PaperPanorama

HEP Phenomenology·hep-ph

Thu·Feb 20, 2025

20 papers12 primary·8 cross-listed·reconstructed*

  1. 01*

    Charge-changing weak interactions for right-handed particles in the Standard Model

    J.D. Franson🇺🇸

    Experiments have shown that the charge-changing weak interaction is purely left-handed, which is taken into account in the Standard Model by the inclusion of a left-handed projection operator in the Lagrangian. Nevertheless, it will be shown here that the Standard Model predicts charge-changing weak interactions for right-handed fermions that can be larger than those for left-handed fermions if the mass is sufficiently large, as is the case for the top quark. Here we are using the conventional terminology in which a massive fermion with its spin parallel to its momentum is referred to as being right-handed in the relativistic limit, where it is in an approximate eigenstate of the chirality operator. These effects are due to the way in which the field of the W boson is quantized, which gives a divergent tensor product in the Feynman propagator in the unitary gauge. It will be shown that the off-diagonal terms in the propagator can convert a left-handed projection operator into a right-handed projection operator, which allows an interaction with right-handed fermions even though the Lagrangian is left-handed. Experiments to date have only demonstrated charge-changing weak interactions for left-handed particles, and an alternative quantization approach that eliminates the divergent off-diagonal terms in the W boson propagator and avoids these difficulties will be considered. The alternative approach appears to be in agreement with existing experiments, but additional high-energy experiments may be required in order to distinguish its predictions from those of the Standard Model.

    hep-phhep-th0 citations
  2. 02*

    Evolution of entropy at small

    G.R.Boroun🇮🇷 · Phuoc Ha🇺🇸

    We explore the evolution of the Deep Inelastic Scattering (DIS) entropy, defined as at small Bjorken variable , where is the observable scale and the gluon distribution is derived from the Dokshitzer-Gribov-Lipatov-Altarelli-Parisi (DGLAP) evolution equations. We aim to evolve the DIS entropy, which is not directly observable, using a Laplace transform technique. This approach allows us to obtain an analytical solution for the DIS entropy based on known initial gluon distribution functions. We consider both leading-order (LO) and higher-order approximations for the DIS entropy, incorporating the evolved gluon distribution function at the initial scale. The DIS entropy, influenced by purely gluonic emissions, varies with higher-order corrections to the running coupling. By comparing theoretical predictions with charged hadron multiplicity data, we define the evolution. Additionally, we investigate the derivative of the scaling entropy, modeling it as a function of the running coupling, to determine the parameter , known as the Pomeron intercept. We find that the values of decrease as the order of evolution increases, which is consistent with the Balitsky-Fadin-Kuraev-Lipatov (BFKL) Pomeron in the LO and NLO approximations. This investigation provides insights into the dynamics of Quantum Chromodynamics (QCD) at high energies.

    hep-phEur.Phys.J.Plus(2026)·1 citation
  3. 03*

    A new study of the interactions of the axion with mesons and photons using a chiral effective Lagrangian model

    Enrico Meggiolaro🇮🇹 · Mirko Tamburini🇮🇹

    In this paper, we extend the results obtained in a previous work and investigate the most interesting decay processes involving axions, photons and the lightest pseudoscalar mesons in the more general case in which the quarks (and, therefore, the mesons) may be charged under the Peccei-Quinn symmetry, making use of a chiral effective Lagrangian model with light quark flavors, which also includes the flavor-singlet pseudoscalar meson and implements the axial anomaly of the fundamental theory. In particular, we compute the axion mass, the electromagnetic coupling of the axion to photons, and the amplitudes and widths of the decay processes .

    hep-phhep-thPRD(2025)·3 citations
  4. 04*

    Extraction of low-mass diffractive cross section from the discrepancy between ATLAS and TOTEM total cross sections

