PaperPanorama

HEP Phenomenology·hep-ph

Thu·Feb 16, 2023

23 papers18 primary·5 cross-listed·reconstructed*

  1. 01*

    Opportunistic CP Violation

    Quentin Bonnefoy🇺🇸 · Emanuele Gendy🇩🇪 · Christophe Grojean🇩🇪 · Joshua T. Ruderman🇺🇸

    In the electroweak sector of the Standard Model, CP violation arises through a very particular interplay between the three quark generations, as described by the Cabibbo--Kobayashi--Maskawa (CKM) mechanism and the single Jarlskog invariant . Once generalized to the Standard Model Effective Field Theory (SMEFT), this peculiar pattern gets modified by higher-dimensional operators, whose associated Wilson coefficients are usually split into CP-even and odd parts. However, CP violation at dimension four, i.e., at the lowest order in the EFT expansion, blurs this distinction: any Wilson coefficient can interfere with and mediate CP violation. In this paper, we study such interferences at first order in the SMEFT expansion, , and we capture their associated parameter space via a set of 1551 linear CP-odd flavor invariants. This construction describes both new, genuinely CP-violating quantities as well as the interference between and CP-conserving ones. We call this latter possibility \textit{opportunistic CP violation}. Relying on an appropriate extension of the matrix rank to Taylor expansions, which we dub \emph{Taylor rank}, we define a procedure to organize the invariants in terms of their magnitude, so as to retain only the relevant ones at a given precision. We explore how this characterization changes when different assumptions are made on the flavor structure of the SMEFT coefficients. Interestingly, some of the CP-odd invariants turn out to be less suppressed than , even when they capture opportunistic CPV, demonstrating that CP-violation in the SM, at dimension 4, is \textit{accidentally small.}

    hep-phJHEP(2023)·17 citations
  2. 03*

    Empirical Determination of the Pion Mass Distribution

    Yin-Zhen Xu🇪🇸 · Khépani Raya🇪🇸 · Zhu-Fang Cui🇨🇳 · Craig D. Roberts🇨🇳 · J. Rodríguez-Quintero🇪🇸

    Existing pion+nucleus Drell-Yan and electron+pion scattering data are used to develop ensembles of model-independent representations of the pion generalised parton distribution (GPD). Therewith, one arrives at a data-driven prediction for the pion mass distribution form factor, . Compared with the pion elastic electromagnetic form factor, is harder: the ratio of the radii derived from these two form factors is . Our data-driven predictions for the pion GPD, related form factors and distributions should serve as valuable constraints on theories of pion structure.

    hep-phhep-exhep-latnucl-ex+1Chin.Phys.Lett.(2023)·24 citations
  3. 04*

    Prospects for ditauonium discovery at colliders

    David d'Enterria🇨🇭 · Hua-Sheng Shao🇫🇷

    The feasibility of observing ditauonium, the bound state of two tau leptons, at colliders (BES III at GeV, Belle II at GeV, a future super tau-charm factory (STCF) at , and the FCC-ee at GeV) as well as in hadronic and photon-photon collisions at the LHC, is studied. Cross sections and expected yields for spin-0 para- () and spin-1 ortho- () ditauonium are presented for nine different production and decay processes. Para-ditauonium can be observed at the FCC-ee via photon fusion in its diphoton decay (). Ortho-ditauonium can be observed at STCF via , where a threshold scan with monochromatized beams can also provide a very precise extraction of the tau lepton mass with a keV) uncertainty or less. Observing pp at the LHC is possible by identifying its displaced vertex with a good control of the combinatorial dimuon background. In addition, we compute the rare decay branching fractions of ditauonium into quarkonium plus a photon.

    hep-phhep-exnucl-exnucl-thPLB(2023)·32 citations
  4. 05*

    Charged lepton-flavor violating processes and suppression of nonunitary mixing effects in low-scale seesaw models

