PaperPanorama

HEP Phenomenology·hep-ph

Mon·Mar 30, 2026

27 papers21 primary·6 cross-listed·reconstructed*

  1. 01*

    Signal-Aware Contrastive Latent Spaces for Anomaly Detection

    Runze Li🇺🇸 · Benjamin Nachman🇺🇸 · Dennis Noll🇺🇸

    High-dimensional feature spaces in particle physics events pose a fundamental challenge to density-estimation-based weakly supervised anomaly detection, whose fidelity degrades rapidly with an increasing number of dimensions. We propose a signal-aware latent space construction using supervised contrastive learning trained on simulated Standard Model backgrounds and a diverse set of hypothesized Beyond the Standard Model (BSM) signals. The resulting latent space is low-dimensional, regularized, and signal-sensitive, enabling high-fidelity density estimation for downstream weakly supervised anomaly detection. We demonstrate the approach in a diphoton final state, testing sensitivity across a broad range of BSM scenarios including supersymmetry models, extended Higgs sectors, heavy neutral resonances, and flavor-changing neutral currents. For signals represented in the contrastive training data, the method can elevate discovery sensitivity from previously inaccessible levels to the discovery regime. Critically, the approach retains sensitivity to BSM models not present during training: interpolation and extrapolation to unseen signal topologies yield substantial improvements in expected significance compared to a background-only baseline. By bridging supervised latent space embedding with weakly supervised anomaly detection, this strategy offers a viable path toward anomaly detection in high-dimensional feature spaces at the LHC and beyond.

    hep-phhep-ex3 citations
  2. 02*

    Prying Open the Dark Sector Window with SBND Off-Target Mode

    Bhaskar Dutta🇺🇸 · Debopam Goswami🇺🇸 · Aparajitha Karthikeyan🇺🇸 · Vishvas Pandey🇺🇸 · Zahra Tabrizi🇨🇭 · Adrian Thompson🇺🇸 · Richard G. Van de Water🇺🇸

    Accelerator-based neutrino experiments with high-intensity proton beams and advanced detector technologies provide a powerful and complementary approach to probing physics beyond the Standard Model. The MiniBooNE experiment at Fermilab pioneered a dedicated Booster Neutrino Beam (BNB) off-target (beam-dump) run, setting leading constraints on sub-GeV dark matter. In this work, we explore the physics opportunities enabled by operating the Short-Baseline Near Detector (SBND) at Fermilab in a future BNB off-target configuration, as well as in a dedicated beam-dump configuration. By redirecting the proton beam away from the nominal beryllium target, or by employing a dedicated beam-dump, neutrino-induced backgrounds are substantially suppressed, thereby enhancing SBND's sensitivity to many new physics scenarios. We demonstrate that such running modes significantly extend the reach for new physics. As representative examples, we present projected sensitivities to light dark matter, axion-like particles, heavy neutral leptons, and meson-portal scenarios.

    hep-phhep-ex2 citations
  3. 03*

    Compressed Stop-Neutralino Spectra from Yukawa Unified Non-Holomorphic Pati-Salam Model: Prospects for the FCC

    Ali Cici🇹🇷 · Busra Nis🇹🇷 · Cem Salih Un🇹🇷

    We explore the weak-scale phenomenology of SUSY models with the gauge symmetry. We include non-holomorphic soft supersymmetry breaking terms arising from perturbations on D-branes. These terms significantly alter the implications of Yukawa unification, as they directly interfere in the threshold corrections to the Yukawa couplings. With these corrections, Yukawa unification can be compatible with low fine-tuning alongside a heavy Higgsino-like lightest supersymmetric particle; however, these solutions are strongly constrained by dark matter observations. Furthermore, in contrast to previous studies, the non-holomorphic contributions accommodate heavy gluino masses in this class of models from approximately 2.2 to 10 TeV while preserving Yukawa unification. These gluinos can be probed up to about 2.5 TeV in high-luminosity collider searches, and up to about 6 TeV at future 100 TeV center-of-mass energy colliders. With the non-holomorphic threshold corrections to Yukawa couplings, Yukawa unification can be accommodated with relatively light third-generation squarks. We find that the supersymmetric spectra can accommodate sbottom masses around 1.5 TeV, making them highly accessible to upcoming experimental searches. The stop can also be as light as about 1.5~TeV, resulting in a compressed stop-neutralino spectrum. Although these solutions lie beyond the sensitivity of current collider searches, they can be potentially probed at future facilities, such as the proposed Future Circular Collider. Our results do not include systematic uncertainties, which can heavily impact the experimental analysis. In this context, our findings serve to highlight potential directions and prospects for new physics searches at future collider experiments. Our results assume that overall systematic uncertainties in background modeling do not exceed .

