TY  - JOUR
AU  - Kaskulov, M.
AU  - Hernandez, E.
AU  - Oset, E.
PY  - 2010
DA  - 2010//
TI  - On the background in the gamma p -> omega(pi(0)gamma)p reaction and mixed event simulation
T2  - Eur. Phys. J. A
JO  - European Physical Journal A
SP  - 223
EP  - 230
VL  - 46
IS  - 2
PB  - Springer
AB  - In this paper we evaluate sources of background of the gamma p -> omega p reaction, with the omega detected through its pi(0)gamma decay channel, to compare with the experiment carried out at ELSA. We find background from gamma p -> pi(0)pi(0)p followed by decay of a pi(0) into two gamma, recombining one pi(0) and one gamma, and from the gamma p -> pi(0)eta p reaction with subsequent decay of the eta into two photons. This background accounts for the data at pi(0)gamma invariant masses beyond 700 MeV, but strength is missing at lower invariant masses which was attributed to photon misidentification events, which we simulate to get a good reproduction of the experimental background. Once this is done, we perform an event mixing simulation to reproduce the calculated background and we find that the method provides a good description of the background. A closer look reveals this is accidental. We show that the mixed event generated background in the region of the omega mass and beyond is completely tied to the events at low pi(0)gamma invariant masses where the d sigma/dM(pi 0 gamma) distribution is much larger. This has as a consequence that the mixed event method produces the same background at high invariant masses independently of the actual background in that region, as a consequence of which, the method is unsuited to give the background at energies around the peak of the omega and beyond.
SN  - 1434-6001
UR  - http://lanl.arxiv.org/abs/1003.2363
UR  - https://doi.org/10.1140/epja/i2010-11033-x
DO  - 10.1140/epja/i2010-11033-x
LA  - English
N1  - ISI:000284869600008
ID  - Kaskulov_etal2010
ER  -