PaperPanorama

HEP Phenomenology·hep-ph

Wed·Apr 5, 2023

24 papers13 primary·11 cross-listed·reconstructed*

  1. 01*

    Fast Point Cloud Generation with Diffusion Models in High Energy Physics

    Vinicius Mikuni🇺🇸 · Benjamin Nachman🇺🇸 · Mariel Pettee🇺🇸

    Many particle physics datasets like those generated at colliders are described by continuous coordinates (in contrast to grid points like in an image), respect a number of symmetries (like permutation invariance), and have a stochastic dimensionality. For this reason, standard deep generative models that produce images or at least a fixed set of features are limiting. We introduce a new neural network simulation based on a diffusion model that addresses these limitations named Fast Point Cloud Diffusion (FPCD). We show that our approach can reproduce the complex properties of hadronic jets from proton-proton collisions with competitive precision to other recently proposed models. Additionally, we use a procedure called progressive distillation to accelerate the generation time of our method, which is typically a significant challenge for diffusion models despite their state-of-the-art precision.

    hep-phhep-exPRD(2023)·80 citations
  2. 02*

    Implications of NSI constraints from ANTARES and IceCube on a simplified model

    J. M. Cabarcas🇨🇴 · Alexander Parada🇨🇴 · Nestor Quintero-Poveda🇨🇴

    Recently the neutrino experiments ANTARES and IceCube have released new constraints to the non-standard neutrino interaction (NSI) parameter (flavor off-diagonal). These new constraints are stronger than those obtained from a combination of COHERENT and neutrino oscillation data. In the light of the recent constraints from ANTARES and IceCube data on the NSI parameter , in this work, we study the new physics implications on the parameter space of a simplified model with lepton flavor violating () couplings. For a boson with a mass heavier than the lepton, our results show that ANTARES and IceCube can provide additional constraints to such a new physics scenario with couplings, when compared to bounds from low-energy flavor physics. Moreover, these neutrino experiments can exclude a similar region than ATLAS experiment, showing the potential to provide complementary information to the one obtained from direct searches at the Large Hadron Collider. The impact of the expected sensitivity at DUNE and Belle II experiments is also studied.

    hep-phhep-exPLB(2024)·2 citations
  3. 03*

    Searching for anomalous quartic gauge couplings at muon colliders using principle component analysis

    Yi-Fei Dong · Ying-Chen Mao · Ji-Chong Yang

    Searching for new physics~(NP) is one of the areas of high-energy physics that requires the most processing of large amounts of data. At the same time, quantum computing has huge potential advantages when dealing with large amounts of data. The principal component analysis~(PCA) algorithm may be one of the bridges connecting these two aspects. On the one hand, it can be used for anomaly detection, and on the other hand, there are corresponding quantum algorithms for PCA. In this paper, we investigate how to use PCA to search for NP. Taking the example of anomalous quartic gauge couplings in the tri-photon process at muon colliders, we find that PCA can be used to search for NP. Compared with the traditional event selection strategy, the expected constraints on the operator coefficients obtained by PCA based event selection strategy are even better.

    hep-phEPJC(2023)·23 citations
  4. 04*

    Mass spectra of hidden heavy-flavor tetraquarks with two and four heavy quarks

    Ting-Qi Yan🇨🇳 · Wen-Xuan Zhang🇨🇳 · Duojie Jia🇨🇳

    Inspired by the observation of the by LHCb and the (with mass MeV) recently by CMS and ATLAS experiments of the LHC in the di- invariant mass spectrum, we systemically study masses of all ground-state configurations of the hidden heavy-flavor tetraquarks and (;) contaning two and four heavy quarks in the MIT bag model with chromomagnetic interaction and enhanced binding energy. Considering color-spin mixing due to chromomagnetic interaction, our mass computation indicates that the observed is likely to be the ground states of hidden-charm tetraquark with computed masses MeV, which has a color partner around MeV. The fully bottom system of tetraquark has masses of 19685 MeV and 19717 MeV for the the ground states. Further computation is given to the tetraquark systems , , , and , suggesting that the is the tetraquark with . All of these tetraquarks are above their lowest thresholds of two mesons and unstable against the strong decays.

