PaperPanorama

HEP Phenomenology·hep-ph

Thu·Jul 17, 2025

28 papers19 primary·9 cross-listed·reconstructed*

  1. 01*

    QED-IR as Topological Quantum Theory of Dressed States

    J. Gamboa🇨🇳 · F. Mendez🇨🇳

    We investigate quantum electrodynamics in the infrared regime (QED-IR) using the adiabatic approximation and the framework of the functional Berry phase. In this approach, the physical state space is exact, nonperturbatively dressed, and endowed with a topological structure. Electrons do not exist as bare particles, but as topologically protected electron--photon clouds, defining a new kind of ``infrared quantum''. These clouds are weakly bound in energy (with a binding scale estimated at \(\Lambda_{\mathrm{IR}} \sim 0.5~\mathrm{meV}\)) and remain stable provided photon energies stay below this threshold. Crucially, the theory becomes exactly solvable in this regime due to the quantization of the functional Berry flux, which governs the infrared dynamics of the dressed states. When hard (high-energy) processes are involved, the topological protection of the dressed states is lifted, and the theory smoothly recovers conventional perturbative QED. In contrast, in the deep infrared, the electromagnetic interaction never fully vanishes, leading to observable effects. We argue that the energy required to dissolve the infrared electron--photon cloud in QED is of order \(\mathrm{meV}\), comparable to the thermal energy of the cosmic microwave background (CMB), \(k_B T_{\mathrm{CMB}} \approx 2.3 \times 10^{-4}\,\mathrm{eV}\). However, the observed temperature anisotropies correspond to fluctuations near \(10^{-9}\,\mathrm{eV}\), far too small to destroy the cloud, though potentially capable of perturbing its topological phase structure. This suggests that CMB deviations could reflect residual topological imprints of the functional infrared dynamics. Finally, we propose that analogous cloud-like structures may manifest in other quantum systems governed by low-energy photon dynamics, such as atomic and molecular environments.

    hep-phhep-thJHEP(2025)·9 citations
  2. 02*

    Comprehensive investigation on baryon number violating nucleon decays involving an axion-like particle

    Wei-Qi Fan🇨🇳 · Yi Liao🇨🇳 · Xiao-Dong Ma🇨🇳 · Hao-Lin Wang🇨🇳

    In this study, we systematically investigate baryon number violating (BNV) nucleon decays into an axion-like particle (ALP), within a low energy effective field theory extended with an ALP, which is referred to as aLEFT. Unlike previous studies in the literature, we consider contributions to nucleon decays from a complete set of dimension-eight BNV aLEFT operators involving light and quarks. We perform the chiral irreducible representation (irrep) decomposition of these interactions under the QCD chiral group , and match them onto the recently developed chiral framework to obtain nucleon-level effective interactions among the ALP, octet baryons, and octet pseudoscalar mesons. Within this framework, we derive general expressions for the decay widths of nucleon two- and three-body decays involving an ALP. Subsequently, we analyze momentum distributions for three-body modes and find that operators belonging to the newly identified chiral irreps exhibit markedly different behavior compared to that in the usual irreps and . In addition, we reanalyze experimental data collected by Super-Kamiokande and establish bounds on the inverse decay widths of these new modes by properly accounting for experimental efficiencies and Cherenkov threshold effects because of the lack of direct constraints on those exotic decay modes. Our recasting constraints are several orders of magnitude more stringent than inclusive bounds used in the literature. Based on these improved bounds, we set conservative limits on associated effective scales across a broad range of ALP mass and predict stringent bounds on certain neutron and hyperon decays involving an ALP.

    hep-phCPC(2026)·9 citations
  3. 03*

    Fully strange tetraquark states via QCD sum rules

    Bing-Dong Wan🇨🇳 · Ji-Chong Yang🇨🇳

    In this paper, we have systematically explored the mass spectrum of fully strange tetraquark candidates within the framework of QCD sum rules, focusing on states with quantum numbers , , , , , and . The analysis reveals the existence of fully strange tetraquark states with masses ranging from approximately to GeV. These predictions are confronted with existing experimental observations of potential fully strange tetraquark resonances, notably the recently reported by the BESIII Collaboration, which may be interpreted as a fully strange tetraquark state. Furthermore, the possible decay modes of these fully strange tetraquark states are analyzed, providing guidance for their identification in current and future high energy experiments such as BESIII, Belle II, and LHCb.

