Total cross-sections and the Regge-pole model
Summary It is shown that all the available high-energy data on total cross-sections can be incorporated within the framework of theSU3 Regge-pole model. The model consists of the exchange of tensor- and vector-meson nonets in addition to the Pomeranchuk trajectory. Some of the points which emerge fr...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Ganguli, S. N. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1973 |
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| Anmerkung: |
© Società Italiana di Fisica 1973 |
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| Übergeordnetes Werk: |
Enthalten in: Il nuovo cimento - [S.l.] : Italian Physical Society, 1965, 17(1973), 1 vom: Sept., Seite 232-244 |
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| Übergeordnetes Werk: |
volume:17 ; year:1973 ; number:1 ; month:09 ; pages:232-244 |
| Links: |
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| DOI / URN: |
10.1007/BF02790296 |
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| Katalog-ID: |
SPR037380494 |
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| 008 | 201007s1973 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1007/BF02790296 |2 doi | |
| 035 | |a (DE-627)SPR037380494 | ||
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| 041 | |a eng | ||
| 100 | 1 | |a Ganguli, S. N. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Total cross-sections and the Regge-pole model |
| 264 | 1 | |c 1973 | |
| 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 1973 | ||
| 520 | |a Summary It is shown that all the available high-energy data on total cross-sections can be incorporated within the framework of theSU3 Regge-pole model. The model consists of the exchange of tensor- and vector-meson nonets in addition to the Pomeranchuk trajectory. Some of the points which emerge from our analysis are: i) the total cross-sections of $ π^{+} $p, $ K^{+} $p, ppeventually increase towards their respective asymptotic limits, while those of their counterparts $ π^{−} $p, $ K^{−} $p and%$\bar pp%$ decrease towards their limiting values; and ii) the ratios Re/Im of the forward amplitudes are in general predicted to be large in magnitude compared to the available data. | ||
| 700 | 1 | |a Sarma, K. V. L. |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Il nuovo cimento |d [S.l.] : Italian Physical Society, 1965 |g 17(1973), 1 vom: Sept., Seite 232-244 |w (DE-627)627248667 |w (DE-600)2556213-7 |x 1826-9869 |7 nnns |
| 773 | 1 | 8 | |g volume:17 |g year:1973 |g number:1 |g month:09 |g pages:232-244 |
| 856 | 4 | 0 | |u https://dx.doi.org/10.1007/BF02790296 |z lizenzpflichtig |3 Volltext |
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| 952 | |d 17 |j 1973 |e 1 |c 09 |h 232-244 | ||
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1973 |
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1973 |
| allfields |
10.1007/BF02790296 doi (DE-627)SPR037380494 (SPR)BF02790296-e DE-627 ger DE-627 rakwb eng Ganguli, S. N. verfasserin aut Total cross-sections and the Regge-pole model 1973 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1973 Summary It is shown that all the available high-energy data on total cross-sections can be incorporated within the framework of theSU3 Regge-pole model. The model consists of the exchange of tensor- and vector-meson nonets in addition to the Pomeranchuk trajectory. Some of the points which emerge from our analysis are: i) the total cross-sections of $ π^{+} $p, $ K^{+} $p, ppeventually increase towards their respective asymptotic limits, while those of their counterparts $ π^{−} $p, $ K^{−} $p and%$\bar pp%$ decrease towards their limiting values; and ii) the ratios Re/Im of the forward amplitudes are in general predicted to be large in magnitude compared to the available data. Sarma, K. V. L. aut Enthalten in Il nuovo cimento [S.l.] : Italian Physical Society, 1965 17(1973), 1 vom: Sept., Seite 232-244 (DE-627)627248667 (DE-600)2556213-7 1826-9869 nnns volume:17 year:1973 number:1 month:09 pages:232-244 https://dx.doi.org/10.1007/BF02790296 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 17 1973 1 09 232-244 |
| spelling |
