PaperPanorama

HEP Phenomenology·hep-ph

Fri·Oct 26, 2018

29 papers—23 primary·6 cross-listed·reconstructed*

  1. 01*

    Thermodynamics and phase diagrams of Polyakov-loop extended chiral models

    Aasmund Folkestad🇳🇴 · Jens O. Andersen🇳🇴

    We study the thermodynamics and phase diagrams of two-flavor quantum chromodynamics using the Polyakov-loop extended quark-meson (PQM) model and the Pisarski-Skokov chiral matrix () model. At temperatures up to and baryon chemical potentials up to , both models show reasonable agreement with the pressure, energy density, and interaction measure as calculated on the lattice. The Polyakov loop is found to rise significantly faster with temperature in models than on the lattice. In the low-temperature and high baryon density regime, the two models predict different states of matter; The PQM model predicts a confined and chirally restored phase, while the model predicts a deconfined and chirally restored phase. At finite isospin density and zero baryon density, the onset of pion condensation at is at , and the transition is second order at all temperatures. The transition temperature for pion condensation coincides with that of the chiral transition for values of the isospin chemical potential larger than approximately . In the model they also coincide with the transition temperature for deconfinement. The results are in good overall agreement with recent lattice simulations of the -- phase diagram.

    hep-phPRD(2019)·28 citations
  2. 02*

    Cosmological Constraints on Unstable Particles: Numerical Bounds and Analytic Approximations

    Keith R. Dienes🇺🇸 · Jason Kumar🇺🇸 · Patrick Stengel🇸🇪 · Brooks Thomas🇺🇸

    Many extensions of the Standard Model predict large numbers of additional unstable particles whose decays in the early universe are tightly constrained by observational data. For example, the decays of such particles can alter the ratios of light-element abundances, give rise to distortions in the cosmic microwave background, alter the ionization history of the universe, and contribute to the diffuse photon flux. Constraints on new physics from such considerations are typically derived for a single unstable particle species with a single well-defined mass and characteristic lifetime. In this paper, by contrast, we investigate the cosmological constraints on theories involving entire ensembles of decaying particles --- ensembles which span potentially broad ranges of masses and lifetimes. In addition to providing a detailed numerical analysis of these constraints, we also formulate a set of simple analytic approximations for these constraints which may be applied to generic ensembles of unstable particles which decay into electromagnetically-interacting final states. We then illustrate how these analytic approximations can be used to constrain a variety of toy scenarios for physics beyond the Standard Model. For ease of reference, we also compile our results in the form of a table which can be consulted independently of the rest of the paper. It is thus our hope that this work might serve as a useful reference for future model-builders concerned with cosmological constraints on decaying particles, regardless of the particular model under study.

    hep-phastro-ph.COPRD(2019)·13 citations
  3. 03*

    Phenomenological consequences of introducing new fermions with exotic charges to , muon (g-2), the primordial Lithium problem, and dark matter

    Lobsang Dhargyal🇮🇳

    In this work we show that, by introducing two singlet right handed fermions carrying opposite charges and while their left handed counterparts are singlet under and neutral under , in the regime where the new charged lepton masses are in the electroweak scale it will be able to explain the small neutrino masses via minimum-inverse seesaw scenario (MISS) as well as the reported and muon discrepancies. Also when the charged fermion masses are well above the electro weak scale the model can not explain the reported and muon discrepancies, but in this regime the model could explain the primordial Lithium problem. The model have another interesting extension where it can produce a stable and singlet under strong interaction scalar baryon that could constitute much of the dark matter mass of the universe which lead to a simple model where ordinary matter and dark-matter having same origin. The model can also provide new annihilation channels for the scalar singlet DM as well as allowing a doubly charged scalar whose signatures could show up in HL-LHC, ILC, CEPC etc.