    hep-ph1 citation
  4. 04*

    Interpreting the results on exclusive modes

    D. Bečirević🇫🇷 · M. Martines🇧🇷 · S. Rosauro-Alcaraz🇫🇷 · O. Sumensari🇫🇷

    We examine the -binned distributions of the decay rate and of the corresponding forward-backward asymmetry which were recently measured by BESIII, showing a mild deviation from the Standard Model predictions. We point out that the proposed solution to remedy the discrepancy by turning on a complex-valued New Physics coupling is in tension with the constraints deduced from the LHC bounds on the high- tail of the relevant Drell-Yan process. We then show that there are several plausible scenarios that are compatible with both the measured low-energy and high-energy constraints but the selected couplings appear to be too small to be observed in the measurements of integrated observables, except for possibly the -binned distribution of the angular observables relevant to or modes.

    hep-phPLB(2026)·3 citations
  5. 05*

    The Radial Mode of Composite Higgs Theories at the LHC

    Gustavo Burdman🇧🇷 · Marvin M. Janini🇧🇷 · Lincoln Pereira🇧🇷 · Murilo Trevisan🇧🇷

    We examine the potential of the LHC to observe the scalar radial excitation present in extensions of the standard model where the Higgs boson is a pseudo Nambu Golstone boson. These include composite Higgs models as well as the twin Higgs model. These states can be light enough to be seen at the LHC, potentially resulting in additional clues about the nature of the Higgs sector. We present the current status of LHC bounds as well as the future prospects for the the high luminosity LHC (HL-LHC). We identify the most sensitive channels as those where the radial state decays to a pair of Higgs bosons, especially at the high luminosity stage. For the minimal composite Higgs models we study, we make use of the LHC Run 2 data with to extract the mass bounds TeV, where the values on the interval depend on the parameters of the model. We show that the reach of the HL-LHC for these cases is , with . For the twin Higgs model radial state, the current bounds are set by Higgs coupling measurements, while for the HL-LHC we obtain the reach TeV, corresponding to the lowest symmetry breaking scale allowed by current data.

    hep-phhep-exJHEP(2026)·0 citations
  6. 06*

    Kaon Boer-Mulders function using a contact interaction

    Dan-Dan Cheng🇨🇳 · Minghui Ding🇨🇳 · Daniele Binosi🇮🇹 · Craig D. Roberts🇨🇳

    Using a symmetry preserving treatment of a vector*vector contact interaction (SCI), results are delivered for the four kaon transverse momentum dependent parton distribution functions (TMDs), viz. helicity-independent (HI) and Boer-Mulders (BM) TMDs for the kaon's , valence degrees of freedom. In completing this analysis, we are able to deliver insights into, amongst other things, the role played by emergent hadron mass (EHM) phenomena in producing these TMDs; the EHM modulating effect of the Higgs-boson coupling that produces the strange quark current mass; the impact of gauge link models on whether predictions satisfy the positivity constraint that bounds the BM function relative to the HI TMD; and the size of the BM shift and effects thereupon of off-diagonal terms in the associated scale-evolution kernel.

    hep-phhep-exhep-latnucl-ex+1EPJC(2026)·3 citations
  7. 07*

    Same-sign dimuon probe of charged lepton flavor violation at electron-photon colliders