    hep-phCPC(2026)·12 citations
  4. 04*

    A radiative lepton model in a non-invertible fusion rule

    Jingqian Chen🇨🇳 · Chao-Qiang Geng🇨🇳 · Hiroshi Okada🇨🇳 · Jia-Jun Wu🇨🇳

    We propose a new mechanism in which electron and muon masses are induced at one-loop level after dynamically violating the symmetry of the Ising fusion rule. In the neutrino sector, while the neutrino mass is generated at one-loop level, the Ising fusion rule plays a role in stabilizing the particles inside the loop. As a result, the symmetry works like a symmetry that is not broken at any loop order. Subsequently, we discuss the lepton flavor violating processes, muon anomalous magnetic dipole moment, and relic density of dark matter, where we specify our dark matter candidate to be a singlet boson and briefly analyze the relic density by estimating the DM annihilation cross section. Finally, we present results for both the DM cross section and the muon , satisfying the neutrino oscillation data as well as the constraints of lepton flavor violations.

    hep-phNPB(2026)·24 citations
  5. 05*

    High spin kaons

    Ya-Rong Wang🇨🇳 · Hao Chen🇨🇳 · Xiao-Hai Liu🇨🇳 · Cheng-Qun Pang🇨🇳

    The COMPASS Collaboration recently reported the observation of strange-meson spectra in the reaction and found and states, with masses of MeV and MeV, respectively. This discovery has significantly renewed interest, prompting a detailed and systematic study of high-spin kaons. In this work, we analyze the mass spectrum and the Okubo-Zweig-Iizuka-allowed two-body strong decay properties of high-spin kaons having , and within the framework of the modified Godfrey-Isgur model and the model. Moreover, we identify critical decay channels, which may serve as useful guidance for future experimental studies.

    hep-phPRD(2025)·2 citations
  6. 06*

    Torsion induced current-scalaron coupling in Einstein-Cartan gravity

    Minxi He🇰🇷 · Muzi Hong🇯🇵 · Kyohei Mukaida🇯🇵

    We investigate the matter current couplings with the scalar degrees of freedom originated from the torsion in Einstein-Cartan (EC) gravity. It has been shown in previous studies that the presence of the operators consisting of torsion components up to dimension four can naturally induce a (pseudo-)scalar degree of freedom, the scalaron. In this work, we consider the couplings between torsion and matter currents in this framework, and show that they can lead to couplings between these currents and the scalaron in the equivalent metric theory. We consider both gauge-invariant and gauge-dependent currents, showing general results and several concrete examples. These results are useful for the discussion of particle production processes after inflation in the EC framework, such as reheating and baryogenesis, and show the connection to the QCD term.

    hep-phastro-ph.COgr-qcJCAP(2026)·7 citations
  7. 07*

    Bias with a Timer: Axion Domain Wall Decay and Dark Matter

    Sally Yuxuan Hao🇨🇳 · Shota Nakagawa🇨🇳 · Yuichiro Nakai🇨🇳 · Motoo Suzuki🇮🇹

    We explore the interplay of the post-inflationary QCD axion and a light scalar field for the axion domain wall decay and dark matter (DM). The scalar field possesses a nonzero vacuum expectation value (VEV) during inflation, so that its interaction with the axion effectively serves as an explicit Peccei-Quinn (PQ) violating term. At a temperature below the PQ phase transition, the effective PQ violating interaction generates the axion potential which generally contains multiple degenerate vacua leading to the formation of the axion string-domain wall networks. The following QCD phase transition provides another contribution to the axion potential making domain walls decay before they dominate the Universe. Later, the scalar field starts to relax to the minimum of its potential with a vanishing VEV, turning off the effective PQ violating interaction so that the axion potential is aligned with the QCD vacuum. We keep track of the evolution of the axion-scalar system and discuss the production of the axion DM through the domain wall decay and the (trapped) misalignment. We find that the string-wall network in some cases can decay due to its structural instability, rather than the volume pressure, and the correct axion DM abundance is realized with the decay constant larger than that of the conventional post-inflationary QCD axion without fine tuning.

