PaperPanorama

HEP Phenomenology·hep-ph

Mon·Jun 6, 2022

23 papers17 primary·6 cross-listed·reconstructed*

  1. 01*

    Information field based global Bayesian inference of the jet transport coefficient

    Man Xie🇨🇳 · Weiyao Ke🇺🇸 · Hanzhong Zhang🇨🇳 · Xin-Nian Wang🇺🇸

    Bayesian statistical inference is a powerful tool for model-data comparisons and extractions of physical parameters that are often unknown functions of system variables. Existing Bayesian analyses often rely on explicit parametrizations of the unknown function. It can introduce long-range correlations that impose fictitious constraints on physical parameters in regions of the variable space that are not probed by the experimental data. We develop an information field (IF) approach to modeling the prior distribution of the unknown function that is free of long-range correlations. We apply the IF approach to the first global Bayesian inference of the jet transport coefficient as a function of temperature () from all existing experimental data on single-inclusive hadron, di-hadron and -hadron spectra in heavy-ion collisions at RHIC and LHC energies. The extracted exhibits a strong -dependence as a result of the progressive constraining power when data from more central collisions and at higher colliding energies are incrementally included. The IF method guarantees that the extracted -dependence is not biased by a specific functional form.

    hep-phnucl-thPRC(2023)·66 citations
  2. 02*

    Revisiting evolution equations for generalised parton distributions

    Valerio Bertone🇫🇷 · Hervé Dutrieux🇫🇷 · Cédric Mezrag🇫🇷 · José M. Morgado🇪🇸 · Hervé Moutarde🇫🇷

    We revisit the evolution of generalised parton distributions (GPDs) in momentum space. We formulate the evolution kernels at one-loop in perturbative QCD (pQCD) in a form suitable for numerical implementation and that allows for an accurate study of their properties. This leads to the first open-source implementation of GPD evolution equations able to cover the entire kinematic region and allowing for heavy-quark-threshold crossings. The numerical implementation of the GPD evolution equations is publicly accessible through the APFEL++ evolution library and is available within the PARTONS framework. Our formulation makes use of the operator definition of GPDs in light-cone gauge renormalised in the scheme. For the sake of clarity, we recompute the evolution kernels at one-loop in pQCD, confirming previous calculations. We obtain general conditions on the evolution kernels deriving from the GPD sum rules and show that our formulation obeys these conditions. We analytically show that our calculation reproduces the DGLAP and the ERBL equations in the appropriate limits and that it guarantees the continuity of GPDs. We numerically check that the evolved GPDs fulfil DGLAP and ERBL limits, continuity, and polynomiality. We benchmark our numerical implementation against analytical evolution in conformal space. Finally, we perform a numerical comparison to an existing implementation of GPD evolution finding a general good agreement on the kinematic region accessible to the latter. This work provides a pedagogical description of GPD evolution equations which benefits from a renewed interest as future colliders, such as the electron-ion colliders in the US and in China, are being designed. It also paves the way to the extension of GPD evolution codes to higher accuracies in pQCD desirable for precision phenomenology at these facilities.

    hep-phEPJC(2022)·33 citations
  3. 03*

    Roles of , , and in the decay

    Guan-Ying Wang🇨🇳 · Neng-Chang Wei🇨🇳 · Hui-Min Yang🇨🇳 · En Wang🇨🇳 · Li-Sheng Geng🇨🇳 · Ju-Jun Xie🇨🇳

    Recently, the Belle Collaboration has measured the decay and reported the and invariant mass distributions, which show the clear signals of the resonances and , respectively. Based on our previous works [Eur. Phys. J. C 76 (2016) 496 and Phys. Rev. D 95 (2017) 074024], we re-analyze this process by considering the -wave and final state interactions within the chiral unitary approach, which dynamically generate the and , respectively. Our results are in good agreement with the Belle measurements, which supports the molecular nature of the and . In addition, the invariant mass distributions are also computed and a cusp structure of is cleary shown around the mass threshold.

    hep-phPRD(2022)·30 citations
  4. 04*

    Bounds on the mass and mixing of and bosons decaying into different pairings of , , or Higgs bosons using CMS data at the LHC

