PPT-Gluon Polarization in Longitudinally Polarized pp Collisions at STAR

Zilong Chang For Collaboration STAR Outline The RHICAGS Annual Users Meeting Z Chang 06092015 Introduction Inclusive jet measurements π 0 measurements Dijet measurements Conclusion. Outline. Review of the Lorentz Oscillator. Reflection of Plasmas and Metals. Polarization of Scattered Light. Polarizers. Applications of Polarizers. Reading – Shen and Kong – Ch. 3. Microscopic Lorentz Oscillator Model. Machine development for spin-filtering experiments at COSY. P. Lenisa. Università. di Ferrara . and. INFN, . Italy. SPIN 2014 – Beijing, . October. 21, 2014. Motivation. The PAX . collaboration. A. lthough acute longitudinally extensive transverse myelitis (LETM) is a key diagnostic component of . neuromyelitis. . optica. (NMO) it may also occur in other conditions such as multiple sclerosis, sarcoidosis and infectious diseases. . Background. N. euromyelitis. . optica. spectrum disorders (NMOSD) are severe, inflammatory, immune-mediated disorders of the central nervous system which predominantly affect the optic nerves and the spinal cord. Longitudinally extensive transverse . In electrodynamics, . polarization. is the property of electromagnetic . wave, such as light , that describes the direction of the transverse . Electric field. E. B. k. For. Linearly polarized light. Wave 3 continue. Polarization. Polarization is a process of turning . unpolarized. light to polarized light. A light wave is an electromagnetic wave that travels through the vacuum of outer space. Light waves are produced by vibrating electric charges.. INTERFERENCE FILTER. Arrangement for filtering monochromatic beam from incident white light is called interference filter.. When a narrow beam of white light is incident on the filter, it undergoes multiple reflections in the dielectric, it loses a major part of its intensity and finally emerges from the filter as a very narrow band with one or two maxima.. tion to Dark Matter Direct Detection. Natsumi. Nagata . Nagoya University / University of Tokyo . 18 December, 2011 @ Nagoya University (GCOE Workshop 2011). Based on [J. . Hisano. , K. . Ishiwata. , N. N., . PlasMA. Nonequilibrium. Dynamics. in Astrophysics and Material Science. YITP, Kyoto, Japan, Oct. 31-Nov. 3, 2011. Tetsufumi. Hirano. Sophia Univ./. the Univ. of Tokyo. Outline. Introduction. Physics of the quark gluon plasma. Travis Salzillo. 1,2. , Rainer Fries. 1. , Guangyao Chen. 1. 1. . Cyclotron Institute, Texas A&M University . 2. REU student from Tarleton State University. Overview. Introduction to QCD and CGC. Polarization. Friday Presentations:. Schwarz (Planck), Patel (JWST), . Cox (SOFIA). Fourier Transforms. A function’s Fourier Transform is a specification of the. . amplitudes. and . phases. of . Akio Ogawa . for the STAR collaboration. Brookhaven National Laboratory. 2017 Feb. 8 . QM2017 @ Chicago. Contents. 2. Introduction - Gluon saturation and RHIC . pA. STAR Forward Calorimeter. Results - Single Spin Asymmetry at . . Rick . Perley. (NRAO-Socorro). Recap, and Plan. Dave has shown you why determining the full polarization state of natural radiation is important. . In this lecture I describe how an interferometer determines the Stokes parameters for distant sources. for Physics. e. +. @ MESA. Low-energy positron physics . Slow positron physics. Polarized positron production. . Conclusions. Eric Voutier. . Institut de Physique Nucléaire. Orsay, . France.