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Photoproduction of J/Ψ J/ and high<br />

mass e + e- <strong>in</strong> ultra-peripheral<br />

ultra peripheral Au+Au<br />

<strong>collisions</strong> <strong>at</strong> √sNN NN = 200 GeV with the<br />

----------- experiment<br />

Mickey Chiu<br />

PLB 679 (2009) 321-329


Rel<strong>at</strong>ivistic Heavy Ion Collider,<br />

<strong>at</strong> Brookhaven N<strong>at</strong>ional<br />

Labor<strong>at</strong>ory (NY,USA)<br />

PHOBOS<br />

PHENIX PHENIX<br />

STAR<br />

RHIC experimental facility<br />

BRAHMS<br />

• Characteristics:<br />

• ~4km of circumference,<br />

• Polarized p to Au nuclei<br />

(soon U)<br />

• HIC: √sNN ~ 6-200 GeV<br />

• p+p: √s ~ 6-500 GeV<br />

Energy Density Frontier<br />

(QCD M<strong>at</strong>ter Frontier)<br />

Sp<strong>in</strong> Frontier<br />

ISSP-Erice Mickey Chiu 2/ 16


“Hadronic” Collider Processes<br />

•You’re probably familiar with the “Hadronic Interactions”<br />

•But there are a lot more processes go<strong>in</strong>g on <strong>at</strong> a hadron collider<br />

Hadronic Interaction:<br />

Au-Au --> X 6.8 barns<br />

γ-γ:<br />

AuAu --> AuAu + e + e - 33 kbarns<br />

AuAu --> AuAu + 2(e + e - ) 680 barns<br />

AuAu --> AuAu + 3(e + e - ) 50 barns<br />

γ-N: L(γ-N )=10 29 cm -2 s -1 2 Au*+Au* 3.67±0.26 barns<br />

X+neutrons<br />

Y+neutrons<br />

Hadronic Interaction<br />

Peripheral Interaction<br />

ISSP-Erice Mickey Chiu 3/ 16


Z 1 e<br />

A<br />

v~c<br />

A<br />

Z 2 e<br />

UPC A+A <strong>in</strong>teraction<br />

γ+γ and γ+A Lum<strong>in</strong>osities<br />

b > 2R<br />

RHIC, LHC L γA/L AA<br />

• The electromagnetic field is equivalent to a large flux of quasi-real photons, and<br />

can be calcul<strong>at</strong>ed per (Fermi)-Weizsacker-Williams:<br />

• Can get large flux due to the coherent effect of protons <strong>in</strong> nucleus (~Z 2 )<br />

• Two processes:<br />

1. photon-photon (coherent)<br />

2. photon-nucleon (<strong>in</strong>coherent,photoproduction)<br />

ISSP-Erice Mickey Chiu 4/ 16


γ+γ (Coherent) vs γ+A (Incoherent) Production<br />

“Coherent” “Incoherent”<br />

W max ,γγ~ 6 GeV<br />

RHIC max. CM energy<br />

ω < ωmax<br />

≈<br />

ISSP-Erice Mickey Chiu 5/ 16<br />

γ<br />

R<br />

W max ,γn ~ 34 GeV<br />

Max p T<br />

p T ,γγ < 1/R nuc ~ 100 MeV p T ,γn k<strong>in</strong>. limited<br />

σ(γγ) ∝ Z 4 ~ 4·10 7<br />

Lum<strong>in</strong>osity<br />

σ(γn)∝ Z 2 ~ 6·10 3


γ Au → J/ψ Au* measurement <strong>in</strong> PHENIX<br />

e +<br />

e -<br />

• UPC dedic<strong>at</strong>ed trigger<br />

• Rapidity gap 3


Possible signal and background sources<br />

• Non-physical sources:<br />

� Cosmic rays:<br />

� no vertex, � no ZDC.<br />

� Beam gas <strong>in</strong>teractions:<br />

�no vertex, � large multiplicities.<br />

⇒ Trigger criterion gets rid of those<br />

• Physical sources:<br />

� Peripheral nuclear A+A <strong>collisions</strong>:<br />

� large multiplicities, � large p T .<br />

� Hadronic diffractive (Pomeron-Pomeron, rapidity gap):<br />

� forward proton emission, � larger p T : p T (γγ) < p T (PP),<br />

� expect like-sign pairs too.<br />

⇒ Analysis cuts gets rid of them<br />

� Incoherent UPC: γ+n → n+J/ψ<br />

� wider p T : p T (γγ) < p T (γP), � asymmetry dN/dy,<br />

� >2 neutrons (<strong>in</strong>duced nuclear break-up) w/ same direction as J/Ψ.<br />