    J. C. Garnica🇲🇽 · G. Hernández-Tomé🇲🇽 · E. Peinado🇲🇽

    We examine the parameter space region of the inverse seesaw model that is consistent with neutrino oscillation data. We focus on the correlation between the current limits from the search of the lepton flavor violating decay and the non-standard effects associated with the presence of new heavy neutrino states. Unlike what we would expect from an inverse seesaw model, we present a structure for the neutrinos mass matrices in which the rates of charged lepton flavor-violating processes are negligible. Additionally, we provide a model based on symmetries for such a scenario.

    hep-phPRD(2023)·9 citations
  5. 06*

    The Phenomenological Research on Higgs and dark matter in the Next-to-Minimal Supersymmetric Standard Model

    Zhaoxia Heng🇨🇳 · Shenshen Yang🇨🇳 · Xingjuan Li🇨🇳 · Liangliang Shang🇨🇳

    The -invariant next-to-minimal supersymmetric standard model (NMSSM) can provide a candidate for dark matter (DM). It can also be used to explain the hypothesis that the Higgs signal observed on the Large Hadron Collider (LHC) comes from the contribution of the two lightest CP-even Higgs bosons, whose masses are near 125 GeV. At present, XENON1T, LUX, and PandaX experiments have imposed very strict restrictions on direct collision cross sections of {dark matter}. In this paper, we consider a scenario that the observed Higgs signal is the superposition of two mass-degenerate Higgs in the -invariant NMSSM and scan the seven-dimension parameter space composing of via the Markov chain Monte Carlo (MCMC) method. We find that the DM relic density, as well as the LHC searches for sparticles, especially the DM direct detections, has provided a strong limit on the parameter space. %Please check intended meaning has been retained. The allowed parameter space is featured by a relatively small GeV and about . In addition, the DM is Higgsino-dominated because of . Moreover, the co-annihilation between and must be taken into account to obtain the reasonable DM relic density.

    hep-phSymmetry(2023)·2 citations
  6. 07*

    Parton Decomposition of Nucleon Spin and Momentum: Gluons from Dressed Quarks

    Peter C. Tandy🇺🇸

    The lowest two Mellin moments of hadronic Generalized Parton Distributions are explored within a model that allows investigation of the inter-related quark and gluon contributions. For light quarks their dynamical connection is strong due to quark dressing. Our principal focus is the angular momentum of the nucleon. This work employs and extends dynamical insights obtained from our recent model results for quark and gluon momentum fractions in both pion and nucleon. The employed model is based on the Rainbow-Ladder truncation of the Dyson-Schwinger equations of QCD. The special case of a 1-loop treatment of a single hadronic quark is used to motivate several insights and obtain initial estimates such as the Wilson line correction to the established Landau gauge model ( for both and ), and the "binding gluon" contribution to (). We obtain the proton within 1\% after inclusion of the pion cloud mechanism to produce the sea. The gluon second Mellin moments of the proton reflect similar dynamics; (, ) are (26\% , 24\%) at model scale, and (40\%, 38\%) at GeV. We also find that is shared almost equally between the total orbital and total intrinsic spin contributions.

    hep-phhep-latnucl-exnucl-thPLB(2023)·5 citations
  7. 08*

    Introduction to color in QCD: Initiation to the birdtrack pictorial technique

    Stéphane Peigné🇫🇷

    These lectures are an elementary introduction to the "birdtrack" color pictorial technique, a useful tool in QCD. We review the basic rules, discuss color conservation and infinitesimal color rotations, learn how to project on partonic color states, how to derive their Casimir charges... and at the same time learn a little bit of representation theory.

    hep-phhep-thmath-phmath.MP5 citations
  8. 09*

    and decays in a model with inverse seesaw neutrinos

    N. H. Thao🇻🇳 · D. T. Binh🇻🇳 · T. T. Hong🇻🇳 · L. T. Hue🇻🇳 · D. P. Khoi🇻🇳

    We will show that the 3-4-1 model with heavy right-handed neutrinos can explain the recent experimental data of anomalies of charged leptons and neutrino oscillations through the inverse seesaw mechanism. In addition, the model can predict large lepton flavor violating decay rates and up to the recent experimental sensitivities.

