2004
DOI: 10.1021/jp046166u
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Muonium Formation as a Probe of Radiation Chemistry in Sub- and Supercritical Carbon Dioxide

Abstract: Muonium (Mu = μ+e-), which can be considered a light isotope of the H atom, has been observed for the first time in supercritical CO2 (ScCO2). It is unreactive on a time scale of a few microseconds and over a wide density range from well below to well above the CO2 critical density ρc = 0.47 g/cm3. The fraction of muon polarization in muonium, P Mu, does not vary significantly at low densities but changes quickly at the highest densities, approaching zero. This density dependence is reflected in a concomitant … Show more

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Cited by 19 publications
(32 citation statements)
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“…Our results are consistent with the experimental results by Percival group [10] and many experimental results by Brewer and Storchak (e.g. Refs [6] and [14]) as well as predictions in [11,13,14]. However, our preliminary results suggests that there is a significant probability of Mu forming in electronic excited states.…”
Section: Applying Qft To Prethermal Electron Capturesupporting
confidence: 93%
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“…Our results are consistent with the experimental results by Percival group [10] and many experimental results by Brewer and Storchak (e.g. Refs [6] and [14]) as well as predictions in [11,13,14]. However, our preliminary results suggests that there is a significant probability of Mu forming in electronic excited states.…”
Section: Applying Qft To Prethermal Electron Capturesupporting
confidence: 93%
“…One model of Mu formation in condensed media is the spur model [9][10][11][12][13]. A simplified view of spur formation is presented in Fig.…”
Section: Muon Thermalization and The Spur Model Of Muonium Formationmentioning
confidence: 99%
“…The fact that we observe this electron/cation (muon) recombination (or interaction due to polaron generation) rates at the microsecond time scale suggests the existence of electron transfer processes with much slower rate than the ultrafast electron transfer leading to Mu formation, which is more than four orders of magnitude faster (faster than ~10 10 s −1 ) 19,20,23,54 .…”
Section: Resultsmentioning
confidence: 73%
“…The information on chemical dynamics is obtained in two ways; one is by following the sub-ns thermalization process that leads to the formation of different species, such as Mu and diamagnetic species 19,20,54,63 . This is obtained by the analysis of the amplitudes of time-dependent spectra of the different fractions (Fig.…”
Section: Resultsmentioning
confidence: 99%
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