PaperPanorama

Nuclear Theory·nucl-th

Monday·March 12, 2018

4 papers2 primary·2 cross-listed

  1. 03

    [Submitted on 8 Mar 2018] (cross-list from physics.comp-ph)

    A reciprocal formulation of non-exponential radiative transfer. 1: Sketch and motivation

    Eugene d'Eon

    Previous proposals to permit non-exponential free-path statistics in radiative transfer have not included support for volume and boundary sources that are spatially uncorrelated from the scattering events in the medium. Birth-collision free paths are treated identically to collision-collision free paths and application of this to general, bounded scenes with inclusions leads to non-reciprocal transport. Beginning with reciprocity as a desired property, we propose a new way to integrate non-exponential transport theory into general scenes. We distinguish between the free-path-length statistics between correlated medium particles and the free-path-length statistics beginning at locations not correlated to medium particles, such as boundary surfaces, inclusions and uncorrelated sources. Reciprocity requires that the uncorrelated free-path distributions are simply the normalized transmittance of the correlated free-path distributions. The combination leads to an equilibrium imbedding of a previously derived generalized transport equation into bounded domains. We compare predictions of this approach to Monte Carlo simulation of multiple scattering from negatively-correlated suspensions of monodispersive hard spheres in bounded two-dimensional domains and demonstrate improved performance relative to previous work. We also derive new, exact, reciprocal, single-scattering solutions for plane-parallel half-spaces over a variety of non-exponential media types.

    Comments:
    16 pages, addressed reviewer comments
    Subjects:
    Computational Physics (physics.comp-ph); cs.GR (cs.GR); Nuclear Theory (nucl-th)
    arXiv:
    1803.03259 [pdf]
    1 citation
  2. 04

    [Submitted on 8 Mar 2018] (cross-list from quant-ph)

    Quantum-Classical Computation of Schwinger Model Dynamics using Quantum Computers

    N. Klco🇺🇸 · E. F. Dumitrescu🇺🇸 · A. J. McCaskey🇺🇸 · T. D. Morris🇺🇸 · R. C. Pooser🇺🇸 · M. Sanz🇪🇸 · E. Solano🇪🇸 · P. Lougovski🇺🇸 · M. J. Savage🇺🇸

    We present a quantum-classical algorithm to study the dynamics of the two-spatial-site Schwinger model on IBM's quantum computers. Using rotational symmetries, total charge, and parity, the number of qubits needed to perform computation is reduced by a factor of , removing exponentially-large unphysical sectors from the Hilbert space. Our work opens an avenue for exploration of other lattice quantum field theories, such as quantum chromodynamics, where classical computation is used to find symmetry sectors in which the quantum computer evaluates the dynamics of quantum fluctuations.

    Comments:
    5 pages, 4 figures, 23 pages supplemental, 8 figures supplemental
    Subjects:
    Quantum Physics (quant-ph); High Energy Physics — Lattice (hep-lat); High Energy Physics — Phenomenology (hep-ph); High Energy Physics — Theory (hep-th); Nuclear Theory (nucl-th)
    arXiv:
    1803.03326 [pdf]
    PRA(2018)·515 citations

Affiliations

first authorsco-authorsvia INSPIRE