� Coherent UPC: γ+γ → e + e - , γ+Α → X+J/ψ, γ+A → jet(s)+A<br />

Sensitive to coherent and <strong>in</strong>coherent UPC<br />

ISSP-Erice Mickey Chiu 7/ 16


The measured <strong>in</strong>variant mass<br />

• 28 unlike-sign pairs and no like-sign pairs of m ee > 2 GeV/c 2<br />

⇒ Clean sample, with zero net charge !<br />

• Invariant mass fit <strong>in</strong>put:<br />

• Coherent cont<strong>in</strong>uum shape derived from theoretical STARLIGHT-MC<br />

<strong>in</strong>put + full detector simul<strong>at</strong>ion and reconstruction<br />

dN/dm e+e- = A · exp( c m e+e- );<br />

γγ→e + e -<br />

γA(n)→J/ψ→e + e -<br />

Simul<strong>at</strong>ed<br />

STARLIGHT<br />

simul<strong>at</strong>ions +<br />

dectector<br />

simul<strong>at</strong>ion &<br />

reconstruction<br />

• J/ψ Gaussian fit shape ⇒ width 155 MeV/c 2 consistent with MC<br />

N(J/ψ) = 9.9 ± 4.1 (st<strong>at</strong>) ± 1.0 (syst)<br />

ISSP-Erice Mickey Chiu 8/ 16


Cont<strong>in</strong>uum component (γ γ→e + e - ) characteristics<br />

γγ→e + e -<br />

γA(n)→J/ψ→e + e -<br />

• N(e + e - ) = 13.7 ± 3.7 ± 1.0<br />

m ee ∈ [2.0,2.8] GeV/c 2<br />

• Slic<strong>in</strong>g <strong>in</strong> mass<br />

• N(e + e - ) = 7.4 ± 2.7 ± 1.0<br />

m ee ∈ [2.0,2.3] GeV/c 2<br />

• N(e + e - ) = 6.2 ± 2.5 ± 1.0<br />

m ee ∈ [2.3,2.8] GeV/c 2<br />

• γγ→e + e - spectra is peaked<br />

<strong>at</strong> very low pt<br />

� p T dist consistent w/<br />

constra<strong>in</strong>t of nucleus form<br />

factor → Evidence of<br />

cont<strong>in</strong>uum e + e - coherent<br />

n<strong>at</strong>ure<br />

ISSP-Erice Mickey Chiu 9/ 16


Cont<strong>in</strong>uum component (γ γ→e + e - ) characteristics<br />

γγ→e + e -<br />

γA(n)→J/ψ→e + e -<br />

• N(e + e - ) = 13.7 ± 3.7 ± 1.0<br />

m ee ∈ [2.0,2.8] GeV/c 2<br />

• Slic<strong>in</strong>g <strong>in</strong> mass<br />

• N(e + e - ) = 7.4 ± 2.7 ± 1.0<br />

m ee ∈ [2.0,2.3] GeV/c 2<br />

• N(e + e - ) = 6.2 ± 2.5 ± 1.0<br />

m ee ∈ [2.3,2.8] GeV/c 2<br />

• γγ→e + e - spectra is peaked<br />

<strong>at</strong> very low pt<br />

� p T dist consistent w/<br />

constra<strong>in</strong>t of nucleus form<br />

factor → Evidence of<br />

cont<strong>in</strong>uum e + e - coherent<br />

n<strong>at</strong>ure<br />

ISSP-Erice Mickey Chiu 10 / 16


Coherent di-electron (γ γ→e + e - ) cross section<br />

• Cross section<br />

STARLIGHT:<br />

WW approx. <strong>in</strong><br />

impact parameter<br />

space with Breit-<br />

Wheeler (LO) eqn<br />

� Results consistent with QED theoretical (STARLIGHT)<br />

calcul<strong>at</strong>ions<br />

• Cave<strong>at</strong>:<br />

Baltz, PRL 100 (2008) 062302<br />

• Recent NLO calcul<strong>at</strong>ions seem to suggest th<strong>at</strong> higher order<br />

