2001
DOI: 10.1103/physrevd.63.113009
|View full text |Cite
|
Sign up to set email alerts
|

Coherent exclusive exponentiation for precision Monte Carlo calculations

Abstract: We present the new coherent exclusive exponentiation ͑CEEX͒, the older exclusive exponentiation ͑EEX͒, and the semianalytical inclusive exponentiation ͑IEX͒ for the process e Ϫ e ϩ → f fϩn␥, where f ϭ , ,d,u,s,c,b, which are valid for center-of-mass energies from the lepton threshold to 1 TeV, that is, for CERN LEP1, LEP2, the SLC, future linear colliders, and b,c, factories, etc. The approaches are based on Yennie-Frautschi-Suura exponentiation. In CEEX, the effects due to photon emission from initial beams a… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

13
654
0
2

Year Published

2002
2002
2024
2024

Publication Types

Select...
7
1

Relationship

0
8

Authors

Journals

citations
Cited by 792 publications
(669 citation statements)
references
References 54 publications
13
654
0
2
Order By: Relevance
“…[35], and equal to 1.06 for both energies; (1+δ) is the radiative correction factor, equal to 0.844 for √ s = 4.23 GeV and 0.848 for √ s = 4.26 GeV obtained using Ref. [29,30] by assuming the line shape of Born cross section σ(e + e − → Z c (3900) ± π ∓ ) to be a BW function with the parameters of the Y(4260) taken from PDG [31]; and B ω and B π 0 are the branching fractions of the decay ω → π + π − π 0 and π 0 → γγ [31], respectively. A conservative estimate of the upper limit of the Born cross section is determined by lowering the efficiency by one standard deviation of the systematic uncertainty.…”
Section: Cross Section Upper Limits and Systematic Uncertaintymentioning
confidence: 99%
See 2 more Smart Citations
“…[35], and equal to 1.06 for both energies; (1+δ) is the radiative correction factor, equal to 0.844 for √ s = 4.23 GeV and 0.848 for √ s = 4.26 GeV obtained using Ref. [29,30] by assuming the line shape of Born cross section σ(e + e − → Z c (3900) ± π ∓ ) to be a BW function with the parameters of the Y(4260) taken from PDG [31]; and B ω and B π 0 are the branching fractions of the decay ω → π + π − π 0 and π 0 → γγ [31], respectively. A conservative estimate of the upper limit of the Born cross section is determined by lowering the efficiency by one standard deviation of the systematic uncertainty.…”
Section: Cross Section Upper Limits and Systematic Uncertaintymentioning
confidence: 99%
“…The decays of ω → π + π − π 0 are generated with the OMEGA DALITZ model in evtgen [27,28]. Initial state radiation (ISR) is simulated with kkmc [29,30], where the Born cross section of e + e − → Z c (3900) ± π ∓ is assumed to follow a Y (4260) Breit-Wigner (BW) line shape with resonance parameters taken from the Particle Data Group (PDG) [31], in which listed as X(4260). Final state radiation (FSR) effects associated with charged particles are handled with PHOTOS [29].…”
Section: Besiii Experiments and Monte Carlo Simulationmentioning
confidence: 99%
See 1 more Smart Citation
“…In this scheme, ISR is modelled with Coherent Exclusive Exponentiation (CEEX) [11] to O(α 2 ) precision. For the e + e − (nγ ) final-state process, BHWIDE [12] (v.1.00) is employed, in which ISR 25 OPAL uses a right-handed coordinate system in which the z axis is along the electron beam direction and the x axis is horizontal.…”
Section: Data and Monte Carlo Samplesmentioning
confidence: 99%
“…This process was simulated using the KK2f/CEEX [19] generator with hadronisation and fragmentation by PYTHIA 6.125 [20]. The CEEX modelling of ISR employs full second-order QED corrections to the matrix element, and applies coherent exponentiation of the QED corrections from interference between ISR and final-state radiation.…”
Section: Data Simulated Backgrounds and Signalsmentioning
confidence: 99%