10.1007/BF02790296 doi (DE-627)SPR037380494 (SPR)BF02790296-e DE-627 ger DE-627 rakwb eng Ganguli, S. N. verfasserin aut Total cross-sections and the Regge-pole model 1973 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1973 Summary It is shown that all the available high-energy data on total cross-sections can be incorporated within the framework of theSU3 Regge-pole model. The model consists of the exchange of tensor- and vector-meson nonets in addition to the Pomeranchuk trajectory. Some of the points which emerge from our analysis are: i) the total cross-sections of $ π^{+} $p, $ K^{+} $p, ppeventually increase towards their respective asymptotic limits, while those of their counterparts $ π^{−} $p, $ K^{−} $p and%$\bar pp%$ decrease towards their limiting values; and ii) the ratios Re/Im of the forward amplitudes are in general predicted to be large in magnitude compared to the available data. Sarma, K. V. L. aut Enthalten in Il nuovo cimento [S.l.] : Italian Physical Society, 1965 17(1973), 1 vom: Sept., Seite 232-244 (DE-627)627248667 (DE-600)2556213-7 1826-9869 nnns volume:17 year:1973 number:1 month:09 pages:232-244 https://dx.doi.org/10.1007/BF02790296 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 17 1973 1 09 232-244 |
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10.1007/BF02790296 doi (DE-627)SPR037380494 (SPR)BF02790296-e DE-627 ger DE-627 rakwb eng Ganguli, S. N. verfasserin aut Total cross-sections and the Regge-pole model 1973 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1973 Summary It is shown that all the available high-energy data on total cross-sections can be incorporated within the framework of theSU3 Regge-pole model. The model consists of the exchange of tensor- and vector-meson nonets in addition to the Pomeranchuk trajectory. Some of the points which emerge from our analysis are: i) the total cross-sections of $ π^{+} $p, $ K^{+} $p, ppeventually increase towards their respective asymptotic limits, while those of their counterparts $ π^{−} $p, $ K^{−} $p and%$\bar pp%$ decrease towards their limiting values; and ii) the ratios Re/Im of the forward amplitudes are in general predicted to be large in magnitude compared to the available data. Sarma, K. V. L. aut Enthalten in Il nuovo cimento [S.l.] : Italian Physical Society, 1965 17(1973), 1 vom: Sept., Seite 232-244 (DE-627)627248667 (DE-600)2556213-7 1826-9869 nnns volume:17 year:1973 number:1 month:09 pages:232-244 https://dx.doi.org/10.1007/BF02790296 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 17 1973 1 09 232-244 |
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10.1007/BF02790296 doi (DE-627)SPR037380494 (SPR)BF02790296-e DE-627 ger DE-627 rakwb eng Ganguli, S. N. verfasserin aut Total cross-sections and the Regge-pole model 1973 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1973 Summary It is shown that all the available high-energy data on total cross-sections can be incorporated within the framework of theSU3 Regge-pole model. The model consists of the exchange of tensor- and vector-meson nonets in addition to the Pomeranchuk trajectory. Some of the points which emerge from our analysis are: i) the total cross-sections of $ π^{+} $p, $ K^{+} $p, ppeventually increase towards their respective asymptotic limits, while those of their counterparts $ π^{−} $p, $ K^{−} $p and%$\bar pp%$ decrease towards their limiting values; and ii) the ratios Re/Im of the forward amplitudes are in general predicted to be large in magnitude compared to the available data. Sarma, K. V. L. aut Enthalten in Il nuovo cimento [S.l.] : Italian Physical Society, 1965 17(1973), 1 vom: Sept., Seite 232-244 (DE-627)627248667 (DE-600)2556213-7 1826-9869 nnns volume:17 year:1973 number:1 month:09 pages:232-244 https://dx.doi.org/10.1007/BF02790296 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 17 1973 1 09 232-244 |