corrections would suppress the e + e- cross-section by ~20%<br />

•<br />

•<br />

α ~ ZαEM ~ 0.6<br />

•<br />

for b~1/λe (Compton wavelength)<br />

Schw<strong>in</strong>ger critical field strength (1.5x1016 Zeγ<br />

Emax ~ ~ E Zαγ<br />

2 crit<br />

b 2 3<br />

= m c / he<br />

V/cm)<br />

E crit<br />

ISSP-Erice Mickey Chiu 11 / 16


γγ→e + e -<br />

J/ψ transverse momentum distribution<br />

γA(n)→J/ψ→e + e -<br />

• The low pT J/ψ consistent with the<br />

Au nuclear form factor F<br />

dNee / dpT = A ·pT ·|F(pT )| 2<br />

⇒ coherent (γγ) J/ψ production<br />

• But there seems to be also an<br />

<strong>in</strong>coherent (γn) J/ψ component<br />

� H<strong>in</strong>ts of both coherent &<br />

<strong>in</strong>coherent J/ψ production<br />

ISSP-Erice Mickey Chiu 12 / 16


J/ψ cross section vs theoretical calcul<strong>at</strong>ions<br />

⇒ dσ/dy | y=0 = 76 ± 31 (st<strong>at</strong>) ±15 (syst) µb<br />

<strong>in</strong>coherent<br />

coherent<br />

[ 1) P.R.L.89 012301 (2002)…]<br />

[ 2) P.L.B626 (2005) 72 ]<br />

[ 3) arXiv0706.2810 [hep-ph] ]<br />

[ 4) arXiv:0706.1532 [hep-ph] ]<br />

[ 1) ]<br />

[ 2) ]<br />

[ 3) ]<br />

[ 4) ]<br />

• Comp<strong>at</strong>ible with coherent<br />

predictions,<br />

• Sensitive to the shadow<strong>in</strong>g<br />

parameteriz<strong>at</strong>ions,<br />

• but... measured pt spectra<br />

suggests both coherent (γΑ) and<br />

<strong>in</strong>coherent (γN) J/ψ production<br />

coherent<br />

[Filho et al, PRC78 044904 (2008)]<br />

ISSP-Erice Mickey Chiu 13 / 16


• Rough comparison with HERA e-p d<strong>at</strong>a, if coherent <strong>in</strong>coherent<br />

r<strong>at</strong>io is 50% - 50%<br />

• HERA (H1 & ZEUS) <strong>in</strong>put<br />

• Result:<br />

Comparison with HERA d<strong>at</strong>a<br />

• αcoh = 1.01 ± 0.07<br />

• α<strong>in</strong>coh = 0.92 ± 0.08<br />

[ZEUS, Eur.Phys.J. C24 (2002) 345]<br />

[H1, Eur.Phys.J. C46 (2006) 585]<br />

⇒ α ~ 1, good agreement with HERA d<strong>at</strong>a hard probes scal<strong>in</strong>g<br />

ISSP-Erice Mickey Chiu 14 / 16


γ+γ, γ+p, γ+A “Applic<strong>at</strong>ions”<br />

•Higgs as well as many SUSY ptcls should be produced <strong>at</strong> the LHC <strong>in</strong> γ+γ and γ+p (γ+A)<br />

•High energy photon <strong>in</strong>teractions <strong>at</strong> the LHC, de Jeneret et al, arXiv:0908.2020<br />

•FP220, FP420<br />

•Observ<strong>at</strong>ion of exclusive charmonium production and gamma+gamma to mu+mu- <strong>in</strong> <strong>p+pbar</strong><br />

<strong>collisions</strong> <strong>at</strong> <strong>sqrt</strong>{s} = 1.96 TeV, CDF, PRL102:242001,2009<br />

Nucleus-Nucleus Interactions<br />

−2<br />

10<br />

2 2<br />

x = mJ<br />

/ Ψ / WγA<br />

= 1.<br />

5x<br />

•Direct measurement of G(x) <strong>at</strong> from photoproduction (σ~g 2 (x))<br />

10 -3 10 -2 10 -1 10 -3 10 -2 10 -1 10 -3 10 -2 10 -1<br />

EPS09: A New Gener<strong>at</strong>ion of NLO and LO Nuclear PDF’s, Eskola,Paukannen,Salgado JHEP 0904:065 2009<br />

•Possibly study dynamics of J/Ψ propag<strong>at</strong>ion through nuclear m<strong>at</strong>ter<br />

•Fe<strong>at</strong>ure or Bug?<br />

•Test of QED <strong>in</strong> strong-coupl<strong>in</strong>g regime?: α=Zα EM ~0.6<br />

ISSP-Erice Mickey Chiu 15 / 16<br />

x


γ+γ, γ+p, γ+A “Applic<strong>at</strong>ions”<br />

•Higgs as well as many SUSY ptcls should be produced <strong>at</strong> the LHC <strong>in</strong> γ+γ and γ+p (γ+A)<br />

•High energy photon <strong>in</strong>teractions <strong>at</strong> the LHC, de Jeneret et al, arXiv:0908.2020<br />

