The DAEMONs (DArk Electric Matter Objects) have been suggested as a possible exotic component in cosmic rays able to contribute to the Dark Matter; they belong to the wide class of the Elementary Black Holes (EBH)deeply discussed in literature. A preliminary possible DAEMONs direct detection -- at $\simeq$ 3σ C.L. -- was originally suggested by the sea-level St. Petersburg experiment (SPb); a DAEMONs flux: (1.0±0.3) DAEMONs/(days m² sr) can be derived. Here the results obtained by the sea-level NEMESIS experiment, which has exploited the same detection approach, are presented; they restrict the DAEMONs flux to be less than 0.32 DAEMONs/(days m² sr) at 90% C.L..

Bernabei, R., Belli, P., Cappella, F., Cerulli, R., D'Angelo, A., Emiliani, F., et al. (2012). Search for DAEMONs with NEMESIS. MODERN PHYSICS LETTERS A, 27(8), 1250031-1-1250031-17 [10.1142/S0217732312500319].

Search for DAEMONs with NEMESIS

BERNABEI, RITA;
2012-01-01

Abstract

The DAEMONs (DArk Electric Matter Objects) have been suggested as a possible exotic component in cosmic rays able to contribute to the Dark Matter; they belong to the wide class of the Elementary Black Holes (EBH)deeply discussed in literature. A preliminary possible DAEMONs direct detection -- at $\simeq$ 3σ C.L. -- was originally suggested by the sea-level St. Petersburg experiment (SPb); a DAEMONs flux: (1.0±0.3) DAEMONs/(days m² sr) can be derived. Here the results obtained by the sea-level NEMESIS experiment, which has exploited the same detection approach, are presented; they restrict the DAEMONs flux to be less than 0.32 DAEMONs/(days m² sr) at 90% C.L..
2012
Pubblicato
Rilevanza internazionale
Articolo
Sì, ma tipo non specificato
Settore FIS/04 - FISICA NUCLEARE E SUBNUCLEARE
Settore FIS/01 - FISICA SPERIMENTALE
English
Con Impact Factor ISI
Dark Matter,DAEMONs,delayed coincidence technique,astroparticle physics
Bernabei, R., Belli, P., Cappella, F., Cerulli, R., D'Angelo, A., Emiliani, F., et al. (2012). Search for DAEMONs with NEMESIS. MODERN PHYSICS LETTERS A, 27(8), 1250031-1-1250031-17 [10.1142/S0217732312500319].
Bernabei, R; Belli, P; Cappella, F; Cerulli, R; D'Angelo, A; Emiliani, F; Incicchitti, A
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2108/61510
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