Observation of chicJ radiative decays to light vector mesons
Using a total of 2.74 x 10(7) decays of the psi(2S) collected with the CLEO-c detector, we present a study of chi(cJ)-->gammaV, where V=rho(0), omega, phi. The transitions chi(c1)-->gammarho(0 and chi(c1)-->gammaomega are observed with B(chi(c1)-->gammarho(0))=(2.43+/-0.19+/-0.22) x 10(-...
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| Veröffentlicht in: | Physical review letters 2008-10, Vol.101 (15), p.151801-151801 |
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| creator | Bennett, J V Mitchell, R E Shepherd, M R Besson, D Pedlar, T K Cronin-Hennessy, D Gao, K Y Hietala, J Kubota, Y Klein, T Lang, B W Poling, R Scott, A W Zweber, P Dobbs, S Metreveli, Z Seth, K K Tan, B J Y Tomaradze, A Libby, J Martin, L Powell, A Wilkinson, G Ecklund, K M Love, W Savinov, V Mendez, H Ge, J Y Miller, D H Shipsey, I P J Xin, B Adams, G S Hu, D Moziak, B Napolitano, J He, Q Insler, J Muramatsu, H Park, C S Thorndike, E H Yang, F Artuso, M Blusk, S Khalil, S Li, J Mountain, R Nisar, S Randrianarivony, K Sultana, N Skwarnicki, T Stone, S Wang, J C Zhang, L M Bonvicini, G Cinabro, D Dubrovin, M Lincoln, A Naik, P Rademacker, J Asner, D M Edwards, K W Reed, J Briere, R A Tatishvili, G Vogel, H Rosner, J L Alexander, J P Cassel, D G Duboscq, J E Ehrlich, R Fields, L Galik, R S Gibbons, L Gray, R Gray, S W Hartill, D L Heltsley, B K Hertz, D Hunt, J M Kandaswamy, J Kreinick, D L Kuznetsov, V E Ledoux, J Mahlke-Krüger, H Mohapatra, D Onyisi, P U E Patterson, J R Peterson, D Riley, D Ryd, A Sadoff, A J Shi, X Stroiney, S Sun, W M Wilksen, T Athar, S B Patel, R Yelton, J Rubin, P Eisenstein, B I |
| description | Using a total of 2.74 x 10(7) decays of the psi(2S) collected with the CLEO-c detector, we present a study of chi(cJ)-->gammaV, where V=rho(0), omega, phi. The transitions chi(c1)-->gammarho(0 and chi(c1)-->gammaomega are observed with B(chi(c1)-->gammarho(0))=(2.43+/-0.19+/-0.22) x 10(-4) and B(chi(c1)-->gammaomega)=(8.3+/-1.5+/-1.2) x 10(-5). In the chi(c1)-->gammarho(0) transition, the final state meson is dominantly longitudinally polarized. Upper limits on the branching fractions of other chi(cJ) states to light vector mesons are presented. |
| format | Article |
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The transitions chi(c1)-->gammarho(0 and chi(c1)-->gammaomega are observed with B(chi(c1)-->gammarho(0))=(2.43+/-0.19+/-0.22) x 10(-4) and B(chi(c1)-->gammaomega)=(8.3+/-1.5+/-1.2) x 10(-5). In the chi(c1)-->gammarho(0) transition, the final state meson is dominantly longitudinally polarized. 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S</creatorcontrib><creatorcontrib>Wang, J C</creatorcontrib><creatorcontrib>Zhang, L M</creatorcontrib><creatorcontrib>Bonvicini, G</creatorcontrib><creatorcontrib>Cinabro, D</creatorcontrib><creatorcontrib>Dubrovin, M</creatorcontrib><creatorcontrib>Lincoln, A</creatorcontrib><creatorcontrib>Naik, P</creatorcontrib><creatorcontrib>Rademacker, J</creatorcontrib><creatorcontrib>Asner, D M</creatorcontrib><creatorcontrib>Edwards, K W</creatorcontrib><creatorcontrib>Reed, J</creatorcontrib><creatorcontrib>Briere, R A</creatorcontrib><creatorcontrib>Tatishvili, G</creatorcontrib><creatorcontrib>Vogel, H</creatorcontrib><creatorcontrib>Rosner, J L</creatorcontrib><creatorcontrib>Alexander, J P</creatorcontrib><creatorcontrib>Cassel, D G</creatorcontrib><creatorcontrib>Duboscq, J E</creatorcontrib><creatorcontrib>Ehrlich, R</creatorcontrib><creatorcontrib>Fields, L</creatorcontrib><creatorcontrib>Galik, R S</creatorcontrib><creatorcontrib>Gibbons, L</creatorcontrib><creatorcontrib>Gray, R</creatorcontrib><creatorcontrib>Gray, S