PaperPanorama

HEP Phenomenology·hep-ph

Thu·Jun 8, 2023

24 papers19 primary·5 cross-listed·reconstructed*

  1. 01*

    High-dimensional and Permutation Invariant Anomaly Detection

    Vinicius Mikuni🇺🇸 · Benjamin Nachman🇺🇸

    Methods for anomaly detection of new physics processes are often limited to low-dimensional spaces due to the difficulty of learning high-dimensional probability densities. Particularly at the constituent level, incorporating desirable properties such as permutation invariance and variable-length inputs becomes difficult within popular density estimation methods. In this work, we introduce a permutation-invariant density estimator for particle physics data based on diffusion models, specifically designed to handle variable-length inputs. We demonstrate the efficacy of our methodology by utilizing the learned density as a permutation-invariant anomaly detection score, effectively identifying jets with low likelihood under the background-only hypothesis. To validate our density estimation method, we investigate the ratio of learned densities and compare to those obtained by a supervised classification algorithm.

    hep-phcs.AIcs.LGhep-exSciPost Phys.(2024)·28 citations
  2. 02*

    Master Integrals for Electroweak corrections to -- Light quark contributions

    Gabriele Fiore🇺🇸 · Ciaran Williams🇺🇸

    We present a calculation of the master integrals (MI's) required for the calculation of the Electroweak corrections to production in which the process contains a light quark loop. The integrals can be broken down into five categories based on the flow of the heavy vector bosons throughout the loop. Three of the families are planar, and two are non-planar. We determine a canonical basis for each family which allows an efficient solution of the resulting differential equations via iterated integrals. We calculate the families in relevant physical kinematics and obtain an efficient numerical evaluation based on an implementation of Chen-iterated integrals.

    hep-phEPJC(2023)·3 citations
  3. 03*

    Cosmological probes of Grand Unification: Primordial Blackholes & scalar-induced Gravitational Waves

    Anish Ghoshal🇵🇱 · Ahmad Moursy🇪🇬 · Qaisar Shafi🇺🇸

    We investigate the inflationary cosmology involving an SU(5) GUT (grand unified theory) singlet scalar with non-minimal coupling to the Ricci scalar. In this scenario the scale of grand unification is set by the inflaton vev when the inflaton rolls down its potential towards its minimum , thereby relating inflationary dynamics to GUT symmetry breaking with a prediction for the tensor-to-scalar ratio to be tested by the next generation CMB experiments. We show in this inflationary framework involving inflection-point how a suitable choice of parameters in leads to a bump in the scalar power spectrum with production of Primordial Blackholes (PBH) of masses g (). We derive the constraints on the self quartic and mixed quartic couplings of the inflaton in SU(5) that are consistent with the inflationary analysis. Moreover, we also show that this scenario leads to large amplitude induced second-order tensor perturbations propagating as Gravitational Waves (GW) with amplitude and peak frequency (0.1 - 1) Hz, which can be detected in the next generation GW observatories like LISA, BBO, ET, etc. Thus, we unify the framework with PBH via inflection-point inflation showing how the upcoming measurements of PBH and GW will enable us to probe the scale of symmetry breaking, and thereby complementing the laboratory based experiments. We also discuss scenarios involving the Pati-Salam and Trinification gauge groups and its impact on quartic and mixed-quartic couplings that may lead to PBH and detectable GW signals.

    hep-phastro-ph.COPRD(2023)·19 citations
  4. 04*

    Functional renormalization group study of neutral and charged pion under magnetic fields in the quark-meson model

    Rui Wen🇨🇳 · Shi Yin🇨🇳 · Wei-jie Fu🇨🇳 · Mei Huang🇨🇳

    We calculated the masses of neutral and charged pion and pion decay constants under an extra magnetic field at zero temperature. The quantum fluctuations are integrated through the functional renormalization group. We consider the quark and meson propagators in the Landau level representation and weak-field expansion, respectively. The neutral pion mass monotonically decreases with the magnetic field, while the charged pion mass monotonically increases with the magnetic field. The pion decay constant and the quark mass show the magnetic catalysis behavior at vanishing temperature. The neutral pion mass and pion decay constant are quantitatively in agreement with the lattice QCD results in the region of , and no non-monotonic mass behavior for charged pion has been observed in this framework.

