Showing 10 of 6240 results
High-statistics differential cross sections and spin density matrix elements for the reaction $\gamma p \to p \omega$ have been measured using the CLAS at Jefferson Lab for center-of-mass (CM) energies from threshold up to 2.84 GeV. Results are reported in 112 10-MeV wide CM energy bins, each subdivided into $\cos{\theta_{CM}^{\omega}}$ bins of width 0.1. These are the most precise and extensive $\omega$ photoproduction measurements to date. A number of prominent structures are clearly present in the data. Many of these have not previously been observed due to limited statistics in earlier measurements.
Differential cross section for the W range 1.72 to 1.73 GeV.
Differential cross section for the W range 1.73 to 1.74 GeV.
Differential cross section for the W range 1.74 to 1.75 GeV.
Differential cross section for the W range 1.75 to 1.76 GeV.
Differential cross section for the W range 1.76 to 1.77 GeV.
Differential cross section for the W range 1.77 to 1.78 GeV.
Differential cross section for the W range 1.78 to 1.79 GeV.
Differential cross section for the W range 1.79 to 1.80 GeV.
Differential cross section for the W range 1.80 to 1.81 GeV.
Differential cross section for the W range 1.81 to 1.82 GeV.
Differential cross section for the W range 1.82 to 1.83 GeV.
Differential cross section for the W range 1.83 to 1.84 GeV.
Differential cross section for the W range 1.84 to 1.85 GeV.
Differential cross section for the W range 1.85 to 1.86 GeV.
Differential cross section for the W range 1.86 to 1.87 GeV.
Differential cross section for the W range 1.87 to 1.88 GeV.
Differential cross section for the W range 1.88 to 1.89 GeV.
Differential cross section for the W range 1.89 to 1.90 GeV.
Differential cross section for the W range 1.90 to 1.91 GeV.
Differential cross section for the W range 1.91 to 1.92 GeV.
Differential cross section for the W range 1.92 to 1.93 GeV.
Differential cross section for the W range 1.93 to 1.94 GeV.
Differential cross section for the W range 1.94 to 1.95 GeV.
Differential cross section for the W range 1.96 to 1.97 GeV.
Differential cross section for the W range 1.97 to 1.98 GeV.
Differential cross section for the W range 1.98 to 1.99 GeV.
Differential cross section for the W range 1.99 to 2.00 GeV.
Differential cross section for the W range 2.00 to 2.01 GeV.
Differential cross section for the W range 2.01 to 2.02 GeV.
Differential cross section for the W range 2.02 to 2.03 GeV.
Differential cross section for the W range 2.03 to 2.04 GeV.
Differential cross section for the W range 2.04 to 2.05 GeV.
Differential cross section for the W range 2.05 to 2.06 GeV.
Differential cross section for the W range 2.06 to 2.07 GeV.
Differential cross section for the W range 2.07 to 2.08 GeV.
Differential cross section for the W range 2.08 to 2.09 GeV.
Differential cross section for the W range 2.09 to 2.10 GeV.
Differential cross section for the W range 2.10 to 2.11 GeV.
Differential cross section for the W range 2.11 to 2.12 GeV.
Differential cross section for the W range 2.12 to 2.13 GeV.
Differential cross section for the W range 2.13 to 2.14 GeV.
Differential cross section for the W range 2.14 to 2.15 GeV.
Differential cross section for the W range 2.15 to 2.16 GeV.
Differential cross section for the W range 2.16 to 2.17 GeV.
Differential cross section for the W range 2.17 to 2.18 GeV.
Differential cross section for the W range 2.18 to 2.19 GeV.
Differential cross section for the W range 2.19 to 2.20 GeV.
Differential cross section for the W range 2.20 to 2.21 GeV.
Differential cross section for the W range 2.21 to 2.22 GeV.
Differential cross section for the W range 2.22 to 2.23 GeV.
Differential cross section for the W range 2.23 to 2.24 GeV.
Differential cross section for the W range 2.24 to 2.25 GeV.
Differential cross section for the W range 2.25 to 2.26 GeV.
Differential cross section for the W range 2.26 to 2.27 GeV.
Differential cross section for the W range 2.27 to 2.28 GeV.
Differential cross section for the W range 2.28 to 2.29 GeV.
Differential cross section for the W range 2.29 to 2.30 GeV.
Differential cross section for the W range 2.30 to 2.31 GeV.
Differential cross section for the W range 2.31 to 2.32 GeV.
Differential cross section for the W range 2.32 to 2.33 GeV.
Differential cross section for the W range 2.33 to 2.34 GeV.
Differential cross section for the W range 2.34 to 2.35 GeV.
Differential cross section for the W range 2.35 to 2.36 GeV.
Differential cross section for the W range 2.36 to 2.37 GeV.
Differential cross section for the W range 2.37 to 2.38 GeV.
Differential cross section for the W range 2.38 to 2.39 GeV.
Differential cross section for the W range 2.39 to 2.40 GeV.
Differential cross section for the W range 2.40 to 2.41 GeV.
Differential cross section for the W range 2.41 to 2.42 GeV.
Differential cross section for the W range 2.42 to 2.43 GeV.
Differential cross section for the W range 2.43 to 2.44 GeV.
Differential cross section for the W range 2.44 to 2.45 GeV.
Differential cross section for the W range 2.45 to 2.46 GeV.
Differential cross section for the W range 2.46 to 2.47 GeV.
Differential cross section for the W range 2.47 to 2.48 GeV.
Differential cross section for the W range 2.48 to 2.49 GeV.
Differential cross section for the W range 2.49 to 2.50 GeV.
Differential cross section for the W range 2.50 to 2.51 GeV.
Differential cross section for the W range 2.51 to 2.52 GeV.
Differential cross section for the W range 2.52 to 2.53 GeV.
Differential cross section for the W range 2.53 to 2.54 GeV.
Differential cross section for the W range 2.54 to 2.55 GeV.
Differential cross section for the W range 2.55 to 2.56 GeV.
Differential cross section for the W range 2.56 to 2.57 GeV.
Differential cross section for the W range 2.57 to 2.58 GeV.
Differential cross section for the W range 2.58 to 2.59 GeV.
Differential cross section for the W range 2.59 to 2.60 GeV.
Differential cross section for the W range 2.60 to 2.61 GeV.
Differential cross section for the W range 2.61 to 2.62 GeV.
Differential cross section for the W range 2.62 to 2.63 GeV.
Differential cross section for the W range 2.63 to 2.64 GeV.
Differential cross section for the W range 2.64 to 2.65 GeV.
Differential cross section for the W range 2.65 to 2.66 GeV.
Differential cross section for the W range 2.66 to 2.67 GeV.
Differential cross section for the W range 2.67 to 2.68 GeV.
Differential cross section for the W range 2.68 to 2.69 GeV.
Differential cross section for the W range 2.69 to 2.70 GeV.
Differential cross section for the W range 2.70 to 2.71 GeV.
Differential cross section for the W range 2.71 to 2.72 GeV.
Differential cross section for the W range 2.72 to 2.73 GeV.
