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S. Motta - One of the best experts on this subject based on the ideXlab platform.

  • Polynomial Approximation of the lense thirring rigid precession frequency
    Monthly Notices of the Royal Astronomical Society, 2018
    Co-Authors: Vittorio De Falco, S. Motta
    Abstract:

    We propose a Polynomial Approximation of the global Lense-Thirring rigid precession frequency to study low frequency quasi-periodic oscillations around spinning black holes. This high-performing Approximation allows to determine the expected frequencies of a precessing thick accretion disc with fixed inner radius and variable outer radius around a black hole with given mass and spin. We discuss the accuracy and the applicability regions of our Polynomial Approximation, showing that the computational times are reduced by a factor of $\approx70$ in the range of minutes.

  • Polynomial Approximation of the Lense–Thirring rigid precession frequency
    Monthly Notices of the Royal Astronomical Society, 2018
    Co-Authors: Vittorio De Falco, S. Motta
    Abstract:

    We propose a Polynomial Approximation of the global Lense-Thirring rigid precession frequency to study low frequency quasi-periodic oscillations around spinning black holes. This high-performing Approximation allows to determine the expected frequencies of a precessing thick accretion disc with fixed inner radius and variable outer radius around a black hole with given mass and spin. We discuss the accuracy and the applicability regions of our Polynomial Approximation, showing that the computational times are reduced by a factor of $\approx70$ in the range of minutes.

Vittorio De Falco - One of the best experts on this subject based on the ideXlab platform.

  • Polynomial Approximation of the lense thirring rigid precession frequency
    Monthly Notices of the Royal Astronomical Society, 2018
    Co-Authors: Vittorio De Falco, S. Motta
    Abstract:

    We propose a Polynomial Approximation of the global Lense-Thirring rigid precession frequency to study low frequency quasi-periodic oscillations around spinning black holes. This high-performing Approximation allows to determine the expected frequencies of a precessing thick accretion disc with fixed inner radius and variable outer radius around a black hole with given mass and spin. We discuss the accuracy and the applicability regions of our Polynomial Approximation, showing that the computational times are reduced by a factor of $\approx70$ in the range of minutes.

  • Polynomial Approximation of the Lense–Thirring rigid precession frequency
    Monthly Notices of the Royal Astronomical Society, 2018
    Co-Authors: Vittorio De Falco, S. Motta
    Abstract:

    We propose a Polynomial Approximation of the global Lense-Thirring rigid precession frequency to study low frequency quasi-periodic oscillations around spinning black holes. This high-performing Approximation allows to determine the expected frequencies of a precessing thick accretion disc with fixed inner radius and variable outer radius around a black hole with given mass and spin. We discuss the accuracy and the applicability regions of our Polynomial Approximation, showing that the computational times are reduced by a factor of $\approx70$ in the range of minutes.

Pencho Petrushev - One of the best experts on this subject based on the ideXlab platform.

  • nonlinear piecewise Polynomial Approximation beyond besov spaces
    Applied and Computational Harmonic Analysis, 2003
    Co-Authors: Borislav Karaivanov, Pencho Petrushev
    Abstract:

    Abstract We study nonlinear n-term Approximation in L p ( R 2 ) (0 R 2 which allow arbitrarily sharp angles. To characterize the rate of Approximation we introduce and develop three families of smoothness spaces generated by multilevel nested triangulations. We call them B-spaces because they can be viewed as generalizations of Besov spaces. We use the B-spaces to prove Jackson and Bernstein estimates for n-term piecewise Polynomial Approximation and consequently characterize the corresponding Approximation spaces by interpolation. We also develop methods for n-term piecewise Polynomial Approximation which capture the rates of the best Approximation.

  • multivariate n term rational and piecewise Polynomial Approximation
    Journal of Approximation Theory, 2003
    Co-Authors: Pencho Petrushev
    Abstract:

    We study nonlinear Approximation in Lp(Rd) (0 1) from (a) n-term rational functions, and (b) piecewise Polynomials generated by different anisotropic dyadic partitions of Rd. To characterize the rates of each such piecewise Polynomial Approximation we introduce a family of smoothness spaces (B-spaces) which can be viewed as an anisotropic variation of Besov spaces. We use the B-spaces to prove Jackson and Bernstein estimates and then characterize the piecewise Polynomial Approximation by interpolation. Our main estimate relates n-term rational Approximation with piecewise Polynomial Approximation in Lp(Rd). This result enables us to obtain a direct estimate for n-term rational Approximation in terms of a minimal B-norm (over all dyadic partitions). We also show that the Haar bases associated with anisotropic dyadic partitions of Rd can be successfully utilized for nonlinear Approximation. We give an effective algorithm for best Haar basis or best B-space selection.

Yoshihito Kazashi - One of the best experts on this subject based on the ideXlab platform.

Pradip Sircar - One of the best experts on this subject based on the ideXlab platform.