    Per Grafström🇮🇹 · Rafał Staszewski🇵🇱

    At the LHC, two experiments - ATLAS and TOTEM - measure the total proton-proton cross section. Unfortunately, a significant discrepancy, persisting at different collision energies, is observed between the values reported by the two groups. This paper considers the hypothesis that this tension is predominantly driven by the assumption about the low-mass diffraction used in one of the measurement methods. It is shown that in such a case it is possible to extract the low-mass diffraction cross section from measurements of ATLAS and TOTEM. The results are compared with other data-driven estimates, showing better agreement than the original assumption.

    hep-phEPJC(2025)·3 citations
  5. 05*

    No gauge cancellation at high energy in the five-vector gauge

    Jaehoon Jeong🇰🇷

    We propose a novel gauge in the five-vector (5V) framework within the Abelian Higgs model. In the Cartesian basis of the complex Higgs field, the 5V gauge ensures non-divergent tree-level amplitudes for each Feynman diagram in the high-energy limit. This framework pinpoints the origin of high-energy divergences in tree-level amplitudes for each diagram, providing a criterion for quantifying the degree of divergences from other gauges. The 5V description necessitates treating the Goldstone field as the fifth gauge-field component, offering deeper insight into the dynamics of massive gauge bosons, particularly its longitudinal mode. The impact of this framework is demonstrated by rigorously comparing tree-level amplitudes from the 5V gauge with those from the conventional 4V gauge and the Feynman diagram gauge, the latter of which exhibits no gauge cancellation, similar to the 5V gauge.

    hep-phPRD(2025)·3 citations
  6. 06*

    Production of Dark Photons through Higher Electromagnetic Moments at LDMX: Simulations and Model Discrimination

    Riccardo Catena🇸🇪 · Taylor R. Gray🇸🇪 · Thomas Jerkvall🇸🇪

    We extend the projected sensitivity of LDMX for sub-GeV dark matter (DM) to the case of dark photons produced through higher order electromagnetic moments. These moments arise from loop diagrams involving portal matter fields, along with the gauge fields of new symmetry groups. Due to the Lorentz structures, in particular the momentum dependence, of these additional interactions, the kinematic distributions expected at missing momentum/energy experiments vary with model in addition to dark photon mass. By considering four additional types of interactions -- magnetic and electric dipole, charge radius, and anapole moment -- we show that LDMX Phase-II is expected to probe the relic target of these additional dark photon models. We compare the analytic with the numerical methods for calculating the dark bremsstrahlung cross section, and compute the kinematic distributions for each model. The potential for model discrimination in the scenario of non-zero signal events at LDMX is discussed. We find that there is a degeneracy between the dark photon mass and model, which can be partially broken by considering both the energy and the transverse momentum of the recoil electron.

    hep-phastro-ph.COhep-exhep-thJHEP(2025)·2 citations
  7. 07*

    Nonresonant quantum dynamics of a relativistic electron in counterpropagating laser beams

    E. Raicher🇮🇱 · Q.Z. Lv🇨🇳

    The quantum dynamics of an ultrarelativistic electron in strong counterpropagating laser beams is investigated. In contrast to the stimulated Compton scattering regime, we consider the case when in the electron rest frame the frequency of the counterpropagating wave greatly exceeds that of the copropagating one. Taking advantage of the corresponding approximation recently developed by the authors for treating the classical dynamics in this setup, we solve the Klein-Gordon and Dirac equations in the quasiclassical approximation in the Wentzel-Kramers-Brillouin (WKB) framework. The obtained wave function for the Dirac equation shows entanglement between the kinetic momentum and spin of the electron, while the spin-averaged momentum coincides with the classical counterpart as expected. The derived wave functions will enable the calculation of the probabilities of nonlinear QED processes in this counterpropagating fields configuration.

    hep-phphysics.plasm-phPRA(2025)·1 citation
  8. 08*

    baryon spectrum and strong decays in a constituent quark model

    Hui-Hua Zhong🇨🇳 · Ming-Sheng Liu🇨🇳 · Li-Ye Xiao🇨🇳 · Kai-Lei Wang🇨🇳 · Qi-Li · Xian-Hui Zhong

