PPT-Resonance states of relativistic two-particle systems

Kapshai VN Grishechkin YuA 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. 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 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. Cascades. Size distributions. Scaling from observables. Size distribution in asteroid belt and . Kuiper. belt. Dust destruction, PR drag, dust dynamics, . Yarkovsky. and YORP effects. Tisserand. . . 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 . Relativistic Programming. Concurrent reading and writing improves performance and scalability. concurrent readers may disagree on the order of concurrent updates. orders may be non-. linearizable. i. Forces and Fields. Since 1932, . the number . of fundamental particles has increased enormously, . and . the . description of . these new particles and their interactions was soon . found to . be inadequate in terms of the two . (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 . Youngho Kim. CIS665: GPU Programming. Building a Million Particle System: Lutz Latta. UberFlow - A GPU-based Particle Engine: Peter Kipfer et al.. Real-Time Particle Systems on the GPU in Dynamic Environments: Shannon Drone. . 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 . Xu . Resonances of weakly bound or unbound nuclei. I. Model development:. Core Gamow Shell Model (CGSM) with realistic nuclear forces. . (resonance + continuum) . Kadmiel. Beauvais, Texas A&M. Advisors: Dr. Youngblood, Dr. . Lui. , Jonathan Button. Funded by NSF . grant number: PHY-1263281. Giant Resonances. Broad resonances in the excitation energy range, 10-30MeV. in a Developing Turbulence. . Shuichi M. ATSUKIYO. . ESST Kyushu Univ.. Collaborator : T. . Hada. Outline . Background. -- motivation. -- acceleration processes in turbulent plasmas. -- parametric instability (PI). PHYS 3446, Fall 2016. 1. PHYS 3446 – Lecture . #11. Wednes. day. , . Oct. . 12. , . 2016. Dr. . Jae. . Yu. Energy . Deposition in Media. Charged Particle Detection. Ionization . Process. Photon Energy Loss. Waves: . Importance of waves. MHD waves, . Plasma waves. Wave-particle interaction:. resonance condition. pitch-angle diffusion. Radiation belt remediation. Waves in Space. MHD waves: . frequencies much below ion gyrofrequency.