Variational Calculus

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Delfim F. M. Torres - One of the best experts on this subject based on the ideXlab platform.

  • a survey on fractional Variational Calculus
    arXiv: Optimization and Control, 2018
    Co-Authors: Ricardo Almeida, Delfim F. M. Torres
    Abstract:

    Main results and techniques of the fractional Calculus of variations are surveyed. We consider Variational problems containing Caputo derivatives and study them using both indirect and direct methods. In particular, we provide necessary optimality conditions of Euler-Lagrange type for the fundamental, higher-order, and isoperimetric problems, and compute approximated solutions based on truncated Grunwald--Letnikov approximations of Caputo derivatives.

  • hahn s symmetric quantum Variational Calculus
    Numerical Algebra Control and Optimization, 2013
    Co-Authors: Artur Brito M C Da Cruz, Natalia Martins, Delfim F. M. Torres
    Abstract:

    We introduce and develop the Hahn symmetric quantum Calculus with applications to the Calculus of variations. Namely, we obtain a necessary optimality condition of Euler--Lagrange type and a sufficient optimality condition for Variational problems within the context of Hahn's symmetric Calculus. Moreover, we show the effectiveness of Leitmann's direct method when applied to Hahn's symmetric Variational Calculus. Illustrative examples are provided.

  • variable order fractional Variational Calculus for double integrals
    Conference on Decision and Control, 2012
    Co-Authors: Tatiana Odzijewicz, Agnieszka B Malinowska, Delfim F. M. Torres
    Abstract:

    We introduce three types of partial fractional operators of variable order. An integration by parts formula for partial fractional integrals of variable order and an extension of Green's theorem are proved. These results allow us to obtain a fractional Euler-Lagrange necessary optimality condition for variable order two-dimensional fractional Variational problems.

  • higher order hahn s quantum Variational Calculus
    Nonlinear Analysis-theory Methods & Applications, 2012
    Co-Authors: Artur Brito M C Da Cruz, Natalia Martins, Delfim F. M. Torres
    Abstract:

    Abstract We prove a necessary optimality condition of Euler–Lagrange type for quantum Variational problems involving Hahn’s derivatives of higher-order.

  • Fractional Variational Calculus with Classical and Combined Caputo Derivatives
    Nonlinear Analysis: Theory Methods and Applications, 2012
    Co-Authors: Tatiana Odzijewicz, Agnieszka B Malinowska, Delfim F. M. Torres
    Abstract:

    We give a proper fractional extension of the classical Calculus of variations by considering Variational functionals with a Lagrangian depending on a combined Caputo fractional derivative and the classical derivative. Euler-Lagrange equations to the basic and isoperimetric problems are proved, as well as transversality conditions.

X Hernandez - One of the best experts on this subject based on the ideXlab platform.

  • deriving star formation histories inverting hertzsprung russell diagrams through a Variational Calculus maximum likelihood method
    Monthly Notices of the Royal Astronomical Society, 1999
    Co-Authors: X Hernandez, D Vallsgabaud, Gerard Gilmore
    Abstract:

    We introduce a new method for solving maximum likelihood problems through Variational Calculus, and apply it to the case of recovering an unknown star formation history, SFR(t), from the resulting Hertzsprung--Russell (HR) diagram. This approach allows a totally non-parametric solution, which has the advantage of requiring no initial assumptions about SFR(t). As a full maximum likelihood statistical model is used, and we take advantage of all the information available in the HR diagram, rather than concentrating on particular features such as turn-off points or luminosity functions. We test the method using a series of synthetic HR diagrams produced from known SFR(t), and find it to be quite successful under noise conditions comparable to those present in current observations. At this point we restrict the analysis to situations in which the metallicity of the system is known, as is the case with the resolved population of dwarf spheroidal companions to the Milky Way or the solar neighbourhood Hipparcos data. We also include tests to quantify the way uncertainties in the assumed metallicity, binary fraction and initial mass function (IMF) affect our inferences.

  • deriving star formation histories inverting hr diagrams through a Variational Calculus maximum likelihood method
    arXiv: Astrophysics, 1998
    Co-Authors: X Hernandez, D Vallsgabaud, Gerard Gilmore
    Abstract:

    We introduce a new method for solving maximum likelihood problems through Variational Calculus, and apply it to the case of recovering an unknown star formation history, $SFR(t)$, from a resulting HR diagram. This approach allows a totally non-parametric solution which has the advantage of requiring no initial assumptions on the $SFR(t)$. As a full maximum likelihood statistical model is used, we take advantage of all the information available in the HR diagram, rather than concentrating on particular features such as turn off points or luminosity functions. We test the method using a series of synthetic HR diagrams produced from known $SFR(t)$, and find it to be quite successful under noise conditions comparable to those present in current observations. At this point we restrict the analysis to situations where the metallicity of the system is known, as is the case with the resolved populations of the dwarf spheroidal companions to the Milky Way or the solar neighbourhood Hipparcos data. We also include tests to quantify the way uncertainties in the assumed metallicity, binary fraction and IMF affect our inferences.