Differential cross section for the W range 2.75 to 2.76 GeV.
Differential cross section for the W range 2.76 to 2.77 GeV.
Differential cross section for the W range 2.77 to 2.78 GeV.
Differential cross section for the W range 2.78 to 2.79 GeV.
Differential cross section for the W range 2.79 to 2.80 GeV.
Differential cross section for the W range 2.80 to 2.81 GeV.
Differential cross section for the W range 2.81 to 2.82 GeV.
Differential cross section for the W range 2.82 to 2.83 GeV.
Differential cross section for the W range 2.83 to 2.84 GeV.
Spin density matrix elements for the W range 1.72 to 1.73 GeV.
Spin density matrix elements for the W range 1.73 to 1.74 GeV.
Spin density matrix elements for the W range 1.74 to 1.75 GeV.
Spin density matrix elements for the W range 1.75 to 1.76 GeV.
Spin density matrix elements for the W range 1.76 to 1.77 GeV.
Spin density matrix elements for the W range 1.77 to 1.78 GeV.
Spin density matrix elements for the W range 1.78 to 1.79 GeV.
Spin density matrix elements for the W range 1.79 to 1.80 GeV.
Spin density matrix elements for the W range 1.80 to 1.81 GeV.
Spin density matrix elements for the W range 1.81 to 1.82 GeV.
Spin density matrix elements for the W range 1.82 to 1.83 GeV.
Spin density matrix elements for the W range 1.83 to 1.84 GeV.
Spin density matrix elements for the W range 1.84 to 1.85 GeV.
Spin density matrix elements for the W range 1.85 to 1.86 GeV.
Spin density matrix elements for the W range 1.86 to 1.87 GeV.
Spin density matrix elements for the W range 1.87 to 1.88 GeV.
Spin density matrix elements for the W range 1.88 to 1.89 GeV.
Spin density matrix elements for the W range 1.89 to 1.90 GeV.
Spin density matrix elements for the W range 1.90 to 1.91 GeV.
Spin density matrix elements for the W range 1.91 to 1.92 GeV.
Spin density matrix elements for the W range 1.92 to 1.93 GeV.
Spin density matrix elements for the W range 1.93 to 1.94 GeV.
Spin density matrix elements for the W range 1.94 to 1.95 GeV.
Spin density matrix elements for the W range 1.95 to 1.96 GeV.
Spin density matrix elements for the W range 1.96 to 1.97 GeV.
Spin density matrix elements for the W range 1.97 to 1.98 GeV.
Spin density matrix elements for the W range 1.98 to 1.99 GeV.
Spin density matrix elements for the W range 1.99 to 2.00 GeV.
Spin density matrix elements for the W range 2.00 to 2.01 GeV.
Spin density matrix elements for the W range 2.01 to 2.02 GeV.
Spin density matrix elements for the W range 2.02 to 2.03 GeV.
Spin density matrix elements for the W range 2.03 to 2.04 GeV.
Spin density matrix elements for the W range 2.04 to 2.05 GeV.
Spin density matrix elements for the W range 2.05 to 2.06 GeV.
Spin density matrix elements for the W range 2.06 to 2.07 GeV.
Spin density matrix elements for the W range 2.07 to 2.08 GeV.
Spin density matrix elements for the W range 2.08 to 2.09 GeV.
Spin density matrix elements for the W range 2.09 to 2.10 GeV.
Spin density matrix elements for the W range 2.10 to 2.11 GeV.
Spin density matrix elements for the W range 2.11 to 2.12 GeV.
Spin density matrix elements for the W range 2.12 to 2.13 GeV.
Spin density matrix elements for the W range 2.13 to 2.14 GeV.
Spin density matrix elements for the W range 2.14 to 2.15 GeV.
Spin density matrix elements for the W range 2.15 to 2.16 GeV.
Spin density matrix elements for the W range 2.16 to 2.17 GeV.
Spin density matrix elements for the W range 2.17 to 2.18 GeV.
Spin density matrix elements for the W range 2.18 to 2.19 GeV.
Spin density matrix elements for the W range 2.19 to 2.20 GeV.
Spin density matrix elements for the W range 2.20 to 2.21 GeV.
Spin density matrix elements for the W range 2.21 to 2.22 GeV.
Spin density matrix elements for the W range 2.22 to 2.23 GeV.
Spin density matrix elements for the W range 2.23 to 2.24 GeV.
Spin density matrix elements for the W range 2.24 to 2.25 GeV.
Spin density matrix elements for the W range 2.25 to 2.26 GeV.
Spin density matrix elements for the W range 2.26 to 2.27 GeV.
Spin density matrix elements for the W range 2.27 to 2.28 GeV.
Spin density matrix elements for the W range 2.28 to 2.29 GeV.
Spin density matrix elements for the W range 2.29 to 2.30 GeV.
Spin density matrix elements for the W range 2.30 to 2.31 GeV.
Spin density matrix elements for the W range 2.31 to 2.32 GeV.
Spin density matrix elements for the W range 2.32 to 2.33 GeV.
Spin density matrix elements for the W range 2.33 to 2.34 GeV.
Spin density matrix elements for the W range 2.34 to 2.35 GeV.
Spin density matrix elements for the W range 2.35 to 2.36 GeV.
Spin density matrix elements for the W range 2.36 to 2.37 GeV.
Spin density matrix elements for the W range 2.37 to 2.38 GeV.
Spin density matrix elements for the W range 2.38 to 2.39 GeV.
Spin density matrix elements for the W range 2.39 to 2.40 GeV.
Spin density matrix elements for the W range 2.40 to 2.41 GeV.
Spin density matrix elements for the W range 2.41 to 2.42 GeV.
Spin density matrix elements for the W range 2.42 to 2.43 GeV.
Spin density matrix elements for the W range 2.43 to 2.44 GeV.
Spin density matrix elements for the W range 2.44 to 2.45 GeV.
Spin density matrix elements for the W range 2.45 to 2.46 GeV.
Spin density matrix elements for the W range 2.46 to 2.47 GeV.
Spin density matrix elements for the W range 2.47 to 2.48 GeV.
Spin density matrix elements for the W range 2.48 to 2.49 GeV.
Spin density matrix elements for the W range 2.49 to 2.50 GeV.
Spin density matrix elements for the W range 2.50 to 2.51 GeV.
Spin density matrix elements for the W range 2.51 to 2.52 GeV.
Spin density matrix elements for the W range 2.52 to 2.53 GeV.
Spin density matrix elements for the W range 2.53 to 2.54 GeV.
Spin density matrix elements for the W range 2.54 to 2.55 GeV.
Spin density matrix elements for the W range 2.55 to 2.56 GeV.
Spin density matrix elements for the W range 2.56 to 2.57 GeV.
Spin density matrix elements for the W range 2.57 to 2.58 GeV.
Spin density matrix elements for the W range 2.58 to 2.59 GeV.
Spin density matrix elements for the W range 2.59 to 2.60 GeV.
Spin density matrix elements for the W range 2.60 to 2.61 GeV.