    Zhong Zhang🇨🇳 · Yu Zhang🇨🇳 · Zeren Simon Wang🇨🇳

    Observation of charged lepton flavor violation would constitute unambiguous evidence for physics beyond the Standard Model (SM). We identify a previously unexplored same-sign dimuon signature in electron--photon collisions, , mediated by an axionlike particle (ALP) with flavor-violating -- couplings. The absence of irreducible SM backgrounds and the on-shell production of the ALP render this channel intrinsically clean and highly sensitive, with only small residual backgrounds arising from detector effects. Such collisions can be realized via laser Compton backscattering at colliders including BEPC-II with the BESIII detector, STCF, CEPC, and ILC. We find that STCF, CEPC, and ILC can probe couplings one to two orders of magnitude below existing bounds. This combination of resonant production, vanishing irreducible background, and same-sign topology would be difficult to achieve in conventional or hadron-collider environments, establishing electron--photon collisions as a uniquely powerful probe of charged lepton flavor violation.

    hep-phhep-exChin.Phys.Lett.(2026)·1 citation
  8. 08*

    Signatures of Type-I Seesaw in Neutrino Oscillation Phenomenology

    Suka Sriyansu Pattanaik🇮🇳 · Sasmita Mishra🇮🇳

    We investigate the low-energy phenomenology of the Type-I seesaw mechanism within a 3+3 framework containing three active and three sterile neutrinos. Using the exact seesaw relation as a bridge between the high-scale sterile-sector parameters and the standard oscillation observables, we perform a comprehensive Monte Carlo scan of the 21-dimensional sterile parameter space, retaining only those configurations consistent with current neutrino oscillation data within . For the viable parameter points, we simulate the modified neutrino oscillation probabilities and event rates at the long-baseline experiments DUNE and NOA, and the medium-baseline reactor experiment JUNO, quantifying their sensitivity to sterile neutrino effects across the eV--GeV mass range. We find that eV-scale sterile neutrinos produce pronounced spectral distortions, while heavier states decouple progressively from oscillation experiments. In parallel, we confront the seesaw predictions with complementary probes: cosmological bounds on , the kinematic mass from beta decay, the effective Majorana mass from neutrinoless double beta decay (), and the charged-lepton-flavor-violating branching ratio . The combination of all constraints significantly narrows the allowed parameter space: the predicted sum of neutrino masses clusters at --~eV, within reach of next-generation cosmological surveys, and eV-scale sterile neutrinos are found to be under significant tension from the current MEG bound on .

    hep-ph1 citation
  9. 09*

    Complete Next-to-Next-to-Leading-Order QCD Correction to Decay

    Chao Zeng🇨🇳 · Bin Gong🇨🇳 · Jian-Xiong Wang🇨🇳 · Ruichang Niu · Xu-Dong Huang🇨🇳 · Cong Li🇨🇳

    We address the long-standing problem of negative decay and production rates in perturbative QCD for exclusive processes by proposing amplitude-level NRQCD factorization as a systematic prescription. Building on this, we present the first complete next-to-next-to-leading-order (NNLO) QCD correction to the decay . The resulting partial width, eV, combines this NNLO contribution with the known up to relativistic correction and shows markedly improved agreement with the high-precision BESIII measurement. In the same way, eV is obtained. The dominant theoretical uncertainty originates from the renormalization scale variation, underscoring the challenge of perturbative convergence at this order and the necessity for future higher-order calculations.

    hep-ph2 citations
  10. 10*

    Finite Temperature NLO Corrections in Relativistic Scatterings: Implications for Dark Matter Freeze-In

    Sampriti Roy🇮🇳 · Pritam Sen🇮🇳 · Satyanarayan Mukhopadhyay🇮🇳

    We study the next-to-leading order (NLO) virtual and thermal corrections to relativistic scattering processes involving scalar particles in the early Universe thermal plasma. Taking the example of freeze-in production of scalar dark matter pairs through these scatterings, we evaluate the impact of the NLO corrections to the annihilation rate and the dark matter yield. We find that including only thermal mass corrections to a leading order interaction rate can overestimate the reduction in these rates, and the full NLO corrections can modify the DM abundance predictions by . It is also observed that while the virtual NLO effects are larger, the finite temperature NLO corrections to the matrix elements in the relativistic regime can modify the DM abundance by , in comparison to the virtual NLO corrections.

