PaperPanorama

HEP Phenomenology·hep-ph

Wed·Jan 15, 2025

29 papers21 primary·8 cross-listed·reconstructed*

  1. 01*

    A Step Toward Interpretability: Smearing the Likelihood

    Andrew J. Larkoski🇺🇸

    The problem of interpretability of machine learning architecture in particle physics has no agreed-upon definition, much less any proposed solution. We present a first modest step toward these goals by proposing a definition and corresponding practical method for isolation and identification of relevant physical energy scales exploited by the machine. This is accomplished by smearing or averaging over all input events that lie within a prescribed metric energy distance of one another and correspondingly renders any quantity measured on a finite, discrete dataset continuous over the dataspace. Within this approach, we are able to explicitly demonstrate that (approximate) scaling laws are a consequence of extreme value theory applied to analysis of the distribution of the irreducible minimal distance over which a machine must extrapolate given a finite dataset. As an example, we study quark versus gluon jet identification, construct the smeared likelihood, and show that discrimination power steadily increases as resolution decreases, indicating that the true likelihood for the problem is sensitive to emissions at all scales.

    hep-phcs.LGhep-exstat.MLJHEP(2025)·3 citations
  2. 02*

    Mixing interactions and effects in the NJL-model

    F.L. Braghin🇧🇷

    The flavor-dependent quark-antiquark contact interactions, induced by vacuum polarization and recently derived for flavor U(3) Nambu-Jona-Lasinio model, are articulated with the resulting mixing effects emerging from flavor symmetry breaking in view. The formal effects of the explicit mixing interactions, , are detailed firstly for the meson mixing problem without the inclusion of 't Hooft interactions induced by instantons. Secondly, it is shown that these mixings, in the scalar channel of quark-antiquark interactions, might give rise to quark mixing in the gap equations. Sixth order quark-antiquark interactions from vacuum polarization, that break symmetry, also contribute.

    hep-phnucl-thPoS(2026)·1 citation
  3. 03*

    In-flight positron annihilation as a probe of feebly interacting particles

    Shyam Balaji🇬🇧 · Pierluca Carenza🇸🇪 · Pedro De la Torre Luque🇪🇸 · Alessandro Lella🇮🇹 · Leonardo Mastrototaro🇮🇹

    Core-collapse supernovae (SNe) provide a unique environment to study Feebly Interacting Particles (FIPs) such as Axion-Like Particles (ALPs), sterile neutrinos, and Dark Photons (DPs). This paper focuses on heavy FIPs produced in SNe, whose decay produces electrons and positrons, generating observable secondary signals during their propagation and annihilation. We focus on the In-flight Annihilation (IA) of positrons, which emerge as the most significant contribution to the resulting gamma-ray spectrum. Using data from COMPTEL and EGRET we derive the most stringent bounds on the FIP-electron couplings for heavy ALPs, sterile neutrinos, and DPs. These results strenghten existing bounds of one or two orders of magnitude, depending on the FIP model.

    hep-phastro-ph.HEhep-thPRD(2025)·12 citations
  4. 04*

    Generic framework for non-perturbative QCD in light hadrons

    Wei-Yang Liu🇺🇸

    In this paper, we review several topological aspects of the QCD vacuum and recent progress on this quantitative unifying framework for the low-lying hadron physics rooted in QCD by introducing the vacuum as a liquid of pseudoparticles. We have developed systematic density expansion on the dilute vacuum to calculate the vacuum expectation values (VEVs) and generalize the calculations to hadronic matrix element and hadronic form factors using the instanton liquid model (ILM). Thereby, the nonperturbative physics can be analyzed in a systematic framework with a few parameters: instanton size and instanton density , and current quark mass .