Spin density matrix elements for the W range 2.61 to 2.62 GeV.
Spin density matrix elements for the W range 2.62 to 2.63 GeV.
Spin density matrix elements for the W range 2.63 to 2.64 GeV.
Spin density matrix elements for the W range 2.64 to 2.65 GeV.
Spin density matrix elements for the W range 2.65 to 2.66 GeV.
Spin density matrix elements for the W range 2.66 to 2.67 GeV.
Spin density matrix elements for the W range 2.67 to 2.68 GeV.
Spin density matrix elements for the W range 2.68 to 2.69 GeV.
Spin density matrix elements for the W range 2.69 to 2.70 GeV.
Spin density matrix elements for the W range 2.70 to 2.71 GeV.
Spin density matrix elements for the W range 2.71 to 2.72 GeV.
Spin density matrix elements for the W range 2.72 to 2.73 GeV.
Spin density matrix elements for the W range 2.73 to 2.74 GeV.
Spin density matrix elements for the W range 2.74 to 2.75 GeV.
Spin density matrix elements for the W range 2.75 to 2.76 GeV.
Spin density matrix elements for the W range 2.76 to 2.77 GeV.
Spin density matrix elements for the W range 2.77 to 2.78 GeV.
Spin density matrix elements for the W range 2.78 to 2.79 GeV.
Spin density matrix elements for the W range 2.79 to 2.80 GeV.
Spin density matrix elements for the W range 2.80 to 2.81 GeV.
Spin density matrix elements for the W range 2.81 to 2.82 GeV.
Spin density matrix elements for the W range 2.82 to 2.83 GeV.
Spin density matrix elements for the W range 2.83 to 2.84 GeV.
We present the first measurements at a hadron collider of differential cross sections for Z+jet+X production in delta phi(Z, jet), |delta y(Z, jet)| and |y_boost(Z, jet)|. Vector boson production in association with jets is an excellent probe of QCD and constitutes the main background to many small cross section processes, such as associated Higgs production. These measurements are crucial tests of the predictions of perturbative QCD and current event generators, which have varied success in describing the data. Using these measurements as inputs in tuning event generators will increase the experimental sensitivity to rare signals.
Differential cross section in bins of PHI(P=3)-PHI(P=4) for Z/GAMMA* transverse momentum > 25 GeV.
Differential cross section in bins of PHI(P=3)-PHI(P=4) for Z/GAMMA* transverse momentum > 45 GeV.
Differential cross section in bins of ABS(YRAP(P=3)-YRAP(P=4)) for Z/GAMMA* transverse momentum > 25 GeV.
Differential cross section in bins of ABS(YRAP(P=3)-YRAP(P=4)) for Z/GAMMA* transverse momentum > 45 GeV.
Differential cross section in bins of ABS(YRAP(P=3)+YRAP(P=4))/2 for Z/GAMMA* transverse momentum > 25 GeV.
Differential cross section in bins of ABS(YRAP(P=3)+YRAP(P=4))/2 for Z/GAMMA* transverse momentum > 45 GeV.
Individual percentage contributions to the systematic error for the binning in PHI(P=3)-PHI(P=4) for Z/GAMMA* transverse momentum > 25 GeV.
Individual percentage contributions to the systematic error for the binning in PHI(P=3)-PHI(P=4) for Z/GAMMA* transverse momentum > 45 GeV.
Individual percentage contributions to the systematic error for the binning in ABS(YRAP(P=3)-YRAP(P=4)) for Z/GAMMA* transverse momentum > 25 GeV.
Individual percentage contributions to the systematic error for the binning in ABS(YRAP(P=3)-YRAP(P=4)) for Z/GAMMA* transverse momentum > 45 GeV.
Individual percentage contributions to the systematic error for the binning in ABS(YRAP(P=3)+YRAP(P=4))/2 for Z/GAMMA* transverse momentum > 25 GeV.
Individual percentage contributions to the systematic error for the binning in ABS(YRAP(P=3)+YRAP(P=4))/2 for Z/GAMMA* transverse momentum > 45 GeV.
Measurements of the double-differential charged pion production cross-section in the range of momentum 0.5 GeV/c < p < 8.0 GeV/c and angle 0.025 rad < theta <0.25 rad in collisions of protons on beryllium, carbon, nitrogen, oxygen, aluminium, copper, tin, tantalum and lead are presented. The data were taken with the large acceptance HARP detector in the T9 beam line of the CERN PS. Incident particles were identified by an elaborate system of beam detectors. The data were taken with thin targets of 5% of a nuclear interaction length. The tracking and identification of the produced particles was performed using the forward system of the HARP experiment. Results are obtained for the double-differential cross section mainly at four incident proton beam momenta (3 GeV/c, 5 GeV/c, 8 GeV/c and 12 GeV/c). Measurements are compared with the GEANT4 and MARS Monte Carlo generators. A global parametrization is provided as an approximation of all the collected datasets which can serve as a tool for quick yields estimates.
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A measurement of elastic deeply virtual Compton scattering gamma* p -> gamma p using e^+ p and e^- p collision data recorded with the H1 detector at HERA is presented. The analysed data sample corresponds to an integrated luminosity of 306 pb^-1, almost equally shared between both beam charges. The cross section is measured as a function of the virtuality Q^2 of the exchanged photon and the centre-of-mass energy W of the gamma* p system in the kinematic domain 6.5 < Q^2 < 80 GeV^2, 30 < W < 140 GeV and |t| < 1 GeV^2, where t denotes the squared momentum transfer at the proton vertex. The cross section is determined differentially in t for different Q^2 and W values and exponential t-slope parameters are derived. Using e^+ p and e^- p data samples, a beam charge asymmetry is extracted for the first time in the low Bjorken x kinematic domain. The observed asymmetry is attributed to the interference between Bethe-Heitler and deeply virtual Compton scattering processes. Experimental results are discussed in the context of two different models, one based on generalised parton distributions and one based on the dipole approach.
The DVCS cross section as a function of Q**2.
The DVCS cross section as a function of W.
The DVCS cross section as a function of W for three different Q**2 regions.
The DVCS cross section DSIG/DT in three different regions of Q**2.
The DVCS cross section DSIG/DT in three regions of W.
Overall value of the SLOPE parameter of the fit to the DSIG/DT distribution.
Overall value of the fit to the W distribution of the form W**POWER.
Value of the power of the fit to the W distribution of the form W**POWER in three Q**2 regions.
Value of the fitted slope parameter in three Q**2 regions.
Value of the fitted slope parameter in three W regions.
The measured beam charge asymmetry defined as the difference in the DSIG/DPHI distributions between E+ P and E- P collisions.