    hep-ph2 citations
  4. 04*

    Quark and glue spectroscopy of scalars and pseudoscalars in SU(3) flavor limit

    Amir H. Fariborz🇺🇸 · Renata Jora🇷🇴 · Maria Lyukova🇺🇸

    Within the framework of the generalized linear sigma model with glueballs recently proposed [1,2], we study the schematic spectroscopy of scalar and pseudoscalar mesons in the SU(3) flavor limit and explore their quark and glue contents. In this framework, for both scalars and pseudoscalars, the two octet physical states are admixtures of quark-antiquark and four-quark components, and the three singlet states contain quark-antiquark, four-quark and glue components. We identify the two scalar octets with and and the two pseudoscalar octets with and . We show that, as expected, the light pseudoscalar octet is made dominantly of quark-antiquarks whereas the light scalar octet has a reversed substructure with a dominant four-quark component. The case of singlets is more complex due to surplus of states up to around 2 GeV. We consider all 35 permutations for identifying the three pseudoscalar singlets of our model with three of the seven experimental candidates. Our numerical simulation unambiguously identifies the lightest and the heaviest pseudoscalar singlets with and , respectively, and favors the identification of the middle singlet with either or [or, to a lesser extent, with ] and thereby allows a probe of their substructures. We then estimate the quark and glue components and find that the three pseudoscalar singlets (from lightest to heaviest) are mainly of quark-antiquark, four-quark and glue substructure, while the corresponding three scalar singlets (from lightest to heaviest) are of four-quark, quark antiquark and glue contents. The masses of pure pseudoscalar and scalar glueballs are estimated around 2.0 and 1.6 GeV, respectively.

    hep-phInt.J.Mod.Phys.A(2019)·5 citations
  5. 05*

    Photoproduction of J/ in non-single-diffractive p+p collisions

    Zehua Cao🇨🇳 · Lijuan Ruan🇺🇸 · Zebo Tang🇨🇳 · Zhangbu Xu🇺🇸 · Chi Yang🇨🇳 · Shuai Yang🇺🇸 · Wangmei Zha🇨🇳

    Recently, significant enhancements of J/ production at very low transverse momenta were observed by the ALICE and STAR collaboration in peripheral hadronic A+A collisions. The anomaly excesses point to evidence of coherent photon-nucleus interactions in violent hadronic heavy-ion collisions, which were conventionally studied only in ultra-peripheral collisions. Assuming that the coherent photoproduction is the underlying mechanism which is responsible for the excess observed in peripheral A+A collisions, its contribution in p+p collisions with nuclear overlap, i.e. non-single-diffractive collisions, is of particular interest. In this paper, we perform a calculation of exclusive J/ photoproduction in non-single-diffractive p+p collisions at RHIC and LHC energies base on the pQCD motivated parametrization from world-wide experimental data, which could be further employed to improve the precision of phenomenal calculations for photoproduction in A+A collisions. The differential rapidity and transverse momentum distributions of J/ from photoproduction are presented. In comparison with the J/ production from hadronic interactions, we find that the contribution of photoproduction is negligible.

    hep-phnucl-thCPC(2019)·7 citations
  6. 06*

    Double-slit experiment at fermi scale: coherent photoproduction in heavy-ion collisions

    Wangmei Zha🇨🇳 · Lijuan Ruan🇺🇸 · Zebo Tang🇨🇳 · Zhangbu Xu🇺🇸 · Shuai Yang🇺🇸

    The double-slit experiment has become a classic thought experiment, for its clarity in expressing the central puzzle of quantum mechanics -- wave-particle complementarity. Such wave-particle duality continues to be challenged and investigated in a broad range of entities with electrons, neutrons, helium atoms, C fullerenes, Bose-Einstein condensates and biological molecules. All existing experiments are performed with the scale larger than angstrom. In this article, we present a double-slit scenario at fermi scale with new entities -- coherent photon products in heavy-ion collisions. Virtual photons from the electromagnetic fields of relativistic heavy ions can fluctuate to quark-antiquark pairs, scatter off a target nucleus and emerge as vector mesons. The two colliding nuclei can take turns to act as targets, forming a double-slit interference pattern. Furthermore, the `which-way' information can be partially solved by the violent strong interactions in the proposed scenario, which demonstrates a key concept of quantum mechanics -- complementary principle.

    hep-phPRC(2019)·43 citations
  7. 07*

    Electroweak monopoles and electroweak baryogenesis

    Suntharan Arunasalam🇦🇺 · Daniel Collison🇦🇺 · Archil Kobakhidze🇦🇺

    We describe electroweak monopoles within the Born-Infeld extension of electroweak theory. We argue for topological stability of these monopoles and computed their mass in terms of the Born-Infeld mass parameters. We then propose a new mechanism for electroweak baryogenesis which takes advantage of the following salient features of the electroweak monopoles: (i) monopoles support extra CP violation in the topological sector of the electroweak theory; (ii) they mediate unsuppressed baryon number violating interactions; (iii) non-thermal production of monopoles during the electroweak phase transitions generates departure from thermal equilibrium. We demonstrate that the observed baryon asymmetry of the universe can be explained in our theory in the presence of electroweak monopoles of mass TeV.