    hep-phhep-th0 citations
  11. 11*

    (3+1)D dilute Glasma initial conditions in simulations of heavy-ion collisions

    Kayran Schmidt🇦🇹

    In this thesis, an approximation for the full (3+1)D dynamics of the Glasma is presented, which breaks boost-invariance on the level of the nuclear fields and leads to rapidity dependence in the final results. For this treatment, the Yang-Mills equations are linearized in covariant gauge, where lower-order, nonlinear contributions are neglected and the dynamics are captured by the (3+1)D dilute Glasma. The analytic solutions of the (3+1)D dilute Glasma are derived in both position and momentum space formulations, providing a comprehensive understanding of the involved (3+1)D dynamics. In position space, the field strength tensor results from the integration of free-streaming gluons that are produced in scattering processes where the initial nuclear fields overlap. In momentum space, the event-averaged gluon number distribution for the (3+1)D dilute Glasma is derived in Coulomb gauge. A generalized, three-dimensional McLerran-Venugopalan nuclear model is developed for nuclei with realistic envelopes and intrinsic longitudinal correlations. Numerical results are presented for the rapidity structure of the energy-momentum tensor, the gluon number distribution, and the transverse energy of the (3+1)D dilute Glasma. In position space, the extended longitudinal collision geometry and finite longitudinal correlation length break boost-invariance. In momentum space, the results each follow universal parametrizations and are fixed by the values of two scaling parameters. Furthermore, the numerical results exhibit limiting fragmentation where the rapidity profiles approach a limiting distribution at large rapidities. This feature is also derived locally in position space for the analytic expressions of the field strength tensor and, in momentum space, for the transverse energy of the (3+1)D dilute Glasma.

    hep-phnucl-th0 citations
  12. 12*

    Constraints on axion-like particles via associated diboson production in hadronic collisions

    Barbara Jäger🇩🇪 · Ozan Semin🇩🇪

    We investigate the sensitivity of current and future hadron-collider experiments to axion-like particles (ALPs) through associated diboson production, focusing on a linear effective field theory framework with bosonic ALP couplings. We analyze the dominant production mechanisms and relevant backgrounds, considering the impact of jet misidentification rates on the diboson background. We present our results using conservative jet-misidentification rates, and derive four dimensional constraints on the ALP couplings to gluons, weak bosons, and photons. Our findings highlight the potential of the high-luminosity phase of the CERN Large Hadron Collider to probe the ALP parameter space in the sub-GeV mass range, as well as the codependencies of the various ALP couplings.

    hep-ph0 citations
  13. 13*

    Neural network enhanced Bayesian global analysis of relativistic heavy ion collisions

    Jussi Auvinen🇫🇮 · Kari J. Eskola🇫🇮 · Henry Hirvonen🇺🇸 · Harri Niemi🇫🇮

    We introduce a novel deep convolutional neural network (NN) -enhanced Bayesian global analysis of bulk observables in highest-energy heavy-ion collisions, using relativistic 2+1 D second-order viscous hydrodynamics with a dynamical freeze-out, and with perturbative QCD and saturation -based initial conditions from the event-by-event EKRT-model. Our analysis has 13+2 free parameters for the QCD-matter properties + initial state, which are constrained by the experimental data from GeV Au+Au collisions at RHIC and TeV Pb+Pb, TeV Pb+Pb, and TeV Xe+Xe collisions at the LHC. We replace the computationally demanding hydrodynamical simulations by NNs, which predict bulk observables directly from the initial energy density profiles, event-by-event, and account for the QCD-matter properties. With the NN output, we train the Gaussian process emulators for obtaining centrality-class averaged observables and their uncertainties. The NNs reduce the computing time significantly, enabling us to include also statistics-hungry flow observables like and the normalized symmetric cumulant in the analysis. In this paper, we demonstrate the feasibility of the NN based Bayesian global analysis. We find the data favoring a specific shear viscosity with a minimum-value plateau at temperatures MeV, with . The bulk viscous coefficient is non-zero at MeV. The Knudsen number at the freeze-out is , while the ratio of the mean free path to the system size at freeze-out is in the range , implying that the freeze-out indeed happens at the expected limit of the applicability of hydrodynamics.

