The photon spectrum in Υ decays
Creators
- 1. Theory Group, Fermilab, P.O. Box 500, Batavia, Illinois 60510 (United States)
- 2. Department of Physics, Carnegie Mellon University, Pittsburgh, Pennsylvania 15213 (United States)
Description
We present a theoretical prediction for the photon spectrum in radiative Υ decay. Parts of the spectrum have already been understood, but an understanding of the end point region has remained elusive. In this paper we provide the missing piece, and resolve a controversy in the literature. We treat the end point region of Υ→Xγ decay within the framework of the soft-collinear effective theory (SCET). Within this approach the Υ structure function arises naturally, and kinematic logarithms are summed by running operators using renormalization group equations. In a previous paper we studied the color-octet contribution to the decay. Here we treat the color-singlet contribution. We combine our result with previous results to obtain the Υ→Xγ spectrum. We find that resumming the color-singlet contribution in the end point gives a result that is in much better agreement with the data than the leading order prediction
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.67.074035;
- arXiv
- arXiv:hep-ph/0212094v1;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 67
- Journal Issue
- 7
- Journal Page Range
- p. 074035-074035.16
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35075490
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COLOR MODEL; PARTICLE DECAY; PHOTONS; RENORMALIZATION; RESONANCE PARTICLES; STRUCTURE FUNCTIONS; UPSILON-10355 MESONS; UPSILON-10580 MESONS
- Descriptors DEC
- BOSONS; BOTTOMONIUM; COMPOSITE MODELS; DECAY; ELEMENTARY PARTICLES; FUNCTIONS; HADRONS; MASSLESS PARTICLES; MATHEMATICAL MODELS; MESONS; PARTICLE MODELS; QUARK MODEL; QUARKONIUM; VECTOR MESONS
Optional Information
- Notes
- (c) 2003 The American Physical Society