PaperPanorama

HEP Phenomenology·hep-ph

Mon·Aug 17, 2015

18 papers14 primary·4 cross-listed·reconstructed*

  1. 01*

    Resummation and Matching of -quark Mass Effects in Production

    Marco Bonvini🇬🇧 · Andrew S. Papanastasiou🇩🇪 · Frank J. Tackmann🇩🇪

    We use a systematic effective field theory setup to derive the production cross section. Our result combines the merits of both fixed 4-flavor and 5-flavor schemes. It contains the full 4-flavor result, including the exact dependence on the -quark mass, and improves it with a resummation of collinear logarithms of . In the massless limit, it corresponds to a reorganized 5-flavor result. While we focus on production, our method applies to generic heavy-quark initiated processes at hadron colliders. Our setup resembles the variable flavor number schemes known from heavy-flavor production in deep-inelastic scattering, but also differs in some key aspects. Most importantly, the effective -quark PDF appears as part of the perturbative expansion of the final result where it effectively counts as an object. The transition between the fixed-order (4-flavor) and resummation (5-flavor) regimes is governed by the low matching scale at which the -quark is integrated out. Varying this scale provides a systematic way to assess the perturbative uncertainties associated with the resummation and matching procedure and reduces by going to higher orders. We discuss the practical implementation and present numerical results for the production cross section at NLO+NLL. We also provide a comparison to the corresponding predictions in the fixed 4-flavor and 5-flavor results and the Santander matching prescription. Compared to the latter, we find a slightly reduced uncertainty and a larger central value, with its central value lying at the lower edge of our uncertainty band.

    hep-phJHEP(2015)·114 citations
  2. 02*

    Intrinsic Fluctuations of the Proton Saturation Momentum Scale in High Multiplicity p+p Collisions

    Larry McLerran🇺🇸 · Prithwish Tribedy🇺🇸

    High multiplicity events in p+p collisions are studied using the theory of the Color Glass Condensate. We show that intrinsic fluctuations of the proton saturation momentum scale are needed in addition to the sub-nucleonic color charge fluctuations to explain the very high multiplicity tail of distributions in p+p collisions. The origin of such intrinsic fluctuations are presumably non-perturbative in nature. Classical Yang Mills simulations using the IP-Glasma model are performed to make quantitative estimations. We find that fluctuations as large as (1) of the average values of the saturation momentum scale can lead to rare high multiplicity events seen in p+p data at RHIC and LHC energies. Using the available data on multiplicity distributions we try to constrain the distribution of the proton saturation momentum scale and make predictions for the multiplicity distribution in 13 TeV p+p collisions.

    hep-phhep-exnucl-exnucl-thNPA(2016)·66 citations
  3. 03*

    Infinite Classes of Cases with Non-trivial Anomaly Cancellation

    S.M. Barr🇺🇸

    It is pointed out that there are infinite classes of cases based on gauge groups of the form SU(p)xSU(q)xU(1) in which gauge anomalies cancel non-trivially for small sets of fermion multiplets that include symmetric tensor representations. These cancellations are non-trivial in the sense that no group-theoretic explanation in terms of embedding in a larger simple group is apparent. The cases presented here could be useful for model building and lead to models with extra leptons and an extra U(1) gauge interaction under which the Standard Model fermions have distinctive charges. In many cases the SU(q)xU(1) groups act as family symmetries.

    hep-ph1 citation
  4. 04*

    A New Dynamical Picture for the Production and Decay of the Mesons

    Richard F. Lebed🇺🇸

    I introduce an entirely new dynamical description for exotic charmoniumlike hadrons, based upon the competing effects of the strong attraction between quarks in a diquark, and the inability of the diquark to hadronize on its own due to being a color nonsinglet. This mechanism naturally explains, for example, the strong preference of the to decay to rather than the , the existence of a state that decays to baryon pairs, and why some but not all exotics lie near hadronic thresholds. Owing to high-energy constituent counting rules, the four-quark nature of the states produces major changes to both the high- scaling of cross sections for producing such states and to the potency of the cusp effect of attracting resonances to pair-production thresholds. The recently observed pentaquark candidates are seen to fit naturally into this scheme.