    hep-phnucl-thPRC(2026)·1 citation
  14. 14*

    The heavy flavor conserving hadronic weak decay of the ground-state bottom baryons

    Peng-Yu Niu🇨🇳 · Qian Wang🇨🇳 · Qiang Zhao🇨🇳

    In this work the heavy flavor conserving (HFC) hadronic weak decays of bottom baryons are studied in the framework of the nonrelativistic constituent quark model (NRCQM). We show that the pole terms play an indispensable role in the description of the branching ratio of . With the pole terms included we can make reliable predictions for . A combined study of the HFC hadronic weak decays allows us to make a reasonable prediction for , which can be searched for at LHCb and Belle-II experiments.

    hep-phChin.Phys.Lett.(2026)·0 citations
  15. 15*

    Non-eikonal corrections to dijet production in DIS

    Néstor Armesto🇪🇸 · Fabio Domínguez🇪🇸 · Adrián Romero🇪🇸

    We compute non-eikonal corrections to dijet production in deep inelastic scattering off a nucleus. Such corrections are expected to be quantitatively important at the energies of the future Electron Ion Collider. We focus on those corrections stemming solely from the finite longitudinal size of the nucleus. For both longitudinally and transversely polarized photons, we provide general, all-order expressions in terms of two-dimensional path integrals. To proceed further, we use the harmonic oscillator approximation for the target averages of Wilson lines. We then expand the general expressions order by order beyond the shockwave limit which provides the eikonal results, up to next-to-next-to-eikonal accuracy. We observe that next-to-eikonal corrections to this observable vanish for the mentioned approximation for target averages, as previously found for single gluon production in proton-nucleus collisions. Finally, we calculate the back-to-back of correlation limit of our expressions.

    hep-phnucl-th0 citations
  16. 16*

    Evaluation of QED cross sections in strong magnetic fields

    Olavi Kiuru🇫🇮

    Quantum electrodynamics (QED) becomes nonlinear when the magnetic field strength surpasses the critical Schwinger limit G. This limit is surpassed, for example, in the magnetospheres of a specific class of neutron stars known as magnetars, which has important consequences for magnetospheric plasma dynamics due to modifications in scattering cross sections. Using a formalism previously applied to the study of magnetic catalysis, I calculate the cross sections of all tree-level 1-to-2, 2-to-1, and 2-to-2 particle QED scattering processes that do not include a photon propagator. The calculations are done in a strong background magnetic field and the results are implemented into an open-source Python package. This article focuses on presenting the formalism and computational techniques required for the calculations, while the impact of the results on, e.g., magnetospheric plasma dynamics is discussed in a companion letter (Kiuru et al. 2026).

    hep-phastro-ph.HEphysics.plasm-ph1 citation
  17. 17*

    Sensitivity to new physics: single-Higgs couplings vs. the trilinear Higgs coupling

    Henning Bahl🇩🇪 · Johannes Braathen🇩🇪 · Martin Gabelmann🇩🇪 · Sven Heinemeyer🇪🇸 · Kateryna Radchenko Serdula🇪🇸 · Alain Verduras Schaeidt🇩🇪 · Georg Weiglein🇩🇪

    The trilinear Higgs self-coupling provides a unique probe of the structure of the Higgs potential and of the nature of the electroweak phase transition, and constitutes a key target for future collider experiments. Recent studies have shown that confronting theoretical predictions for the trilinear Higgs coupling with current experimental bounds offers a powerful and complementary way to test effects of physics beyond the Standard Model (BSM), in particular those arising from extended Higgs sectors. Meanwhile, substantial progress has been achieved in the precise calculation and automation of the trilinear Higgs coupling in a wide class of BSM models. This contribution discusses several BSM scenarios, compatible with existing constraints, in which sizeable deviations in the trilinear Higgs coupling w.r.t. the Standard Model (SM) value are predicted, while other Higgs observables remain close to their SM expectations and are therefore difficult to probe experimentally. These results highlight the strong physics motivation for a precise measurement of the trilinear Higgs coupling at a future Higgs factory.