    hep-phastro-ph.COhep-thJHEP(2026)·3 citations
  8. 08*

    No Hiding in the Dark: Cosmological Bounds on Heavy Neutral Leptons with Dark Decay Channels

    P. S. Bhupal Dev🇺🇸 · Quan-feng Wu🇨🇳 · Xun-Jie Xu🇨🇳

    Heavy neutral leptons (HNLs) are well-motivated new physics candidates. The mixing of sub-GeV HNLs with active neutrinos is severely constrained by cosmology. In particular, the success of Big Bang Nucleosynthesis (BBN) requires the HNL lifetime to be shorter than about 0.02 sec if they were in thermal equilibrium, thus excluding a wide range of mixing angles accessible to terrestrial experiments. In order to justify the laboratory searches in this cosmologically-forbidden region, it is often argued that adding new dark sector decay modes of HNLs can evade the stringent BBN constraint. Here we rule out this possibility and show that, contrary to the naive expectation, HNLs with significant dark decay modes actually lead to stronger cosmological bounds. This is mainly because of the increase in the extra radiation energy density in the Universe around the BBN epoch, which causes observable effects in the primordial helium fraction and . Our result has major implications for laboratory searches of HNLs.

    hep-phastro-ph.COhep-exPRD(2026)·12 citations
  9. 09*

    Boosted dark matter versus dark matter-induced neutrinos from single and stacked blazars

    Andrea Giovanni De Marchi🇮🇹 · Alessandro Granelli🇮🇹 · Jacopo Nava🇮🇹 · Filippo Sala🇮🇹

    The physics responsible for the production of observed high-energy neutrinos have not been established so far, neither for the diffuse astrophysical ones nor for those detected from single blazars. We recently proposed that both could be explained by deep inelastic scatterings between sub-GeV dark matter (DM) around blazars and protons within their jets. Here, we compute the proton-recoil signals at the neutrino detectors Super-Kamiokande, KamLAND, Borexino, JUNO, Hyper-Kamiokande and DUNE induced by DM that is itself boosted by the scatterings with protons in blazar jets. We do it for the four cases of vector, axial, scalar and pseudoscalar mediators of DM-quark interactions. We perform the analysis for the single blazar TXS 0506+056 and for a sample of more than 300 stacked blazars. We find that searches for such blazar-boosted DM leave room for a variety of DM models to explain observations of high-energy neutrinos. We check that the depletion of the DM spike induced by DM-proton and DM-DM interactions does not compromise the DM interpretation for high-energy neutrinos, but challenges other blazar-DM signals.

    hep-phastro-ph.HEJHEP(2025)·16 citations
  10. 10*

    Bulk viscosity and -component fluids

    Saga Säppi🇪🇸

    Understanding the hydrodynamics of out-of-equilibrium dense viscous fluids is of key importance to accurate descriptions of physical systems such as compact stars, particularly their mergers. We consider a near-equilibrium relativistic fluid with independent and small chemical potentials restoring the system back towards equilibrium. By diagonalising the evolution equation for the out-of-equilibrium chemical potentials, we construct an explicit evolution equation for the bulk scalar of the system in second-order hydrodynamics in terms of equilibrium quantities. We find expressions for the transport quantities and show that in the rest frame of the fluid, the system admits a Green's function corresponding to an -component fluid.

    hep-phgr-qchep-thnucl-thPRD(2026)·1 citation
  11. 11*

    Do Cosmic String Segments Emit Gravitational Waves?