    In this work, we study the baryon spectrum up to the excitations within a semi-relativistic constituent quark potential model, where the mixing between different configurations with the same spin-parity numbers is dynamically considered. Furthermore, the strong decay properties for the excited states are evaluated within an improved chiral quark model by including the relativistic correction term. In a unified framework, we provide a reasonable explanation of the widths, masses, and mass splittings, for the newly observed resonances , , , , , , and . It is found that the configuration mixing is crucial for understanding the strong decay properties and mass splittings, while the relativistic correction term of the strong transition operator plays an important role in the states dominated by the radial excitations. We expect our study can provide useful references for establishing a more abundant spectrum.

    hep-ph6 citations
  9. 09*

    Testing New Physics in Oscillations at a Neutrino Factory

    Peter B. Denton🇺🇸 · Julia Gehrlein🇺🇸 · Chui-Fan Kong🇨🇳

    A neutrino factory is a potential successor to the upcoming generation of neutrino oscillation experiments and a possible precursor to next-generation muon colliders. Such a machine would provide a well-characterized beam of , , , and neutrinos with comparable statistics. Here we show the sensitivity of a neutrino factory to new oscillation physics scenarios such as vector neutrino non-standard interactions and CPT violation. We study two different potential setups for a neutrino factory with different assumptions on charge identification in the far detector. We find that 10 years of a neutrino factory combined with 10 years of DUNE can improve over most of the current constraints on these scenarios and even over forecasted constraints by 20 years of DUNE. Additionally, we find that a neutrino factory can break degeneracies between the standard oscillation parameters and neutrino non-standard interaction parameters present at DUNE.

    hep-phhep-exNPB(2025)·4 citations
  10. 10*

    Anomalous Dimension of a General Effective Gauge Theory I: Bosonic Sector

    Jason Aebischer🇨🇭 · Luigi C. Bresciani🇮🇹 · Nudzeim Selimovic🇮🇹

    We classify the physical operators of the most general bosonic effective gauge theory up to dimension six using on-shell methods. Based on this classification, we compute the complete one-loop anomalous dimension employing both on-shell unitarity-based and geometric techniques. Our analysis fully accounts for the mixing of operators with different dimensions. The results broadly apply to any Effective Field Theory with arbitrary gauge symmetry and bosonic degrees of freedom. To illustrate their utility, we perform a complete cross-check of results on the renormalization of the Standard Model Effective Field Theory (SMEFT), scalar theory, and the SMEFT extended with an axion-like particle. Additionally, we present new results for axion-like particles with CP-violating interactions.

    hep-phhep-thJHEP(2025)·33 citations
  11. 11*

    Isolating Unisolated Upsilons with Anomaly Detection in CMS Open Data

    Rikab Gambhir🇺🇸 · Radha Mastandrea🇺🇸 · Benjamin Nachman🇺🇸 · Jesse Thaler🇺🇸

    We present the first study of anti-isolated Upsilon decays to two muons () in proton-proton collisions at the Large Hadron Collider. Using a machine learning (ML)-based anomaly detection strategy, we "rediscover" the in 13 TeV CMS Open Data from 2016, despite overwhelming anti-isolated backgrounds. We elevate the signal significance to using these methods, starting from using the dimuon mass spectrum alone. Moreover, we demonstrate improved sensitivity from using an ML-based estimate of the multi-feature likelihood compared to traditional "cut-and-count" methods. Our work demonstrates that it is possible and practical to find real signals in experimental collider data using ML-based anomaly detection, and we distill a readily-accessible benchmark dataset from the CMS Open Data to facilitate future anomaly detection developments.

