PaperPanorama

HEP Phenomenology·hep-ph

Wed·Sep 19, 2018

22 papers—15 primary·7 cross-listed·reconstructed*

  1. 01*

    Dark Tridents at Off-Axis Liquid Argon Neutrino Detectors

    André de Gouvêa🇺🇸 · Patrick J. Fox🇺🇸 · Roni Harnik🇺🇸 · Kevin J. Kelly🇺🇸 · Yue Zhang🇺🇸

    We present dark tridents, a new channel for exploring dark sectors in short-baseline neutrino experiments. Dark tridents are clean, distinct events where, like neutrino tridents, the scattering of a very weakly coupled particle leads to the production of a lepton--antilepton pair. Dark trident production occurs in models where long-lived dark-sector particles are produced along with the neutrinos in a beam-dump environment and interact with neutrino detectors downstream, producing an on-shell boson which decays into a pair of charged leptons. We focus on a simple model where the dark matter particle interacts with the standard model exclusively through a dark photon, and concentrate on the region of parameter space where the dark photon mass is smaller than twice that of the dark matter particle and hence decays exclusively into standard-model particles. We compute event rates and discuss search strategies for dark tridents from dark matter at the current and upcoming liquid argon detectors aligned with the Booster beam at Fermilab -- MicroBooNE, SBND, and ICARUS -- assuming the dark sector particles are produced off-axis in the higher energy NuMI beam. We find that MicroBooNE has already recorded enough data to be competitive with existing bounds on this dark sector model, and that new regions of parameter space will be probed with future data and experiments.

    hep-phhep-exJHEP(2019)·46 citations
  2. 02*

    Solving integral equations in

    Juerg Gasser (Albert Einstein Center for fundamental Physics, University of Bern)🇨🇭 · Akaki Rusetsky (University of Bonn and BCTP)🇩🇪

    A dispersive analysis of decays has been performed in the past by many authors. The numerical analysis of the pertinent integral equations is hampered by two technical difficulties: i) The angular averages of the amplitudes need to be performed along a complicated path in the complex plane. ii) The averaged amplitudes develop singularities along the path of integration in the dispersive representation of the full amplitudes. It is a delicate affair to handle these singularities properly, and independent checks of the obtained solutions are demanding and time consuming. In the present article, we propose a solution method that avoids these difficulties. It is based on a simple deformation of the path of integration in the dispersive representation (not in the angular average). Numerical solutions are then obtained rather straightforwardly. We expect that the method also works for .

    hep-phEPJC(2018)·35 citations
  3. 03*

    Form Factors and Generalized Parton Distributions of Heavy Quarkonia in Basis Light Front Quantization

    Lekha Adhikari🇺🇸 · Yang Li🇺🇸 · Meijian Li🇺🇸 · James P. Vary🇺🇸

    We calculate the electromagnetic (charge, magnetic and quadrupole) form factors and the associated static moments of heavy quarkonia (charmonia and bottomonia) using the Basis Light Front Quantization (BLFQ) approach. For this work, we adopt light front wavefunctions (LFWFs) generated by a holographic QCD confining potential and a one-gluon exchange interaction with fixed coupling. We compare our BLFQ results with the limiting case of a single BLFQ basis state description of heavy quarkonia and with other available results. These comparisons provide insights into relativistic effects. Using the same LFWFs generated in the BLFQ approach, we also present the generalized parton distributions (GPDs) for selected mesons including those for radially excited mesons such as and . Our GPD results establish the foundation within BLFQ for further investigating hadronic structure such as probing the spin structure of spin-one hadrons in the off-forward limit.

    hep-phnucl-thPRC(2019)·39 citations
  4. 04*

    Dual chiral density waves in nuclear matter

    Hiroaki Abuki🇯🇵 · Yusuke Takeda🇯🇵 · Masayasu Harada🇯🇵

    We study inhomogeneous chiral phases in nuclear matter using a hadronic model with the parity doublet structure. With an extended ansatz for the dual chiral density wave off the chiral limit, we numerically determine the phase structure. A new type of dual chiral density wave where the condensate has nonvanishing space average is confirmed and it comes to occupy a wide range of low density region as the chiral invariant mass parameter is lowered.

