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Volumn 55, Issue 1, 1971, Pages 288-309

Iodine revisited

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[No Author keywords available]

Indexed keywords


EID: 0004975106     PISSN: 00219606     EISSN: None     Source Type: Journal    
DOI: 10.1063/1.1675521     Document Type: Article
Times cited : (466)

References (118)
  • 3
    • 0000734540 scopus 로고
    • For the most accurate evaluation of the molecular constants and U(R) curve for state X, see
    • (1970) J. Chem. Phys. , vol.52 , pp. 2683
    • LeRoy, R.J.1
  • 11
    • 85038172652 scopus 로고    scopus 로고
    • For any [formula omitted] configuration, Recknagel shows that the energy is [formula omitted] C, [formula omitted] [formula omitted] [formula omitted] and [formula omitted] for the [formula omitted] [formula omitted] [formula omitted] [formula omitted] [formula omitted] and [formula omitted] states, respectively, where a, b, c are various specific integrals.
    • For [formula omitted] the near coincidence of the first three states shows that [formula omitted] The [formula omitted] minus [formula omitted] energy difference should then be [formula omitted] The [formula omitted] minus [formula omitted] and the [formula omitted] minus [formula omitted] differences should each be [formula omitted] Now for the integrals a and b we have experimental data7 for the [formula omitted] molecule: [formula omitted] and [formula omitted] for [formula omitted] the values should be similar but somewhat greater, giving [formula omitted] about, say, 2.7 eV. Applying the factor 0.37 as above, we arrive at estimates of 1.0 eV for the energy differences [formula omitted] minus [formula omitted] and [formula omitted] minus [formula omitted] in the 2332 configuration of [formula omitted] (b) Dr. I. Hanazaki has very kindly gone through the calculations for the [formula omitted] case and shown that the results are exactly the same as for the [formula omitted] case.
  • 12
    • 84951245522 scopus 로고    scopus 로고
    • For a [formula omitted] configuration as in the 2310 configuration of [formula omitted] Recknagel shows that the energy is [formula omitted] C, [formula omitted] [formula omitted] [formula omitted] [formula omitted] for the respective states [formula omitted] [formula omitted] [formula omitted] [formula omitted] [formula omitted] and [formula omitted]
    • The observed energy difference between the [formula omitted] and [formula omitted] states is 2.6 eV, which is 2a. The difference between [formula omitted] and [formula omitted] yields [formula omitted] from which [formula omitted]
  • 15
    • 85038182576 scopus 로고    scopus 로고
    • case the 2332 states [formula omitted] and/or [formula omitted] and [formula omitted]) were lower in energy than 1441, [formula omitted] as has sometimes been suggested, the correlations in Fig. 1 would have to be changed, but these possibilities are here deemed rather strongly improbable (cf. Sec. VI).
  • 16
    • 84951221055 scopus 로고    scopus 로고
    • The validity of this assumption is uncertain.
    • It was based on the following thought: The repulsion energy of two He atoms (MO configuration [formula omitted]) at 0.75 Å is about the same (about 10 eV) as the repulsion energy of two H atoms in the [formula omitted] [formula omitted] state at 0.75 Å.
  • 17
    • 84951258650 scopus 로고
    • For [formula omitted] the value 7.2 a.u. calculated by
    • 8a In Table II, it is assumed that the states dissociate as indicated in Table I. However, in case the order of states of given case c character is actually reversed, the corresponding coefficients in Table I would be interchanged. For example, if 2341, [formula omitted] lies below 2422, [formula omitted] instead of above it as estimated in Table I, the corresponding coefficients in Table II (together with their dissociation products) would be interchanged.
    • (1968) Can. J. Phys. , vol.46 , pp. 2336
    • Fisher, C.F.1
  • 23
    • 36849099837 scopus 로고
    • See p. 5419 for estimate for intensity of continuum of [formula omitted] absorption.
    • (1969) J. Chem. Phys. , vol.51 , pp. 5414
    • Chutjian, A.1
  • 37
    • 85038172966 scopus 로고    scopus 로고
    • 19 in which it was assumed that the predissociating state is 2332, [formula omitted]
  • 38
    • 85038191712 scopus 로고    scopus 로고
    • See reference to it on p. 555 of Ref. 28.
  • 39
    • 85038182918 scopus 로고    scopus 로고
    • As discussed above, most probably the [formula omitted] curve which crosses the B curve is that from 1441, [formula omitted] but possibly it is the 2332, [formula omitted] or [formula omitted] curve.
  • 41
    • 84951220014 scopus 로고
    • The 2341, [formula omitted] for which [formula omitted] would also be very weakly possible. The selection rule [formula omitted] (hence [formula omitted]) holds for spectroscopic transitions between two case a [formula omitted] states; see
    • Van Nostrand, New York, 2nd ed.; The same rule should hold to some extent in case c; but in any event, the strongest known [formula omitted] transition in iodine, [formula omitted] (see Sec. V) is weak.
    • (1950) Spectra of Diatomic Molecules , pp. 242
    • Herzberg, G.1
  • 42
    • 85038192914 scopus 로고    scopus 로고
    • 21 shows the 2341, [formula omitted] curve as running entirely below the B curve, which would be very unfavorable for collisional predissociation.
    • But such a location of this [formula omitted] curve seems to be clearly excluded by the considerations on which Table I and Fig. 1 are based.
