PaperPanorama

HEP Phenomenology·hep-ph

Thu·Dec 21, 2023

53 papers37 primary·16 cross-listed·reconstructed*

  1. 01*

    Advancing the understanding of energy-energy correlators in heavy-ion collisions

    João Barata🇺🇸 · Paul Caucal🇫🇷 · Alba Soto-Ontoso🇨🇭 · Robert Szafron🇺🇸

    We investigate the collinear limit of the energy-energy correlator (EEC) in a heavy-ion context. First, we revisit the leading-logarithmic (LL) resummation of this observable in vacuum following a diagrammatic approach. We argue that this route allows to naturally incorporate medium-induced effects into the all-orders structure systematically. As an example, we show how the phase-space constraints imposed by the medium on vacuum-like emissions can be incorporated into the LL result by modifying the anomalous dimensions. On the fixed-order side, we calculate the expansion of the in-medium EEC for a splitting using, for the first time, the exact matrix element. When comparing this result to previously used approximations in the literature, we find up to deviations in the regime of interest for jet quenching signatures. Energy loss effects are also quantified and further suppress the EEC at large angles. These semi-analytic studies are complemented with a phenomenological study using the jet quenching Monte Carlo JetMed. Finally, we argue that the imprint of medium-induced effects in energy-energy correlators can be enhanced by using an alternative definition that takes as input Lund primary declusterings instead of particles.

    hep-phhep-exnucl-thJHEP(2024)·78 citations
  2. 02*

    Initial-state and final-state effects on hadron production in small collision systems

    Ivan Vitev🇺🇸 · Weiyao Ke🇺🇸

    Heavy meson production in reactions with nuclei is an active new frontier to understand QCD dynamics and the process of hadronization in nuclear matter. Measurements in various colliding systems at RHIC and LHC, including Pb-Pb, Xe-Xe, O-O, p-Pb, and p-O, enable precision tests of the medium-size, temperature, and mass dependencies of the in-medium parton propagation and shower formation. We employ a coupled DGLAP evolution framework that takes advantage of splitting functions recently obtained in soft-collinear effective theory with Glauber gluons (SCET) and hard thermal loop (HTL) motivated collisional energy loss effects. With jet quenching effects constrained to the nuclear modification factor of charged hadrons in Pb-Pb collisions at 5.02 TeV, we present predictions for light and heavy-meson in Xe-Xe, O-O and p-Pb collisions at the LHC. We find that the nuclear modification scales non-trivially with the quark mass and medium properties. In particular, there can be sizeable collision-induced attenuation of heavy mesons in small systems such as oxygen-oxygen and high-multiplicity p-Pb events. Finally, we analyze the impact of different models of initial-state parton dynamics on the search for QGP signatures in small colliding systems.

    hep-phEPJ Web Conf.(2024)·2 citations
  3. 03*

    Double Higgs Boson Production via Photon Fusion at Muon Colliders within the Triplet Higgs Model

    Bathiya Samarakoon🇺🇸 · Terrance M. Figy🇺🇸

    In this paper, we present predictions for scattering cross-section the of Higgs boson pair production via photon fusion at future muon colliders, focusing specifically the production processes . We investigated the impact of three choices the photon structure functions on cross-section predictions for a range model input parameters within the theoretical framework of the Higgs Triplet Model.

    hep-phPRD(2024)·5 citations
  4. 04*

    Impact of SeaQuest data on sea-quark PDFs at large

    S. Alekhin🇩🇪 · M.V. Garzelli🇩🇪 · S. Kulagin🇷🇺 · S.-O. Moch🇩🇪

    We investigate the impact of the recently released FNAL-E906 (SeaQuest) data on the ratio of proton-deuteron and proton-proton Drell-Yan production cross-sections on the sea quark PDFs. We find that they have constraining power on the light-quark sea isospin asymmetry and on the ratio at large longitudinal momentum fraction values, and that their constraints turn out to be compatible with those from Drell-Yan data in collider experiments (Tevatron and Large Hadron Collider) and in the old fixed-target experiment by the FNAL-E866 collaboration. We study the impact of nuclear corrections due to the deuteron target, finding them within 1% in most of the kinematic region covered by SeaQuest. We perform a new proton PDF fit, including SeaQuest data, using the ABMP16 methodology and we compare it to the ABMP16 baseline.

    hep-phPoS(2024)·0 citations
  5. 05*

    Study of the hidden-heavy pentaquarks and states

    Wen-Xuan Zhang🇨🇳 · Chang-Le Liu🇨🇳 · Duojie Jia🇨🇳

    In light of the recently observed resonance states and by LHCb Collaboration in decay channel, we perform a systematical study of all possible hidden-heavy pentaquarks with strangeness , in unified framework of MIT bag model. The color-spin wavefunctions presented in terms of Young-Yamanouchi bases and transformed into baryon-meson couplings, are utilized to calculate masses, magnetic moments and ratios of partial widths. With numerical analysis, the observed is likely to be a compact pentaquark, and favors two-peak structure of and states. Further predictions on hadron properties and decay channels are given to compact , states and bottom sectors.

    hep-phPRD(2024)·20 citations
  6. 06*

    An Algebraic Roadmap of Particle Theories, Part II: Theoretical checkpoints

    N. Furey🇩🇪

    An optimal algebraic model of particle physics has a number of checkpoints to pass. As a minimum, models should conform to the Coleman-Mandula theorem (or establish a loophole), evade familiar fermion doubling problems, naturally explain the Standard Model's chirality, exclude B-L gauge symmetry at low energy, and explain the existence of three generations. We demonstrate how the model introduced in [1] passes checkpoints , and has yet to cross . We close by elucidating an unexpected appearance of spacetime symmetries.

    hep-phhep-thAnnalen Phys.(2025)·7 citations
  7. 07*

    Questions of flavor physics and neutrino mass from a flipped hypercharge

    Duong Van Loi🇻🇳 · Phung Van Dong🇻🇳 · N. T. Duy🇻🇳 · Nguyen Huy Thao🇻🇳

    The flavor structure of quarks and leptons is not yet fully understood, but it hints a more fundamental theory of non-universal generations. We therefore propose a simple extension of the Standard Model by flipping (i.e., enlarging) the hypercharge to for which both and depend on generations of both quark and lepton. By anomaly cancellation, this extension not only explains the existence of just three fermion generations as observed but also requires the presence of a right-handed neutrino per generation, which motivates seesaw neutrino mass generation. Furthermore, in its minimal version with a scalar doublet and two scalar singlets, the model naturally generates the measured fermion-mixing matrices while it successfully accommodates several flavor anomalies observed in the neutral meson mixings, -meson decays, lepton-flavor-violating processes of charged leptons, as well as satisfying constraints from particle colliders.

    hep-phPRD(2024)·5 citations
  8. 08*

    Discovery of optical emission from the supernova remnant G108.2-0.6 and its atomic environment

