'Baryon density' diaporamas de présentation

The Current status of the MPD@NICA Project at JINR

The Current status of the MPD@NICA Project at JINR. A.Litvinenko for MPD@NICA collaboration litvin@moonhe.jinr.ru. MPD@NICA Project. The M ulti P urpose D etector( MPD ) is designed to study Heavy I on collisions at the N uclotron-based heavy I on

1.11k views • 84 slides

The MPD@NICA Project at JINR

The MPD@NICA Project at JINR. A.Litvinenko for MPD@NICA collaboration litvin@moonhe.jinr.ru. The MPD@NICA Project at JINR. A.Litvinenko for MPD@NICA collaboration litvin@moonhe.jinr.ru. VBLHEP. Outline. Introduction Motivation Observables Detector conception Conclusions.

1.18k views • 71 slides

Cosmic Microwave Background

Cosmic Microwave Background. Primary Temperature Anisotropies Polarization Secondary Anisotropies. Coherent Picture Of Formation Of Structure In The Universe. Photons freestream: Inhomogeneities turn into anisotropies. t ~100,000 years.

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Chiral phase transition and chemical freeze out

Chiral phase transition and chemical freeze out. Understanding the phase diagram. Order parameters. Nuclear matter and quark matter are separated from other phases by true critical lines Different realizations of global symmetries Quark matter: SSB of baryon number B

700 views • 55 slides

Hiroyuki Sako ( ASRC/J-PARC, JAEA ) f or J-PARC HI Collaboration QM2014, Darmstadt

Towards the Heavy-Ion Program at J-PARC. 1. Introduction 2. H eavy ion acceleration scheme 3. Physics goals 4 . E xperimental design 5. Summary. Hiroyuki Sako ( ASRC/J-PARC, JAEA ) f or J-PARC HI Collaboration QM2014, Darmstadt. Introduction. LHC RHIC. SPS.

615 views • 49 slides

Hiroyuki Sako ( ASRC/J-PARC, JAEA ) f or J-PARC HI Collaboration QM2014, Darmstadt

Towards the Heavy-Ion Program at J-PARC. 1. Introduction 2. H eavy ion acceleration scheme 3. Physics goals 4 . E xperimental design 5. Summary. Hiroyuki Sako ( ASRC/J-PARC, JAEA ) f or J-PARC HI Collaboration QM2014, Darmstadt. Introduction. LHC RHIC. SPS.

647 views • 49 slides

626 views • 44 slides

Hadronic Matter at High Baryon Density

506 views • 41 slides

The C ompressed B aryonic M atter experiment

528 views • 40 slides

Leptons, Photons & the CMB

Leptons, Photons & the CMB. Ned Wright, UCLA 16 Aug 2007. Nobel Prize in Physics 2006. John Mather for the CMB Spectrum George Smoot for the CMB anisotropy. COBE View of the CMB Sky. Two Fluids in the Early Universe. Most of the mass is dark matter 80-90% of the density Zero pressure

500 views • 38 slides

Zhangbu Xu ?????

Search for Exotic Particles. Zhangbu Xu ?????. Strange Quark Matter. n, e, ?. Low Charge-to-Mass Ratio |Z|/m<<1 (A=2 ?10 57 ) Hybrid states (H-d, ? q -p). Witten, PRD 30 (1984)272 Jaffe, PRL 38 (1977)617E. Why Strange Quark Matter?. QCD Allowed New States

507 views • 38 slides

Are di-leptons sensitive messengers from the hot and dense stage?

497 views • 35 slides

THE EARLY UNIVERSE NEUTRINO CONNECTION

THE EARLY UNIVERSE NEUTRINO CONNECTION. GARY STEIGMAN THE OHIO STATE UNIVERSITY. LEOFEST. CuTAPP 2005 , Ringberg Castle , April 27, 2005. ~ 100 s after the Big Bang Primordial Nucleosynthesis. ~ 0.1 s after the Big Bang Neutrinos Decouple.

440 views • 35 slides

Cosmic Microwave Background and determination of cosmological parameters

??. Cosmic Microwave Background and determination of cosmological parameters. ??????. Full sky map of microwave background radiation #1. T =2.725K Cosmic Microwave Background CMB. ??????. Hubble parameter. Density parameter. cosmological constant (dark energy).

480 views • 33 slides

High Energy Dilepton Experiments

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Cosmological MHD

Cosmological MHD. Hui Li Collaborators: S. Li, M. Nakamura, S. Diehl, B. Oshea, P. Kronberg, S. Colgate (LANL) H. Xu, M. Norman (UCSD), R. Cen (Princeton). Observational overview of large scale magnetic fields Several examples of numerical modeling of cosmological MHD.

402 views • 25 slides

Determining the Special Orientations in Deformed 238 U + 238 U Collisions at CSR

Determining the Special Orientations in Deformed 238 U + 238 U Collisions at CSR. Kejun Wu 1 , Fei Xie 1 , Feng Liu 1 , Nu Xu 1,2 1) Institute of Particle Physics, Huazhong Normal University, China 2) Nuclear Science Division, LBNL, Berkeley, CA 94720, USA. Outline. Motivation

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X - and X + production in Pb+Pb collisions at 40A ? GeV at SPS

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Nuclei yields and elliptic flow in Au+Au 200GeV collision and comparison to the models

Nuclei yields and elliptic flow in Au+Au 200GeV collision and comparison to the models. Jianhang Zhou (Rice University) For STAR collaboration. Motivation.

201 views • 10 slides

Visualization of large astrophysical simulations datasets

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