Gerard Gilmore - One of the best experts on this subject based on the ideXlab platform.

  • deriving star formation histories inverting hertzsprung russell diagrams through a Variational Calculus maximum likelihood method
    Monthly Notices of the Royal Astronomical Society, 1999
    Co-Authors: X Hernandez, D Vallsgabaud, Gerard Gilmore
    Abstract:

    We introduce a new method for solving maximum likelihood problems through Variational Calculus, and apply it to the case of recovering an unknown star formation history, SFR(t), from the resulting Hertzsprung--Russell (HR) diagram. This approach allows a totally non-parametric solution, which has the advantage of requiring no initial assumptions about SFR(t). As a full maximum likelihood statistical model is used, and we take advantage of all the information available in the HR diagram, rather than concentrating on particular features such as turn-off points or luminosity functions. We test the method using a series of synthetic HR diagrams produced from known SFR(t), and find it to be quite successful under noise conditions comparable to those present in current observations. At this point we restrict the analysis to situations in which the metallicity of the system is known, as is the case with the resolved population of dwarf spheroidal companions to the Milky Way or the solar neighbourhood Hipparcos data. We also include tests to quantify the way uncertainties in the assumed metallicity, binary fraction and initial mass function (IMF) affect our inferences.

  • deriving star formation histories inverting hr diagrams through a Variational Calculus maximum likelihood method
    arXiv: Astrophysics, 1998
    Co-Authors: X Hernandez, D Vallsgabaud, Gerard Gilmore
    Abstract:

    We introduce a new method for solving maximum likelihood problems through Variational Calculus, and apply it to the case of recovering an unknown star formation history, $SFR(t)$, from a resulting HR diagram. This approach allows a totally non-parametric solution which has the advantage of requiring no initial assumptions on the $SFR(t)$. As a full maximum likelihood statistical model is used, we take advantage of all the information available in the HR diagram, rather than concentrating on particular features such as turn off points or luminosity functions. We test the method using a series of synthetic HR diagrams produced from known $SFR(t)$, and find it to be quite successful under noise conditions comparable to those present in current observations. At this point we restrict the analysis to situations where the metallicity of the system is known, as is the case with the resolved populations of the dwarf spheroidal companions to the Milky Way or the solar neighbourhood Hipparcos data. We also include tests to quantify the way uncertainties in the assumed metallicity, binary fraction and IMF affect our inferences.

D Vallsgabaud - One of the best experts on this subject based on the ideXlab platform.

  • deriving star formation histories inverting hertzsprung russell diagrams through a Variational Calculus maximum likelihood method
    Monthly Notices of the Royal Astronomical Society, 1999
    Co-Authors: X Hernandez, D Vallsgabaud, Gerard Gilmore
    Abstract:

    We introduce a new method for solving maximum likelihood problems through Variational Calculus, and apply it to the case of recovering an unknown star formation history, SFR(t), from the resulting Hertzsprung--Russell (HR) diagram. This approach allows a totally non-parametric solution, which has the advantage of requiring no initial assumptions about SFR(t). As a full maximum likelihood statistical model is used, and we take advantage of all the information available in the HR diagram, rather than concentrating on particular features such as turn-off points or luminosity functions. We test the method using a series of synthetic HR diagrams produced from known SFR(t), and find it to be quite successful under noise conditions comparable to those present in current observations. At this point we restrict the analysis to situations in which the metallicity of the system is known, as is the case with the resolved population of dwarf spheroidal companions to the Milky Way or the solar neighbourhood Hipparcos data. We also include tests to quantify the way uncertainties in the assumed metallicity, binary fraction and initial mass function (IMF) affect our inferences.

  • deriving star formation histories inverting hr diagrams through a Variational Calculus maximum likelihood method
    arXiv: Astrophysics, 1998
    Co-Authors: X Hernandez, D Vallsgabaud, Gerard Gilmore
    Abstract:

    We introduce a new method for solving maximum likelihood problems through Variational Calculus, and apply it to the case of recovering an unknown star formation history, $SFR(t)$, from a resulting HR diagram. This approach allows a totally non-parametric solution which has the advantage of requiring no initial assumptions on the $SFR(t)$. As a full maximum likelihood statistical model is used, we take advantage of all the information available in the HR diagram, rather than concentrating on particular features such as turn off points or luminosity functions. We test the method using a series of synthetic HR diagrams produced from known $SFR(t)$, and find it to be quite successful under noise conditions comparable to those present in current observations. At this point we restrict the analysis to situations where the metallicity of the system is known, as is the case with the resolved populations of the dwarf spheroidal companions to the Milky Way or the solar neighbourhood Hipparcos data. We also include tests to quantify the way uncertainties in the assumed metallicity, binary fraction and IMF affect our inferences.

Natalia Martins - One of the best experts on this subject based on the ideXlab platform.