activity
19962011
most citedI=0, C=-1 mesons from 1940 to 2410 MeV

47 citations · 47 across the 1 of their papers we have counts for

collaborators

12 papers

hep-ex2011★ 47 cited

I=0, C=-1 mesons from 1940 to 2410 MeV

A. V. Anisovich, C. A. Baker, C. J. Batty +6

New Crystal Barrel data are reported for pbar-p -> omega-eta and pbar-p -> omega-pizero-pizero with omega decaying to piplus-piminus-pizero. The omega-eta data confirm angular dist…

hep-ph2009

The rho -> gamma pi and omega -> gamma pi decays in quark-model approach and estimation of coupling for pion emission by quark

A. V. Anisovich, V. V. Anisovich, L. G. Dakhno +3

In the framework of the relativistic and gauge invariant spectral integral technique, we calculate radiative decays rho(770)-> gamma pi(140) and omega(780)-> gamma pi(140) supposin…

nucl-ex2007

Photoproduction of pi0-mesons off protons from the Delta(1232) region to E(gamma) = 3 GeV

H. van Pee, O. Bartholomy, V. Crede

Photoproduction of pi0 mesons was studied with the Crystal-Barrel detector at ELSA for incident energies from 300 MeV to 3 GeV. Differential cross sections d sigma /d Omega, d sigm…

nucl-ex2007

Photoproduction of pi0 omega off protons for E(gamma) < 3 GeV

J. Junkersfeld

Differential and total cross-sections for photoproduction of gamma proton to proton pi0 omega and gamma proton to Delta+ omega were determined from measurements of the CB-ELSA expe…

hep-ph2005

Quark--antiquark states and their radiative transitions in terms of the spectral integral equation. {\Huge III.} Light mesons

V. V. Anisovich, L. G. Dakhno, M. A. Matveev +2

We continue the investigation of mesons in terms of the spectral integral equation initiated before [hep-ph/0510410, hep-ph/0511005] for the and systems: in thi…

hep-ex2004

Neutral pion photoproduction off protons in the energy range 0.3 GeV < E(gamma) < 3 GeV

Olivia Bartholomy, Volker Crede, Harald van Pee

Single pi0 photoproduction has been studied with the CB-ELSA experiment at Bonn using tagged photon energies between 0.3 and 3.0 GeV. The experimental setup covers a very large sol…