Observation of electron secondaries from $ V^{0} $ decays
Summary Three examples of $ V^{0} $ particles having electron secondaries have been observed in a cloud chamber exposed to a 1.9 GeV $ π^{−} $ beam from the Cosmotron. The experimental evidence is suggestive of the decay scheme, Ke30 → π± + $ e^{∓} $ + v.
Gespeichert in:
| Autor*in: |
Block, M. M. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Italienisch |
| Erschienen: |
1956 |
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| Anmerkung: |
© Società Italiana di Fisica 1956 |
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| Übergeordnetes Werk: |
Enthalten in: Il nuovo cimento - Pisa, 1855, 4(1956), 1 vom: Juli, Seite 46-50 |
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| Übergeordnetes Werk: |
volume:4 ; year:1956 ; number:1 ; month:07 ; pages:46-50 |
| Links: |
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| DOI / URN: |
10.1007/BF02823449 |
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| Katalog-ID: |
SPR037295640 |
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| 008 | 201007s1956 xx |||||o 00| ||ita c | ||
| 024 | 7 | |a 10.1007/BF02823449 |2 doi | |
| 035 | |a (DE-627)SPR037295640 | ||
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| 041 | |a ita | ||
| 100 | 1 | |a Block, M. M. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Observation of electron secondaries from $ V^{0} $ decays |
| 264 | 1 | |c 1956 | |
| 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 1956 | ||
| 520 | |a Summary Three examples of $ V^{0} $ particles having electron secondaries have been observed in a cloud chamber exposed to a 1.9 GeV $ π^{−} $ beam from the Cosmotron. The experimental evidence is suggestive of the decay scheme, Ke30 → π± + $ e^{∓} $ + v. | ||
| 520 | |a Riassunto In una camera a nebbia esposta ad un fascio di mesoni $ π^{−} $ di 1.9 GeV del cosmotrone si sono osservati tre esempi di particelle $ V^{0} $ dotate di elettroni seoondari. I risultati sperimentali suggeriscono Jo schema di decadimento Ke30 → $ π^{±} $ + $ e^{∓} $ + v. | ||
| 700 | 1 | |a Harth, E. M. |4 aut | |
| 700 | 1 | |a Blevins, M. E. |4 aut | |
| 700 | 1 | |a Slaughter, G. G. |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Il nuovo cimento |d Pisa, 1855 |g 4(1956), 1 vom: Juli, Seite 46-50 |w (DE-627)626757762 |w (DE-600)2554784-7 |x 1827-6121 |7 nnns |
| 773 | 1 | 8 | |g volume:4 |g year:1956 |g number:1 |g month:07 |g pages:46-50 |
| 856 | 4 | 0 | |u https://dx.doi.org/10.1007/BF02823449 |z lizenzpflichtig |3 Volltext |
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| 952 | |d 4 |j 1956 |e 1 |c 07 |h 46-50 | ||
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1956 |
| publishDate |
1956 |
| allfields |
10.1007/BF02823449 doi (DE-627)SPR037295640 (SPR)BF02823449-e DE-627 ger DE-627 rakwb ita Block, M. M. verfasserin aut Observation of electron secondaries from $ V^{0} $ decays 1956 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1956 Summary Three examples of $ V^{0} $ particles having electron secondaries have been observed in a cloud chamber exposed to a 1.9 GeV $ π^{−} $ beam from the Cosmotron. The experimental evidence is suggestive of the decay scheme, Ke30 → π± + $ e^{∓} $ + v. Riassunto In una camera a nebbia esposta ad un fascio di mesoni $ π^{−} $ di 1.9 GeV del cosmotrone si sono osservati tre esempi di particelle $ V^{0} $ dotate di elettroni seoondari. I risultati sperimentali suggeriscono Jo schema di decadimento Ke30 → $ π^{±} $ + $ e^{∓} $ + v. Harth, E. M. aut Blevins, M. E. aut Slaughter, G. G. aut Enthalten in Il nuovo cimento Pisa, 1855 4(1956), 1 vom: Juli, Seite 46-50 (DE-627)626757762 (DE-600)2554784-7 1827-6121 nnns volume:4 year:1956 number:1 month:07 pages:46-50 https://dx.doi.org/10.1007/BF02823449 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_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 4 1956 1 07 46-50 |
| spelling |
