ZEUS fits-report request for preliminary April 3rd 2006

Slides:



Advertisements
Similar presentations
Luca Stanco - PadovaEW and NP at HERA, Photon EW at HERA Luca Stanco – INFN Padova on behalf of ZEUS and H1 collaborations and RELATED NEW PHYSICS.
Advertisements

High Energy neutrino cross-sections HERA-LHC working week Oct 2007 A M Cooper-Sarkar, Oxford Updated predictions of high energy ν and ν CC cross-sections.
ZEUS high Q 2 e + p NC measurements and high-x cross sections A.Caldwell Max Planck Institute for Physics On behalf of the ZEUS Collaboration Allen Caldwell.
ISDM 2005, Kromeriz Kamil Sedlak, Jets in photoproduction at HERA 1 Jets in Photoproduction & at low Q 2 at HERA On behalf of the H1 and ZEUS Collaborations.
Report on fitting FINAL new data: e- CC (175pb -1 : P=0.30, 71pb -1, P=-0.27, 104pb -1 )(DESY ) e- NC (169pb -1, P=+0.29, P=-0.27)(DESY ) Now.
QCD Studies at HERA Ian C. Brock Bonn University representing the ZEUS and H1 Collaborations.
H1/ZEUS fitters meeting Jan 15 th 2010 Am Cooper-Sarkar Mostly about fitting the combined F2c data New work on an FFN fit PLUS Comparing HERAPDF to Tevatron.
Tobias Haas: Recent results from HERA The Dynamics of Proton Structure: Recent Results from HERA 23 August, 2005 Tobias Haas Deutsches Elektronensynchrotron.
M.KapishinDiffraction and precise QCD measurements at HERA 1 Rencontres de Moriond QCD 2012 M.Kapishin, JINR on behalf of the H1 and ZEUS Collaborations.
EW Corrections for CMS Z and Drell-Yan Measurements Dimitri Bourilkov University of Florida For the CMS Collaboration Working Group on Electroweak precision.
The New HERAPDF Nov HERA SFgroup AM Cooper-Sarkar Appears compatible with HERAPDF0.1 when doing fits at Q20=4.0 GeV2 But humpy gluon is Chisq favoured.
A few slides to summarise what Alessandro and I were up to for March 24th video meeting Taking for granted that W+/- are good measurements to make- are.
Predictions for high energy neutrino cross-sections from ZEUS-S Global fit analysis S Chekanov et al, Phys Rev D67, (2002) The ZEUS PDFs are sets.
Constraints on the Scale of New Physics Phenomena from the Combined LEP II  f f and γγ Measurements Dimitri Bourilkov University of Florida for the LEP.
Possibility of tan  measurement with in CMS Majid Hashemi CERN, CMS IPM,Tehran,Iran QCD and Hadronic Interactions, March 2005, La Thuile, Italy.
PDF fits with free electroweak parameters Overview of what has happened since March’06 Collaboration meeting Emphasis on the NC couplings au,vu,ad,vd and.
ICHEP'06, V. Chekelian, NC DIS at HERA1 Vladimir Chekelian (MPI for Physics, Munich) e  p 27.5 GeV 920 GeV  s = 318 GeV DIS & NC & Polarisation.
Searches for the Standard Model Higgs at the Tevatron presented by Per Jonsson Imperial College London On behalf of the CDF and DØ Collaborations Moriond.
NEW RESULTS FROM JET PHYSICS AT HERA Thomas Schörner-Sadenius Hamburg University 2 nd HERA-LHC Workshop June 2006.
DIJET (and inclusive-jet) CROSS SECTIONS IN DIS AT HERA T. Schörner-Sadenius (for the ZEUS collaboration) Hamburg University DIS 06, April 2006 Tsukuba,
1 EPS2003, Aachen Nikos Varelas ELECTROWEAK & HIGGS PHYSICS AT DØ Nikos Varelas University of Illinois at Chicago for the DØ Collaboration
HERA-LHC workshop 21 st -24 th March 2005 Claire Gwenlan (with the help of Sasha Glazov, Max Klein, Gordana Lastovicka-Medin, Tomas Lastovicka)  Introduction.
NLO QCD fits How far can we get without jet data/HERA-II data? A. M. Cooper-Sarkar March-04 Collaboration Meeting ZEUSNOTE Extended ZEUS-S fits.
More on NLOQCD fits ZEUS Collab Meeting March 2003 Eigenvector PDF sets- ZEUS-S 2002 PDFS accessible on HEPDATA High x valence distributions from ZEUS-Only.
