2006
DOI: 10.1140/epjc/s2006-02614-7
|View full text |Cite
|
Sign up to set email alerts
|

Electron–positron annihilation into three pions and the radiative return

Abstract: The Monte Carlo event generator PHOKHARA, which simulates hadron and muon production at electron-positron colliders through radiative return, has been extended to final states with three pions. A model for the form factor based on generalized vector dominance has been employed, which is consistent with presently available experimental observations.

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
1

Citation Types

5
79
0

Year Published

2013
2013
2022
2022

Publication Types

Select...
5
2

Relationship

2
5

Authors

Journals

citations
Cited by 50 publications
(84 citation statements)
references
References 25 publications
(43 reference statements)
5
79
0
Order By: Relevance
“…An indirect comparison of the results in Refs. [3,6,7] was also reported in Ref. [8] via a comparison of the two Monte Carlo programs PHOKHARA [9] and KK MC [10], as these two Monte Carlos have the realizations of the results in Ref.…”
mentioning
confidence: 72%
See 3 more Smart Citations
“…An indirect comparison of the results in Refs. [3,6,7] was also reported in Ref. [8] via a comparison of the two Monte Carlo programs PHOKHARA [9] and KK MC [10], as these two Monte Carlos have the realizations of the results in Ref.…”
mentioning
confidence: 72%
“…[6,7], where the result is obtained by an independent method via a leptonic tensor calculated to investigate radiative return, with particular emphasis on the 1-2 GeV cms energy regime. This permits a cross-check at the NNLL level of the corresponding results.…”
mentioning
confidence: 99%
See 2 more Smart Citations
“…The main difference in the event selection with respect to the LA analysis is that the detection of the ISR photon is vetoed. The simulation of signal and ISR background events makes use of the Phokhara [25] event generator, which takes into account next-to-leading-order radiative corrections. The maximum transverse momentum of the pp system must be smaller than 0.15 GeV/c, and the missing mass squared M 2 miss < 1 GeV/c 2 , consistently with an event with a missing photon at small polar angle.…”
Section: Measurement Of E + E − → Ppmentioning
confidence: 99%