ebook img

Total gamma-gamma and gamma*-gamma* Cross Sections Measured at LEP PDF

4 Pages·0.1 MB·English
Save to my drive
Quick download
Download
Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.

Preview Total gamma-gamma and gamma*-gamma* Cross Sections Measured at LEP

1 Total γγ and γ γ Cross Sections Measured at LEP ∗ ∗ Albert De Roecka a CERN, 1211 Geneva 23, Switzerland Recentresultsontotalcross-sectionmeasurementsinγγ andγ∗γ∗ collisionsatLEParereported. Phenomeno- 1 logical fits to thedata are presented. 0 0 2 n 1. Introduction the Monte Carlo model used to correct the data: a J it affects the absolute normalization by approxi- At LEP2 photon-photon collisions constitute 9 mately 20%, as derived from using two different a large part of the inclusive cross-section. models, PYTHIA [3] and PHOJET [4]. An im- 1 Quasi real photons are emitted according to a portantuncertaintyisthediffractivecontribution v Weizs¨acker-Williamsenergyspectrumbythelep- tothecross-section. Sucheventstoalargeextent 6 ton beams. Two photon events can be tagged by escape detection; depending on the model only 7 one or both of the scattered electrons, or anti- 0 6% to 20% of the diffractive events are selected tagged,in which case the electrons remain in the 1 by the standard analysis cuts. 0 beampipe. Tagging detectors measure electrons In Fig. 1 data on σ from the LEP and pre- γγ 1 typically down to 30 mrad. In this paper we re- LEPexperimentsareshown,comparedtovarious 0 port results on anti-tagged (i.e. almost real pho- theoreticalmodelsasreviewedin[5]. ThenewL3 / ∗ ∗ h tonγγ)anddoubletagged(i.e.γ γ )totalcross- dataarestillpreliminaryandareacombinationof p sectionmeasurements. Theanalysesarebasedon - approximately 390 pb−1, from e+e− data taken data takenat√see =189and192−202GeV[6]. p Contrary to previously published data [1], these e at √see =189−202 GeV in ’98 and ’99. data are determined using both PHOJET and h PYTHIA, and are therefore above published val- : v ues. The cross-section clearly rises with increas- 2. Total γγ Cross-Section Xi ing Wγγ. The OPAL and L3 data are consistent Photons at high energies can fluctuate in two- with each other. This is less so for the pre-LEP r a fermion pairs or vector mesons with the same data [7],of whichonlya selectionis shownin the JPC quantum numbers as for the photon. Hence figure. a photon can behave like a hadron, with an All models predict a rise with the collision en- additional pointlike component. Total inclusive ergy, but the strength of the rise differs and the hadron-hadron cross-sections are known to rise predictions at high energy show dramatic differ- gentlywiththecentre-of-mass(CMS)energy. An ences. In proton-like-models (dash-dotted [8–10], outstanding question is whether σ rises faster dashed[11],dotted[12]andsolid[13]curves),the γγ than σ , expected from the additional pointlike curvature follows closely that of proton-proton pp component in the photon structure. cross-section, in QCD based models (upper [14] LEP allows to study γγ interaction cross- and lower [5] bands), the rise is obtained using sectionasfunctionoftheCMSenergyW . L3[1] the pQCD jet cross-section. γγ and OPAL [2] have measured σ in the region A large contribution to the errors of the cross- γγ 5 < W < 145 GeV and 10 < W < 110 section is due to the uncertainty of the model γγ γγ GeV respectively. The challenge of this measure- dependent correction factors, which are strongly ment is the reconstruction of W from the vis- point-to-point correlated and partially hide the γγ ible hadronic final state. The result depends on 2 1000 800 Regge/Pomeron, SaS L3 preliminary 900 GLMN BKKS BSW 800 Aspen EMM 700 600 600 (nb)tot500 ]b s n 400 [ 400 300 gg s 200 TPC Desy 1984 1999 data 100 LEP2-L3 189 GeV and DESY 86 200 1998 data 192-202 GeV LEP2-OPAL 189 GeV OPAL 1 10 √s (GeV)102 103 0 Figure 1. Data on σγγ, versus Wγγ (denoted as 50 100 150 √s) compared with models (see text). W [GeV] gg Figure 2. Data on σ from OPAL and L3, com- γγ pared with fits through the data (see text). significanceoftheriseofthecross-section. There- fore Fig. 2 shows the L3 data without the