86,177 research outputs found

    The Cosmological Constant Problem and Re-interpretation of Time

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    We abandon the interpretation that time is a global parameter in quantum mechanics, replace it by a quantum dynamical variable playing the role of time. This operational re-interpretation of time provides a solution to the cosmological constant problem. The expectation value of the zero-point energy under the new time variable vanishes. The fluctuation of the vacuum energy as the leading contribution to the gravitational effect gives a correct order to the observed "dark energy". The "dark energy" as a mirage is always seen comparable with the matter energy density by an observer using the internal clock time. Conceptual consequences of the re-interpretation of time are also discussed.Comment: 9 pages, no figure; v3: improved discussion on remote simultaneity; v4: improved discussion on coincidence problem, reproduced Einstein theory of gravity from quantum reference frame, typos corrected, updated to the final version published in Nuclear Physics

    Dark Energy from Quantum Uncertainty of Distant Clock

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    The observed cosmic acceleration was attributed to an exotic dark energy in the framework of classical general relativity. The dark energy behaves very similar with vacuum energy in quantum mechanics. However, once the quantum effects are seriously taken into account, it predicts a completely wrong result and leads to a severe fine-tuning. To solve the problem, the exact meaning of time in quantum mechanics is reexamined. We abandon the standard interpretation of time in quantum mechanics that time is just a global parameter, replace it by a quantum dynamical variable playing the role of physical clock. We find that synchronization of two spatially separated clocks can not be precisely realized at quantum level. There is an intrinsic quantum uncertainty of distant clock time, which implies an apparent vacuum energy fluctuation and gives an observed dark energy density ρde=6πLP2LH2\rho_{de}=\frac{6}{\pi}L_{P}^{-2}L_{H}^{-2} at tree level approximation, where LPL_{P} and LHL_{H} are the Planck and Hubble scale cutoffs. The fraction of the dark energy is given by Ωde=2π\Omega_{de}=\frac{2}{\pi}, which does not evolve with the internal clock time. The "dark energy" as a quantum cosmic variance is always seen comparable with the matter energy density by an observer using the internal clock time. The corrected distance-redshift relation of cosmic observations due to the distant clock effect are also discussed, which again gives a redshift independent fraction Ωde=2π\Omega_{de}=\frac{2}{\pi}. The theory is consistent with current cosmic observations.Comment: 7 pages, no figure; v2:added discussion on distance-redshift relation; v3:improved discussion on distance-redshift relation, an independent calculation to the redshift variance over redshift squared is given, dark energy fraction agrees with 2/pi; v4:typos corrected, updated to the final version published in Journal of High Energy Physics, Volume 2015, Issue

    Two-loop Renormalization Group Equations in General Gauge Field Theories

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    The complete set of two-loop renormalization group equations in general gauge field theories is presented. This includes the \beta functions of parameters with and without a mass dimension

    Dynamics of conduction blocks in a model of paced cardiac tissue

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    We study numerically the dynamics of conduction blocks using a detailed electrophysiological model. We find that this dynamics depends critically on the size of the paced region. Small pacing regions lead to stationary conduction blocks while larger pacing regions can lead to conduction blocks that travel periodically towards the pacing region. We show that this size-dependence dynamics can lead to a novel arrhythmogenic mechanism. Furthermore, we show that the essential phenomena can be captured in a much simpler coupled-map model.Comment: 8 pages 6 figure

    Probing the QCD Critical Point with Higher Moments of Net-proton Multiplicity Distributions

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    Higher moments of event-by-event net-proton multiplicity distributions are applied to search for the QCD critical point in the heavy ion collisions. It has been demonstrated that higher moments as well as moment products are sensitive to the correlation length and directly connected to the thermodynamic susceptibilities computed in the Lattice QCD and Hadron Resonance Gas (HRG) model. In this paper, we will present measurements for kurtosis (κ\kappa), skewness (SS) and variance (σ2\sigma^{2}) of net-proton multiplicity distributions at the mid-rapidity (y<0.5|y|<0.5) and 0.4<pT<0.80.4<p_{T}<0.8 GeV/cc for Au+Au collisions at sNN\sqrt{s_{NN}}=19.6, 39, 62.4, 130 and 200 GeV, Cu+Cu collisions at sNN\sqrt{s_{NN}}=22.4, 62.4 and 200 GeV, d+Au collisions at sNN\sqrt{s_{NN}}=200 GeV and p+p collisions at sNN\sqrt{s_{NN}}=62.4 and 200 GeV. The moment products κσ2\kappa \sigma^{2} and SσS \sigma of net-proton distributions, which are related to volume independent baryon number susceptibility ratio, are compared to the Lattice QCD and HRG model calculations. The κσ2\kappa \sigma^{2} and SσS \sigma of net-proton distributions are consistent with Lattice QCD and HRG model calculations at high energy, which support the thermalization of the colliding system. Deviations of κσ2\kappa \sigma^{2} and SσS \sigma for the Au+Au collisions at low energies from HRG model calculations are also observed.Comment: 10 pages, 8 figures, Proceedings of 27th Winter Workshon on Nuclear Dynamics. Feb. 6-13 (2011
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