    Gunay Payli🇹🇷 · Hicran Bakis🇹🇷 · Ebru Aktekin🇹🇷 · Hidetoshi Sano🇯🇵 · Aytap Sezer🇹🇷

    We report the first detection of optical emission from the shell-type Galactic supernova remnant (SNR) G108.20.6. We obtained H images and long-slit spectra using the 1.5-m RTT150 telescope to examine the morphological and spectral characteristics of the SNR. We detected several filaments along its north and south regions, which is consistent with its SNR nature. The spectra exhibit [SII]/H ratios in the range of 0.41.1, indicating emission from shock-heated gas. The oxygen doublet emission lines [OI]6300, 6363 detected in the south region also support the indicator of the presence of shocks. We estimate the electron density using the [SII] 6716/6731 ratio ranging from 15 to 1800 cm. The spectra show a relatively low shock velocity of 80 km s with the pre-shock cloud density of 1857 cm. The H/H ratios show significant variation across the observed regions with extinction ranging from 0.22 to 1.65. We also analyzed the archival HI data and estimated the kinematic distance to the SNR of 0.8 kpc and dynamical age as 7010 kyr of G108.20.6.

    hep-phastro-ph.GAMNRAS(2023)·4 citations
  9. 10*

    Infinite order results for charged sectors of the Standard Model

    Oleg Antipin🇭🇷 · Jahmall Bersini🇯🇵 · Pantelis Panopoulos🇰🇷 · Francesco Sannino🇩🇰 · Zhi-Wei Wang🇨🇳

    We determine anomalous dimensions of a family of fixed hypercharge operators in the Standard Model featuring the general Cabibbo-Kobayashi-Maskawa structure. The results are obtained at infinite orders in the couplings and to leading and subleading orders in the charge. The computed anomalous dimensions are shown to agree with the maximum known order in perturbation theory. We further show that the large hypercharge sector of the Standard Model is characterised by a non-Abelian vector condensation phase.

    hep-phhep-thJHEP(2024)·9 citations
  10. 11*

    Nuclear mass radius and pressure in the Skyrme model

    Alberto García Martín-Caro🇪🇸 · Miguel Huidobro🇪🇸 · Yoshitaka Hatta🇺🇸

    We compute the mass radius, scalar radius, tensor radius, baryon number radius and mechanical radius of nuclei with baryon number in the Skyrme model. The relations between these radii and the nuclear gravitational form factors are investigated. We also compute the `pressure' distribution and find that it is negative in the core region for all the nuclei with . This suggests that the way mechanical stability is achieved in nuclei is qualitatively different than in the nucleon.

    hep-phnucl-thPRD(2024)·20 citations
  11. 12*

    Cosmological implications of inflaton-mediated dark and visible matter scatterings after reheating

    Deep Ghosh🇮🇳 · Sourav Gope🇮🇳 · Satyanarayan Mukhopadhyay🇮🇳

    The initial density of dark matter (DM) particles, otherwise secluded from the standard model (SM), may be generated at reheating, with an initial temperature ratio for internal thermalizations, . This scenario necessarily implies inflaton-mediated scatterings between DM and SM after reheating, with a rate fixed by the relic abundance of DM and the reheat temperature. These scatterings can be important for an inflaton mass and reheat temperature as high as and , respectively, since the thermally averaged collision terms become approximately independent of the inflaton mass when the bath temperature is larger than the mass. The impact of these scatterings on DM cosmology is studied modeling the perturbative reheating physics by a gauge-invariant set of inflaton interactions upto dimension-5 with the SM gauge bosons, fermions and the Higgs fields. It is observed that an initially lower (higher) DM temperature will rapidly increase (decrease), even with very small couplings to the inflaton. There is a sharp lower bound on the DM mass below which the relic abundance cannot be satisfied due to faster back-scatterings depleting DM quanta to SM particles. For low DM masses, the CMB constraints become stronger due to the collisions for , probing values as small as , and weaker for . The BBN constraints become stronger due to the collisions for lower DM masses, probing as small as , and weaker for higher DM mass. Thus inflaton-mediated collisions with predictable rates, relevant even for high-scale inflation models, can significantly impact the cosmology of light DM.

    hep-phastro-ph.COPRD(2024)·4 citations
  12. 13*

    Proton PDFs with non-linear corrections from gluon recombination

    Pit Duwentäster🇫🇮 · Vadim Guzey🇫🇮 · Ilkka Helenius🇫🇮 · Hannu Paukkunen🇫🇮

    We present numerical studies of the leading non-linear corrections to the Dokshitzer-Gribov-Lipatov-Altarelli-Parisi evolution equations of parton distribution functions (PDFs) resulting from gluon recombination. The effect of these corrections is to reduce the pace of evolution at small momentum fractions , while slightly increasing it at intermediate . By implementing the non-linear evolution in the xFitter framework, we have carried out fits of proton PDFs using data on lepton-proton deep inelastic scattering from HERA, BCDMS and NMC. While we find no evidence for the presence of non-linearities, they cannot be entirely excluded either and we are able to set limits for their strength. In terms of the recombination scale , which plays a similar role as the saturation scale in the dipole picture of the proton, we find that . We also quantify the impact of the non-linear terms for the longitudinal structure function at the Electron-Ion Collider and the Large Hadron Electron Collider and find that these measurements could provide stronger constraints on the projected effects.

    hep-phPRD(2024)·9 citations
  13. 14*

    Associated production of heavy quarkonium and meson in the improved color evaporation model with KaTie

    Alexey Chernyshev🇷🇺 · Vladimir Saleev🇷🇺

    In the article, we study associated production of prompt and mesons in the improved color evaporation model using the high-energy factorization approach as it is realized in the Monte-Carlo event generator KaTie. The modified Kimber-Martin-Ryskin-Watt model for unintegrated parton distribution functions is used. We predict cross sections for associated and meson hadroproduction via the single and double parton scattering mechanisms using the set of model parameters which has been fixed early for description of prompt single and pair heavy quarkonium production at the LHC energies. We found the results of calculations agree with the LHCb Collaboration data at the energies TeV and we present theoretical predictions for the energy TeV .

    hep-phPRD(2024)·6 citations
  14. 15*

    New physics interpretations for nonstandard values of

    Rafael Boto🇵🇹 · Dipankar Das🇮🇳 · Jorge C. Romao🇵🇹 · Ipsita Saha🇮🇳 · Joao P. Silva🇵🇹

    Current measurement of the signal strength invite us to speculate about possible new physics interactions that exclusively affect without altering the other signal strengths. Additional consideration of tree-unitarity enables us to correlate the nonstandard values of with an upper limit on the scale of new physics. We find that even when deviates from the SM value by only , the scale of new physics should be well within the reach of the LHC.

