Simulation of DVCS with an EIC using MILOU Salvatore Fazio BNL g* p g p University of Washington – INT Seattle, WA – USA November 1-13, 2010
Download ReportTranscript Simulation of DVCS with an EIC using MILOU Salvatore Fazio BNL g* p g p University of Washington – INT Seattle, WA – USA November 1-13, 2010
Simulation of DVCS with an EIC using MILOU Salvatore Fazio BNL g* p g p University of Washington – INT Seattle, WA – USA November 1-13, 2010 Planing of the talk The eRHIC accelerator and an EIC detector compared to HERA Strategy of a DVCS measurement Hera results Extension to EIC DVCS simulation for an EIC Summary Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 2 From HERA to an EIC collider 27.5 GeV electrons/positrons on 920 GeV EIC/eRHIC protons →√s=318 GeV 2 colliding experiments: H1 and ZEUS Polarized egun Beamdump eRHIC detector 6 pass 2.5 GeV ERL Total lumi collected at HERA: 500 pb-1, polarization of electrons/positrons at HERA II HERA STAR 20 - 30 GeV electrons on 325 (125) GeV protons (nuclei). Polarization of electrons and protons (nuclei) Lumi: 1.4 x 1034 cm-2s-1 For exclusive diffraction the concept is similar to HERA but: • Dedicated forward instrumentation • Higher tracker coverage • Very High lumi! Detectors not originally designed for forward physics, Roman pots added later S. Fazio: INT-workshop, Univ. of Nov. 9, 2010 Washington, Seattle 3 The EIC detector p/N e REAR FORWARD Estimated b*≈ 8 cm pc/2.5 Similarities with HERA detectors: • Hermetic • Asymmetric 4.5 cm neutrons 11.2 cm e IP q=10 mrad 2 Nov. 9, 2010 4 6 8 Dipole: 2.5 m, 6 T q=18 mrad 10 12 Important (as respect of HERA) improvements: • Central Tracking Detector • better em calorimeter resolution • Very forward calorimetry • Rear Trackers! • Roman pots from the early biginning 14 16 Quad Gradient: 200 T/m S. Fazio: INT-workshop, Univ. of Washington, Seattle 4 20 0.44 m 0.329 m 0.188036 m 10 30 GeV e- 30 60 m 90 m © D.Trbojevic Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 5 Deeply Virtual Compton Scattering γ* VM (ρ, ω, φ, J/ψ, Υ) V γ* DVCS (γ) IP p p p p Scale: Q2 + M2 γ Q2 DVCS properties: • Similar to VM production, but γ instead of VM in the final state • No VM wave-function involved • Important to determine Generalized Parton Distributions sensible to the correlations in the proton • GPDs are an ingredient for estimating diffractive cross sections at LHC Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle GPD GPD 6 Accessing the GPDs quantum number of final state selects different GPDs: theoretically very clean ~ ~ DVCS (g): H, E, H, E VM (r, w, f): H E info on quark flavors ~ ~ PS mesons (p, h): H E 1 1 z z J q + J g Dq + Lzq + J gz 2 2 q q 1 z J q Dq + Lzq 2 q q 1 1 z q q Jq x dx H + E t0 2 -1 Nov. 9, 2010 ) S. Fazio: INT-workshop, Univ. of Washington, Seattle p0 h 2Du+Dd 2Du-Dd ρ0 ω f ρ+ 2u+d, 9g/4 2u-d, 3g/4 s, g J/ψ g u-d 7 DVCS @ ZEUS - Strategy DVCS BH e e g g* p p g sample: no tracks matching to the second candidate e sample: a track match to the second candidate Wrong-sign sample: a negative track match to the second candidate Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle (DVCS+BH) (BH+ dilepton + J/) (dilepton + J/) 8 DVCS @ HERA Fit: σ ~ Wδ Q2 dependence for the W slope not clear within the uncertainties! ZEUS: JHEP05(2009)108 H1: Phys.Lett.B659:796-806,2008 t measured indirectly: 2 2 t ~ PTg + PT2 e Nov. 9, 2010 d e -b |t | dt by roman pots! Fit : No evidence for W dependence of b S. Fazio: INT-workshop, Univ. of Washington, Seattle 9 t dependence The ZEUS result is in agreement with H1 b = 4.5 ± 1.3 ± 0.4 …nevertheless it seems to suggest a lower