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

    Defrosting and Blast Freezing Dark Matter

    Marcos M. Flores🇺🇸 · Chris Kouvaris🇬🇷 · Alexander Kusenko🇺🇸

    We show that the present-day dark matter abundance can be produced through a novel mechanism that involves a very rapid thermal freeze-out caused by inhomogeneous heating and successive fast cooling of small fireballs in the early Universe. The fireballs can be produced from energy deposited in small scale structure growth induced by Yukawa interactions in certain particle species. Yukawa interactions are known to cause growth of halos even during a radiation dominated era, and the same interactions facilitate cooling and collapse of the halos by the emission of scalars. Energy deposited in the Standard Model plasma at the locations of the halo collapse can heat the plasma, re-establishing thermal equilibrium. The subsequent expansion and cooling of plasma fireballs leads to freeze-out of dark matter on timescales much shorter than the Hubble time. This mechanism can produce the right abundance of dark matter for masses and annihilation cross sections previously thought to be ruled out.

    hep-phPRD(2023)·9 citations
  6. 06*

    Electroweak Corrections to Higgs Boson Decays in a Complex Singlet Extension of the SM and their Phenomenological Impact

    Felix Egle🇩🇪 · Margarete Mühlleitner🇩🇪 · Rui Santos🇵🇹 · João Viana🇵🇹

    The complex singlet extension CxSM of the Standard Model (SM) is a simple extension of the SM with two visible Higgs bosons in the spectrum and a Dark Matter (DM) candidate. In this paper we complete the computation of the next-to-leading (NLO) electroweak (EW) corrections to on-shell and non-loop-induced Higgs decays. Our calculations are implemented in the code EWsHDECAY which also includes the relevant QCD corrections. Performing an extensive parameter scan in the model and including all relevant theoretical and experimental single- and di-Higgs as well as DM constraints, we obtain a viable parameter sample. We find that current DM constraints are able to test the model in DM mass regions where collider searches are not sensitive. The relative EW corrections turn out to be large for scenarios with relatively large couplings, threshold effects or small leading-order (LO) widths. Otherwise, they are of typical EW size and can amount up to about 20-25%. The theory uncertainty derived from the change of the renormalization scheme dependence then is of a few per cent. While the NLO corrections applied in the constraints due to single- and di-Higgs searches impact the validity of specific parameter points, the overall shape of the allowed parameter region is not yet sensitive to the EW corrections. This picture will change with further increased experimental precision in the future and necessitates precise predictions on the theory side as presented in this paper.

    hep-phJHEP(2023)·15 citations
  7. 07*

    Charged meson masses under strong magnetic fields: gauge invariance and Schwinger phases

    D. Gomez Dumm🇦🇷 · S. Noguera🇪🇸 · N. N. Scoccola🇦🇷

    We study the role of the Schwinger phase (SP) that appears in the propagator of a charged particle in the presence of a static and uniform magnetic field . We first note that this phase cannot be removed by a gauge transformation; far from this, we show that it plays an important role in the restoration of the symmetries of the system. Next, we analyze the effect of SPs in the one-loop corrections to charged pion and rho meson selfenergies. To carry out this analysis we consider first a simple form for the meson-quark interactions, and then we study the and propagators within the Nambu-Jona-Lasinio model, performing a numerical analysis of the dependence of meson lowest energy states. For both and mesons, we compare the numerical results arising from the full calculation -- in which SPs are included in the propagators, and meson wavefunctions correspond to states of definite Landau quantum number -- and those obtained within alternative schemes in which SPs are neglected (or somehow eliminated) and meson states are described by plane waves of definite four-momentum.