    P. Osland🇳🇴 · A. A. Pankov🇧🇾 · I. A. Serenkova🇧🇾

    The full CMS Run 2 datasets with time-integrated luminosity of 137 fb in the diboson channels are used to probe benchmark models with extended gauge sectors such as , left-right symmetric (LR) and the sequential standard model (extended gauge model, EGM), that predict the existence of neutral - and charged -bosons decaying to a pair of bosons , , and in the semileptonic final state. These benchmark models are used to interpret the results. Exclusion limits at the 95% C.L. on the and resonance production cross section times branching ratio to electroweak gauge boson pairs in the resonance mass range between 1.0 and 4.5 TeV are here converted to constraints on - and - mixing parameters and masses. We present exclusion regions on the parameter spaces of the and and show that the obtained exclusion regions are significantly extended compared to those derived from the previous analysis performed with Tevatron data as well as with the CMS data collected at 7 and 8 TeV in Run 1. The reported limits are the most restrictive to date.

    hep-ph7 citations
  5. 05*

    Application of Generalized Quaternion in Physics

    Liaofu Luo🇨🇳 · Jun Lv🇨🇳

    The applications of quaternion in physics are discussed with an emphasis on elementary particle symmetry and interaction. Three colours of the quark and the quantum chromodynamics (QCD) can be introduced directly from the invariance of basic equations under the quaternion phase transformation (quaternion gauge invariance). The generalized quaternions obey the SU(3) symmetry. QCD is essentially the quantum quaternion dynamics. The further generalization of SU(3) quaternion to G2 octonion is worked out. We demonstrate that the G2 octonion contains seven tri-generator sets of SU(2) symmetry and three of them form SU(3) subgroup. A model of the elementary particle classification and interaction based on octonion gauge theory is proposed. The model unifies the colour and flavour of all particles. It provides a framework for the unified description of four kinds of elementary particles (quarks, leptons, gauge fields and Higgs bosons) and their interactions.

    hep-ph0 citations
  6. 06*

    Axion dark matter with thermal friction

    Kiwoon Choi🇰🇷 · Sang Hui Im🇰🇷 · Hee Jung Kim🇰🇷 · Hyeonseok Seong🇰🇷

    Cosmological evolution of axion field in the early universe might be significantly affected by a thermal friction induced by the axion coupling to thermalized hidden sector. We examine the effects of such a thermal friction on axion dark matter density and its perturbation when the thermal friction dominates over the Hubble friction until when the axion field begins to oscillate around the potential minimum. We show that in the presence of sizable thermal friction there can be an exponential decay phase of the axion field before the oscillation phase, during which the axion energy density is efficiently dissipated into hidden thermal bath. Consequently, the previously excluded parameter region due to overclosing relic axion density becomes cosmologically viable with thermal friction. In particular, a QCD axion much lighter than eV is viable without tuning the initial misalignment angle. We also find that thermal friction can affect the density perturbation of axion dark matter in various ways. For instance, it can alleviate the large-scale isocurvature bound on axion dark matter in the pre-inflationary PQ breaking scenario, which would make the pre-inflationary axion dark matter compatible with high scale inflation over a wide range of model parameters. In the post-inflationary PQ breaking scenario, thermal friction can also significantly change the scaling behavior of axionic strings, and therefore the typical size of the resultant axion miniclusters.

    hep-phastro-ph.COJHEP(2023)·16 citations
  7. 07*

    Towards a theory of hadron resonances

    Maxim Mai🇺🇸 · Ulf-G. Meißner🇩🇪 · Carsten Urbach🇩🇪

    In this review, we present the current state of the art of our understanding of the spectrum of excited strongly interacting particles and discuss methods that allow for a systematic and model-independent calculation of the hadron spectrum. These are lattice QCD and effective field theories. Synergies between both approaches can be exploited allowing for deeper understanding of the hadron spectrum. Results based on effective field theories and hadron-hadron scattering in lattice QCD or combinations thereof are presented and discussed. We also show that the often used Breit-Wigner parameterization is at odds with chiral symmetry and should not be used in case of strongly coupled channels.

