Other
Scientific paper
Feb 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002m%26ps...37..257h&link_type=abstract
Meteoritics & Planetary Science, vol. 37, no. 2, pp. 257-267 (2002)
Other
16
Scientific paper
Active capture is a new process for the incorporation of large quantities of heavy noble gases into growing surfaces. Adsorption in the conventional sense involves surface bonding by polarization (Van der Waals forces). What is referred to as "anomalous adsorption" of heavy noble gases involves chemical bonds and can occur when other (more chemically active) species are not available to preempt sites with unfilled bonds. Anomalous adsorption has been observed under conditions of fracture, vacuum deposition and ionizing radiation. Active capture depends upon anomalous adsorption to retain noble gases on a surface long enough to be captured in a growing surface film as it is deposited. The fundamental principle may be the impingement onto the growing film with sufficient energy to liberate surface electrons (work function energy of a few electronvolts) so that they are retained by anomalous adsorption long enough to be entrapped in the growing surface. Trapping efficiencies of ~1% have been observed for Kr and Xe in laboratory experiments, implying a fundamentally new mechanism for the incorporation of heavy noble gases onto surfaces. It may play a role in explaining the large concentrations of planetary noble gases contained in phase-Q.
Hohenberg Charles M.
Meshik Alex
Thonnard N. .
No associations
LandOfFree
Active capture and anomalous adsorption: New mechanisms for the incorporation of heavy noble gases does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Active capture and anomalous adsorption: New mechanisms for the incorporation of heavy noble gases, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Active capture and anomalous adsorption: New mechanisms for the incorporation of heavy noble gases will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1108449