PPT-Gluon Polarization in Longitudinally Polarized pp Collisions at STAR

Author : ellena-manuel | Published Date : 2018-10-10

Zilong Chang For Collaboration STAR Outline The RHICAGS Annual Users Meeting Z Chang 06092015 Introduction Inclusive jet measurements π 0 measurements Dijet measurements

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Gluon Polarization in Longitudinally Polarized pp Collisions at STAR: Transcript


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. XIII  WORKSHOP ON HIGH ENERGY SPIN PHYSICS . Dubna, Russia . September 1 - 5, 2009. . AZIMUTHAL ASYMMETRIES IN SEMI-INCLUSIVE PRODUCTION OF HADRONS ON THE LONGITUDINALLY POLARIZED DEUTERIUM TARGET. . Recontres. De . Moriond. QCD and High Energy Interactions . . La . Thulie. March 10. h. –17. th. 2012. Suppression of Hadrons . at Forward Rapidity at RHIC. Final State . of a Au-Au . Class Activities: . Polarization (1). Class Activities: . Polarization (2). A stationary point charge +Q is near a block of polarization material (a linear dielectric). The net electrostatic force on the block due to the point charge is . in . Interferometry. . 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. 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.. 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. 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 . Yuri . Kovchegov. The Ohio State University. based on work in collaboration with G. . Chirilli. . and D. . Wertepny. , . arXiv:1501.03106. [. hep-ph. ] . Outline. Introduction: classical gluon production problem in AA collisions and why it is important.. LL2 section 50. m. onochromatic plane wave. Constant. complex vector,. defines polarization state,. which is definite (elliptical). Approximately monochromatic plane wave. Contains frequencies in some interval . . 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.

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