    Akifumi Chitose🇯🇵 · Masahiro Ibe🇯🇵 · Shunsuke Neda🇯🇵 · Satoshi Shirai🇯🇵

    Cosmic strings are predicted in various extensions of the Standard Model, including grand unified theories. Depending on the symmetry-breaking pattern, they can be either topologically stable or metastable. Intriguingly, metastable strings have been proposed as a possible origin of the gravitational wave (GW) background observed by recent pulsar timing array experiments. When metastable strings decay, they fragment into segments with monopoles and antimonopoles attached at their endpoints. The monopole and antimonopole are strongly pulled by the string tension. Violent oscillations of these segments have been considered as a potential GW source, in addition to contributions from string loops. We show that, in realistic situations, the monopoles frequently collide with thermal fluctuations on the string segments, which act as a resistance and prevent the oscillation. As a result, we find that the contribution from string segments to the GW background is negligible.

    hep-phastro-ph.CO9 citations
  12. 12*

    Quantum Tomography in Neutral Meson and Antimeson Systems

    Kun Cheng🇺🇸 · Tao Han🇺🇸 · Matthew Low🇺🇸 · Tong Arthur Wu🇺🇸

    The flavor space of particles produced in collider environments contains informative quantum correlations. We present a systematic approach for constructing the complete flavor density matrix for a meson and antimeson system () in the Bloch vector space at a given time , which can be at or after production. We point out that the and systems are superior to the and systems for quantum tomography because of their flavor oscillation and decay properties. Performing quantum tomography for the system can facilitate the study of production mechanisms, decoherence phenomena, quantum information variables, and potential new sources of CP violation.

    hep-phhep-exquant-phPRL(2026)·17 citations
  13. 13*

    Natural Ultralight Dark Matter: The Quadratic Twin

    Cédric Delaunay🇫🇷 · Michael Geller🇮🇱 · Zamir Heller-Algazi🇮🇱 · Gilad Perez🇮🇱 · Konstantin Springmann🇮🇱

    Scalar ultralight dark matter (ULDM) is uniquely accessible to tabletop experiments such as clocks and interferometers, and its search has been the focus of a vast experimental effort. However, the scalar ULDM mass is not protected from radiative corrections, and the entirety of the parameter space within reach of experiments suffers from a severe naturalness problem. In this paper, we propose a new twin mechanism that protects the mass of the scalar ULDM. Our scalar ULDM is a pseudo-Nambu-Goldstone boson with quadratic couplings to the Standard Model (SM) and to a twin copy of the SM, with a mirror symmetry exchanging each SM particle with its twin. Due to the mirror symmetry, the leading-order mass correction is quadratic in the (tiny) coupling while the linear order is canceled. This opens up vast regions of parameter space for natural quadratically coupled ultralight dark matter, within the sensitivity of existing and future experiments.

    hep-phPRD(2026)·17 citations
  14. 14*

    Multi-loop spectra in general scalar EFTs and CFTs

    Johan Henriksson🇨🇭 · Franz Herzog🇬🇧 · Stefanos R. Kousvos🇮🇹 · Jasper Roosmale Nepveu🇹🇼

    We consider the most general effective field theory (EFT) Lagrangian with scalar fields and derivatives, and renormalise it to substantially higher loop order than existing results in the literature. EFT Lagrangians have phenomenological applications, for example by encoding corrections to the Standard Model from unknown new physics. At the same time, scalar EFTs capture the spectrum of Wilson--Fisher conformal field theories (CFTs) in dimensions. Our results are enabled by a more efficient version of the method for renormalisation, in which the IR divergences are subtracted via a small-momentum asymptotic expansion. In particular, we renormalise the most general set of composite operators up to engineering dimension six and Lorentz rank two. We exhibit direct applications of our results to Ising (), , and hypercubic () CFTs, relevant for a plethora of real-world critical phenomena. The computed scaling dimensions agree well with known non-perturbative results, and they lead to new predictions where such results do not yet exist. We thereby expand the understanding of generic EFTs and open new possibilities in diverse fields, such as the numerical conformal bootstrap.

    hep-phcond-mat.stat-mechhep-thPLB(2026)·21 citations
  15. 15*

    A Step in Flux to Suppress Axion Isocurvature

    Priyesh Chakraborty🇺🇸 · Junyi Cheng🇺🇸 · Matthew Reece🇺🇸 · Zekai Wang🇨🇳

    The QCD axion in the pre-inflation scenario faces a stringent isocurvature constraint, which requires a relatively low Hubble scale during inflation. If the axion was heavier than the Hubble scale during inflation, its isocurvature is suppressed and the constraint disappears. We point out a novel mechanism for achieving this, relying on the topological nature of a BF-type (monodromy) mass for the axion. Such a mass term has an integer coefficient, so it could naturally have been very large during inflation and exactly zero by the time of the QCD phase transition. This integer can be viewed as a quantized flux, which is discharged in a first-order phase transition that proceeds by the nucleation of charged branes. This mechanism can be embedded in cosmology in several different ways, with tunneling during, at the end of, or after inflation. We provide a detailed case study of the scenario in which the tunneling event occurs during inflation. We also comment briefly on possible UV completions within extra-dimensional gauge theories and string theory. Intriguingly, the phase transition could be accompanied by the emergence of the chiral Standard Model field content from a non-chiral theory during inflation.

