PPT-Relativistic Particle Acceleration

in a Developing Turbulence Shuichi M ATSUKIYO ESST Kyushu Univ Collaborator T Hada Outline Background motivation acceleration processes in turbulent plasmas parametric instability PI. The Relativistic String All lecture courses on string theory start with a discussion of the point particle Ours is no exception Well take a 64258ying tour through the physics o f the relativistic point particle Section 3.4a. The difference quotient:. When we let . h. approach 0, we saw the rate at which a function. w. as changing at a particular point . x. …. Definition: Instantaneous Rate of Change. The . Acceleration Mechanisms. 1. Acceleration Mechanisms. There is clear observational evidence that hadrons and electrons are accelerated to extreme energies by astrophysical objects. direct evidence: charged cosmic rays. Denver. 1. The Accelerating Universe. Roger Blandford. KIPAC. Stanford. Greed is Good?. Extraordinarily high energies. Zevatrons. ? >100J at source (~home run). Most astrophysical sources are conspicuously . . In classical mechanics, the momentum of a particle is defined as a product of its mass and its velocity, . . In an isolated system of particles, with no net force acting on the system, the total momentum of the system remains the same. However , we can see from a simple though experiment that the quantity . Yuri . Lyubarsky. Ben-Gurion University. Beer-. Sheva. , Israel . Universality of . relativistic jets. M 87. M 87. Crab in X-rays. GRBs. t. ime, s. t. ime, s. PKS 2155-304 . Pulsar magnetosphere. (Fermi acceleration at shock: most standard, nice powerlaw, few free parameters). main . signatures to . be determined: . E. min . , . E. max. [. Ã. timescale . t. acc. (E. ) ], . spectral slope . Kapshai. V.N., . Grishechkin. . Yu.A. .. F. . Scorina. Gomel State University. Plan of the. . talk. resonance states. . in. . nonrelativistic . QM. equations of . quasipotential. type. integral equations in the RCR and scattering amplitudes. Section 3.4a. The difference quotient:. When we let . h. approach 0, we saw the rate at which a function. w. as changing at a particular point . x. …. Definition: Instantaneous Rate of Change. The . Mass Transport (Acceleration?). J. Arons. UC Berkeley. Question: How Does Return Current in PSR Magnetosphere Form?. . What is density of current carriers?. Consequences (many): How do beamed gamma rays get emitted?. . In classical mechanics, the momentum of a particle is defined as a product of its mass and its velocity, . . In an isolated system of particles, with no net force acting on the system, the total momentum of the system remains the same. However , we can see from a simple though experiment that the quantity . Sources. 1. Sources of high-energy particles. We now have clear observational diagnostics for particle acceleration. synchrotron radiation (radio, sometimes X-ray). inverse Compton scattering (X-ray, . Siming. Liu. University of Glasgow. Collaborators. Vahe. ’ . Petrosian. , . Yanwei. Jiang: Stanford University. Zhonghui. Fan: Yunnan University. Oct. 2008 Krakow, Poland . Outline. I: Observations: Distribution. based on the course by. Joël . Le . Duff. Many Thanks!. CAS on Advanced Level Accelerator Physics Course . Trondheim, 18-29 August 2013. Summary of the 2 lectures:. Acceleration methods. Accelerating.