Multiplicity distributions at 250 GeV/c, a comparison of fits
Abstract The multiplicity distribution of all charged particles, as well as that of negatives and positives taken separately have been fitted by a number of recently proposed parametrizations. The negative binomial (2 parameters) and Laguerre distribution (3 parameters), in general, give good and ve...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Geraedts, P. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
1989 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer-Verlag 1989 |
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| Übergeordnetes Werk: |
Enthalten in: Zeitschrift für Physik - Springer-Verlag, 1979, 44(1989), 2 vom: Juni, Seite 331-335 |
|---|---|
| Übergeordnetes Werk: |
volume:44 ; year:1989 ; number:2 ; month:06 ; pages:331-335 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF01557338 |
|---|
| Katalog-ID: |
OLC2091906107 |
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| 520 | |a Abstract The multiplicity distribution of all charged particles, as well as that of negatives and positives taken separately have been fitted by a number of recently proposed parametrizations. The negative binomial (2 parameters) and Laguerre distribution (3 parameters), in general, give good and very similar fits, but one of the parameters of the Laguerre distribution remains undetermined by the fit. The Krasznovszky-Wagner distribution (3 parameters) is better than the two first ones for full phase space, but slightly worse in intermediate rapidity intervals. Its disadvantage is the behaviour atn=0. The Branching distribution does not fit at an energy of$$\sqrt s = 22$$ GeV. | ||
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10.1007/BF01557338 doi (DE-627)OLC2091906107 (DE-He213)BF01557338-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Geraedts, P. verfasserin aut Multiplicity distributions at 250 GeV/c, a comparison of fits 1989 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1989 Abstract The multiplicity distribution of all charged particles, as well as that of negatives and positives taken separately have been fitted by a number of recently proposed parametrizations. The negative binomial (2 parameters) and Laguerre distribution (3 parameters), in general, give good and very similar fits, but one of the parameters of the Laguerre distribution remains undetermined by the fit. The Krasznovszky-Wagner distribution (3 parameters) is better than the two first ones for full phase space, but slightly worse in intermediate rapidity intervals. Its disadvantage is the behaviour atn=0. The Branching distribution does not fit at an energy of$$\sqrt s = 22$$ GeV. Field Theory Phase Space Elementary Particle Quantum Field Theory Particle Acceleration Haupt, T. aut Kittel, W. aut Enthalten in Zeitschrift für Physik Springer-Verlag, 1979 44(1989), 2 vom: Juni, Seite 331-335 (DE-627)130618799 (DE-600)795252-1 (DE-576)016125487 0170-9739 nnns volume:44 year:1989 number:2 month:06 pages:331-335 https://doi.org/10.1007/BF01557338 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4126 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4315 GBV_ILN_4319 GBV_ILN_4323 AR 44 1989 2 06 331-335 |
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10.1007/BF01557338 doi (DE-627)OLC2091906107 (DE-He213)BF01557338-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Geraedts, P. verfasserin aut Multiplicity distributions at 250 GeV/c, a comparison of fits 1989 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1989 Abstract The multiplicity distribution of all charged particles, as well as that of negatives and positives taken separately have been fitted by a number of recently proposed parametrizations. The negative binomial (2 parameters) and Laguerre distribution (3 parameters), in general, give good and very similar fits, but one of the parameters of the Laguerre distribution remains undetermined by the fit. The Krasznovszky-Wagner distribution (3 parameters) is better than the two first ones for full phase space, but slightly worse in intermediate rapidity intervals. Its disadvantage is the behaviour atn=0. The Branching distribution does not fit at an energy of$$\sqrt s = 22$$ GeV. Field Theory Phase Space Elementary Particle Quantum Field Theory Particle Acceleration Haupt, T. aut Kittel, W. aut Enthalten in Zeitschrift für Physik Springer-Verlag, 1979 44(1989), 2 vom: Juni, Seite 331-335 (DE-627)130618799 (DE-600)795252-1 (DE-576)016125487 0170-9739 nnns volume:44 year:1989 number:2 month:06 pages:331-335 https://doi.org/10.1007/BF01557338 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4126 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4315 GBV_ILN_4319 GBV_ILN_4323 AR 44 1989 2 06 331-335 |
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10.1007/BF01557338 doi (DE-627)OLC2091906107 (DE-He213)BF01557338-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Geraedts, P. verfasserin aut Multiplicity distributions at 250 GeV/c, a comparison of fits 1989 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1989 Abstract The multiplicity distribution of all charged particles, as well as that of negatives and positives taken separately have been fitted by a number of recently proposed parametrizations. The negative binomial (2 parameters) and Laguerre distribution (3 parameters), in general, give good and very similar fits, but one of the parameters of the Laguerre distribution remains undetermined by the fit. The Krasznovszky-Wagner distribution (3 parameters) is better than the two first ones for full phase space, but slightly worse in intermediate rapidity intervals. Its disadvantage is the behaviour atn=0. The Branching distribution does not fit at an energy of$$\sqrt s = 22$$ GeV. Field Theory Phase Space Elementary Particle Quantum Field Theory Particle Acceleration Haupt, T. aut Kittel, W. aut Enthalten in Zeitschrift für Physik Springer-Verlag, 1979 44(1989), 2 vom: Juni, Seite 331-335 (DE-627)130618799 (DE-600)795252-1 (DE-576)016125487 0170-9739 nnns volume:44 year:1989 number:2 month:06 pages:331-335 https://doi.org/10.1007/BF01557338 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4126 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4315 GBV_ILN_4319 GBV_ILN_4323 AR 44 1989 2 06 331-335 |