    hep-phPTEP(2023)·3 citations
  9. 10*

    Four-loop splitting functions in QCD -- The quark-quark case

    G. Falcioni🇬🇧 · F. Herzog (U. Edinburgh)🇬🇧 · S. Moch (U. Hamburg)🇩🇪 · A. Vogt (Liverpool U.)🇬🇧

    We have computed the even- moments of the pure-singlet quark splitting function at the fourth order of perturbative QCD via the anomalous dimensions of off-shell flavour-singlet operator matrix elements. Our results, derived analytically for a general gauge group, agree with all results obtained for this function so far, in particular with the lowest six even moments obtained via physical cross sections. Using these results and all available endpoint constraints, we construct approximations for at four loops that should be sufficient for most collider-physics applications. Together with the known results for the non-singlet splitting function at this order, this effectively completes the quark-quark contribution for the evolution of parton distribution at NLO accuracy. Our new results thus provide a major step towards fully consistent NLO calculations at the LHC and the reduction of the residual uncertainty in the parton evolution to the percent level.

    hep-phPLB(2023)·88 citations
  10. 11*

    Semileptonic decays of spin-entangled baryon-antibaryon pairs

    Varvara Batozskaya (1 and 2)🇨🇳 · Andrzej Kupsc (3 and 2)🇸🇪 · Nora Salone (2)🇵🇱 · Jakub Wiechnik (2 and 4) ((1) IHEP Beijing, (2) NCBJ Warsaw, (3) Uppsala University, (4) Warsaw University)🇵🇱

    A modular representation for the semileptonic decays of baryons originating from spin polarized and correlated baryon-antibaryon pairs is derived. The complete spin information of the decaying baryon is propagated to the daughter baryon via a real-valued matrix. It allows to obtain joint differential distributions in sequential processes involving the semileptonic decay in a straightforward way. The formalism is suitable for extraction of the semileptonic formfactors in experiments where strange-baryon-antibaryon pairs are produced in electron-positron annihilation or in charmonia decays. We give examples such as the complete angular distributions in the process, where and . The formalism can also be used to describe the distributions in semileptonic decays of charm and bottom baryons. Using the same principles, the modules to describe electromagnetic and neutral current weak baryon decay processes involving a charged lepton-antilepton pair can be obtained. As an example, we provide the decay matrix for the Dalitz transition between two spin-1/2 baryons.

    hep-phPRD(2023)·20 citations
  11. 12*

    Impact of vorticity and viscosity on the hydrodynamic evolution of hot QCD medium

    Bhagyarathi Sahoo🇮🇳 · Captain R. Singh🇮🇳 · Dushmanta Sahu🇮🇳 · Raghunath Sahoo🇮🇳 · Jan-e Alam🇮🇳

    The strongly interacting transient state of quark-gluon plasma (QGP) medium created in ultra-relativistic collisions survives for a duration of a few fm/c. The spacetime evolution of QGP crucially depends on the equation of state (EoS), vorticity, viscosity, and external magnetic field. In the present study, we obtain the lifetime of a vortical QGP fluid within the ambit of relativistic second-order viscous hydrodynamics. We observe that the coupling of vorticity and viscosity significantly increases the lifetime of vortical QGP. The inclusion of a static magnetic field, vorticity, and viscosity makes the evolution slower. However, the static magnetic field slightly decreases the QGP lifetime by accelerating the evolution process for a non-rotating medium. We also report the rate of change of vorticity in the QGP, which will be helpful in studying the behavior of the medium in detail.