    hep-phhep-exhep-latnucl-ex+1Phys.Rept.(2023)·156 citations
  8. 08*

    Electroweak renormalization based on gauge-invariant vacuum expectation values of non-linear Higgs representations: 2. extended Higgs sectors

    Stefan Dittmaier🇩🇪 · Heidi Rzehak🇩🇪

    A recently proposed scheme for a gauge-invariant treatment of tadpole corrections in spontaneously broken gauge theories - called Gauge-Invariant Vacuum expectation value Scheme (GIVS) - is applied to a singlet Higgs extension of the Standard Model and to the Two-Higgs Doublet Model. In contrast to previously used tadpole schemes, the GIVS unifies the gauge-invariance property with perturbative stability. For the Standard Model this was demonstrated for the conversion between on-shell and MSbar renormalized masses, where the GIVS leads to very moderate, gauge-independent electroweak corrections. In models with extended scalar sectors, issues with tadpole renormalization exist if Higgs mixing angles are renormalized with MSbar conditions, which is the major subject of this article. In detail, we first formulate non-linear representations of the extended scalar sectors, which is an interesting subject in its own right. Then we formulate the GIVS which employs these non-linear representations in the calculation of the tadpole renormalization constants, while actual higher-order calculations in the GIVS proceed in linear representations as usual. Finally, for the considered models we discuss the next-to-leading-order (electroweak and QCD) corrections to the decay processes fermions of the CP-even neutral Higgs bosons h and H using MSbar-renormalized Higgs mixing angles with the GIVS and previously used tadpole treatments.

    hep-phJHEP(2022)·19 citations
  9. 09*

    Electron Mass Singularities in Semileptonic Kaon Decays

    Chien-Yeah Seng🇩🇪 · William J. Marciano🇺🇸 · Ulf-G. Meißner🇩🇪

    We show that recent improvements in the long-distance quantum electrodynamics (QED) corrections to the radiative inclusive decay rate using the Sirlin representation are free from infrared divergences and collinear electron mass singularities in the limit , as predicted by the Kinoshita-Lee-Nauenberg theorem. We also verify that in massless QED with the simultaneous dimensional regularization of QED photon infrared divergences and electron mass singularities leads to the same result for the inclusive rate in the limit of four space-time dimensions. The equivalence of the two approaches results in part from an interesting interplay between a small chirality-breaking effect in the massless electron limit and the generalization of space-time algebra and phase space integrals to dimensions. Our finding supports the small theoretical uncertainty claimed for radiative inclusive rates and reaffirms its utility in precision unitarity tests of the quark mixing matrix.

    hep-phhep-exhep-latnucl-ex+1PRD(2022)·3 citations
  10. 10*

    Bottomed baryon decays with invisible Majorana fermions

    Geng Li🇨🇳 · Chia-Wei Liu🇨🇳 · Chao-Qiang Geng🇨🇳

    We study the invisible Majorana fermions of in bottomed baryon decays with flavor-changing neutral currents (FCNCs) based on the model-independent effective Lagrangian between the quarks and invisible particles. From the bounds of the coupling constants extracted from the experiments, we examine the decay branching ratios of , , , , , and , which can be as large as , and for GeV, respectively. Some of these decays are accessible to the future experimental searches, such as Belle II.

    hep-phPRD(2022)·4 citations
  11. 11*

    The geometric SMEFT

    Michael Trott🇩🇰

    Effective field theories, like the Standard Model Effective Field Theory (SMEFT), are defined by a chosen field content and a set of symmetries, up to a cut off scale . Usually, in order to perform calculations, gauge independent field re-definitions consistent with the symmetries of the theory are then used to redefine the fields. This procedure results in a fixed (non-redundant) operator basis, that is not itself field re-definition invariant. Recently, an alternative approach of identifying and calculating with field space geometry has been developed. Field redefinition invariants, characterising field space geometry, appear in observables in amplitude perturbations, and have an expansion in terms of local operators. In the case of the SMEFT, calculating via the geometric approach is known as the geoSMEFT. This approach makes it much easier to calculate at high orders in in the SMEFT, and can directly result in a complete characterisation of an amplitude perturbation in the expansion. Using the geoSMEFT, several consistent and complete results are now known. We define the geoSMEFT and demonstrate its use in some examples.