    hep-phhep-exphysics.data-anPRL(2025)·22 citations
  12. 12*

    A Method to Simultaneously Facilitate All Jet Physics Tasks

    Vinicius Mikuni🇺🇸 · Benjamin Nachman🇺🇸

    Machine learning has become an essential tool in jet physics. Due to their complex, high-dimensional nature, jets can be explored holistically by neural networks in ways that are not possible manually. However, innovations in all areas of jet physics are proceeding in parallel. We show that specially constructed machine learning models trained for a specific jet classification task can improve the accuracy, precision, or speed of all other jet physics tasks. This is demonstrated by training on a particular multiclass generation and classification task and then using the learned representation for different generation and classification tasks, for datasets with a different (full) detector simulation, for jets from a different collision system (pp versus ep), for generative models, for likelihood ratio estimation, and for anomaly detection. We consider, our OmniLearn approach thus as a jet-physics foundation model. It is made publicly available for use in any area where state-of-the-art precision is required for analyses involving jets and their substructure.

    hep-phhep-exPRD(2025)·57 citations
  13. 13*

    Primordial black holes

    Guillermo Ballesteros🇪🇸

    The possibility that dark matter could be primordial black holes is discussed with an emphasis on the most commonly studied inflationary dynamics that could have produced them.

    astro-ph.COgr-qchep-phhep-th1 citation
  14. 14*

    Violation of non-Abelian Bianchi identity and QCD topology

    Tsuneo Suzuki🇯🇵

    When Abelian monopoles due to violation of the non-Abelian Bianchi identity J{\mu}(x) condense in the vacuum, color confinement of QCD is realized by the Abelian dual Meissner effect. Moreover VNABI affects also topological features of QCD. Firstly, the topological charge density is not expressed by a total derivative of the Chern-Simons density K{\mu}(x), but has an additional term L(x)=2Tr(J{\mu}(x)A{\mu}(x)). Secondly, the axial U(1) anomaly is similarly modified, while keeping the Atiyah-Singer index theorem unchanged. However, if the integrated additional term is not zero, it is not integer nor gauge invariant, so that VNABI would not be allowed in QCD. Using the Wu-Yang arguments, it is however proved that becomes vanishing. is evaluated also in the framework of Monte-Carlo simulations on SU(2) lattices in details with partial gauge fixings such as the Maximal Center gauge (MCG). When the gradient flow method is used, the term tends to vanish after small gradient flow time (). The biggest effect of VNABI on QCD topology seems to be that self-dual instantons can not be a classical solution of QCD at space-time points where VNABI occurs. One has to find an alternative mechanism explaining integer topological charge, etc. The bosonic definition of the topological charge and its Abelian counterpart written by Abelian field strengths are measured also on the lattices. When is zero, =3 is expected theoretically.

    hep-lathep-phhep-thPTEP(2026)·0 citations
  15. 15*

    Neutrino Oscillation in Core Collapse Supernova: The Impact of Spacetime Geometry

    Indrajit Ghose🇮🇳 · Amitabha Lahiri🇮🇳

    Neutrino flavor evolution inside a core-collapse supernova is a topic of active research. The core of a supernova is an intense source of neutrinos and antineutrinos. Self-interaction among neutrinos (as well as antineutrinos) gives rise to a rich phenomenology not seen in terrestrial situations. In studies of the dynamics of flavor evolution in such environments, the gravitational effects are generally ignored. Although the curvature outside a dense core does not deviate much from a flat space, the spin of the neutrinos can still couple to the torsion of the spacetime. These extra degrees of freedom of curved spacetime have interaction strengths that are proportional to the density of the neutrinos and the other fermions \cite{Chakrabarty:2019cau} \cite{Barick:2023qjq} as well as the coupling constants of the spin-torsion interaction. We have studied the effects of such interactions in flavor evolution inside a core-collapse supernova \cite{Ghose:Manuscript}. The self-interaction gets modified by the spin-torsion interaction and the oscillation dynamics is modified. We have seen that there are noticeable changes in the flavor dynamics when the neutrino density is uniform. We have also studied the effects of such interaction in a realistic core-collapse supernova (CCSN). As neutrino astronomy enters the precision era, this study will shed light on the potential of neutrino fluxes from CCSN to probe the neutrino-neutrino interaction.