    hep-phhep-lathep-thnucl-th8 citations
  5. 05*

    Confront a dilaton model with the LHC measurements

    J.E. Wu🇨🇳 · Q.S. Yan🇨🇳

    The origin of the Higgs boson (), discovered in 2012, remains a mystery. In the metric affine theory (MAT) framework, we study the scalar potential and investigate a couple of scenarios for the symmetry breaking mechanisms with a dilaton model which is derived from the geometry. The LHC constraints for the couplings of Yukawa couplings, Higgs-weak vector bosons and Higgs self-couplings, in this model are examined, which identify the parameter space where the discovered Higgs boson GeV can be dilaton-dominant and the features of Higgs self-couplings are explored. It is found that via the measurements of Higgs pair production, the High Luminosity LHC (HL-LHC) running can either confirm or rule out the dilaton dominance.

    hep-phPRD(2026)·2 citations
  6. 06*

    Modified Coherence and the Transverse Extent of Jets

    Amit Kumar🇨🇦 · Abhijit Majumder🇺🇸 · Chathuranga Sirimanna🇺🇸 · Yasuki Tachibana🇯🇵

    We present a study of the transverse size of parton showers and their diminishing interaction with the medium in the high virtuality stage of jet evolution. We consider the process of a hard quark produced in deep inelastic scattering off a large nucleus. Single gluon radiation from this quark, in the absence of scattering, is re-derived using wave-packets. This allows for a derivation of the quantum uncertainty size of the hard quark, at the point of splitting. This uncertainty size is then incorporated within a Monte-Carlo shower routine yielding transverse shower sizes noticeably larger than the classical antenna size of the shower. No clear relation is found between the full uncertainty size of the shower and the virtuality of the originating parton. The single gluon emission from the hard quark is then re-analysed for the case of single rescattering off the remainder of the nucleus. A relation is derived between the jet transport coefficient and the gluon Transverse Momentum Dependent Parton Distribution Function (gTMDPDF). Solving this relation, for a simple case, clearly demonstrates the weakening of with the virtuality of the hard splitting parton.

    hep-phnucl-thPRC(2025)·9 citations
  7. 07*

    Covariant analysis of electromagnetic current on the light cone: exposition with scalar Yukawa theory

    Wenyu Zhang🇨🇳 · Yang Li🇨🇳 · James P. Vary🇺🇸

    We present the first systematic investigation of the Lorentz covariance of the charge form factor for a strongly coupled scalar theory in (3+1)-dimensions. Our results are based on the first non-perturbative solution of the scalar Yukawa theory with a Fock sector expansion including up to thee-particles (one mock nucleon plus two mock pions or two mock nucleons plus one mock anti-nucleon). The light-front Hamiltonian is constructed and renormalized using a Fock sector dependent scheme. The derived eigenvalue equation is then solved non-perturbatively to obtain the wave functions, which are then used to compute the current matrix element. We perform a covariant analysis of the current matrix element taking into account possible violation of the Poincaré symmetry due to the Fock sector truncation. The physical form factor depends on two boost invariants , instead of the single Lorentz invariant . Instead of adopting the conventional Drell-Yan frame , we evaluate the form factor in general frames, and use the frame dependence to quantitatively gauge the loss of the Lorentz covariance. Our numerical result shows that as more Fock sectors are included, the frame dependence reduces dramatically. In particular, the anti-nucleon degree of freedom plays an important role in the reduction of the frame dependence, even though it only takes a small portion within the state vector. We also find that there is no zero-mode contribution to the current for the scalar Yukawa theory.

    hep-phhep-thnucl-thJHEP(2025)·3 citations
  8. 08*

    New Constraints on Axion Mediated Dipole-Dipole Interactions

    Zitong Xu🇨🇳 · Xing Heng🇨🇳 · Guoqing Tian🇨🇳 · Di Gong🇨🇳 · Lei Cong🇩🇪 · Wei Ji🇩🇪 · Dmitry Budker🇩🇪 · Kai Wei🇨🇳

