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Solar X-rays as Signature for New Particles

Massive axions of the Kaluza-Klein type, created inside the solar core, can be gravitationally trapped by the Sun itself in orbits inside/outside the Sun, where they accumulate over cosmic times. Their radiative decay can give rise to various solar phenomena, like the celebrated solar coronal heatin...

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Autor principal: Zioutas, K.
Lenguaje:eng
Publicado: 2004
Materias:
Acceso en línea:http://cds.cern.ch/record/741130
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author Zioutas, K.
author_facet Zioutas, K.
author_sort Zioutas, K.
collection CERN
description Massive axions of the Kaluza-Klein type, created inside the solar core, can be gravitationally trapped by the Sun itself in orbits inside/outside the Sun, where they accumulate over cosmic times. Their radiative decay can give rise to various solar phenomena, like the celebrated solar coronal heating, which lacks a conventional explanation since its first observation in 1939. Such and other recent observations favour the existence of a halo of exotic particles near the Sun. X-ray telescopes can provide novel and important information. The underlying solar axion scenario is presented in details in ref.'s [4,15]
id cern-741130
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2004
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spelling cern-7411302023-03-14T20:26:19Zhttp://cds.cern.ch/record/741130engZioutas, K.Solar X-rays as Signature for New ParticlesAstrophysics and AstronomyMassive axions of the Kaluza-Klein type, created inside the solar core, can be gravitationally trapped by the Sun itself in orbits inside/outside the Sun, where they accumulate over cosmic times. Their radiative decay can give rise to various solar phenomena, like the celebrated solar coronal heating, which lacks a conventional explanation since its first observation in 1939. Such and other recent observations favour the existence of a halo of exotic particles near the Sun. X-ray telescopes can provide novel and important information. The underlying solar axion scenario is presented in details in ref.'s [4,15]Massive axions of the Kaluza-Klein type, created inside the solar core, can be gravitationally trapped by the Sun itself in orbits inside/outside the Sun, where they accumulate over cosmic times. Their radiative decay can give rise to various solar phenomena, like the celebrated solar coronal heating, which lacks a conventional explanation since its first observation in 1939. Such and other recent observations favour the existence of a halo of exotic particles near the Sun. X-ray telescopes can provide novel and important information. The underlying solar axion scenario is presented in details in ref.'s [4,15]astro-ph/0406203oai:cds.cern.ch:7411302004
spellingShingle Astrophysics and Astronomy
Zioutas, K.
Solar X-rays as Signature for New Particles
title Solar X-rays as Signature for New Particles
title_full Solar X-rays as Signature for New Particles
title_fullStr Solar X-rays as Signature for New Particles
title_full_unstemmed Solar X-rays as Signature for New Particles
title_short Solar X-rays as Signature for New Particles
title_sort solar x-rays as signature for new particles
topic Astrophysics and Astronomy
url http://cds.cern.ch/record/741130
work_keys_str_mv AT zioutask solarxraysassignaturefornewparticles