    hep-phnucl-th8 citations
  5. 05*

    Musings on cosmological relaxation and the hierarchy problem

    Joerg Jaeckel🇩🇪 · Viraf M. Mehta🇩🇪 · Lukas T. Witkowski🇩🇪

    Recently Graham, Kaplan and Rajendran [1] proposed cosmological relaxation as a mechanism for generating a hierarchically small Higgs vacuum expectation value. Inspired by this we collect some thoughts on steps towards a solution to the electroweak hierarchy problem and apply them to the original model of cosmological relaxation [1]. To do so, we study the dynamics of the model and determine the relation between the fundamental input parameters and the electroweak vacuum expectation value. Depending on the input parameters the model exhibits three qualitatively different regimes, two of which allow for hierarchically small Higgs vacuum expectation values. One leads to standard electroweak symmetry breaking whereas in the other regime electroweak symmetry is mainly broken by a Higgs source term. While the latter is not acceptable in a model based on the QCD axion, in non-QCD models this may lead to new and interesting signatures in Higgs observables.

    hep-phhep-thPRD(2016)·48 citations
  6. 06*

    Can thermal inflation be consistent with baryogenesis in gauge-mediated SUSY breaking models?

    Taku Hayakawa🇯🇵 · Masahiro Kawasaki🇯🇵 · Masaki Yamada🇯🇵

    Thermal inflation is an attractive idea to dilute cosmic density of unwanted particles such as moduli fields which cause cosmological difficulties. However, it also dilutes preexisting baryon asymmetry and some viable baryogenesis is necessary for a cosmologically consistent scenario. We investigate whether the Affleck-Dine mechanism can produce baryon asymmetry enough to survive after the dilution in gauge-mediated SUSY breaking models. Flat directions except for flat direction cannot provide such huge baryon number because of Q-ball formation. We show that although the flat direction is special in terms of having -term which prevents Q-ball formation, it cannot explain the observed baryon asymmetry either.

    hep-phastro-ph.COPRD(2016)·5 citations
  7. 07*

    Solving the Balitsky-Kovchegov equation at next to leading order accuracy

    T. Lappi🇫🇮 · H. Mäntysaari🇫🇮

    We present the first numerical solution to the next to leading order Balitsky-Kovchegov (BK) equation in coordinate space in the large- limit. In addition to the dipole operator we also solve the evolution of the "conformal dipole" for which the conformal invariance breaking double logarithmic term is absent from the evolution equation. The NLO corrections are shown to slow down the evolution. We show that the solution depends strongly on the details of the initial condition, and that the solution to the equation is not positive definite with all initial conditions relevant for phenomenological applications.

    hep-phnucl-thNucl.Part.Phys.Proc.(2016)·0 citations
  8. 08*

    Numerical solution for the Schwinger-Dyson equation at finite temperature in Abelian gauge theory

    Hiroaki Kohyama🇹🇼

    We present the exact numerical solutions for the Schwinger-Dyson equations at finite temperature with general gauge in Abelian gauge theory. We then study the chiral phase transition on temperature from the obtained solutions. We find that, within the quenched Schwinger-Dyson equations, there exists substantial gauge dependence on the solutions and the critical temperature.

    hep-ph0 citations
  9. 09*

    A quantum information theoretic analysis of three flavor neutrino oscillations

    Subhashish Banerjee🇮🇳 · Ashutosh Kumar Alok🇮🇳 · R. Srikanth🇮🇳 · Beatrix C. Hiesmayr🇦🇹

    Correlations exhibited by neutrino oscillations are studied via quantum information theoretic quantities. We show that the strongest type of entanglement, genuine multipartite entanglement, is persistent in the flavour changing states. We prove the existence of Bell-type nonlocal features, in both its absolute and genuine avatars. Finally, we show that a measure of nonclassicality, dissension, which is a generalization of quantum discord to the tripartite case, is nonzero for almost the entire range of time in the evolution of an initial electron-neutrino. Via these quantum information theoretic quantities capturing different aspects of quantum correlations, we elucidate the differences between the flavour types, shedding light on the quantum-information theoretic aspects of the weak force.