    hep-phnucl-thEPJ Web Conf.(2018)·10 citations
  5. 05*

    An extension of the SM based on effective Peccei-Quinn Symmetry

    Daijiro Suematsu🇯🇵

    Peccei-Quinn (PQ) mechanism based on a chiral global U(1) symmetry is considered to be a simple and elegant solution for strong CP problem. Fact that the mechanism could be experimentally examined through the axion search makes it much more interesting and recently it causes a lot of attention again. However, it is also known that the mechanism is annoyed by two serious problems, that is, a domain wall problem and goodness of global symmetry. Any global symmetry is considered not to be exact due to the quantum effect of gravity. In this paper, we consider a solution to these problems, in which quark mass hierarchy and mixing, neutrino mass generation and existence of dark matter are closely related. In our solution, PQ symmetry is assumed to be induced through symmetry breaking at an intermediate scale of a local U(1) symmetry, and a global U(1) symmetry which plays a role of Froggatt-Nielsen symmetry . In the lepton sector, a remnant of the PQ symmetry controls neutrino mass generation and dark matter existence.

    hep-phEPJC(2018)·11 citations
  6. 06*

    High Scale Type-II Seesaw, Dominant Double Beta Decay within Cosmological Bound and Verifiable LFV Decays in SU(5)

    M. K. Parida (SOADU)🇮🇳 · Rajesh Satpathy (SOADU)🇮🇳

    Very recently a novel implementation of type-II seesaw mechanism for neutrino mass has been proposed in SU(5) grand unified theory with a number of desirable new physical phenomena beyond the standard model.Introducing heavy right-haded neutrinos and extra fermion singlets, in this work we show how the type-I seeaw cancellation mechanism works in this SU(5) framework. Besides predicting verifiable LFV decays, we further show that the model predicts dominant double beta decay with normal hierarchy or inverted hierarchy of active light neutrino masses in concordance with cosmological bound. In addition, a novel mechanism for heavy right-handed neutrino mass generation independent of type-II seesaw predicted mass hierarchy, is suggested in this work.

    hep-phAdv.High Energy Phys.(2019)·9 citations
  7. 07*

    CP transformed mixed antisymmetry for neutrinos and its consequences

    Roopam Sinha🇮🇳 · Probir Roy🇮🇳 · Ambar Ghosal🇮🇳

    We propose a complex extension of mixed antisymmetry in the neutrino Majorana mass matrix . This can be implemented in the Lagrangian by a generalized CP transformation (labeled by a mixing parameter ) on the left-chiral flavor neutrino fields. We investigate its implications for leptonic CP violation and neutrino phenomenology in general. Interestingly, the mixing parameter gets correlated with the Dirac CP phase and the atmospheric mixing angle through an analytical relation. In general, for arbitrary , both and are nonmaximal. We discuss the corresponding results for the CP asymmetry parameter in neutrino oscillation experiments. For a nonmaximal , one of the two Majorana phases is different from or , thereby leading to nonvanishing Majorana CP violation with observable consequences for the neutrinoless double beta () decay process. We numerically work out in detail the predictions for that process in relation to various ongoing and forthcoming experiments. We also work out the predictions of our scheme on flavor flux ratios at neutrino telescopes. While exact CP transformed interchange antisymmetry () leads to an exact equality among those ratios, taking a value , a tiny deviation can cause a drastic change in them. Careful measurement of these flux ratios in future will further constrain the parameter .