Measurements of the double-differential pi+/- production cross-section in the range of momentum 100 MeV/c <= p <= 800 MeV/c and angle 0.35 rad <= theta <= 2.15 rad using pi+/- beams incident on beryllium, aluminium, carbon, copper, tin, tantalum and lead targets are presented. The data were taken with the large acceptance HARP detector in the T9 beam line of the CERN PS. The secondary pions were produced by beams in a momentum range from 3 GeV/c to 12.9 GeV/c hitting a solid target with a thickness of 5% of a nuclear interaction length. The tracking and identification of the produced particles was performed using a small-radius cylindrical time projection chamber (TPC) placed inside a solenoidal magnet. Incident particles were identified by an elaborate system of beam detectors. Results are obtained for the double-differential cross-sections d2sigma/dpdtheta at six incident beam momenta. Data at 3 GeV/c, 5 GeV/c, 8 GeV/c, and 12 GeV/c are available for all targets while additional data at 8.9 GeV/c and 12.9 GeV/c were taken in positive particle beams on Be and Al targets, respectively. The measurements are compared with several generators of GEANT4 and the MARS Monte Carlo simulation.
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The exclusive reaction $\gamma p \to p \pi^+ \pi^-$ was studied in the photon energy range 3.0 - 3.8 GeV and momentum transfer range $0.4<-t<1.0$ GeV$^2$. Data were collected with the CLAS detector at the Thomas Jefferson National Accelerator Facility. In this kinematic range the integrated luminosity was about 20 pb$^{-1}$. The reaction was isolated by detecting the $\pi^+$ and proton in CLAS, and reconstructing the $\pi^-$ via the missing-mass technique. Moments of the di-pion decay angular distributions were derived from the experimental data. Differential cross sections for the $S$, $P$, and $D$-waves in the $M_{\pi^+\pi^-}$ mass range $0.4-1.4$ GeV were derived performing a partial wave expansion of the extracted moments. Besides the dominant contribution of the $\rho(770)$ meson in the $P$-wave, evidence for the $f_0(980)$ and the $f_2(1270)$ mesons was found in the $S$ and $D$-waves, respectively. The differential production cross sections $d\sigma/dt$ for individual waves in the mass range of the above-mentioned mesons were extracted. This is the first time the $f_0(980)$ has been measured in a photoproduction experiment.
Moments YLM(LM=00) of the di-pion angular distribution for -T.
Moments YLM(LM=00) of the di-pion angular distribution for -T.
Moments YLM(LM=00) of the di-pion angular distribution for -T.
Moments YLM(LM=00) of the di-pion angular distribution for -T.
Moments YLM(LM=00) of the di-pion angular distribution for -T.
Moments YLM(LM=00) of the di-pion angular distribution for -T.
Moments YLM(LM=10) of the di-pion angular distribution for -T.
Moments YLM(LM=10) of the di-pion angular distribution for -T.
Moments YLM(LM=10) of the di-pion angular distribution for -T.
Moments YLM(LM=10) of the di-pion angular distribution for -T.
Moments YLM(LM=10) of the di-pion angular distribution for -T.
Moments YLM(LM=10) of the di-pion angular distribution for -T.
Moments YLM(LM=11) of the di-pion angular distribution for -T.
Moments YLM(LM=11) of the di-pion angular distribution for -T.
Moments YLM(LM=11) of the di-pion angular distribution for -T.
Moments YLM(LM=11) of the di-pion angular distribution for -T.
Moments YLM(LM=11) of the di-pion angular distribution for -T.
Moments YLM(LM=11) of the di-pion angular distribution for -T.
Moments YLM(LM=20) of the di-pion angular distribution for -T.
Moments YLM(LM=20) of the di-pion angular distribution for -T.
Moments YLM(LM=20) of the di-pion angular distribution for -T.
Moments YLM(LM=20) of the di-pion angular distribution for -T.
Moments YLM(LM=20) of the di-pion angular distribution for -T.
Moments YLM(LM=20) of the di-pion angular distribution for -T.
Moments YLM(LM=21) of the di-pion angular distribution for -T.
Moments YLM(LM=21) of the di-pion angular distribution for -T.
Moments YLM(LM=21) of the di-pion angular distribution for -T.
Moments YLM(LM=21) of the di-pion angular distribution for -T.
Moments YLM(LM=21) of the di-pion angular distribution for -T.
Moments YLM(LM=21) of the di-pion angular distribution for -T.
Moments YLM(LM=22) of the di-pion angular distribution for -T.
Moments YLM(LM=22) of the di-pion angular distribution for -T.
Moments YLM(LM=22) of the di-pion angular distribution for -T.
Moments YLM(LM=22) of the di-pion angular distribution for -T.
Moments YLM(LM=22) of the di-pion angular distribution for -T.
Moments YLM(LM=22) of the di-pion angular distribution for -T.
Moments YLM(LM=30) of the di-pion angular distribution for -T.
Moments YLM(LM=30) of the di-pion angular distribution for -T.
Moments YLM(LM=30) of the di-pion angular distribution for -T.
Moments YLM(LM=30) of the di-pion angular distribution for -T.
Moments YLM(LM=30) of the di-pion angular distribution for -T.
Moments YLM(LM=30) of the di-pion angular distribution for -T.
Moments YLM(LM=31) of the di-pion angular distribution for -T.
Moments YLM(LM=31) of the di-pion angular distribution for -T.
Moments YLM(LM=31) of the di-pion angular distribution for -T.
Moments YLM(LM=31) of the di-pion angular distribution for -T.
Moments YLM(LM=31) of the di-pion angular distribution for -T.
Moments YLM(LM=31) of the di-pion angular distribution for -T.
Moments YLM(LM=32) of the di-pion angular distribution for -T.
Moments YLM(LM=32) of the di-pion angular distribution for -T.
Moments YLM(LM=32) of the di-pion angular distribution for -T.
Moments YLM(LM=32) of the di-pion angular distribution for -T.
Moments YLM(LM=32) of the di-pion angular distribution for -T.
Moments YLM(LM=32) of the di-pion angular distribution for -T.
Moments YLM(LM=33) of the di-pion angular distribution for -T.
Moments YLM(LM=33) of the di-pion angular distribution for -T.
Moments YLM(LM=33) of the di-pion angular distribution for -T.
Moments YLM(LM=33) of the di-pion angular distribution for -T.
Moments YLM(LM=33) of the di-pion angular distribution for -T.
Moments YLM(LM=33) of the di-pion angular distribution for -T.
Moments YLM(LM=40) of the di-pion angular distribution for -T.
Moments YLM(LM=40) of the di-pion angular distribution for -T.
Moments YLM(LM=40) of the di-pion angular distribution for -T.
Moments YLM(LM=40) of the di-pion angular distribution for -T.
Moments YLM(LM=40) of the di-pion angular distribution for -T.
Moments YLM(LM=40) of the di-pion angular distribution for -T.
Moments YLM(LM=41) of the di-pion angular distribution for -T.
Moments YLM(LM=41) of the di-pion angular distribution for -T.
Moments YLM(LM=41) of the di-pion angular distribution for -T.
Moments YLM(LM=41) of the di-pion angular distribution for -T.
Moments YLM(LM=41) of the di-pion angular distribution for -T.
Moments YLM(LM=41) of the di-pion angular distribution for -T.
Moments YLM(LM=42) of the di-pion angular distribution for -T.