    The search for axions sits at the intersection of solving critical problems in fundamental physics, including the strong CP problem in QCD, uncovering the nature of dark matter, and understanding the origin of the universe's matter-antimatter asymmetry. The measurement of axion-mediated spin-dependent interactions offers a powerful approach for axion detection. However, it has long been restricted to regions outside the 'axion window' due to a significant trade-off: the need to effectively suppress the magnetic leakage from highly polarized spin sources while simultaneously detecting sub-femtotesla level exotic physics signals at sub-decimeter-scale distances. In this work, we report new experimental results on axion-mediated exotic spin-spin interactions using an iron-shielded SmCo spin source in combination with a specially designed self-compensation comagnetometer. Employing a composite shielding structure, we achieved a suppression of the magnetic field by up to . This enabled us to establish new constraints on the coupling between electrons and neutrons, surpassing previous experimental limits by more than 10000 times within the axion window. Furthermore, we also set strongest constraints on the coupling between electrons and protons. The proposed method holds substantial potential not only for advancing the search for new physics beyond the Standard Model but also for enabling transformative applications in biological and chemical research.

    hep-phastro-ph.HEphysics.atom-phquant-phPRL(2025)·12 citations
  9. 10*

    Gravitational Waves dynamics with Higgs portal and U(1) X SU(2) interactions

    Lucia A.Popa🇷🇴

    We show that a mixture of Higgs boson with a heavy scalar singlet with large vacuum expectation value ( vev) is a viable model of inflation that satisfy the existing observational data, the perturbativity constraints, avoiding in the same time the EW vacuum metastability as long as the Higgs portal interactions lead to positive tree-level threshold corrections for SM Higgs quartic coupling. The tree-level threshold corrections lead to the change of Hubble expansion rate during inflation with impact on the evolution of the axion-gauge field spectator sector, modifying the time-dependent mass parameter of the gauge field fluctuation. We evaluate this effect on the GW sourced tensor modes while accounting for the consistency and backreaction constraints and show that the Higgs portal interactions enhance the GW signal sourced by the gauge field fluctuations in the CMB B-mode ploarization power spectra. We address the detectability of the GW sourced by the gauge field fluctuations in presence of Higgs portal interactions for the experimental configuration of the future CMB polarization LiteBird space mission. We find that the sourced GW tensor-to-scalar ratio in presence of Higgs portal interactions is enhanced to a level that overcomes the vacuum tensor-to-scalar ratio by a factor of 10, much above the detection threshold of the LiteBird experiment, in agreement with the existing observational constraints on the curvature fluctuations and the allowed parameter space of Higgs portal interactions. We also show that a large enhancement of the sourced GW can be also detected by experiments such as pulsar timing arrays and laser/atomic interferometers. Moreover, a significant Higgs-singlet mixing can be probed by the LHC Higgs searchers.

    hep-phPhys.Dark Univ.(2025)·0 citations
  10. 11*

    New Limits on Ultralight Axionlike Dark Matter from Reanalyzed Data

    K. Y. Zhang🇨🇳 · L. Y. Wu🇨🇳 · H. Yan🇨🇳

    New limits on the axion-nucleon coupling over the axion mass region eV are derived by reanalyzing data from laboratory measurements on Lorentz and violation. These results establish the first laboratory constraints on the axion-nucleon coupling for axion masses below eV. For eV, the results improve upon previous laboratory limits by more than 3 orders of magnitude, exceeding for the first time the astrophysical limits from supernova SN1987A cooling. For the axion mass range of interest corresponding to ultralow frequencies, the crucial local phase of the axion field is considered. Furthermore, the obtained limits are nearly equivalent to those projected for a recently proposed experiment employing high-intensity neutron beams at the European Spallation Source. For an alternative type of axion-nucleon interaction, the quadratic wind coupling, the constraints exceed the current best results by approximately 2 orders of magnitude.

    hep-phastro-ph.HEPRL(2025)·8 citations
  11. 12*

    Exclusive leptoproduction of a light vector meson at the twist-3 in a GTMD framework