•FP220, FP420<br />

•Observ<strong>at</strong>ion of exclusive charmonium production and gamma+gamma to mu+mu- <strong>in</strong> <strong>p+pbar</strong><br />

<strong>collisions</strong> <strong>at</strong> <strong>sqrt</strong>{s} = 1.96 TeV, CDF, PRL102:242001,2009<br />

Nucleus-Nucleus Interactions<br />

−2<br />

10<br />

2 2<br />

x = mJ<br />

/ Ψ / WγA<br />

= 1.<br />

5x<br />

•Direct measurement of G(x) <strong>at</strong> from photoproduction (σ~g 2 (x))<br />

PHENIX UPC J/Psi<br />

10 -3 10 -2 10 -1 10 -3 10 -2 10 -1 10 -3 10 -2 10 -1<br />

EPS09: A New Gener<strong>at</strong>ion of NLO and LO Nuclear PDF’s, Eskola,Paukannen,Salgado JHEP 0904:065 2009<br />

•Possibly study dynamics of J/Ψ propag<strong>at</strong>ion through nuclear m<strong>at</strong>ter<br />

•Fe<strong>at</strong>ure or Bug?<br />

•Test of QED <strong>in</strong> strong-coupl<strong>in</strong>g regime?: α=Zα EM ~0.6<br />

ISSP-Erice Mickey Chiu 16 / 16<br />

x


γ+γ, γ+p, γ+A “Applic<strong>at</strong>ions”<br />

•Higgs as well as many SUSY ptcls should be produced <strong>at</strong> the LHC <strong>in</strong> γ+γ and γ+p (γ+A)<br />

•High energy photon <strong>in</strong>teractions <strong>at</strong> the LHC, de Jeneret et al, arXiv:0908.2020<br />

•FP220, FP420<br />

•Observ<strong>at</strong>ion of exclusive charmonium production and gamma+gamma to mu+mu- <strong>in</strong> <strong>p+pbar</strong><br />

<strong>collisions</strong> <strong>at</strong> <strong>sqrt</strong>{s} = 1.96 TeV, CDF, PRL102:242001,2009<br />

Nucleus-Nucleus Interactions<br />

−2<br />

10<br />

2 2<br />

x = mJ<br />

/ Ψ / WγA<br />

= 1.<br />

5x<br />

•Direct measurement of G(x) <strong>at</strong> from photoproduction (σ~g 2 (x))<br />

PHENIX UPC J/Psi<br />

10 -3 10 -2 10 -1 10 -3 10 -2 10 -1 10 -3 10 -2 10 -1<br />

EPS09: A New Gener<strong>at</strong>ion of NLO and LO Nuclear PDF’s, Eskola,Paukannen,Salgado JHEP 0904:065 2009<br />

•Possibly study dynamics of J/Ψ propag<strong>at</strong>ion through nuclear m<strong>at</strong>ter<br />

•Fe<strong>at</strong>ure or Bug?<br />

•Test of QED <strong>in</strong> strong-coupl<strong>in</strong>g regime?: α=Zα EM ~0.6<br />

ISSP-Erice Mickey Chiu 17 / 16<br />

x


Summary<br />

• First measurement of J/ψ→e + e - photo-production and of twophoton<br />

production of high-mass e + e - <strong>in</strong> nucleus-nucleus<br />

<strong>in</strong>teractions<br />

• Other hadron collider measurements: CDF(J/Ψ,Ψ’…), STAR (ρ)<br />

• Test<strong>in</strong>g of our understand<strong>in</strong>g of these processes<br />

• Coherent vs Incoherent<br />

• Does DESY experience transl<strong>at</strong>e to hadron-hadron colliders?<br />

• Indic<strong>at</strong>ions are th<strong>at</strong> it does<br />

• How to trigger (experimental issues)<br />

• Good progress on this issue<br />

• Important for<br />

• Future searches for new physics <strong>in</strong> diffractive p+p and Pb+Pb <strong>at</strong> LHC<br />

• Can reach mass <strong>at</strong> TeV scales – good sensitivity to Higgs and SUSY<br />

• Constra<strong>in</strong>ts on QCD background to above searches by measurement<br />

of g(x) and g A (x) <strong>at</strong> low x<br />

• Gluon S<strong>at</strong>ur<strong>at</strong>ion<br />

• Understand<strong>in</strong>g J/Ψ propag<strong>at</strong>ion through nuclear m<strong>at</strong>ter?<br />

• Tests of EM <strong>in</strong> strong coupl<strong>in</strong>g regime – Reaches Schw<strong>in</strong>ger Limit<br />

ISSP-Erice Mickey Chiu 18 / 16

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