    hep-phPRD(2024)·23 citations
  15. 16*

    Fifth Force and Hyperfine Splitting in Muonic Atoms

    Jingxuan Chen🇨🇳 · Qian Wu🇨🇳 · Xurong Chen · Qian Wang🇨🇳

    The potential existence of a fifth fundamental force, mediated by the X17 boson, has generated significant interest. This force can manifest itself as either a vector or pseudoscalar particle. In order to gain insight into the effective potentials produced by the X17 boson for hyperfine interactions in muonic systems, we conduct calculations for both the pseudoscalar and vector hypotheses. Our study reveals that, for muonic atoms with nuclear charge numbers ranging from 10 to 15, the energy shift associated with the fifth force can be as high as 0.61 eV. These effects have the potential to be detected through the utilization of high-precision X-ray detectors that are used to analyze the energy spectrum of muonic characteristic X-rays.

    hep-ph0 citations
  16. 17*

    Fierz identities at the one-loop level

    Jason Aebischer🇨🇭

    One-loop Fierz identities are discussed, together with general basis transformations in Effective Field theories at the tree- and one-loop level. To this end, the notion of one-loop shifts is introduced, together with several examples that illustrate the virtues of this method.

    hep-ph0 citations
  17. 18*

    Structure of the resonance

    Jiong-Jiong Liu🇨🇳 · Zhan-Wei Liu🇨🇳 · Kan Chen🇨🇳 · Dan Guo🇨🇳 · Derek B. Leinweber🇦🇺 · Xiang Liu🇨🇳 · Anthony W. Thomas🇦🇺

    We examine the internal structure of the through an analysis of lattice QCD simulations and experimental data within Hamiltonian effective field theory. Two scenarios are presented. The first describes the as a bare three-quark basis state, which mixes with the , , and meson-baryon channels. In the second scenario, the is dynamically generated from these isospin-0 coupled channels. The scattering data and the pole structures of the and the can be simultaneously described well in both scenarios. However, a comparison of the finite-volume spectra to lattice QCD calculations reveals significant differences between these scenarios, with a clear preference for the first case. Thus the lattice QCD results play a crucial role in allowing us to distinguish between these two scenarios for the internal structure of the .

    hep-phhep-latnucl-thPRD(2024)·15 citations
  18. 19*

    Hadron Production in Ultra-relativistic Nuclear Collisions and Finite Baryon-Size Effects

    Sameer Ahmad Mir🇮🇳 · Nasir Ahmad Rather🇮🇳 · Iqbal Mohi Ud Din🇮🇳 · Saeed Uddin🇮🇳

    We investigate relative hadron yield production of various like and unlike mass particles in ultra-relativistic heavy ion collisions by employing a statistical thermal model with finite-sized baryons (antibaryons) to imitate the hard-core repulsive interactions leading to the excluded volume type effect. A strong evidence of strangeness suppression relative to the non-strange ones, mainly pions, particularly at higher energies is also observed. This study also indicates that at chemical freeze-out the particle ratios and strangeness suppression in the system obtained theoretically are sensitive to baryonic (antibaryonic) hard-core radius (). A comparison with earlier analysis involving the strangeness suppression effect is made where baryons and antibaryons were treated as point-like particles. The available experimental data showing energy dependence of various particle ratios are well described throughout the range of centre-of-mass energy (). The value of hard-core radius between 0.76 to 0.79 fm is found to fit the data quite well using minimization technique. Two different chemical freeze-out stages are found where the earlier one belongs to baryonic (hyperonic), antibaryonic (antihyperonic) states and the later one to mesonic degrees of freedom.

    hep-phnucl-thJ.Phys.G(2025)·10 citations
  19. 20*

    Probing Higgs-muon interactions at a multi-TeV muon collider

    Eugenia Celada🇬🇧 · Tao Han🇺🇸 · Wolfgang Kilian🇩🇪 · Nils Kreher🇩🇪 · Yang Ma🇮🇹 · Fabio Maltoni🇧🇪 · Davide Pagani🇮🇹 · Jürgen Reuter🇩🇪 · Tobias Striegl🇩🇪 · Keping Xie🇺🇸

    We study the capabilities of a muon collider, at 3 and 10 TeV center-of-mass energy, of probing the interactions of the Higgs boson with the muon. We consider all the possible processes involving the direct production of EW bosons ( and ) with up to five particles in the final state. We study these processes both in the HEFT and SMEFT frameworks, assuming that the dominant BSM effects originate from the muon Yukawa sector. Our study shows that a Muon Collider has sensitivity beyond the LHC, as it not only relies on the Higgs-decay branching fraction to muons. A 10 TeV muon collider provides a unique sensitivity on muon and (multi-) Higgs interactions, significantly better than the 3 TeV option. We find searches based purely on multi-Higgs production to be particularly effective in probing these couplings.

    hep-phhep-exJHEP(2024)·18 citations
  20. 21*

    Chiral perturbation theory and Bose-Einstein condensation in QCD

    Jens O. Andersen🇳🇴 · Martin Kjøllesdal Johnsrud🇳🇴 · Qing Yu🇨🇳 · Hua Zhou🇨🇳

    We present recent results in three-flavor chiral perturbation theory at finite isospin and strangeness chemical potentials at zero temperature. The phase diagram to in the -- plane is mapped out with and without electromagnetic effects. The phase diagram consists of a vacuum phase and three Bose-condensed phases with condensates of , , and , respectively. Including electromagnetic interactions, the Bose-condensed phases become Higgs phases via the Higgs mechanism. The tree-level spectrum for the mesons and gauge bosons is also derived. We calculate the pressure, energy density, isospin density, and speed of sound in the pion-condensed phase to for three-flavor PT. The results are compared with recent lattice simulations and the agreement is very good for isospin chemical potentials up to approximately 200 MeV. Moreover, by integrating out the -quark, we show that the thermodynamic quantities can be mapped onto their two-flavor counterparts with renormalized parameters. %to for two-flavor PT in the chiral limit. We also consider the nonrelativistic limit. It is shown that the energy density can be matched onto the classic result by Lee, Huang and Yang (LHY) for a dilute Bose, with an -wave scattering length that includes radiative corrections. The breaking of the symmetry in the Bose-condensed phases gives rise to a Goldstone bosons, whose dispersion is linear for momenta . In this regime, we use Son's prescription to construct an effective theory for the Goldstone field which is valid in this regime. It is shown that its damping rate is of order . This result is in agreement with Beliav's for a dilute Bose gas.

