Published July 1, 2003 | Version v1
Journal article

Study of parton kT smearing effects in direct photon production at the Fermilab Tevatron

  • 1. Centre for Detector and Related Software Technology, Department of Physics and Astrophysics, University of Delhi, Delhi 110 007 (India)

Description

Previous detailed studies of direct photon production from both fixed-target and collider experiments have witnessed a pattern of deviation between the measured inclusive cross sections and the corresponding theoretical expectations in the low transverse momentum (pT) regime. Most data sets display steeper pT dependence than the next-to-leading-order (NLO) perturbative QCD (PQCD) calculations with standard choices of scales and parton distribution functions in this region. A simple implementation of higher-order soft-gluon corrections to the NLO PQCD predictions significantly improves the agreement between data and theory. This interesting feature motivated us to investigate the DOe and CDF measurements of inclusive photon cross section at √(s)=1.8 TeV from the run 1b and also at √(s)=630 GeV. We use the latest updated parton distribution function CTEQ6M in the NLO QCD calculations for direct photon cross section to describe the data. The conventional theoretical uncertainties originating from scale dependence and gluon distributions have been illustrated. We estimate the impact of additional soft-gluon radiation on the direct photon production using PYTHIA (LO PQCD), which adds transverse momentum kT to initial-state partons through a Gaussian smearing. The impact of kT effects on the discrepancy in the low-pT region is explored using a phenomenological model, wherein we merge the NLO calculations with kT correction factors. We show that this approach provides a much more acceptable description of the Fermilab Tevatron data

Additional details

Identifiers

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
68
Journal Issue
1
Journal Page Range
p. 014017-014017.10
ISSN
0556-2821
CODEN
PRVDAQ

Optional Information

Notes
(c) 2003 The American Physical Society