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10.1007/BF02790296 doi (DE-627)SPR037380494 (SPR)BF02790296-e DE-627 ger DE-627 rakwb eng Ganguli, S. N. verfasserin aut Total cross-sections and the Regge-pole model 1973 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1973 Summary It is shown that all the available high-energy data on total cross-sections can be incorporated within the framework of theSU3 Regge-pole model. The model consists of the exchange of tensor- and vector-meson nonets in addition to the Pomeranchuk trajectory. Some of the points which emerge from our analysis are: i) the total cross-sections of $ π^{+} $p, $ K^{+} $p, ppeventually increase towards their respective asymptotic limits, while those of their counterparts $ π^{−} $p, $ K^{−} $p and%$\bar pp%$ decrease towards their limiting values; and ii) the ratios Re/Im of the forward amplitudes are in general predicted to be large in magnitude compared to the available data. Sarma, K. V. L. aut Enthalten in Il nuovo cimento [S.l.] : Italian Physical Society, 1965 17(1973), 1 vom: Sept., Seite 232-244 (DE-627)627248667 (DE-600)2556213-7 1826-9869 nnns volume:17 year:1973 number:1 month:09 pages:232-244 https://dx.doi.org/10.1007/BF02790296 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 17 1973 1 09 232-244 |
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Enthalten in Il nuovo cimento 17(1973), 1 vom: Sept., Seite 232-244 volume:17 year:1973 number:1 month:09 pages:232-244 |
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Ganguli, S. N. |
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Ganguli, S. N. Total cross-sections and the Regge-pole model |
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total cross-sections and the regge-pole model |
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Total cross-sections and the Regge-pole model |
| abstract |
Summary It is shown that all the available high-energy data on total cross-sections can be incorporated within the framework of theSU3 Regge-pole model. The model consists of the exchange of tensor- and vector-meson nonets in addition to the Pomeranchuk trajectory. Some of the points which emerge from our analysis are: i) the total cross-sections of $ π^{+} $p, $ K^{+} $p, ppeventually increase towards their respective asymptotic limits, while those of their counterparts $ π^{−} $p, $ K^{−} $p and%$\bar pp%$ decrease towards their limiting values; and ii) the ratios Re/Im of the forward amplitudes are in general predicted to be large in magnitude compared to the available data. © Società Italiana di Fisica 1973 |
| abstractGer |
Summary It is shown that all the available high-energy data on total cross-sections can be incorporated within the framework of theSU3 Regge-pole model. The model consists of the exchange of tensor- and vector-meson nonets in addition to the Pomeranchuk trajectory. Some of the points which emerge from our analysis are: i) the total cross-sections of $ π^{+} $p, $ K^{+} $p, ppeventually increase towards their respective asymptotic limits, while those of their counterparts $ π^{−} $p, $ K^{−} $p and%$\bar pp%$ decrease towards their limiting values; and ii) the ratios Re/Im of the forward amplitudes are in general predicted to be large in magnitude compared to the available data. © Società Italiana di Fisica 1973 |
| abstract_unstemmed |
Summary It is shown that all the available high-energy data on total cross-sections can be incorporated within the framework of theSU3 Regge-pole model. The model consists of the exchange of tensor- and vector-meson nonets in addition to the Pomeranchuk trajectory. Some of the points which emerge from our analysis are: i) the total cross-sections of $ π^{+} $p, $ K^{+} $p, ppeventually increase towards their respective asymptotic limits, while those of their counterparts $ π^{−} $p, $ K^{−} $p and%$\bar pp%$ decrease towards their limiting values; and ii) the ratios Re/Im of the forward amplitudes are in general predicted to be large in magnitude compared to the available data. © Società Italiana di Fisica 1973 |
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2024-07-03T22:30:52.524Z |
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N.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Total cross-sections and the Regge-pole model</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">1973</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Società Italiana di Fisica 1973</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Summary It is shown that all the available high-energy data on total cross-sections can be incorporated within the framework of theSU3 Regge-pole model. 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