    hep-phcond-mat.quant-gashep-latPRD(2025)·13 citations
  21. 22*

    Generalized angular-order parton showers in Herwig 7

    Joon-Bin Lee🇰🇷 · M.R. Masouminia🇬🇧 · Michael H. Seymour🇬🇧 · Un-ki Yang🇰🇷

    This paper presents the inaugural investigation of beyond the Standard Model (BSM) radiation processes, framed as a generalized, process- and model-independent parton shower algorithm within Herwig 7, based on direct translations of Universal FeynRules Output (UFO) constructed via Herwig's ufo2herwig module. Leveraging the fact that shower kinematics are dictated by the spins of involved particles, we calculate comprehensive helicity-dependent branching kernels for all feasible splittings of scalars, fermions, and vector bosons, tailored to Herwig 7's angular-ordering (AO) parton shower algorithm. Utilizing these kernels, we derive BSM splitting functions in the quasi-collinear limit, ensuring compatibility with the Standard Model (SM) and supersymmetry (SUSY) splitting functions when analogous parameter conditions are applied. These newly derived functions have been integrated into the Herwig 7 event generator framework. Comparative analyses with fixed-order matrix element calculations show good agreement for single radiation events. Moreover, the results showcase the influence of BSM radiation at the Large Hadron Collider (LHC) and envisage its implications for future collider endeavours. This research augments our comprehension of BSM radiation effects, with significant bearings on present and prospective collider-based inquiries.

    hep-phJHEP(2024)·8 citations
  22. 23*

    Renormalon-based resummation of Bjorken polarised sum rule in holomorphic QCD

    César Ayala🇨🇱 · Camilo Castro-Arriaza🇨🇱 · Gorazd Cvetič🇨🇱

    Approximate knowledge of the renormalon structure of the Bjorken polarised sum rule (BSR) leads to the corresponding BSR characteristic function that allows us to evaluate the leading-twist part of BSR. In our previous work \cite{pPLB}, this evaluation (resummation) was performed using perturbative QCD (pQCD) coupling in specific renormalisation schemes. In the present paper, we continue this work, by using instead holomorphic couplings [] that have no Landau singularities and thus require, in contrast to the pQCD case, no regularisation of the resummation formula. The and terms are included in the Operator Product Expansion (OPE) of inelastic BSR, and fits are performed to the available experimental data in a specific interval where . We needed relatively high in the pQCD case since the pQCD coupling has Landau singularities at . Now, when holomorphic (AQCD) couplings are used, no such problems occur: for the AQCD and AQCD variants the preferred values are . The preferred values of in general cannot be unambiguously extracted, due to large uncertainties of the experimental BSR data. At a fixed value of , the values of the and residue parameters are determined in all cases, with the corresponding uncertainties.

    hep-phNPB(2024)·8 citations
  23. 24*

    Double Higgs production at the HL-LHC: probing a loop-enhanced model with kinematical distributions

    Leandro Da Rold🇦🇷 · Manuel Epele🇦🇷 · Anibal D. Medina🇦🇷 · Nicolás I. Mileo🇦🇷 · Alejandro Szynkman🇦🇷

    We study di-Higgs production via gluon fusion at the high luminosity LHC in the presence of new physics, focusing on the final states. Taking a minimal set of three scalar leptoquarks (LQs) with cubic and quartic interactions with the Higgs and choosing four benchmark points with a light LQ, we perform a detailed analysis of differential distributions of the di-Higgs production cross section, studying the imprints of the new physics states running in the loops. Simulating the signal and main backgrounds, we study the influence of the new physics in differential distributions such as the invariant mass of the subsystems of final particles, the transverse momentum, and angular variables, finding in particular a resonance peak associated with the light LQ. It turns out that the angular separation of the photons, which is correlated with the resonance LQ peak, is a very sensitive observable that helps in discriminating the new physics signal from the Standard Model background. We find that for two of our benchmarks discovery could be reached with 3 ab, whereas exclusion limits at 95% C.L. could be claimed with 0.60-0.75 ab. For the other two benchmarks that have heavier LQ masses significances of order 2 are possible for 3 ab. A similar analysis could be applied to other loop-enhanced models.

    hep-phhep-exJHEP(2024)·4 citations
  24. 25*

    Leptogenesis from a Phase Transition in a Dynamical Vacuum

    Dipendu Bhandari🇮🇳 · Arghyajit Datta🇰🇷 · Arunansu Sil🇮🇳

    We show that a phase transition may take place in the early Universe at a temperature via a Standard Model singlet scalar field which happens to couple to right handed neutrinos (RHN) resulting a temperature dependent mass for them that finally relaxes to a constant value after electroweak phase transition (EWPT). As a result, a requisite amount of lepton asymmetry can be produced at a temperature close to satisfying the observed baryon asymmetry of the Universe via sphaleron process even when the zero temperature masses of the RHNs fall in sub GeV regime providing a testable scenario for leptogenesis. Interestingly, the framework is also capable of predicting a primordial lepton asymmetry (generated at a temperature below the EWPT), as hinted by helium abundance measuring experiments, bearing a correlation with early phase of leptogenesis.

    hep-phastro-ph.COPRD(2024)·12 citations
  25. 26*

    Twist-3 contribution to deeply virtual electroproduction of pions

    Goran Duplančić🇭🇷 · Peter Kroll🇩🇪 · Kornelija Passek-K.🇭🇷 · Lech Szymanowski🇵🇱

    The twist-3 contribution, consisting of twist-2 transversity generalized parton distributions (GPDs) and a twist-3 meson wave function, to deeply virtual pion electroproduction is discussed. The twist-3 meson wave function includes both the and the Fock components. Two methods to regularize the end-point singularities are introduced - quark transverse momenta and a gluon mass. Using existing GPD parameterizations the transverse and the transverse-transverse interference cross sections for production are calculated and compared to experimental data.

    hep-phhep-exPRD(2024)·11 citations
  26. 27*

    A 95 GeV Higgs Boson in the Georgi-Machacek Model

    Ting-Kuo Chen🇺🇸 · Cheng-Wei Chiang🇹🇼 · Sven Heinemeyer🇪🇸 · Georg Weiglein🇩🇪

    CMS and ATLAS have reported small excesses in the search for low-mass Higgs bosons in the di-photon decay channel at exactly the same mass, GeV. These searches rely on improved analysis techniques, enhancing in particular the discrimination against the background. In models beyond the Standard Model (SM) that extend the Higgs sector with triplets, doubly-charged Higgs bosons are predicted which can contribute substantially to the di-photon decay rate of a light Higgs boson. The Georgi-Machacek (GM) Model is of particular interest in this context, since despite containing Higgs triplets it preserves the electroweak -parameter to be1 at the tree level. We show that within the GM model, a Higgs boson with a mass of GeV with a di-photon decay rate as observed by CMS and ATLAS can be well described. We discuss the di-photon excess in conjunction with an excess in the final state observed at LEP and an excess observed by CMS in the di-tau final state, which have been found at comparable masses with local significances of about and , respectively. The presence of a Higgs boson at about GeV within the GM model would imply good prospects of the searches for additional light Higgs bosons. In particular, the observed excess in the di-photon channel would be expected to be correlated in the GM model with a light doubly-charged Higgs boson in the mass range between GeV and GeV, which motivates dedicated searches in upcoming LHC Runs.