    hep-phEPJC(2023)·16 citations
  5. 05*

    Anomalies in Particle Physics

    Andreas Crivellin🇨🇭

    I provide a (personal) review of the current hints for physics beyond the Standard Model, called ``anomalies'', obtained both at the intensity frontier (flavour and electroweak precision observables) and in direct LHC searches. This includes the deviations from the Standard Model predictions in semi-leptonic decays, the anomalous magnetic moment of the muon, the Cabibbo Angle Anomaly, the mass as well as non-resonant di-lepton searches, the hints for new scalar particles around GeV, GeV, GeV and the (di-)di-jet excess at TeV (TeV). Possible explanations in terms of new particles are briefly summarized and discussed.

    hep-phhep-exhep-latnucl-ex+1PoS(2024)·8 citations
  6. 06*

    The Phase Transition in the holographic Hard-Wall model

    Matteo Rinaldi🇮🇹 · Vicente Vento🇪🇸

    A Hawking-Page phase transition between AdS thermal and AdS Black Hole was presented as a mechanism for explaining the QCD deconfinement phase transition within holographic models. In order to implement temperature dependence in the confined phase we use a hard-wall AdS/QCD model, where the geometry at low temperatures is described also by a Black Hole metric. We then investigate the temperature dependence of glueball states described as gravitons propagating in deformed background spaces. Finally, we use potential models to physically describe the implications of our study.

    hep-phPRD(2023)·3 citations
  7. 07*

    The Tensor Pomeron and Low-x Deeply Virtual Compton Scattering

    Piotr Lebiedowicz🇵🇱 · Antoni Szczurek🇵🇱 · Otto Nachtmann🇩🇪

    The two-tensor-pomeron model is applied to deeply virtual Compton scattering (DVCS) on a proton. A good description of the DVCS HERA data at small Bjorken- is achieved due to a sizeable interference of soft and hard pomeron contributions. We present two fits which differ somewhat in the strength of the hard pomeron contribution. We describe, in the same framework, both the low and high regimes and the transition between them. We find that the soft-pomeron contribution is considerable up to GeV. The reggeon exchange term is particularly relevant for describing the scattering of a real photon on a proton measured at lower energies at FNAL. We find that the ratio of cross-sections for longitudinally and transversely polarized virtual photons strongly increases with . Our findings may be checked in future lepton-nucleon scattering experiments in the low- regime, for instance, at a future Electron-Ion Collider (EIC) at the BNL and LHeC at the LHC.

    hep-phActa Phys.Polon.Supp.(2023)·0 citations
  8. 08*

    -Exchange Contributions in Low-Energy Parity-Violating Scattering

    Qian-Qian Guo🇨🇳 · Hai-Qing Zhou🇨🇳

    In this work, the -exchange contributions in the low-energy elastic parity-violating scattering are discussed with the approximation . By expanding the and interactions on the momentum of photon and considering both the leading-order and the next-to-leading order interactions, we calculate the amplitudes of the -exchange diagrams. After performing the loop integral, we expand the results in the low energy limit, and obtain the analytic expressions for the amplitudes. Numerical comparisons show that the analytic expressions are very close to the full results over a large region. We investigate the power behaviors of these contributions and find that some are enhanced by a kinematic factor in the low energy limit. Additionally, in some cases, the imaginary parts of the contributions from the next-to-leading-order interactions are at the same order as those from the leading-order interactions. Furthermore, the corresponding contributions to the physical observable quantity are also discussed. Combining all the properties together, we conclude that these analytic expressions describe the leading-order contributions of all -exchange helicity amplitudes in the region with , where is the fine structure constant, is the mass of proton, and are the small quantities related to the momentum transfer and the center-of-mass energy.

