Correlations and Charge Composition of UHECR without Knowledge of Galactic Magnetic Field

We develop a formalism which allows to study correlations of charged UHECR with potential sources without using any Galactic Magnetic Field (GMF) model. The method is free of subjective chose of parameters on which the significance of correlations depends strongly. We show that correlations of the A...

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Detalles Bibliográficos
Autores principales: Tinyakov, Peter, Tkachev, Igor
Lenguaje:eng
Publicado: 2003
Materias:
Astrophysics and Astronomy
Acceso en línea:http://cds.cern.ch/record/617594
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author Tinyakov, Peter
Tkachev, Igor
author_facet Tinyakov, Peter
Tkachev, Igor
author_sort Tinyakov, Peter
collection CERN
description We develop a formalism which allows to study correlations of charged UHECR with potential sources without using any Galactic Magnetic Field (GMF) model. The method is free of subjective chose of parameters on which the significance of correlations depends strongly. We show that correlations of the AGASA dataset with BL Lacs (found previously after reconstruction of particle trajectories in a specific GMF) are present intrinsically and can be detected without reference to a particular model of magnetic field.
id cern-617594
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2003
record_format invenio
spelling cern-6175942023-03-20T10:06:43Zhttp://cds.cern.ch/record/617594engTinyakov, PeterTkachev, IgorCorrelations and Charge Composition of UHECR without Knowledge of Galactic Magnetic FieldAstrophysics and AstronomyWe develop a formalism which allows to study correlations of charged UHECR with potential sources without using any Galactic Magnetic Field (GMF) model. The method is free of subjective chose of parameters on which the significance of correlations depends strongly. We show that correlations of the AGASA dataset with BL Lacs (found previously after reconstruction of particle trajectories in a specific GMF) are present intrinsically and can be detected without reference to a particular model of magnetic field.We develop a formalism which allows to study correlations of charged UHECR with potential sources without using any Galactic Magnetic Field (GMF) model. The method is free of subjective chose of parameters on which the significance of correlations depends strongly. We show that correlations of the AGASA dataset with BL Lacs (found previously after reconstruction of particle trajectories in a specific GMF) are present intrinsically and can be detected without reference to a particular model of magnetic field.astro-ph/0305363oai:cds.cern.ch:6175942003-05-20
spellingShingle Astrophysics and Astronomy
Tinyakov, Peter
Tkachev, Igor
Correlations and Charge Composition of UHECR without Knowledge of Galactic Magnetic Field
title Correlations and Charge Composition of UHECR without Knowledge of Galactic Magnetic Field
title_full Correlations and Charge Composition of UHECR without Knowledge of Galactic Magnetic Field
title_fullStr Correlations and Charge Composition of UHECR without Knowledge of Galactic Magnetic Field
title_full_unstemmed Correlations and Charge Composition of UHECR without Knowledge of Galactic Magnetic Field
title_short Correlations and Charge Composition of UHECR without Knowledge of Galactic Magnetic Field
title_sort correlations and charge composition of uhecr without knowledge of galactic magnetic field
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/617594
work_keys_str_mv AT tinyakovpeter correlationsandchargecompositionofuhecrwithoutknowledgeofgalacticmagneticfield
AT tkachevigor correlationsandchargecompositionofuhecrwithoutknowledgeofgalacticmagneticfield

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