10.1007/BF02823449 doi (DE-627)SPR037295640 (SPR)BF02823449-e DE-627 ger DE-627 rakwb ita Block, M. M. verfasserin aut Observation of electron secondaries from $ V^{0} $ decays 1956 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1956 Summary Three examples of $ V^{0} $ particles having electron secondaries have been observed in a cloud chamber exposed to a 1.9 GeV $ π^{−} $ beam from the Cosmotron. The experimental evidence is suggestive of the decay scheme, Ke30 → π± + $ e^{∓} $ + v. Riassunto In una camera a nebbia esposta ad un fascio di mesoni $ π^{−} $ di 1.9 GeV del cosmotrone si sono osservati tre esempi di particelle $ V^{0} $ dotate di elettroni seoondari. I risultati sperimentali suggeriscono Jo schema di decadimento Ke30 → $ π^{±} $ + $ e^{∓} $ + v. Harth, E. M. aut Blevins, M. E. aut Slaughter, G. G. aut Enthalten in Il nuovo cimento Pisa, 1855 4(1956), 1 vom: Juli, Seite 46-50 (DE-627)626757762 (DE-600)2554784-7 1827-6121 nnns volume:4 year:1956 number:1 month:07 pages:46-50 https://dx.doi.org/10.1007/BF02823449 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_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 4 1956 1 07 46-50 |
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10.1007/BF02823449 doi (DE-627)SPR037295640 (SPR)BF02823449-e DE-627 ger DE-627 rakwb ita Block, M. M. verfasserin aut Observation of electron secondaries from $ V^{0} $ decays 1956 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1956 Summary Three examples of $ V^{0} $ particles having electron secondaries have been observed in a cloud chamber exposed to a 1.9 GeV $ π^{−} $ beam from the Cosmotron. The experimental evidence is suggestive of the decay scheme, Ke30 → π± + $ e^{∓} $ + v. Riassunto In una camera a nebbia esposta ad un fascio di mesoni $ π^{−} $ di 1.9 GeV del cosmotrone si sono osservati tre esempi di particelle $ V^{0} $ dotate di elettroni seoondari. I risultati sperimentali suggeriscono Jo schema di decadimento Ke30 → $ π^{±} $ + $ e^{∓} $ + v. Harth, E. M. aut Blevins, M. E. aut Slaughter, G. G. aut Enthalten in Il nuovo cimento Pisa, 1855 4(1956), 1 vom: Juli, Seite 46-50 (DE-627)626757762 (DE-600)2554784-7 1827-6121 nnns volume:4 year:1956 number:1 month:07 pages:46-50 https://dx.doi.org/10.1007/BF02823449 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_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 4 1956 1 07 46-50 |
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10.1007/BF02823449 doi (DE-627)SPR037295640 (SPR)BF02823449-e DE-627 ger DE-627 rakwb ita Block, M. M. verfasserin aut Observation of electron secondaries from $ V^{0} $ decays 1956 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1956 Summary Three examples of $ V^{0} $ particles having electron secondaries have been observed in a cloud chamber exposed to a 1.9 GeV $ π^{−} $ beam from the Cosmotron. The experimental evidence is suggestive of the decay scheme, Ke30 → π± + $ e^{∓} $ + v. Riassunto In una camera a nebbia esposta ad un fascio di mesoni $ π^{−} $ di 1.9 GeV del cosmotrone si sono osservati tre esempi di particelle $ V^{0} $ dotate di elettroni seoondari. I risultati sperimentali suggeriscono Jo schema di decadimento Ke30 → $ π^{±} $ + $ e^{∓} $ + v. Harth, E. M. aut Blevins, M. E. aut Slaughter, G. G. aut Enthalten in Il nuovo cimento Pisa, 1855 4(1956), 1 vom: Juli, Seite 46-50 (DE-627)626757762 (DE-600)2554784-7 1827-6121 nnns volume:4 year:1956 number:1 month:07 pages:46-50 https://dx.doi.org/10.1007/BF02823449 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_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 4 1956 1 07 46-50 |
| allfieldsSound |