    hep-phhep-exPRD(2024)·45 citations
  27. 28*

    Two body non-leptonic decays from LCSR and implications for

    Alexander Lenz🇩🇪 · Maria Laura Piscopo🇩🇪 · Aleksey V. Rusov🇩🇪

    Motivated by the recent measurements of CP violating effects in singly Cabibbo suppressed decays, we revisit the theoretical predictions of these channels. Using up-to-date values for the decay constants and form factors, we find already within naive QCD factorisation surprisingly good agreement between the central values of the branching ratios and the corresponding experimental data. We further extend the study of these modes by employing the method of light-cone sum rules (LCSR) with light-meson light-cone distribution amplitudes. Using for the first time this framework to compute the leading contribution to the decay amplitude, we can again describe well the experimental branching ratios for the modes , , and . The combination of our results with known predictions for the penguin contributions, obtained with LCSR, leads to an upper bound for the value of direct CP violation expected in the Standard Model of which is approximately a factor six smaller than the current measurement.

    hep-phhep-exJHEP(2024)·29 citations
  28. 29*

    Introduction to the PanScales framework, version 0.1

    Melissa van Beekveld🇳🇱 · Mrinal Dasgupta🇬🇧 · Basem Kamal El-Menoufi🇬🇧 · Silvia Ferrario Ravasio🇨🇭 · Keith Hamilton🇬🇧 · Jack Helliwell🇬🇧 · Alexander Karlberg🇨🇭 · Rok Medves🇬🇧 · Pier Francesco Monni🇨🇭 · Gavin P. Salam🇬🇧 · Ludovic Scyboz🇦🇺 · Alba Soto-Ontoso🇨🇭 · Gregory Soyez🇫🇷 · Rob Verheyen🇬🇧

    In this article, we document version 0.1 of the PanScales code for parton shower simulations. With the help of a few examples, we discuss basic usage of the code, including tests of logarithmic accuracy of parton showers. We expose some of the numerical techniques underlying the logarithmic tests and include a description of how users can implement their own showers within the framework. Some of the simpler logarithmic tests can be performed in a few minutes on a modern laptop. As an early step towards phenomenology, we also outline some aspects of a preliminary interface to Pythia, for access to its hard matrix elements and its hadronisation modules.

    hep-phSciPost Phys.Codeb.(2024)·28 citations
  29. 30*

    Kaluza-Klein Spectroscopy from Neutron Oscillations into Hidden Dimensions

    Gia Dvali🇩🇪 · Manuel Ettengruber🇩🇪 · Anja Stuhlfauth🇩🇪

    Neutrons and neutrinos are natural probes for new physics. Since they carry no conserved gauge quantum numbers, both can easily mix with the fermions from hidden sectors. A particularly interesting effect is the oscillation of a neutron or a neutrino into a fermion propagating in large extra dimensions. In fact, such a mixing has been identified as the possible origin of small neutrino mass. In this paper, we study neutron oscillations into an extra-dimensional fermion and show that this effect provides a resonance imaging of the Kaluza-Klein tower. The remarkable feature of this phenomenon is its generic nature: because of a fine spacing of the Kaluza-Klein tower, neutrons at a variety of energy levels, both free or within nuclei, find a bulk oscillation partner. In particular, the partner can be a Kaluza-Klein mode of the same species that gives mass to the neutrino. The existence of bulk states matching the neutron energy levels of nuclear spectra gives rise to tight constraints as well as to potentially observable effects. For a free neutron, we predict recurrent resonant oscillations occurring with the values of the magnetic field correlated with the KK levels. We derive bounds on extra dimensions from ultra-cold neutron experiments and suggest signatures for refined measurements, which, in particular, can probe the parameter space motivated by the Hierarchy Problem. Ultra-cold neutron experiments offer a unique way of Kaluza-Klein spectroscopy.

    hep-phgr-qchep-thPRD(2024)·15 citations
  30. 31*

    Blowing in the Dark Matter Wind

    Hannah Day🇺🇸 · Da Liu🇺🇸 · Markus A. Luty🇺🇸 · Yue Zhao🇺🇸

    Interactions between dark matter and ordinary matter will transfer momentum, and therefore give rise to a force on ordinary matter due to the dark matter `wind.' We show that this force can be maximal in a realistic model of dark matter, meaning that an order-1 fraction of the dark matter momentum incident on a target of ordinary matter is reflected. The model consists of light () scalar dark matter with an effective interaction , where is an electron or nucleon field. If the coupling is repulsive and sufficiently strong, the field is excluded from ordinary matter, analogous to the Meissner effect for photons in a superconductor. We show that there is a large region of parameter space that is compatible with existing constraints, where the force is large enough to be detected by existing force probes, such as satellite tests of the equivalence principle and torsion balance experiments. However, shielding of the dark matter by ordinary matter prevents existing experiments from being sensitive to the dark matter force. We show that precise measurements of spacecraft trajectories proposed to test long distance modifications of gravity are sensitive to this force for a wide range of parameters.

    hep-phhep-exJHEP(2024)·24 citations
  31. 32*

    Phenomenology of a Deconstructed Electroweak Force

    Joe Davighi🇨🇭 · Alastair Gosnay🇬🇧 · David J Miller🇬🇧 · Sophie Renner🇬🇧

    We study an effective theory of flavour in which the interaction is `flavour-deconstructed' near the TeV scale. This arises, for example, in UV models that unify all three generations of left-handed fermions via an symmetry. Flavour-universality of the electroweak force emerges accidentally (but naturally) from breaking the gauge group to its diagonal subgroup, delivering hierarchical fermion masses and left-handed mixing angles in the process. The heavy gauge bosons transform as two triplets that mediate new flavour non-universal forces. The lighter of these couples universally to the light generations, allowing consistency with flavour bounds even for a TeV scale mass. Constraints from flavour, high mass LHC searches, and electroweak precision are then highly complementary, excluding masses below 9 TeV. The heavier triplet must instead be hundreds of TeV to be consistent with meson mixing constraints. Because only the lighter triplet couples to the Higgs, we find radiative Higgs mass corrections of a few hundred GeV, meaning this model of flavour is arguably natural. The natural region will, however, be almost completely covered by the planned electroweak programme at FCC-ee. On shorter timescales, significant parameter space will be explored by the High-Luminosity LHC measurements at high-, and upcoming lepton flavour violation experiments, principally Mu3e.

    hep-phJHEP(2024)·32 citations
  32. 33*

    Hilbert series for covariants and their applications to Minimal Flavor Violation

    Benjamín Grinstein🇺🇸 · Xiaochuan Lu🇺🇸 · Luca Merlo🇪🇸 · Pablo Quílez🇺🇸

    We elaborate how to apply the Hilbert series method to enumerating group covariants, which transform under any given representation, including but going beyond group invariants. Mathematically, group covariants form a module over the ring of the invariants. The number of independent covariants is given by the rank of the module, which can be computed by taking a ratio of two Hilbert series. In many cases, the rank equals the dimension of the group covariant representation. When this happens, we say that there is a \textit{rank saturation}. We apply this technology to revisit the hypothesis of Minimal Flavor Violation in constructing Effective Field Theories beyond the Standard Model. We find that rank saturation is guaranteed in this case, leading to the important consequence that the MFV symmetry principle does not impose any restriction on the EFT, \textit{i.e.} MFV SMEFT = SMEFT, in the absence of additional assumptions.

