2-7 June 2016
Auditorium Maximum
Europe/Warsaw timezone
14th International Workshop on Meson Production, Properties and Interaction
Home > Timetable > Session details
PDF | iCal

Parallel Session B2

Place

Location: Auditorium Maximum
Date: 2 Jun 16:55 - 18:35

Conveners

    • Guo, Feng-Kun (Institute of Theoretical Physics, CAS)

Timetable | Contribution List

Displaying 5 contributions out of 5
Type: parallel talk Session: Parallel Session B2
In a recent analysis of the exclusive production of $\eta-\pi$ and $\eta’-\pi$ meson systems with a 191 GeV/c pion beam on a proton target at COMPASS, an unexpected enhancement of $\eta’-\pi$ over $\eta-\pi$ was observed for the odd partial waves. These carry exotic quantum numbers therefore cannot be associated with the conventional quark-antiquark states. The collected data covers a wide r ... More
Presented by Vladiszlav PAUK on 2/6/2016 at 15:55
Type: parallel talk Session: Parallel Session B2
We shall describe the physics program with tagged forward protons, focusing on Central Exclusive Production (CEP) in polarized proton-proton collisions at the Relativistic Heavy Ion Collider (RHIC), with the STAR detector at $\sqrt{s} = 200$ GeV. Preliminary results in CEP of two oppositely charged pions and kons produced in the processes $pp\to pp \pi^+\pi^-$ and $pp\to pp K^+ K^-$ shall be pres ... More
Presented by Włodek GURYN on 2/6/2016 at 18:15
Type: parallel talk Session: Parallel Session B2
The Pierre Auger Observatory allows the study of ultra-high energy cosmic rays around and above 100 eV center-of-mass energy, inaccessible to accelerator experiments. A single cosmic ray initiate a chain reaction of billions interactions called extensive air showers. These interactions rely on extrapolations and in kinematic regions beyond those tested at accelerators. We report the constrains ... More
Presented by João ESPADANAL on 2/6/2016 at 16:55
Type: parallel talk Session: Parallel Session B2
IceCube's detection of ultra-high energy neutrino events heralds the beginning of neutrino astronomy. At very-high energies (100 TeV - 1 PeV), the dominant background to the astrophysical signal is the flux of prompt neutrinos, coming from the semi-leptonic decay of charmed mesons produced by cosmic ray collisions in the atmosphere. This is due to the very short lifetime of the charmed mesons, whi ... More
Presented by Tomasz PALCZEWSKI on 2/6/2016 at 17:15
Type: parallel talk Session: Parallel Session B2
A first measurement is presented of exclusive photoproduction of $\rho^0$ mesons associated with leading neutrons at HERA. The data were taken with the H1 detector in the years 2006 and 2007 at a centre-of-mass energy of $\sqrt(s)$ = 319 GeV and correspond to an integrated luminosity of 1.16 pb$^{−1}$ . The $\rho^0$ mesons with transverse momenta $p_T$ < 1 GeV are reconstructed from their decays ... More
Presented by Lidia GOERLICH on 2/6/2016 at 17:35
Building timetable...