    hep-ph2 citations
  12. 12*

    Tree-level soft emission of a quark pair in association with a gluon

    Vittorio Del Duca🇨🇭 · Claude Duhr🇩🇪 · Rayan Haindl🇨🇭 · Zhengwen Liu🇩🇪

    We compute the tree-level current for the emission of a soft quark-antiquark pair in association with a gluon. This soft current is the last missing ingredient to understand the infrared singularities that can arise in next-to-next-to-next-to-leading-order (NLO) computations in QCD. Its square allows us to understand for the first time the colour correlations induced by the soft emission of a quark pair and a gluon. We find that there are three types of correlations: Besides dipole-type correlations that have already appeared in soft limits of tree-level amplitudes, we uncover for the first time also a three-parton correlation involving a totally symmetric structure constant. We also study the behaviour of collinear splitting amplitudes in the triple-soft limit, and we derive the corresponding factorisation formula.

    hep-phJHEP(2023)·31 citations
  13. 13*

    Identifying quenched jets in heavy ion collisions with machine learning

    Lihan Liu · Julia Velkovska · Marta Verweij

    Measurements of jet substructure in ultra-relativistic heavy ion collisions suggest that the jet showering process is modified by the interaction with quark gluon plasma. Modifications of the hard substructure of jets can be explored with modern data-driven techniques. In this study, a machine learning approach to the identification of quenched jets is designed. Jet showering processes are simulated with a jet quenching model Jewel and a non-quenching model Pythia 8. Sequential substructure variables are extracted from the jet clustering history following an angular-ordered sequence and are used in the training of a neural network built on top of a long short-term memory network. We show that this approach successfully identifies the quenching effect in the presence of the large uncorrelated background of soft particles created in heavy ion collisions.

    hep-phhep-exphysics.comp-phJHEP(2023)·20 citations
  14. 14*

    Axion effects in the stability of hybrid stars

    Bruno S. Lopes🇧🇷 · Ricardo L. S. Farias🇧🇷 · Veronica Dexheimer🇺🇸 · Aritra Bandyopadhyay🇨🇳 · Rudnei O. Ramos🇧🇷

    We investigate the effects of including strong charge-parity (CP) violating effects through axion fields in the microscopic equation of state of massive hybrid neutron stars. We assume that their cores contain deconfined quark matter and include the effects of axions via an effective 't Hooft determinant interaction. The hadronic crusts are described using different approaches in order to make our results more general. We find that the presence of axions stabilizes massive hybrid neutron stars against gravitational collapse by weakening the deconfinement phase transition and bringing it to lower densities. This enables to reproduce hybrid neutron stars in agreement with modern astrophysical constraints.

    hep-phastro-ph.HEhep-thnucl-thPRD(2022)·24 citations
  15. 15*

    On interplay between flavour anomalies and neutrino properties

    Felipe F. Freitas🇵🇹 · João Gonçalves🇵🇹 · António P. Morais🇵🇹 · Roman Pasechnik🇸🇪 · Werner Porod🇩🇪

    A minimal extension of the Standard Model (SM) featuring two scalar leptoquarks, an SU(2) doublet with hypercharge 1/6 and a singlet with hypercharge 1/3, is proposed as an economical benchmark model for studies of an interplay between flavour physics and properties of the neutrino sector. The presence of such type of leptoquarks radiatively generates neutrino masses and offers a simultaneous explanation for the current B-physics anomalies involving decays. The model can also accommodate both the muon magnetic moment and the recently reported mass anomalies, while complying with the most stringent lepton flavour violating observables.