    hep-phhep-thJHEP(2024)·18 citations
  33. 34*

    Neutrino masses from new Weinberg-like operators: Phenomenology of TeV scalar multiplets

    Alessio Giarnetti🇮🇹 · Juan Herrero-Garcia🇪🇸 · Simone Marciano🇮🇹 · Davide Meloni🇮🇹 · Drona Vatsyayan🇪🇸

    The unique dimension- effective operator, , known as the Weinberg operator, generates tiny Majorana masses for neutrinos after electroweak spontaneous symmetry breaking. If there are new scalar multiplets that take vacuum expectation values (VEVs), they should not be far from the electroweak scale. Consequently, they may generate new dimension- Weinberg-like operators which in turn also contribute to Majorana neutrino masses. In this study, we consider scenarios with one or two new scalars up to quintuplet SU(2) representations. We analyse the scalar potentials, studying whether the new VEVs can be induced and therefore are naturally suppressed, as well as the potential existence of pseudo-Nambu-Goldstone bosons. Additionally, we also obtain general limits on the new scalar multiplets from direct searches at colliders, loop corrections to electroweak precision tests and the -boson mass.

    hep-phJHEP(2024)·19 citations
  34. 35*

    An EFT approach to baryon number violation: lower limits on the new physics scale and correlations between nucleon decay modes

    Arnau Bas i Beneito🇪🇸 · John Gargalionis🇪🇸 · Juan Herrero-Garcia🇪🇸 · Arcadi Santamaria🇪🇸 · Michael A. Schmidt🇦🇺

    Baryon number is an accidental symmetry of the Standard Model at the Lagrangian level. Its violation is arguably one of the most compelling phenomena predicted by physics beyond the Standard Model. Furthermore, there is a large experimental effort to search for it including the Hyper-K, DUNE, JUNO, and THEIA experiments. Therefore, an agnostic, model-independent, analysis of baryon number violation using the power of Effective Field Theory is very timely. In particular, in this work we study the contribution of dimension six and seven effective operators to nucleon decays taking into account the effects of Renormalisation Group Evolution. We obtain lower limits on the energy scale of each operator and study the correlations between different decay modes. We find that for some operators the effect of running is very significant.

    hep-phJHEP(2024)·37 citations
  35. 36*

    JLab spectral functions of argon in NuWro and their implications for MicroBooNE

    Rwik Dharmapal Banerjee🇵🇱 · Artur M. Ankowski🇵🇱 · Krzysztof M. Graczyk🇵🇱 · Beata E. Kowal🇵🇱 · Hemant Prasad🇵🇱 · Jan T. Sobczyk🇵🇱

    The Short-Baseline Neutrino program in Fermilab aims to resolve the nature of the low-energy excess events observed in LSND and MiniBooNE, and analyze with unprecedented precision neutrino interactions with argon. These studies require reliable estimate of neutrino cross sections, in particular for charged current quasielastic scattering (CCQE). Here, we report updates of the NuWro Monte Carlo generator that, most notably, bring the state-of-the-art spectral functions to model the ground state properties of the argon nucleus, and improve the accuracy of the cross sections at low energies by accounting for the effects of the nuclear Coulomb potential. We discuss these developments in the context of electron and neutrino interactions, by comparing updated NuWro predictions to experimental data from Jefferson Laboratory Hall A and MicroBooNE. The MicroBooNE CCQE data are described with the per degree of freedom of 0.7, compared with 1.0 in the local Fermi gas model. The largest improvement is observed for the angular distributions of the produced protons, where the reduces nearly by half. Being obtained using the axial form factor parametrization from MINERvA, our results indicate a~consistency between the CCQE measurements in MINERvA and MicroBooNE.

    hep-phnucl-thPRD(2024)·16 citations
  36. 37*

    iDMEu: An initiative for Dark Matter in Europe and beyond

    Marco Cirelli🇫🇷 · Caterina Doglioni🇬🇧 · Federica Petricca🇩🇪

    We introduce the initiative for Dark Matter in Europe and beyond (iDMEu), a collective effort by a group of particle and astroparticle physicists to set up an online resource meta-repository, a common discussion platform and a series of meetings on everything concerning Dark Matter. This document serves as a status report as well as a citable item concerning iDMEu.

    hep-phastro-ph.COastro-ph.GAhep-ex+1PoS(2024)·1 citation
  37. 38*

    One and Two-Body Current Contributions to Lepton-Nucleus Scattering

    Alessandro Lovato🇺🇸 · Noemi Rocco🇺🇸 · Noah Steinberg🇺🇸

    Modeling lepton-nucleus scattering with the accuracy required to extract neutrino-oscillation parameters from long- and short-baseline experiments necessitates retaining most quantum-mechanical effects. One such effect is the interference between one- and two-body current operators in the transition currents, which has been known to enhance the cross-sections, especially in transverse kinematics. In this work, we incorporate such interference in the spectral function formalism, which combines relativistic currents and kinematics with an accurate description of the initial target state. Our analysis of lepton-scattering off C demonstrates that interference effects appreciably enhance the transverse electromagnetic response functions and the flux-folded neutrino-nucleus cross section, in both cases, improving the agreement with experimental data. We discuss the impact on the neutrino-oscillation program and the determination of nucleon axial form factors.

    nucl-thhep-phPRC(2025)·22 citations
  38. 39*

    The role of longitudinal decorrelations for measurements of anisotropic flow in small collision systems

    Sangwook Ryu🇺🇸 · Bjoern Schenke🇺🇸 · Chun Shen🇺🇸 · Wenbin Zhao🇺🇸

    Within a (3+1)D viscous hydrodynamic model we compute anisotropic flow in small system collisions as performed at the Relativistic Heavy Ion Collider and measured by the STAR and PHENIX Collaborations. We emphasize the importance of the rapidity dependence of the geometry for interpreting the differences encountered in measurements by the two collaborations.

    nucl-thhep-phnucl-exEPJ Web Conf.(2024)·5 citations
  39. 40*

    Schwinger-Unruh-Hawking radiation on manifolds

    Tomohiro Matsuda🇯🇵

    The whole picture of gauge theory is described by manifolds, while the field equation provides only a part (a section) of the manifold. Just as a three-dimensional object is reconstructed from two planar images, a monopole is constructed by combining two solutions. The Schwinger and the Unruh effects and the Hawking radiation are the production of particles out of the ``vacuum''. If the '''vacuum'' on the manifold is properly defined, these phenomena should be described as local phenomena. However, calculations using the field equations have so far resulted in unnatural extrapolations. We present a method for properly defining the ``vacuum'' and explain how to resolve the local particle production on manifolds. By defining the Stokes phenomena on the manifold, the Schwinger effect is naturally accompanied by the Unruh effect. Also, unlike the conventional Unruh effect, calculations on manifolds do not suffer from the entanglement between disconnected wedges.

    hep-thgr-qchep-ph0 citations
  40. 41*

    What is the correct definition of entropy for general relativistic field theory?

