The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model
Summary The reaction pp→$ pnπ^{+} $ and isobar production in%$pp \to {\mathcal{N}}^{ * + + } (1236)%$ n have been studied at 10 GeV/c. Our data are compared with one-pion exchange models with form factors and with absorption corrections.
Gespeichert in:
| Autor*in: |
Dehne, H. -C. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1968 |
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| Schlagwörter: |
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| Anmerkung: |
© Società Italiana di Fisica 1968 |
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| Übergeordnetes Werk: |
Enthalten in: Il nuovo cimento - [S.l.] : Italian Physical Society, 1965, 53(1968), 1 vom: Jan., Seite 232-241 |
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| Übergeordnetes Werk: |
volume:53 ; year:1968 ; number:1 ; month:01 ; pages:232-241 |
| Links: |
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| DOI / URN: |
10.1007/BF02824936 |
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| Katalog-ID: |
SPR02062350X |
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| 008 | 201006s1968 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1007/BF02824936 |2 doi | |
| 035 | |a (DE-627)SPR02062350X | ||
| 035 | |a (SPR)BF02824936-e | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rakwb | ||
| 041 | |a eng | ||
| 100 | 1 | |a Dehne, H. -C. |e verfasserin |4 aut | |
| 245 | 1 | 4 | |a The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model |
| 264 | 1 | |c 1968 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a © Società Italiana di Fisica 1968 | ||
| 520 | |a Summary The reaction pp→$ pnπ^{+} $ and isobar production in%$pp \to {\mathcal{N}}^{ * + + } (1236)%$ n have been studied at 10 GeV/c. Our data are compared with one-pion exchange models with form factors and with absorption corrections. | ||
| 650 | 4 | |a Absorption Model |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Isobar Production |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Incident Proton Momentum |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Isobar Region |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Additional Form Factor |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Díaz, J. |4 aut | |
| 700 | 1 | |a Strömer, K. |4 aut | |
| 700 | 1 | |a Schmitt, A. |4 aut | |
| 700 | 1 | |a Swanson, W. P. |4 aut | |
| 700 | 1 | |a Borecka, I. |4 aut | |
| 700 | 1 | |a Knies, G. |4 aut | |
| 700 | 1 | |a Wolf, G. |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Il nuovo cimento |d [S.l.] : Italian Physical Society, 1965 |g 53(1968), 1 vom: Jan., Seite 232-241 |w (DE-627)627248667 |w (DE-600)2556213-7 |x 1826-9869 |7 nnns |
| 773 | 1 | 8 | |g volume:53 |g year:1968 |g number:1 |g month:01 |g pages:232-241 |
| 856 | 4 | 0 | |u https://dx.doi.org/10.1007/BF02824936 |z lizenzpflichtig |3 Volltext |
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| 951 | |a AR | ||
| 952 | |d 53 |j 1968 |e 1 |c 01 |h 232-241 | ||
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1968 |
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1968 |
| allfields |
10.1007/BF02824936 doi (DE-627)SPR02062350X (SPR)BF02824936-e DE-627 ger DE-627 rakwb eng Dehne, H. -C. verfasserin aut The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model 1968 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1968 Summary The reaction pp→$ pnπ^{+} $ and isobar production in%$pp \to {\mathcal{N}}^{ * + + } (1236)%$ n have been studied at 10 GeV/c. Our data are compared with one-pion exchange models with form factors and with absorption corrections. Absorption Model (dpeaa)DE-He213 Isobar Production (dpeaa)DE-He213 Incident Proton Momentum (dpeaa)DE-He213 Isobar Region (dpeaa)DE-He213 Additional Form Factor (dpeaa)DE-He213 Díaz, J. aut Strömer, K. aut Schmitt, A. aut Swanson, W. P. aut Borecka, I. aut Knies, G. aut Wolf, G. aut Enthalten in Il nuovo cimento [S.l.] : Italian Physical Society, 1965 53(1968), 1 vom: Jan., Seite 232-241 (DE-627)627248667 (DE-600)2556213-7 1826-9869 nnns volume:53 year:1968 number:1 month:01 pages:232-241 https://dx.doi.org/10.1007/BF02824936 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_65 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_121 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_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_374 GBV_ILN_602 GBV_ILN_647 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_2018 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_2043 GBV_ILN_2044 GBV_ILN_2048 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_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_2158 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2193 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_2808 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_4277 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_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4346 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 GBV_ILN_4753 AR 53 1968 1 01 232-241 |
| spelling |