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

    Following the muon track of hierarchical sectors at LHCb

    Xabier Cid Vidal🇪🇸 · Titus Mombächer🇪🇸 · Maria Ramos🇪🇸 · Emilio Xosé Rodríguez Fernández🇪🇸

    This paper reports a study of the experimental signatures of hierarchical sectors beyond the Standard Model characterized by a flavor-violating heavy vector and a set of light pseudo-Goldstone bosons , spanning a large range of lifetimes. The non-minimal scalar spectrum triggers novel decays into multiple leptons that would have escaped the reach of current searches. Novel displaced vertex analyses at LHCb are therefore discussed to probe the hierarchical new physics, extending the scope of the tracking system of the detector. Additionally, the reach of the proposed CODEX-b experiment is studied as well. By exploiting the use of tracks only reconstructed in subsystems of the detector at the high-level LHCb trigger, and could be reached in the muon channel across seven orders of magnitude in the lifetime of the Goldstone bosons. Correspondingly, heavy-light particle couplings of order could be tested, potentially ruling out composite Higgs scenarios where the heavy and light sectors couple strongly.

    hep-phhep-exJHEP(2022)·3 citations
  17. 17*

    The Charged Higgs from the Bottom-Up: Probing Flavor at the LHC

    Nishita Desai🇮🇳 · Alberto Mariotti🇧🇪 · Mustafa Tabet🇩🇪 · Robert Ziegler🇩🇪

    We systematically study model-independent constraints on the three generic charged Higgs couplings to -quarks and up-type quarks. While existing LHC searches have focussed on the coupling, we emphasize that the LHC plays a crucial role in probing also and couplings, since constraints from flavor physics are weak. In particular we propose various new searches that can significantly extend the present reach on the parameter space by: i) looking for light charged Higgses that decay into -quarks, ii) probing charged Higgs couplings to light and top quarks using multi--jet signatures, iii) looking for single -quarks in low-mass dijet searches, iv) searching for charge asymmetries induced by charged Higgs production via couplings.

    hep-phhep-exJHEP(2022)·8 citations
  18. 18*

    Chiral anomaly induces superconducting baryon crystal

    Geraint W. Evans🇬🇧 · Andreas Schmitt🇬🇧

    It was previously shown within chiral perturbation theory that the ground state of QCD in a sufficiently large magnetic field and at nonvanishing, but not too large, baryon chemical potential is a so-called chiral soliton lattice. The crucial ingredient of this observation was the chiral anomaly in the form of a Wess-Zumino-Witten term, which couples the baryon chemical potential to the magnetic field and the gradient of the neutral pion field. It was also shown that the chiral soliton lattice becomes unstable towards charged pion condensation at larger magnetic fields. We point out that this instability bears a striking resemblance to the second critical magnetic field of a type-II superconductor, however with the superconducting phase appearing upon increasing the magnetic field. The resulting phase has a periodically varying charged pion condensate that coexists with a neutral pion supercurrent. We construct this phase analytically in the chiral limit and show that it is energetically preferred. Just like an ordinary type-II superconductor, it exhibits a hexagonal array of magnetic flux tubes, and, due to the chiral anomaly, a spatially oscillating baryon number of the same crystalline structure.

    hep-thhep-phnucl-thJHEP(2022)·39 citations
  19. 19*

    New insights into the oscillation of the nucleon electromagnetic form factors

    Qin-He Yang🇨🇳 · Ling-Yun Dai🇨🇳 · Di Guo🇨🇳 · Johann Haidenbauer🇩🇪 · Xian-Wei Kang🇨🇳 · Ulf-G. Meißner🇩🇪

    The electromagnetic form factors of the proton and the neutron in the timelike region are investigated. Electron-positron annihilation into antinucleon-nucleon () pairs is treated in distorted wave Born approximation, including the final-state interaction in the system. The latter is obtained by a Lippmann-Schwinger equation for potentials derived within SU(3) chiral effective field theory. By fitting to the phase shifts and (differential) cross section data, a high quality description is achieved. With these amplitudes, the oscillations of the electromagnetic form factors of the proton and the neutron are studied. It is found that each of them can be described by two fractional oscillators. One is characterized as \lq overdamped' and dominates near the threshold, while the other is \lq underdamped' and plays an important role in the high-energy region. These two oscillators are essential to understand the distributions of polarized electric charges induced by hard photons for the nucleons.

    nucl-thhep-phSci.Bull.(2023)·28 citations
  20. 20*

    Single top and rare top quark production (including FCNC searches) at ATLAS and CMS