W</creatorcontrib><creatorcontrib>Hartill, D L</creatorcontrib><creatorcontrib>Heltsley, B K</creatorcontrib><creatorcontrib>Hertz, D</creatorcontrib><creatorcontrib>Hunt, J M</creatorcontrib><creatorcontrib>Kandaswamy, J</creatorcontrib><creatorcontrib>Kreinick, D L</creatorcontrib><creatorcontrib>Kuznetsov, V E</creatorcontrib><creatorcontrib>Ledoux, J</creatorcontrib><creatorcontrib>Mahlke-Krüger, H</creatorcontrib><creatorcontrib>Mohapatra, D</creatorcontrib><creatorcontrib>Onyisi, P U E</creatorcontrib><creatorcontrib>Patterson, J R</creatorcontrib><creatorcontrib>Peterson, D</creatorcontrib><creatorcontrib>Riley, D</creatorcontrib><creatorcontrib>Ryd, A</creatorcontrib><creatorcontrib>Sadoff, A J</creatorcontrib><creatorcontrib>Shi, X</creatorcontrib><creatorcontrib>Stroiney, S</creatorcontrib><creatorcontrib>Sun, W M</creatorcontrib><creatorcontrib>Wilksen, T</creatorcontrib><creatorcontrib>Athar, S 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The transitions chi(c1)-->gammarho(0 and chi(c1)-->gammaomega are observed with B(chi(c1)-->gammarho(0))=(2.43+/-0.19+/-0.22) x 10(-4) and B(chi(c1)-->gammaomega)=(8.3+/-1.5+/-1.2) x 10(-5). In the chi(c1)-->gammarho(0) transition, the final state meson is dominantly longitudinally polarized. Upper limits on the branching fractions of other chi(cJ) states to light vector mesons are presented.</description><issn>0031-9007</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2008</creationdate><recordtype>article</recordtype><recordid>eNo1j7tqwzAYRjW0NGnaVyiauhlkSbYk6FJCrwSyZDe6_GpUbMuVZEPevoGm04GPwwfnCq0JYXWlCBErdJvzNyGkpq28QataKqUaKdfoaW8ypEWXEEccPbbHYD9x0i6cpwWwA6tPGZeI-_B1LHgBW2LCA-Q45jt07XWf4f7CDTq8vhy279Vu__axfd5VU8NlJSgFK6hWnloO2gvSGi6pl9Q5abjVnlnJOfEWeK2pNsLRxivXMkqYaRTboMe_2ynFnxly6YaQLfS9HiHOuWuVEFQJchYfLuJsBnDdlMKg06n7z2W_-lZQWA</recordid><startdate>20081010</startdate><enddate>20081010</enddate><creator>Bennett, J V</creator><creator>Mitchell, R E</creator><creator>Shepherd, M R</creator><creator>Besson, D</creator><creator>Pedlar, T K</creator><creator>Cronin-Hennessy, D</creator><creator>Gao, K Y</creator><creator>Hietala, J</creator><creator>Kubota, Y</creator><creator>Klein, T</creator><creator>Lang, B W</creator><creator>Poling, 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L</creatorcontrib><creatorcontrib>Kuznetsov, V E</creatorcontrib><creatorcontrib>Ledoux, J</creatorcontrib><creatorcontrib>Mahlke-Krüger, H</creatorcontrib><creatorcontrib>Mohapatra, D</creatorcontrib><creatorcontrib>Onyisi, P U E</creatorcontrib><creatorcontrib>Patterson, J R</creatorcontrib><creatorcontrib>Peterson, D</creatorcontrib><creatorcontrib>Riley, D</creatorcontrib><creatorcontrib>Ryd, A</creatorcontrib><creatorcontrib>Sadoff, A J</creatorcontrib><creatorcontrib>Shi, X</creatorcontrib><creatorcontrib>Stroiney, S</creatorcontrib><creatorcontrib>Sun, W M</creatorcontrib><creatorcontrib>Wilksen, T</creatorcontrib><creatorcontrib>Athar, S B</creatorcontrib><creatorcontrib>Patel, R</creatorcontrib><creatorcontrib>Yelton, J</creatorcontrib><creatorcontrib>Rubin, P</creatorcontrib><creatorcontrib>Eisenstein, B I</creatorcontrib><creatorcontrib>CLEO Collaboration</creatorcontrib><collection>PubMed</collection><collection>MEDLINE - Academic</collection><jtitle>Physical review letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bennett, J V</au><au>Mitchell, R E</au><au>Shepherd, M R</au><au>Besson, D</au><au>Pedlar, T K</au><au>Cronin-Hennessy, D</au><au>Gao, K Y</au><au>Hietala, J</au><au>Kubota, Y</au><au>Klein, T</au><au>Lang, B W</au><au>Poling, R</au><au>Scott, A W</au><au>Zweber, P</au><au>Dobbs, S</au><au>Metreveli, Z</au><au>Seth, K