Moments YLM(LM=42) of the di-pion angular distribution for -T.
Moments YLM(LM=42) of the di-pion angular distribution for -T.
Moments YLM(LM=42) of the di-pion angular distribution for -T.
Moments YLM(LM=42) of the di-pion angular distribution for -T.
Moments YLM(LM=42) of the di-pion angular distribution for -T.
Moments YLM(LM=43) of the di-pion angular distribution for -T.
Moments YLM(LM=43) of the di-pion angular distribution for -T.
Moments YLM(LM=43) of the di-pion angular distribution for -T.
Moments YLM(LM=43) of the di-pion angular distribution for -T.
Moments YLM(LM=43) of the di-pion angular distribution for -T.
Moments YLM(LM=43) of the di-pion angular distribution for -T.
Moments YLM(LM=44) of the di-pion angular distribution for -T.
Moments YLM(LM=44) of the di-pion angular distribution for -T.
Moments YLM(LM=44) of the di-pion angular distribution for -T.
Moments YLM(LM=44) of the di-pion angular distribution for -T.
Moments YLM(LM=44) of the di-pion angular distribution for -T.
Moments YLM(LM=44) of the di-pion angular distribution for -T.
S wave cross section for -T.
S wave cross section for -T.
S wave cross section for -T.
S wave cross section for -T.
S wave cross section for -T.
S wave cross section for -T.
P wave cross section for -T.
P wave cross section for -T.
P wave cross section for -T.
P wave cross section for -T.
P wave cross section for -T.
P wave cross section for -T.
Pm wave cross section for -T.
Pm wave cross section for -T.
Pm wave cross section for -T.
Pm wave cross section for -T.
Pm wave cross section for -T.
Pm wave cross section for -T.
P0 wave cross section for -T.
P0 wave cross section for -T.
P0 wave cross section for -T.
P0 wave cross section for -T.
P0 wave cross section for -T.
P0 wave cross section for -T.
Pp wave cross section for -T.
Pp wave cross section for -T.
Pp wave cross section for -T.
Pp wave cross section for -T.
Pp wave cross section for -T.
Pp wave cross section for -T.
D wave cross section for -T.
D wave cross section for -T.
D wave cross section for -T.
D wave cross section for -T.
D wave cross section for -T.
D wave cross section for -T.
Dm wave cross section for -T.
Dm wave cross section for -T.
Dm wave cross section for -T.
Dm wave cross section for -T.
Dm wave cross section for -T.
Dm wave cross section for -T.
D0 wave cross section for -T.
D0 wave cross section for -T.
D0 wave cross section for -T.
D0 wave cross section for -T.
D0 wave cross section for -T.
D0 wave cross section for -T.
Dp wave cross section for -T.
Dp wave cross section for -T.
Dp wave cross section for -T.
Dp wave cross section for -T.
Dp wave cross section for -T.
Dp wave cross section for -T.
F wave cross section for -T.
F wave cross section for -T.
F wave cross section for -T.
F wave cross section for -T.
F wave cross section for -T.
F wave cross section for -T.
Fm wave cross section for -T.
Fm wave cross section for -T.
Fm wave cross section for -T.
Fm wave cross section for -T.
Fm wave cross section for -T.
Fm wave cross section for -T.
F0 wave cross section for -T.
F0 wave cross section for -T.
F0 wave cross section for -T.
F0 wave cross section for -T.
F0 wave cross section for -T.
F0 wave cross section for -T.
Fp wave cross section for -T.
Fp wave cross section for -T.
Fp wave cross section for -T.
Spin density matrix elements for the P-wave for -T.
Spin density matrix elements for the P-wave for -T.
Spin density matrix elements for the P-wave for -T.
Spin density matrix elements for the P-wave for -T.
Spin density matrix elements for the P-wave for -T.
Spin density matrix elements for the P-wave for -T.
Spin density matrix elements for the interference between the S- and P-waves for -T.
Spin density matrix elements for the interference between the S- and P-waves for -T.
Spin density matrix elements for the interference between the S- and P-waves for -T.
Spin density matrix elements for the interference between the S- and P-waves for -T.
Spin density matrix elements for the interference between the S- and P-waves for -T.
The results of mid-rapidity ($0 < y < 0.8$) neutral pion spectra over an extended transverse momentum range ($1 < p_T < 12$ GeV/$c$) in $\sqrt{s_{NN}}$ = 200 GeV Au+Au collisions, measured by the STAR experiment, are presented. The neutral pions are reconstructed from photons measured either by the STAR Barrel Electro-Magnetic Calorimeter (BEMC) or by the Time Projection Chamber (TPC) via tracking of conversion electron-positron pairs. Our measurements are compared to previously published $\pi^{\pm}$ and $\pi^0$ results. The nuclear modification factors $R_{\mathrm{CP}}$ and $R_{\mathrm{AA}}$ of $\pi^0$ are also presented as a function of $p_T$ . In the most central Au+Au collisions, the binary collision scaled $\pi^0$ yield at high $p_T$ is suppressed by a factor of about 5 compared to the expectation from the yield of p+p collisions. Such a large suppression is in agreement with previous observations for light quark mesons and is consistent with the scenario that partons suffer considerable energy loss in the dense medium formed in central nucleus-nucleus collisions at RHIC.
The differential cross section for the process $\gamma \gamma \to \eta \pi^0$ has been measured in the kinematic range $0.84 \GeV < W < 4.0 \GeV$, $|\cos \theta^*|<0.8$, where $W$ and $\theta^*$ are the energy and $\pi^0$ (or $\eta$) scattering angle, respectively, in the $\gamma\gamma$ center-of-mass system. The results are based on a 223 fb$^{-1}$ data sample collected with the Belle detector at the KEKB $e^+ e^-$ collider. Clear peaks due to the $a_0(980)$ and $a_2(1320)$ are visible. The differential cross sections are fitted in the energy region $0.9 \GeV < W < 1.46 \GeV$ to obtain the parameters of the $a_0(980)$. Its mass, width and $\Gamma_{\gamma \gamma} \B (\eta \pi^0)$ are measured to be $982.3 ^{+0.6}_{-0.7} ^{+3.1}_{-4.7} \MeV/c^2$, $75.6 \pm 1.6 ^{+17.4}_{-10.0} \MeV$ and $128 ^{+3}_{-2} ^{+502}_{-43} \eV$, respectively. The energy and angular dependences above 3.1 GeV are compared with those measured in the $\pi^0 \pi^0$ channel. The integrated cross section over $|\cos \theta^*|<0.8$ has a $W^{-n}$ dependence with $n = 10.5 \pm 1.2 \pm 0.5$, which is slightly larger than that for $\pi^0 \pi^0$. The differential cross sections show a $\sin^{-4} \theta^*$ dependence similar to $\gamma \gamma \to \pi^0 \pi^0$. The measured cross section ratio, $\sigma(\eta \pi^0)/\sigma(\pi^0 \pi^0) = 0.48 \pm 0.05 \pm 0.04$, is consistent with a QCD-based prediction.
