1982
DOI: 10.1016/0550-3213(82)90271-1
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A search for anomalous hydrogen in enriched D2O, using a time-of-flight spectrometer

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Cited by 165 publications
(109 citation statements)
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“…There are strict constraints on n 1 /n H based on hydrogen anomalous isotope searches in sea water. These constraints set an upper limit for n 1 /n H at 10 −29 − 10 −28 [54]. However, it has been speculated that due to the heaviness of the millicharged particles, anomalous isotopes might concentrate at larger depths inside the oceans.…”
Section: B Anomalous Isotope Constraintsmentioning
confidence: 99%
“…There are strict constraints on n 1 /n H based on hydrogen anomalous isotope searches in sea water. These constraints set an upper limit for n 1 /n H at 10 −29 − 10 −28 [54]. However, it has been speculated that due to the heaviness of the millicharged particles, anomalous isotopes might concentrate at larger depths inside the oceans.…”
Section: B Anomalous Isotope Constraintsmentioning
confidence: 99%
“…Although it is convenient to present these limits in one figure, we caution that there is only a weak relationship between the limits set by these searches, which are based on very different sets of assumptions. For example, by far the most stringent limits have been set on +1e charged, hydrogen-like strangelets [6]. However, the non-existence of +1e charged strangelets does not automatically rule out the existence of strangelets of higher charges.…”
Section: Past Searchesmentioning
confidence: 99%
“…Smith et al [6] took advantage of the existing industrial scale heavy-water enrichment facility. Starting from 1.2×10 8 l of natural water, 2×10 -5 l of D 2 O sample was extracted with multi-step electrolysis, first in a factory and then in the laboratory.…”
Section: Mass Spectrometry (Ms) 2 Hmentioning
confidence: 99%
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“…Both direct searches for dark matter and searches for anomalously heavy seawater [52] preclude dark matter from having SU(3) C charge. This places strong limits on the mass of any new stable colored particle; gluinos, for example, can evade cosmological bounds only if their masses are less than about a TeV [39], and seawater tests may lower the allowed mass to ∼ 100 GeV.…”
Section: Jhep01(2011)013mentioning
confidence: 99%