    hep-phPRD(2023)·16 citations
  8. 08*

    Progress on from Lattice QCD

    Hartmut Wittig🇩🇪

    I review the status of lattice QCD calculations of the hadronic contributions to the muon's anomalous magnetic moment, focussing on the hadronic vacuum polarisation contribution which dominates the uncertainty of the Standard Model prediction.This quantity exhibits a tension between recent lattice QCD results and the traditional data-driven dispersive method. I discuss the implications for the running of the electromagnetic coupling and the consistency of global fits using electroweak precision data.

    hep-phhep-lat31 citations
  9. 09*

    The chiral anomaly and the pion transition form factor: beyond the cutoff

    Hao Dang🇨🇳 · Zanbin Xing🇨🇳 · M. Atif Sultan🇨🇳 · Khépani Raya🇪🇸 · Lei Chang🇨🇳

    In the presence of a momentum cutoff, effective theories seem unable to faithfully reproduce the so called chiral anomaly in the Standard Model. A novel prospect to overcome this related issue is discussed herein via the calculation of the transition form factor, , whose normalization is intimately connected with the chiral anomaly and dynamical chiral symmetry breaking (DCSB). To compute such transition, we employ contact interaction model of Quantum Chromodynamics (QCD) under a modified rainbow ladder truncation, which automatically generates a quark anomalous magnetic moment term, weighted by a strenght parameter . This term, whose origin is also connected with DCSB, is interpreted as an additional interaction that mimics the complex dynamics beyond the cutoff. By fixing to produce the value of dictated by the chiral anomaly, the computed transition form factor, as well as the interaction radius and neutral pion decay width, turn out to be comparable with QCD-based studies and experimental data.

    hep-phPRD(2023)·9 citations
  10. 10*

    suppression in a rotating magnetized holographic QGP matter

    Yan-Qing Zhao🇨🇳 · Defu Hou🇨🇳

    We study the dissociation effect of in magnetized, rotating QGP matter at finite temperature and chemical potential using gauge/gravity duality. By incorporating angular velocity into the holographic magnetic catalysis model, we analyze the influence of temperature, chemical potential, magnetic field, and angular velocity on the properties of meson. The results reveal that temperature, chemical potential, and rotation enhance the dissociation effect and increase the effective mass in the QGP phase. However, the magnetic field suppresses dissociation, and its effect on the effective mass is non-trivial. Additionally, we explore the interplay between magnetic field and rotation, identifying a critical angular velocity that determines the dominant effect. As a parallel study, we also examine the rotation effect in the holographic inverse magnetic catalysis model, although the magnetic field exhibits distinctly different behaviors in these two models, the impact of rotation on the dissociation effect of is similar. Finally, we investigate the influence of electric field and demonstrate that it also speeds up the dissociation.

    hep-phEPJC(2023)·18 citations
  11. 12*

    Coupled-channel influence on the line shape

    N. N. Achasov🇷🇺 · G. N. Shestakov🇷🇺

    The current situation with the recently discovered resonance is very paradoxical: it is believed that must be strongly coupled with two vector mesons, but there is no direct experimental confirmation of this yet. Based on the assumption that the is a state similar to the four-quark state from the MIT bag, belonging to either the or the multiplet, we analyze the influence of the strong coupling to the vector channels , , and on its line shape in the decay channels into pseudoscalar mesons , , and . This effect depends on the location of the resonance mass relative to the nominal thresholds of vector channels. For example, if MeV, then the influence turns out to be hidden in a fairly wide range of coupling constants. On the whole, our analysis shows that, to confirm the presence of the strong coupling to the vector channels, utterly required is the direct detection of the decays , , . The appearance of even certain hints at the existence of these decays would make it possible to fundamentally advance in understanding the nature of the new state.

