PPT-Particle rapidity distribution in proton-nucleus collisions

arXiv14083108 hep ph Gin és MARTINEZGARCIA Subatech CNRSIN2P3 École des Mines de Nantes Université de Nantes Oral presentation in the 10th International Workshop on High . 1 Matter and Radiation. Ks5 AS Physics AQA 2450. Mr D Powell. Matter & Radiation p4. 1. Quarks & Leptons p18. 2. Quantum Phenomena p30. 3. Electric Current p46. 4. Alternating Currents p74. 6. isospin. ratio from nucleons to fragments. Yingxun. Zhang(. 张英逊. ). China Institute of Atomic Energy. The 11. th. International Conference on Nucleus-Nucleus Collisions, . 31May, NN2012, San Antonio, TX. Prino. INFN – . Sezione. di Torino. Heavy-. flavour. production. in heavy-ion collisions. BEAUTY2016, Marseille, May 5. th. . 2016. 2. Heavy-Ion Collisions. Goal: study the properties of nuclear . Jiangyong Jia, BNL and Stony Brook University. July 20–23, . 2017. 3D initial condition and final state dynamics. 2. More dramatic at lower √s due to stopping. . Collectivity is important . bg. in study of chirality, criticality, . Outline. February 9, 2008. Quark Matter 2008. 2. Results. dN/dy. Stopping. Summary. and discussion. Experiment and motivation. Motivation: . reference to understand baryon transport. February 9, 2008. Marzia . Nardi. INFN Torino (Italy). nardi@to.infn.it. Quark Matter 2009, Knoxville. Student Day . WHY ?. General interest:. Unsolved problems of QCD. QCD out of the perturbative regime. Looking for universal properties. baryon number at intermediate coupling. Holography beyond . h. /. s. =1/4. p. Wilke van der Schee. Based on work . Åsmund. Folkestad, . Sašo. Grozdanov and Krishna Rajagopal. References: 1501.04952, 1507.08195, 1610.08976 (PRL), 1907.xxxxx. 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.. Quiz. Nuclear Physics Topics. Nuclear/Radioactive Decay. Nuclear Spin. Fission and Fusion. 1. What is this ?. Ans. : Magnet levitating above a high-. Tc. . superconductor. . This is the “. Meissner. The Atom Science �� Chemistry for Kids The atom is the basic building block for all matter in the universe. Atoms are extremely small and are made up of a few even smaller particles. T . . For elements of higher atomic number, the ratio rises to approximately 1.6 to 1 . As a nuclide departs from this stable ratio, changes in the nucleus occur which tend to bring the product to a more stable arrangement. . 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. Uncertainty Problems. Reinhard W. Schulte, MD, . MS, Loma . Linda . University. Funded by grants from. NIH: R01 grant from NIBIB, , P20 grant from NCI with UCSF and LBNL. Binational Science Foundation (image reconstruction and fast computing). Misha. . Veldhoen. (Utrecht University). For the ALICE collaboration. Hard Probes 2012. Cagliari, Italy. Measured by the ALICE detector, . TeV. Hadronization. at high and low .