    hep-phastro-ph.COhep-thJHEP(2026)·7 citations
  16. 16*

    Sommerfeld Enhancement from Quantum Forces for Dark Matter

    Steven Ferrante🇺🇸 · Maxim Perelstein🇺🇸 · Bingrong Yu🇺🇸

    Quantum forces are long-range interactions that arise only at the loop level. In this work, we study the Sommerfeld enhancement of dark matter (DM) annihilation cross sections caused by quantum forces. One notable feature of quantum forces is that they are subject to coherent enhancement in the presence of a background of mediator particles, which occurs in many situations in cosmology. We show that this effect has important implications for the Sommerfeld enhancement and DM physics. For the first time, we calculate the Sommerfeld factor induced by quantum forces for both bosonic and fermionic mediators, including the background corrections. We observe several novel features of the Sommerfeld factor that do not exist in the case of the Yukawa potential, such as temperature-induced resonance peaks for massless mediators, and having both enhancement and suppression effects in the same model with different DM masses. As direct applications, we discuss the DM phenomenology affected by the Sommerfeld enhancement from quantum forces, including thermal freeze-out, CMB spectral distortion from DM annihilation, and DM indirect detection. We highlight one particularly interesting effect relevant to indirect detection caused by the Sommerfeld enhancement in a non-thermal background of bosonic mediators in the galaxy, in which case the DM mass is shifted due to the background correction and the effective cross section for DM annihilation can be either enhanced or suppressed. This may be important for DM searches in the Milky Way or its satellite galaxies.

    hep-phastro-ph.COhep-thJHEP(2025)·3 citations
  17. 17*

    Invisible jets from composite neutrinos

    Matteo Borrello🇮🇹 · Marco Costa🇨🇦 · Diego Redigolo🇮🇹

    We propose a novel experimental probe of neutrino couplings to a composite sterile sector, leveraging the unique signature of neutrino disintegration into "invisible jets" in high-energy neutrino scattering. Focusing on scenarios where the invisible jet invariant mass significantly exceeds the confinement scale, we compute production rates within the conformal window. In this regime, invisible jet production leads to an energy-dependent enhancement of the neutral-to-charged current ratio in neutrino-nucleus scattering. Using NuTeV measurements, we derive new bounds and assess the sensitivity of upcoming experiments such as SHiP and the Forward Physics Facility at CERN. We sketch models where these probes surpass constraints from electroweak gauge boson and Higgs invisible branching ratios. In contrast, neutrino-electron scattering modifications are suppressed by the lower center-of-mass energy and are unlikely to be observable at DUNE.

    hep-phhep-exJHEP(2026)·5 citations
  18. 18*

    Phase-space sectors for ordered momentum mappings in local subtraction up to NLO

    Xuan Chen🇨🇳 · Matteo Marcoli🇬🇧

    Ordered momentum mappings present optimal convergence in soft and collinear configurations and are particularly suitable for the numerical implementation of local subtraction schemes. However, ordered mappings cannot be directly applied in the presence of multiple unordered emissions, which typically appear beyond the leading-colour approximation. A possible solution consists in separating individual singularities at the level of local counterterms by means of partial fractioning, which can become cumbersome at higher orders and introduce large cancellations in intermediate steps of the calculations. We present a simple decomposition of the phase space into sectors to isolate classes of infrared configurations which can be addressed with a specific ordered momentum mapping. With such decomposition, the singularities of any matrix element can be subtracted with ordered mappings, without the need of partial fractioning. We illustrate the required phase-space sectors for up to three unordered emissions and discuss applications in the context of the antenna subtraction method. The mapping algorithm described here has been recently employed for the first differential NLO of jet production at electron-positron colliders.

