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Jets as a probe of the Quark Gluon Plasma Jets as a probe of the Quark Gluon Plasma Christine Nattrass Yale University Goldhaber Lecture 2008 Christine Nattrass Yale University Goldhaber Lecture 2008
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 2 Outline What is a quark gluon plasma? Why do we want to study it? How do we study it? What have we learned? Conclusions
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 3 The structure of matter http://www.ehs.utoronto.ca/services/radiation/radtraining/module1.htm
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 4 Who was Gertrude Goldhaber? Gertrude Scharff Goldhaber July 14, 1911 — February 2, 1998 http://cwp.library.ucla.edu/Phase2/Goldhaber,_Gertr ude_Scharff@812345678.html http://upload.wikimedia.org/wikipedia/commons/a/aa/Beta-minus_Decay.svg http://universe-review.ca/I14-05-nuclearenergy.jpg http://www.nap.edu/html/biomems/ggoldhaber.html Beta decay – demonstrated that the beta particle was an electron Shell model – provided experimental evidence for closed shells in heavy nuclei Created first 3-D plot
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 5 Nucleons – the proton and neutron NeutronProton http://en.wikipedia.org/wiki/Image:Quark_structure_neutron.svg http://en.wikipedia.org/wiki/Image:Quark_structure_proton.svg
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 6 Other particles - hadrons Baryons Mesons
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 7 The Standard Model Electromagnetic force http://e4.physik.uni-dortmund.de/bin/view/ATLAS/SmBilder?PhotoarchivePlugin_page=1&PhotoarchivePlugin_view=detailed Strong force Weak force
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 8 What keeps the nucleus together? distance strength Electromagnetic force Strongforce
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 9 How to make a Quark Gluon Plasma
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 10 Evolution of the Universe Reheating Matter ?The universe gets cooler ! ? Need temperatures around 1.5·10 12 K ~10 6 times hotter than the core of the sun 10 6 yrs 3 min 6 sec 2·10 -6 sec 2 10 -10 sec 10 -35 sec 10 9 yrs ? 10 -44 sec
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 11 A heavy ion collision Relativistic pancakes Quark soup Explosive hadron soda
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 12 Relativistic Heavy Ion Collider STAR PHENIX PHOBOSBRAHMS1.2k
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 13 The STAR detector ~4m~4m ~4m~4m Over 1,200 tons
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 14 Peripheral collision
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 15 Central collision ~2000 tracks
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 16 What are jets? proton Jets –hard scattering of partons (quarks and gluons) Studied in dozens of experiments
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 17 Jets – azimuthal correlations trigger Phys Rev Lett 90, 082302 p+p dijet
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 18 Jets – azimuthal correlations p+p dijet
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 19 Looking in two dimensions d+Au
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 20 In two dimensions in Au+Au nucl-ex/0701074
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 21 What I've studied nucl-ex/0701074 Different systems and energies Cu+Cu √ s NN = 200 GeV Cu+Cu √ s NN = 62 GeV Au+Au √ s NN = 62 GeV Different particles K 0 S,, Results: Jet looks like p+p, Ridge looks like the rest of the A+A collision Ridge grows with energy The fewer nucleons in the collision, the smaller the Ridge
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 22 Conclusions If we get nuclear matter dense enough, we make a new phase of matter This quark gluon plasma is similar to what was present in the early universe We can produce a QGP in heavy ion collisions We can study it using probes such as jets proton
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 23 Conclusions We see evidence of a hot, dense medium from studying jets at RHIC One of the jets almost disappears The other jet is modified dramatically
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Christine Nattrass (Yale), Goldhaber Seminar, BNL, May 23, 2008 24 Many, many thanks to John Harris Helen Caines Jana Bielcikova The entire Yale group, past and present STAR
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