    hep-phhep-exnucl-exnucl-thPRC(2023)·3 citations
  9. 09*

    The isospin and compositeness of the state

    L. R. Dai🇨🇳 · L. M. Abreu🇧🇷 · A. Feijoo🇪🇸 · E. Oset🇪🇸

    We perform a fit to the LHCb data on the state in order to determine its nature. We use a general framework that allows to have the , components forming a molecular state, as well as a possible nonmolecular state or contributions from missing coupled channels. From the fits to the data we conclude that the state observed is clearly of molecular nature from the , components and the possible contribution of a nonmolecular state or missing channels is smaller than 3\%, compatible with zero. We also determine that the state has isospin with a minor isospin breaking from the different masses of the channels involved, and the probabilities of the , channels are of the order of 69\% and 29\% with uncertainties of 1\%. The differences between these probabilities should not be interpreted as a measure of the isospin violation. Due to the short range of the strong interaction where the isospin is manifested, the isospin nature is provided by the couplings of the state found to the , components, and our results for these couplings indicate that we have an state with a very small isospin breaking. We also find that the potential obtained provides a repulsive interaction in , preventing the formation of an state, in agreement with what is observed in the experiment.

    hep-phEPJC(2023)·35 citations
  10. 10*

    Search for vector-like leptons at a Muon Collider

    Qilong Guo🇨🇳 · Leyun Gao🇨🇳 · Yajun Mao🇨🇳 · Qiang Li🇨🇳

    A feasibility study is performed for searching vector-like leptons at a muon collider, in the context of the "4321 model", an ultraviolet-complete model with rich collider phenomenology together with potential to explain recent existing some B physics measurements or anomalies. In this paper, we perform a Monte Carlo study with various machine learning techniques, and examine the projected sensitivity on vector-like leptons over a wide mass range at a TeV-scale muon collider. We find that a 3 TeV muon collider with only 10/fb of data can already be sensitive to cover the mass range of a vector-like lepton up to 1450 GeV.

    hep-phhep-exCPC(2023)·12 citations
  11. 11*

    Effective Field Theory descriptions of Higgs boson pair production

    Lina Alasfar🇩🇪 · Luca Cadamuro🇫🇷 · Christina Dimitriadi🇩🇪 · Arnaud Ferrari🇸🇪 · Ramona Gröber🇮🇹 · Gudrun Heinrich🇩🇪 · Tom Ingebretsen Carlson🇸🇪 · Jannis Lang🇩🇪 · Serhat Ördek · Laura Pereira Sánchez🇸🇪 · Ludovic Scyboz🇬🇧 · Jörgen Sjölin🇸🇪

    Higgs boson pair production is traditionally considered to be of particular interest for a measurement of the trilinear Higgs self-coupling. Yet it can offer insights into other couplings as well, since - in an effective field theory (EFT) parameterisation of potential new physics - both the production cross section and kinematical properties of the Higgs boson pair depend on various other Wilson coefficients of EFT operators. This note summarises the ongoing efforts related to the development of EFT tools for Higgs boson pair production in gluon fusion, and provides recommendations for the use of distinct EFT parameterisations in the Higgs boson pair production process. This document also outlines where further efforts are needed and provides a detailed analysis of theoretical uncertainties. Additionally, benchmark scenarios are updated. We also re-derive a parameterisation of the next-to-leading order (NLO) QCD corrections in terms of the EFT Wilson coefficients both for the total cross section and the distribution in the invariant mass of the Higgs boson pair, providing for the first time also the covariance matrix. A reweighting procedure making use of the newly derived coefficients is validated, which can be used to significantly speed up experimental analyses.

    hep-phhep-exSciPost Phys.Comm.Rep.(2024)·49 citations
  12. 12*

    Fast flavor evolution in dense neutrino systems, as described in quantum field theory

    R. F. Sawyer🇺🇸

    Investigations of dense neutrino cloud evolution through quantum kinetic equations led to the possibility of ``fast flavor" (FF) processes. It is shown here that the usual quantum kinetic equations, while signaling the instabilities that make some instances of FF possible, are being erroneously interpreted. Approaching the subject directly from the quantum field theory that defines the standard model shows the computational structures in most of the recent FF literature to be completely invalid. Our revisions also underlie what promise to be new early universe applications and a general result for relic supernova neutrinos that could be tested as a feature of the diffuse neutrino spectrum.

    hep-phPRD(2023)·4 citations
  13. 13*

    Anomalous Tau Neutrino Appearance from Light Mediators in Short-Baseline Neutrino Experiments