    hep-phEPJC(2026)·3 citations
  19. 19*

    Parton distribution and fragmentation functions with massive gluons

    Gustavo B. Bopsin🇧🇷 · Bruno El-Bennich🇧🇷 · Gastão Krein🇧🇷 · Fernando E. Serna🇨🇴 · Roberto C. da Silveira🇧🇷

    The correct description of the hadron's structure requires understanding how quarks and gluons form the observable hadrons and how they are distributed within them. Two key nonperturbative quantities encapsulate this information: parton distribution functions (PDFs) and fragmentation functions (FFs). The former define a probabilistic light-front momentum distribution of partons within a hadron, whereas the latter describe the hadronization process of high-energy partons. Computing these functions analytically poses significant challenges, as it demands models that accurately incorporate the nonperturbative infrared dynamics of Quantum Chromodynamics (QCD). In this work, we compute the pion PDF and its elementary and full FFs using the Curci-Ferrari (CF) model. This model enables the exploration of nonperturbative QCD effects by introducing a gluon-mass scale within the Landau gauge QCD Lagrangian. The two-point quark and gluon correlation functions derived from the CF model agree well with lattice QCD results and reproduce the pion decay constant in the chiral limit, consistent with chiral perturbation theory. The resulting pion PDF and FFs computed with the CF quark propagator and pion Bethe-Salpeter amplitude are in good qualitative and quantitative agreement with those obtained using the Qin-Chang model, a benchmark approach to nonperturbative QCD. These findings support the broader applicability of the Curci-Ferrari model in hadron phenomenology.

    hep-phhep-exnucl-thPRD(2025)·5 citations
  20. 20*

    Testing the effective action approach to bubble nucleation in holography

    Oscar Henriksson🇫🇮 · Niko Jokela🇫🇮 · Xin Li🇫🇮

    The nucleation of bubbles during a first-order phase transition has recently been explored using holographic duality, which can provide an important complement to standard perturbative methods. These computations typically require finding static and spatially inhomogeneous saddle points, known as critical bubbles, which correspond in the gravitational dual to solutions of nonlinear partial differential equations. A computationally simpler alternative is to use the gravitational dual to derive the effective action of the boundary theory in a derivative expansion, and then solve the resulting lower-dimensional equations of motion. Once the effective action, typically truncated at two derivatives, is obtained, the holographic theory can be set aside, and bubble solutions can be found from ordinary differential equations. In this paper, we test this approach in a simple holographic setup: a scalar field in the probe limit in a black brane background, with nonlinear multi-trace boundary conditions. We compute critical bubble solutions both from the effective action and by solving the scalar field equation of motion directly in the gravity theory, and find good agreement between the two methods.

    hep-thgr-qchep-phJHEP(2026)·4 citations
  21. 21*

    Instability of regular planar black holes in four dimensions arising from an infinite sum of curvature corrections

    Antonio De Felice🇯🇵 · Shinji Tsujikawa🇯🇵

    In four-dimensional scalar-tensor theories derived via dimensional regularization with a conformal rescaling of the metric, we study the stability of planar black holes (BHs) whose horizons are described by two-dimensional compact Einstein spaces with vanishing curvature. By taking an infinite sum of Lovelock curvature invariants, it is possible to construct BH solutions whose metric components remain nonsingular at , with a scalar-field derivative given by , where is the radial coordinate. We show that such BH solutions suffer from a strong coupling problem, where the kinetic term of the even-parity scalar-field perturbation associated with the timelike coordinate vanishes everywhere. Moreover, we find that these BHs are subject to both ghost and Laplacian instabilities for odd-parity perturbations near . Consequently, the presence of these pathological features rules out regular planar BHs with the scalar-field profile as physically viable and stable configurations.

    gr-qchep-phhep-thPRD(2025)·4 citations
  22. 22*

    Investigating Universal Relations in Compact Stars featuring Admixed Exotic Dense Matter