    hep-ph4 citations
  18. 18*

    Universal Geometric Scaling in Cosmic Ray Spallation: Evidence of a Dynamical Causal Horizon from AMS-02

    Yi Yang🇹🇼

    The interpretation of high-precision cosmic ray spectra is fundamentally bottlenecked by uncertainties in fragmentation cross-sections. Traditional kinematic models, driven by phase-space expansions, typically predict complex, energy-dependent evolutions. However, AMS-02 measurements reveal that at high rigidities (~GV), secondary-to-secondary flux ratios (Li/B, Be/B, and Li/Be) strictly converge to energy-independent plateaus. To understand this anomaly, we explore a macroscopic geometric framework. The ultra-relativistic spallation of a target nucleus snaps residual strong-interaction flux tubes, inducing an extreme deceleration on the remnant. Using a semi-microscopic estimation based on the Woods-Saxon potential and pion exchange, we suggest this dynamically generates a causal horizon with an effective Unruh temperature ~MeV. Utilizing the Be/B ratio as an absolute calibration channel, we extract an asymptotic scale of ~MeV, remarkably consistent with our theoretical estimation and the established nuclear liquid-gas phase transition limit. Subsequent blind tests on Lithium ratios demonstrate a universal zero-slope convergence, providing compelling evidence that a constant geometric thermal bath effectively supersedes complex microscopic kinematics at high energies.

    hep-phhep-ex1 citation
  19. 19*

    Global Structure, Non-Invertible PQ Symmetry, and the DFSZ Domain Wall Problem

    Gongjun Choi🇺🇸 · Sungwoo Hong🇰🇷 · Seth Koren🇺🇸

    In recent years it has become increasingly clear that the previously overlooked ``global structure'' of symmetry groups can encode significant theoretical structure and, more importantly, have substantial phenomenological implications. With this in mind we re-examine the DFSZ axion, which suffers from a domain wall problem due to the Standard Model generation structure. We show that global structure acting between the Peccei-Quinn symmetry and the electroweak gauge group plays a crucial role in determining the precise nature of the domain wall problem, which has important implications in both cubic and quartic DFSZ. We then demonstrate that the stability of the domain walls is enforced by a non-invertible chiral symmetry in quark flavor models which have additional global structure acting between the color and the gauged quark flavor groups. The strategy of Non-invertible Naturalness then leads us to UV theories that resolve the domain wall problem through small-instanton-induced breaking of non-invertible symmetries. Finally, we sketch potential gravitational wave signatures arising from the annihilation of axion domain walls. Our work illustrates the importance of considerations of global structure in realistic models of particle physics.

    hep-phastro-ph.COhep-th5 citations
  20. 20*

    Simulating Axion Electrodynamics in Magnetized Plasmas: Energy transfer in the inhomogeneous and strongly varying limit

    Fabrizio Corelli🇮🇹 · Estanis Utrilla Ginés🇪🇸 · Enrico Cannizzaro🇵🇹 · Andrea Caputo🇨🇭 · Samuel J. Witte🇬🇧

    In this work we study the electromagnetic response induced by axions in a magnetized plasma, focusing specifically on characterizing energy transfer and energy losses from the ambient axion field in highly inhomogeneous and strongly varying backgrounds. Using a suite of both frequency-domain and time-domain simulations, we solve for: the efficiency of photon excitation in a rapidly varying background, the indirect excitation of Alfvén modes, occurring when a Langmuir-Ordinary (LO) mode is resonantly excited near a combined cutoff-resonance of the dispersion relations of the LO and Alfvén modes, and the excitation of electric fields in small localized plasma under-densities. We identify a particularly interesting regime in which energy can be transferred into sub-luminal plasma modes () with an efficiency greater than that of super-luminal modes (). Our results highlight a variety of less conventional ways in which axions (and other light degrees of freedom that mix with electromagnetism, such as dark photons or gravitons) can interact in extreme astrophysical environments.

