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Series Lecture on Laser Plasma Physics

at Shanghai Jiao Tong University June 27&28, July 4&5, 2009. Series Lecture on Laser Plasma Physics.  H. Takabe (Aki). Professor, Institute of Laser Engineering and School for Physics and School for Space and Earth Science, Graduate School of Science, Osaka University, Japan

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Series Lecture on Laser Plasma Physics

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  1. at Shanghai Jiao Tong UniversityJune 27&28, July 4&5, 2009 Series Lecture on Laser Plasma Physics  H. Takabe (Aki) Professor, Institute of Laser Engineering andSchool for Physics and School for Space and Earth Science, Graduate School of Science, Osaka University, Japan Visiting Professor, Shanghai Jiao Tong UniversityShanghai, China

  2. Chapter 1Introduction

  3. 1.1 Self-introduction

  4. Takabe-G: Laser Astrophysics (1) ILE OSAKA Creation of Mimic Black Hole in Laboratory Universe Black Hole Experimental Data Laboratory Black Hole Photo-ionization in X-ray Binary with Black Hole Radiation Temperature of 0.5 keV has been achieved. Neutron Star

  5. Takabe-G: Laser Astrophysics (2) ILE OSAKA Challenging 100 year-standing mystery of Cosmic Ray=Collisionless Shock Physics = SN1006 Collisionless Shock Formation by Self-Organization (Kato-Takabe Theory) 30 Light Years Density Universe Averaged Density Shock Front Shock Jump Laboratory Self-Generated E and B fields Space

  6. 1.2 High-Power Laser Maiman (1960) Ruby Laser

  7. Early Stage of Laser for Inertial Confinement Fusion in Livermore, USA

  8. What is laser?

  9. Laser Welding

  10. Gekko XII Laser, Osaka Univ. Big Laser Facilities ILE, Osaka University Gekko Amplifiers

  11. Nonlinear Optics Harmonic Conversion with Nonlinear Crystal Shorter Wavelength is better for Laser Plasma Interaction

  12. 1.3 Plasmas What is Plasma ? Solid Liquid Gas Plasmas

  13. Lightening 1.4 Plasmas in Nature and Life

  14. How gamma-ray appears accompanied with lightening

  15. Solar Flare

  16. Plasmas Corona Mass Ejection

  17. Aurora

  18. Plasmas 1.5 Plasmas in Universe 藤井旭、「星のたんじょう」（金の星社）

  19. Planetary Nebula (Hour Glass Nebula) Hubble Space Telescope (NASA)

  20. Supernova Explosion

  21. Crab Nebula and Neutron Star

  22. Quark Gluon Plasma Before collision After collision ビッグバン 中性子星

  23. Surface：6000K Structure of Sun Center:1.5keV

  24. Convection near the surface of the Sun

  25. Temperature Density

  26. 1.6 How to describe Plasmas Lorentz force and gyro motion

  27. Drift motion

  28. Maxwell Equations Faraday’s Law Ampere’s Law Poisson Equation Absence of Magnetic Monopole

  29. Hydrodynamic Equations Continuity Motion Energy

  30. Basic Equations for Plasma Fluid Model Ion Fluid Electron Fluid Maxwell Equations Charge and Current Densities

  31. Ludwig Boltzmann (1844-1906) Suicide in 1906 S = -k ln W Boltzmann wrote in1898 “I am conscious of being only an individual struggling weakly against the stream of time.” Increasingly subject to depressions, Boltzmann committed suicide in 1906 only shortly before Perrin’s experiment on Brownian motion (1908) and Mililan’s oil-drop experiment (1909) provided very direct evidence for the discrete structure of matter. (Statistical Physics, Berkeley Phys. 5) P. 162

  32. Boltzmann Equation f(t,r,v): Velocity distribution function Vlasov Equation

  33. From Particle Image to Fluid Image [E.A.] (Phase Space) (Particles) (Ensembles) [Velocity moments] (Real Space) (Distribution Func.) [CE expansion] (Fluid Eqs.) (Moment Eqs.)

  34. Fokker-Planck Equation

  35. Radiation Transport Equation

  36. Hamiltonian for N-electron system How to solve: MCHF, HF, Para-potential Method OPAL at LLNL

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