    Vivek Baruah Thapa🇮🇳 · Anil Kumar🇮🇳 · Vishal Parmar🇮🇹 · Monika Sinha🇮🇳

    The dense material in a compact star from a supernova remnant is beyond terrestrial experimentation, so phenomenological modeling is used to match astrophysical observations. This is crucial due to the complex sensitivity of compact star features to dense matter properties. Despite modeling flexibility, certain universal relationships among compact star features hold true, regardless of the matter model. Our study examines these universal relationships, focusing on the moment of inertia, tidal Love number, and quadrupole moment, as well as correlations between non-radial oscillation frequencies and star compactness. We consider baryonic stars with cores of heavier baryons. Our findings show that baryonic stars with cores of heavier baryons follow the universal relations, and the f-mode oscillation frequency's universality relative to tidal deformability is notable, with an error margin under 1.

    astro-ph.HEhep-phJ.Subatomic Part.Cosmol.(2025)·0 citations
  23. 23*

    Scrutinizing the cosmogenic origin of the KM3-230213A event: A Multimessenger Perspective

    Alessandro Cermenati🇮🇹 · Antonio Ambrosone🇮🇹 · Roberto Aloisio🇮🇹 · Denise Boncioli🇮🇹 · Carmelo Evoli🇮🇹

    The recent detection of the neutrino event KM3-230213A (~220 PeV) by the KM3NeT/ARCA telescope, the most energetic ever observed, could represent the long-awaited evidence for a cosmogenic origin, arising from the interaction of an ultra-high-energy cosmic ray with background photons. Its secure confirmation would mark a major advance in high-energy astrophysics. We perform a self-consistent multimessenger transport calculation of protons and their secondary -rays and neutrinos from cosmologically evolving sources, confronting predictions with data from the Pierre Auger Observatory, IceCube, KM3NeT, and the Fermi-LAT isotropic -ray background. A steep sub-ankle proton component saturates the diffuse -ray background and is disfavoured, whereas a hard proton spectrum extending beyond ~eV with evolution reproduces KM3-230213A without violating any limits. This scenario requires a proton fraction \% at ~eV and excludes faster-evolving sources. Joint UHE-neutrino and -ray observations thus sharpen constraints on extragalactic cosmic-ray sources and set targets for AugerPrime and next-generation neutrino telescopes.

    astro-ph.HEhep-ph10 citations
  24. 24*

    Dark Matter Clumps as Sources of Gravitational-Wave Glitches in LIGO/Virgo/KAGRA data

    Ezequiel Alvarez🇦🇷 · Scott Perkins🇺🇸 · Federico Ravanedo🇦🇷 · Nicolas Yunes🇺🇸

    We consider the hypothetical possibility that non-stationary glitch features in the noise of ground-based gravitational-wave detectors could be produced by small dark matter clumps that pass through the earth in the vicinity of gravitational-wave detectors. We first derive the gravitational-wave strain that would be generated by the passage of such a dark matter clump. We find that the strain is primarily sourced by the Newtonian gravitational acceleration of the mirrors toward the clump and by the Shapiro time delay of the photons in the laser beams as they pass through the gravitational potential created by the dark matter clump. We also find that the Newtonian acceleration effect dominates the gravitational-wave strain for both ground and space-based interferometers. We then compare our dark matter clump, gravitational-wave strain model to 84 Koi-Fish glitches detected during the second observing run of the LIGO/Virgo/KAGRA collaboration through a Markov Chain Monte Carlo Bayesian analysis. We find that all glitches but 9 can be confidently rejected as having originated from dark matter clumps. For the remaining glitches, the dark matter hypothesis cannot be excluded, and the maximum \textit{a posteriori} parameters yield minimum densities of about , within the model. These results allow us to place the first direct upper limits with gravitational-wave detectors on the local over-density of dark matter in the form of clumps in the local neighborhood of Earth, namely .