    Renaud Boussarie🇫🇷 · Michael Fucilla🇫🇷 · Lech Szymanowski🇵🇱 · Samuel Wallon🇫🇷

    We provide the most general description of the exclusive leptoproduction of a light vector meson, at high center-of-mass energy, within the CGC/shockwave formalism. We keep a twist-3 accuracy in channel, thus being able to describe all possible helicity amplitudes, including the ones for the production of a transversally polarized meson. In this latter case, we overcome the well-known issue of endpoint singularities by promoting the GPD to a GTMD given by matrix elements of dipole and double dipole operators. The all-twists treatment of the proton (nucleon) target allow to safely twist-expand the general vacuum-to-meson matrix elements. Therefore, unlike previous attempts in the modified perturbative approach, our final results are expressed in terms of the twist-3 collinear distribution amplitudes, introduced in the context of the higher-twist collinear formalism.

    hep-phhep-exActa Phys.Polon.Supp.(2025)·1 citation
  12. 13*

    Enhanced quantum radiation with flying-focus laser pulses

    Martin S. Formanek🇨🇿 · John P. Palastro🇺🇸 · Dillon Ramsey🇺🇸 · Antonino Di Piazza🇺🇸

    The emission of a photon by an electron in an intense laser field is one of the most fundamental processes in electrodynamics and underlies the many applications that utilize high-energy photon beams. This process is typically studied for electrons colliding head-on with a stationary-focus laser pulse. Here, we show that the energy lost by electrons in the quantum regime and the yield of emitted photons can be substantially increased by replacing a stationary-focus pulse with an equal-energy flying-focus pulse whose focus co-propagates with the electrons. These advantages of the flying focus result from the energy loss and the photon yield scaling more favorably with the interaction time than the laser intensity in the quantum regime, with the latter also holding in the classical regime. Monte Carlo simulations of electrons colliding with equal-energy stationary and flying-focus laser pulses demonstrate these advantages.

    hep-phPRA(2025)·4 citations
  13. 14*

    Kinematic power corrections to DVCS to twist-six accuracy

    V. M. Braun🇩🇪 · Yao Ji🇩🇪 · A. N. Manashov🇩🇪

    We calculate and power corrections with , where is the target mass and is the momentum transfer, to several key observables in Deeply Virtual Compton Scattering (DVCS). We find that the power expansion is well convergent up to for most of the observables, but is naturally organized in terms of rather than the nominal hard scale . We also argue that target mass corrections remain under control and do not endanger QCD factorization for coherent DVCS on nuclei. These results remove an important source of uncertainties due to the frame dependence and violation of electromagnetic Ward identities in the QCD predictions for the DVCS amplitudes in the leading-twist approximation.

    hep-phPRD(2025)·10 citations
  14. 15*

    Computation of FCC-ee Sensitivity to Heavy New Physics with Interactions of Any Flavor Structure

    Ben Allanach🇬🇧 · Eetu Loisa🇬🇧

    We present a tool to compute the sensitivity of the Future Circular Electron--Positron Collider (FCC-ee) to the interactions of new, heavy particles via publicly available extensions to the smelli and flavio computer programs. We parameterize new particles' effects without any flavor assumptions and take into account the projected experimental and correlated theoretical uncertainties of various electroweak and Higgs observables at the proposed collider. We illustrate a use of the tool by estimating the sensitivity of the FCC-ee to a model with flavor-specific couplings which explains anomalies inferred from present-day measurements and Standard Model predictions of observables that involve the transition.

    hep-phPRD(2025)·4 citations
  15. 16*

    Feynman Diagrams

    Stefan Weinzierl🇩🇪

    We give a concise and pedagogical introduction to Feynman diagrams. After discussing a toy model which requires only undergraduate mathematics, we focus on relativistic quantum field theory. We review the derivation of Feynman rules from the Lagrangian of the theory and we discuss modern methods to compute tree and loop diagrams.

    hep-ph1 citation
  16. 17*

    QCD condensates and from -decay: Summary

    S. Narison · LUPM (CNRS and Univ. Montpellier, FR) · iHEPMAD (Univ. Antananarivo, MG)

    In this talk, I summarize the recent determinations in Ref.[1] of the QCD condensates and within the SVZ expansion using the ratio of Laplace sum rule (LSR) and -like moments within stability criteria in the axial-vector (A) and V-A channels of the - semi-hadronic decays. The factorization of the four-quark condensate is violated by a factor 6 like in the case of the Hadrons data. There is no exponential growth of the size of higher dimension condensates which does not favour (by duality) a significant effect of the so-called Duality Violation (DV). The extracted value of is in good agreement with the one from and indicates that the determination at the observed -mass is not the optimal one and leads to an overestimate of its actual value.

