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Modification of the omega-meson lifetime in nuclear matter.

Authors :
Kotulla M
Trnka D
Mühlich P
Anton G
Bacelar JC
Bartholomy O
Bayadilov D
Beloglazov YA
Bogendörfer R
Castelijns R
Crede V
Dutz H
Ehmanns A
Elsner D
Ewald R
Fabry I
Fuchs M
Essig K
Funke Ch
Gothe R
Gregor R
Gridnev AB
Gutz E
Höffgen S
Hoffmeister P
Horn I
Hössl J
Jaegle I
Junkersfeld J
Kalinowsky H
Klein F
Klein F
Klempt E
Konrad M
Kopf B
Krusche B
Langheinrich J
Löhner H
Lopatin IV
Lotz J
Lugert S
Menze D
Messchendorp JG
Mertens T
Metag V
Mosel U
Nanova M
Novotny R
Ostrick M
Pant LM
van Pee H
Pfeiffer M
Roy A
Radkov A
Schadmand S
Schmidt Ch
Schmieden H
Schoch B
Shende S
Suft G
Sumachev VV
Szczepanek T
Süle A
Thoma U
Varma R
Walther D
Weinheimer Ch
Wendel Ch
Source :
Physical review letters [Phys Rev Lett] 2008 May 16; Vol. 100 (19), pp. 192302. Date of Electronic Publication: 2008 May 13.
Publication Year :
2008

Abstract

Information on hadron properties in the nuclear medium has been derived from the photoproduction of omega mesons on the nuclei C, Ca, Nb, and Pb using the Crystal Barrel/TAPS detector at the ELSA tagged photon facility in Bonn. The dependence of the omega-meson cross section on the nuclear mass number has been compared with three different types of models: a Glauber analysis, a Boltzmann-Uehling-Uhlenbeck analysis of the Giessen theory group, and a calculation by the Valencia theory group. In all three cases, the inelastic omega width is found to be 130-150 MeV/c(2) at normal nuclear matter density for an average 3-momentum of 1.1 GeV/c. In the rest frame of the omega meson, this inelastic omega width corresponds to a reduction of the omega lifetime by a factor approximately 30. For the first time, the momentum dependent omegaN cross section has been extracted from the experiment and is in the range of 70 mb.

Details

Language :
English
ISSN :
0031-9007
Volume :
100
Issue :
19
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
18518443
Full Text :
https://doi.org/10.1103/PhysRevLett.100.192302