Femtoscopy in √s = 200 GeV p+p collisions at RHIC-PHENIX Andrew Glenn for the collaboration Lawrence Livermore National Lab HAW09: Joint APS/DNP JPS Meeting.

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Femtoscopy in √s = 200 GeV p+p collisions at RHIC-PHENIX Andrew Glenn for the collaboration Lawrence Livermore National Lab HAW09: Joint APS/DNP JPS Meeting LLNL-PRES

Why measure Hanbury Brown Twiss in p+p? Baseline measurement for heavy ion Proving ground for understanding and dealing with non-HBT correlations (energy-momentum correlations) – Event selection – Relative to jet – Multiplicity – … Capability likely needed for future heavy ion analyses relative to jet axis. Medium response measurable in freeze out hyper-surface? (Similar to HBT relative to reaction plane.) Z. Chajecki, M. Lisa Phys.Rev.C78:064903,2008 Chesler & Yaffe, (hep-th) Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 2

HBT nomenclature x Actual q distribution Background q distribution = The source S can be directly recovered with imaging Make assumptions about the source adapted from Annu. Rev. Nucl. Part. Sci : Detector Simplified for identical particles or Bose-Einstein Enhancement at Low q Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 3

A few analysis details Run5 p+p minimum biased (~2.5M like sign pion pairs) Run5 p+p minimum biased (~2.5M like sign pion pairs) Charged pions identified by time of flight from West PbScCharged pions identified by time of flight from West PbSc Matching cuts reduce backgroundsMatching cuts reduce backgrounds Pair selection cuts to remove merging and splittingPair selection cuts to remove merging and splitting No Monte Carlo based corrections so more selective pair cutsNo Monte Carlo based corrections so more selective pair cuts Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 4

1-D Correlations Staring point for 1D imaging analysis Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 5

Slices of 3-D Correlation side out long Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 6

A few words on fitting Fit data for q o 2 +q l 2 +q s 2 <(0.4GeV/c) 2 PYTHIA used as sanity check to limit fit range and help minimize impact of non-HBT correlations one example of many slices 1 q long (GeV/c) q side (GeV/c) Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 7

Transverse Mass Dependence Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 8

Au+Au Comparison Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 9

Spherical Harmonic Expansion Preferred for imaging over spline basis – D. A. Brown and P. Danielewicz, Phys. Lett. B 398, 252 (1997) [arXiv:nucl-th ] – D. A. Brown et. al. Phys.Rev.C72:054902,2005. May reveal non-HBT correlations in a more immediate way. Traditionally starts from 3D foreground and background distributions – Maximizes statistics and acceptance issues – New method for directly computing A. Kisiel and D. Brown arXiv: Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 10 Quark Matter 2005 Zbigniew Chajęcki STAR Collaboration STAR

similarly for in matrix notation is a measurement with uncertainty; what’s the variance? Wigner 3j arXiv: Kisiel and Brown Direct Spherical Harmonic Decomposition Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 11

Minimize the chi2 This assumes the variance on M q is ~0 for large mixing depth. if one uses complex numbers directly as matrix elements. Assumes elements complex numbers based on the format. I personally see no reason to do an analysis using the traditional Cartesian binning to Y lm. If you do, please let me (and the rest of the world) know. There can be experimental corrections such as: Merging/splitting Monte Carlo corrections applied directly as weights to Y lm Purity correction, P decompose P spherical harmonics and divide C measured There can be experimental corrections such as: Merging/splitting Monte Carlo corrections applied directly as weights to Y lm Purity correction, P decompose P spherical harmonics and divide C measured arXiv: Kisiel and Brown Direct Spherical Harmonic Decomposition II For one q bin Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 12

Statistic Study: Glimpse at the Future Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting Use foreground and background q count distributions from real data. Assume random q direction. Errors are not correlated q bin to bin, but are C lm to C l’m’ 13 random q direction Monte Carlo

Summary Pion correlations in minimum biased collisions for PHENIX west arm acceptance do not appear to show significant energy momentum correlations within statistics. Measured radii consistent with centrality extrapolation from Au+Au Plenty still to look at (spherical harmonic decomposition, multiplicity dependence…) Jet selected events on the horizon (will need tools to deal with energy-momentum contamination) Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 14

Jet Selected p+p Teaser An early look at events with a reconstructed jet show this should be interesting. Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 15

Aside on likelihood fitting Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 16 Not in Annu. Rev. Nucl. Part. Sci :

Baseline in p+p, d+Au and Au+Au  Some coefficients don’t vanish for large Q  Bias from zero is larger for more peripheral collisions  This problem is getting more significant for small systems (pp & dAu)  It can be due to  an experimental artifact  long range correlations (e.g. Jets)  problem with momentum conservation ?  or ? Quark Matter Zbigniew Chajęcki for the STAR Collaboration

Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 18

arXiv: Andrew Glenn, Joint HAW09 APS/DNP JPS Meeting 19