Matter ~13.8 Billion Years Ago

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Presentation transcript:

Matter ~13.8 Billion Years Ago Visit of Oslo Students at CERN , 7.5.13 Sedat Altınpınar

Motivation

Going deeper in structure…

Standard Model

Strong Interaction is different... Electron - Proton Quark - Quark Vstrong(r) (GeV) r (fm) VEM(r) (eV) r (nm) kr r c 3 4 V s strong + - = h a ) (

From Infrared to Ultraviolet Infrared slavery Ultraviolet Behaviour

Nobel 2004 Gross, Wilczek, Politzer

Does it exist in nature ? QGP

We can recreate it: LHC @ CERN

4 LHC Experiments

Nucleus-Nucleus Collision

ALICE

Event in ALICE

How to study matter ? Properties of matter: Conductivity, color, density, phase states, magnetism,… Example method: Partonic energy loss, ergo kind of finding a Bethe-Bloch for partons. Probe: Quarks. For example energy loss of heavy quarks (c and b) delivers important informations about the Quark-Gluon Plasma. Measurement: Yields of electrons originating from hadrons and hadrons themselves containing heavy quarks like D0(c, u(bar)), B0(b(bar), u),...

The Observable RAA RAA the Nuclear Modification Factor Nucleus-Nucleus Collision Proton-Proton Collision Baseline of RAA

Hydrodynamics -> Elliptic flow v2 Interactions among the produced particles: Pressure gradients generate positive elliptic flow v2

It’s liquid !

Phase Diagram of Nuclear Matter

Thank you for listening And many other observables and ideas Thank you for listening