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Limits on Exotic Heavily Ionizing Particles from the Geological Abundance of Fullerenes
The C_{60} molecule exhibits a remarkable stability and inertness that leads to its survival in ancient carbonaceous rocks initially subject to the high temperatures requisite for its formation. Elementary particles having very high electronic stopping powers can similarly form C_{60} and higher ful...
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
1999
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1103/PhysRevLett.83.3097 http://cds.cern.ch/record/379839 |
_version_ | 1780893365835923456 |
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author | Collar, J I Zioutas, Konstantin |
author_facet | Collar, J I Zioutas, Konstantin |
author_sort | Collar, J I |
collection | CERN |
description | The C_{60} molecule exhibits a remarkable stability and inertness that leads to its survival in ancient carbonaceous rocks initially subject to the high temperatures requisite for its formation. Elementary particles having very high electronic stopping powers can similarly form C_{60} and higher fullerenes in their wake. Combined, these two features point at the possibility of using the C_{60} presence (or absence) in selected bulk geological samples as a new type of solid-state nuclear track detector, with applications in astro-particle physics. |
id | cern-379839 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 1999 |
record_format | invenio |
spelling | cern-3798392019-09-30T06:29:59Zdoi:10.1103/PhysRevLett.83.3097http://cds.cern.ch/record/379839engCollar, J IZioutas, KonstantinLimits on Exotic Heavily Ionizing Particles from the Geological Abundance of FullerenesAstrophysics and AstronomyThe C_{60} molecule exhibits a remarkable stability and inertness that leads to its survival in ancient carbonaceous rocks initially subject to the high temperatures requisite for its formation. Elementary particles having very high electronic stopping powers can similarly form C_{60} and higher fullerenes in their wake. Combined, these two features point at the possibility of using the C_{60} presence (or absence) in selected bulk geological samples as a new type of solid-state nuclear track detector, with applications in astro-particle physics.astro-ph/9902310oai:cds.cern.ch:3798391999 |
spellingShingle | Astrophysics and Astronomy Collar, J I Zioutas, Konstantin Limits on Exotic Heavily Ionizing Particles from the Geological Abundance of Fullerenes |
title | Limits on Exotic Heavily Ionizing Particles from the Geological Abundance of Fullerenes |
title_full | Limits on Exotic Heavily Ionizing Particles from the Geological Abundance of Fullerenes |
title_fullStr | Limits on Exotic Heavily Ionizing Particles from the Geological Abundance of Fullerenes |
title_full_unstemmed | Limits on Exotic Heavily Ionizing Particles from the Geological Abundance of Fullerenes |
title_short | Limits on Exotic Heavily Ionizing Particles from the Geological Abundance of Fullerenes |
title_sort | limits on exotic heavily ionizing particles from the geological abundance of fullerenes |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.1103/PhysRevLett.83.3097 http://cds.cern.ch/record/379839 |
work_keys_str_mv | AT collarji limitsonexoticheavilyionizingparticlesfromthegeologicalabundanceoffullerenes AT zioutaskonstantin limitsonexoticheavilyionizingparticlesfromthegeologicalabundanceoffullerenes |