    hep-phPRD(2019)·19 citations
  8. 08*

    Reflections on the Origin of the EMC Effect

    Anthony W. Thomas🇦🇺

    In the 35 years since the European Muon Collaboration announced the astonishing result that the valence structure of a nucleus was very different from that of a free nucleon, many explanations have been suggested. The first of the two most promising explanations is based upon the different effects of the strong Lorentz scalar and vector mean fields known to exist in a nucleus on the internal structure of the nucleon-like clusters which occupy shell model states. The second links the effect to the modification of the structure of nucleons involved in short-range correlations, which are far off their mass shell. We explore some of the methods which have been proposed to give complementary information on this puzzle, especially the spin-dependent EMC effect and the isovector EMC effect, both proposed by Cloet, Bentz and Thomas. It is shown that the predictions for the spin dependent EMC effect, in particular, differ substantially within the mean-field and short-range correlation approaches. Hence the measurement of the spin dependent EMC effect at Jefferson Lab should give us a deeper understanding of the origin of the EMC effect and, indeed, of the structure of atomic nuclei.

    hep-phnucl-thIJMPE(2019)·21 citations
  9. 09*

    Top production at large p_t at NLO+NLL accuracy

    Matteo Cacciari🇫🇷

    We introduce a new version of the FONLL code, now capable of calculating differential distributions for top quark production with next-to-leading-log resummation of log(p_t/m) terms. Numerical results for LHC and FCC kinematics are presented. In the transverse momentum region presently explored by ATLAS and CMS, no significant difference with respect to available fixed order predictions is predicted by FONLL. The large transverse momentum resummation of FONLL may instead become relevant if top is ever measured at transverse momentum scales of several TeV.

    hep-phPoS(2018)·1 citation
  10. 10*

    A Deeply Bound Dibaryon is Incompatible with Neutron Stars and Supernovae

    Samuel D. McDermott🇺🇸 · Sanjay Reddy🇺🇸 · Srimoyee Sen🇺🇸

    We study the effect of a dibaryon, S, in the mass range 1860 MeV < m_S < 2054 MeV, which is heavy enough not to disturb the stability of nuclei and light enough to possibly be cosmologically metastable. Such a deeply bound state can act as a baryon sink in regions of high baryon density and temperature. We find that the ambient conditions encountered inside a newly born neutron star are likely to sustain a sufficient population of hyperons to ensure that a population of S dibaryons can equilibrate in less than a few seconds. This would be catastrophic for the stability of neutron stars and the observation of neutrino emission from the proto-neutron star of Supernova 1987A over ~ O(10)s. A deeply bound dibaryon is therefore incompatible with the observed supernova explosion, unless the cross section for S production is severely suppressed.

    hep-phastro-ph.HEnucl-thPRD(2019)·18 citations
  11. 11*

    Wilson coefficients for Higgs boson production and decoupling relations to

    Marvin Gerlach🇩🇪 · Florian Herren🇩🇪 · Matthias Steinhauser🇩🇪

    An important ingredient for the calculation of Higgs boson properties in the infinite top quark mass limit is the knowledge of the effective coupling between the Higgs bosons and gluons, i.e. the Wilson coefficients and for one and two Higgs bosons, respectively. In this work we calculate for the first time to four loops in a direct, diagrammatic way, discussing in detail all issues arising due to the renormalization of operator products. Furthermore, we also calculate the Wilson coefficient for the coupling of a single Higgs boson to gluons as well as all four loop decoupling relations in QCD with general SU colour factors. The latter are related to and via low-energy theorems.

