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The Infra‐Red Spectrum of C2H6

dc.contributor.authorSmith, Lincoln G.en_US
dc.date.accessioned2010-05-06T22:53:31Z
dc.date.available2010-05-06T22:53:31Z
dc.date.issued1949-02en_US
dc.identifier.citationSmith, Lincoln G. (1949). "The Infra‐Red Spectrum of C2H6." The Journal of Chemical Physics 17(2): 139-167. <http://hdl.handle.net/2027.42/70901>en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/70901
dc.description.abstractThe infra‐red spectrum of C2H6 gas has been studied in the region between 1.6 and 13μ with a spectrometer of high resolving power. From measurements on four resolved ∥ bands the value IB0 = (42.234±0.011)×10−40 g cm2 has been obtained for the large moment of inertia in the ground state. From measurements on the three fundamental ⊥ bands the best value at present available for the small moment of inertia is IA = 10.81×10−40 g cm2. Because of uncertainties concerning the perturbations of degenerate state ν8, of which a semi‐quantitative explanation which is apparently basically correct has been obtained, this value is provisional but appears to be fairly reliable. With these values of IB0 and IA, if one assumes C☒C = 1.55A, one obtains C☒H = 1.098A and ≰HCC = 109° 3′. From the considerations of the perturbations of state ν8 and of the frequencies and line spacings of the combination ⊥ bands, spectroscopic evidence indicating that the configuration of C2H6 is staggered (point group D3d) has for the first time been obtained. Also from these considerations the reliable value ν8 = 1472.2 cm−1 and the values ν4 = 290 cm−1 for the torsion frequency and ν12 = 1190 cm−1 for the ``uncertain'' frequency have been obtained. The latter two values are perhaps somewhat more reliable and not inconsistent with values obtained previously by other methods. These and other results are summarized in Figs. 1 and 14 and in Tables XII—XV.en_US
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dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleThe Infra‐Red Spectrum of C2H6en_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumPalmer Physical Laboratory, Princeton, New Jersey, and University of Michigan, Ann Arbor, Michiganen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/70901/2/JCPSA6-17-2-139-1.pdf
dc.identifier.doi10.1063/1.1747206en_US
dc.identifier.sourceThe Journal of Chemical Physicsen_US
dc.identifier.citedreferenceL. G. Smith and W. M. Woodward, Phys. Rev. 61, 386A (1942).en_US
dc.identifier.citedreferenceG. Herzberg, Infrared and Raman Spectra of Polyatomic Molecules (D. Van Nostrand Company, Inc., New York, 1945).en_US
dc.identifier.citedreferenceReference 2, p. 342.en_US
dc.identifier.citedreferenceThe staggered configuration is also favored by the recent theoretical considerations of E. N. Lassettre and Laurence B. Davis (J. Chem. Phys. 16, 151 (1948)).en_US
dc.identifier.citedreferenceL. G. Smith, Rev. Sci. Inst. 13, 54, 63 and 65 (1942).en_US
dc.identifier.citedreferenceIn the case of Fig. 2b the curve was replotted from the original photograph which was marred by bad zero drift. Hence in this figure the dashed zero line is straight and horizontal.en_US
dc.identifier.citedreferenceC. F. Meyer and A. Levin, Phys. Rev. 34, 44 (1929).en_US
dc.identifier.citedreferenceG. Herzberg, Molecular Spectra and Molecular Structure I. Diatomic Molecules (Prentice‐Hall Inc., New York, 1939), p. 60.en_US
dc.identifier.citedreferenceHere, as elsewhere in this report, the notation is essentially that used throughout references 2 and 8, the subscript 0 instead of the superscript ″ is used on rotational constants of the ground state and J ≡ J″.J≡J″.en_US
dc.identifier.citedreferenceJ. B. Howard, J. Chem. Phys. 5, 442 (1937).en_US
dc.identifier.citedreferenceJ. W. M. DuMond and E. R. Cohen, Rev. Mod. Phys. 20, 82 (1948).en_US
dc.identifier.citedreferenceJahn’s rule, cf. reference 2, p. 276 and Tables 20, 22 and 31.en_US
dc.identifier.citedreferenceA. Levin and C. F. Meyer, J. Opt. Soc. Amer. 16, 137 (1928).en_US
dc.identifier.citedreferenceJ. B. Howard, J. Chem. Phys. 5, 451 (1937).en_US
dc.identifier.citedreferenceR. G. Owens and E. F. Barker, J. Chem. Phys. 10, 146 (1942). The wave number values reported by these authors are systematically lower than those in Table I by about 0.1 cm−1.0.1cm−1.en_US
dc.identifier.citedreferenceE. Bartholomé and J. Karweil, Zeits. f. Physik. Chemie B39, 1 (1938).en_US
dc.identifier.citedreferenceS. L. Gerhard and D. M. Dennison, Phys. Rev. 43, 197 (1933).en_US
dc.identifier.citedreferenceIt is assumed here that the energies of each set of levels are represented by a single‐valued function of K in which K is taken positive for +l levels+llevels (transitions to which give rise to RQRQ lines) and negative for −l levels−llevels (cf. reference 2, p. 403).en_US
dc.identifier.citedreferenceH. H. Nielsen, Phys. Rev. 60, 794 (1941).en_US
dc.identifier.citedreferenceCf. reference 2, p. 429 and footnote 9.en_US
dc.identifier.citedreferenceL. Pauling and L. O. Brockway, Jr., J. Am. Chem. Soc. 59, 1223 (1937).en_US
dc.identifier.citedreferenceThe ζ value of a combination state and hence ΔνΔν of the corresponding band are independent of what non‐degenerate vibrations are excited in the state. (Cf. reference 30 below.)en_US
dc.identifier.citedreferenceIt is possible that the group of lines 5 to 13 of Fig. 10 near 3217 cm−13217cm−1 whose spacings are rather irregular, but roughly the same as for the band at 3257.8 cm−1,3257.8cm−1, corresponds to a combination of ν4ν4 and another component of ν10.ν10.en_US
dc.identifier.citedreferenceS. Bhagavantam, Ind. J. Phys. 6, 596 (1931) and B. L. Crawford, Jr., W. H. Avery, and J. W. Linnett, J. Chem. Phys. 6, 682 (1938).en_US
dc.identifier.citedreferenceG. Glockler and M. M. Renfrew, J. Chem. Phys. 6, 295 (1938).en_US
dc.identifier.citedreferenceG. B. Kistiakowsky, J. R. Lacher and F. Stitt, J. Chem. Phys. 7, 289 (1939).en_US
dc.identifier.citedreferenceF. Stitt, J. Chem. Phys. 7, 297 (1939).en_US
dc.identifier.citedreferenceHerzberg (reference 2, p. 405) citing Howard (see reference 14), who does not consider this sum, erroneously states that this sum is zero.en_US
dc.identifier.citedreferenceWe speak in this section of the ΔνΔν of a band even though such a band is inactive.en_US
dc.identifier.citedreferenceM. Johnston and D. M. Dennison, Phys. Rev. 48, 868 (1935).en_US
dc.identifier.citedreferenceW. H. Avery and C. F. Ellis, J. Chem. Phys. 10, 10 (1942).en_US
dc.identifier.citedreferenceVery weak absorption near 1216 cm−11216cm−1 has been observed under low dispersion by Avery and Ellis (see reference 31) and attributed by them to band ν11−ν4.ν11−ν4.en_US
dc.owningcollnamePhysics, Department of


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