1,636 research outputs found

    Charge stripes due to electron correlations in the two-dimensional spinless Falicov-Kimball model

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    We calculate the restricted phase diagram for the Falicov-Kimball model on a two-dimensional square lattice. We consider the limit where the conduction electron density is equal to the localized electron density, which is the limit related to the S_z=0 states of the Hubbard model. After considering over 20,000 different candidate phases (with a unit cell of 16 sites or less) and their thermodynamic mixtures, we find only about 100 stable phases in the ground-state phase diagram. We analyze these phases to describe where stripe phases occur and relate these discoveries to the physics behind stripe formation in the Hubbard model.Comment: (34 pages, 9 figures, submitted to Journal of Statistical Physics to celebrate Elliott Lieb's 70th birthday

    How healthy is your communication?

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    Take your temperature with an effective thermometer… Maybe it\u27s time to take the temperature of your communication program

    Formalising the Continuous/Discrete Modeling Step

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    Formally capturing the transition from a continuous model to a discrete model is investigated using model based refinement techniques. A very simple model for stopping (eg. of a train) is developed in both the continuous and discrete domains. The difference between the two is quantified using generic results from ODE theory, and these estimates can be compared with the exact solutions. Such results do not fit well into a conventional model based refinement framework; however they can be accommodated into a model based retrenchment. The retrenchment is described, and the way it can interface to refinement development on both the continuous and discrete sides is outlined. The approach is compared to what can be achieved using hybrid systems techniques.Comment: In Proceedings Refine 2011, arXiv:1106.348

    Quantum Stability of (2+1)-Spacetimes with Non-Trivial Topology

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    Quantum fields are investigated in the (2+1)-open-universes with non-trivial topologies by the method of images. The universes are locally de Sitter spacetime and anti-de Sitter spacetime. In the present article we study spacetimes whose spatial topologies are a torus with a cusp and a sphere with three cusps as a step toward the more general case. A quantum energy momentum tensor is obtained by the point stripping method. Though the cusps are no singularities, the latter cusps cause the divergence of the quantum field. This suggests that only the latter cusps are quantum mechanically unstable. Of course at the singularity of the background spacetime the quantum field diverges. Also the possibility of the divergence of topological effect by a negative spatial curvature is discussed. Since the volume of the negatively curved space is larger than that of the flat space, one see so many images of a single source by the non-trivial topology. It is confirmed that this divergence does not appear in our models of topologies. The results will be applicable to the case of three dimensional multi black hole\cite{BR}.Comment: 17 pages, revtex, 3 uuencoded figures containe

    Infinite partition monoids

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    Let PX\mathcal P_X and SX\mathcal S_X be the partition monoid and symmetric group on an infinite set XX. We show that PX\mathcal P_X may be generated by SX\mathcal S_X together with two (but no fewer) additional partitions, and we classify the pairs α,βPX\alpha,\beta\in\mathcal P_X for which PX\mathcal P_X is generated by SX{α,β}\mathcal S_X\cup\{\alpha,\beta\}. We also show that PX\mathcal P_X may be generated by the set EX\mathcal E_X of all idempotent partitions together with two (but no fewer) additional partitions. In fact, PX\mathcal P_X is generated by EX{α,β}\mathcal E_X\cup\{\alpha,\beta\} if and only if it is generated by EXSX{α,β}\mathcal E_X\cup\mathcal S_X\cup\{\alpha,\beta\}. We also classify the pairs α,βPX\alpha,\beta\in\mathcal P_X for which PX\mathcal P_X is generated by EX{α,β}\mathcal E_X\cup\{\alpha,\beta\}. Among other results, we show that any countable subset of PX\mathcal P_X is contained in a 44-generated subsemigroup of PX\mathcal P_X, and that the length function on PX\mathcal P_X is bounded with respect to any generating set

    On aspects of self-consistency in the Dyson-Schwinger approach to QED and \lambda (\phi^\star \phi)^2 theories

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    We investigate some aspects of the self-consistency in the Dyson-Schwinger approach to both the QED and the self-interacting scalar field theories. We prove that the set of the Dyson-Schwinger equations, together with the Green-Ward-Takahashi identity, is equivalent to the analogous set of integral equations studied in condensed matter, namely many-body perturbation theory, where it is solved self-consistently and iteratively. In this framework, we compute the non-perturbative solution of the gap equation for the self-interacting scalar field theory.Comment: 9 pages, to appear on Phys. Rev.

    Quantum Complex Scalar Field in the Two-Dimensional Spacetime with Closed Timelike Curves and a Time-Machine Problem

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    It is considered the quantum complex scalar field which obeys the authomorphic condition in the two-dimensional spacetime with closed timelike curves and the chronology horizon. The renormalized stress-energy tensor is obtained. It is shown that the value of the stress-energy tensor is regular at the chronology horizon for specific authomorphic parameters. Thus the particular example of field configuration is given for which the Hawking's chronology protection conjecture is violated.Comment: 21(Latex)Postscript file of the figure may be received from author, CQG-94-100

    Divergences in the Effective Action for Acausal Spacetimes

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    The 1--loop effective Lagrangian for a massive scalar field on an arbitrary causality violating spacetime is calculated using the methods of Euclidean quantum field theory in curved spacetime. Fields of spin 1/2, spin 1 and twisted field configurations are also considered. In general, we find that the Lagrangian diverges to minus infinity at each of the nth polarised hypersurfaces of the spacetime with a structure governed by a DeWitt-Schwinger type expansion.Comment: 17 pages, Late
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