    hep-phJHEP(2018)·50 citations
  12. 12*

    Revisiting RGEs for general gauge theories

    Ingo Schienbein🇫🇷 · Florian Staub🇩🇪 · Tom Steudtner🇬🇧 · Kseniia Svirina🇫🇷

    We revisit the renormalisation group equations (RGE) for general renormalisable gauge theories at one- and two-loop accuracy. We identify and correct various mistakes in the literature for the -functions of the dimensionful Lagrangian parameters (the fermion mass, the bilinear and trilinear scalar couplings) as well as the dimensionless quartic scalar couplings. There are two sources for these discrepancies. Firstly, the known expressions for the scalar couplings assume a diagonal wave-function renormalisation which is not appropriate for models with mixing in the scalar sector. Secondly, the dimensionful parameters have been derived in the literature using a dummy field method which we critically re-examine, obtaining revised expressions for the -function of the fermion mass. We perform an independent cross-check using well-tested supersymmetric RGEs which confirms our results. The numerical impact of the changes in the -function for the fermion mass terms is illustrated using a toy model with a heavy vector-like fermion pair coupled to a scalar gauge singlet. Unsurprisingly, the correction to the running of the fermion mass becomes sizeable for large Yukawa couplings of the order of O(1). Furthermore, we demonstrate the importance of the correction to the -functions of the scalar quartic couplings using a general type-III Two-Higgs-Doublet-Model. All the corrected expressions have been implemented in updated versions of the Mathematica package SARAH and the Python package PyR@TE.

    hep-phhep-thNPB(2019)·75 citations
  13. 13*

    Quantum corrections to the Classical Statistical Approximation for the expanding quantum field

    A.V. Leonidov🇷🇺 · A.A. Radovskaya🇷🇺

    We found the deviation of the equation of state from ultrarelativistic one due to quantum corrections for a nonequilibrium longitudinally expanding scalar field. Relaxation of highly excited quantum field is usually described in terms of Classical Statistical Approximation (CSA). However, the expansion of the system reduces the applicability of such a semiclassical approach as the CSA making quantum corrections important. We calculate the evolution of the trace of the energy-momentum tensor within the Keldysh-Schwinger framework for static and longitudinal expanding geometries. We provide analytical and numerical arguments for the appearance of the nontrivial intermediate regime where quantum corrections are significant.

    hep-phEPJC(2019)·7 citations
  14. 14*

    Final-state interactions of the Higgs boson in quark-gluon matter

    David d'Enterria🇨🇭 · Constantin Loizides🇺🇸

    In the first version of this paper \cite{dEnterria:2018bqi}, we presented a study of the final-state interactions of the Higgs boson in the hot and dense quark-gluon systems produced in pp, pPb, and PbPb collisions at CERN LHC and FCC energies. By computing the leading-order diagrams of the Higgs-parton scattering cross sections in perturbative QCD, and by embedding the produced Higgs bosons in an expanding quark-gluon medium modeled with 2D+1 viscous hydrodynamics with various QCD equations of state, we presented estimates of the expected scalar boson yields as functions of transverse momentum , and produced medium space-time size. A moderate suppression of the scalar boson yields was predicted due to medium-enhanced decays, in detriment of the channels that are typically used to observe the Higgs particle. After our work appeared, J. Ghiglieri and U. Wiedemann \cite{Ghiglieri:2019lzz} have presented thermal-field-theory calculations that indicate that the partial decays widths remain basically unaffected by interactions with surrounding partons in the kinematic range of relevance of our study. Such a theoretical result, in contradiction with our estimates, has brought us to revisit our calculations and to realize of the quantitative importance of thermal virtual corrections, neglected in our first work, that are as large as the real ones and of opposite sign. Such virtual corrections significantly reduce the Higgs-parton "absorption" cross sections originally computed in Ref. \cite{dEnterria:2018bqi}, and make the Higgs boson suppression negligible in the kinematic regime considered.

    hep-phhep-exnucl-exnucl-th13 citations
  15. 15*

    A new parametrization for the scalar pion form factors

    Stefan Ropertz🇩🇪 · Christoph Hanhart🇩🇪 · Bastian Kubis🇩🇪

    We derive a new parametrization for the scalar pion form factors that allows us to analyze data over a large energy range via the inclusion of resonances, and at the same time to ensure consistency with the high-accuracy dispersive representations available at low energies. As an application the formalism is used to extract resonance properties of excited scalar mesons from data for . In particular we find for the pole positions of and and , respectively. In addition, from their residues we calculate the respective branching ratios into to be and .

    hep-phhep-exnucl-thEPJC(2018)·90 citations
  16. 16*

    Impact of QCD jets and heavy-quark production in cosmic-ray proton atmospheric showers up to 10 eV