High Q 2 Structure Functions and Parton Distributions Ringberg Workshop 2003 : New Trends in HERA physics Benjamin Portheault LAL Orsay On behalf of the.
Single Top Quark Studies, L. Li (UC Riverside) ICHEP 08, July Liang Li University of California, Riverside for the CDF, DØ and H1 Collaborations.
Treatment of correlated systematic errors PDF4LHC August 2009 A M Cooper-Sarkar Systematic differences combining ZEUS and H1 data  In a QCD fit  In a.
Jets and α S in DIS Maxime GOUZEVITCH Laboratoire Leprince-Ringuet Ecole Polytechnique – CNRS/IN2P3, France On behalf of the collaboration On behalf of.
11 QCD analysis with determination of α S (M Z ) based on HERA inclusive and jet data: HERAPDF1.6 A M Cooper-Sarkar Low-x meeting June 3 rd 2011 What inclusive.
Jet Studies at CDF Anwar Ahmad Bhatti The Rockefeller University CDF Collaboration DIS03 St. Petersburg Russia April 24,2003 Inclusive Jet Cross Section.
H1 QCD analysis of inclusive cross section data DIS 2004, Štrbské Pleso, Slovakia, April 2004 Benjamin Portheault LAL Orsay On behalf of the H1 Collaboration.
XXI Physics in Collision Conference Seoul Korea June Christopher M. Cormack Rutherford Appleton Laboratory High Q 2 Physics.
H1 and ZEUS Combined PDF Fit DIS08 A M Cooper Sarkar on behalf of ZEUS and H1 HERA Structure Function Working Group NLO DGLAP PDF fit to the combined HERA.
MSTW update James Stirling (with Alan Martin, Robert Thorne, Graeme Watt)
Top couplings: ILC-B physics interplay Top couplings: ILC-B physics interplay TYL-FJPPL B physics TYL-FJPPL B physics February 20, 2015 LAL February 20,
N. RaicevicMoriond QCD Structure Functions and Extraction of PDFs at HERA Nataša Raičeviċ University of Montenegro On behalf of the H1 and ZEUS Collaborations.
1 Proton Structure Functions and HERA QCD Fit HERA+Experiments F 2 Charged Current+xF 3 HERA QCD Fit for the H1 and ZEUS Collaborations Andrew Mehta (Liverpool.
1 A M Cooper-Sarkar University of Oxford ICHEP 2014, Valencia.
Search for New Physics at HERA Andrea Parenti (DESY) for the H1 and ZEUS collaborations CIPANP 2009 S. Diego, 28/05/2009.
1 Proton Structure and Hard QCD AM Cooper-Sarkar, Oxford Phys Rev D93(2016)
Multilepton production at HERA
Lecture -3.
WW CROSS SECTIONS AND |Vcs| On behalf the LEP collaborations
Michigan State University
Global QCD Analysis and Collider Phenomenology — CTEQ
Charged Current Cross Sections with polarised lepton beam at ZEUS
Status of the HERA-B Analysis 58th PRC Open session, May 26, 2005
News from HERAPDF A M Cooper-Sarkar PDF4LHC CERN March
Sílvia Bravo i Gallart IFAE, Barcelona Moriond-QCD, 18 March 2002
New processes? New ideas
The two-Higgs-doublet model implementation in MadGraph v4
Measuring Fine Tuning Peter Athron In collaboration with David Miller.
- Structure of Matter and QCD
HERA I - Preliminary H1 and ZEUS QCD Fit
Treatment of heavy quarks in ZEUS PDF fits
HESSIAN vs OFFSET method
W Charge Asymmetry at CDF
Electroweak Results from DØ
PDF4LHC: LHC needs February 2008 A M Cooper-Sarkar, Oxford
ATLAS 2.76 TeV inclusive jet measurement and its PDF impact A M Cooper-Sarkar PDF4LHC Durham Sep 26th 2012 In 2011, 0.20 pb-1 of data were taken at √s.
Physics at LHC: Selected results from EW sector and news on Run II
Charged Current Cross Sections with polarised lepton beam at ZEUS
An Introduction to HERA Physics
Top mass measurements at the Tevatron and the standard model fits
Hadronic Final states and extraction of αs and parton densities
Heavy Flavour Content of the Proton
ZEUS High Q2 data from HERA-II +PDF fits
- Structure of Matter and QCD
- Structure of Matter and QCD
Trijets in Neutral Current Deep Inelastic Scattering
Presentation transcript:

