1,432 research outputs found

    Spectral Properties of the Ruelle Operator for Product Type Potentials on Shift Spaces

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    We study a class of potentials ff on one sided full shift spaces over finite or countable alphabets, called potentials of product type. We obtain explicit formulae for the leading eigenvalue, the eigenfunction (which may be discontinuous) and the eigenmeasure of the Ruelle operator. The uniqueness property of these quantities is also discussed and it is shown that there always exists a Bernoulli equilibrium state even if ff does not satisfy Bowen's condition. We apply these results to potentials f:{−1,1}N→Rf:\{-1,1\}^\mathbb{N} \to \mathbb{R} of the form f(x1,x2,…)=x1+2−γ x2+3−γ x3+...+n−γ xn+… f(x_1,x_2,\ldots) = x_1 + 2^{-\gamma} \, x_2 + 3^{-\gamma} \, x_3 + ...+n^{-\gamma} \, x_n + \ldots with γ>1\gamma >1. For 3/2<γ≤23/2 < \gamma \leq 2, we obtain the existence of two different eigenfunctions. Both functions are (locally) unbounded and exist a.s. (but not everywhere) with respect to the eigenmeasure and the measure of maximal entropy, respectively.Comment: To appear in the Journal of London Mathematical Societ

    The Thermal Environment of the Fiber Glass Dome for the New Solar Telescope at Big Bear Solar Observatory

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    The New Solar Telescope (NST) is a 1.6-meter off-axis Gregory-type telescope with an equatorial mount and an open optical support structure. To mitigate the temperature fluctuations along the exposed optical path, the effects of local/dome-related seeing have to be minimized. To accomplish this, NST will be housed in a 5/8-sphere fiberglass dome that is outfitted with 14 active vents evenly spaced around its perimeter. The 14 vents house louvers that open and close independently of one another to regulate and direct the passage of air through the dome. In January 2006, 16 thermal probes were installed throughout the dome and the temperature distribution was measured. The measurements confirmed the existence of a strong thermal gradient on the order of 5 degree Celsius inside the dome. In December 2006, a second set of temperature measurements were made using different louver configurations. In this study, we present the results of these measurements along with their integration into the thermal control system (ThCS) and the overall telescope control system (TCS).Comment: 12 pages, 11 figures, submitted to SPIE Optics+Photonics, San Diego, U.S.A., 26-30 August 2007, Conference: Solar Physics and Space Weather Instrumentation II, Proceedings of SPIE Volume 6689, Paper #2

    Two-Dimensional Spectroscopy of Photospheric Shear Flows in a Small delta Spot

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    In recent high-resolution observations of complex active regions, long-lasting and well-defined regions of strong flows were identified in major flares and associated with bright kernels of visible, near-infrared, and X-ray radiation. These flows, which occurred in the proximity of the magnetic neutral line, significantly contributed to the generation of magnetic shear. Signatures of these shear flows are strongly curved penumbral filaments, which are almost tangential to sunspot umbrae rather than exhibiting the typical radial filamentary structure. Solar active region NOAA 10756 was a moderately complex, beta-delta sunspot group, which provided an opportunity to extend previous studies of such shear flows to quieter settings. We conclude that shear flows are a common phenomenon in complex active regions and delta spots. However, they are not necessarily a prerequisite condition for flaring. Indeed, in the present observations, the photospheric shear flows along the magnetic neutral line are not related to any change of the local magnetic shear. We present high-resolution observations of NOAA 10756 obtained with the 65-cm vacuum reflector at Big Bear Solar Observatory (BBSO). Time series of speckle-reconstructed white-light images and two-dimensional spectroscopic data were combined to study the temporal evolution of the three-dimensional vector flow field in the beta-delta sunspot group. An hour-long data set of consistent high quality was obtained, which had a cadence of better than 30 seconds and sub-arcsecond spatial resolution.Comment: 23 pages, 6 gray-scale figures, 4 color figures, 2 tables, submitted to Solar Physic