    hep-phhep-exhep-latJ.Subatomic Part.Cosmol.(2025)·3 citations
  17. 18*

    Neutrino Oscillations in the Three Flavor Paradigm

    Peter B. Denton🇺🇸

    The three-flavor neutrino oscillation model describes the well-studied phenomenon of neutrinos produced in association with one charged lepton: electron, muon, or tau, and then later detected in association with a possibly different charged lepton. While somewhat surprising, the firm experimental discovery of the phenomenon in the late 1990s and early 2000s has lead to a revolution in particle physics as the nature of neutrinos has been explored with heightened vigor ever since. At the core of the phenomenon are the six neutrino oscillation parameters. These parameters are fundamental and not predicted from anything else in our model of particle physics. At the time of writing this chapter, many of them have been measured, but several key questions remain that are to be answered by neutrino oscillations themselves. These questions have motivated some of the largest and most involved particle physics experiments built to date. This chapter will develop the basics of neutrino oscillation theory and build intuition for the role of the oscillation parameters and how they are measured, as well as the important role of the matter effect in neutrino oscillations.

    hep-phhep-exEncyclopedia of Particle Physics, 3, 194 …·16 citations
  18. 19*

    Inflationary scenarios beyond the Standard Model

    Alberto Salvio🇮🇹

    The aim of this chapter is to explain in clear and pedagogical terms how some particle-physics models and/or mechanisms can naturally lead to inflation and how this can provide testable predictions that can help us find new physics effects. Two well-established features of theoretical particle physics are linked to an essential property of inflation, a naturally-flat inflaton potential: (1) scale invariance, broken by small quantum corrections, and (2) Goldstone's theorem. It is also illustrated how to combine several scenarios of this type to obtain a rather general particle-physics motivated inflationary setup.

    hep-phastro-ph.COhep-thEncyclopedia of Particle Physics, Volume …·0 citations
  19. 20*

    Polarimetric searches for axion dark matter and high-frequency gravitational waves using optical cavities

    Camilo García-Cely🇪🇸 · Luca Marsili🇪🇸 · Andreas Ringwald🇩🇪 · Aaron D. Spector🇩🇪

    We revisit birefringence effects associated with the evolution of the polarization of light as it propagates through axion dark matter or the background of a passing gravitational wave (GW). We demonstrate that this can be described by a unified formalism, highlighting a synergy between searches for axions and high-frequency GWs. We show that by exploiting this framework, the optical cavities used by the ALPS II experiment can potentially probe axion masses in the range , offering competitive sensitivity with existing laboratory and astrophysical searches. Also building on this approach, we propose using these optical cavities to search for high-frequency GWs by measuring changes in the polarization of their laser. This makes it a promising method for exploring, in the near future, GWs with frequencies above MHz and strain sensitivities on the order of . Such sensitivity allows the exploration of currently unconstrained parameter space, complementing other high-frequency GW experiments. This work contributes to the growing community investigating novel approaches for high-frequency GW detection.

    hep-phastro-ph.IMgr-qchep-exPRD(2025)·6 citations
  20. 21*

    Two-Loop Anomalous Dimensions in the LEFT: Dimension-Six Four-Fermion Operators in NDR

    Jason Aebischer🇨🇭 · Pol Morell🇪🇸 · Marko Pesut🇨🇭 · Javier Virto🇪🇸

    We derive the complete set of two-loop anomalous dimensions describing the mixing of four-fermion operators in the Low Energy Effective Field Theory (LEFT). The calculation is performed in Naive Dimensional Regularization with anticommuting (the NDR scheme), and the results are given in the "JMS basis" of dimension-six operators. The derivation relies on known results for UV poles in two-loop diagrams in QCD, which are then used to derive the two-loop Anomalous Dimension Matrix (ADM) for the full set of four-fermion operators including , and corrections. The method employed is an extension of a common approach to deal with traces containing in NDR. Our results have been implemented in the public code DsixTools. We also discuss and provide the results in the LEFT with 5, 4 and 3 active quark flavors.

