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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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Lenguaje: | eng |
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2004
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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 |
record_format | invenio |
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 |