The total cross section integrated over ABS(COS(THETA*)) < 0.8.
The differential cross section as a function of angle for W = 0.85 GeV.
The differential cross section as a function of angle for W = 0.87 GeV.
The differential cross section as a function of angle for W = 0.89 GeV.
The differential cross section as a function of angle for W = 0.91 GeV.
The differential cross section as a function of angle for W = 0.93 GeV.
The differential cross section as a function of angle for W = 0.95 GeV.
The differential cross section as a function of angle for W = 0.97 GeV.
The differential cross section as a function of angle for W = 0.99 GeV.
The differential cross section as a function of angle for W = 1.01 GeV.
The differential cross section as a function of angle for W = 1.03 GeV.
The differential cross section as a function of angle for W = 1.05 GeV.
The differential cross section as a function of angle for W = 1.07 GeV.
The differential cross section as a function of angle for W = 1.09 GeV.
The differential cross section as a function of angle for W = 1.11 GeV.
The differential cross section as a function of angle for W = 1.13 GeV.
The differential cross section as a function of angle for W = 1.15 GeV.
The differential cross section as a function of angle for W = 1.17 GeV.
The differential cross section as a function of angle for W = 1.19 GeV.
The differential cross section as a function of angle for W = 1.21 GeV.
The differential cross section as a function of angle for W = 1.23 GeV.
The differential cross section as a function of angle for W = 1.25 GeV.
The differential cross section as a function of angle for W = 1.27 GeV.
The differential cross section as a function of angle for W = 1.29 GeV.
The differential cross section as a function of angle for W = 1.31 GeV.
The differential cross section as a function of angle for W = 1.33 GeV.
The differential cross section as a function of angle for W = 1.35 GeV.
The differential cross section as a function of angle for W = 1.37 GeV.
The differential cross section as a function of angle for W = 1.39 GeV.
The differential cross section as a function of angle for W = 1.41 GeV.
The differential cross section as a function of angle for W = 1.43 GeV.
The differential cross section as a function of angle for W = 1.45 GeV.
The differential cross section as a function of angle for W = 1.47 GeV.
The differential cross section as a function of angle for W = 1.49 GeV.
The differential cross section as a function of angle for W = 1.51 GeV.
The differential cross section as a function of angle for W = 1.53 GeV.
The differential cross section as a function of angle for W = 1.55 GeV.
The differential cross section as a function of angle for W = 1.57 GeV.
The differential cross section as a function of angle for W = 1.59 GeV.
The differential cross section as a function of angle for W = 1.62 GeV.
The differential cross section as a function of angle for W = 1.66 GeV.
The differential cross section as a function of angle for W = 1.70 GeV.
The differential cross section as a function of angle for W = 1.74 GeV.
The differential cross section as a function of angle for W = 1.78 GeV.
The differential cross section as a function of angle for W = 1.82 GeV.
The differential cross section as a function of angle for W = 1.86 GeV.
The differential cross section as a function of angle for W = 1.90 GeV.
The differential cross section as a function of angle for W = 1.94 GeV.
The differential cross section as a function of angle for W = 1.98 GeV.
The differential cross section as a function of angle for W = 2.02 GeV.
The differential cross section as a function of angle for W = 2.06 GeV.
The differential cross section as a function of angle for W = 2.10 GeV.
The differential cross section as a function of angle for W = 2.14 GeV.
The differential cross section as a function of angle for W = 2.18 GeV.
The differential cross section as a function of angle for W = 2.22 GeV.
The differential cross section as a function of angle for W = 2.26 GeV.
The differential cross section as a function of angle for W = 2.30 GeV.
The differential cross section as a function of angle for W = 2.34 GeV.
The differential cross section as a function of angle for W = 2.38 GeV.
The differential cross section as a function of angle for W = 2.45 GeV.
The differential cross section as a function of angle for W = 2.55 GeV.
The differential cross section as a function of angle for W = 2.65 GeV.
The differential cross section as a function of angle for W = 2.75 GeV.
The differential cross section as a function of angle for W = 2.85 GeV.
The differential cross section as a function of angle for W = 2.95 GeV.
The differential cross section as a function of angle for W = 3.05 GeV.
The differential cross section as a function of angle for W = 3.15 GeV.
The differential cross section as a function of angle for W = 3.25 GeV.
The differential cross section as a function of angle for W = 3.35 GeV.
The differential cross section as a function of angle for W = 3.45 GeV.
The differential cross section as a function of angle for W = 3.55 GeV.
The differential cross section as a function of angle for W = 3.65 GeV.
The differential cross section as a function of angle for W = 3.75 GeV.
The differential cross section as a function of angle for W = 3.85 GeV.
The differential cross section as a function of angle for W = 3.95 GeV.
The process $ep \to e^{\prime}p^{\prime}\pi^0$ has been measured at $Q^2$ = 6.4 and 7.7 \ufourmomts in Jefferson Lab's Hall C. Unpolarized differential cross sections are reported in the virtual photon-proton center of mass frame considering the process $\gamma^{\ast}p \to p^{\prime}\pi^0$. Various details relating to the background subtractions, radiative corrections and systematic errors are discussed. The usefulness of the data with regard to the measurement of the electromagnetic properties of the well known $\Delta(1232)$ resonance is covered in detail. Specifically considered are the electromagnetic and scalar-magnetic ratios $R_{EM}$ and $R_{SM}$ along with the magnetic transition form factor $G_M^{\ast}$. It is found that the rapid fall off of the $\Delta(1232)$ contribution continues into this region of momentum transfer and that other resonances
Differential cross sections at Q**2=6.564 GeV**2, EPSILON=0.4523, W=1.112 GeV and COS(THETA(*))=-0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.564 GeV**2, EPSILON=0.4523, W=1.112 GeV and COS(THETA(*))=-0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.564 GeV**2, EPSILON=0.4523, W=1.112 GeV and COS(THETA(*))=-0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.564 GeV**2, EPSILON=0.4523, W=1.112 GeV and COS(THETA(*))=-0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.564 GeV**2, EPSILON=0.4523, W=1.112 GeV and COS(THETA(*))=-0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.564 GeV**2, EPSILON=0.4523, W=1.112 GeV and COS(THETA(*))=0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.564 GeV**2, EPSILON=0.4523, W=1.112 GeV and COS(THETA(*))=0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.564 GeV**2, EPSILON=0.4523, W=1.112 GeV and COS(THETA(*))=0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.564 GeV**2, EPSILON=0.4523, W=1.112 GeV and COS(THETA(*))=0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.564 GeV**2, EPSILON=0.4523, W=1.112 GeV and COS(THETA(*))=0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.5 GeV**2, EPSILON=0.45, W=1.152 GeV and COS(THETA(*))=-0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.5 GeV**2, EPSILON=0.45, W=1.152 GeV and COS(THETA(*))=-0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.5 