    astro-ph.HEhep-phSpringer Proc.Phys.(2026)·0 citations
  16. 16*

    Dynamics of domain walls with bias directions

    Yuan-Jie Li🇨🇳 · Jing Liu🇨🇳 · Zong-Kuan Guo🇨🇳

    The spontaneous breaking of a discrete symmetry can lead to the formation of domain walls in the early Universe. In this work, we explore the impact of bias directions on the dynamics of domain walls, mainly focusing on the model with a biased potential. Utilizing the Press-Ryden-Spergel method, we numerically investigate the dynamics of domain walls with lattice simulations. We find notable differences in the dynamics of domain walls due to bias directions. Our results indicate that the annihilation time depends not only on the vacuum energy difference but also on bias directions described by the relative potential difference .

    astro-ph.COgr-qchep-phPRD(2025)·13 citations
  17. 18*

    Digit quantum simulation of a fermion field in an expanding universe

    Jia-Qi Gong🇨🇳 · Ji-Chong Yang🇨🇳

    Quantum simulation is a rapidly evolving tool with great potential for research at the frontiers of physics, and is particularly suited to be used in computationally intensive lattice simulations, such as problems with non-equilibrium. In this work, a basic scenario, namely free fermions in an expanding universe, is considered and quantum simulations are used to perform the evolution and study the phenomena involved. Using digital quantum simulations with the Jordan-Wigner transformation and Trotter expansion, the evolutions of fermion number density, correlation functions, polarization, and chiral condensation are analyzed. A spread out phenomenon can be observed in the simulation, which is a consequence of momentum redshift. This work also demonstrates the simplicity and convenience of using quantum simulations when studying time-evolution problems.

    quant-phgr-qchep-phPRD(2025)·6 citations
  18. 19*

    Dynamical Confinement and Magnetic Traps for Charges and Spins

    Afshin Besharat🇨🇦 · Alexander A. Penin🇨🇦

    We use the effective field theory approach to systematically study the dynamics of classical and quantum systems in an oscillating magnetic field. We find that the fast field oscillations give rise to an effective interaction which is able to confine charged particles as well as neutral particles with a spin magnetic moment. The effect is reminiscent of the renown dynamical stabilization of charges by the oscillating electric field and provides a foundation for a new class of magnetic traps. The properties characteristic to the dynamical magnetic confinement are reviewed.

    cond-mat.mes-hallhep-phhep-thPRA(2026)·1 citation
  19. 20*

    Theoretical Physics Benchmark (TPBench) -- a Dataset and Study of AI Reasoning Capabilities in Theoretical Physics

    Daniel J.H. Chung🇺🇸 · Zhiqi Gao🇺🇸 · Yurii Kvasiuk🇺🇸 · Tianyi Li🇺🇸 · Moritz Münchmeyer🇺🇸 · Maja Rudolph🇸🇬 · Frederic Sala🇺🇸 · Sai Chaitanya Tadepalli🇺🇸

    We introduce a benchmark to evaluate the capability of AI to solve problems in theoretical physics, focusing on high-energy theory and cosmology. The first iteration of our benchmark consists of 57 problems of varying difficulty, from undergraduate to research level. These problems are novel in the sense that they do not come from public problem collections. We evaluate our data set on various open and closed language models, including o3-mini, o1, DeepSeek-R1, GPT-4o and versions of Llama and Qwen. While we find impressive progress in model performance with the most recent models, our research-level difficulty problems are mostly unsolved. We address challenges of auto-verifiability and grading, and discuss common failure modes. While currently state-of-the art models are still of limited use for researchers, our results show that AI assisted theoretical physics research may become possible in the near future. We discuss the main obstacles towards this goal and possible strategies to overcome them. The public problems and solutions, results for various models, and updates to the data set and score distribution, are available on the website of the dataset tpbench.org.

    cs.LGastro-ph.COcs.AIhep-ph+1Mach.Learn.Sci.Tech.(2025)·23 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.