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The Infra‐Red Absorption Spectrum of Propane

dc.contributor.authorWu, Violet L.en_US
dc.contributor.authorBarker, E. F.en_US
dc.date.accessioned2010-05-06T22:45:22Z
dc.date.available2010-05-06T22:45:22Z
dc.date.issued1941-07en_US
dc.identifier.citationWu, Violet L.; Barker, E. F. (1941). "The Infra‐Red Absorption Spectrum of Propane." The Journal of Chemical Physics 9(7): 487-491. <http://hdl.handle.net/2027.42/70815>en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/70815
dc.description.abstractOf the twenty‐seven internal degrees of freedom of propane, all nondegenerate, twenty‐two may appear as fundamental absorption bands. These bands fall into three symmetry classes, designated A1, B1 and B2, and distinguishable by their characteristic contours. Because of overlapping, however, it is impossible in many cases to determine their positions precisely. This is especially true in the regions of the C☒H valence and deformation frequencies. Some ten or twelve fundamental bands may be identified with confidence as well as a number of combinations. An A1 band at 870 cm—1 and a B2 band at 748 cm—1 have been partially resolved, the line spacing being about 1.47 cm—1 in agreement with predictions based upon electron diffraction measurements. The fine structure of the B1 bands has not been observed (the predicted spacing is 0.5 cm—1) but the interval between maxima of the P and R branches is approximately 26 cm—1 as expected. With 24 cm‐atmospheres of gas no bands were observed between 15μ and 35μ, although the symmetrical C☒C deformation might be expected to produce a band of appreciable intensity within these limits. This frequency has apparently been observed in Raman spectra at 375 cm—1.en_US
dc.format.extent3102 bytes
dc.format.extent258814 bytes
dc.format.mimetypetext/plain
dc.format.mimetypeapplication/pdf
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleThe Infra‐Red Absorption Spectrum of Propaneen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumHarrison M. Randall Laboratory of Physics, University of Michigan, Ann Arbor, Michiganen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/70815/2/JCPSA6-9-7-487-1.pdf
dc.identifier.doi10.1063/1.1750943en_US
dc.identifier.sourceThe Journal of Chemical Physicsen_US
dc.identifier.citedreferenceE. Bartholomé, Zeits. f. Physik. Chemie B23, 152 (1933).en_US
dc.identifier.citedreferenceP. Daure, Ann. de Physique 12, 375 (1929); S. Bhagavantam, Ind. J. Phys. 6, 595 (1932); K. W. F. Kohlrausch and F. Köppl, Zeits. f. Physik. Chemie B26, 209 (1934).en_US
dc.identifier.citedreferenceL. Pauling and L. O. Brockway, J. Am. Chem. Soc. 59, 1223 (1937).en_US
dc.identifier.citedreferenceD. M. Dennison, Rev. Mod. Phys. 3, 280 (1931).en_US
dc.identifier.citedreferenceH. H. Nielsen, Phys. Rev. 38, 1432 (1931).en_US
dc.identifier.citedreferenceR. M. Badger and L. R. Zumwalt, J. Chem. Phys. 6, 711 (1938).en_US
dc.identifier.citedreferenceA. Dadieu and K. W. F. Kohlrausch, Akad. Wiss. Wien. 139, 165 (1930).en_US
dc.identifier.citedreferenceS. L. Gerhard and D. M. Dennison, Phys. Rev. 43, 197 (1933).en_US
dc.owningcollnamePhysics, Department of


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