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Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy – A Conference in Athens, Greece, 11-13 July 2016

Co-organised by: Università degli Studi di Roma "Tor Vergata" (under the DEXTEROUS project) and the Research Center for Astronomy and Applied Mathematics (RCAAM) of the Academy of Athens Rationale: The decision to organize this meeting was taken after noting that there has been since long a number of groups developing diverse symbolic tools or computer-algebraic methods for implementing…

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Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy – A Conference in Athens, Greece, 11-13 July 2016 | hamiltonian2016.wordpress.com Reviews
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Co-organised by: Università degli Studi di Roma Tor Vergata (under the DEXTEROUS project) and the Research Center for Astronomy and Applied Mathematics (RCAAM) of the Academy of Athens Rationale: The decision to organize this meeting was taken after noting that there has been since long a number of groups developing diverse symbolic tools or computer-algebraic methods for implementing…
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Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy – A Conference in Athens, Greece, 11-13 July 2016 | hamiltonian2016.wordpress.com Reviews

https://hamiltonian2016.wordpress.com

Co-organised by: Università degli Studi di Roma "Tor Vergata" (under the DEXTEROUS project) and the Research Center for Astronomy and Applied Mathematics (RCAAM) of the Academy of Athens Rationale: The decision to organize this meeting was taken after noting that there has been since long a number of groups developing diverse symbolic tools or computer-algebraic methods for implementing…

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Speakers – Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy

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Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy. A Conference in Athens, Greece, 11-13 July 2016. Eduardo Andrade-Ines (Institut de Mécanique Céléste et de Calcul des Ephémérides – IMCCE). Luca Biasco (Università degli Studi Roma Tre). Alessandra Celletti (Università degli Studi di Roma Tor Vergata ). Helen Christodoulidi (University of Patras). George Contopoulos (Academy of Athens) Special Lecture. Konstantinos Efstathiou (University of Groningen).

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Location & Accommodation – Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy

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Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy. A Conference in Athens, Greece, 11-13 July 2016. Research Center for Astronomy and Applied Mathematics of the Academy of Athens. Soranou Efesiou 4, Athens, 11527. Following is the access map to the meeting’s venue from the nearby Metro Station KATEHAKI. The conference venue is a 10 mins walk from the Metro Station Katehaki. We have also made special deals with the following two hotels:. Transfer from/to th...

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Program – Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy

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Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy. A Conference in Athens, Greece, 11-13 July 2016. Monday 11 July 2016. KAM theory and quasi-periodic attractors of some dissipative systems. On the (computer-assisted) application of an a posteriori KAM theorem. KAM Theory for secondary tori in mechanical systems. Quasi periodic coorbital motions. Invariant tori in the spatial three-body problem. Rapporteur’s summary of morning talks (P. Robutel). Dynamics ...

4

Abstracts – Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy

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Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy. A Conference in Athens, Greece, 11-13 July 2016. Abstracts are also available as a PDF file. In alphabetical order by author. Secular Dynamics of S-type Orbits in Binary Star Systems. KAM Theory for secondary tori in mechanical systems. We prove the persistence of secondary tori for general mechanical systems. Work in collaboration with L. Chierchia. Presentation in PDF format. The classical Hill problem (...

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Research Center for Astronomy | Academy of Athens

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How to reach us. Galactic Dynamics and Galactic Morphology. PhD and Masters Theses. Past and Future Events. Computational perturbative methods for Hamiltonian systems Applications in physics and astronomy 2016. The Role and The Origin of the Magnetic Fields in Astrophysics March 2013. 13th European Solar Physics Meeting, 2011. Chaos in Galactic Dynamics 2007. Galaxies and Chaos 2002. Education and Outreach Activities. Latest processed SDO/HMI full-disk magnetogram. Tuesday 4 April 2017.

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Research Center for Astronomy | Academy of Athens

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How to reach us. Galactic Dynamics and Galactic Morphology. PhD and Masters Theses. Past and Future Events. Computational perturbative methods for Hamiltonian systems Applications in physics and astronomy 2016. The Role and The Origin of the Magnetic Fields in Astrophysics March 2013. 13th European Solar Physics Meeting, 2011. Chaos in Galactic Dynamics 2007. Galaxies and Chaos 2002. Education and Outreach Activities. Latest processed SDO/HMI full-disk magnetogram. Tuesday 14 March 2017. How to reach us.

