Microscopic black hole detection in UHECR: the double bang signature

Detalhes bibliográficos
Autor(a) principal: Cardoso, V.
Data de Publicação: 2005
Outros Autores: Espírito Santo, M. C., Paulos, M., Pimenta, M., Tomé, B.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)
Texto Completo: http://hdl.handle.net/10316/4426
https://doi.org/10.1016/j.astropartphys.2004.09.006
Resumo: According to recent conjectures on the existence of large extra dimensions in our universe, black holes could be produced during the interaction of Ultra High Energy Cosmic Rays with the atmosphere. However, and so far, the proposed signatures are based on statistical effects, not allowing identification on an event by event basis, and may lead to large uncertainties. In this note, events with a double bang topology, where the production and instantaneous decay of a microscopic black hole (first bang) is followed, at a measurable distance, by the decay of an energetic tau lepton (second bang) are proposed as an almost background free signature. The characteristics of these events and the capability of large cosmic ray experiments to detect them are discussed.
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spelling Microscopic black hole detection in UHECR: the double bang signatureExtra-dimensionsBlack holesNeutrinosDouble bangAccording to recent conjectures on the existence of large extra dimensions in our universe, black holes could be produced during the interaction of Ultra High Energy Cosmic Rays with the atmosphere. However, and so far, the proposed signatures are based on statistical effects, not allowing identification on an event by event basis, and may lead to large uncertainties. In this note, events with a double bang topology, where the production and instantaneous decay of a microscopic black hole (first bang) is followed, at a measurable distance, by the decay of an energetic tau lepton (second bang) are proposed as an almost background free signature. The characteristics of these events and the capability of large cosmic ray experiments to detect them are discussed.http://www.sciencedirect.com/science/article/B6TJ1-4DNR97P-1/1/5b79ccee7f6ee463fd956af353c27ee92005info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleaplication/PDFhttp://hdl.handle.net/10316/4426http://hdl.handle.net/10316/4426https://doi.org/10.1016/j.astropartphys.2004.09.006engAstroparticle Physics. 22:5-6 (2005) 399-407Cardoso, V.Espírito Santo, M. C.Paulos, M.Pimenta, M.Tomé, B.info:eu-repo/semantics/openAccessreponame:Repositório Científico de Acesso Aberto de Portugal (Repositórios Cientìficos)instname:Agência para a Sociedade do Conhecimento (UMIC) - FCT - Sociedade da Informaçãoinstacron:RCAAP2020-11-06T16:48:46ZPortal AgregadorONG
dc.title.none.fl_str_mv Microscopic black hole detection in UHECR: the double bang signature
title Microscopic black hole detection in UHECR: the double bang signature
spellingShingle Microscopic black hole detection in UHECR: the double bang signature
Cardoso, V.
Extra-dimensions
Black holes
Neutrinos
Double bang
title_short Microscopic black hole detection in UHECR: the double bang signature
title_full Microscopic black hole detection in UHECR: the double bang signature
title_fullStr Microscopic black hole detection in UHECR: the double bang signature
title_full_unstemmed Microscopic black hole detection in UHECR: the double bang signature
title_sort Microscopic black hole detection in UHECR: the double bang signature
author Cardoso, V.
author_facet Cardoso, V.
Espírito Santo, M. C.
Paulos, M.
Pimenta, M.
Tomé, B.
author_role author
author2 Espírito Santo, M. C.
Paulos, M.
Pimenta, M.
Tomé, B.
author2_role author
author
author
author
dc.contributor.author.fl_str_mv Cardoso, V.
Espírito Santo, M. C.
Paulos, M.
Pimenta, M.
Tomé, B.
dc.subject.por.fl_str_mv Extra-dimensions
Black holes
Neutrinos
Double bang
topic Extra-dimensions
Black holes
Neutrinos
Double bang
description According to recent conjectures on the existence of large extra dimensions in our universe, black holes could be produced during the interaction of Ultra High Energy Cosmic Rays with the atmosphere. However, and so far, the proposed signatures are based on statistical effects, not allowing identification on an event by event basis, and may lead to large uncertainties. In this note, events with a double bang topology, where the production and instantaneous decay of a microscopic black hole (first bang) is followed, at a measurable distance, by the decay of an energetic tau lepton (second bang) are proposed as an almost background free signature. The characteristics of these events and the capability of large cosmic ray experiments to detect them are discussed.
publishDate 2005
dc.date.none.fl_str_mv 2005
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dc.identifier.uri.fl_str_mv http://hdl.handle.net/10316/4426
http://hdl.handle.net/10316/4426
https://doi.org/10.1016/j.astropartphys.2004.09.006
url http://hdl.handle.net/10316/4426
https://doi.org/10.1016/j.astropartphys.2004.09.006
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Astroparticle Physics. 22:5-6 (2005) 399-407
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