    P. S. Bhupal Dev🇺🇸 · Bhaskar Dutta🇺🇸 · Tao Han🇺🇸 · Doojin Kim🇺🇸

    We point out a new mechanism giving rise to anomalous tau neutrino appearance at the near detectors of beam-focused neutrino experiments, without extending the neutrino sector. The charged mesons () produced and focused in the target-horn system can decay to a (neutrino-philic) light mediator via the helicity-unsuppressed three-body decays. If such a mediator carries non-vanishing hadronic couplings, it can also be produced via the bremsstrahlung of the incident proton beam. The subsequent decay of the mediator to a tau neutrino pair results in tau neutrino detection at the near detectors, which is unexpected under the standard three-flavor neutrino oscillation paradigm. We argue that the signal flux from the charged meson decays can be significant enough to discover the light mediator signal at the on-axis liquid-argon near detector of the DUNE experiment, due to the focusing of charged mesons. In addition, we show that ICARUS-NuMI, an off-axis near detector of the NuMI beam, as well as DUNE, can observe a handful of tau neutrino events induced by beam-proton bremsstrahlung.

    hep-phhep-exPLB(2024)·12 citations
  14. 14*

    Bootstrapping the relativistic two-body problem

    Christoph Dlapa🇩🇪 · Gregor Kälin🇩🇪 · Zhengwen Liu🇩🇰 · Rafael A. Porto🇩🇪

    We describe the formalism to compute gravitational-wave observables for compact binaries via the effective field theory framework in combination with modern tools from collider physics. We put particular emphasis on solving the "multi-loop" integration problem via the methodology of differential equations and expansion by regions. This allows us to "bootstrap" the two-body relativistic dynamics in the Post-Minkowskian (PM) expansion from boundary data evaluated in the near-static (soft) limit. We illustrate the procedure with the derivation of the total spacetime impulse in the scattering of non-spinning bodies to 4PM (three-loop) order, i.e. , including conservative and dissipative effects.

    hep-thgr-qchep-phJHEP(2023)·86 citations
  15. 15*

    Color-factor symmetry of the amplitudes of Yang-Mills and biadjoint scalar theory using perturbiner methods

    Stephen G. Naculich🇺🇸

    Color-factor symmetry is a property of tree-level gauge-theory amplitudes containing at least one gluon. BCJ relations among color-ordered amplitudes follow directly from this symmetry. Color-factor symmetry is also a feature of biadjoint scalar theory amplitudes as well as of their equations of motion. In this paper, we present a new proof of color-factor symmetry using a recursive method derived from the perturbiner expansion of the classical equations of motion.

    hep-thhep-phJHEP(2023)·3 citations
  16. 16*

    SpinorHelicity4D: a Mathematica toolbox for the four-dimensional spinor-helicity formalism

    Manuel Accettulli Huber🇬🇧

    We present the Mathematica package SpinorHelicity4D, a dedicated suite for analytic and numeric calculations involving four-dimensional massless and massive spinor-helicity formalism. Analytic features of the package include for example: manipulation of contracted and uncontracted spinor quantities, automated application of Schouten identities for expression simplification, contractions of spinor products into chains, re-expression of chains in terms of Dirac traces and evaluation of such traces, derivatives of arbitrary functions of spinor quantities. Numeric features of the package include among others: generation of arbitrary -point numerical complex kinematics, allowing for both massless and massive external states, fully numeric or parametric kinematics, and numeric generation on either or , the latter providing output immediately suitable for finite field applications. Furthermore, the package features user-friendly, intuitive but also highly customizable input options, thus providing an approachable tool for the casual user while still supporting more advanced applications for more adept and frequent users. All of the output is returned in the standard bracket notation, making it easily interpretable, but at the same it retains all of the analytic properties of the objects, allowing for copy-pasted and manipulated output to be provided as new input. This makes it ideal for front-end applications on a Mathematica notebook, while still allowing for deployment on a cloud server for more heavy calculations.

    hep-thhep-ph10 citations
  17. 18*

    Scaling functions of the three-dimensional , and models and their finite size dependence in an external field

