Exclusive $ ωπ^{0} $ production with $ muons^{⋆} $
Abstract Using 160GeV muon scattering data collected with the COMPASS experiment at CERN, the exclusive production of $ ωπ^{0} $ via virtual photons was studied. Selective population of a peak around 1250MeV is observed. Possible contributions from spin-parity $ 1^{-} $ are searched for, inspecting...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Bettinelli, M. [verfasserIn] Dünnweber, W. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2008 |
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| Übergeordnetes Werk: |
Enthalten in: The European physical journal - Berlin : Springer, 1998, 38(2008), 2 vom: 18. Juli, Seite 155-158 |
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| Übergeordnetes Werk: |
volume:38 ; year:2008 ; number:2 ; day:18 ; month:07 ; pages:155-158 |
| Links: |
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| DOI / URN: |
10.1140/epja/i2008-10620-8 |
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| Katalog-ID: |
SPR008271356 |
|---|
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| 520 | |a Abstract Using 160GeV muon scattering data collected with the COMPASS experiment at CERN, the exclusive production of $ ωπ^{0} $ via virtual photons was studied. Selective population of a peak around 1250MeV is observed. Possible contributions from spin-parity $ 1^{-} $ are searched for, inspecting decay angular correlations. In particular, the orientation of the ω decay plane may allow a distinction from the $ 1^{+} $b1(1235) state. Our observation is compared with indications of a $ \rho{^\prime}$(1250) in annihilation and in γp . | ||
| 700 | 1 | |a Dünnweber, W. |e verfasserin |4 aut | |
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10.1140/epja/i2008-10620-8 doi (DE-627)SPR008271356 (SPR)i2008-10620-8-e DE-627 ger DE-627 rakwb eng 530 ASE 33.40 bkl 33.50 bkl Bettinelli, M. verfasserin aut Exclusive $ ωπ^{0} $ production with $ muons^{⋆} $ 2008 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Using 160GeV muon scattering data collected with the COMPASS experiment at CERN, the exclusive production of $ ωπ^{0} $ via virtual photons was studied. Selective population of a peak around 1250MeV is observed. Possible contributions from spin-parity $ 1^{-} $ are searched for, inspecting decay angular correlations. In particular, the orientation of the ω decay plane may allow a distinction from the $ 1^{+} $b1(1235) state. Our observation is compared with indications of a $ \rho{^\prime}$(1250) in annihilation and in γp . Dünnweber, W. verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 38(2008), 2 vom: 18. Juli, Seite 155-158 (DE-627)25372290X (DE-600)1459066-9 1434-601X nnns volume:38 year:2008 number:2 day:18 month:07 pages:155-158 https://dx.doi.org/10.1140/epja/i2008-10620-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_267 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 ASE 33.50 ASE AR 38 2008 2 18 07 155-158 |
| spelling |
10.1140/epja/i2008-10620-8 doi (DE-627)SPR008271356 (SPR)i2008-10620-8-e DE-627 ger DE-627 rakwb eng 530 ASE 33.40 bkl 33.50 bkl Bettinelli, M. verfasserin aut Exclusive $ ωπ^{0} $ production with $ muons^{⋆} $ 2008 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Using 160GeV muon scattering data collected with the COMPASS experiment at CERN, the exclusive production of $ ωπ^{0} $ via virtual photons was studied. Selective population of a peak around 1250MeV is observed. Possible contributions from spin-parity $ 1^{-} $ are searched for, inspecting decay angular correlations. In particular, the orientation of the ω decay plane may allow a distinction from the $ 1^{+} $b1(1235) state. Our observation is compared with indications of a $ \rho{^\prime}$(1250) in annihilation and in γp . Dünnweber, W. verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 38(2008), 2 vom: 18. Juli, Seite 155-158 (DE-627)25372290X (DE-600)1459066-9 1434-601X nnns volume:38 year:2008 number:2 day:18 month:07 pages:155-158 https://dx.doi.org/10.1140/epja/i2008-10620-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_267 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 ASE 33.50 ASE AR 38 2008 2 18 07 155-158 |
| allfields_unstemmed |
10.1140/epja/i2008-10620-8 doi (DE-627)SPR008271356 (SPR)i2008-10620-8-e DE-627 ger DE-627 rakwb eng 530 ASE 33.40 bkl 33.50 bkl Bettinelli, M. verfasserin aut Exclusive $ ωπ^{0} $ production with $ muons^{⋆} $ 2008 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Using 160GeV muon scattering data collected with the COMPASS experiment at CERN, the exclusive production of $ ωπ^{0} $ via virtual photons was studied. Selective population of a peak around 1250MeV is observed. Possible contributions from spin-parity $ 1^{-} $ are searched for, inspecting decay angular correlations. In particular, the orientation of the ω decay plane may allow a distinction from the $ 1^{+} $b1(1235) state. Our observation is compared with indications of a $ \rho{^\prime}$(1250) in annihilation and in γp . Dünnweber, W. verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 38(2008), 2 vom: 18. Juli, Seite 155-158 (DE-627)25372290X (DE-600)1459066-9 1434-601X nnns volume:38 year:2008 number:2 day:18 month:07 pages:155-158 https://dx.doi.org/10.1140/epja/i2008-10620-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_267 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 ASE 33.50 ASE AR 38 2008 2 18 07 155-158 |
