Jet activity versus alignment
Abstract. The hypothesis of the relation between the observed alignment of spots in x-ray films in cosmic ray emulsion experiments and the features of events in which jets prevail at super-high energies is tested. Due to the strong dynamical correlation between jet axis directions and that between t...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Lokhtin, I. P. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2005 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer-Verlag Berlin/Heidelberg 2005 |
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| Übergeordnetes Werk: |
Enthalten in: The European physical journal / C - Springer-Verlag, 1998, 44(2005), 1 vom: Sept., Seite 51-57 |
|---|---|
| Übergeordnetes Werk: |
volume:44 ; year:2005 ; number:1 ; month:09 ; pages:51-57 |
| Links: |
|---|
| DOI / URN: |
10.1140/epjc/s2005-02274-1 |
|---|
| Katalog-ID: |
OLC2069085880 |
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| 520 | |a Abstract. The hypothesis of the relation between the observed alignment of spots in x-ray films in cosmic ray emulsion experiments and the features of events in which jets prevail at super-high energies is tested. Due to the strong dynamical correlation between jet axis directions and that between the momenta of jet particles (almost collinearity), the evaluated degree of alignment is considerably larger than that for randomly selected chaotically located spots in the x-ray film. It appears to be comparable with the experimental data provided that the height of the primary interaction, the collision energy and the total energy of the selected clusters meet certain conditions. The Monte Carlo generator PYTHIA, which basically well describes jet events in hadron-hadron interactions, was used for the analysis. | ||
| 650 | 4 | |a Axis Direction | |
| 650 | 4 | |a Collision Energy | |
| 650 | 4 | |a Particle Acceleration | |
| 650 | 4 | |a Dynamical Correlation | |
| 650 | 4 | |a Primary Interaction | |
| 700 | 1 | |a Managadze, A. K. |4 aut | |
| 700 | 1 | |a Sarycheva, L. I. |4 aut | |
| 700 | 1 | |a Snigirev, A. M. |4 aut | |
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10.1140/epjc/s2005-02274-1 doi (DE-627)OLC2069085880 (DE-He213)s2005-02274-1-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Lokhtin, I. P. verfasserin aut Jet activity versus alignment 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin/Heidelberg 2005 Abstract. The hypothesis of the relation between the observed alignment of spots in x-ray films in cosmic ray emulsion experiments and the features of events in which jets prevail at super-high energies is tested. Due to the strong dynamical correlation between jet axis directions and that between the momenta of jet particles (almost collinearity), the evaluated degree of alignment is considerably larger than that for randomly selected chaotically located spots in the x-ray film. It appears to be comparable with the experimental data provided that the height of the primary interaction, the collision energy and the total energy of the selected clusters meet certain conditions. The Monte Carlo generator PYTHIA, which basically well describes jet events in hadron-hadron interactions, was used for the analysis. Axis Direction Collision Energy Particle Acceleration Dynamical Correlation Primary Interaction Managadze, A. K. aut Sarycheva, L. I. aut Snigirev, A. M. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 44(2005), 1 vom: Sept., Seite 51-57 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:44 year:2005 number:1 month:09 pages:51-57 https://doi.org/10.1140/epjc/s2005-02274-1 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_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2003 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4317 AR 44 2005 1 09 51-57 |
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10.1140/epjc/s2005-02274-1 doi (DE-627)OLC2069085880 (DE-He213)s2005-02274-1-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Lokhtin, I. P. verfasserin aut Jet activity versus alignment 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin/Heidelberg 2005 Abstract. The hypothesis of the relation between the observed alignment of spots in x-ray films in cosmic ray emulsion experiments and the features of events in which jets prevail at super-high energies is tested. Due to the strong dynamical correlation between jet axis directions and that between the momenta of jet particles (almost collinearity), the evaluated degree of alignment is considerably larger than that for randomly selected chaotically located spots in the x-ray film. It appears to be comparable with the experimental data provided that the height of the primary interaction, the collision energy and the total energy of the selected clusters meet certain conditions. The Monte Carlo generator PYTHIA, which basically well describes jet events in hadron-hadron interactions, was used for the analysis. Axis Direction Collision Energy Particle Acceleration Dynamical Correlation Primary Interaction Managadze, A. K. aut Sarycheva, L. I. aut Snigirev, A. M. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 44(2005), 1 vom: Sept., Seite 51-57 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:44 year:2005 number:1 month:09 pages:51-57 https://doi.org/10.1140/epjc/s2005-02274-1 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_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2003 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4317 AR 44 2005 1 09 51-57 |