model dependent errors. The size of the rise is quanti- fied by a Regge inspired fit, X sǫ1 +Y s−η1, 1 1 · · i.e. the sum of a pomeron and a Reggeon term. L3findsY 1000nbfromitsownfits. Hencewe 1 ∼ The exponents ǫ1 = αIP 1 and η1 = αR 1 made fitsusingthe publishedOPALandprelimi- − − are usually assumed to be universal, whereas the narynewL3datapoints,ignoringcorrelationsbe- coefficients are process dependent. For η1, which tweenthepointsandignoringtheuncertaintydue is determined by low energy hadronic data, the to the model dependence. Refitting the OPAL value of 0.34 is taken [15]. αIP and αR are the data but with Y1 as determined by L3, one finds pomeron and Reggeon intercept, respectively. ǫ =0.205 0.042(χ2/NDF =1/3). Refittingall 1 ± For its fits, OPAL fixed the coefficient of the the data,leavingY free,givesǫ =0.238 0.029 1 1 ± Reggeon term, while L3 fitted the magnitude of (χ2/NDF = 2.7/9). Is this rise driven by the Y1. The L3 fit yields for the pomeron term: point at largest Wγγ from L3? Removing this ǫǫ11 ==0.01.0216+−300±..0022500.[021].4T[6h]ewcuhrilveesOsPhoAwLtphuebLli3shfietds pnooinsitgnfriofimcanthtechfiatnggieveosfǫt1h=e e0x.p22o3ne±nt0..033,hence withfree(solidline)andfixed(dashedline)value The correspondingvalueforǫ inhadroniccol- 1 of ǫ1,(ǫ1 = 0.095). Correlations between the lisions is in the range 0.08 0.095, hence the γγ − pointsaretakenintoaccountinthesefits. L3ob- cross-section appears to rise significantly faster servedthatthevalueofǫ1doesnotdependsignif- than hadron cross-sections. icantlyonthemodelusedforcorrectingthedata. Recently, Donnachie-Landshoff [16] proposed TheslopefoundbyOPALisconsiderablysmaller a model which includes two pomeron terms in than the L3 one, despite agreement between the an attempt to save the universality of the soft data points. This can be traced back to the as- pomeron. Thetotalcross-sectionisthenassumed sumption on the Regge coefficient, Y1, which is to be described by fixedbyOPALduetoabsenceofitsownmeasure- ments below W =10GeV toa value of320nb. σ =X sǫ1 +X sǫ2 +Y s−η1, (1) γγ 1 2 1 3 The second pomeron term was added mainly to describe the γ∗p data. From fits to pp and γ(∗)p 183GeV data the exponents ǫ = 0.0808 ǫ = 0.418 and 189-202GeV 1 2 1 η = 0.34 are extracted. An intriguing ques- PHOJET 1 tion is whether the X term is present in the γγ ) QPM 2 b data. A fit, as described above, to the prelim- (p -1 Y 10 inary L3 data with Wγγ > 20 GeV, and with d two pomerons only, gives X2 = 2.5 0.6 nb, /ee ± withχ2/NDF =4.5/3. FittingallOPALandL3 sd -2 10 data to the full expressionof eq.( 1), keeping the ǫ ,ǫ and η fixed, gives X =5.0 0.9 nb, with 1 2 1 2 ± L3 Preliminary χ2/NDF =2.3/9. Hence,withinthismodel,and -3 10 within the restrictions of the fits made, the extra 2 3 4 5 6 hard pomeron term appears to be required in γγ Y=ln(S/S ) 0 data at the 4σ level or higher. Whilethecross-sectioninγγ appearstoberis- ing faster than in pp, the γp cross section can be Figure 3. The ee eeX cross-section for double described by a single pomeron term with expo- → tagged events, measured by L3, compared with nent 0.0808. It is therefore important that the model predictions (see text). rise in the γγ data gets established more thor- oughly. This canbe accomplishedwithmoreand improvedcross-sectionmeasurements in the high W range AND also with better measurements γγ at low W from LEP or elsewhere. The latter γγ is important because the fit result depends sig- OPAL preliminary nAinficeaxnptelyrimonenthteatknVoEwPlePdgineoNfotvhiesiRbiergskgehoanstberemen. []/dY pb10-1 a) scheduled to measure σ at low W . sd γγ γγ -2 10 OPAL QPM 3. Total γ∗γ∗ Cross-Section PHOJET Kwiecinski et al. -3 10 The study of virtual photon-photon scattering 0 1 2 3 4 5 6 Y has recently been discussed as a definite probe []Y nb b) oevfotlhuetiohnaredqu(aBtFioKnLd)espcormibeersosnca[t1t7e]r.inTghperoBceFsKseLs sd/dgVgV10 in QCD in the limit of large energies and fixed, but sufficiently large momentum transfers. The 1 Kim99 Bartels99 BFKLpomeronhasbeenintensivelyinvestigated 0 1 2 3 4 5 6 in the context of small–x deep inelastic electron- Y proton scattering at