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10.1140/epja/i2008-10620-8 doi (DE-627)SPR008271356 (SPR)i2008-10620-8-e DE-627 ger DE-627 rakwb eng 530 ASE 33.40 bkl 33.50 bkl Bettinelli, M. verfasserin aut Exclusive $ ωπ^{0} $ production with $ muons^{⋆} $ 2008 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Using 160GeV muon scattering data collected with the COMPASS experiment at CERN, the exclusive production of $ ωπ^{0} $ via virtual photons was studied. Selective population of a peak around 1250MeV is observed. Possible contributions from spin-parity $ 1^{-} $ are searched for, inspecting decay angular correlations. In particular, the orientation of the ω decay plane may allow a distinction from the $ 1^{+} $b1(1235) state. Our observation is compared with indications of a $ \rho{^\prime}$(1250) in annihilation and in γp . Dünnweber, W. verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 38(2008), 2 vom: 18. Juli, Seite 155-158 (DE-627)25372290X (DE-600)1459066-9 1434-601X nnns volume:38 year:2008 number:2 day:18 month:07 pages:155-158 https://dx.doi.org/10.1140/epja/i2008-10620-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_267 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 ASE 33.50 ASE AR 38 2008 2 18 07 155-158 |
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10.1140/epja/i2008-10620-8 doi (DE-627)SPR008271356 (SPR)i2008-10620-8-e DE-627 ger DE-627 rakwb eng 530 ASE 33.40 bkl 33.50 bkl Bettinelli, M. verfasserin aut Exclusive $ ωπ^{0} $ production with $ muons^{⋆} $ 2008 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Using 160GeV muon scattering data collected with the COMPASS experiment at CERN, the exclusive production of $ ωπ^{0} $ via virtual photons was studied. Selective population of a peak around 1250MeV is observed. Possible contributions from spin-parity $ 1^{-} $ are searched for, inspecting decay angular correlations. In particular, the orientation of the ω decay plane may allow a distinction from the $ 1^{+} $b1(1235) state. Our observation is compared with indications of a $ \rho{^\prime}$(1250) in annihilation and in γp . Dünnweber, W. verfasserin aut Enthalten in The European physical journal Berlin : Springer, 1998 38(2008), 2 vom: 18. Juli, Seite 155-158 (DE-627)25372290X (DE-600)1459066-9 1434-601X nnns volume:38 year:2008 number:2 day:18 month:07 pages:155-158 https://dx.doi.org/10.1140/epja/i2008-10620-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_267 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4012 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 ASE 33.50 ASE AR 38 2008 2 18 07 155-158 |
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530 ASE 33.40 bkl 33.50 bkl Exclusive $ ωπ^{0} $ production with $ muons^{⋆} $ |
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exclusive $ ωπ^{0} $ production with $ muons^{⋆} $ |
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Exclusive $ ωπ^{0} $ production with $ muons^{⋆} $ |
| abstract |
Abstract Using 160GeV muon scattering data collected with the COMPASS experiment at CERN, the exclusive production of $ ωπ^{0} $ via virtual photons was studied. Selective population of a peak around 1250MeV is observed. Possible contributions from spin-parity $ 1^{-} $ are searched for, inspecting decay angular correlations. In particular, the orientation of the ω decay plane may allow a distinction from the $ 1^{+} $b1(1235) state. Our observation is compared with indications of a $ \rho{^\prime}$(1250) in annihilation and in γp . |
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Abstract Using 160GeV muon scattering data collected with the COMPASS experiment at CERN, the exclusive production of $ ωπ^{0} $ via virtual photons was studied. Selective population of a peak around 1250MeV is observed. Possible contributions from spin-parity $ 1^{-} $ are searched for, inspecting decay angular correlations. In particular, the orientation of the ω decay plane may allow a distinction from the $ 1^{+} $b1(1235) state. Our observation is compared with indications of a $ \rho{^\prime}$(1250) in annihilation and in γp . |
| abstract_unstemmed |
Abstract Using 160GeV muon scattering data collected with the COMPASS experiment at CERN, the exclusive production of $ ωπ^{0} $ via virtual photons was studied. Selective population of a peak around 1250MeV is observed. Possible contributions from spin-parity $ 1^{-} $ are searched for, inspecting decay angular correlations. In particular, the orientation of the ω decay plane may allow a distinction from the $ 1^{+} $b1(1235) state. Our observation is compared with indications of a $ \rho{^\prime}$(1250) in annihilation and in γp . |
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Selective population of a peak around 1250MeV is observed. Possible contributions from spin-parity $ 1^{-} $ are searched for, inspecting decay angular correlations. In particular, the orientation of the ω decay plane may allow a distinction from the $ 1^{+} $b1(1235) state. Our observation is compared with indications of a $ \rho{^\prime}$(1250) in annihilation and in γp .</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Dünnweber, W.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">The European physical journal</subfield><subfield code="d">Berlin : Springer, 1998</subfield><subfield code="g">38(2008), 2 vom: 18. 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