    hep-phhep-exnucl-exnucl-thPRD(2023)·9 citations
  12. 13*

    Higgs boson rapidity distribution in bottom annihilation at NNLL and beyond

    Goutam Das🇩🇪

    We present precise resummed predictions for Higgs boson rapidity distribution through bottom quark annihilation at next-to-next-to-leading logarithmic (NNLL) accuracy matched to next-to-next-to-leading order (NNLO) and at next-to-next-to-next-to-leading logarithmic (N3LL) accuracy matched to next-to-next-to-next-to-leading order soft-virtual (N3LOsv) in the strong coupling. Exploiting the universal behavior of soft radiation near the threshold, we determine the analytic expressions for the process-dependent and universal perturbative ingredients for threshold resummation in double singular limits of partonic threshold variables . Subsequently, the threshold resummation is performed in the double Mellin space within the standard QCD framework. The new third-order process-dependent non-logarithmic coefficients are determined using three-loop bottom quark form factor and third-order quark soft distribution function in rapidity distribution. The effect of these new resummed coefficients are studied at the TeV LHC. We observe a better perturbative convergence in the resummed predictions on the Higgs rapidity spectrum in bottom quark annihilation. We also find that the NNLL and N3LL corrections are sizeable which typically are of the order of and over the respective available fixed orders with the scale uncertainty remaining at the same level as the fixed order.

    hep-phPRD(2023)·9 citations
  13. 14*

    Investigating the spectroscopy behavior of undetected -wave charmed baryons

    Si-Qiang Luo🇨🇳 · Xiang Liu🇨🇳

    In this work, we investigate the spectroscopic properties of -wave charmed baryons, which have not yet been observed in experiments. We employ a non-relativistic potential model and utilize the Gaussian expansion method to obtain the mass spectra of these charmed baryons. Additionally, we focus on the two-body Okubo-Zweig-Iizuka allowed strong decay behaviors, which plays a crucial role in characterizing the properties of these baryons. Our comprehensive analyses of the mass spectra and two-body Okubo-Zweig-Iizuka allowed decay behaviors provides valuable insights for future experimental investigations. This study significantly contributes to our understandings of the spectroscopic properties of -wave charmed baryons.

    hep-phhep-exPRD(2023)·23 citations
  14. 15*

    Higgs Inflation and the Electroweak Gauge Sector

    Stephon Alexander🇺🇸 · Cyril Creque-Sarbinowski🇺🇸 · Humberto Gilmer🇺🇸 · Katherine Freese🇺🇸

    We introduce a new method that allows for the Higgs to be the inflaton. That is, we let the Higgs be a pseudo-Nambu-Goldstone (pNG) boson of a global coset symmetry that spontaneously breaks at an energy scale and give it a suitable Chern-Simons interaction, with the dimensionless Chern-Simons coupling strength and an decay constant. As a result, slow-roll inflation occurs via -induced friction down a steep sinusoidal potential. In order to obey electroweak symmetry, the lowest-order Chern-Simons interaction is required to be quadratic in the Higgs with coupling strength . Higher-order interaction terms keep the full Lagrangian nearly invariant under the approximate pNG shift symmetry. Employing the simplest symmetry coset , -folds of inflation occur when , with the weak isospin gauge coupling constant. Small values of the decay constant, , which are needed to address the Higgs hierarchy problem, are ruled out by electric dipole measurements and so successfully explaining inflation requires large . We discuss possible methods to achieve such large couplings and other alternative Higgs inflation scenarios outside the standard modified-gravity framework.

    hep-phastro-ph.COgr-qcFortsch.Phys.(2025)·3 citations
  15. 16*

    Heavy QCD axion dark matter from avoided level crossing

    David Cyncynates🇺🇸 · Jedidiah O. Thompson🇺🇸

    The QCD axion offers a natural resolution to the strong CP problem and provides a compelling dark matter candidate. If the QCD axion constitutes all the dark matter, the simplest models pick out a narrow range of masses around . We point out a natural production mechanism for QCD axion dark matter at masses up to existing astrophysical bounds ( for the most minimal models and for nucleophobic models). If the QCD axion mixes with a sterile axion, the relative temperature dependence of their potentials can lead to an avoided level crossing of their mass eigenstates. This leads to a near-total transfer of energy density from the sterile axion to the QCD axion, resulting in a late-time QCD axion abundance sufficient to make up all of present-day dark matter. Our result provides additional theoretical motivation for several direct detection experiments that will probe this part of parameter space in the near future.

