K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June2008 1 Status of KK femtoscopy in ALICE (Based on Alice Week presentation) ‏ Konstantin Mikhaylov.

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K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June Status of KK femtoscopy in ALICE (Based on Alice Week presentation) ‏ Konstantin Mikhaylov and Alexey Stavinskiy ITEP, Russia

Outline K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June Physics Motivation of KK femtoscopy Experimental results Distortions of K+K+ correlation function: - PID's of Kaons - Pair PID - Splitting-merging - Resonances ( vτ ≥ source size): K*, Φ First results for K+K- Conclusion

Physics motivation Measured space-time extent of the particle emitting region for KK is pure than for ππ. Kaon femtoscopy signal is cleaner than pion femtoscopy signal since Kaons are less affected by resonance decay. The m T dependence: m T (KK) > m T (ππ). The strangeness distillation mechanism could lead to strong temporal emission asymmetries between kaons and anti-kaons [S.Soff et al., J.Phys.G23,2095(1997);D.Ardouin et al.,Phys.Lett.B446,191(1999)]. Due to the highest branching ratio of Φ meson is KK the ΦΦ residual correlations could be seen from KK correlation function. K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June2008 3

Experimental results CERN-SPS: Pb+Pb at 158 AGeV/c RHIC-STAR: Au+Au sqrt(S NN )=200GeV R = 4.09 ± 0.46(stat.) ± 0.31(sys) fm and λ = 0.92±0.23(stat)±0.13(sys) at the mean transversemass = 1.07 GeV. [PRL,87(2001)112301] [Phys.Rev.C 74 (2006),054902] K+K+K+K+ K0SK0SK0SK0S K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June The duration time Δτ=sqrt(r 2 out -r 2 side )/β= 2.2± 5.2(stat.) ± 5.1(sys) fm

Experimental results II t RHIC-PHENIX: Au+Au sqrt(S NN )=200GeV [M. Heffner J., Phys. G 30 (2004) S1043-S1047], [nucl-ex/ ] an approximately “universal” m T dependence is usually attributed to collective flow KK one dimensional radius 3-5 fm K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June2008 5

ALICE Software and input K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June Aliroot (with AliFemto) v4-12-Rev-02 Local analysis of 3K events PDC2007: HIJING PbPb 5.5 TeV (dN ch /dy~6500 )‏ 1D KK correlations 0.1 < P T < 1.0 GeV/c Anti-splitting cut Gaussian distr.: d 3 N/d 3 r*~ exp(-r* 2 /(4r 0 2 ))‏ KK r 0 : 2 and 5 fm Source size for kaons from K* decay was corrected on v K* τ K* : r' 0 =sqrt(r 0 2 +(v K* τ K* ) 2 )‏

PID K.Mikhaylov,A.Stavinsky ITEP Alice Week, CERN 31March K π p K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June2008 7

K+ Mothers K + direct 38% K K*(892)0 35% K K*(892)+ 19% K Φ 8%, it is two times better than π+ (π + prim /π + all =19%)‏ K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June2008 8

π Mothers Resonances can play significant role for ππ correlations K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June2008 9

Pair PID 100 events TeV HIJING Q INV 45% K dir K dir 7%7222( %)‏ K dir K K* ( %)‏ K dir K K*+ 7652( %)‏ K K*0 K K*+ 39% 8181( %)‏ K K*+ K K*+ 2067( %)‏ K K*0 K K*0 8077( %)‏ K dir K Φ 3129( %)‏ K Φ K Φ 345( %)‏ K K*0 (K K*+ )K Φ 5022( %)‏ Other exotic (K dir K D0,...) 1352( %)‏ (KK) fake 46896( %)‏ Total (100%)‏ K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June

K+K+:Model&”Experiment” Splitting cut was applied K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June

Source “expansion” due to K* K dir K dir source size is smaller than K dir K K* due to K* decay length Assume K* source size the same as K dir K dir (r 0 )‏ Measured source in second case: r' 0 = sqrt(r 0 2 +(vτ) 2 ) [K dir K K* ] or r' 0 = sqrt(r 0 2 +(v 1 τ 1 ) 2 +(v 2 τ 2 ) 2 )[K K* K K* ] Get v of K* from generator (vτ~2.6 fm)‏ K K K*(cτ=4fm)‏ K π K Both K are direct One K is direct and the other one from K* decay r0r0 r measured K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June

K+K+: K* source “expansion”(2fm)‏ ‏ Source “expansion” due to K* decay (r 0 =2fm, K* vτ ~ 2.6fm)‏ r 0 =2fm r' 0 =2.6fm Non Gaussian shape K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June

K + K + : K* “expansion” (5fm)‏ ‏ Source “expansion” due to K* decay (r 0 =5fm, K* vτ ~ 2.6fm)‏ r 0 =5fm r' 0 =5.5fm K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June

K+K-: Model&”Experiment” Φ → K+K-

K+K-: K* “expansion”(2fm)‏ K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June r 0 =2fm r' 0 =2.6fm Non Gaussian shape

ΦΦ residual CF in K+K- K.Mikhaylov,A.Stavinsky ITEP STAR Meeting, Dubna 11June

ΦΦ residual CF in K+K PbPb events Kaons only from K* decay only Need More statistics K 0 K (+/-) is better K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June

Conclusion 1. There are several sources of the KK correlation function “distortion”: Single Kaon purity, Pair purity, Splitting-merging, Resonances 2. K* expansion could be important for KK 3. Study of correlated background to be continued (fake pairs!)‏ 4. K 0 S K +(-) is for ΦΦ residual correlations? Thank you for your attention!

Extra Slides

K+K+:Different contribution K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June

K+K-: Different contribution K.Mikhaylov, A.Stavinsky ITEP STAR Meeting, Dubna 11June With K* Correlated background!!!

Extra Slides Fake contribution to K+K+ Good KK: Fake KK : pi+K+ : pi+pi+ : pK+ : e+K+ : mu+K+ : pi+e+ : ppi+ : others :