The Knowledge Bank is scheduled for regular maintenance on Thursday, August 13th through Friday, August 14th. During this time, users will not be able to register, login, or submit content.

Show simple item record

dc.creatorBrazier, C. R.en_US
dc.creatorRuiz, J. I.en_US
dc.date.accessioned2008-01-11T21:39:50Z
dc.date.available2008-01-11T21:39:50Z
dc.date.issued2005en_US
dc.identifier2005-MH-01en_US
dc.identifier.urihttp://hdl.handle.net/1811/30335
dc.descriptionAuthor Institution: Department of Chemistry, California State University Long Beach, Long Beach, CA 90840en_US
dc.description.abstractAn electronic spectrum of the SiB molecule has been observed for the first time. The SiB molecule was produced in a Corona Excited Supersonic Expansion source using a mixture of diborane and silane gases seeded in helium. The emitted light was dispersed with a 1.3m spectrometer and recorded with a CCD camera. The region from 200nm to 800nm was examined and a single electronic system, A$^4\Pi -X^4\Sigma ^-$ observed with a 0-0 origin at 18432\wn . Supersonic cooling results in a rotational temperature of 20K and most emission is from the lowest $\Omega$=5/2 component. Observation of the $\Omega$=3/2 component gives the spin-orbit splitting as -23.9 \wn . The 0-0, 0-1, 0-2, 1-0, 1-2, and 1-3 bands have been analyzed.en_US
dc.language.isoEnglishen_US
dc.publisherOhio State Universityen_US
dc.titleTHE ELECTRONIC SPECTRUM OF SiBen_US
dc.typearticleen_US


Files in this item

Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail
Thumbnail

Items in Knowledge Bank are protected by copyright, with all rights reserved, unless otherwise indicated.

This item appears in the following Collection(s)

Show simple item record