    hep-phgr-qchep-th0 citations
  21. 21*

    The Physics and Prospects of Super-Tau Charm Factories

    Alexey A. Petrov🇺🇸 · Yangheng Zheng🇨🇳

    The proposed Super tau-charm factories are a powerful new class of high-luminosity electron-positron colliders operating in the center-of-mass energy range between 2 and 7 GeV, a region that spans thresholds for tau leptons, open-charm hadrons, charmonium and charmonium-like states, hyperons, and light hadrons. With unprecedented data samples, threshold kinematics, and quantum-coherent production, these facilities offer unique opportunities to advance precision tests of the Standard Model and to search for physics beyond it. In this review, we examine the physics prospects of the Super Tau-Charm Facility, focusing on precision charm measurements, CP violation in mesons and baryons, tau lepton properties and rare decays, and nonperturbative QCD phenomena such as hadronization, spectroscopy, and time-like form factors. We also discuss the experimental landscape, technological challenges, and complementarity with existing and planned facilities. Together, these capabilities position super tau-charm factories at the forefront of the precision frontier in particle physics.

    hep-phhep-exnucl-exnucl-th2 citations
  22. 22*

    Primordial Black Hole interpretation of the sub-solar merger event S251112cm

    Md Riajul Haque🇨🇳 · Fabio Iocco🇮🇹 · Luca Visinelli🇮🇹

    The LIGO-Virgo-KAGRA (LVK) candidate event S251112cm suggests the presence of at least one compact object with sub-solar masses. Since such objects cannot be produced through standard stellar evolution, this observation provides a potential indication of non-standard formation channels. Primordial black holes (PBHs), formed from the collapse of primordial density fluctuations in the early Universe, are a well-motivated candidate. We investigate the interpretation of S251112cm as the merger of two PBHs with masses in the range 0.1-1. Combining analytic estimates of the PBH merger rate with current observational constraints on their abundance and the sensitivity of LVK searches, we compute the probability of observing such an event. Within a relaxed constraint scenario, the probability reaches unity in the range -, while it remains sizable, , in more conservative scenarios and at lower masses. Our results show that a PBH interpretation of S251112cm is viable within current bounds. Owing to the dependence of our results on astrophysical uncertainties, such as those affecting the constraints on the abundance of PBHs, they cannot be regarded as conclusive with respect to the nature of the detected event. At the same time, our analysis highlights the potential of sub-solar gravitational wave events as a probe of PBHs and their contribution to dark matter.

    astro-ph.COgr-qchep-ph9 citations
  23. 23*

    Dark energy from string theory: an introductory review

    David Andriot🇫🇷

    Dark energy, the main constituent in our expanding universe, responsible for its acceleration, is currently being observed with unprecedented precision through various experiments. While several cosmological models can fit this latest data, deriving some of them from string theory would provide a valuable theoretical prior, with information on the nature of dark energy. This article reviews the efforts towards such a derivation, namely the options from string theory to get a cosmological constant (a de Sitter solution) or a dynamical dark energy (via a quintessence model). After providing a brief historical perspective, we first review proven or conjectured constraints on obtaining dark energy from string theory, in classical or asymptotic regimes. Circumventing such obstructions, by changing regime or ansatz, one can try to construct a de Sitter solution: we present a long list of such attempts, and the difficulties encountered. Among them, we discuss in detail efforts towards classical de Sitter solutions. Then, we review quintessence from string theory, focusing on single-field exponential models. Related topics are discussed, including the coupling to matter, the comparison to observational data, and the absence of a cosmological event horizon.

    hep-thastro-ph.COgr-qchep-ph+224 citations
  24. 24*

    Efficient computation of the N-th rank QED polarization tensor: Universal worldline structure of form factors