    hep-phastro-ph.COPRD(2023)·37 citations
  16. 17*

    Gravitational waves from phase transitions and cosmic strings in neutrino mass models with multiple majorons

    Pasquale Di Bari🇬🇧 · Stephen F. King🇬🇧 · Moinul Hossain Rahat🇬🇧

    We explore the origin of Majorana masses within the majoron model and how this can lead to the generation of a distinguishable primordial stochastic background of gravitational waves. We first show how in the simplest majoron model only a contribution from cosmic string can be within the reach of planned experiments. We then consider extensions containing multiple complex scalars, demonstrating how in this case a spectrum comprising contributions from both a strong first order phase transition and cosmic strings can naturally emerge. We show that the interplay between multiple scalar fields can amplify the phase transition signal, potentially leading to double peaks over the wideband sloped spectrum from cosmic strings. We also underscore the possibility of observing such a gravitational wave background to provide insights into the reheating temperature of the universe. We conclude highlighting how the model can be naturally combined with scenarios addressing the origin of matter of the universe, where baryogenesis occurs via leptogenesis and a right-handed neutrino plays the role of dark matter.

    hep-phastro-ph.COhep-thJHEP(2024)·18 citations
  17. 18*

    Novel approaches to determine and meson production fractions

    Florian Bernlochner🇩🇪 · Martin Jung🇮🇹 · Munira Khan🇩🇪 · Greg Landsberg🇺🇸 · Zoltan Ligeti🇺🇸

    We propose novel methods to determine the and decay rates. The precision to which they and their ratio are known yields at present a limiting uncertainty around in measurements of absolute decay rates, and thus in a variety of applications, such as precision determinations of elements of the Cabibbo-Kobayashi-Maskawa matrix and flavor symmetry relations. The new methods we propose are based in one case on exploiting the data sets, in the other case on the different average number of charged tracks in and decays. We estimate future sensitivities using these methods and discuss possible measurements of at the (HL-)LHC.

    hep-phhep-exPRD(2024)·16 citations
  18. 19*

    Exploration of hadronization through heavy flavor production at the future Electron-Ion Collider

    Xuan Li🇺🇸

    The future Electron-Ion Collider (EIC), which is expected to start construction at Brookhaven National Laboratory in 2025, will utilize high-luminosity high-energy electron+proton and electron+nucleus collisions to explore several fundamental questions in the high energy and nuclear physics fields. Exploring how matter is formed from quarks and gluons, which is referred to as the hadronization process, is one of the EIC science objectives. The EIC project detector design led by the ePIC collaboration can realize a series of high precision heavy flavor hadron and jet measurements. Heavy flavor jet substructure and heavy flavor hadrons inside jets, which can provide direct information about the heavy quark hadronization process, have been studied in simulation for electron+proton and electron+nucleus collisions at EIC. The associated physics projections and comparison with latest theoretical calculations will be presented.

    hep-phhep-exnucl-exnucl-th0 citations
  19. 20*

    Momentum Shell in Quarkyonic Matter from Explicit Duality: A Dual Model for Cold, Dense QCD

    Yuki Fujimoto🇺🇸 · Toru Kojo🇯🇵 · Larry D. McLerran🇺🇸

    We present a model of cold QCD matter that bridges nuclear and quark matter through the duality relation between quarks and baryons. The baryon number and energy densities are expressed as functionals of either the baryon momentum distribution, , or the quark distribution, , which are subject to the constraints on fermions, . The theory is ideal in the sense that the confinement of quarks into baryons is reflected in the duality relation between and , while other possible interactions among quarks and baryons are all neglected. The variational problem with the duality constraints is formulated and we explicitly construct analytic solutions, finding two distinct regimes: A nuclear matter regime at low density and a Quarkyonic regime at high density. In the Quarkyonic regime, baryons underoccupy states at low momenta but form a momentum shell with on top of a quark Fermi sea. Such a theory describes a rapid transition from a soft nuclear equation of state to a stiff Quarkyonic equation of state. At this transition, there is a rapid increase in the pressure.

