7-12 June 2018
Auditorium Maximum
Europe/Warsaw timezone
15th International Workshop on Meson Production, Properties and Interaction
Parallel Session B5
Place
Location: Auditorium Maximum
Date:
11 Jun 15:00 - 16:25
Conveners
-
- Ramstein, Beatrice (Institut de Physique Nucleaire Orsay)
Timetable | Contribution List
Displaying 4
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In 2017-2018 the CMD-3 detector continued collecting data at the electron-positron collider VEPP-2000. After upgrading the positron injection facility, an average luminosity
increased by a factor of three. In 2017 the scan was performed in the center-of-mass energy range from 1 to 2 GeV while in 2018 we scanned the energy region below 1 GeV to measure the pion form factor and omega meson paramete
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Presented by Guennady FEDOTOVICH
on
11/6/2018
at
13:25
Pion production in $NN$ collisions is one of the sources of information on the $NN$ interaction and on the contribution of nucleon resonances. In particular, two-pion production in the few energy range, carries information both on $\pi\pi$ dynamics and on single and double baryon excitation.
The High Acceptance Di-Electron Spectrometer (HADES)[1] installed at GSI
Helmholtz-Zentrum für Schweri
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Presented by Amel BELOUNNAS
on
11/6/2018
at
14:05
In 2017 the SND and CMD-3 experiments resumed to take data at the VEPP-2000 $e^+e^-$ collider after its upgrade. Using are a new positron source allows significantly increase collider luminocity. We present current status of the SND and CMD-3 experiments and recent result of data analysis, in particular,
on the processes $e+e-\to \pi^+\pi^-$, $K\bar{K}$, $n\bar{n}$,
$\pi^+\pi^-\eta$, $\pi^+\pi^\
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Presented by Konstantin BELOBORODOV
on
11/6/2018
at
13:00
The chiral anomaly refers to the classical axial symmetry of QCD broken by quantum fluctuations. For pseudoscalar mesons, the chiral anomaly generates a sizable mixing of nonstrange and strange components, leading to the physical states $\eta(547)$ and $\eta(958)$ (the mixing angle is about $-42^{\circ}$).
Yet, what about mesons with different quantum numbers? We present a classifications of meso
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Presented by Francesco GIACOSA
on
11/6/2018
at
13:45