    Frithjof Karsch🇩🇪 · Marius Neumann🇩🇪 · Mugdha Sarkar🇹🇼

    We analyze scaling functions in the -, , and universality classes and their finite size dependence using Monte Carlo simulations of improved models. Results for the scaling functions are fitted to the Widom-Griffiths form, using a parametrization also used in analytic calculations. We find good agreement on the level of scaling functions and the location of maxima in the universal part of susceptibilities. We also find that an earlier parametrization of the scaling function, using 14 parameters, is well reproduced when using the Widom-Griffiths form with only three parameters. We furthermore show that finite size corrections to the scaling functions are distinctively different in the and universality classes and determine the volume dependence of the peak locations in order parameter and mixed susceptibilities.

    hep-latcond-mat.stat-mechhep-phPRD(2023)·17 citations
  18. 19*

    Investigation of the cause of the discrepancies between calculated running sums for nuclear matrix elements of two-neutrino double- decay

    J. Terasaki🇨🇿

    A qualitative difference in the running sum for the nuclear matrix element of the two-neutrino double- decay of Xe was found four years ago between quasiparticle random-phase approximation (QRPA) and shell model calculations. The former result has large increase and decrease with respect to the excitation energy of the intermediate state, and the latter one is an almost monotonically and mildly increasing function. My QRPA calculations independently of the above one do not have a remarkable decrease. This discrepancy is a serious problem affecting the reliability of calculations of the neutrinoless double- decay, and the cause was unknown. I perform several relevant test calculations and make an analytical consideration to find the cause, which is found to be in the strength of the attractive interactions. The possible major local decrease in the running sum is also explained analytically. The interactions of my QRPA calculation are appropriate in terms of the strength, thus the almost monotonic behavior is reasonable.

    nucl-thhep-exhep-phnucl-exPRC(2023)·2 citations
  19. 20*

    Axion-photon conversion of GRB221009A

    Luohan Wang🇨🇳 · Bo-Qiang Ma🇨🇳

    The newly observed gamma ray burst GRB221009A exhibits the existence of 10~TeV-scale photons, and the axion-photon conversion has been suggested as a candidate to explain such energetic features of GRB221009A. In this work we adopt a model to calculate the conversion probability of the energetic photons from GRB221009A to the Earth. The result shows that the penetration probability of photons with energy above ~TeV can be up to to depending on the coupling constant and the axion mass , together on the magnetic field parameters of the source galaxy of GRB221009A. We show that the parameters of the source galaxy, with the magnetic field handled by a cellular model, contribute a lot of uncertainties to the penetration probability, so we have more freedom to reconcile a variety of axionlike particle parameters from other observations with the Large High Altitude Air Shower Observatory observation. By comparing the results in this article with the data from Large High Altitude Air Shower Observatory, we can obtain more precise constraints on the ranges of these parameters.

    astro-ph.HEhep-phPRD(2023)·25 citations
  20. 21*

    Hybrid stars with reactive interfaces: analysis within the Nambu-Jona-Lasinio model

    C. H. Lenzi🇧🇷 · G. Lugones🇧🇷 · C. Vasquez🇧🇷

    It has been shown recently that quark-hadron conversions at the interface of a hybrid star may have a key role on the dynamic stability of the compact object. In this work we perform a systematic study of hybrid stars with reactive interfaces using a model-agnostic piecewise-polytropic hadronic equation of state and the Nambu-Jona-Lasinio model for three-flavor quark matter. For the hadronic phase we use a soft, an intermediate and a stiff parametrization that match at {with predictions} based on chiral effective field theory (cEFT) interactions. In the NJL Lagrangian we include scalar, vector and 't Hooft interactions. The vector coupling constant is treated as a free parameter. We also consider that there is a split between the deconfinement and the chiral phase transitions which is controlled by changing the conventional value of the vacuum pressure in the NJL thermodynamic potential by , being a free parameter. We analyze the mass-radius (-) relation in the case of rapid () and slow () conversions, being the reaction timescale. In the case of slow interface reactions we find - curves with a cusp at the maximum mass point where a pure hadronic branch and a slow-stable hybrid star (SSHS) branch coincide. We find that the length of the slow-stable branch grows with the increase of the transition density and the energy density jump at the hadron-quark interface. We calculate the tidal deformabilities of SSHSs and analyse them in the light of the GW170817 event.