    hep-phastro-ph.COhep-th6 citations
  8. 08*

    Neutrino phenomenology in the flavored NMSSM without domain wall problems

    M. A. Ouahid🇲🇦 · M. A. Loualidi🇲🇦 · R. Ahl Laamara🇲🇦 · E. H. Saidi🇲🇦

    We propose a next-to-minimal supersymmetric Standard Model (NMSSM) extended by an flavor symmetry and three right-handed neutrinos providing a detailed study of the neutrino sector and a solution to the domain wall problem. In this proposal, neutrino masses are generated through Type I seesaw mechanism while the mixing angles are described by the trimaximal mixing realized using the NMSSM singlet S and only two flavon fields. The phenomenology of neutrino parameters is studied for normal and inverted mass hierarchies. In particular, we numerically evaluated the observables related to neutrino masses and mixing, namely, , , , and where we find that the ranges of and are accessible by current and future experiments while the obtained ranges of and lie within the current experimental data. Another attractive feature we discussed in this paper is the circumvention of the domain wall problem induced by the spontaneous breaking of the discrete symmetry. We first showed that the domain walls in the charged lepton sector occur at high energy scale leading to unproblematic domain walls, while in the neutrino sector they are inevitable. Then, to solve this problem, we reconsidered the well-known approach that relies on the explicit breaking of the discrete symmetry through the insertion of Planck-suppressed operators induced by supergravity. \keywords{Neutrino physics, Discrete flavor symmetry,Trimaximal mixing, Domain walls}

    hep-phPRD(2020)·13 citations
  9. 09*

    Effective models of WIMP Direct Detection in DAMA/LIBRA-phase2

    Sunghyun Kang🇰🇷 · Stefano Scopel🇰🇷 · Gaurav Tomar🇰🇷 · Jong-Hyun Yoon🇰🇷

    Since the DAMA/LIBRA collaboration released updated results from their search for the annual modulation signal expected from Dark Matter (DM) scattering in their NaI detectors, we have fitted the updated DAMA result for the modulation amplitudes for a Weakly Interacting Massive Particle (WIMP) signal, parameterizing the interaction with nuclei in terms of the most general effective Lagrangian for a WIMP particle spin 1/2, systematically assuming dominance of one of the 14 possible interaction terms and a standard Maxwellian for the WIMP velocity distribution. We find that most of the couplings of the non-relativistic effective Hamiltonian can provide a better fit compared to the standard Spin Independent interaction case, and with a reduced fine-tuning of the three parameters (WIMP mass, WIMP-nucleon effective cross-section and ratio between the WIMP-neutron and the WIMP-proton couplings). In addition, effective models for which the cross section depends explicitly on the WIMP incoming velocity can provide a better fit of the DAMA data at large values of compared to the standard velocity-independent cross-section due to a different phase of the modulation amplitudes. All the best fit solutions are in tension with exclusion plots of both XENON1T and PICO60.

    hep-phPoS(2019)·1 citation
  10. 10*

    Non-standard scaling laws of WIMP-nucleus interactions in WIMP direct detection

    Sunghyun Kang🇰🇷 · Stefano Scopel🇰🇷 · Gaurav Tomar🇰🇷 · Jong-Hyun Yoon🇰🇷

    Guided by the non-relativistic effective field theory of interactions between Weakly Interacting Massive Particles (WIMPs) of spin 1/2 and nuclei we study direct detection exclusion plots for an example of non-standard spin-dependent interaction and compare it to the standard one. We analyze an extensive list of 15 existing experiments including the effects of momentum dependence and isospin violation. In our analysis, we fixed the dark matter velocity distribution to a Maxwellian.

    hep-phPoS(2019)·0 citations
  11. 11*

    R-parity from string compactification

    Jihn E. Kim🇰🇷

    In this paper, we embed the parity as a discrete subgroup of a global symmetry \UoR\,obtained from compactification of heterotic string . A part of \UoR\,transformation is the shift of the anticommuting variable to which necessarily incoorporate the transformation of internal space coordinate. Out of six internal spaces, we identify three U(1)'s whose charges are denoted as , and . The \UoR~is defined as \UEE\UKK~where \UEE~is the part from and \UKK~is the part generated by , and . We propose a method to define a \UoR~direction. The needed vacuum expectation values for breaking gauge U(1)'s except U(1) of the standard model carry \UoR~charge 4 modulo 4 such that \UoR~is broken down to at the grand unification scale. is broken to between the intermediate () and the electroweak scales (). The conditions we impose are proton longevity, a large top quark mass, and acceptable magnitudes for the term and neutrino masses.

