretized. In addition, we propose a numerical method to obtain the field configurations and the mass of the non-BPS dyons by use of ``modified" gradient flow equations.

    hep-thhep-phPRD(2025)·0 citations
  36. 36*

    What triggers type Ia supernovae: Prompt detonations from primordial black holes or companion stars?

    Heinrich Steigerwald

    We set up and perform collision rate simulations between dark matter in the form of asteroid-mass primordial black holes (PBHs) and white dwarf stars. These encounters trigger prompt detonations and could be the key to solving the ignition mystery of type Ia supernovae. Our framework is flexible enough to cover the full range of progenitor white dwarf masses, host galaxy stellar masses, galactocentric radial offsets, and cosmic time. The rate distribution pattern is consistent with exhaustive literature observational determinations for a slightly extended log-normal PBH mass spectrum. Most strikingly, the so far unexplained brightness distribution comes out without finetuning. We find no severe contradictions, except that the inferred PBH mass scale is unpredicted from first principles.

    astro-ph.COastro-ph.HEgr-qchep-ph+1PRD(2025)·1 citation
  37. 37*

    Dark-matter-induced transients over cosmic time: The role of star formation history profiles

    Heinrich Steigerwald

    The dark matter (DM) conundrum is one of the most intriguing due to its resistance in direct detection experiments. In recent years, attempts to identify non-gravitational signatures as the result of DM traversing or accumulating within stars have attracted a lot of attention. These calculations are usually evaluated at the order-of-magnitude level for stellar populations where the DM density is highest, such as galactic centers. However, if the signature implies the destruction of the host star, their population could have been diminished over a Hubble time in the most DM-dense regions, unless replenished by star formation. This circumstance exemplifies the need for galactic star formation history profiles when deriving DM-induced transient rates, in particular for predicting the host-offset distribution. Here, we combine theoretical and empirical scaling relations of galaxy structure, star formation, and stellar initial mass function to construct a simple and efficient framework that permits us to estimate the target population formation rate and mass function within galactocentric radial zones across galaxy stellar masses and cosmic time. In a companion paper, we apply the framework to the hypothesis that DM in the form of primordial black holes accounts for the ignition of normal type Ia supernovae when colliding with white dwarf stars.

    astro-ph.GAastro-ph.COastro-ph.HEhep-ph+1PRD(2025)·1 citation
  38. 38*

    Generalized Collective Coordinate Quantization of Solitons with Topological Terms

    Taichi Tsukamoto🇯🇵

    We show that the pentaquark does not exist in the Skyrme model. For the solitons of the theory with topological terms, the standard collective coordinate quantization does not construct the proper low energy effective theory. In the presence of topological terms, zero modes are classified into three groups: dynamical zero modes with constant velocity, cyclotron zero modes in a circular orbit, and static constraint zero modes. According to the mode expansion, the topological term contributes to the moduli metric of the dynamical zero modes. In addition, constraint zero modes do not have the kinetic term and produce constraints that strongly restrict the spectrum instead. In this paper, we propose a generalized collective coordinate quantization method and apply it to the SU(3) Skyrmion with the Wess- Zumino-Witten term. We find five constraints. These reproduce the results of [1], eliminating all the SU(3) multiplets except the nucleon octet and baryon decuplet from the baryon spectrum.

    hep-thhep-phPRD(2026)·0 citations
  39. 39*

    Non-minimal light-curvature couplings and black-hole imaging

    Raúl Carballo-Rubio🇪🇸 · Héloïse Delaporte🇩🇰 · Astrid Eichhorn🇩🇪 · Pedro G. S. Fernandes🇩🇪

    Non-minimal couplings between the electromagnetic field strength and the spacetime curvature are part of the effective field theory of gravity and matter. They alter the local propagation of light in a significant way if the ratio of spacetime curvature to the non-minimal coupling is of order one. Spacetime curvature can become appreciable around black holes, and yet the effect of non-minimal couplings on electromagnetic observations of black holes remains underexplored. A particular feature of the non-minimal coupling between the electromagnetic field-strength and the Riemann tensor is that it generates two distinct photon rings for different polarizations. Working within the paradigm of lensing bands and focusing on the lensing band, we illustrate by which diagnostics a modified light propagation may be distinguished from a modified spacetime geometry and how constraints on the value of the non-minimal coupling can be obtained

    astro-ph.HEgr-qchep-phPRD(2025)·7 citations
  40. 40*

    5-Dimensional Gravitational Raman Scattering: Scalar Wave Perturbations in Schwarzschild-Tangherlini Spacetime

    Samim Akhtar🇮🇳 · Yilber Fabian Bautista🇫🇷 · Cristoforo Iossa🇨🇭 · Zihan Zhou🇺🇸

    In this Letter, we study scalar wave perturbations of arbitrary frequency to the 5D Schwarzschild-Tangherlini black hole (STBH) within general relativity. For the first time, we derive a closed formula for the 5D partial wave gravitational Raman scattering amplitude applicable to a broad class of boundary conditions, expressed in terms of the Nekrasov-Shatashvili (NS) function for the reduced confluent Heun problem. Furthermore, up to we compute the dynamical , and the static , scalar tidal Love numbers of the STBH by matching an effective field theory description for a scalar wave scattering off the black hole, to our novel ultraviolet-NS solutions. The matched Love numbers do not vanish and present renormalization group running behavior.

    hep-thastro-ph.HEgr-qchep-phPRD(2025)·12 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.