Observation of B+ → pp̄π+, B0 → pp̄K0, and B+ → pp̄K*+

M. Z. Wang, K. Abe, T. Abe, I. Adachi, H. Aihara, Y. Asano, T. Aso, V. Aulchenko, T. Aushev, A. M. Bakich, A. Bay, I. Bizjak, A. Bondar, A. Bozek, M. Bračko, T. E. Browder, M. C. Chang, P. Chang, Y. Chao, K. F. ChenB. G. Cheon, R. Chistov, S. K. Choi, Y. Choi, Y. K. Choi, P. H. Chu, A. Chuvikov, M. Danilov, L. Y. Dong, A. Drutskoy, S. Eidelman, V. Eiges, C. Fukunaga, N. Gabyshev, A. Garmash, T. Gershon, G. Gokhroo, B. Golob, T. Hara, H. Hayashii, M. Hazumi, T. Hokuue, Y. Hoshi, W. S. Hou, H. C. Huang, K. Inami, A. Ishikawa, R. Itoh, H. Iwasaki, M. Iwasaki, Y. Iwasaki, J. H. Kang, N. Katayama, H. Kawai, T. Kawasaki, H. Kichimi, H. J. Kim, H. Kim, J. H. Kim, S. K. Kim, K. Kinoshita, P. Koppenburg, S. Korpar, P. Križan, P. Krokovny, A. Kuzmin, Y. J. Kwon, J. S. Lange, S. H. Lee, T. Lesiak, A. Limosani, S. W. Lin, J. MacNaughton, G. Majumder, F. Mandl, T. Matsumoto, W. Mitaroff, H. Miyake, H. Miyata, T. Nagamine, Y. Nagasaka, E. Nakano, S. Nishida, O. Nitoh, S. Ogawa, T. Ohshima, S. Okuno, S. L. Olsen, W. Ostrowicz, H. Ozaki, P. Pakhlov, H. Palka, C. W. Park, H. Park, N. Parslow, L. E. Piilonen, M. Rozanska, H. Sagawa, S. Saitoh, Y. Sakai, T. R. Sarangi, O. Schneider, A. J. Schwartz, S. Semenov, H. Shibuya, V. Sidorov, J. B. Singh, N. Soni, S. Stanič, M. Starič, A. Sugiyama, K. Sumisawa, T. Sumiyoshi, S. Suzuki, S. Y. Suzuki, F. Takasaki, K. Tamai, N. Tamura, M. Tanaka, Y. Teramoto, T. Tomura, T. Tsuboyama, T. Tsukamoto, S. Uehara, S. Uno, G. Varner, K. E. Varvell, C. H. Wang, J. G. Wang, Y. Watanabe, Y. Yamada, A. Yamaguchi, Y. Yamashita, M. Yamauchi, H. Yanai, J. Ying, Y. Yuan, Y. Yusa, C. C. Zhang, Z. P. Zhang, V. Zhilich, D. Žontar

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Abstract

The observation of B+ → pp̄π+, which is dominated by the b→u tree diagram was studied. The observation of B 0 → pp̄K0 and B+→pp̄K *+ was also presented and the mesurement of B +→pp̄K+ was improved. It was found that a search for the B0→pp̄K*0 mode yielded only an upper limit. The pp̄ mass spectra was also studied to see if the threshold peaking confirmed with the newly observed modes.

Original languageEnglish
Article number131801
Pages (from-to)131801-1-131801-6
JournalPhysical review letters
Volume92
Issue number13
DOIs
Publication statusPublished - 2004 Apr 2

Bibliographical note

Funding Information:
We wish to thank the KEKB accelerator group for the excellent operation of the KEKB accelerator. We acknowledge support from the Ministry of Education, Culture, Sports, Science, and Technology of Japan and the Japan Society for the Promotion of Science; from the Australian Research Council and the Australian Department of Education, Science and Training; from the National Science Foundation of China under Contract No. 10175071; from the Department of Science and Technology of India; from the BK21 program of ?>the Ministry of Education of Korea and the CHEP ?>SRC program of the Korea Science and Engineering Foundation; from the Polish State Committee for Scientific Research under Contract No. 2P03B 01324; from the Ministry of Science and Technology of the Russian Federation; from the Ministry of Education, Science and Sport of the Republic of Slovenia; from the National Science Council and the Ministry of Education of Taiwan; and from the U.S. Department of Energy.

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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