    Xabier Feal🇺🇸 · Andrey Tarasov🇺🇸 · Raju Venugopalan🇺🇸

    We derived in arXiv:2206.04188 arXiv:2211.15712 a compact expression for the -th rank QED polarization tensor in a -dimensional worldline framework. This fully off-shell object, a function of external photon four-momenta, is a key ingredient in high-order computations of cusp anomalous dimensions and lepton anomalous magnetic moments. We demonstrate here that can further be expressed simply in terms of a small number of independent ``head" form factors (each representing Feynman diagrams) which have a universal structure in terms of sums over fermion Green functions and (propertime derivative of) their boson worldline superpartners. This worldline representation bypasses explicit Wick contractions and avoids tensor reductions to scalar loop integrals à la Passarino and Veltman, order by order in perturbation theory. We give explicit expressions for the -th and -th rank head form factors and provide a computer script generalizing these results to arbitrary external photons. The multiplicity of heads, and their growth with , can be understood in terms of orbits of the permutation group. We employ the Burnside-Cauchy-Frobenius lemma to show that it scales as terms as opposed to the terms in conventional perturbation theory. We reexpress worldline parameter integrals that define the -th rank heads as Feynman parameter integrals to reproduce the seminal results by Karplus and Neuman for the on-shell light-by-light amplitude and extend these to the fully off-shell case in massless QED employing a tailored integration-by-parts procedure. In a follow-up paper, we will discuss the direct computation of worldline integrals, potentially providing a further advantage relative to Feynman diagram computations at high orders in perturbation theory.

    hep-thhep-phnucl-thPRD(2026)·0 citations
  25. 25*

    Implication of dressed form of relational observable on von Neumann algebra

    Min-Seok Seo🇰🇷

    In quantum gravity, physically meaningful operator is required to be invariant under the diffeomorphisms. Such gauge invariant operator is typically given by the relational observable, the operator localized in relation to some background states. We point out that the relational observable can be comprehensively written in the form of the dressed operator. For the background having boundary where the diffeomorphisms are not gauged, we can use the gravitational Wilson line for dressing, then the relational observable is nonlocal. In contrast, when the background breaks some isometries, as can be found in quasi-de Sitter space, dressing can be local, which is a kind of Stückelberg mechanism. Since dressing resembles the outer automorphism in the von Neumann algebra, we may investigate the algebraic structure of the background by considering the dressed form of the relational observable. From this, we can understand that quasi-de Sitter space is described by the Type II algebra where the trace diverges in the decoupling limit of gravity. It is different from the Type II algebra of de Sitter space where the finite size of trace can be defined in the same limit. This shows that the isometry preserving and breaking backgrounds are quite different in the algebraic structure no matter how small the breaking effect is.

    hep-thgr-qchep-ph0 citations
  26. 26*

    Probing Sub-MeV Dark Matter with Neutron-Capture Spectroscopy

    B. Meirose🇸🇪 · D. Milstead🇸🇪

    We present a general, discovery-grade framework for searching for weakly coupled new particles emitted in nuclear de-excitation following neutron capture. Rather than relying on isolated spectral features, the method exploits correlated ``satellite-line combs'': multiple weak -ray lines appearing at a common energy offset below known capture transitions. By combining likelihood information across many parent lines and multiple target nuclei, the approach strongly suppresses nuclear-structure ambiguities and instrumental artifacts. We also discuss optimal target selection and practical experimental implementation with high-resolution HPGe detectors.

    nucl-exhep-exhep-phnucl-th0 citations
  27. 27*

    Hardware-Aware Tensor Networks for Real-Time Quantum-Inspired Anomaly Detection at Particle Colliders

    Sagar Addepalli🇺🇸 · Prajita Bhattarai🇺🇸 · Abhilasha Dave🇺🇸 · Julia Gonski🇺🇸

    Quantum machine learning offers the ability to capture complex correlations in high-dimensional feature spaces, crucial for the challenge of detecting beyond the Standard Model physics in collider events, along with the potential for unprecedented computational efficiency in future quantum processors. Near-term utilization of these benefits can be achieved by developing quantum-inspired algorithms for deployment in classical hardware to enable applications at the "edge" of current scientific experiments. This work demonstrates the use of tensor networks for real-time anomaly detection in collider detectors. A spaced matrix product operator (SMPO) is developed that provides sensitivity to a variety beyond the Standard Model benchmarks, and can be implemented in field programmable gate array hardware with resources and latency consistent with trigger deployment. The cascaded SMPO architecture is introduced as an SMPO variation that affords greater flexibility and efficiency in ways that are key to edge applications in resource-constrained environments. These results reveal the benefit and near-term feasibility of deploying quantum-inspired ML in high energy colliders.

    cs.LGhep-phphysics.ins-det2 citations

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