2008
DOI: 10.1140/epjc/s10052-008-0747-7
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Results of the search for strange quark matter and Q-balls with the SLIM experiment

Abstract: The SLIM experiment at the Chacaltaya high altitude laboratory was sensitive to nuclearites and Q-balls, which could be present in the cosmic radiation as possible Dark Matter components. It was sensitive also to strangelets, i.e. small lumps of Strange Quark Matter predicted at such altitudes by various phenomenological models. The analysis of 427 m 2 of Nuclear Track Detectors exposed for 4.22 years showed no candidate event. New upper limits on the flux of downgoing nuclearites and Q-balls at the 90% C.L. w… Show more

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Cited by 45 publications
(34 citation statements)
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“…The sensitivity expected from the analysis of ∼ 159 days of data taken in 2009 is shown in Figure 3. The ANTARES preliminary sensitivity is compared with previous limits from the MACRO [2] and SLIM [3] …”
Section: Resultsmentioning
confidence: 99%
See 1 more Smart Citation
“…The sensitivity expected from the analysis of ∼ 159 days of data taken in 2009 is shown in Figure 3. The ANTARES preliminary sensitivity is compared with previous limits from the MACRO [2] and SLIM [3] …”
Section: Resultsmentioning
confidence: 99%
“…[2], for nuclearites of mass M N > 10 14 GeV, while the SLIM (Search for LIght Monopoles) high altitude experiment in Bolivia has set flux upper limits of 1.3 · 10 −15 cm −2 s −1 sr −1 (90% C.L.) [3], for nuclearite masses M N > 10 10 GeV.…”
Section: Introductionmentioning
confidence: 99%
“…Except for n = 0 cases, the gravitational source in (15) vanishes in the center in the x-y plane. Furthermore, this field configuration has planar symmetry in the z direction.…”
Section: (A)mentioning
confidence: 99%
“…Currently direct searches for neutral Q-balls and for electrically charged Q-balls are in progress in Super-Kamiokande II [14] and in the SLIM Experiment [15], respectively. Furthermore, it has been shown that gravitational waves are emitted during Q-ball formation and could be detected by nextgeneration gravitational detectors [16],…”
Section: Introductionmentioning
confidence: 99%
“…The two telescopes rely on different technologies (scintillators for Explorer, Figure 1. The 90% confidence level upper limit on the flux of nuclearites of experiments with different techniques [7][8][9]12]. The "old" mica limits [12] are dependent from several additional assumptions, respect to the other experiments.…”
Section: The Nautilus and Explorer Gravitational Wave Bar Detectors Umentioning
confidence: 99%