    hep-phhep-exJHEP(2026)·34 citations
  21. 22*

    Primordial Non-Gaussianity from Light Compact Scalars

    Priyesh Chakraborty🇺🇸

    We study the non-Gaussianities generated by light axions, or compact scalar fields, during inflation. To correctly calculate their impact on primordial statistics, we will argue that it is necessary to account for the periodicity, or gauge symmetry, of the compact scalars. We illustrate this point by comparing the predictions for the squeezed kinematic limit of the primordial bispectrum generated by two cases: a non-compact scalar and a compact scalar . We demonstrate that while a light non-compact scalar predicts a bispectrum of the so-called local shape, the light compact scalar predicts a qualitatively different shape characterised by the ratio of the Hubble scale to its field-space circumference. In doing so, we show that ignoring the gauge symmetry of the compact scalar during inflation leads to spurious infrared enhancements which are softened by working with appropriate gauge-invariant operators. In addition, we connect our results for the primordial bispectrum with late-time cosmological observables and show that it is possible to measure the decay constant of the compact scalar using galaxy clustering measurements.

    hep-thastro-ph.COhep-phJHEP(2025)·18 citations
  22. 23*

    Self-similar inverse cascade from generalized symmetries

    Yuji Hirono🇯🇵 · Kohei Kamada🇨🇳 · Naoki Yamamoto🇯🇵 · Ryo Yokokura🇯🇵

    We investigate the role of generalized symmetries in driving non-equilibrium and non-linear phenomena, specifically focusing on turbulent systems. While conventional turbulence studies have revealed inverse cascades driven by conserved quantities integrated over the entire space, such as helicity in three spatial dimensions, the influence of higher-form symmetries, whose conserved charges are defined by integration over subspaces, remains largely unexplored. We demonstrate a novel mechanism where higher-form symmetries naturally induce a self-similar inverse cascade. Taking axion electrodynamics with non-linear topological interaction as a paradigmatic example, we show that the conserved charge associated with its 1-form symmetry drives the system toward large-scale coherent structures through a universal scaling behavior characterized by analytically determined scaling exponents. Our findings suggest that higher-form symmetries can provide a fundamental organizing principle for understanding non-equilibrium phenomena and the emergence of coherent structures in turbulent systems.

    hep-thcond-mat.mes-hallhep-phnlin.CD+1PRL(2026)·1 citation
  23. 24*

    Tidal Love Numbers of Neutron Stars in Horndeski Theories

    Robin Fynn Diedrichs🇩🇪 · Shinji Tsujikawa🇯🇵 · Kent Yagi🇺🇸

    Precision measurements of the gravitational wave signal from compact binary inspirals allow us to constrain the internal structure of those objects via physical parameters such as the tidal Love numbers. In scalar-tensor theories, one typically finds new types of Love numbers that are usually not considered or simply absent in General Relativity, which further allows us to constrain deviations from General Relativity. Building upon previous results, we present the linear perturbation equations necessary to calculate static and even-parity tidal Love numbers in Horndeski theories, the most general scalar-tensor theories with second-order field equations of motion. We further focus on the quadrupolar Love numbers and demonstrate how these can be extracted from the asymptotic expansion of the perturbation fields. We find that there is a potential ambiguity in extracting the Love numbers in this way, which we resolve by performing supplementary calculations in the effective field theory framework. We show that, in the case of scalar-tensor theories, the tidal Love numbers are not directly given by the term in the asymptotic expansion of the perturbation fields, as there is an additional contribution to this term independent of the Love numbers. We calculate such a contribution for a minimally coupled scalar field and also for the Damour-Esposito-Farèse model. For the latter, we find that the Love numbers can differ by , if this additional contribution is not taken into account.