trend! dσ/dt measured for the first time by a direct measurement of the outgoing proton 4-momentum using the LPS spectrometer Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 10 W-dependence: summary Summary of the W,t-dependence for all VMs + DVCS measured at HERA Fit: σ ~ Wδ Fit : d e -b |t | dt Exclusive production of VMs can be a golden measurement for an EIC Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 11 Measuring t indirectly with an EIC To successfully measure t indirectly from the electron and photon candidates t ~ PT2g +PT2 2 e it is important: Tracker coverage (tracker has higher momentum resolution than Cal!) Reso of the CTD @ ZEUS: σ(pT)/pT =0.0058pT⊕0.0065⊕ 0.0014/pT DVCS/BH CTD acceptance @ ZEUS BH Always measure a track when we can -> better momentum resolution but not only… More acceptance for DVCS! High resolution em calorimetry (crucial! Remember that one particle is a photon!) For ZEUS it was σ(E)/E=0.18/√E Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 12 Direct t measurement at EIC But… is an indirect measurement of t really an issue for EIC? We’ll get roman pots in the forward region at EIC! Silicon micro-strips resolution: 0.5% for PL ; 5 MeV for PT L = 27.77 pb-1 55 events (DVCS + BH) EIC lumi for eRHIC: 1.4 1034* Ep/325 cm-2s-1 assuming 50% operations efficiency one week corresponds to: L(1 w)= 0.5 * 604800(s in a week) * (1.4x1034 cm-2s-1) = 4*1039 cm-2 = 4000pb-1 + Roman Pots ~ 8000 events/week !! assuming the same acceptance ad LPS (~2%) Calculations are absolutely not rigorous! But give an idea… Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 13 t vs proton scattering angle t=(p4-p2)2 = 2[(mpin.mpout)-(EinEout - pzinpzout)] t=(p3–p1)2 = mρ2-Q2 - 2(Eγ*Eρ-pxγ*pxρ-pyγ*pyρ-pzγ*pzρ) 4 GeV el x 50 GeV prot 4 x 100 very strong correlation between t and “recoiling” proton angle Roman pots need to be very well integrated resolution on t! Nov. 9, 2010 4 x 250 S. Fazio: INT-workshop, Univ. of Washington, Seattle 14 MILOU Written by E. Perez, L Schoeffel, L. Favart [arXiv:hep-ph/0411389v1] The code MILOU contains two different models for DVCS simulation: FFS d dxdQ2 dt 3 DVCS Based on: Frankfurt, Freund and Strikman (FFS) [Phys. Rev. D 67, 036001 (1998). Err. Ibid. D 59 119901 (1999)] p 2 3 s 1 + 1 - y ) 2 2 2xR Q 6 )e -b t F22 x,Q2 )1 + r 2 ) • Old model: written before data came out! • Used by H1 and ZEUS for their DVCS measurements • The ALLM parametrization for F2 is used Based on: A. Freund and M. McDermott All ref. in: http://durpdg.dur.ac.uk/hepdata/dvcs.html GPDs-based • GPDs, evolved at NLO by an indipendent code which provides tables of CFF - at LO, the CFFs are just a convolution of GPDs: ei2 H (,Q ,t) = -1 -Hi x, ,Q2,t )dx 1 - x - i u,d,s 2 Nov. 9, 2010 1 S. Fazio: INT-workshop, Univ. of Washington, Seattle 15 MILOU • provide the real and imaginary parts of Compton form factors (CFFs), used to calculate cross sections for DVCS and DVCS-BH interference. d 3 xB y I = dxdyd| t | dfd 16p 2Q2 1+ 2 e 3 I BH 2 I DVCS f = fN - f l = T - f N 2x mN Q BH 2 BH e6 BH 2 2 c 0 + c n cosnf ) + s1 sinf ) 2 2 2 x y (1+ ) D P1 (f )P2 (f ) n 1 2 2 e 6 DVCS DVCS DVCS 2 2 c 0 + c n cosnf ) + sn sinnf ) yQ n 1 I 3 I e 6 I c + c cosnf ) + s1 sinf ) I 3 2 xy D P1 (f )P2 (f ) 0 n 1 n 2 • The B slope is allowed to be costant or to vary with Q2: ) d d t exp BQ2 )t ; with : BQ2 ) lnQ2 ) • Proton dissociation (ep → eγY) can be included Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 16 Phase space • 1.5 < Q2 < 100 GeV2 • 10-4 < x < 0.1 • 0.01 < y < 0.85 • 0 < |t| < 1.5 GeV2 • Radiative corrections: OFF • t slope: B = 5.00 (costant) • GPDs evolved at NLO • ALLM param. used for F2 (FFS model) 100 k event generated for each config. 