PPT-Two non-equilibrium problems in heavy-ion collisions:

Author : jane-oiler | Published Date : 2016-08-08

Critical dynamics amp Sphaleron transitions Raju Venugopalan BNLHeidelberg Hirschegg 2016 January 1722 2016 Outline N onequilibrium dynamics of two situations of

Presentation Embed Code

Download Presentation

Download Presentation The PPT/PDF document "Two non-equilibrium problems in heavy-io..." is the property of its rightful owner. Permission is granted to download and print the materials on this website for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.

Two non-equilibrium problems in heavy-ion collisions:: Transcript

Critical dynamics amp Sphaleron transitions Raju Venugopalan BNLHeidelberg Hirschegg 2016 January 1722 2016 Outline N onequilibrium dynamics of two situations of interest in heavyion collisions. Satisfiability. and Constraint Satisfaction Problems. by Carla P. Gomes, Bart Selman, . Nuno. . Crato. and . henry. . Kautz. Presented by . Yunho. Kim. Provable Software Lab, KAIST. Contents. Heavy-Tailed Phenomena in . interesting ?. Interaction of heavy quarks with the plasma. . - . our model (elastic and inelastic collisions, LPM). . - comparison with data. . - how far we are with our understanding. . P. é. ter. Petreczky. . . Bielefeld, July 2013. Study of the strongly interacting matter and its new . “phases”. Past: . AGS, SPS, . E. cm. =(1-17) . Rainer Fries. Texas A&M University & RIKEN BNL. Workshop on RHIC Paradigms. UT Austin, April 14, 2010. Austin: RHIC Paradigms. 2. Rainer Fries. Overview. Introduction Recombination. Satisfiability. and Constraint Satisfaction Problems. by Carla P. Gomes, Bart Selman, . Nuno. . Crato. and . henry. . Kautz. Presented by . Yunho. Kim. Provable Software Lab, KAIST. Contents. Heavy-Tailed Phenomena in . He came from traditional nuclear physics, and is one of the few I know who made the transition to high energy heavy ion physics with a modern perspective.. People fall into three categories:. Those who make things happen.. . AGS. . -- . Heavy . Ion . P. rograms. Hideki Hamagaki. (. hamagaki_hideki@pilot.nias.ac.jp. ). Institute for Innovative Science and Technology. Nagasaki Institute of Applied Science. Contents. Introduction. 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. The Haber process proceeds as follows:. . 2NH. 3 (g). + 92KJ ↔ N. 2 (g). + 3H. 2 (g) . . If the equilibrium concentrations are:. [NH. 3. ] = 3.1x10. -2. M. [N. 2. ] = 8.5x10. -1. M. [H. 2. W. A. Horowitz. The Ohio State University. February 23, 2010. 16-Nov-10. 1. UCT Seminar. With many thanks to Brian Cole, . Miklos. . Gyulassy. , Ulrich Heinz, and Yuri . Kovchegov. Introduction. What is a heavy ion collision?. Collisions. @ LHC ++. 1. One. central ALICE event for . Pb+Pb @ 2.76 . TeV.A. => E(. kin_total. )= 574 GeV . 0-5% central: . 25000 . particles. Relativistic. AA . and. . eA. . Collisions. 2. “versus” AdS/CFT. Perils, Pitfalls, Progress, Prospects. W.A. . Zajc. Physics Department. Columbia University, New York, NY. . ( . this talk available . at . http://. www.phenix.bnl.gov/phenix/WWW/publish/zajc/sp/presentations/Durham. with heavy-ions. Hou. . Keong. (Tim) Lou,. Simon . Knapen. , . Tongyan. Lin and Tom Melia. PhysRevLett.118.171801. a. Pb. Light Dark Matter 2017. *Disclaimer: Not Dark Matter! Sorry!. “Light”? “Dark”? . Bedanga. Mohanty. NISER. (For STAR Collaboration). Based on STAR: . arXiv. : 1701.07065 . 01/20. Goals of Heavy-Ion Collision. Find out the phase structure of QCD phase . d. iagram . e. xperimentally.

Download Document

Here is the link to download the presentation.
"Two non-equilibrium problems in heavy-ion collisions:"The content belongs to its owner. You may download and print it for personal use, without modification, and keep all copyright notices. By downloading, you agree to these terms.