3,214 research outputs found

    Feynman rules for Coulomb gauge QCD

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    The Coulomb gauge in nonabelian gauge theories is attractive in principle, but beset with technical difficulties in perturbation theory. In addition to ordinary Feynman integrals, there are, at 2-loop order, Christ-Lee (CL) terms, derived either by correctly ordering the operators in the Hamiltonian, or by resolving ambiguous Feynman integrals. Renormalization theory depends on the subgraph structure of ordinary Feynamn graphs. The CL terms do not have subgraph structure. We show how to carry out enormalization in the presene of CL terms, by re-expressing these as `pseudo-Feynman' inegrals. We also explain how energy divergences cancel.Comment: 8 pages, 10 figue

    Multi-temperature zone, droplet-based microreactor for increased temperature control in nanoparticle synthesis

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    Microreactors are an emerging technology for the controlled synthesis of nanoparticles. The Multi-Temperature zone Microreactor (MTM) described in this work utilizes thermally isolated heated and cooled regions for the purpose of separating nucleation and growth processes as well as to provide a platform for a systematic study on the effect of reaction conditions on nanoparticle synthesis. © 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim

    A QCD Analysis of the Mass Structure of the Nucleon

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    {}From the deep-inelastic momentum sum rule and the trace anomaly of the energy-momentum tensor, I derive a separation of the nucleon mass into the contributions of the quark and gluon kinetic and potential energies, the quark masses, and the trace anomaly.Comment: 9 pages, MIT-CTP #2368, revtex with 1 tabl

    A Co-axial Multi-tube Heat Exchanger Applicable for a Geothermal ORC Power Plant

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    AbstractThe study proposes a Co-axial multi-tube heat exchanger (CMTHE) applicable to geothermal heat extraction. The heat exchanger is integrated with a 50kW geothermal ORC power plant having a working fluid of R-245fa. Two field tests were performed to examine the system response of the ORC system subject to change of CMTHE. In case 1 where the flow rate in the shell-side of CMTHE is maintained, the pressure variation in the shell-side of CMTHE casts minor variations on heat extraction, ORC power generation, and ORC efficiency during the transient. Moreover, the effect of pressure has barely any influence of the final states of heat extraction, ORC power generation, and ORC efficiency. In case 2 where the pressure is preserved in the CMTHE, it is found that a decrease of flow rate in the CMTHE results in degradation of heat extraction, ORC power generation and ORC system efficiency. On the contrary, increasing the flow rate in the CMTHE leads to a rise of heat extraction, ORC power generation and ORC system efficiency. Unlike that in case 1, the effect of flow rate has a detectable effect on the final states of heat extraction, ORC power generation, and ORC efficiency

    EVAPORATION OF QUARK DROPS DURING THE COSMOLOGICAL Q-H TRANSITION

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    We have carried out a study of the hydrodynamics of disconnected quark regions during the final stages of the cosmological quark-hadron transition. A set of relativistic Lagrangian equations is presented for following the evaporation of a single quark drop and results from the numerical solution of this are discussed. A self-similar solution is shown to exist and the formation of baryon number density inhomogeneities at the end of the drop contraction is discussed.Comment: 12 pages Phys. Rev. format, uuencoded postscript file including 12 figure

    Hadronic Charmed Meson Decays Involving Axial Vector Mesons

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    Cabibbo-allowed charmed meson decays into a pseudoscalar meson and an axial-vector meson are studied. The charm to axial-vector meson transition form factors are evaluated in the Isgur-Scora-Grinstein-Wise quark model. The dipole momentum dependence of the D→KD\to K transition form factor and the presence of a sizable long-distance WW-exchange are the two key ingredients for understanding the data of D→Kˉa1D\to \bar Ka_1. The K1A−K1BK_{1A}-K_{1B} mixing angle of the strange axial-vector mesons is found to be ≈±37∘\approx \pm37^\circ or ±58∘\pm58^\circ from τ→K1ντ\tau\to K_1\nu_\tau decays. The study of D→K1(1270)π,K1(1400)πD\to K_1(1270)\pi, K_1(1400)\pi decays excludes the positive mixing-angle solutions. It is pointed out that an observation of the decay D0→K1−(1400)π+D^0\to K_1^-(1400)\pi^+ at the level of 5×10−45\times 10^{-4} will rule out θ≈−37∘\theta\approx -37^\circ and favor the solution θ≈−58∘\theta\approx -58^\circ. Though the decays D0→Kˉ10π0D^0\to \bar K_1^0\pi^0 are color suppressed, they are comparable to and even larger than the color-allowed counterparts: Kˉ10(1270)π0∼K1−(1270)π+\bar K_1^0(1270)\pi^0\sim K_1^-(1270)\pi^+ and Kˉ10(1400)π0>K1−(1400)π+\bar K_1^0(1400)\pi^0> K_1^-(1400)\pi^+. The finite width effect of the axial-vector resonance is examined. It becomes important for a1(1260)a_1(1260) in particular when its width is near 600 MeV.Comment: 19 page

    Uniaxial Phase Transition in Si : Ab initio Calculations

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    Based on a previously proposed thermodynamic analysis, we study the relative stabilities of five Si phases under uniaxial compression using ab initio methods. The five phases are diamond, beta-tin, sh, sc, and hcp structures. The possible phase-transition patterns were investigated by considering the phase transitions between any two chosen phases of the five phases. By analyzing the different conributions to the relative pahse stability, we identified the most important factors in reducing the phase-transition pressures at uniaxial compression. We also show that it is possible to have phase transitions occur only when the phases are under uniaxial compression, in spite of no phase transition when under hydrostatic commpression. Taking all five phases into consideration, the phase diagram at uniaxial compression was constructed for pressures under 20 GPa. The stable phases were found to be diamond, beta-tin and sh structures, i.e. the same as those when under hydrostatic condition. According to the phase diagram, direct phase transition from the diamond to the sh phase is possible if the applied uniaxial pressures, on increasing, satisfy the condition of Px>Pz. Simiilarly, the sh-to-beta-tin transition on increeasing pressures is also possible if the applied uniaxial pressures are varied from the condition of Px>Pz, on which the phase of sh is stable, to that of Px<Pz, on which the beta-tin is stable
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