    Shuichi Yokoyama🇯🇵

    Recently, the author and collaborators proposed a method to construct a new conserved charge different from the Noether one for general relativistic field theory on curved space-time with energy-momentum tensor covariantly conserved, and that the new conserved charge describes the entropy of the system. As concrete evidence of the proposals, it was shown that such a new conserved charge indeed exists for several classic gravitational systems, and that the proposed entropy density computed in them satisfies the local Euler's relation and the first law of thermodynamics concurrently and non-perturbatively with respect to the Newton constant. These developments are reviewed including brief discussions of physical implications of the local thermodynamic relations.

    hep-thastro-ph.SRgr-qchep-phPoS(2024)·1 citation
  41. 42*

    Probing light scalars with not quite black holes

    Ximeng Li🇨🇳 · Jing Ren🇨🇳

    The rapid progress in gravitational wave astronomy has provided an opportunity for investigating the presence of long-range scalar forces that exclusively manifest around astrophysical black holes. In this paper, we explore a new possibility in this context, particularly in connection to the hypothesis that astrophysical black holes might be horizonless ultracompact objects (UCOs). In the absence of horizons, UCOs could feature unique interiors with extreme environments. This could help generate non-trivial scalar profiles and significant scalar charges. For demonstration, we consider 2-2-holes in quadratic gravity as a concrete example of UCOs. These objects can be formed by ordinary gases and closely resemble black holes externally. However, they have distinct interiors characterized by high curvatures and substantial redshift. In particular, the gases inside could reach extremely high temperatures or densities, making them an ideal object for investigating the generation of scalar profiles by UCOs. Within a minimal model of the scalar field, we find that this unique environment enables the generation of a substantial scalar charge for astrophysical 2-2-holes, which is challenging for other stellar objects. The predicted scalar charge-to-mass ratio of 2-2-holes remains nearly constant across a wide range of masses, offering different predictions for gravitational wave observations compared to other mechanisms.

    gr-qchep-phPRD(2024)·3 citations
  42. 43*

    Explicit form for the most general Lorentz transformation revisited

    Howard E. Haber🇺🇸

    Explicit formulae for the Lorentz transformation matrices corresponding to a pure boost and a pure three-dimensional rotation are very well-known. Significantly less well-known is the explicit formula for a general Lorentz transformation with arbitrary nonzero boost and rotation parameters. We revisit this more general formula by presenting two different derivations. The first derivation (which is somewhat simpler than previous ones appearing in the literature) evaluates the exponential of a real matrix , where is a product of the diagonal matrix and an arbitrary real antisymmetric matrix. The formula for depends only on the eigenvalues of and makes use of the Lagrange interpolating polynomial. The second derivation exploits the observation that the spinor product \eta^\dagger\overline{\sigma}^{\lower3pt\hbox{\scriptstyle \mu}}\chi transforms as a Lorentz four-vector, where and are two-component spinors. The advantage of the latter derivation is that the corresponding formula for a general Lorentz transformation reduces to the computation of the trace of a product of matrices. Both computations are shown to yield equivalent expressions for .

    physics.class-phhep-phSymmetry(2024)·4 citations
  43. 44*

    An effective field theory of damped ferromagnetic systems

    Jingping Li🇺🇸

    Using the in-in formalism, we generalize the recently constructed magnetoelastic EFT arXiv:2112.13873 [hep-th] to describe the damping dynamics of ferromagnetic systems at long wavelengths. We find that the standard Gilbert damping term naturally arises as the simplest leading-order symmetry-consistent non-conservative contribution within the in-in framework. The EFT is easily generalized to scenarios with anisotropy and inhomogeneity. In particular, we find the classic Landau-Lifshitz damping term emerges when isotropy is broken by a constant external background field. This provides a first principle explanation for distinguishing the two types of damping dynamics that were originally constructed phenomenologically. Furthermore, the EFT framework could also incorporate intrinsic anisotropy of the material in a straightforward way using the spurion method. For systems with inhomogeneity such as nontrivial spin textures, we find that the leading order derivative correction yields the generalized Gilbert damping equations that were found in condensed matter literature. This shows that the EFT approach enables us to derive the form of higher-derivative-order corrections in a systematic way. Lastly, using the phonon-magnon coupling deduced in the magnetoelastic EFT, we are able to make a prediction for the generic form of the phononic contribution to the damping equation.

    hep-thcond-mat.mes-hallhep-phnucl-th1 citation
  44. 45*

    Neutrino spin oscillations in gravitational fields in noncommutative higher dimensions

    S.A. Alavi🇮🇷 · T. Fallahi Serish🇮🇷

    Investigation of neutrino spin oscillation in the gravitational fields of black holes (BHs) is one of the interesting topics in neutrino physics. On the other hand, in recent years, many studies have been devoted to the exploration of different physical phenomena in higher dimensions. Non-commutative geometry has also been focus of researchers in recent years to explore the structure of space-time more deeply and accurately. In this work, the neutrino spin oscillation in the non-commutative higher dimensional gravitational fields of Schwarzschild and Reissner Nordstrom metrics is studied. The effects of noncommutativity of space are calculated and its role in different dimensions is discussed. Considering the fact that in the non-commutative space, for certain values of eta, no event horizon exists and consequently, there will be no BH, some upper bounds for the non-commutative parameter are obtained.

    hep-thastro-ph.HEgr-qchep-phMod.Phys.Lett.A(2025)·0 citations
  45. 46*

    Photons from neutrinos: the gamma ray echo of a supernova neutrino burst

    Cecilia Lunardini🇺🇸 · Joshua Loeffler🇺🇸 · Mainak Mukhopadhyay🇺🇸 · Matthew J. Hurley🇺🇸 · Ebraheem Farag🇺🇸 · F. X. Timmes🇺🇸

    When a star undergoes core collapse, a vast amount of energy is released in a ~10 s long burst of neutrinos of all species. Inverse beta decay in the star's hydrogen envelope causes an electromagnetic cascade which ultimately results in a flare of gamma rays - an "echo" of the neutrino burst - at the characteristic energy of 0.511 MeV. We study the phenomenology and detectability of this flare. Its luminosity curve is characterized by a fast, seconds-long, rise and an equally fast decline, with a minute- or hour-long plateau in between. For a near-Earth star (distance D<1 kpc) the echo will be observable at near future gamma ray telescopes with an effective area of 10^3 cm^2 or larger. Its observation will inform us on the envelope size and composition. In conjunction with the direct detection of the neutrino burst, it will also give information on the neutrino emission away from the line of sight and will enable tests of neutrino propagation effects between the stellar surface and Earth.