GeV**2, EPSILON=0.45, W=1.152 GeV and COS(THETA(*))=-0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.5 GeV**2, EPSILON=0.45, W=1.152 GeV and COS(THETA(*))=-0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.5 GeV**2, EPSILON=0.45, W=1.152 GeV and COS(THETA(*))=-0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.5 GeV**2, EPSILON=0.45, W=1.152 GeV and COS(THETA(*))=0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.5 GeV**2, EPSILON=0.45, W=1.152 GeV and COS(THETA(*))=0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.5 GeV**2, EPSILON=0.45, W=1.152 GeV and COS(THETA(*))=0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.5 GeV**2, EPSILON=0.45, W=1.152 GeV and COS(THETA(*))=0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.5 GeV**2, EPSILON=0.45, W=1.152 GeV and COS(THETA(*))=0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.432 GeV**2, EPSILON=0.4478, W=1.192 GeV and COS(THETA(*))=-0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.432 GeV**2, EPSILON=0.4478, W=1.192 GeV and COS(THETA(*))=-0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.432 GeV**2, EPSILON=0.4478, W=1.192 GeV and COS(THETA(*))=-0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.432 GeV**2, EPSILON=0.4478, W=1.192 GeV and COS(THETA(*))=-0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.432 GeV**2, EPSILON=0.4478, W=1.192 GeV and COS(THETA(*))=-0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.432 GeV**2, EPSILON=0.4478, W=1.192 GeV and COS(THETA(*))=0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.432 GeV**2, EPSILON=0.4478, W=1.192 GeV and COS(THETA(*))=0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.432 GeV**2, EPSILON=0.4478, W=1.192 GeV and COS(THETA(*))=0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.432 GeV**2, EPSILON=0.4478, W=1.192 GeV and COS(THETA(*))=0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.432 GeV**2, EPSILON=0.4478, W=1.192 GeV and COS(THETA(*))=0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.36 GeV**2, EPSILON=0.4458, W=1.232 GeV and COS(THETA(*))=-0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.36 GeV**2, EPSILON=0.4458, W=1.232 GeV and COS(THETA(*))=-0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.36 GeV**2, EPSILON=0.4458, W=1.232 GeV and COS(THETA(*))=-0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.36 GeV**2, EPSILON=0.4458, W=1.232 GeV and COS(THETA(*))=-0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.36 GeV**2, EPSILON=0.4458, W=1.232 GeV and COS(THETA(*))=-0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.36 GeV**2, EPSILON=0.4458, W=1.232 GeV and COS(THETA(*))=0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.36 GeV**2, EPSILON=0.4458, W=1.232 GeV and COS(THETA(*))=0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.36 GeV**2, EPSILON=0.4458, W=1.232 GeV and COS(THETA(*))=0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.36 GeV**2, EPSILON=0.4458, W=1.232 GeV and COS(THETA(*))=0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.36 GeV**2, EPSILON=0.4458, W=1.232 GeV and COS(THETA(*))=0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.288 GeV**2, EPSILON=0.4434, W=1.272 GeV and COS(THETA(*))=-0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.288 GeV**2, EPSILON=0.4434, W=1.272 GeV and COS(THETA(*))=-0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.288 GeV**2, EPSILON=0.4434, W=1.272 GeV and COS(THETA(*))=-0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.288 GeV**2, EPSILON=0.4434, W=1.272 GeV and COS(THETA(*))=-0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.288 GeV**2, EPSILON=0.4434, W=1.272 GeV and COS(THETA(*))=-0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.288 GeV**2, EPSILON=0.4434, W=1.272 GeV and COS(THETA(*))=0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.288 GeV**2, EPSILON=0.4434, W=1.272 GeV and COS(THETA(*))=0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.288 GeV**2, EPSILON=0.4434, W=1.272 GeV and COS(THETA(*))=0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.288 GeV**2, EPSILON=0.4434, W=1.272 GeV and COS(THETA(*))=0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.288 GeV**2, EPSILON=0.4434, W=1.272 GeV and COS(THETA(*))=0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.212 GeV**2, EPSILON=0.4411, W=1.312 GeV and COS(THETA(*))=-0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.212 GeV**2, EPSILON=0.4411, W=1.312 GeV and COS(THETA(*))=-0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.212 GeV**2, EPSILON=0.4411, W=1.312 GeV and COS(THETA(*))=-0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.212 GeV**2, EPSILON=0.4411, W=1.312 GeV and COS(THETA(*))=-0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.212 GeV**2, EPSILON=0.4411, W=1.312 GeV and COS(THETA(*))=-0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.212 GeV**2, EPSILON=0.4411, W=1.312 GeV and COS(THETA(*))=0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.212 GeV**2, EPSILON=0.4411, W=1.312 GeV and COS(THETA(*))=0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.212 GeV**2, EPSILON=0.4411, W=1.312 GeV and COS(THETA(*))=0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.212 GeV**2, EPSILON=0.4411, W=1.312 GeV and COS(THETA(*))=0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.212 GeV**2, EPSILON=0.4411, W=1.312 GeV and COS(THETA(*))=0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.136 GeV**2, EPSILON=0.4383, W=1.352 GeV and COS(THETA(*))=-0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.136 GeV**2, EPSILON=0.4383, W=1.352 GeV and COS(THETA(*))=-0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.136 GeV**2, EPSILON=0.4383, W=1.352 GeV and COS(THETA(*))=-0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.136 GeV**2, EPSILON=0.4383, W=1.352 GeV and COS(THETA(*))=-0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.136 GeV**2, EPSILON=0.4383, W=1.352 GeV and COS(THETA(*))=-0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.136 GeV**2, EPSILON=0.4383, W=1.352 GeV and COS(THETA(*))=0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.136 GeV**2, EPSILON=0.4383, W=1.352 GeV and COS(THETA(*))=0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.136 GeV**2, EPSILON=0.4383, W=1.352 GeV and COS(THETA(*))=0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.136 GeV**2, EPSILON=0.4383, W=1.352 GeV and COS(THETA(*))=0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.136 GeV**2, EPSILON=0.4383, W=1.352 GeV and COS(THETA(*))=0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.06 GeV**2, EPSILON=0.4351, W=1.392 GeV and COS(THETA(*))=-0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=6.06 GeV**2, EPSILON=0.4351, W=1.392 GeV and COS(THETA(*))=-0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.06 GeV**2, EPSILON=0.4351, W=1.392 GeV and COS(THETA(*))=-0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.06 GeV**2, EPSILON=0.4351, W=1.392 GeV and COS(THETA(*))=-0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.06 GeV**2, EPSILON=0.4351, W=1.392 GeV and COS(THETA(*))=-0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.06 GeV**2, EPSILON=0.4351, W=1.392 GeV and COS(THETA(*))=0.1 for the small SOS spectrometer.
Differential cross sections at Q**2=6.06 GeV**2, EPSILON=0.4351, W=1.392 GeV and COS(THETA(*))=0.3 for the small SOS spectrometer.
Differential cross sections at Q**2=6.06 GeV**2, EPSILON=0.4351, W=1.392 GeV and COS(THETA(*))=0.5 for the small SOS spectrometer.
Differential cross sections at Q**2=6.06 GeV**2, EPSILON=0.4351, W=1.392 GeV and COS(THETA(*))=0.7 for the small SOS spectrometer.