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10.1007/BF01557338 doi (DE-627)OLC2091906107 (DE-He213)BF01557338-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Geraedts, P. verfasserin aut Multiplicity distributions at 250 GeV/c, a comparison of fits 1989 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1989 Abstract The multiplicity distribution of all charged particles, as well as that of negatives and positives taken separately have been fitted by a number of recently proposed parametrizations. The negative binomial (2 parameters) and Laguerre distribution (3 parameters), in general, give good and very similar fits, but one of the parameters of the Laguerre distribution remains undetermined by the fit. The Krasznovszky-Wagner distribution (3 parameters) is better than the two first ones for full phase space, but slightly worse in intermediate rapidity intervals. Its disadvantage is the behaviour atn=0. The Branching distribution does not fit at an energy of$$\sqrt s = 22$$ GeV. Field Theory Phase Space Elementary Particle Quantum Field Theory Particle Acceleration Haupt, T. aut Kittel, W. aut Enthalten in Zeitschrift für Physik Springer-Verlag, 1979 44(1989), 2 vom: Juni, Seite 331-335 (DE-627)130618799 (DE-600)795252-1 (DE-576)016125487 0170-9739 nnns volume:44 year:1989 number:2 month:06 pages:331-335 https://doi.org/10.1007/BF01557338 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4126 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4315 GBV_ILN_4319 GBV_ILN_4323 AR 44 1989 2 06 331-335 |
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10.1007/BF01557338 doi (DE-627)OLC2091906107 (DE-He213)BF01557338-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Geraedts, P. verfasserin aut Multiplicity distributions at 250 GeV/c, a comparison of fits 1989 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag 1989 Abstract The multiplicity distribution of all charged particles, as well as that of negatives and positives taken separately have been fitted by a number of recently proposed parametrizations. The negative binomial (2 parameters) and Laguerre distribution (3 parameters), in general, give good and very similar fits, but one of the parameters of the Laguerre distribution remains undetermined by the fit. The Krasznovszky-Wagner distribution (3 parameters) is better than the two first ones for full phase space, but slightly worse in intermediate rapidity intervals. Its disadvantage is the behaviour atn=0. The Branching distribution does not fit at an energy of$$\sqrt s = 22$$ GeV. Field Theory Phase Space Elementary Particle Quantum Field Theory Particle Acceleration Haupt, T. aut Kittel, W. aut Enthalten in Zeitschrift für Physik Springer-Verlag, 1979 44(1989), 2 vom: Juni, Seite 331-335 (DE-627)130618799 (DE-600)795252-1 (DE-576)016125487 0170-9739 nnns volume:44 year:1989 number:2 month:06 pages:331-335 https://doi.org/10.1007/BF01557338 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_20 GBV_ILN_21 GBV_ILN_22 GBV_ILN_30 GBV_ILN_40 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2006 GBV_ILN_2012 GBV_ILN_2014 GBV_ILN_2018 GBV_ILN_2409 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4126 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4315 GBV_ILN_4319 GBV_ILN_4323 AR 44 1989 2 06 331-335 |
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Multiplicity distributions at 250 GeV/c, a comparison of fits |
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Multiplicity distributions at 250 GeV/c, a comparison of fits |
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Geraedts, P. |
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Zeitschrift für Physik |
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Geraedts, P. Haupt, T. Kittel, W. |
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10.1007/BF01557338 |
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530 |
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multiplicity distributions at 250 gev/c, a comparison of fits |
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Multiplicity distributions at 250 GeV/c, a comparison of fits |
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Abstract The multiplicity distribution of all charged particles, as well as that of negatives and positives taken separately have been fitted by a number of recently proposed parametrizations. The negative binomial (2 parameters) and Laguerre distribution (3 parameters), in general, give good and very similar fits, but one of the parameters of the Laguerre distribution remains undetermined by the fit. The Krasznovszky-Wagner distribution (3 parameters) is better than the two first ones for full phase space, but slightly worse in intermediate rapidity intervals. Its disadvantage is the behaviour atn=0. The Branching distribution does not fit at an energy of$$\sqrt s = 22$$ GeV. © Springer-Verlag 1989 |
| abstractGer |
Abstract The multiplicity distribution of all charged particles, as well as that of negatives and positives taken separately have been fitted by a number of recently proposed parametrizations. The negative binomial (2 parameters) and Laguerre distribution (3 parameters), in general, give good and very similar fits, but one of the parameters of the Laguerre distribution remains undetermined by the fit. The Krasznovszky-Wagner distribution (3 parameters) is better than the two first ones for full phase space, but slightly worse in intermediate rapidity intervals. Its disadvantage is the behaviour atn=0. The Branching distribution does not fit at an energy of$$\sqrt s = 22$$ GeV. © Springer-Verlag 1989 |
| abstract_unstemmed |
Abstract The multiplicity distribution of all charged particles, as well as that of negatives and positives taken separately have been fitted by a number of recently proposed parametrizations. The negative binomial (2 parameters) and Laguerre distribution (3 parameters), in general, give good and very similar fits, but one of the parameters of the Laguerre distribution remains undetermined by the fit. The Krasznovszky-Wagner distribution (3 parameters) is better than the two first ones for full phase space, but slightly worse in intermediate rapidity intervals. Its disadvantage is the behaviour atn=0. The Branching distribution does not fit at an energy of$$\sqrt s = 22$$ GeV. © Springer-Verlag 1989 |
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