    nucl-thastro-ph.HEhep-phPRL(2024)·63 citations
  20. 21*

    Dark Matter Constraints from Isomeric Hf

    D. S. M. Alves🇺🇸 · S. R. Elliott🇺🇸 · R. Massarczyk🇺🇸 · S. J. Meijer🇺🇸 · H. Ramani🇺🇸

    We describe a first measurement of the radiation from a Hf sample to search for dark matter. The flux from this sample, possessed by Los Alamos National Laboratory nuclear chemistry, was measured with a Ge detector at a distance of 4 ft due to its high activity. We search for s that cannot arise from the radioactive decay of Hf, but might arise from the production of a nuclear state due to the inelastic scattering with dark matter. The limits obtained on this flux are then translated into constraints on the parameter space of inelastic dark matter. Finally, we describe the potential reach of future studies with Hf.

    nucl-exhep-phhep-thPRL(2023)·11 citations
  21. 22*

    The magnetic dual chiral density wave phase in a rotating cold quark matter

    H. Mortazavi Ghalati🇮🇷 · N. Sadooghi🇮🇷

    The effect of rotation on the formation of the magnetic dual chiral density wave (\MD) in a dense and magnetized cold quark matter is studied. This phase is supposed to exist in the extreme conditions prevailing, e.g., in a neutron star. These conditions are, apart from high densities and strong magnetic fields, a relatively large angular velocity. To answer the question of whether the rotation enhances or suppresses the formation of this phase, we first determine the effect of rotation on the energy dispersion relation of a fermionic system in the presence of a constant magnetic field and then focus on the thermodynamic potential of the model at low temperature and finite chemical potential . The thermodynamic potential consists, in particular, of an anomalous part leading to certain topological effects. We show that in comparison with the nonrotating case, a term proportional to the angular velocity appears in this anomalous potential. We then solve the corresponding gap equations to the chiral and spatial modulation condensates, and study the dependence of these dynamical variables on the chemical potential (), magnetic field (), and angular velocity (). It turns out that the interplay between these parameters suppresses the formation of the \MD~phase in relevant regimes for cold neutron stars. This is interpreted as the manifestation of the inverse magnetorotational catalysis, which is also reflected in the phase portraits -, -, and -, explored in this work.

    nucl-thhep-phPRD(2023)·12 citations
  22. 23*

    Electromagnetic high-frequency gravitational wave detection

    Valerie Domcke🇨🇭

    Ultra-high frequency gravitational waves in the MHz to THz regime promise a unique possibility to probe the very early universe, particle physics at very high energies and exotic astrophysical objects - but achieving the sensitivity required for detection is an immense challenge. This is a brief summary of recent progress in electromagnetic high-frequency gravitational wave searches, which are based on classical electromagnetism in a space-time perturbed by gravitational waves. A particular focus is given to synergies with axion searches and atomic precision measurements. This article was prepared as proceedings for Moriond EW 2023.

    gr-qcastro-ph.COhep-ph16 citations
  23. 24*

    Causality Bounds in Quadratic Inflation from Purely Virtual Particles

    Alessandro Dondarini🇮🇹

    The "" slow roll inflation combined with General Relativity is largely excluded by Planck data. In this paper, we consider the same potential combined with the gravity of purely virtual particles (or fakeons), where the would-be ghost introduced by the Weyl tensor term, , is quantized with the fakeon prescription. We compute the tensor power spectrum in the full theory by means of the Cosmic Renormalization Group formalism and critically examine its physical meaning. In particular, we show that it is not possible to retrieve the power spectrum of the fakeon free-theory by considering the decoupling limit of the purely virtual particles. We provide a physical explanation in terms of the causal structure of the theory to infer that a model of quadratic inflation from purely virtual particles is also discarded from a phenomenological point of view.

    hep-thgr-qchep-phPRD(2023)·3 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.