Differential cross sections at Q**2=6.06 GeV**2, EPSILON=0.4351, W=1.392 GeV and COS(THETA(*))=0.9 for the small SOS spectrometer.
Differential cross sections at Q**2=7.924 GeV**2, EPSILON=0.226, W=1.112 GeV and COS(THETA(*))=-0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.924 GeV**2, EPSILON=0.226, W=1.112 GeV and COS(THETA(*))=-0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.924 GeV**2, EPSILON=0.226, W=1.112 GeV and COS(THETA(*))=-0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.924 GeV**2, EPSILON=0.226, W=1.112 GeV and COS(THETA(*))=0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.924 GeV**2, EPSILON=0.226, W=1.112 GeV and COS(THETA(*))=0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.924 GeV**2, EPSILON=0.226, W=1.112 GeV and COS(THETA(*))=0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.848 GeV**2, EPSILON=0.2251, W=1.152 GeV and COS(THETA(*))=-0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.848 GeV**2, EPSILON=0.2251, W=1.152 GeV and COS(THETA(*))=-0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.848 GeV**2, EPSILON=0.2251, W=1.152 GeV and COS(THETA(*))=-0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.848 GeV**2, EPSILON=0.2251, W=1.152 GeV and COS(THETA(*))=0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.848 GeV**2, EPSILON=0.2251, W=1.152 GeV and COS(THETA(*))=0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.848 GeV**2, EPSILON=0.2251, W=1.152 GeV and COS(THETA(*))=0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.772 GeV**2, EPSILON=0.2236, W=1.192 GeV and COS(THETA(*))=-0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.772 GeV**2, EPSILON=0.2236, W=1.192 GeV and COS(THETA(*))=-0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.772 GeV**2, EPSILON=0.2236, W=1.192 GeV and COS(THETA(*))=-0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.772 GeV**2, EPSILON=0.2236, W=1.192 GeV and COS(THETA(*))=0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.772 GeV**2, EPSILON=0.2236, W=1.192 GeV and COS(THETA(*))=0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.772 GeV**2, EPSILON=0.2236, W=1.192 GeV and COS(THETA(*))=0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.692 GeV**2, EPSILON=0.2222, W=1.232 GeV and COS(THETA(*))=-0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.692 GeV**2, EPSILON=0.2222, W=1.232 GeV and COS(THETA(*))=-0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.692 GeV**2, EPSILON=0.2222, W=1.232 GeV and COS(THETA(*))=-0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.692 GeV**2, EPSILON=0.2222, W=1.232 GeV and COS(THETA(*))=0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.692 GeV**2, EPSILON=0.2222, W=1.232 GeV and COS(THETA(*))=0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.692 GeV**2, EPSILON=0.2222, W=1.232 GeV and COS(THETA(*))=0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.608 GeV**2, EPSILON=0.2211, W=1.272 GeV and COS(THETA(*))=-0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.608 GeV**2, EPSILON=0.2211, W=1.272 GeV and COS(THETA(*))=-0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.608 GeV**2, EPSILON=0.2211, W=1.272 GeV and COS(THETA(*))=-0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.608 GeV**2, EPSILON=0.2211, W=1.272 GeV and COS(THETA(*))=0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.608 GeV**2, EPSILON=0.2211, W=1.272 GeV and COS(THETA(*))=0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.608 GeV**2, EPSILON=0.2211, W=1.272 GeV and COS(THETA(*))=0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.524 GeV**2, EPSILON=0.2195, W=1.312 GeV and COS(THETA(*))=-0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.524 GeV**2, EPSILON=0.2195, W=1.312 GeV and COS(THETA(*))=-0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.524 GeV**2, EPSILON=0.2195, W=1.312 GeV and COS(THETA(*))=-0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.524 GeV**2, EPSILON=0.2195, W=1.312 GeV and COS(THETA(*))=0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.524 GeV**2, EPSILON=0.2195, W=1.312 GeV and COS(THETA(*))=0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.524 GeV**2, EPSILON=0.2195, W=1.312 GeV and COS(THETA(*))=0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.436 GeV**2, EPSILON=0.218, W=1.352 GeV and COS(THETA(*))=-0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.436 GeV**2, EPSILON=0.218, W=1.352 GeV and COS(THETA(*))=-0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.436 GeV**2, EPSILON=0.218, W=1.352 GeV and COS(THETA(*))=-0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.436 GeV**2, EPSILON=0.218, W=1.352 GeV and COS(THETA(*))=0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.436 GeV**2, EPSILON=0.218, W=1.352 GeV and COS(THETA(*))=0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.348 GeV**2, EPSILON=0.2161, W=1.392 GeV and COS(THETA(*))=-0.83 for the large SOS spectrometer.
Differential cross sections at Q**2=7.348 GeV**2, EPSILON=0.2161, W=1.392 GeV and COS(THETA(*))=-0.5 for the large SOS spectrometer.
Differential cross sections at Q**2=7.348 GeV**2, EPSILON=0.2161, W=1.392 GeV and COS(THETA(*))=-0.17 for the large SOS spectrometer.
Differential cross sections at Q**2=7.348 GeV**2, EPSILON=0.2161, W=1.392 GeV and COS(THETA(*))=0.17 for the large SOS spectrometer.
We present the first measurement of dijet angular distributions in ppbar collisions at sqrt{s}=1.96TeV at the Fermilab Tevatron Collider. The measurement is based on a dataset corresponding to an integrated luminosity of up to 0.7fb-1 collected with the D0 detector. Dijet angular distributions have been measured over a range of dijet masses, from 0.25TeV to above 1.1TeV. The data are in good agreement with the predictions of perturbative QCD and are used to constrain new physics models including quark compositeness, large extra dimensions, and TeV-1 scale extra dimensions. For all models we set the most stringent direct limits to date.
Normalized differential distribution in CHI(dijet) for two-jet mass 250 to 300 GeV and the non perturbative correction factor.
Normalized differential distribution in CHI(dijet) for two-jet mass 300 to 400 GeV and the non perturbative correction factor.
Normalized differential distribution in CHI(dijet) for two-jet mass 400 to 500 GeV and the non perturbative correction factor.
Normalized differential distribution in CHI(dijet) for two-jet mass 500 to 600 GeV and the non perturbative correction factor.
Normalized differential distribution in CHI(dijet) for two-jet mass 600 to 700 GeV and the non perturbative correction factor.
Normalized differential distribution in CHI(dijet) for two-jet mass 700 to 800 GeV and the non perturbative correction factor.
Normalized differential distribution in CHI(dijet) for two-jet mass 800 to 900 GeV and the non perturbative correction factor.
Normalized differential distribution in CHI(dijet) for two-jet mass 900 to 1000 GeV and the non perturbative correction factor.
Normalized differential distribution in CHI(dijet) for two-jet mass 1000 to1100 GeV and the non perturbative correction factor.
Normalized differential distribution in CHI(dijet) for two-jet mass > 1100 GeV and the non perturbative correction factor.
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