    hep-phhep-exnucl-exnucl-thEPJC(2023)·23 citations
  12. 13*

    Radiative production and decays of the exotic and its siblings

    Vanamali Shastry🇵🇱 · Francesco Giacosa🇵🇱

    We study the production of the light hybrid isoscalars and the yet undiscovered as intermediate states in the radiative decays of the charmonium () to two conventional mesons using a flavor symmetric Lagrangian. For this purpose, we use the process as the reference. We find that some of the decay channels have branching ratios similar to or larger than that of the channel and are sensitive to the mixing between the hybrid isoscalars. We propose that relatively stable channel be explored for the presence of the light hybrid isoscalar . We also exploit the strong decay channels containing at least one vector meson to study the radiative decays of the whole hybrid nonet . We find that the hybrids cannot radiatively decay into the pseudoscalars. Furthermore, the vector decay channels () of the hybrid isoscalars are sensitive to the strangeness content of the hybrids. We also provide estimates for the branching fractions for the radiative production and partial widths for the radiative decays of the hybrids.

    hep-phhep-exNPA(2023)·20 citations
  13. 14*

    Estimated of violation in meson decays into and mesons

    Behnam Mohammadi🇮🇷 · Elnaz Amirkhanlou🇮🇷

    The decay is favorable mode for studying violation in the interference between mixing and decay for and mesons. The latest analysis of the parameters has been performed by the LHCb collaboration values of , , , , and . We have been estimated the parameters and of the decay as and . In the following, we have obtained the values of and and direct violation of . Also, we have calculated the branching ratio of decay. The values obtained in this work are comparable with the corresponding experimental values.

    hep-phEPJC(2023)·0 citations
  14. 15*

    Exclusive meets inclusive at small Bjorken-: how to relate exclusive measurements to PDFs based on evolution equations

    Hervé Dutrieux🇫🇷 · Michael Winn🇫🇷 · Valerio Bertone🇫🇷

    Exclusive heavy-vector-meson photoproduction is a prominent signal in collider experiments with hadron beams. At the highest photon-hadron collision energies, this process is considered as a candidate to constrain gluon parton distribution functions (PDFs) at small longitudinal momentum fractions. However, in the framework of collinear factorisation, exclusive particle production is described in terms of generalised parton distributions (GPDs). In this contribution, we investigate at the leading order in the connection between GPDs and PDFs. Our main result is a proposal to quantify the systematic uncertainty inherent to this connection. We put our approach into context with respect to the Shuavev transform. Our uncertainty estimate can be straightforwardly adapted to higher fixed orders and small- resummations. The question of extrapolating GPDs to vanishing skewness is paramount for the programme of the Electron Ion Collider (EIC), notably for the extraction of the radial distributions of partons.

    hep-phPRD(2023)·13 citations
  15. 16*

    Can LIGO Detect Non-Annihilating Dark Matter?

    Sulagna Bhattacharya🇮🇳 · Basudeb Dasgupta🇮🇳 · Ranjan Laha🇮🇳 · Anupam Ray🇺🇸

    Dark matter from the galactic halo can accumulate in neutron stars and transmute them into sub-2.5 black holes if the dark matter particles are heavy, stable, and have interactions with nucleons. We show that non-detection of gravitational waves from mergers of such low-mass black holes can constrain the interactions of non-annihilating dark matter particles with nucleons. We find benchmark constraints with LIGO O3 data, viz., cm for bosonic DM with PeV (or GeV, if they can Bose-condense) and cm for fermionic DM with PeV. These bounds depend on the priors on DM parameters and on the currently uncertain binary neutron star merger rate density. However, with increased exposure by the end of this decade, LIGO will probe cross-sections that are many orders of magnitude below the neutrino floor and completely test the dark matter solution to missing pulsars in the Galactic center, demonstrating a windfall science-case for gravitational wave detectors as probes of particle dark matter.

    hep-phastro-ph.COastro-ph.HEPRL(2023)·77 citations
  16. 17*

    Triple-Pomeron Diffraction Peak as a Signature of UHE Proton-Initiated Spectra of Gammas and Neutrinos in Astrophysics