K</au><au>Tan, B J Y</au><au>Tomaradze, A</au><au>Libby, J</au><au>Martin, L</au><au>Powell, A</au><au>Wilkinson, G</au><au>Ecklund, K M</au><au>Love, W</au><au>Savinov, V</au><au>Mendez, H</au><au>Ge, J Y</au><au>Miller, D H</au><au>Shipsey, I P J</au><au>Xin, B</au><au>Adams, G S</au><au>Hu, D</au><au>Moziak, B</au><au>Napolitano, J</au><au>He, Q</au><au>Insler, J</au><au>Muramatsu, H</au><au>Park, C S</au><au>Thorndike, E H</au><au>Yang, F</au><au>Artuso, M</au><au>Blusk, S</au><au>Khalil, S</au><au>Li, J</au><au>Mountain, R</au><au>Nisar, S</au><au>Randrianarivony, K</au><au>Sultana, N</au><au>Skwarnicki, T</au><au>Stone, S</au><au>Wang, J C</au><au>Zhang, L M</au><au>Bonvicini, G</au><au>Cinabro, D</au><au>Dubrovin, M</au><au>Lincoln, A</au><au>Naik, P</au><au>Rademacker, J</au><au>Asner, D M</au><au>Edwards, K W</au><au>Reed, J</au><au>Briere, R A</au><au>Tatishvili, G</au><au>Vogel, H</au><au>Rosner, J L</au><au>Alexander, J P</au><au>Cassel, D G</au><au>Duboscq, J E</au><au>Ehrlich, R</au><au>Fields, L</au><au>Galik, R S</au><au>Gibbons, L</au><au>Gray, R</au><au>Gray, S W</au><au>Hartill, D L</au><au>Heltsley, B K</au><au>Hertz, D</au><au>Hunt, J M</au><au>Kandaswamy, J</au><au>Kreinick, D L</au><au>Kuznetsov, V E</au><au>Ledoux, J</au><au>Mahlke-Krüger, H</au><au>Mohapatra, D</au><au>Onyisi, P U E</au><au>Patterson, J R</au><au>Peterson, D</au><au>Riley, D</au><au>Ryd, A</au><au>Sadoff, A J</au><au>Shi, X</au><au>Stroiney, S</au><au>Sun, W M</au><au>Wilksen, T</au><au>Athar, S B</au><au>Patel, R</au><au>Yelton, J</au><au>Rubin, P</au><au>Eisenstein, B I</au><aucorp>CLEO Collaboration</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Observation of chicJ radiative decays to light vector mesons</atitle><jtitle>Physical review letters</jtitle><addtitle>Phys Rev Lett</addtitle><date>2008-10-10</date><risdate>2008</risdate><volume>101</volume><issue>15</issue><spage>151801</spage><epage>151801</epage><pages>151801-151801</pages><issn>0031-9007</issn><abstract>Using a total of 2.74 x 10(7) decays of the psi(2S) collected with the CLEO-c detector, we present a study of chi(cJ)-->gammaV, where V=rho(0), omega, phi. The transitions chi(c1)-->gammarho(0 and chi(c1)-->gammaomega are observed with B(chi(c1)-->gammarho(0))=(2.43+/-0.19+/-0.22) x 10(-4) and B(chi(c1)-->gammaomega)=(8.3+/-1.5+/-1.2) x 10(-5). In the chi(c1)-->gammarho(0) transition, the final state meson is dominantly longitudinally polarized. Upper limits on the branching fractions of other chi(cJ) states to light vector mesons are presented.</abstract><cop>United States</cop><pmid>18999588</pmid><tpages>1</tpages></addata></record> |
| fulltext | fulltext |
| identifier | ISSN: 0031-9007 |
| ispartof | Physical review letters, 2008-10, Vol.101 (15), p.151801-151801 |
| issn | 0031-9007 |
| language | eng |
| recordid | cdi_proquest_miscellaneous_69772970 |
| source | American Physical Society Journals |
| title | Observation of chicJ radiative decays to light vector mesons |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-07T16%3A47%3A04IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_pubme&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Observation%20of%20chicJ%20radiative%20decays%20to%20light%20vector%20mesons&rft.jtitle=Physical%20review%20letters&rft.au=Bennett,%20J%20V&rft.aucorp=CLEO%20Collaboration&rft.date=2008-10-10&rft.volume=101&rft.issue=15&rft.spage=151801&rft.epage=151801&rft.pages=151801-151801&rft.issn=0031-9007&rft_id=info:doi/&rft_dat=%3Cproquest_pubme%3E69772970%3C/proquest_pubme%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=69772970&rft_id=info:pmid/18999588&rfr_iscdi=true |