ZEUS fits-report request for preliminary April 3rd 2006 A.M.Cooper-Sarkar and C. Gwenlan – team-1 K.Nagano and S. Shimizu – team -2 Web page:http://www-pnp.physics.ox.ac.uk/~cooper/polarised/ewfit.html Report on fitting new data on e- CC and NC polarised Improvement to PDF uncertainties Electroweak parameter fits: MW , MW/ GF ,MW/ g Electroweak NC couplings: au ad vu vd and T3uL/R, T3dL/R sin2ƏW

Including the new data in the standard PDF fit formalism Request preliminary New CC e- data with –ve polarisation P= -0.268297 Lumi= 78.8 pb-1 ±3.5% vs fit predictions for ZEUS-JETS fit including these data New CC e- data with +ve polarisation P= 0.328555 Lumi=42.7pb-1 ±3.5% vs fit predictions for ZEUS-JETS fit including these data

Request preliminary New NC e- data with –ve polarisation P= -0.268297 Lumi= 78.8 pb-1 ±3.5% New NC e- data with +ve polarisation P= +0.328555 Lumi=42.7pb-1 ±3.5% vs fit predictions from ZEUS-JETS fit including these data

Data set χ2/n.d.p n.d.p. CC P- 0.79 37 CC P+ 0.85 33 NC P- 0.94 90 NC P+ 1.06 Request preliminary PDFs from the new fit compared to published ZEUS-JETS fit – central values of the PDFs hardly change at all…..

Team 2 analysis check

Request preliminary BUT the PDF uncertainties are reduced at high-x, particularly for xuv …..as expected since NC and CC e- cross-sections are both u dominated

Request preliminary Improvement in uncertainty remains up to high scales- important for LHC physics!

Team-2 analysis

Electroweak parameter fits Now let MW be a free parameter of the fit, together with the PDF parameters How does MW enter the fit? In the factor GF2 MW4/(Q2+MW2)2 Value of MW (=80.4 SM) Specifications of the fit Request preliminary 79.1 ± 0.77 ± 0.99 79.1 ± 0.80 ± 0.97 79.1 ± 0.82 ± 0.98 77.6 ± 1.4 ± 2.5 78.9 ± 2.0(stat) ± 1.8 (sys) +2.2 -1.8 (PDF) 82.87 ± 1.82(exp) +0.32-0.18 (model) ZEUS-jets RTVFN plus new NC/CC e- polarised data ZEUs-only ZMVFN plus new NC/CC e- polarised data Team-2 value Zeus-only ZMVFN ZEUS HERA-I data done by this EW+PDF fit method ZEUS DESY-03-093 published HERA-I result H1 HERA-I data done by EW+PDF method Note model dependence is small because there is little correlation between EW and QCD sector of the fit

Request preliminary values in this colour Zeus-jets RTVFN Check with ZEUS-only ZMVFN Team 2 analysis values in this colour Can also fit BOTH GF and MW remember GF SM= 1.11639×10-5 Or we can fit a more general formalism: fit g and MW in g2 / (Q2 + MW2)2 such that g2=GF2 MW4 = 0.07542 for standard model, GF=1.127 ± 0.013 ± 0.014 ×10-5 GF=1.123 ± 0.013 ± 0.014 ×10-5 GF=1.122 ± 0.014 ± 0.011 ×10-5 MW=82.8 ± 1.5 ± 1.3 MW=83.1 ± 1.5 ± 1.2 MW=83.3 ± 1.6 ± 1.0 g= 0.0772 ± 0.0021 ± 0.0019 g= 0.0776 ± 0.0021 ± 0.0016 g= 0.0778 ± 0.0022 ± 0.0016 MW=82.8 ± 1.5 ± 1.3 MW=83.1 ± 1.5 ± 1.1 MW=83.2 ± 1.6 ± 1.0 This is the most general way to present our data

