NTHU & NCTS Workshop

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Recent Development of 
    Mathematics at
    Tsing-Hua University

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June 6, 2006

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                    Shing-Tung Yau

                                                                      Veblen Prize 1981
                                                          Fields Medal 1982
                                                      MacArthur Fellow 1985
                                                        Crafoord Prize 1994
                                                   National Medal of Science

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                  Á¿ÃD: Mathematics in the 21st Century,
                  
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              ®É¶¡: 1:00-2:00 pm


         
    ¦aÂI: ²MµØ¤j¾Çºî¦X¤TÀ]¤G¼Ó 201«Ç

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¦aÂI: ²M¤jºî¦X¤TÀ]¥|¼Ó¡ALecture Room A
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(1) ½²ªF©M ±Ð±Â Dong-Ho Tsai, 2:30-3:15 pm
       Some New Results for Plane Curves Expansion

    Abstract:

    We show that for embedded or convex plane curves expansion, the difference u(x,t)-r(t) in support functions between the expanding curves rt (with support function u(x,t)) and some expanding circles Ct (with support function r(t)) has its anymptotic shape as t¡÷¡Û. Moreover the isoperimetric difference L2 -4ƒTA is de-creasing and it converges to a constant б¡Ö0 if the expansion speed is asymptotically a constant and the initial curve is not a circle. For convex initial curves, if the ex-pansion speed is asymptotically infinite, them L2 -4ƒTA decrease to б=0 and there exists an asymptotic center of expansion for rt.

(2) ¤ý°¶¦¨ ±Ð±Â Wei-Cheng Wang, 3:30-4:15 pm
       Energy and Helicity Preserving Schemes for Hydro-and   

       Manetohydro-dynamics flows with symmetry

      Abstract:

    We introduce a family of efficient and robust numerical schemes devised for incompressible flows and MHD equation that admit a coordinate symmetry, such as the rotational symmetry.

The conservation of energy and helicity is achieved by recasting all the nonlinear terms (including the convection term, the Lorentz force and the electromotive force) into Jacobians. The conservation of energy and helicity then becomes transparent by employing the permutation identities associated with the Jacobians. This permutation identity is preserved in the discrete setting by our proposed scheme. In addition, the conservation property also holds in the vicinity of the axis of rotation, which is sometimes referred to as a geometric or pole singularity. The same permutation identity also gives a priori error estimates of our scheme. To our knowledge, this is the first rigorous error estimate of finite difference schemes for axisymmetric flows in the presence of the pole singularity.

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(3) ³¯°ê¼ý ±Ð±Â Kuo-Chang Chen, 4:30-5:15 pm
       The three-body problem from a variational point of view

Abstract:

    The three-body problem concerns the motion of three celestial bodies moving in space in accordance with Newton¡¦s law of universal gravitation. Except for self-similar solutions, which were completely classified by Euler and Lagrange in the 18th century, classical existence proofs for solutions of the three-body problem are largely relying on a perturbation method due to Poincaré. A vast amount of solutions were discovered by numerical simulations but yet without any analytical proof for their existence. In recent years variational methods have been successfully applied to the n-body [problem to construct miscellaneous solutions. In this talk I will briefly describe these recent progresses on the three-body problem. In particular, I will outline a variational proof for the existence of retrograde triple stars and some bizarre planets for double stars.

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