    Limit theorems for von Mises statistics of a measure preserving transformation

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    For a measure preserving transformation TT of a probability space (X,F,μ)(X,\mathcal F,\mu) we investigate almost sure and distributional convergence of random variables of the form x→1Cn∑i1<n,...,id<nf(Ti1x,...,Tidx), n=1,2,...,x \to \frac{1}{C_n} \sum_{i_1<n,...,i_d<n} f(T^{i_1}x,...,T^{i_d}x),\, n=1,2,..., where ff (called the \emph{kernel}) is a function from XdX^d to R\R and C1,C2,...C_1, C_2,... are appropriate normalizing constants. We observe that the above random variables are well defined and belong to Lr(μ)L_r(\mu) provided that the kernel is chosen from the projective tensor product Lp(X1,F1,μ1)⊗π...⊗πLp(Xd,Fd,μd)⊂Lp(μd)L_p(X_1,\mathcal F_1, \mu_1) \otimes_{\pi}...\otimes_{\pi} L_p(X_d,\mathcal F_d, \mu_d)\subset L_p(\mu^d) with p=d r, r ∈[1,∞).p=d\,r,\, r\ \in [1, \infty). We establish a form of the individual ergodic theorem for such sequences. Next, we give a martingale approximation argument to derive a central limit theorem in the non-degenerate case (in the sense of the classical Hoeffding's decomposition). Furthermore, for d=2d=2 and a wide class of canonical kernels ff we also show that the convergence holds in distribution towards a quadratic form ∑m=1∞λmηm2\sum_{m=1}^{\infty} \lambda_m\eta^2_m in independent standard Gaussian variables η1,η2,...\eta_1, \eta_2,.... Our results on the distributional convergence use a TT--\,invariant filtration as a prerequisite and are derived from uni- and multivariate martingale approximations

    A Phase I/II first-line study of R-CHOP plus B-cell receptor/NF-κB-double-targeting to molecularly assess therapy response

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    The ImbruVeRCHOP trial is an investigator-initiated, multicenter, single-arm, open label Phase I/II study for patients 61-80 years of age with newly diagnosed CD20+ diffuse large B-cell lymphoma and a higher risk profile (International Prognostic Index ≥2). Patients receive standard chemotherapy (CHOP) plus immunotherapy (Rituximab), a biological agent (the proteasome inhibitor Bortezomib) and a signaling inhibitor (the Bruton's Tyrosine Kinase-targeting therapeutic Ibrutinib). Using an all-comers approach, but subjecting patients to another lymphoma biopsy acutely under first-cycle immune-chemo drug exposure, ImbruVeRCHOP seeks to identify an unbiased molecular responder signature that marks diffuse large B-cell lymphoma patients at risk and likely to benefit from this regimen as a double, proximal and distal B-cell receptor/NF-κB-co-targeting extension of the current R-CHOP standard of care. EudraCT-Number: 2015-003429-32; ClinicalTrials.gov identifier: NCT03129828

    Finite type approximations of Gibbs measures on sofic subshifts

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    Consider a H\"older continuous potential ϕ\phi defined on the full shift A^\nn, where AA is a finite alphabet. Let X\subset A^\nn be a specified sofic subshift. It is well-known that there is a unique Gibbs measure μϕ\mu_\phi on XX associated to ϕ\phi. Besides, there is a natural nested sequence of subshifts of finite type (Xm)(X_m) converging to the sofic subshift XX. To this sequence we can associate a sequence of Gibbs measures (μϕm)(\mu_{\phi}^m). In this paper, we prove that these measures weakly converge at exponential speed to μϕ\mu_\phi (in the classical distance metrizing weak topology). We also establish a strong mixing property (ensuring weak Bernoullicity) of μϕ\mu_\phi. Finally, we prove that the measure-theoretic entropy of μϕm\mu_\phi^m converges to the one of μϕ\mu_\phi exponentially fast. We indicate how to extend our results to more general subshifts and potentials. We stress that we use basic algebraic tools (contractive properties of iterated matrices) and symbolic dynamics.Comment: 18 pages, no figure
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