    David d'Enterria🇨🇭 · Tanguy Pierog🇩🇪 · Guanhao Sun🇨🇭

    The PYTHIA 6 Monte Carlo (MC) event generator, commonly used in collider physics, is interfaced for the first time with a fast transport simulation of a hydrogen atmosphere, with the same density as air, in order to study the properties of extended atmospheric showers (EAS) produced by cosmic ray protons with energies E-- eV. At variance with the hadronic MC generators (EPOS-LHC, QGSJET, and SIBYLL) commonly used in cosmic-rays physics, PYTHIA includes the generation of harder hadronic jets and heavy (charm and bottom) quarks, thereby producing higher transverse momentum final particles, that could explain several anomalies observed in the data. The electromagnetic, hadronic, and muonic properties of EAS generated with various settings of PYTHIA 6, tuned to proton-proton data measured at the LHC, are compared to those from EPOS-LHC, QGSJET 01, QGSJET II, and SIBYLL 2.1. Despite their different underlying parton dynamics, the characteristics of the EAS generated with PYTHIA 6 are in between those predicted by the rest of MC generators. The only exceptions are the muonic components at large transverse distances from the shower axis, where PYTHIA predicts more activity than the rest of the models. Heavy-quark production, as implemented in this study for a hydrogen atmosphere, does not seem to play a key role in the EAS muon properties, pointing to nuclear effects as responsible of the muon anomalies observed in the air-shower data.

    ↳ astro-ph.HEhep-exhep-phnucl-ex+1ApJ(2019)·15 citations
  17. 17*

    Dark Monopoles in Grand Unified Theories

    Maria de Lourdes Z. P. Deglmann🇧🇷 · Marco A. C. Kneipp🇧🇷

    We consider a Yang-Mills-Higgs theory with gauge group broken to by a Higgs field in the adjoint representation. We obtain monopole solutions whose magnetic field is not in the Cartan Subalgebra. Since their magnetic field vanishes in the direction of the generator of the electromagnetic group , we call them Dark Monopoles. These Dark Monopoles must exist in some Grand Unified Theories (GUTs) without the need to introduce a dark sector. We analyze the particular case of GUT, where we obtain that their mass is , where is a monotonically increasing function of with and We also give a geometrical interpretation to their non-abelian magnetic charge.

    ↳ hep-thhep-phJHEP(2019)·5 citations
  18. 18*

    Squeezed vacuum used to accelerate the search for a weak classical signal

    M. Malnou🇺🇸 · D. A. Palken🇺🇸 · B. M. Brubaker🇺🇸 · Leila R. Vale🇺🇸 · Gene C. Hilton🇺🇸 · K. W. Lehnert🇺🇸

    Many experiments that interrogate fundamental theories require detectors whose sensitivities are limited by the laws of quantum mechanics. In cavity-based searches for axionic dark matter, vacuum fluctuations in the two quadratures of the cavity electromagnetic field limit the sensitivity to an axion-induced field. In an apparatus designed to partially mimic existing axion detectors, we demonstrate experimentally that such quantum limits can be overcome through the use of squeezed states. By preparing a microwave cavity in a squeezed state and measuring just the squeezed quadrature, we enhance the spectral scan rate by a factor of . This enhancement is in excellent quantitative agreement with a theoretical model accounting for both imperfect squeezing and measurement.

    ↳ quant-phhep-phPRX(2019)·116 citations
  19. 19*

    Weak radius of the proton

    C. J. Horowitz🇺🇸

    The weak charge of the proton determines its coupling to the boson. The distribution of weak charge is found to be dramatically different from the distribution of electric charge. The proton's weak radius fm is 80\% larger than its charge radius fm because of a very large pion cloud contribution. This large weak radius can be measured with parity violating electron scattering and may provide insight into the structure of the proton, various radiative corrections, and possible strange quark contributions.

