PPT-Polarized p + A Physics at Forward Rapidity at STAR

Author : mofferro | Published Date : 2020-06-16

Akio Ogawa for the STAR collaboration Brookhaven National Laboratory 2017 Feb 8 QM2017 Chicago Contents 2 Introduction Gluon saturation and RHIC pA STAR Forward

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Polarized p + A Physics at Forward Rapidity at STAR: Transcript


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 . 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. 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. arXiv:1408.3108 [hep-. ph. ]. Gin. és. MARTINEZ-GARCIA. Subatech. (CNRS/IN2P3 - . École. des Mines de Nantes – . Université. de Nantes). Oral presentation in the 10th International Workshop on High . . 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 . in relation to The long Term Goals. Physics in 2015+ for . h. >1. E.C. Aschenauer. STAR@UCLA, August 2013. 2. (un-)polarized . pp. (un-)polarized . pA. . unravel the underlying . subprocesses. . Board . member. . Dr. Mikhail . Igorevich. . Panasyuk. Director. Department of Physics. Moscow State University. Russia. Journal. of Astrobiology and Outreach. Biography. Mikhail . Igorevich. . Panasyuk. George . Igo. for STAR Collaboration. DIFFRACTION . 2012. Puerto del . Carmen,Lanzarote. Sept 10-15. Solenoidal Magnet – 0.5 Tesla field. Beam Pipe. Time Projection Chamber (TPC). Barrel Electromagnetic Calorimeter - BEMC. bandgap. energy illuminates a negative electron affinity (NEA) . GaAs. . photocathode, spin-polarized electrons are emitted [2, 3]. The degree of polarization is defined to be . where . N. ↑. and . a look . at . at. . heavy . quarkonium. data . in . p-. Pb. collisions. 1. E. Scomparin (INFN-Torino. ). INT Seattle, October 8 2014. Charmonia. and . bottomonia. in . p-. Pb. : . what is available from run-1 ?. D. iffraction at HFIR HB-3A. flipper. Collimator with guide field. S-bender supermirror polarizer. HB-3A. High neutron polarization ratio (>94%) and a good transmission (16% based on the diffraction on a 2 mm size . Zilong. Chang. For. Collaboration. STAR. Outline. The RHIC/AGS Annual Users Meeting -- Z. Chang 06/09/2015. Introduction. Inclusive jet measurements. π. 0. . measurements. Di-jet measurements. Conclusion. PSTP2019. Knoxville, Tennessee, September 26. th. 2019. P. Lenisa – University of Ferrara and INFN. for the LHC-spin study group. 2. A bit of (pre) history. Teflon-coated storage cell filled with polarized H proposed by Prof. W. . Learning Intentions . Properties of Stars. In this topic we are going to examine: . temperature and colour of a star. spectral class. the power of a star. stellar luminosity. apparent brightness. symbols. 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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