10.1007/BF02823449 doi (DE-627)SPR037295640 (SPR)BF02823449-e DE-627 ger DE-627 rakwb ita Block, M. M. verfasserin aut Observation of electron secondaries from $ V^{0} $ decays 1956 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier © Società Italiana di Fisica 1956 Summary Three examples of $ V^{0} $ particles having electron secondaries have been observed in a cloud chamber exposed to a 1.9 GeV $ π^{−} $ beam from the Cosmotron. The experimental evidence is suggestive of the decay scheme, Ke30 → π± + $ e^{∓} $ + v. Riassunto In una camera a nebbia esposta ad un fascio di mesoni $ π^{−} $ di 1.9 GeV del cosmotrone si sono osservati tre esempi di particelle $ V^{0} $ dotate di elettroni seoondari. I risultati sperimentali suggeriscono Jo schema di decadimento Ke30 → $ π^{±} $ + $ e^{∓} $ + v. Harth, E. M. aut Blevins, M. E. aut Slaughter, G. G. aut Enthalten in Il nuovo cimento Pisa, 1855 4(1956), 1 vom: Juli, Seite 46-50 (DE-627)626757762 (DE-600)2554784-7 1827-6121 nnns volume:4 year:1956 number:1 month:07 pages:46-50 https://dx.doi.org/10.1007/BF02823449 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_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 4 1956 1 07 46-50 |
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Enthalten in Il nuovo cimento 4(1956), 1 vom: Juli, Seite 46-50 volume:4 year:1956 number:1 month:07 pages:46-50 |
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Enthalten in Il nuovo cimento 4(1956), 1 vom: Juli, Seite 46-50 volume:4 year:1956 number:1 month:07 pages:46-50 |
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Il nuovo cimento |
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Block, M. M. @@aut@@ Harth, E. M. @@aut@@ Blevins, M. E. @@aut@@ Slaughter, G. G. @@aut@@ |
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Block, M. M. Observation of electron secondaries from $ V^{0} $ decays |
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Observation of electron secondaries from $ V^{0} $ decays |
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Observation of electron secondaries from $ V^{0} $ decays |
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Observation of electron secondaries from $ V^{0} $ decays |
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observation of electron secondaries from $ v^{0} $ decays |
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Observation of electron secondaries from $ V^{0} $ decays |
| abstract |
Summary Three examples of $ V^{0} $ particles having electron secondaries have been observed in a cloud chamber exposed to a 1.9 GeV $ π^{−} $ beam from the Cosmotron. The experimental evidence is suggestive of the decay scheme, Ke30 → π± + $ e^{∓} $ + v. Riassunto In una camera a nebbia esposta ad un fascio di mesoni $ π^{−} $ di 1.9 GeV del cosmotrone si sono osservati tre esempi di particelle $ V^{0} $ dotate di elettroni seoondari. I risultati sperimentali suggeriscono Jo schema di decadimento Ke30 → $ π^{±} $ + $ e^{∓} $ + v. © Società Italiana di Fisica 1956 |
| abstractGer |
Summary Three examples of $ V^{0} $ particles having electron secondaries have been observed in a cloud chamber exposed to a 1.9 GeV $ π^{−} $ beam from the Cosmotron. The experimental evidence is suggestive of the decay scheme, Ke30 → π± + $ e^{∓} $ + v. Riassunto In una camera a nebbia esposta ad un fascio di mesoni $ π^{−} $ di 1.9 GeV del cosmotrone si sono osservati tre esempi di particelle $ V^{0} $ dotate di elettroni seoondari. I risultati sperimentali suggeriscono Jo schema di decadimento Ke30 → $ π^{±} $ + $ e^{∓} $ + v. © Società Italiana di Fisica 1956 |
| abstract_unstemmed |
Summary Three examples of $ V^{0} $ particles having electron secondaries have been observed in a cloud chamber exposed to a 1.9 GeV $ π^{−} $ beam from the Cosmotron. The experimental evidence is suggestive of the decay scheme, Ke30 → π± + $ e^{∓} $ + v. Riassunto In una camera a nebbia esposta ad un fascio di mesoni $ π^{−} $ di 1.9 GeV del cosmotrone si sono osservati tre esempi di particelle $ V^{0} $ dotate di elettroni seoondari. I risultati sperimentali suggeriscono Jo schema di decadimento Ke30 → $ π^{±} $ + $ e^{∓} $ + v. © Società Italiana di Fisica 1956 |
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Observation of electron secondaries from $ V^{0} $ decays |
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2024-07-03T22:06:23.424Z |
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