    ↳ nucl-thhep-phnucl-exPLB(2019)·7 citations
  20. 20*

    The Lyman- forest as a diagnostic of the nature of the dark matter

    Antonella Garzilli (1)🇩🇰 · Andrii Magalich (2)🇳🇱 · Tom Theuns (3)🇬🇧 · Carlos S. Frenk (3)🇬🇧 · Christoph Weniger (4)🇳🇱 · Oleg Ruchayskiy (1)🇩🇰 · Alexey Boyarsky (2) ((1) Discovery Center, Niels Bohr Institute, Copenhagen University, (2) Lorentz Institute, Leiden University, (3) Institute for Computational Cosmology, University of Durham, (4) GRAPPA, University of Amsterdam)🇳🇱

    The observed Lyman- flux power spectrum (FPS) is suppressed on scales below . This cutoff could be due to the high temperature, , and pressure, , of the absorbing gas or, alternatively, it could reflect the free streaming of dark matter particles in the early universe. We perform a set of very high resolution cosmological hydrodynamic simulations in which we vary , and the amplitude of the dark matter free streaming, and compare the FPS of mock spectra to the data. We show that the location of the dark matter free-streaming cutoff scales differently with redshift than the cutoff produced by thermal effects and is more pronounced at higher redshift. We, therefore, focus on a comparison to the observed FPS at . We demonstrate that the FPS cutoff can be fit assuming cold dark matter, but it can be equally well fit assuming that the dark matter consists of keV sterile neutrinos in which case the cutoff is due primarily to the dark matter free streaming.

    ↳ astro-ph.COhep-phMNRAS(2019)·82 citations
  21. 21*

    Evaluation of CP-violation in HfF

    A.N. Petrov (1,2)🇷🇺 · L.V. Skripnikov (1,2)🇷🇺 · A.V. Titov (1,2)🇷🇺 · V. V. Flambaum (3) ((1) B.P.Konstantinov Petersburg Nuclear Physics Institute, Gatchina, Leningrad district, Russia (2) Dept. of Physics, Saint Petersburg State University, Saint Petersburg, Russia (3) School of Physics, The University of New South Wales, Sydney, Australia)🇦🇺

    CP violation effects produced by the nuclear magnetic quadrupole moment (MQM), electron electric dipole moment (EDM) and scalarpseudoscalar nucleuselectron neutral current (SP) interaction in HfF and HfF are calculated. The role of the hyperfine interaction is investigated. It is shown that the MQM shift can be distinguished from the electron EDM and SP ones due to the implicit dependence of MQM shift on the hyperfine sublevel. The MQM effect is expressed in terms of the proton (EDM), QCD vacuum angle and quark chromo-EDMs.

    ↳ physics.atom-phhep-phnucl-thPRA(2018)·22 citations
  22. 22*

    New Scalar Field Quartessence

    Robert Brandenberger🇨🇦 · Rodrigo R. Cuzinatto🇧🇷 · Jürg Fröhlich🇨🇭 · Ryo Namba🇨🇦

    We propose a cosmological scenario involving a scalar field, , that is a source of Dark Matter as well as of Dark Energy. Besides , the Lagrangian of the field theory envisaged in our scenario contains a second field , for simplicity assumed to be a scalar, too. For fixed values of , the potential term decays exponentially at large positive values of . While is not coupled to Standard Model fields, is assumed to be coupled to them, and the Green functions of depend on the cosmological redshift in the expanding universe. We assume that the term in the Lagrangian coupling to is such that, at redshifts larger than some critical redshift , is trapped near , and oscillations of about describing massive scalar particles give rise to Dark Matter. At redshifts below , the field is no longer trapped near the origin and starts to `roll' towards large field values. A homogenous component of emerges that acts as Dark Energy. Within over-dense regions, such as galaxies and galaxy clusters, the redshifting of stops, and therefore remains trapped near as long as is smaller than the redshift when structures on galactic scales decouple from the Hubble flow. Thus, at the present time, describes both Dark Energy and Dark Matter.

    ↳ gr-qcastro-ph.COhep-phhep-thJCAP(2019)·36 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.