D120121 Parton Distribution Functions, Part 2. D120122 CT10-NNLO Parton Distribution Functions.

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Presentation transcript:

D Parton Distribution Functions, Part 2

D CT10-NNLO Parton Distribution Functions

D CT10-NNLO compared to MSTW2008 (NNLO)

D CT10-NNLO compared to MSTW2008 (NNLO)

D CT10-NNLO error pdfs

D D. Uncertainties of Parton Distribution Functions 1. “Errors” and Uncertainties 2. Propagation of Experimental “Errors” 3. PDF Uncertainties 4. The role of  S in Global Analysis 5. Implications for LHC Physics

D Mark Twain … from "Chapters from My Autobiography", published in 1906 … "Figures often beguile me, particularly when I have the arranging of them myself; in which case the remark attributed to Disraeli would often apply with justice and force: There are three kinds of lies: lies, damned lies, and statistics.” Lecture 2: Errors and Uncertainties in the Global Analysis of QCD

D “Errors” and Uncertainties How accurately can we determine the PDFs? The accuracy is limited by … Experimental “errors” Theory “errors” Parametrization errors  ep = PDF  C Data ; We’re trying to determine this ; Calculation statistical; systematic LO, NLO, NNLO; choice of momentum value of  S PDF uncertainty

D Parametrization In the CTEQ Global Analysis, we parametrize the PDFs f i (x,Q) at a low Q scale, Q 0 = 1.3 GeV. For example, ( q = u or d ; q v = q – q ) Potentially, 6 x ( )=36 parameters. Then f i (x,Q) is DETERMINED for Q > Q 0 by the renormalization group evolution equations (DGLAP). Find the parameter values {a i0 … a i5 } such that theory and data agree most closely. _ { The a i ’s are different for different flavors} ( CT10-NNLO has 25 parameters.) PDF uncertainty

25 random choices of the 5 parameters D Parametrization PDF uncertainty We hope that the parametrization if sufficiently general that the best choice of parameters will fit the “true” function...

D Propagation of Experimental “Errors” Consider the data from a single experiment. The experimental collaboration will publish a set of measurements, {M i ; i = 1, 2, 3,…, N dp }. Each measurement M i has several parts, M i = { D i ;  0i ; {  i, = 1, 2, 3, …, N sy }} D i = central data value; average of many events.  0i = correlated errors; 1 standard deviation of the statistical error for D i.  i } = correlated errors;  i = 1 standard deviation of the systematic error type ; N sy = the number of sources of systematic error. So, where X i = the “true value”. (r 0i and r are normalized random variables)

D Propagation of Experimental “Errors”  2 analysis The simplest case is N sy = 0 (no systematic errors). So let’s start by assuming N sy = 0. (Later we’ll include systematic errors.) Define where T i (a) = the theoretical value for measurement M i, which depends on a set of theoretical parameters {a 1, a 2, a 3, …, a D }. Minimize  2 (a); ∂  2 / ∂a k = 0 for k = 1, 2, 3,…, D. which yields the central fit The variations of  2 around the minimum tells us the uncertainty

D Propagation of Experimental “Errors” Ludwig Otto Hesse Hessian Analysis In a small neighborhood of {a (0) }, Now, make a prediction based on the theory, for some other quantity Q: the Hessian matrix, H jk the allowed variation,  a j

D Propagation of Experimental “Errors” Parameter variations in the eigenvector basis Then we have D  2 alternative fits of the theory parameters, and one central fit. Eigenvectors of the Hessian, (m = 1, 2, 3, …, D) The distance along the eigenvector v (m) is allowed to vary by an amount of order  (1/ (m) ) 1/2. (“tolerance”)

D Propagation of Experimental “Errors” Systematic errors We have  i = standard deviation of systematic error, of D i  0i = standard deviation of the uncorrelated error, of D i (r and r 0i are unknown random variables, of order 1) We want {T i (a)} to fit {X i } as closely as possible, from the knowledge we have. Minimize this  2 with respect to both {a k } and {r }. I.e., we fit the theory T i (a) to “optimally shifted data”,

D Propagation of Experimental “Errors” Results of the Global Analysis of QCD { f i (0) (x,Q 2 ) } = the central fit (i = 0,  1,  2,  3,  4,  5) { f i (k) (x,Q 2 ) } = the error PDFs; alternative fits (k = 1, 2, 3,...,50) k = 1,2 Eigenvector 1  directions k = 3,4 Eigenvector 2  directions … k = 2n-1,2n Eigenvector n  directions … … accessible at the CT10-NNLO web site, or the Durham Parton Distribution Generator