    O. I. Piskounova🇷🇺

    Production of ultra-high-energy (UHE) particles in astrophysics should not be different from the hadron production at the contemporary proton colliders. LHC experiments are providing us with the proton spectra at very high energy (VHE) that are measured in the center-of-mass system (c.m.s.). The proton spectrum in c.m.s. has two special features that are important at HE hadron collisions: the growing central-rapidity part with hadron-antihadron pair production and the valuable diffractive peak in the region of the leading proton due to the triple-pomeron term. The QCD phenomenological studies of previous years gave us the Quark-Gluon String Model for the calculations of baryon and meson production spectra in a full kinematical range of rapidities. The collider proton production spectrum was recalculated to the laboratory system of coordinates, which is natural for astrophysical observations. The specifics of collider distributions of protons are reflected in astrophysical spectra as the knee of cosmic proton spectrum and as the spectrum bulge at the UHE area in cosmic spectra of protons, neutrinos, and gamma-photons. They help us to conclude that the energy distribution of baryon production plays an important role in the production of UHE cosmic particles. The remarkable result of this approach is the estimation of maximal energy (Emax) of initial protons (and antiprotons) from the energy of knee in the proton spectrum that give us GeV.

    hep-ph0 citations
  17. 18*

    Using the Sun and the Moon as Source masses and the Earth's Rotation as a Modulation to Search for Exotic Spin-Dependent Interactions at Astronomical Distances

    L. Y. Wu🇨🇳 · K. Y. Zhang🇨🇳 · M. Peng🇨🇳 · J. Gong🇨🇳 · H. Yan🇨🇳

    Exotic spin-dependent interactions mediated by new light particles led to solutions to several important questions in modern physics. Such interactions involving a scalar coupling at one vertex and a pseudo-scalar coupling at the polarized neutron vertex can be induced by the exchange of spin-0 bosons, or a vector/axial-vector coupling / at one vertex and an axial-vector coupling at the polarized neutron vertex can be induced by the exchange of spin-1 bosons. If such new interactions exist, the Sun and the Moon can induce sidereal variations of effective fields along the direction perpendicular to the Earth's rotation axis. We derived new experimental upper limits on such exotic spin-dependent interactions at astronomical interaction ranges by analyzing existing data from laboratory measurements on the Lorentz and CPT violation. We set the most stringent experimental limits on ranging from m to m. Previously, the best limit on at this range is from astrophysics. The result is the first time laboratory limits surpass the astrophysical ones on the scalar-pseudoscalar type interaction, to our best knowledge. We report new constraints on vector-axial-vector and axial-axial-vector type interaction at the range of astronomical scales. The new limits on vector-axial-vector are improved by as much as 12 orders of magnitude. We also apply the analysis to the Hari-Dass interactions and obtain corresponding new constraints on the interactions. We discuss the possibilities of using the beam method to further search the interaction involving other particles, such as electrons, muons, etc., based on the same idea.

    hep-phastro-ph.EPPRL(2023)·19 citations
  18. 19*

    Production of Strange and Charm Hadrons in Pb+Pb Collisions at 5.02 TeV

    Wen-bin Chang🇨🇳 · Rui-qin Wang🇨🇳 · Jun Song🇨🇳 · Feng-lan Shao🇨🇳 · Qun Wang🇨🇳 · Zuo-tang Liang🇨🇳

    Using a quark combination model with the equal-velocity combination approximation, we study the production of hadrons with strangeness and charm flavor quantum numbers in Pb+Pb collisions at 5.02 TeV. We present analytical expressions and numerical results for these hadrons' transverse momentum spectra and yield ratios. Our numerical results agree well with the experimental data available. The features of strange and charm hadron production in the quark--gluon plasma at the early stage of heavy ion collisions are also discussed.