Now consider fits to electroweak NC couplings as well as PDF parameters At LO the NC unpolarised structure functions are given by F20 = i Ai0(Q2) [xqi(x,Q2) + xqi(x,Q2)] xF30= i Bi0(Q2) [xqi(x,Q2) - xqi(x,Q2)] Ai0(Q2) = ei2 – 2 ei vi ve PZ + (ve2+ae2)(vi2+ai2) PZ2 Bi0(Q2) = – 2 ei ai ae PZ + 4ai ae vi ve PZ2 PZ2 = Q2/(Q2 + M2Z) 1/sin2θW And the unpolarised cross-section is given by σ0 = Y+ F20 + Y- xF30 The polarised structure functions are given by F2P = i AiP(Q2) [xqi(x,Q2) + xqi(x,Q2)] xF3P= i BiP(Q2) [xqi(x,Q2) - xqi(x,Q2)] AiP(Q2) = 2 ei vi ae PZ - 2 ve ae (vi2+ai2) PZ2 BiP(Q2) = 2 ei ai ve PZ - 2 ai vi (ve2+ae2) PZ2 and the polarised cross-section is given by σP = Y+ F2P + Y- xF3P So that the total cross-section is given by σ = σ0 + P σP Given that ve is very small and that the γ/Z interference terms in PZ dominate the PZ2 terms, we can see that infromation on au, ad comes from unpolarised xF30 and infromation on vu,vd comes from polarised F2P

au ad vu vd SM formalism ai = T3i , vi = T3i – 2ei sin2ƏW Let ai and vi be free as well as PDFparameters. Perform fits with 2, 3 or 4 EW parameters free au ad vu vd SM value 0.5 -0.5 0.196 0.346 2 EW param. 0.50±0.04±0.09 0.19±0.06±0.06 2 EW param -0.49±0.14±0.28 -0.37±0.14±0.16 0.48±0.06±0.10 -0.55±0.10±0.21 0.12±0.10±0.05 -0.47±0.15±0.19 3 EW param 0.49±0.03±0.07 ad=-au 0.12±0.10±0.06 -0.48±0.15±0.18 4 EW param 0.59±0.18±0.44 -0.10±0.70±1.73 0.10±0.12±0.22 -0.55±0.20±0.51 Request preliminary on 2 and 3 EW parameter values The 4- parameter fit has fallen foul of a double minimum- (which was avoided by pure luck with the earlier collab. meeting version of the data)- see later

New 4-parameter fit contours compared to: H1 4-parameter contours, ZEUS-4 parameter from HERA-I and to what we thought we had got from new data at the time of the collaboration meeting au/vu contour is not so different and is much better than without polarised data The ad/vd contour is a somwehat different shape and more extended in ad, BUT still a substantial improvement in vd when compared to HERA-I data

ZEUS-only ZMVFN version of previous Table au ad vu vd SM value 0.5 -0.5 0.196 0.346 2 EW param. 0.51±0.04±0.09 0.18±0.06±0.05 2 EW param -0.55±0.13±0.22 -0.32±0.14±0.13 0.51±0.07±0.11 -0.51±0.17±0.24 0.13±0.10±0.04 -0.45±0.15±0.19 3 EW param 0.51±0.03±0.09 ad=-au 0.13±0.11±0.05 -0.44±0.17±0.18 4 EW param 0.64±0.15±0.19 0.04±0.61±1.01 0.13±0.17±0.22 -0.47±0.39±0.65

au ad vu vd Team-2 analysis values SM value 0.5 -0.5 0.196 0.346 2 param. 0.52±0.04±0.09 0.18±0.06±0.06 -0.56±0.13±0.23 -0.33±0.14±0.14 0.51±0.07±0.12 -0.52±0.17±0.24 0.13±0.10±0.05 -0.46±0.15±0.19 3 param 0.51±0.03±0.08 ad=-au 0.14±0.11±0.07 -0.43±0.18±0.21 4 param 0.66±0.12±0.12 0.09±0.53±0.73 0.14±0.17±0.20 -0.44±0.40±0.61 Excellent agreeent of 2 and 3 parameter values, good agreement of 4-parameter values..but note the fit is unstable for 4-parameters because of the double minimum, so small differences get magnified

