Collisional quenching of O(1D) by O(3P)
dc.contributor.author | Yee, Jeng-Hwa | en_US |
dc.contributor.author | Guberman, Steven L. | en_US |
dc.contributor.author | Dalgarno, A. | en_US |
dc.date.accessioned | 2006-04-10T13:45:33Z | |
dc.date.available | 2006-04-10T13:45:33Z | |
dc.date.issued | 1990-05 | en_US |
dc.identifier.citation | Yee, 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.uri | http://www.sciencedirect.com/science/article/B6V6T-46YSKVX-6T/2/fc09b3198def427ac5891b28f2b00e25 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/28609 | |
dc.description.abstract | Metastable 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.extent | 435715 bytes | |
dc.format.extent | 3118 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.language.iso | en_US | |
dc.publisher | Elsevier | en_US |
dc.title | Collisional quenching of O(1D) by O(3P) | en_US |
dc.type | Article | en_US |
dc.rights.robots | IndexNoFollow | en_US |
dc.subject.hlbsecondlevel | Atmospheric, Oceanic and Space Sciences | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Space Physics Research Laboratory, University of Michigan, Ann Arbor, MI 48109, U.S.A. | en_US |
dc.contributor.affiliationother | Institute for Scientific Research, 33 Bedford Street, Lexington, MA 02173, U.S.A. | en_US |
dc.contributor.affiliationother | Harvard-Smithsonian Center for Astrophysics, Cambridge, MA 02138, U.S.A. | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/28609/1/0000418.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1016/0032-0633(90)90071-W | en_US |
dc.identifier.source | Planetary and Space Science | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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