10.1007/BF02824936 doi (DE-627)SPR02062350X (SPR)BF02824936-e DE-627 ger DE-627 rakwb eng Dehne, H. -C. verfasserin aut The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model 1968 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1968 Summary The reaction pp→$ pnπ^{+} $ and isobar production in%$pp \to {\mathcal{N}}^{ * + + } (1236)%$ n have been studied at 10 GeV/c. Our data are compared with one-pion exchange models with form factors and with absorption corrections. Absorption Model (dpeaa)DE-He213 Isobar Production (dpeaa)DE-He213 Incident Proton Momentum (dpeaa)DE-He213 Isobar Region (dpeaa)DE-He213 Additional Form Factor (dpeaa)DE-He213 Díaz, J. aut Strömer, K. aut Schmitt, A. aut Swanson, W. P. aut Borecka, I. aut Knies, G. aut Wolf, G. aut Enthalten in Il nuovo cimento [S.l.] : Italian Physical Society, 1965 53(1968), 1 vom: Jan., Seite 232-241 (DE-627)627248667 (DE-600)2556213-7 1826-9869 nnns volume:53 year:1968 number:1 month:01 pages:232-241 https://dx.doi.org/10.1007/BF02824936 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_65 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_121 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_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_374 GBV_ILN_602 GBV_ILN_647 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_2018 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_2043 GBV_ILN_2044 GBV_ILN_2048 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_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_2158 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2193 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_2808 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_4277 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_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4346 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 GBV_ILN_4753 AR 53 1968 1 01 232-241 |
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10.1007/BF02824936 doi (DE-627)SPR02062350X (SPR)BF02824936-e DE-627 ger DE-627 rakwb eng Dehne, H. -C. verfasserin aut The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model 1968 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1968 Summary The reaction pp→$ pnπ^{+} $ and isobar production in%$pp \to {\mathcal{N}}^{ * + + } (1236)%$ n have been studied at 10 GeV/c. Our data are compared with one-pion exchange models with form factors and with absorption corrections. Absorption Model (dpeaa)DE-He213 Isobar Production (dpeaa)DE-He213 Incident Proton Momentum (dpeaa)DE-He213 Isobar Region (dpeaa)DE-He213 Additional Form Factor (dpeaa)DE-He213 Díaz, J. aut Strömer, K. aut Schmitt, A. aut Swanson, W. P. aut Borecka, I. aut Knies, G. aut Wolf, G. aut Enthalten in Il nuovo cimento [S.l.] : Italian Physical Society, 1965 53(1968), 1 vom: Jan., Seite 232-241 (DE-627)627248667 (DE-600)2556213-7 1826-9869 nnns volume:53 year:1968 number:1 month:01 pages:232-241 https://dx.doi.org/10.1007/BF02824936 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_65 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_121 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_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_374 GBV_ILN_602 GBV_ILN_647 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_2018 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_2043 GBV_ILN_2044 GBV_ILN_2048 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_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_2158 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2193 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_2808 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_4277 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_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4346 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 GBV_ILN_4753 AR 53 1968 1 01 232-241 |
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10.1007/BF02824936 doi (DE-627)SPR02062350X (SPR)BF02824936-e DE-627 ger DE-627 rakwb eng Dehne, H. -C. verfasserin aut The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model 1968 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1968 Summary The reaction pp→$ pnπ^{+} $ and isobar production in%$pp \to {\mathcal{N}}^{ * + + } (1236)%$ n have been studied at 10 GeV/c. Our data are compared with one-pion exchange models with form factors and with absorption corrections. Absorption Model (dpeaa)DE-He213 Isobar Production (dpeaa)DE-He213 Incident Proton Momentum (dpeaa)DE-He213 Isobar Region (dpeaa)DE-He213 Additional Form Factor (dpeaa)DE-He213 Díaz, J. aut Strömer, K. aut Schmitt, A. aut Swanson, W. P. aut Borecka, I. aut Knies, G. aut Wolf, G. aut Enthalten in Il nuovo cimento [S.l.] : Italian Physical Society, 1965 53(1968), 1 vom: Jan., Seite 232-241 (DE-627)627248667 (DE-600)2556213-7 1826-9869 nnns volume:53 year:1968 number:1 month:01 pages:232-241 https://dx.doi.org/10.1007/BF02824936 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_65 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_121 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_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_374 GBV_ILN_602 GBV_ILN_647 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_2018 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_2043 GBV_ILN_2044 GBV_ILN_2048 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_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_2158 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2193 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_2808 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_4277 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_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4346 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 GBV_ILN_4753 AR 53 1968 1 01 232-241 |