    gr-qchep-phhep-thPRD(2025)·15 citations
  24. 25*

    Topological susceptibility and excess kurtosis in SU(3) Yang-Mills theory

    Stephan Durr🇩🇪 · Gianluca Fuwa🇩🇪

    We present a high-precision study of the topological susceptibility in pure gauge theory in four space-time dimensions. The result is based on ensembles at seven lattice spacings and in seven physical volumes to facilitate a controlled continuum and infinite-volume extrapolation. We use a gluonic topological charge measurement, with gradient flow smoothing in the operator. Two complementary smoothing strategies are used (one keeps the flow time fixed in lattice units, one in physical units). Our data support the idea that both strategies yield a universal continuum limit; we find or . Our appendix data suggest that the excess kurtosis decreases for large box sizes .

    hep-lathep-phPRD(2026)·9 citations
  25. 26*

    Birefringence in fermion-attenuated gravitational wave power spectrum

    Jinglong Liu🇨🇳 · Stephon Alexander🇺🇸 · Antonino Marciano🇨🇳

    Within the framework of Chern-Simons gravity, a theory that dynamically violates parity, we analyze the power spectrum of gravitational waves in light of the damping effect due to the free streaming relativistic neutrinos and dark fermions. The power spectrum is expressed terms of right- and left-handed polarizations, and the evolution of the gravitational waves is studied numerically. Birefringence is explicitly shown in the power spectrum, though the difference in the amplitudes is small. Specific features of peaks and dips appear gravitational wave power spectrum mirroring chiral gravitational wave mediated parametric resonance during reheating. Our result represents a useful tool to test Chern-Simons gravity and enables to constrain mechanisms of inflation and reheating related to this theory. We predict a falsifiable pattern of observable peaks and dips in the chiral independent gravitational power spectrum, eventually observable in next space-borne gravitational interferometers, including LISA, Taiji and Tianqin.

    gr-qcastro-ph.COhep-phhep-thPLB(2025)·3 citations
  26. 27*

    Lake- and Surface-Based Detectors for Forward Neutrino Physics

    Nicholas W. Kamp🇺🇸 · Carlos A. Argüelles🇺🇸 · Albrecht Karle🇺🇸 · Jennifer Thomas🇺🇸 · Tianlu Yuan🇺🇸

    We propose two medium-baseline, kiloton-scale neutrino experiments to study neutrinos from LHC proton-proton collisions: SINE, a surface-based scintillator panel detector observing muon neutrinos from the CMS interaction point, and UNDINE, a water Cherenkov detector submerged in lake Geneva observing all-flavor neutrinos from LHCb. Using a Monte Carlo simulation, we estimate millions of neutrino interactions during the high-luminosity LHC era. We show that these datasets can constrain neutrino cross sections, charm production in collisions, and strangeness enhancement as a solution to the cosmic-ray muon puzzle. SINE and UNDINE thus offer a cost-effective medium-baseline complement to the proposed short-baseline forward physics facility.

    hep-exhep-phPRD(2026)·9 citations
  27. 28*

    Two- versus three-body approach to femtoscopic hadron-deuteron correlations

    Stanislaw Mrowczynski🇵🇱

    The three-body approach to hadron-deuteron correlations is shown to turn into a two-body approach if the three-particle hadron-deuteron wave function factorizes into the deuteron wave-function and the wave function of a hadron motion relative to the deuteron. Then, the hadron-deuteron correlation function is as in the two-body approach only the source radius somewhat changes. For this reason, as we argue, the two-body approach works well for kaon-deuteron correlations but it fails for proton-deuteron ones in case of small sources. Applying the three-body approach generalized to the case where the radius of the hadron source is different from the nucleon source radius, we derive the source radius formula which used in the two-body approach gives the correlation function as in the `factorized' three-body one. The formula is discussed in the context of existing and future experimental data.

    nucl-thhep-phnucl-exPLB(2025)·6 citations

* Reconstructed cohort: no mailing for this day survives in the archive. Papers are grouped by their submission times and arXiv's announcement cut-off, assuming announcement without delay; positions follow identifier order. Validated at ~91% exact-day agreement against the archived era.