1,917 research outputs found

    Before sailing on a domain-wall sea

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    We discuss the very different roles of the valence-quark and the sea-quark residual masses (mresvm_{res}^v and mressm_{res}^s) in dynamical domain-wall fermions simulations. Focusing on matrix elements of the effective weak hamiltonian containing a power divergence, we find that mresvm_{res}^v can be a source of a much bigger systematic error. To keep all systematic errors due to residual masses at the 1% level, we estimate that one needs amress≤10−3a m_{res}^s \le 10^{-3} and amresv≤10−5a m_{res}^v \le 10^{-5}, at a lattice spacing a∼0.1a\sim 0.1 fm. The practical implications are that (1) optimal use of computer resources calls for a mixed scheme with different domain-wall fermion actions for the valence and sea quarks; (2) better domain-wall fermion actions are needed for both the sea and the valence sectors.Comment: latex, 25 pages. Improved discussion in appendix, including correction of some technical mistakes; ref. adde

    Chiral Fermions on the Lattice through Gauge Fixing -- Perturbation Theory

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    We study the gauge-fixing approach to the construction of lattice chiral gauge theories in one-loop weak-coupling perturbation theory. We show how infrared properties of the gauge degrees of freedom determine the nature of the continuous phase transition at which we take the continuum limit. The fermion self-energy and the vacuum polarization are calculated, and confirm that, in the abelian case, this approach can be used to put chiral gauge theories on the lattice in four dimensions. We comment on the generalization to the nonabelian case.Comment: 31 pages, 5 figures, two refs. adde

    A simple derivation of the Overlap Dirac Operator

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    We derive the vector-like four dimensional overlap Dirac operator starting from a five dimensional Dirac action in the presence of a delta-function space-time defect. The effective operator is obtained by first integrating out all the fermionic modes in the fixed gauge background, and then identifying the contribution from the localized modes as the determinant of an operator in one dimension less. We define physically relevant degrees of freedom on the defect by introducing an auxiliary defect-bound fermion field and integrating out the original five dimensional bulk field.Comment: 9 pages, LaTe

    Existence of Wormholes in f(G)f(\mathcal{G}) Gravity using Symmetries

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    The current study examines the geometry of static wormholes with anisotropic matter distribution in context of modified f(G)f(\mathcal{G}) gravity. We consider the well known Noether and conformal symmetries, which help in investigating wormholes in f(G)f(\mathcal{G}) gravity. For this purpose, we develop symmetry generators associated with conserved quantities by taking into consideration the f(G)f(\mathcal{G}) gravity model. Moreover, we use the conservation relationship gained from the classical Noether method and conformal Killing symmetries to develop the metric potential. These symmetries provide a strong mathematical background to investigate wormhole solutions by incorporating some suitable initial conditions. The obtained conserved quantity performs a significant role in defining the essential physical characteristics of the shape-function and energy conditions. Further, we also describe the stability of obtained wormholes solutions by employing the equilibrium condition in modified f(G)f(\mathcal{G}) gravity. It is observed from graphical representation of obtained wormhole solutions that Noether and conformal Killing symmetries provide the results with physically accepted patterns.Comment: 10 pages, 7 figure

    f(G,T)f(\mathcal{G},\mathrm{\textit{T}}) Gravity Bouncing Universe with Cosmological Parameters

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    In recent few years, the Gauss-Bonnet f(G,T)f(\mathcal{G},\mathrm{\textit{T}}) theory of gravity has fascinated considerable researchers owing to its coupling of trace of the stress-energy tensor TT with the Gauss-Bonnet term G\mathcal{G}. In this context, we focuss ourselves to study bouncing universe with in f(G,T)f(\mathcal{G},\mathrm{\textit{T}}) gravity background. Some important preliminaries are presented along with the discussion of cosmological parameters to develop a minimal background about f(G,T)f(\mathcal{G},\mathrm{\textit{T}}) theory of gravity. The exact bouncing solutions with physical analysis are provided with the choice of two equation of state parameters. It is shown that the results do agree with the present values of deceleration, jerk and snap parameters. Moreover, it is concluded that the model parameters are quite important for the validity of conservation equation (as the matter coupled theories do not obey the usual conservation law).Comment: 12 pages, 10 figure

    Running coupling and mass anomalous dimension of SU(3) gauge theory with two flavors of symmetric-representation fermions

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    We have measured the running coupling constant of SU(3) gauge theory coupled to Nf=2 flavors of symmetric representation fermions, using the Schrodinger functional scheme. Our lattice action is defined with hypercubic smeared links which, along with the larger lattice sizes, bring us closer to the continuum limit than in our previous study. We observe that the coupling runs more slowly than predicted by asymptotic freedom, but we are unable to observe fixed point behavior before encountering a first order transition to a strong coupling phase. This indicates that the infrared fixed point found with the thin-link action is a lattice artifact. The slow running of the gauge coupling permits an accurate determination of the mass anomalous dimension for this theory, which we observe to be small, gamma_m < 0.6, over the range of couplings we can reach. We also study the bulk and finite-temperature phase transitions in the strong coupling region.Comment: 17 pages, 16 figures. Substantial modifications to explain why the fat-link result for the beta function supersedes our thin-link result; also updated the phase diagram to reflect additional numerical work. Added references. Final versio

    Toward 'socially constructive' social constructions of leadership

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    In their introductory editorial essay for this special issue, David Grant and Gail Fairhurst have done us a great service by valiantly producing a "Sailing Guide" to the Social Construction of Leadership (Fairhurst & Grant, 2010). As with rounding the Capes, this is not a task for the faint of heart. A sailing guide is designed to provide vital knowledge about a particular sea or coast, providing us with charts, warnings about potential hazards and an indication where we might find safe havens in a storm. Their sailing guide does this to great effect as it skilfully "boxes the compass" by revealing all of the potential directions that one might set one‟s sail by if one was sufficiently foolhardy to embark on a cruise of the social construction of leadership

    The Phase Diagram and Spectrum of Gauge-Fixed Abelian Lattice Gauge Theory

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    We consider a lattice discretization of a covariantly gauge-fixed abelian gauge theory. The gauge fixing is part of the action defining the theory, and we study the phase diagram in detail. As there is no BRST symmetry on the lattice, counterterms are needed, and we construct those explicitly. We show that the proper adjustment of these counterterms drives the theory to a new type of phase transition, at which we recover a continuum theory of (free) photons. We present both numerical and (one-loop) perturbative results, and show that they are in good agreement near this phase transition. Since perturbation theory plays an important role, it is important to choose a discretization of the gauge-fixing action such that lattice perturbation theory is valid. Indeed, we find numerical evidence that lattice actions not satisfying this requirement do not lead to the desired continuum limit. While we do not consider fermions here, we argue that our results, in combination with previous work, provide very strong evidence that this new phase transition can be used to define abelian lattice chiral gauge theories.Comment: 42 pages, 30 figure
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