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10.1007/BF02824936 doi (DE-627)SPR02062350X (SPR)BF02824936-e DE-627 ger DE-627 rakwb eng Dehne, H. -C. verfasserin aut The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model 1968 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1968 Summary The reaction pp→$ pnπ^{+} $ and isobar production in%$pp \to {\mathcal{N}}^{ * + + } (1236)%$ n have been studied at 10 GeV/c. Our data are compared with one-pion exchange models with form factors and with absorption corrections. Absorption Model (dpeaa)DE-He213 Isobar Production (dpeaa)DE-He213 Incident Proton Momentum (dpeaa)DE-He213 Isobar Region (dpeaa)DE-He213 Additional Form Factor (dpeaa)DE-He213 Díaz, J. aut Strömer, K. aut Schmitt, A. aut Swanson, W. P. aut Borecka, I. aut Knies, G. aut Wolf, G. aut Enthalten in Il nuovo cimento [S.l.] : Italian Physical Society, 1965 53(1968), 1 vom: Jan., Seite 232-241 (DE-627)627248667 (DE-600)2556213-7 1826-9869 nnns volume:53 year:1968 number:1 month:01 pages:232-241 https://dx.doi.org/10.1007/BF02824936 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_65 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_121 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_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_374 GBV_ILN_602 GBV_ILN_647 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_2018 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_2043 GBV_ILN_2044 GBV_ILN_2048 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_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_2158 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2193 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_2808 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_4277 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_4328 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4346 GBV_ILN_4367 GBV_ILN_4393 GBV_ILN_4700 GBV_ILN_4753 AR 53 1968 1 01 232-241 |
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English |
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Enthalten in Il nuovo cimento 53(1968), 1 vom: Jan., Seite 232-241 volume:53 year:1968 number:1 month:01 pages:232-241 |
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Enthalten in Il nuovo cimento 53(1968), 1 vom: Jan., Seite 232-241 volume:53 year:1968 number:1 month:01 pages:232-241 |
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Absorption Model Isobar Production Incident Proton Momentum Isobar Region Additional Form Factor |
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Il nuovo cimento |
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Dehne, H. -C. @@aut@@ Díaz, J. @@aut@@ Strömer, K. @@aut@@ Schmitt, A. @@aut@@ Swanson, W. P. @@aut@@ Borecka, I. @@aut@@ Knies, G. @@aut@@ Wolf, G. @@aut@@ |
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1968-01-01T00:00:00Z |
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SPR02062350X |
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| author |
Dehne, H. -C. |
| spellingShingle |
Dehne, H. -C. misc Absorption Model misc Isobar Production misc Incident Proton Momentum misc Isobar Region misc Additional Form Factor The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model |
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The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model Absorption Model (dpeaa)DE-He213 Isobar Production (dpeaa)DE-He213 Incident Proton Momentum (dpeaa)DE-He213 Isobar Region (dpeaa)DE-He213 Additional Form Factor (dpeaa)DE-He213 |
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misc Absorption Model misc Isobar Production misc Incident Proton Momentum misc Isobar Region misc Additional Form Factor |
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The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model |
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| title_full |
The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model |
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Dehne, H. -C. |
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Dehne, H. -C. Díaz, J. Strömer, K. Schmitt, A. Swanson, W. P. Borecka, I. Knies, G. Wolf, G. |
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Elektronische Aufsätze |
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Dehne, H. -C. |
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10.1007/BF02824936 |
| title_sort |
reaction pp→pn $ π^{+} $ at 10 gev/c and the ope model |
| title_auth |
The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model |
| abstract |
Summary The reaction pp→$ pnπ^{+} $ and isobar production in%$pp \to {\mathcal{N}}^{ * + + } (1236)%$ n have been studied at 10 GeV/c. Our data are compared with one-pion exchange models with form factors and with absorption corrections. © Società Italiana di Fisica 1968 |
| abstractGer |
Summary The reaction pp→$ pnπ^{+} $ and isobar production in%$pp \to {\mathcal{N}}^{ * + + } (1236)%$ n have been studied at 10 GeV/c. Our data are compared with one-pion exchange models with form factors and with absorption corrections. © Società Italiana di Fisica 1968 |
| abstract_unstemmed |
Summary The reaction pp→$ pnπ^{+} $ and isobar production in%$pp \to {\mathcal{N}}^{ * + + } (1236)%$ n have been studied at 10 GeV/c. Our data are compared with one-pion exchange models with form factors and with absorption corrections. © Società Italiana di Fisica 1968 |
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| title_short |
The reaction pp→pn $ π^{+} $ at 10 GeV/c and the OPE model |
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https://dx.doi.org/10.1007/BF02824936 |
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| author2 |
Díaz, J. Strömer, K. Schmitt, A. Swanson, W. P. Borecka, I. Knies, G. Wolf, G. |
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Díaz, J. Strömer, K. Schmitt, A. Swanson, W. P. Borecka, I. Knies, G. Wolf, G. |
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| doi_str |
10.1007/BF02824936 |
| up_date |
2024-07-03T17:14:45.914Z |
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|
| score |
7.399515 |