15 research outputs found

    Intrinsic ergodicity beyond specification: beta-shifts, S-gap shifts, and their factors

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    We give sufficient conditions for a shift space (Σ,σ)(\Sigma,\sigma) to be intrinsically ergodic, along with sufficient conditions for every subshift factor of Σ\Sigma to be intrinsically ergodic. As an application, we show that every subshift factor of a β\beta-shift is intrinsically ergodic, which answers an open question included in Mike Boyle's article "Open problems in symbolic dynamics". We obtain the same result for SS-gap shifts, and describe an application of our conditions to more general coded systems. One novelty of our approach is the introduction of a new version of the specification property that is well adapted to the study of symbolic spaces with a non-uniform structure.Comment: 27 pages, 1 figure, minor changes based on referee's suggestions, in v.3 the result on coded systems has been moved to the introduction, resulting in small changes to numbering (lettering) of result

    Single π0\pi^0 Production Off Neutrons Bound in Deuteron with Linearly Polarized Photons

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    The quasifree γdπ0n(p)\overrightarrow{\gamma} d\to\pi^0n(p) photon beam asymmetry, Σ\Sigma, has been measured at photon energies, EγE_\gamma, from 390 to 610 MeV, corresponding to center of mass energy from 1.271 to 1.424 GeV, for the first time. The data were collected in the A2 hall of the MAMI electron beam facility with the Crystal Ball and TAPS calorimeters covering pion center-of-mass angles from 49 to 148^\circ. In this kinematic region, polarization observables are sensitive to contributions from the Δ(1232)\Delta (1232) and N(1440)N(1440) resonances. The extracted values of Σ\Sigma have been compared to predictions based on partial-wave analyses (PWAs) of the existing pion photoproduction database. Our comparison includes the SAID, MAID, and Bonn-Gatchina analyses; while a revised SAID fit, including the new Σ\Sigma measurements, has also been performed. In addition, isospin symmetry is examined as a way to predict π0n\pi^0n photoproduction observables, based on fits to published data in the channels π0p\pi^0p, π+n\pi^+n, and πp\pi^-p.Comment: 11 pages, 9 figures, 5 tables; fixed 2 glitche

    Radar return from vehicles in the ionosphere.

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