    nucl-thhep-phSymmetry(2023)·3 citations
  19. 20*

    The effect of weak magnetic photon emission from quark-gluon plasma

    Jing-An Sun🇨🇳 · Li Yan🇨🇳

    We propose a novel effect that accounts for the photon emission from a quark-gluon plasma in the presence of a weak external magnetic field. Although the weak magnetic photon emission from quark-gluon plasma only leads to a small correction to the photon production rate, the induced photon spectrum can be highly azimuthally anisotropic, as a consequence of the coupled effect of the magnetic field and the longitudinal dynamics in the background medium. With respect to a realistic medium evolution containing a tilted fireball configuration, the direct photon elliptic flow from experiments is reproduced. In comparison to the experimental data of direct photon elliptic flow, in heavy-ion collisions the magnitude of the magnetic field before 1 fm/c can be extracted. For the top energy of RHIC collisions, right after the pre-equilibrium evolution, is found no larger than a few percent of the pion mass square.

    nucl-thhep-phnucl-exPLB(2024)·16 citations
  20. 21*

    Tension between implications from PREX-2 data and gravitational tidal response on dense matter equation of state

    Vivek Baruah Thapa🇮🇳 · Monika Sinha🇮🇳

    Recently an improved value of neutron skin thickness of was reported in Lead Radius EXperiment-2 (PREX-2) to be fm which corresponds to high estimations of nuclear symmetry energy () and its slope (). The updated values of and commensurating to the neutron star observable estimations lie exterior to the astrophysical observed range. The higher values of at deduced from recent PREX-2 data correlates to matter being easily deformable (yielding higher radius values) around intermediate matter densities leading to higher values of creating a tension between the terrestrial and astrophysical observations. In this study, we exploit this tension to constrain the -scalar meson coupling parameter space.

    astro-ph.HEhep-phEPJ Web Conf.(2023)·2 citations
  21. 22*

    Gravitational Wave Backgrounds from Colliding ECOs

    Hannah Banks🇬🇧 · Dorota M. Grabowska🇨🇭 · Matthew McCullough🇨🇭

    Long baseline atom interferometers offer an exciting opportunity to explore mid-frequency gravitational waves. In this work we survey the landscape of possible contributions to the total 'gravitational wave background' in this frequency band and advocate for targeting this observable. Such an approach is complimentary to searches for resolved mergers from individual sources and may have much to reveal about the Universe. We find that the inspiral phases of stellar-mass compact binaries cumulatively produce a signal well within reach of the proposed AION-km and AEDGE experiments. Hypothetical populations of dark sector exotic compact objects, harbouring just a tiny fraction of the dark energy density, could also generate signatures unique to mid- and low-frequency gravitational wave detectors, providing a novel means to probe complexity in the dark sector.

    gr-qcastro-ph.HEhep-exhep-phPRD(2023)·19 citations
  22. 23*

    Search for scalar induced gravitational waves in the International Pulsar Timing Array Data Release 2 and NANOgrav 12.5 years datasets

    Virgile Dandoy🇩🇪 · Valerie Domcke🇨🇭 · Fabrizio Rompineve🇨🇭

    We perform a Bayesian search in the latest Pulsar Timing Array (PTA) datasets for a stochastic gravitational wave (GW) background sourced by curvature perturbations at scales . These re-enter the Hubble horizon at temperatures around and below the QCD crossover phase transition in the early Universe. We include a stochastic background of astrophysical origin in our search and properly account for constraints on the curvature power spectrum from the overproduction of primordial black holes (PBHs). We find that the International PTA Data Release 2 significantly favors the astrophysical model for its reported common-spectrum process, over the curvature-induced background. On the other hand, the two interpretations fit the NANOgrav 12.5 years dataset equally well. We then set new upper limits on the amplitude of the curvature power spectrum at small scales. These are independent from, and competitive with, indirect astrophysical bounds from the abundance of PBH dark matter. Upcoming PTA data releases will provide the strongest probe of the curvature power spectrum around the QCD epoch.

    astro-ph.COgr-qchep-phSciPost Phys.Core(2023)·90 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.