    hep-phhep-thPRD(2019)·13 citations
  12. 12*

    Matching the Quasi Meson Distribution Amplitude in RI/MOM scheme

    Yu-Sheng Liu🇨🇳 · Wei Wang🇨🇳 · Ji Xu🇨🇳 · Qi-An Zhang🇨🇳 · Shuai Zhao🇨🇳 · Yong Zhao🇺🇸

    The -dependence of light-cone distribution amplitude (LCDA) can be directly calculated from a quasi distribution amplitude (DA) in lattice QCD within the framework of large-momentum effective theory (LaMET). In this paper, we study the one-loop renormalization of the quasi-DA in the regularization-independent momentum subtraction (RI/MOM) scheme. The renormalization factor for the quasi parton distribution function can be used to renormalize the quasi-DA provided that they are implemented on lattice and in perturbation theory in the same manner. We derive the one-loop matching coefficient that matches quasi-DA in the RI/MOM scheme onto LCDA in the scheme. Our result provides the crucial step to extract the LCDAs from lattice matrix elements of quasi-DAs.

    hep-phhep-latnucl-thPRD(2019)·46 citations
  13. 13*

    Supersymmetric Models in Light of Improved Higgs Mass Calculations

    E. Bagnaschi🇨🇭 · H. Bahl🇩🇪 · J. Ellis🇬🇧 · J. Evans🇰🇷 · T. Hahn🇩🇪 · S. Heinemeyer🇪🇸 · W. Hollik🇩🇪 · K. A. Olive🇺🇸 · S. Paßehr🇫🇷 · H. Rzehak🇩🇰 · I. V. Sobolev🇩🇪 · G. Weiglein🇩🇪 · J. Zheng🇯🇵

    We discuss the parameter spaces of supersymmetry (SUSY) scenarios taking into account the improved Higgs-mass prediction provided by FeynHiggs 2.14.1. Among other improvements, this prediction incorporates three-loop renormalization-group effects and two-loop threshold corrections, and can accommodate three separate mass scales: m_{\tilde q} (for squarks), m_{\tilde g} (for gluinos) and m_{\tilde\chi} (for electroweakinos). Furthermore, it contains an improved treatment of the DRbar scalar top parameters avoiding problems with the conversion to on-shell parameters, that yields more accurate results for large SUSY-breaking scales. We first consider the CMSSM, in which the soft SUSY-breaking parameters m_0 and m_{1/2} are universal at the GUT scale, and then sub-GUT models in which universality is imposed at some lower scale. In both cases, we consider the constraints from the Higgs-boson mass M_h in the bulk of the (m_0, m_{1/2}) plane and also along stop coannihilation strips where sparticle masses may extend into the multi-TeV range. We then consider the minimal anomaly-mediated SUSY-breaking (mAMSB) scenario, in which large sparticle masses are generic. In all these scenarios the substantial improvements between the calculations of M_h in FeynHiggs 2.14.1 and FeynHiggs 2.10.0, which was used in an earlier study, change significantly the preferred portions of the models' parameter spaces. Finally, we consider the pMSSM11, in which sparticle masses may be significantly smaller and we find only small changes in the preferred regions of parameter space.

    hep-phEPJC(2019)·34 citations
  14. 14*

    Constraining the invisible neutrino decay with KM3NeT-ORCA

    P.F. de Salas🇪🇸 · S. Pastor🇪🇸 · C.A. Ternes🇪🇸 · T. Thakore🇪🇸 · M. Tórtola🇪🇸

    Several theories of particle physics beyond the Standard Model consider that neutrinos can decay. In this work we assume that the standard mechanism of neutrino oscillations is altered by the decay of the heaviest neutrino mass state into a sterile neutrino and, depending on the model, a scalar or a Majoron. We study the sensitivity of the forthcoming KM3NeT-ORCA experiment to this scenario and find that it could improve the current bounds coming from oscillation experiments, where three-neutrino oscillations have been considered, by roughly two orders of magnitude. We also study how the presence of this neutrino decay can affect the determination of the atmospheric oscillation parameters and , as well as the sensitivity to the neutrino mass ordering.