30 X 325: • E_el = 10 GeV ep -> egp)= 0.186 nb (FFS_ALLM) ep -> egp)= 0.376 nb (GPDs) 20 X 250: • E_el = 5 GeV ep -> egp)= 0.16 nb (FFS_ALLM) ep -> egp)= 0.32 nb (GPDs) 10 X 100: • E_el = 0 GeV ep -> egp)= 8.1*10-2 nb (FFS_ALLM) ep -> egp)= 0.16 nb (GPDs) 5 X 50: • E_el = 0 GeV ep -> egp)= 8.1*10-2 nb (FFS_ALLM) ep -> egp)= 0.16 nb (GPDs) eRHIC Luminosity Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 17 qg vs Eg 30 X 325 Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 18 qg vs Eg 20 X 250 Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 19 qg vs Eg 10 X 100 Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 20 qg vs Eg 5 X 50 Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 21 t-xsec (ep -> gp) FFS - 30 X 325 by roman pots! • 1.5 < Q2 < 100 GeV2 • 10-4 < x < 0.1 • 0.01 < y < 0.8 L = 0.54 fb-1 EIC lumi: 4 fb-1/month @ 30x325 Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle • Precision enormously improved • Roman pots acceptance not yet included in the simolation 22 t-xsec GPDs conv. - 30 X 325 • 1.5 < Q2 < 100 GeV2 • 10-4 < x < 0.1 • 0.01 < y < 0.8 Systematics will dominate!! Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 23 t-xsec 20 X 250 10 X 100 5 X 50 dominated by gluon contributions EIC will provide sufficient luminosity to bin in multi-dimensions wide x and Q2 range needed to extract GPDs … we can do a fine binning in Q2 and W! Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 24 Scanning the phase space… 30 X 325 20 X 250 Logarithmic bins: 1 < Q2 < 100 GeV2 10-4 < x < 0.1 10 X 100 Nov. 9, 2010 5 X 50 S. Fazio: INT-workshop, Univ. of Washington, Seattle 25 Scanning the phase space… 30 X 325 20 X 250 10 X 100 5 X 50 Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 26 30x325-t-xsec Veri precice scan! Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 27 20x250-t-xsec GPD Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle FFS 28 10x100 5x50 t-xsec Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 29 DVCS: the beam-charge asymmetry A = ADVCS +ABH +AI 2 2 2 2 Interference term: Beam charge asymmetry: DVCS and BH: identical final state → they Interfere AI ReADVCS )+ImADVCS ) d + - d AC = + - Re ADVCS ) d + d The phi angle At EIC: d+ - d AC = d + + d Nov. 9, 2010 Possible if a positron beam Thanks to a good tracker coverage S. Fazio: INT-workshop, Univ. of Washington, Seattle 30 DVCS on nuclear targets How does the nuclear environment modify parton-parton correlations? How do nucleon properties change in the nuclear medium? DVCS in coherent region: new insights into ‘generalized EMC effect’? (Bethe-Heitler) Nuclear GPDs ≠ GPDs of free nucleon Enhancement of effect when leaving forward limit? caused by transverse motion of partons in nuclei? important role of mesonic degrees of freedom? manifest in strong increase of real part of τDVCS with atomic mass number A? MC simulation for DVCS on nuclei coming soon thanks to an updated version of MILOU code Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 31 Summary A lot of experience carried over from HERA Simulation shows how an EIC forward program can sensibly improve HERA results and go beyond Uncertainties will be dominated by systematics Large potential for diffractive-DIS studies using polarized and unpolarized protons and nuclei Outlook: Simulation of asymmetries Simulation of DVCS on nuclei Updating the MILOU code to status of art (Re_Amp, NNLO…) Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 32 Back up Nov. 9, 2010 S. Fazio: INT-workshop, Univ. of Washington, Seattle 33