phi photo-production from Li, C, Al, and Cu nuclei at Egamma=1.5 - 2.4 GeV
| dc.creator | Ishikawa, T. | |
| dc.creator | Ahn, D. S. | |
| dc.creator | Ahn, J. K. | |
| dc.creator | Akimune, H. | |
| dc.creator | Chang, W. C. | |
| dc.creator | Date, S. | |
| dc.creator | Fujimura, H. | |
| dc.creator | Fujiwara, M. | |
| dc.creator | Hicks, K. | |
| dc.creator | Hotta, T. | |
| dc.creator | Imai, K. | |
| dc.creator | Kawai, H. | |
| dc.creator | Kino, K. | |
| dc.creator | Kohri, H. | |
| dc.creator | Matsumura, T. | |
| dc.creator | Mibe, T. | |
| dc.creator | Miwa, K. | |
| dc.creator | Miyabe, M. | |
| dc.creator | Morita, M. | |
| dc.creator | Murakami, T. | |
| dc.creator | Muramatsu, N. | |
| dc.creator | Nakamura, H. | |
| dc.creator | Nakamura, M. | |
| dc.creator | Nakano, T. | |
| dc.creator | Niiyama, M. | |
| dc.creator | Nomachi, M. | |
| dc.creator | Ohashi, Y. | |
| dc.creator | Ooba, T. | |
| dc.creator | Oshuev, D. S. | |
| dc.creator | Rangacharyulu, C. | |
| dc.creator | Sakaguchi, A. | |
| dc.creator | Shiino, Y. | |
| dc.creator | Sakemi, Y. | |
| dc.creator | Shimizu, H. | |
| dc.creator | Sugaya, Y. | |
| dc.creator | Sumihama, M. | |
| dc.creator | Toi, Y. | |
| dc.creator | Toyokawa, H. | |
| dc.creator | Wang, C. W. | |
| dc.creator | Yorita, T. | |
| dc.creator | Yosoi, M. | |
| dc.creator | Zegers, R. G. T. | |
| dc.date | 2004-11-09 | |
| dc.date.accessioned | 2026-07-07T06:26:58Z | |
| dc.date.available | 2026-07-07T06:26:58Z | |
| dc.description | The photo-production of $ϕ$ mesons from Li, C, Al, and Cu at forward angles has been measured at $E_gamma$=1.5--2.4 GeV. The number of events for incoherent phi photo-production is found to have a target mass number dependence of $A^{0.72\pm 0.07}$ in the kinematical region of $|t|\le 0.6$ ${\rm GeV}^2/c^2$. The total cross section of the $ϕ$-nucleon interaction, $σ_{ϕN}$, has been estimated as $35^{+17}_{-11}$ mb using the $A$-dependence of the $ϕ$ photo-production yield and a Glauber-type multiple scattering theory. This value is much larger than $σ_{ϕN}$ in free space, suggesting that the $ϕ$ properties might change in the nuclear medium. | |
| dc.description | 12 pages 4 figures, submitted to Phys. Lett. B | |
| dc.identifier | https://arxiv.org/abs/nucl-ex/0411016 | |
| dc.identifier | http://arxiv.org/abs/nucl-ex/0411016 | |
| dc.identifier | Phys.Lett. B608 (2005) 215-222 | |
| dc.identifier | doi:10.1016/j.physletb.2005.01.023 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/97282 | |
| dc.subject | Nuclear Experiment | |
| dc.title | phi photo-production from Li, C, Al, and Cu nuclei at Egamma=1.5 - 2.4 GeV | |
| dc.type | text |