D Propagation of Experimental “Errors” PDF Uncertainty symmetric errors Consider the prediction of a quantity Q. Ideally, This is the “Master Formula” for symmetric errors. But the behavior in the neighborhood of the minimum is not perfectly quadratic. So, instead, asymmetric errors

D Democracy among Experiments … from the previous page, including the correlated shifts {r } expt. P is a penalty that prevents its experiment from deviating too much (90% C.L.) from the theory. Minimize  2 global. Diagonalize the full Hessian Matrix. Final Result: f i (0) (x,Q 2 ) and 50 variations {f i (k) (x,Q 2 )} …the eigenvector-basis PDF variations. Propagation of Experimental “Errors”

D CT10-NNLO Table Ndp Chi^2 Nsy 1/ 159 HERA1X Combined HERA1 NC+CC DIS (2009) 2/ 101 BcdF2pCor BCDMS collaboration 3/ 102 BcdF2dCor BCDMS collaboration 4/ 103 NmcF2pCor NMC collaboration 5/ 104 NmcRatCor NMC collaboration 6/ 108 cdhswf P Berge et al Z Phys C (1991) 7/ 109 cdhswf P Berge et al Z Phys C (1991) 8/ 110 ccfrf2.mi Yang&Bodek model-independent 9/ 111 ccfrf3.md Shaevitz&Seligman model-dependent processed by SK 10/ 201 e DY Q^3 dSig/dQ dy proton on heavy target 11/ 203 e866f E866 experiment: pd / 2pp 12/ 225 cdfLasy W production: decay lepton asymmetry CDF Run-1 13/ 140 HN+67F2c H1 neutral current charm 14/ 143 HN+90X0c H1 neutral current charm 15/ 156 ZN+67F2c ZEUS neutral current charm 16/ 157 ZN+80F2c ZEUS neutral current charm 17/ 124 NuTvNuChXN NuTev Neutrino Dimuon Reduced xSec 18/ 125 NuTvNbChXN NuTev Neutrino Dimuon Reduced xSec 19/ 126 CcfrNuChXN Ccfr Neutrino Dimuon Reduced xSec 20/ 127 CcfrNbChXN Ccfr Neutrino Dimuon Reduced xSec 21/ 204 e866ppxf E866 experiment: DY pp: Q^3 dSig/dQ dxf 22/ 260 ZyD02a Z rapidity dist. (D0 TeV II-a) 23/ 261 ZyCDF Z rapidity dist. (CDF TeV II) 24/ 227 cdfLasy W production: decay lepton asymmetry CDF Run-2 25/ 231 d02Easy W production: decay elec asymmetry D0 Run-2 Pt>25 26/ 234 d02Masy W production: decay muon asymmetry D0 Run-2 Pt>20 27/ 504 cdf2jtCor (run II: cor.err; ptmin & ptmax) 28/ 514 d02jtCor (run II: cor.err; ptmin & ptmax) Experimental Data Used in the CT10 Analysis Egalitarianism among Experiments

D next ……

D Uncertainties of Parton Distribution Functions

D CT10-NNLO Error PDFs

D CT10-NNLO Error PDFs -- ratio plots for valence quarks and gluon

D CT10-NNLO Error PDFs -- ratio plots : antiquarks / gluon

E E. Applications to LHC Physics

E LHC predictions The search for New Physics will require high precision comparisons between standard model predictions and experimental measurements. We seek discrepancies between standard model theory and data. The CT10-NNLO PDFs – central fit and eigenvector basis variations – will be used in the theory predictions. Please understand the importance of the Master Formula!

E … from the CT10 paper(NLO)

E … from the CT10 paper(NLO)

E Total cross sections for production of electroweak bosons (Dr. Zhao Li) Boson Colliderunit CT10 (NLO)CT10-NNLOMSTW2008 W+ LHC14nb 12.2    0.2 W+ LHC7nb 6.0    0.1 W+ Tevatronnb 1.35    0.02 W-LHC14nb 8.9    0.2 W-LHC7nb 4.10    0.07 ZLHC14nb 2.07    0.03 ZLHC7nb 0.96    0.02 ZTevatronpb 260  9263  8261  5 H(sm)LHC14pb 101  999  8102  7 H(sm)LHC7pb 31.2    1.3 H(sm)Tevatronpb 1.77   0.11

E Luminosity Functions Consider production of a high-mass state at the LHC.

E The luminosity function is a measure of the rate of production --- the contribution of PDFs to that rate --- for states with the corresponding quantum numbers. The uncertainty of the L.F. is a good estimate of the PDF uncertainty for that process. M = 50, 100, 200, 400, 800 GeV