An experiment to search for intermediate mass magnetic monopoles (105-1012 GeV/c2) and for strangelets or nuclearites in the cosmic radiation is exposed at Chacaltaya Laboratory (5230 m a.s.l.) and at Koksil, Himalaya, (4275 m a.s.l.). With the large area of nuclear track detectors (440 m2 at Chacaltaya and 100 m2 at Koksil) and the long time exposure will reach a sensitivity to the flux of SQM about 10-15 cm-2 s-1 sr-1 sr. The results of the analysis, in terms of search for SQM, of large array of detectors at Chacaltaya and exposed for more than 3.5 y are here reported.

Search for SQM in cosmic rays at high altitude laboratories / S. Balestra; S. Cecchini; F. Fabbri; A. Kumar; S. Manzoor; J. McDonald; E. Medinaceli; L. Patrizii; J. Pinfold; V. Popa; I. Qureshi; O. Saavedra; G. Sher; M. Shahzad; M. Spurio; V. Togo; A. Velarde; A. Zanini. - In: JOURNAL OF PHYSICS. CONFERENCE SERIES. - ISSN 1742-6596. - ELETTRONICO. - 39:(2006), pp. 194-196. (Intervento presentato al convegno TAUP 2005: PROCEEDINGS OF THE NINTH INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS tenutosi a Zaragoza, Spain nel 10–14 September 2005).

Search for SQM in cosmic rays at high altitude laboratories.

CECCHINI, STEFANO;MEDINACELI VILLEGAS, EDUARDO;PATRIZII, LAURA;POPA, VLAD;SPURIO, MAURIZIO;
2006

Abstract

An experiment to search for intermediate mass magnetic monopoles (105-1012 GeV/c2) and for strangelets or nuclearites in the cosmic radiation is exposed at Chacaltaya Laboratory (5230 m a.s.l.) and at Koksil, Himalaya, (4275 m a.s.l.). With the large area of nuclear track detectors (440 m2 at Chacaltaya and 100 m2 at Koksil) and the long time exposure will reach a sensitivity to the flux of SQM about 10-15 cm-2 s-1 sr-1 sr. The results of the analysis, in terms of search for SQM, of large array of detectors at Chacaltaya and exposed for more than 3.5 y are here reported.
2006
194
196
Search for SQM in cosmic rays at high altitude laboratories / S. Balestra; S. Cecchini; F. Fabbri; A. Kumar; S. Manzoor; J. McDonald; E. Medinaceli; L. Patrizii; J. Pinfold; V. Popa; I. Qureshi; O. Saavedra; G. Sher; M. Shahzad; M. Spurio; V. Togo; A. Velarde; A. Zanini. - In: JOURNAL OF PHYSICS. CONFERENCE SERIES. - ISSN 1742-6596. - ELETTRONICO. - 39:(2006), pp. 194-196. (Intervento presentato al convegno TAUP 2005: PROCEEDINGS OF THE NINTH INTERNATIONAL CONFERENCE ON TOPICS IN ASTROPARTICLE AND UNDERGROUND PHYSICS tenutosi a Zaragoza, Spain nel 10–14 September 2005).
S. Balestra; S. Cecchini; F. Fabbri; A. Kumar; S. Manzoor; J. McDonald; E. Medinaceli; L. Patrizii; J. Pinfold; V. Popa; I. Qureshi; O. Saavedra; G. Sher; M. Shahzad; M. Spurio; V. Togo; A. Velarde; A. Zanini
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/36843
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