HERA. However, despite clear hints [18], the presence of so called ln1/x terms in deep inelastic scattering at HERA has Figure 4. The γ∗γ∗ cross-section, measured by not been unambiguously established yet. OPAL, compared with model predictions (see ∗ ∗ The γ γ cross-section has been advocated as text). anexcellentmeasurementtoseelow-xorsocalled BFKLeffects[19,20]. Thesemeasurementscanbe performed by tagging both scattered electrons, which forces the virtuality of both photons to 4 be in the multi-GeV region. New measurements REFERENCES from L3 [21] and OPAL [22] of the double tag 1. L3 Collab., M. Acciarri et al., Phys. Lett. cross-sectionareshownas function of the ’length B408 (1997) 450. of the gluon ladder Y’ in Fig. 3 and Fig. 4. Here 2. OPAL Collab., G. Abbiendi et al, Eur.Phys. Y = lns/s and s = pQ2Q2/(y y ). The mea- 0 0 1 2 1 2 J. C14 (2000) 199. surements are made for the region 34 < θ < 55 e 3. T. Sjo¨strand, Comp. Phys. Commun. 82 mrad,E >0.4E (OPAL)and30mrad<θ , e beam e (1994) 74; LU-TP-95-20(1995). E > 40 GeV (L3), which leads to an average e Q2 of 17 (OPAL) and 15 (L3). L3 observes 4. R.EngelandJ.Ranft,Phys.Rev.D54(1996) h i h i 4244. thatthecross-sectionislargerthantheQPMand 5. R.M. Godbole and G. Pancheri, hep- PHOJET 1.05 (which does not contain BFKL) ∗ ∗ ph/0010104. predictions. L3furtherfitstheγ γ cross-section to σγ∗γ∗ = σ0/pQ21Q22Y ·(s/s0)αIP−1, and finds 67.. LS.3SCo¨oldllnaebr.-,RIeCmHbEoPld,20h0e0p,-eOxs/a0k0a0,9P02652.2. α = 0.36 0.02, i.e. considerably larger than IP ± 8. S. Schuler and T. Sjostrand, Z. Phys. C68 the pomeron term in γγ. The OPAL data are (1995) 607. above the QPM and PHOJET1.10 predictions, 9. A. Corsetti, R.M. Godbole and G. Pancheri, but much less significantly than the L3 data. A Phys. Lett. B435 (1998) 441. possible difference is the sensitivity to radiative 10. A. Donnachie and P. V. Landshoff, corrections of the two measurements [22]. The Phys. Lett. B296 (1992) 227. OPAL measurement was optimized to minimize 11. T.T. Wu, Mod. Phys. Lett. A15 (2000) 9. these effects. 12. E. Gotsman, E. Levin, U. Maor, E. Naftali, The LO BFKL calculation (Bartels99) is con- Eur. Phys. J. C14 (2000) 5. siderably above the data at large Y. Better 13. M. Block, E. Gregores, F. Halzen and G. descriptions are found when NLO corrections Pancheri, Phys. Rev. D60 (1999) 54024. are taken into account (Kim99, Kwiecinski et 14. B. Badelek, M. Krawczyk, J. Kwiecinski and al.) [23,24]. In particular the calculation of [24], M. Stasto, hep-ph/0001161. whichpredictsmoderateBFKLeffectsintheLEP 15. Review of Particle Physics, Phys. Rev. D54 region, describes the data well. (1996) 191. 16. A. Donnachie, P.V. Landshoff, Phys. Lett. 4. Conclusion B437 (1998) 408. 17. E.A.Kuraev, L.N.Lipatov and V.S.Fadin, The total γγ cross-section measurements from Sov. Phys. JETP 45 (1977) 199; LEPshowanintriguingrisewithincreasingW . γγ I.I.Balitski and L.N.Lipatov, Sov. J. Nucl. Thereisnowsomeevidencethatthisriseisfaster ∗ ∗ Phys. 28 (1978) 822. thaninhadron-hadroninteractions. Inγ γ scat- 18. A.M.Cooper,R.C.E.Devenish,A.DeRoeck, tering there is evidence in the L3 data that the Int. J. Mod. Phys A13 (1998) 3385. cross-sectionisaboveexpectationwhennoBFKL 19. J.Bartels,A.DeRoeck,H.LotterPhys.Lett. effects are taken into account. The evidence in B389 (1997) 742; the OPAL data is broadly consistentwith the L3 J. Bartels et al., hep-ph/9710500. observationbutthesignificanceoftheexcessover 20. S.J. Brodsky, F. Hautmann and D.E. Soper, non-BFKL calculations is weaker. Phys Rev. D56 (1997) 6957. 21. L3 Collab., M. Acciarri et al., Phys. Lett. B 5. Acknowledgement 453 (1999) 333; ICHEP 2000, Osaka, P587. 22. M. Przybycien, talk at Photon2000. Ithanktheorganizersofthisinterestingconfer- 23. S. J. Brodsky et al., JETP Lett. 70 (1999) ence for there hospitality and support, and Ste- 155; V. Kim, private communication. fan So¨ldner-Remboldfor a carefulreading of this 24. J. Kwiecinski, P. Motyka, hep-ph/0010029. manuscript.

See more

The list of books you might like

Most books are stored in the elastic cloud where traffic is expensive. For this reason, we have a limit on daily download.