Request preliminary for these 2-EW parameter contours Team- 2 contours for 2-EW parameter fits

Comparison of 2EW parameter contours with those of H1, and with LEP and CDF results

For further comment on au/ad see Team 2 analysis- next slide Alternative 2-EW parameter contours, reflecting how our data access au/ad in XF30(unpolarised) and vu/vd in F2P(polarised) Request preliminary for vu/vd, this exploits the information in new polarised data For further comment on au/ad see Team 2 analysis- next slide

Team 2 au/ad and vu/vd 2-parameter contours: Note the double minimum in au/ad space – the central values of 0.51,-0.52 are NOT at the centre of this contour..but in the bottom bulge. There is clearly an alternative minimum at au~0.65, ad~0.1..that is what is found by the 4-parameter fit

Contours from the 3-EW parameter fit just for information Contours from the 3-EW parameter fit just for information. Note this graph is constructed by flipping au in sign to give ad=-au.

Team-2 contours from 3 parameter fit Team-2 contours from 3 parameter fit..note this graph should have au flipped in sign to give ad=-au, to make sense of it

And BSM formalism ai = T3iL-T3iR , vi = T3iL+T3iR – 2ei sin2ƏW Alternative ways to present the NC couplings using SM formalism ai = T3iL , vi = T3iL – 2ei sin2ƏW: And BSM formalism ai = T3iL-T3iR , vi = T3iL+T3iR – 2ei sin2ƏW (note sin2ƏWalso enters the PZ propagator and ve) Request preliminary: values in this table ZEUS-ONLY ZMVFN Team-2 values in this colour T3uL T3dL T3uR T3dR sin2ƏW 0.47±0.05±0.13 0.50±0.06±0.12 0.50±0.06±0.13 SM formalism -0.55±0.18±0.35 -0.53±0.19±0.32 -0.50±0.22±0.42 0.231±0.024±0.070 0.234±0.024±0.061 0.229±0.017±0.071 0.5 BSM :2 EW param fit -0.5 -0.05±0.05±0.12 -0.06±0.05±0.11 -0.14±0.15±0.28 -0.16±0.14±0.25 0.2315 BSM:3 EW param fit -0.07±0.07±0.07 -0.08±0.07±0.05 -0.26±0.19±0.19 -0.22±0.21±0.13 0.238±0.011±0.023 0.236±0.012±0.020

Team-2 version of T3u/T3d contour Request preliminary T3u/T3d contour from the 3-EW parameter SM formalism fit This is essentially an au/ad contour with added constraints from the SM formalism Team-2 version of T3u/T3d contour

Other contours from the T3u/ T3d/ sin2ƏW 3 EW param Other contours from the T3u/ T3d/ sin2ƏW 3 EW param. SM job for information

Request preliminary the T3uR /T3dR contour from the 2 EW parameter BSM fit also shown compared to the H1 contour

Contours from the T3uR / T3dR/ sin2ƏW 3-EW parameter beyond SM formalism fit for information

Conclusions Very nice electroweak results Agreement with 2nd analysis Lets go for preliminary at DIS06

4-param fit contours (statistical) only for information

H1 4-parameter contours, ZEUS-4 parameter from HERA-I Comparison to: H1 4-parameter contours, ZEUS-4 parameter from HERA-I and to what we thought we had got from new data at the time of the collaboration meeting au/vu contour is not so different and is much better than without polarised data The ad/vd contour is a somwehat different shape and more extended in ad, BUT still a substantial improvement in vd when compared to HERA-I data

Team-2 4parameter contours