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Collisional quenching of O(1D) by O(3P)

dc.contributor.authorYee, Jeng-Hwaen_US
dc.contributor.authorGuberman, Steven L.en_US
dc.contributor.authorDalgarno, A.en_US
dc.date.accessioned2006-04-10T13:45:33Z
dc.date.available2006-04-10T13:45:33Z
dc.date.issued1990-05en_US
dc.identifier.citationYee, J. H., Guberman, Steven L., Dalgarno, A. (1990/05)."Collisional quenching of O(1D) by O(3P)." Planetary and Space Science 38(5): 647-652. <http://hdl.handle.net/2027.42/28609>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6V6T-46YSKVX-6T/2/fc09b3198def427ac5891b28f2b00e25en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/28609
dc.description.abstractMetastable O(1D) atoms may be quenched in collisions with ground state O(3P) atoms by transitions in the avoided crossing regions of the three lowest 3[Pi]g states of O2 of which the lowest separates to O(3P) + O(3P) and the two upper to O(3P) + O(1D). Quantal calculations of the adiabatic potential energy curves of the 3[Pi]g , states are carried out with particular attention to an avoided crossing region in the lowest two states around a nuclear separation of 3.2a0. Diabatic potential matrix elements are constructed from the adiabatic curves by imposing the requirement that they be smooth everywhere. A multistate diabatic formulation is used to describe the scattering and the cross-sections for the collision-induced quenching of O(1D) atoms are calculated.The rate coefficient for the quenching of O(1D) atoms by O(3P) atoms is obtained as a function of temperature. At 1000 K, the value is 1.0 x 10-11 cm3 s-1, accurate probably to a factor of two. The theoretical rate coefficient is consistent with the empirical value inferred from upper atmosphere data.en_US
dc.format.extent435715 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleCollisional quenching of O(1D) by O(3P)en_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumSpace Physics Research Laboratory, University of Michigan, Ann Arbor, MI 48109, U.S.A.en_US
dc.contributor.affiliationotherInstitute for Scientific Research, 33 Bedford Street, Lexington, MA 02173, U.S.A.en_US
dc.contributor.affiliationotherHarvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, U.S.A.en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/28609/1/0000418.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0032-0633(90)90071-Wen_US
dc.identifier.sourcePlanetary and Space Scienceen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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