    hep-phhep-exPLB(2019)·45 citations
  15. 15*

    All-orders behaviour and renormalons in top-mass observables

    Silvia Ferrario Ravasio🇮🇹 · Paolo Nason🇮🇹 · Carlo Oleari🇮🇹

    We study a simplified model of top production and decay, consisting in a virtual vector boson decaying into a massive-massless - quark-antiquark pair. The top has a finite width and further decays into a stable vector boson and a quark. We then consider the emission or the virtual exchange of one gluon, with all possible light-quark loop insertions. These are the dominant diagrams in the limit of an infinite number of light flavours. We devise a procedure to compute this process fully, by analytic and numerical methods, and for any infrared-safe final-state observables. We examine the results at arbitrary orders in perturbation theory, and assess the factorial growth associated with renormalons. We look for renormalon effects leading to corrections of order , that we dub `linear' renormalons, in the inclusive cross section (with and without selection cuts), in the mass of the reconstructed-top system, and in the average energy of the final-state boson, considering both the pole and the scheme for the top mass. We find that the total cross section without cuts, if expressed in terms of the mass, does not exhibit linear renormalons, but, as soon as selection cuts are introduced, jets-related linear renormalons arise in any mass scheme. In addition, we show that the reconstructed mass is affected by linear renormalons in any scheme and that the average energy of the boson (that we consider as a simplified example of leptonic observable), in any mass scheme, has a renormalon in the narrow-width limit, that is however screened at large orders for finite top widths, provided the top mass is in the scheme.

    hep-phJHEP(2019)·37 citations
  16. 16*

    Feasibility of studying the K resonance using K femtoscopy

    T. J. Humanic🇺🇸

    The feasibility of using K femtoscopy to experimentally study the K resonance is considered. The K resonance is challenging to study due to its broad width and proximity in mass to the K, both of which predominantly decay via the K channel. One of the main interests in the K is that it is considered a candidate for a tetraquark state. It is proposed to use two-particle femtoscopic methods with K pairs produced in proton-proton and heavy ion collisions assuming a strong final-state interaction between them due to elastic scattering and/or via the K resonance. Calculations of K correlation functions are made to estimate the strength of these final-state interactions and to see if this signal can be adequately separated from the K background. A possible signature of diquark versus tetraquark behavior of the K final-state interaction is also discussed.

    hep-phhep-exJ.Phys.G(2019)·2 citations
  17. 17*

    The hMSSM approach for Higgs self-couplings revisited

    Stefan Liebler🇩🇪 · Margarete Mühlleitner🇩🇪 · Michael Spira🇨🇭 · Maximilian Stadelmaier🇩🇪

    We compare the decay of the heavy Higgs boson into two SM-like Higgs bosons, , calculated in a Feynman-diagrammatic approach at the one-loop level based on the one hand on the full effective potential involving the top quark and stops in the Minimal Supersymmetric Standard Model (MSSM) accompanied by the matched Two-Higgs-Doublet Model (2HDM) as its low-energy limit and on the other hand on the hMSSM approximation. We identify missing contributions due to the top quark in the Higgs self-couplings of the hMSSM, that - when taken into account - lead to a good agreement between the hMSSM and a full MSSM calculation, at least in the limit of the Higgsino mass parameter being small compared to the stop spectrum. We also thoroughly analyze momentum-dependent and kinetic corrections intrinsic to the Feynman-diagrammatic approach and the matching to the effective Lagrangian, respectively, for both our calculation in the MSSM and the hMSSM and for the latter suggest to include additional corrections from the top quark, which are independent of the unknown supersymmetric spectrum.

    hep-phEPJC(2019)·16 citations
  18. 18*

    Probing new electroweak states via precision measurements at the LHC and future colliders

    Luca Di Luzio🇮🇹 · Ramona Gröber🇩🇪 · Giuliano Panico🇪🇸

    Several new physics scenarios, motivated e.g. by dark matter, feature new electroweakly charged states where the lightest particle in the multiplet is stable and neutral. In such cases direct searches at LHC are notoriously difficult, while electroweak precision tests both at hadron and lepton colliders offer the possibility to indirectly probe those states. In this work, we assess the sensitivity of the high-luminosity phase of the LHC on new electroweak multiplets via the modification of neutral and charged Drell-Yan processes, and compare the reach of future hadron and lepton colliders presently under consideration.