    astro-ph.HEhep-phnucl-thApJ(2024)·1 citation
  46. 47*

    Starobinsky Inflation in the Swampland

    Dieter Lust🇩🇪 · Joaquin Masias🇩🇪 · Benjamin Muntz🇩🇪 · Marco Scalisi🇩🇪

    We argue that the Starobinsky model of inflation, realised via an term in the Lagrangian, can originate from quantum effects due to a tower of light species. By means of two separate arguments, we show how this implies that the scale of the term must be of order of the species scale , namely the energy at which gravity becomes strongly coupled. We discuss the implications and challenges of this scenario for inflation, inflationary reheating, and string theory embeddings. In this context, we collect strong evidence to conclude that Starobinsky inflation lies in the Swampland.

    hep-thastro-ph.COgr-qchep-phJHEP(2024)·41 citations
  47. 48*

    Gravity-gauge Anomaly Constraints on the Energy-momentum Tensor

    Rémy Larue🇫🇷 · Jérémie Quevillon🇫🇷 · Roman Zwicky🇬🇧

    We derive constraints on the four dimensional energy-momentum tensor from gravitational and gauge anomalies. Our work can be considered an extension of Duff's analysis [1] to include parity-odd terms and explicit symmetry breaking. The constraints imply the absence of the parity-odd and terms, for theories whose symmetries are compatible with dimensional regularisation, in a model-independent way. Remarkably, even in the case of explicit symmetry breaking the -anomaly is found to be finite and unambiguous after applying the symmetry constraints. We compute mixed gravity-gauge anomalies at leading order and deduce phenomenological consequences for vector bosons associated with global chiral symmetries.

    hep-thgr-qchep-phJHEP(2024)·15 citations
  48. 49*

    Inflation (2025)

    John Ellis🇬🇧 · Vincent Vennin🇫🇷 · David Wands🇬🇧

    This is a review article for The Review of Particle Physics 2026 (aka the Particle Data Book), appearing as Chapter 23. It forms a compact review of our understanding of cosmological inflation near the end of 2025. Topics included are Scalar Field Cosmology; Primordial Perturbations from Inflation; Models; Model Comparison; Constraints on Reheating; Beyond Single-Field Inflation; Initial-conditions and Fine-tuning; Future Probes of Inflation.

    astro-ph.COhep-phhep-thPhys. Rev. D 110, 030001 (2024) and 2025 …·42 citations
  49. 50*

    SENSEI: First Direct-Detection Results on sub-GeV Dark Matter from SENSEI at SNOLAB

    SENSEI Collaboration: Prakruth Adari🇺🇸 · Itay M. Bloch🇺🇸 · Ana M. Botti🇺🇸 · Mariano Cababie🇦🇷 · Gustavo Cancelo🇺🇸 · Brenda A. Cervantes-Vergara🇲🇽 · Michael Crisler🇺🇸 · Miguel Daal🇮🇱 · Ansh Desai🇺🇸 · Alex Drlica-Wagner🇺🇸 · Rouven Essig🇺🇸 · Juan Estrada🇺🇸 and 24 other authors

    We present the first results from a dark matter search using six Skipper-CCDs in the SENSEI detector operating at SNOLAB. We employ a bias-mitigation technique of hiding approximately 46% of our total data and aggressively mask images to remove backgrounds. Given a total exposure after masking of 100.72 gram-days from well-performing sensors, we observe 55 two-electron events, 4 three-electron events, and no events containing 4 to 10 electrons. The two-electron events are consistent with pileup from one-electron events. Among the 4 three-electron events, 2 appear in pixels that are likely impacted by detector defects, although not strongly enough to trigger our "hot-pixel" mask. We use these data to set world-leading constraints on sub-GeV dark matter interacting with electrons and nuclei.

    astro-ph.COhep-exhep-phphysics.ins-detPRL(2025)·186 citations
  50. 51*

    Non-Polynomial Interactions as a Path Towards a Non-Renormalizable UV-Completion

    Mikhail Shaposhnikov🇨🇭 · Sebastian Zell🇧🇪

    We propose a new class of single-field scalar quantum field theories with non-polynomial interactions leading to a two-point Green's function that can be naturally continued beyond the naive cutoff scale. This provides a new prospect for self-completing theories in the UV-domain. In our approach, the formal power series for the scalar potential has a vanishing radius of convergence and is defined through Borel resummation. We discuss concrete examples, among others with a spectral function that vanishes at large momenta, potentially leading to an asymptotically free theory. Finally, we give an outlook on future research, with a view towards possible applications to inflation and gravity.

    hep-thhep-phPLB(2024)·3 citations
  51. 52*

    Bubble velocities and oscillon precursors in first-order phase transitions

    Dalila Pîrvu🇨🇦 · Matthew C. Johnson🇨🇦 · Sergey Sibiryakov🇨🇦

    Metastable `false' vacuum states are an important feature of the Standard Model of particle physics and many theories beyond it. Describing the dynamics of a phase transition out of a false vacuum via the nucleation of bubbles is essential for understanding the cosmology of vacuum decay and the full spectrum of observables. In this paper, we study vacuum decay by numerically evolving ensembles of field theories in 1+1 dimensions from a metastable state. We demonstrate that for an initial Bose-Einstein distribution of fluctuations, bubbles form with a Gaussian spread of center-of-mass velocities and that bubble nucleation events are preceded by an oscillon -- a long-lived, time-dependent, pseudo-stable configuration of the field. Defining an effective temperature from the long-wavelength amplitude of fluctuations in the ensemble of simulations, we find good agreement between theoretical finite temperature predictions and empirical measurements of the decay rate, velocity distribution and critical bubble solution. We comment on the generalization of our results and the implications for cosmological observables.

    hep-thastro-ph.COhep-lathep-phJHEP(2024)·29 citations
  52. 53*

    Proton and neutron electromagnetic radii and magnetic moments from lattice QCD

    Miguel Salg🇩🇪 · Dalibor Djukanovic🇩🇪 · Georg von Hippel🇩🇪 · Harvey B. Meyer🇩🇪 · Konstantin Ottnad🇩🇪 · Hartmut Wittig🇩🇪

    We present results for the electromagnetic form factors of the proton and neutron computed on the -flavor Coordinated Lattice Simulations (CLS) ensembles including both quark-connected and -disconnected contributions. The -, pion-mass, lattice-spacing, and finite-volume dependence of our form factor data is fitted simultaneously to the expressions resulting from covariant chiral perturbation theory including vector mesons amended by models for lattice artefacts. From these fits, we determine the electric and magnetic radii and the magnetic moments of the proton and neutron, as well as the Zemach radius of the proton. To assess the influence of systematic effects, we average over various cuts in the pion mass and the momentum transfer, as well as over different models for the lattice-spacing and finite-volume dependence, using weights derived from the Akaike Information Criterion (AIC).

    hep-lathep-phnucl-thEPJ Web Conf.(2024)·1 citation

* 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.