    nucl-thastro-ph.HEastro-ph.SRhep-phPRD(2023)·11 citations
  21. 22*

    Kinetic relaxation and Bose-star formation in multicomponent dark matter- I

    Mudit Jain🇺🇸 · Mustafa A. Amin🇺🇸 · Jonathan Thomas🇺🇸 · Wisha Wanichwecharungruang🇺🇸

    Using wave kinetics, we estimate the emergence time-scale of gravitating Bose-Einstein condensates/Bose stars in the kinetic regime for a general multicomponent Schrödinger-Poisson (SP) system. We identify some effects of the diffusion and friction pieces in the wave-kinetic Boltzmann equation (at leading order in perturbation theory) and provide estimates for the kinetic nucleation rate of condensates. We test our analysis using full dimensional simulations of multicomponent SP system. With an eye towards applications to multicomponent dark matter, we investigate two general cases in detail. First is a massive spin- field with components (scalar , vector and tensor ). We find that for a democratic population of different components, the condensation time-scale is , where is the condensation time scale for the scalar case. Second is the case of two scalars with different boson masses. In this case, we map-out how the condensation time depends on the ratios of their average mass densities and boson masses, revealing competition and assistance between components, and a guide towards which component condenses first. For instance, with and not too disparate mass densities, we verify that the time scale of condensation of the first species quickly becomes independent of , whereas for equal average number densities, the emergence time scale decreases with increasing .

    astro-ph.COhep-phnlin.PSPRD(2023)·44 citations
  22. 23*

    A novel integrated Sachs-Wolfe effect from Early Dark Energy

    Tristan L. Smith🇺🇸 · John T. Giblin Jr.🇺🇸 · Mustafa A. Amin🇺🇸 · Mary Gerhardinger🇺🇸 · Ericka Florio🇺🇸 · Matthew Cerep🇺🇸 · Shar Daniels🇺🇸

    We study the nonlinear effects of minimally coupled, massless, cosmological scalar fields on the cosmic microwave background (CMB). These fields can exhibit post-recombination parametric resonance and subsequent nonlinear evolution leading to novel contributions to the gravitational potential. We compute the resulting contributions to the CMB temperature anisotropies through the time-variation of the gravitational potential (i.e., the integrated Sachs-Wolfe (ISW) effect). We find that fields that constitute 5% of the total energy density and become dynamical at can produce marginally observable ISW signals at multipoles . Fields that become dynamical at earlier times and/or have initial displacements at a flatter part of their potential, produce ISW contributions that are significantly larger and at higher multipoles. We calculate these dynamics and the resulting evolution of gravitational perturbations using analytic estimates alongside detailed nonlinear lattice simulations, which couple scalar fields and cosmological fluids to a perturbed metric. Finally, we discuss the possibility of detecting these features with future high-resolution CMB observations.

    astro-ph.COhep-phPRD(2023)·9 citations
  23. 24*

    Eternal binaries

    Jaime Redondo-Yuste🇩🇰 · Vitor Cardoso🇩🇰 · Caio F. B. Macedo🇧🇷 · Maarten van de Meent🇩🇰

    The two-body problem is extensively studied in open systems and asymptotically flat spacetimes. However, there are many systems where radiation is trapped: they range from radiating charges in cavities to low-energy excitations of massive degrees of freedom, to anti-de Sitter spacetimes. Here, we study the problem of motion of a pointlike particle orbiting a massive compact object inside a cavity. We first show that - assuming circular motion - there are initial conditions for which the self-force vanishes and the binary is eternal. We then consider the evolution of the system under radiation reaction in a toy model which we argue captures the essentials of orbiting particles. We show that eternal circular binaries may exist. We also show that the presence of cavity modes leads to chaos in regimes of strong coupling or when the system is initialized close enough to a resonance. Our results have implications for physics in anti-de Sitter spacetimes and possibly for binaries evolving within dark matter haloes, if it consists on massive fundamental fields.

    gr-qcastro-ph.HEhep-phhep-thPRD(2023)·2 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.