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10.1140/epjc/s2005-02274-1 doi (DE-627)OLC2069085880 (DE-He213)s2005-02274-1-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Lokhtin, I. P. verfasserin aut Jet activity versus alignment 2005 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer-Verlag Berlin/Heidelberg 2005 Abstract. The hypothesis of the relation between the observed alignment of spots in x-ray films in cosmic ray emulsion experiments and the features of events in which jets prevail at super-high energies is tested. Due to the strong dynamical correlation between jet axis directions and that between the momenta of jet particles (almost collinearity), the evaluated degree of alignment is considerably larger than that for randomly selected chaotically located spots in the x-ray film. It appears to be comparable with the experimental data provided that the height of the primary interaction, the collision energy and the total energy of the selected clusters meet certain conditions. The Monte Carlo generator PYTHIA, which basically well describes jet events in hadron-hadron interactions, was used for the analysis. Axis Direction Collision Energy Particle Acceleration Dynamical Correlation Primary Interaction Managadze, A. K. aut Sarycheva, L. I. aut Snigirev, A. M. aut Enthalten in The European physical journal / C Springer-Verlag, 1998 44(2005), 1 vom: Sept., Seite 51-57 (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:44 year:2005 number:1 month:09 pages:51-57 https://doi.org/10.1140/epjc/s2005-02274-1 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_62 GBV_ILN_70 GBV_ILN_130 GBV_ILN_267 GBV_ILN_2003 GBV_ILN_2018 GBV_ILN_4029 GBV_ILN_4116 GBV_ILN_4277 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4310 GBV_ILN_4317 AR 44 2005 1 09 51-57 |
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Jet activity versus alignment |
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Lokhtin, I. P. |
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The European physical journal / C |
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Lokhtin, I. P. Managadze, A. K. Sarycheva, L. I. Snigirev, A. M. |
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Lokhtin, I. P. |
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10.1140/epjc/s2005-02274-1 |
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530 |
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jet activity versus alignment |
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Jet activity versus alignment |
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Abstract. The hypothesis of the relation between the observed alignment of spots in x-ray films in cosmic ray emulsion experiments and the features of events in which jets prevail at super-high energies is tested. Due to the strong dynamical correlation between jet axis directions and that between the momenta of jet particles (almost collinearity), the evaluated degree of alignment is considerably larger than that for randomly selected chaotically located spots in the x-ray film. It appears to be comparable with the experimental data provided that the height of the primary interaction, the collision energy and the total energy of the selected clusters meet certain conditions. The Monte Carlo generator PYTHIA, which basically well describes jet events in hadron-hadron interactions, was used for the analysis. © Springer-Verlag Berlin/Heidelberg 2005 |
| abstractGer |
Abstract. The hypothesis of the relation between the observed alignment of spots in x-ray films in cosmic ray emulsion experiments and the features of events in which jets prevail at super-high energies is tested. Due to the strong dynamical correlation between jet axis directions and that between the momenta of jet particles (almost collinearity), the evaluated degree of alignment is considerably larger than that for randomly selected chaotically located spots in the x-ray film. It appears to be comparable with the experimental data provided that the height of the primary interaction, the collision energy and the total energy of the selected clusters meet certain conditions. The Monte Carlo generator PYTHIA, which basically well describes jet events in hadron-hadron interactions, was used for the analysis. © Springer-Verlag Berlin/Heidelberg 2005 |
| abstract_unstemmed |
Abstract. The hypothesis of the relation between the observed alignment of spots in x-ray films in cosmic ray emulsion experiments and the features of events in which jets prevail at super-high energies is tested. Due to the strong dynamical correlation between jet axis directions and that between the momenta of jet particles (almost collinearity), the evaluated degree of alignment is considerably larger than that for randomly selected chaotically located spots in the x-ray film. It appears to be comparable with the experimental data provided that the height of the primary interaction, the collision energy and the total energy of the selected clusters meet certain conditions. The Monte Carlo generator PYTHIA, which basically well describes jet events in hadron-hadron interactions, was used for the analysis. © Springer-Verlag Berlin/Heidelberg 2005 |
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Jet activity versus alignment |
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