    hep-phhep-exJHEP(2019)·94 citations
  19. 19*

    A light complex scalar for the electron and muon anomalous magnetic moments

    Jia Liu (Chicago U., EFI)🇺🇸 · Carlos E.M. Wagner (Chicago U., EFI & Argonne & Chicago U., KICP)🇺🇸 · Xiao-Ping Wang (Argonne)🇺🇸

    The anomalous magnetic moments of the electron and the muon are interesting observables, since they can be measured with great precision and their values can be computed with excellent accuracy within the Standard Model (SM). The current experimental measurement of this quantities show a deviation of a few standard deviations with respect to the SM prediction, which may be a hint of new physics. The fact that the electron and the muon masses differ by two orders of magnitude and the deviations have opposite signs makes it difficult to find a common origin of these anomalies. In this work we introduce a complex singlet scalar charged under a Peccei-Quinn-like (PQ) global symmetry together with the electron transforming chirally under the same symmetry. In this realization, the CP-odd scalar couples to electron only, while the CP-even part can couple to muons and electrons simultaneously. In addition, the CP-odd scalar can naturally be much lighter than the CP-even scalar, as a pseudo-Goldstone boson of the PQ-like symmetry, leading to an explanation of the suppression of the electron anomalous magnetic moment with respect to the SM prediction due to the CP-odd Higgs effect dominance, as well as an enhancement of the muon one induced by the CP-even component.

    hep-phhep-exJHEP(2019)·121 citations
  20. 20*

    S-wave heavy quarkonium spectrum with next-to-next-to-next-to-leading logarithmic accuracy

    C. Anzai🇪🇸 · D. Moreno🇪🇸 · A. Pineda🇪🇸

    We obtain the Potential NRQCD Lagrangian relevant for S-wave states with next-next-to-next-to-leading logarithmic (NNNLL) accuracy. We compute the heavy quarkonium mass of spin-averaged (angular momentum) states, with otherwise arbitrary quantum numbers, with NNNLL accuracy. These results are complete up to a missing contribution of the two-loop soft running.

    hep-phPRD(2018)·11 citations
  21. 21*

    Fiducial polarization observables in hadronic WZ production: A next-to-leading order QCD+EW study

    Julien Baglio🇩🇪 · LE Duc Ninh🇻🇳

    We present a study at next-to-leading-order (NLO) of the process , where , at the Large Hadron Collider. We include the full NLO QCD corrections and the NLO electroweak (EW) corrections in the double-pole approximation. We define eight fiducial polarization coefficients directly constructed from the polar-azimuthal angular distribution of the decay leptons. These coefficients depend strongly on the kinematical cuts on the transverse momentum or rapidity of the individual leptons. Similarly, fiducial polarization fractions are also defined and they can be directly related to the fiducial coefficients. We perform a detailed analysis of the NLO QCD+EW fiducial polarization observables including theoretical uncertainties stemming from the scale variation and parton distribution function uncertainties, using the fiducial phase space defined by the ATLAS and CMS experiments. We provide results in the helicity coordinate system and in the Collins-Soper coordinate system, at a center-of-mass energy of 13 TeV. The EW corrections are found to be important in two of the angular coefficients related to the boson, irrespective of the kinematical cuts or the coordinate system. Meanwhile, those EW corrections are very small for the bosons.

    hep-phhep-exJHEP(2019)·46 citations
  22. 22*

    The -parity Violating Decays of Charginos and Neutralinos in the B-L MSSM

    Sebastian Dumitru🇺🇸 · Burt A. Ovrut🇺🇸 · Austin Purves🇺🇸

    The MSSM is the MSSM with three right-handed neutrino chiral multiplets and gauged symmetry. The symmetry is broken by the third family right-handed sneutrino acquiring a VEV, thus spontaneously breaking -parity. Within a natural range of soft supersymmetry breaking parameters, it is shown that a large and uncorrelated number of initial values satisfy all present phenomenological constraints; including the correct masses for the , bosons, having all sparticles exceeding their present lower bounds and giving the experimentally measured value for the Higgs boson. For this "valid" set of initial values, there are a number of different LSPs, each occurring a calculable number of times. We plot this statistically and determine that among the most prevalent LSPs are chargino and neutralino mass eigenstates. In this paper, the -parity violating decay channels of charginos and neutralinos to standard model particles are determined, and the interaction vertices and decay rates computed analytically. These results are valid for any chargino and neutralino, regardless of whether or not they are the LSP. For chargino and neutralino LSPs, we will-- in a subsequent series of papers --present a numerical study of their RPV decays evaluated statistically over the range of associated valid initial points.