    hep-phquant-phEPJC(2015)·117 citations
  10. 10*

    Threshold Neutral Pion Photoproduction on the Proton

    Astrid Hiller Blin🇪🇸 · Manuel Vicente Vacas🇪🇸 · Tim Ledwig🇪🇸

    The neutral pion photoproduction on the proton near threshold has a very small scattering cross section when compared to the charged channels, which in ChPT is explained by strong cancellations between the lowest order pieces. Therefore it is very sensitive to higher-order corrections of chiral perturbation theory. We perform a fully covariant calculation up to chiral order p^3 and we investigate the effect of the inclusion of the Delta(1232) resonance as an explicit degree of freedom. We show that the convergence improves, leading to a much better agreement with data at a wide range of energies.

    hep-phJPS Conf.Proc.(2016)·2 citations
  11. 11*

    Could Geoneutrinos Interact With the Geomagnetic Field?

    C.A.B. Quintero🇧🇷 · J.A. Helayël Neto🇧🇷

    In the present paper, we consider the possibility of interaction between geoneutrinos and the geomagnetic field, by adopting an approach based on the Dirac's equation with a non-minimal coupling that accounts for the magnetic interaction of the massive neutrinos. In our approach, we see that the magnetic interaction is controlled by a dimensionless parameter, , and we estimate the mean value of this interaction to be of the order of .

    hep-phphysics.geo-ph0 citations
  12. 12*

    Electronic and nuclear contributions in sub-GeV dark matter scattering: A case study with hydrogen

    Jiunn-Wei Chen🇹🇼 · Hsin-Chang Chi🇹🇼 · C.-P. Liu🇹🇼 · Chih-Liang Wu🇹🇼 · Chih-Pan Wu🇹🇼

    Scattering of sub-GeV dark matter (DM) particles with hydrogen atoms is studied in this paper. The interactions of DM with electrons and nucleons are both included and formulated in a general framework based on nonrelativistic effective field theory. On the assumption of same dark matter coupling strengths, it is found that DM-electron interactions dominate the inelastic atomic transitions to discrete excited states and ionization continuum around the threshold regions, and DM-nucleon interactions become more important with increasing energy and dominate in elastic scattering. The conclusion should apply, qualitatively, to practical detector species so that electronic and nuclear contributions in DM scattering processes can be disentangled, while issues including binding effects and recoil mechanism in many-body systems will require further detailed calculations.

    hep-phPRD(2015)·26 citations
  13. 13*

    NLO+NLL limits on and gauge boson masses

    Tomáš Ježo🇮🇹 · Michael Klasen🇩🇪 · David R. Lamprea🇩🇪 · Florian Lyonnet🇺🇸 · Ingo Schienbein🇫🇷

    QCD resummation predictions for the production of new charged () and neutral () heavy gauge bosons decaying leptonically are presented. These results are obtained with our resummation code at next-to-leading order and next-to-leading logarithmic (NLO+NLL) accuracy. Our predictions are compared to PYTHIA at leading order (LO) supplemented with parton showers (PS) and FEWZ at NLO and next-to-next-to-leading order (NNLO) for the -differential and total cross sections in the Sequential Standard Model (SSM) and general SU(2)SU(2)U(1) models. We show that the importance of resummation for total cross sections increases with the gauge boson mass. Finally, the latest ATLAS and CMS results are reinterpreted to derive new limits at NLO+NLL on and boson masses in general extensions of the Standard Model.

    hep-ph6 citations
  14. 14*

    Production cross section estimates for strongly-interacting Electroweak Symmetry Breaking Sector resonances at particle colliders

    Antonio Dobado🇪🇸 · Feng-Kun Guo🇩🇪 · Felipe J. Llanes-Estrada🇪🇸

    We are exploring a generic strongly-interacting Electroweak Symmetry Breaking Sector (EWSBS) with the low-energy effectie field theory for the four experimentally known particles (, , ) and its dispersion-relation based unitary extension. In this contribution we provide simple estimates for the production cross section of pairs of the EWSBS bosons and their resonances at proton-proton colliders as well as in a future (or potentially a ) collider with a typical few-TeV energy. We examine the simplest production mechanisms, tree-level production through a (dominant when quantum numbers allow) and the simple effective boson approximation (in which the electroweak bosons are considered as collinear partons of the colliding fermions). We exemplify with custodial isovector and isotensor resonances at 2 TeV, the energy currently being discussed because of a slight excess in the ATLAS 2-jet data. We find it hard, though not unthinkable, to ascribe this excess to one of these rescattering resonances. An isovector resonance could be produced at a rate smaller than, but close to earlier CMS exclusion bounds, depending on the parameters of the effective theory. The excess is then problematic and requires additional physics (such as an additional scalar resonance). The isotensor one (that would describe all charge combinations) has a smaller cross section.