    Samuel May (for the ATLAS and CMS Collaborations)🇺🇸

    Measurements of single top and rare top quark production may be sensitive to theories of physics beyond the standard model (SM), including those in which the energy scale of new physics is beyond the energies directly accessible at the Large Hadron Collider. Such models may be observable through signatures like forbidden SM interactions or deviations of the top quark's couplings from the SM predictions. An overview of recent searches from the ATLAS and CMS Collaborations is presented, with a focus on flavor-changing neutral currents.

    hep-exhep-ph0 citations
  21. 21*

    Magnetar Hard X-Ray Emission from Axion-like Particle Conversion

    Jean-François Fortin🇨🇦 · Marianne Gratton🇨🇦

    We explore the possibility that axion-like-particles (ALPs), which would be produced in the core of magnetars and would then convert in the magnetosphere into photons, can explain magnetar hard X-ray spectra. We remark that this scenario would also provide answers to some questions related to magnetar heating. Indeed, considering that magnetars have: 1) hard X-ray spectra that are difficult to explain with known mechanisms; 2) large photon luminosities that force high core temperatures; 3) high core temperatures that imply large neutrino emissivities; 4) and large neutrino emissivities that lead to small magnetar lifetimes in contradiction to observations -- explaining the hard X-ray spectra with ALPs could decrease the core temperatures and thus the neutrino emissivities, allowing for longer magnetar lifetimes as expected from observations. In this work, we initiate the study of this scenario for three magnetars with extreme luminosities, and conclude that the general idea is likely worth investigating in more detail.

    astro-ph.HEhep-phJCAP(2022)·2 citations
  22. 22*

    A Note on the Analytic Structure of Celestial Amplitudes

    Jiayin Gu🇨🇳 · Ying-Ying Li🇺🇸 · Lian-Tao Wang🇺🇸

    Celestial amplitudes, obtained by applying Mellin transform and analytic continuation on "ordinary" amplitudes, have interesting properties which may provide useful insights on the underlying theory. Their analytic structures are thus of great interest and need to be better understood. In this paper, we critically examine the analytic structure of celestial amplitudes in a massless low-energy effective field theory. We find that, fixed-order loop contributions, which generate multipoles on the negative -plane, in general do not provide an accurate description of the analytic structure of celestial amplitudes. By resumming over the leading logarithmic contributions using renormalization group equations (RGEs), we observe much richer analytic structures, which generally contain branch cuts. It is also possible to generate multipoles or shifted single poles if the RGEs satisfy certain relations. Including sub-leading logarithmic contributions is expected to introduce additional corrections to the picture. However, without a new approach, it is difficult to make a general statement since the analytic form of the Mellin transform is challenging to obtain.

    hep-thhep-phJHEP(2022)·1 citation
  23. 23*

    Neutrino Rocket Jet Model: An Explanation of High-velocity Pulsars and their Spin-down Evolution

    Zheng Li🇨🇳 · Qiu-He Peng🇨🇳 · Miao Kang🇨🇳 · Xiang Liu🇨🇳 · Ming Zhang🇨🇳 · Yong-Feng Huang🇨🇳 · Chih-Kang Chou🇨🇳

    The fact that the spatial velocity of pulsars is generally higher than that of their progenitor stars has bothered astronomers for nearly 50 years. It has been extensively argued that the high pulsar velocity should be acquired during a natal kick process on a timescale of 100ms - 10s in the supernova explosion, in which some asymmetrical dynamical mechanism plays a key role. However, a satisfactory picture generally is still lacking. In this study, it is argued that the neutrino rocket model can well account for the high speed as well as the long-term evolution behaviors of pulsars. The neutrinos are emitted from superfluid vortex neutrons through the neutrino cyclotron radiation mechanism. The unique characters of left-handed neutrinos and right-handed antineutrinos resulting from the nonconservation of parity in weak interactions play a major role in the spatial asymmetry. The continuous acceleration of pulsars can be naturally explained by this model, which yields a maximum velocity surpassing 1000 km s. The alignment between the spinning axis and the direction of motion observed for the Crab pulsar (PSR 0531) and the Vela pulsar (PSR 0833) can be well accounted for. The observed correlation between the spin-down rate and the period of long-period pulsars with s can also be satisfactorily explained.

    astro-ph.HEhep-phApJ(2022)·5 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.