    hep-phhep-thJHEP(2019)·21 citations
  23. 23*

    Eikonal and asymptotic fits to high energy data for , , and : An update with curvature corrections

    Loyal Durand🇺🇸 · Phuoc Ha🇺🇸

    We update our eikonal fit and comprehensive asymptotic fits to high energy data on proton--proton and antiproton--proton scattering for , , , , and . The fits include the new TOTEM values of total proton-proton cross section, , and at = 13 TeV and the Telescope Array value of the total proton-proton cross section at = 95 TeV, data from the latest measurements of the inelastic cross sections at = 8 TeV (by TOTEM and ATLAS) and 13 TeV (by CMS, ATLAS, and TOTEM). An important new feature of this work is the correction of the data to include the effects of curvature in on the values of , at , and obtained by extrapolation from the larger values of where the differential cross section is measured, The effects are significant. The stability of the fits is excellent and the new results agree well with the predictions of earlier fits. This work again confirms the evidence for the proton asymptotically becoming a black disk of gluons.

    hep-phPRD(2019)·5 citations
  24. 24*

    The experimental status of direct searches for exotic physics beyond the standard model at the Large Hadron Collider

    Salvatore Rappoccio🇺🇸

    The standard model of particle physics is an extremely successful theory of fundamental interactions, but it has many known limitations. It is therefore widely believed to be an effective field theory that describes interactions near the TeV scale. A plethora of strategies exist to extend the standard model, many of which contain predictions of new particles or dynamics that could manifest in proton-proton collisions at the Large Hadron Collider (LHC). As of now, none have been observed, and much of the available phase space for natural solutions to outstanding problems is excluded. If new physics exists, it is therefore either heavy (i.e. slightly above the reach of current searches) or hidden (i.e. currently indistinguishable from standard model backgrounds). We summarize the existing searches, and discuss future directions at the LHC.

    ↳ hep-exhep-phRev.Phys.(2019)·74 citations
  25. 25*

    Light-Quark Resonances at COMPASS

    Stefan Wallner (for the COMPASS Collaboration)🇩🇪

    The main goal of the spectroscopy program at COMPASS is to explore the light-meson spectrum in the mass range below about using diffractive dissociation reactions. Our flagship channel is the production of three charged pions in the reaction: , for which COMPASS has acquired the so far world's largest dataset of roughly exclusive events using an beam. In order to extract the parameters of the and resonances that appear in the system, we performed the so far most comprehensive resonance-model fit, using Breit-Wigner parametrizations. This method in combination with the high statistical precision of our data allows us to study ground and excited states. We study the resonance in the and decays. In addition to the ground state resonance , we have found evidence for the . We also study the spectrum of states by simultaneously describing four waves using three resonances, the , the , and the . Using a novel analysis approach, where the resonance-model fit is performed simultaneously in narrow bins of the squared four-momentum transfer between the beam pion and the target proton, allows us to study the dependence of resonant and non-resonant components included in our model. We observe that for most of the partial waves, the non-resonant components show a steeper spectrum compared to the resonances and that the spectrum of most of the resonances becomes shallower with increasing resonance mass. We also study the dependence of the relative phases between resonance components. The pattern we observe is consistent with a common production mechanism of these states.

    ↳ hep-exhep-phPoS(2018)·3 citations
  26. 26*

    GeV observations of the extended pulsar wind nebulae constrain the pulsar interpretations of the cosmic-ray positron excess