    gr-qcastro-ph.HEhep-phPRD(2026)·0 citations
  25. 25*

    The asymptotically-free gauge theories

    Ben Gripaios🇬🇧 · Khoi Le Nguyen Nguyen🇬🇧

    We show how to classify the asymptotically-free gauge theories in four spacetime dimensions, focussing here on the case of purely fermionic matter. The classification depends on the fact (which we prove) that both the dimension and Dynkin index of irreducible representations of a simple Lie algebra are strictly increasing functions of each Dynkin label. This implies not only that the number of asymptotically-free representations of any one semisimple Lie algebra is finite, but also that they can be written down in a systematic fashion using tables for the asymptotically-free irreducible representations of simple Lie algebras, which we supply. These tables show that at most two out of a possible ten Dynkin labels can be non-zero and that no Dynkin label can exceed four. The extension to bosonic matter or supersymmetric theories is straightforward.

    hep-thhep-phJHEP(2026)·4 citations
  26. 26*

    The BAO-CMB Tension and Implications for Inflation

    Elisa G. M. Ferreira🇯🇵 · Evan McDonough🇨🇦 · Lennart Balkenhol🇫🇷 · Renata Kallosh🇺🇸 · Lloyd Knox🇺🇸 · Andrei Linde🇺🇸

    The scalar spectral index is a powerful test of inflationary models. The tightest constraint on to date derives from the combination of cosmic microwave background (CMB) data with baryon acoustic oscillation (BAO) data. The resulting constraint is shifted significantly upward relative to the constraint from CMB alone, with the consequence that previously preferred inflationary models are seemingly disfavored by . Here we show that this shift in is the combined effect of a degeneracy between and BAO parameters exhibited by CMB data and the tension between CMB datasets and DESI BAO data under the assumption of the standard cosmological model. Given the crucial role of in discriminating between inflationary models, we urge caution in interpreting CMB+BAO constraints on until the BAO-CMB tension is resolved.

    astro-ph.COgr-qchep-phhep-thPRD(2026)·94 citations
  27. 27*

    (Super)Gravity from Positivity

    Brando Bellazzini🇫🇷 · Alex Pomarol🇪🇸 · Marcello Romano🇫🇷 · Francesco Sciotti🇪🇸

    We investigate whether the effective theory for isolated, massive, and weakly interacting spin- particles is compatible with causality and unitarity-i.e., the positivity of scattering amplitudes. We find no solution to positivity constraints, except when gravitons are also present and couple in a (nearly) supersymmetric way. Gravity is thus bootstrapped from -matrix consistency conditions for the longitudinal and transverse polarizations of massive spin- states. For two such particles forming a -charged state, a (gravi)photon gauging the symmetry is also required, with couplings characteristic of supergravity and consistent with both the no global symmetry and weak gravity conjectures. We further explore the EFT-hedron associated with the longitudinal polarizations, the Goldstinos, through novel - symmetric dispersion relations. We identify the extremal UV models that lie at the corners of the allowed parameter space, recovering familiar models of supersymmetry breaking and uncovering new ones.

    hep-thhep-phJHEP(2026)·23 citations
  28. 28*

    Supergravity from the Bottom Up

    Tony Gherghetta🇺🇸 · Wenqi Ke🇺🇸

    We employ on-shell methods to construct scattering amplitudes and derive effective theories involving massive spin-3/2 fermions interacting with spin 0, 1 and 2 bosons. The four-point massive amplitudes are constructed using an all-line-transverse momentum shift, assuming that in the massless limit, three-point interactions are smooth and the Ward identity is satisfied. For a Majorana spin-3/2 fermion with mass , we show that interactions with only spin 0 and massive spin-1 bosons do not lead to an effective theory valid up to a cutoff that is independent of particle masses. Instead, adding an interaction with a spin-2 graviton gives rise to four-point amplitudes with a Planck scale unitarity cutoff that reproduces well-known results from supergravity, such as -term breaking with a complex scalar and -term breaking with an additional massive photon. These bottom-up results are then extended to two Majorana spin-3/2 fermions where an interacting effective theory valid up to again requires the introduction of the spin-2 graviton. Unitarity up to the Planck scale is then achieved when the two Majorana spin-3/2 fermions have unequal masses, and necessarily couple to two massive spin-1 states corresponding to the spontaneous breaking of supergravity to . Our results, obtained from the bottom-up and without any Lagrangian, imply that broken supergravity is the unique, effective theory involving interactions of massive spin-3/2 fermions valid up to a cutoff that does not depend on particle masses.

    hep-thhep-phJHEP(2026)·6 citations

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