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How to reach us. Galactic Dynamics and Galactic Morphology. PhD and Masters Theses. Past and Future Events. Computational perturbative methods for Hamiltonian systems Applications in physics and astronomy 2016. The Role and The Origin of the Magnetic Fields in Astrophysics March 2013. 13th European Solar Physics Meeting, 2011. Chaos in Galactic Dynamics 2007. Galaxies and Chaos 2002. Education and Outreach Activities. Latest processed SDO/HMI full-disk magnetogram. Tuesday 14 March 2017. 01,042) marks th...

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Research Center for Astronomy | Academy of Athens

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How to reach us. Galactic Dynamics and Galactic Morphology. PhD and Masters Theses. Past and Future Events. Computational perturbative methods for Hamiltonian systems Applications in physics and astronomy 2016. The Role and The Origin of the Magnetic Fields in Astrophysics March 2013. 13th European Solar Physics Meeting, 2011. Chaos in Galactic Dynamics 2007. Galaxies and Chaos 2002. Education and Outreach Activities. Latest processed SDO/HMI full-disk magnetogram. Tuesday 14 March 2017.

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Research Center for Astronomy | Academy of Athens

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How to reach us. Galactic Dynamics and Galactic Morphology. PhD and Masters Theses. Past and Future Events. Computational perturbative methods for Hamiltonian systems Applications in physics and astronomy 2016. The Role and The Origin of the Magnetic Fields in Astrophysics March 2013. 13th European Solar Physics Meeting, 2011. Chaos in Galactic Dynamics 2007. Galaxies and Chaos 2002. Education and Outreach Activities. Latest processed SDO/HMI full-disk magnetogram. Tuesday 14 March 2017. The conference C...

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Research Center for Astronomy | Academy of Athens

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How to reach us. Galactic Dynamics and Galactic Morphology. PhD and Masters Theses. Past and Future Events. Computational perturbative methods for Hamiltonian systems Applications in physics and astronomy 2016. The Role and The Origin of the Magnetic Fields in Astrophysics March 2013. 13th European Solar Physics Meeting, 2011. Chaos in Galactic Dynamics 2007. Galaxies and Chaos 2002. Education and Outreach Activities. Latest processed SDO/HMI full-disk magnetogram. Tuesday 14 March 2017.

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Research Center for Astronomy | Academy of Athens

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How to reach us. Galactic Dynamics and Galactic Morphology. PhD and Masters Theses. Past and Future Events. Computational perturbative methods for Hamiltonian systems Applications in physics and astronomy 2016. The Role and The Origin of the Magnetic Fields in Astrophysics March 2013. 13th European Solar Physics Meeting, 2011. Chaos in Galactic Dynamics 2007. Galaxies and Chaos 2002. Education and Outreach Activities. Latest processed SDO/HMI full-disk magnetogram. Tuesday 4 April 2017.

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How to reach us. Galactic Dynamics and Galactic Morphology. PhD and Masters Theses. Past and Future Events. Computational perturbative methods for Hamiltonian systems Applications in physics and astronomy 2016. The Role and The Origin of the Magnetic Fields in Astrophysics March 2013. 13th European Solar Physics Meeting, 2011. Chaos in Galactic Dynamics 2007. Galaxies and Chaos 2002. Education and Outreach Activities. Latest processed SDO/HMI full-disk magnetogram. Tuesday 4 April 2017. Hamiltonian pertu...

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Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy – A Conference in Athens, Greece, 11-13 July 2016

Computational perturbative methods for Hamiltonian systems – Applications in physics and astronomy. A Conference in Athens, Greece, 11-13 July 2016. Università degli Studi di Roma “Tor Vergata”. Under the DEXTEROUS project) and the Research Center for Astronomy and Applied Mathematics (RCAAM). Of the Academy of Athens. Analytical and semi-analytical methods. Study of convergence – accumulation of small divisors. Computer-algebraic techniques, special manipulators and computational environments. Cefthim a...

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