    hep-phhep-exCommun.Theor.Phys.(2015)·19 citations
  15. 15*

    Uncertainty relation for quantum gravity

    Ya. I. Azimov🇷🇺

    Discussion of physical realization of coordinates demonstrates that the quantum theory of gravity (still absent) should be non-local and, probably, non-commutative as well.

    hep-thgr-qchep-phInt.J.Mod.Phys.A(2016)·0 citations
  16. 16*

    Dark Matter Halos as Particle Colliders: A Unified Solution to Small-Scale Structure Puzzles from Dwarfs to Clusters

    Manoj Kaplinghat🇺🇸 · Sean Tulin🇨🇦 · Hai-Bo Yu🇺🇸

    Astrophysical observations spanning dwarf galaxies to galaxy clusters indicate that dark matter (DM) halos are less dense in their central regions compared to expectations from collisionless DM N-body simulations. Using detailed fits to DM halos of galaxies and clusters, we show that self-interacting DM (SIDM) may provide a consistent solution to the DM deficit problem across all scales, even though individual systems exhibit a wide diversity in halo properties. Since the characteristic velocity of DM particles varies across these systems, we are able to measure the self-interaction cross section as a function of kinetic energy and thereby deduce the SIDM particle physics model parameters. Our results prefer a mildly velocity-dependent cross section, from on galaxy scales to on cluster scales, consistent with the upper limits from merging clusters. Our results dramatically improve the constraints on SIDM models and may allow the masses of both DM and dark mediator particles to be measured even if the dark sector is completely hidden from the Standard Model, which we illustrate for the dark photon model.

    astro-ph.COastro-ph.GAhep-phPRL(2016)·659 citations
  17. 17*

    Testing Lorentz symmetry with planetary orbital dynamics

    Aurélien Hees🇿🇦 · Quentin G. Bailey🇺🇸 · Christophe Le Poncin-Lafitte🇫🇷 · Adrien Bourgoin🇫🇷 · Attilio Rivoldini🇧🇪 · Brahim Lamine🇫🇷 · Frédéric Meynadier🇫🇷 · Christine Guerlin🇫🇷 · Peter Wolf🇫🇷

    Planetary ephemerides are a very powerful tool to constrain deviations from the theory of General Relativity using orbital dynamics. The effective field theory framework called the Standard-Model Extension (SME) has been developed in order to systematically parametrize hypothetical violations of Lorentz symmetry (in the Standard Model and in the gravitational sector). In this communication, we use the latest determinations of the supplementary advances of the perihelia and of the nodes obtained by planetary ephemerides analysis to constrain SME coefficients from the pure gravity sector and also from gravity-matter couplings. Our results do not show any deviation from GR and they improve current constraints. Moreover, combinations with existing constraints from Lunar Laser Ranging and from atom interferometry gravimetry allow us to disentangle contributions from the pure gravity sector from the gravity-matter couplings.

    gr-qcastro-ph.EPhep-phPRD(2015)·71 citations
  18. 18*

    J=3/2 charmed hypertriton

    H. Garcilazo🇲🇽 · A. Valcarce🇪🇸 · T.F. Carames🇪🇸

    By solving exact three-body equations, we study the three-baryon system with charm . We look for possible bound states using baryon-baryon interactions obtained from a chiral constituent quark model. The smaller effect of the conversion reverses the order of the and states, rather close on the strange sector. The diminishing of the kinetic energy due to the large reduced mass gives rise to a bound state in the channel. After correcting for Coulomb effects the binding energy would be between 140 and 715 keV.

    nucl-thhep-phPRC(2015)·23 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.