    Shao-Qiang Xi🇨🇳 · Ruo-Yu Liu🇩🇪 · Zhi-Qiu Huang🇨🇳 · Kun Fang🇨🇳 · Xiang-Yu Wang🇨🇳

    It has long been suggested that nearby pulsars within are the leading candidate of the 10-500 GeV cosmic-ray positron excess measured by PAMELA and other experiments. The recent measurement of surface brightness profile of TeV nebulae surrounding Geminga and PSR~B0656+14 by the High-Altitude Water Cherenkov Observatory (HAWC) suggests inefficient diffusion of particles from the sources, giving rise to a debate on the pulsar interpretation of the cosmic-ray positron excess. Here we argue that GeV observations provide more direct constraints on the positron density in the TeV nebulae in the energy range of 10-500 GeV and hence on the origin of the observed positron excess. Motivated by this, we search for GeV emission from the TeV nebulae with the \textsl{Fermi} Large Area Telescope (LAT). No spatially-extended GeV emission is detected from these two TeV nebulae in the framework of two-zone diffusion spatial templates, suggesting a relatively low density of GeV electrons/positrons in the TeV nebulae. A joint modelling of the data from HAWC and \textsl{Fermi}-LAT disfavors Geminga and PSR~B0656+14 as the dominant source of the positron excess at GeV for the usual Kolmogorov-type diffusion, while for an energy-independent diffusion, a dominant part of the positron excess contributed by them cannot be ruled out by the current data.

    ↳ astro-ph.HEastro-ph.COhep-phApJ(2019)·52 citations
  27. 27*

    Gravitational Waves Induced by non-Gaussian Scalar Perturbations

    Rong-gen Cai🇨🇳 · Shi Pi🇯🇵 · Misao Sasaki🇯🇵

    We study gravitational waves (GWs) induced by non-Gaussian curvature perturbations. We calculate the density parameter per logarithmic frequency interval, , given that the power spectrum of the curvature perturbation has a narrow peak at some small scale , with a local-type non-Gaussianity, and constrain the nonlinear parameter with the future LISA sensitivity curve as well as with constraints from the abundance of the primordial black holes (PBHs). We find that the non-Gaussian contribution to increases as , peaks at , and has a sharp cutoff at . The non-Gaussian part can exceed the Gaussian part if . If both a slope with and the multiple-peak structure around a cutoff are observed, it can be recognized as a smoking gun of the primordial non-Gaussianity. We also find that if PBHs with masses of to are identified as cold dark matter of the Universe, the corresponding GWs must be detectable by LISA-like detectors, irrespective of the value of or .

    ↳ astro-ph.COgr-qchep-phhep-thPRL(2019)·510 citations
  28. 28*

    Navigating Collinear Superspace

    Timothy Cohen🇺🇸 · Gilly Elor🇺🇸 · Andrew J. Larkoski🇺🇸 · Jesse Thaler🇺🇸

    We introduce a new set of effective field theory rules for constructing Lagrangians with supersymmetry in collinear superspace. In the standard superspace treatment, superfields are functions of the coordinates , and supersymmetry preservation is manifest at the Lagrangian level in part due to the inclusion of auxiliary - and -term components. By contrast, collinear superspace depends on a smaller set of coordinates , where is a complex Grassmann number without a spinor index. This provides a formulation of supersymmetric theories that depends exclusively on propagating degrees of freedom, at the expense of obscuring Lorentz invariance and introducing inverse momentum scales. After establishing the general framework, we construct collinear superspace Lagrangians for free chiral matter and non-Abelian gauge fields. For the latter construction, an important ingredient is a superfield representation that is simultaneously chiral, anti-chiral, and real; this novel object encodes residual gauge transformations on the light cone. Additionally, we discuss a fundamental obstruction to constructing interacting theories with chiral matter; overcoming these issues is the subject of our companion paper, where we introduce a larger set of superfields to realize the full range of interactions compatible with . Along the way, we provide a novel framing of reparametrization invariance using a spinor decomposition, which provides insight into this important light-cone symmetry.

    ↳ hep-thhep-phJHEP(2020)·6 citations
  29. 29*

    Properties of the ground state of electronic excitations in carbon-like nanocones

    Yurii A. Sitenko🇺🇦 · Volodymyr M. Gorkavenko🇺🇦

    On the basis of the continuum model for long-wavelength charge carriers, originating in the tight-binding approximation for the nearest-neighbour interaction of atoms in the crystalline lattice, we consider quantum ground-state effects of electronic excitations in Dirac materials with two-dimensional monolayer honeycomb structures warped into nanocones by a disclination; the nonzero size of the disclination is taken into account, and a boundary condition at the edge of the disclination is chosen to ensure self-adjointness of the Dirac-Weyl Hamiltonian operator. We show that the quantum ground-state effects are independent of the disclination size and find circumstances when they are independent of a parameter of the boundary condition. The magnetic flux circulating in the angular direction around the nanocone apex and the pseudomagnetic flux directed orthogonally to the nanocone surface are shown to be induced in the ground state.

    ↳ cond-mat.mes-hallcond-mat.mtrl-scicond-mat.str-elhep-phLow Temp.Phys.(2018)·9 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.