  • 43
    • 85038179243 scopus 로고    scopus 로고
    • The estimated vertical energy of 2341, [formula omitted] is only 0.3 eV above that of [formula omitted] in Table I, and a reversed order is almost as likely as not.
    • If the order were reversed, the [formula omitted] curve would dissociate to two [formula omitted] atoms, crossing the B curve a little above where the [formula omitted] crosses.
  • 46
    • 85038186795 scopus 로고    scopus 로고
    • 26a
    • An exact value is difficult to determine because the weak continuum of [formula omitted] overlaps the much stronger absorption of the B←X bands.
  • 47
    • 85038172156 scopus 로고    scopus 로고
    • Other interactions with higher-energy states should be included in a complete configuration-interaction calculation, but we may assume these to be about the same for [formula omitted] and [formula omitted]
  • 48
    • 85038184652 scopus 로고    scopus 로고
    • References 36 and 37 are in good agreement on the value [formula omitted] as estimated from their absorption curves.
    • However, Tellinghuisen estimates a somewhat higher value, perhaps [formula omitted]
  • 49
    • 85038174590 scopus 로고    scopus 로고
    • The dipole strengths for [formula omitted] and [formula omitted] are given as 2D because of the twofold degeneracy of [formula omitted] and [formula omitted] where D refers to a single component.
    • On the other hand, [formula omitted] is non-degenerate.
  • 51
    • 85038193235 scopus 로고    scopus 로고
    • 33 forbidding [formula omitted] in case a and thereby indicating weakness in case c) shows that his argument is invalid.
  • 52
    • 85038187613 scopus 로고    scopus 로고
    • The matrix element between [formula omitted] and [formula omitted] is zero; they are mixed only indirectly via [formula omitted]
  • 53
    • 85038183235 scopus 로고    scopus 로고
    • 46 of 0.43 for the oscillator strength of 1441, [formula omitted] with [formula omitted] for this transition (see Sec. VI for discussion).
  • 59
    • 85038187238 scopus 로고    scopus 로고
    • The vertical energies at [formula omitted] of state X should be somewhat less than those given by [formula omitted] since the first peak of the vibrational wavefunction at the inner limb of the upper U(R) curve, which approximately determines the position of [formula omitted] is somewhat outside the point of intersection of the vibrational energy level with the U(R) curve. This difference has been ignored here in Table I in the case of the 1441, [formula omitted] state.
    • For the [formula omitted] curve, it is taken into account by utilizing the segment of U(R) curve deduced by Mathieson and Rees.
  • 65
    • 34250924476 scopus 로고
    • At shorter wavelengths are several systems some, at least, of which are Rydberg bands (for a pictorial representation, see Ref. 47).
    • Z. Phys.
    • (1935) Z. Physik , vol.97 , pp. 603
    • Cordes, H.1
  • 72
    • 0000818340 scopus 로고
    • Other values are 0.2 according to
    •  but their value was incidental to another investigation and seems to have been only very roughly determined;
    • (1968) J. Phys. Chem. , vol.72 , pp. 3046
    • Huebert, B.J.1    Martin, R.M.2
  • 75
    • 85038179821 scopus 로고    scopus 로고
    • The same effect has been observed by others, e.g., R. Millikan (private communication).
  • 76
    • 84951235529 scopus 로고    scopus 로고
    • particular, note the discordant interval [formula omitted] between the [formula omitted] and 53 969 bands in the [formula omitted] column where all the neighboring intervals are near [formula omitted] likewise the discordant interval [formula omitted] between the 53 827 and 53 923 bands in the [formula omitted] column where all the neighboring intervals are near [formula omitted]
    • These discrepancies are far too large to be accounted for by experimental error, whereas Eq. (11) represents all the bands but the first two (out of 94 Fk Cordes bands) with an average discrepancy of something like [formula omitted]
  • 83
    • 84951220014 scopus 로고
    • Transitions [formula omitted] and [formula omitted] should be much weaker since there is a strict selection rule [formula omitted] in case a, hence [formula omitted] if [formula omitted] as here [cf.
    • Van Nostrand, New York; although [formula omitted] becomes possible in case c as here, such transitions should be relatively weak, especially in view of the fact that the only known [formula omitted] transitions in [formula omitted] (in particular, 2431, [formula omitted]) are weak.
    • (1950) Spectra of Diatomic Molecules , pp. 242-3
    • Herzberg, G.1
  • 103
    • 85038190979 scopus 로고    scopus 로고
    • Preceded by a few weaker anti-Stokes lines beginning at 1860 Å.
  • 104
    • 85038177840 scopus 로고    scopus 로고
    • Oldenberg reported some overlapping of continuous background and diffuse bands beginning at λ 2042.
  • 105
    • 85038174561 scopus 로고    scopus 로고
    • 71 did.
  • 109
    • 85038187038 scopus 로고    scopus 로고
    • [formula omitted] cannot be exactly determined from these data since for the longer exciting wavelengths, heated iodine was used, and excitation must have come from initially vibrating molecules. Here absorption must be in the KM and PR bands.
    • In any event, [formula omitted] is obviously smaller for the longer exciting wavelengths.
  • 110
    • 85038186486 scopus 로고    scopus 로고
    • Reference 90, Eqs. (23) and (25).
  • 111
    • 85038192686 scopus 로고    scopus 로고
    • The change in [formula omitted] in Eq. (13) is less important for [formula omitted] than the change in [formula omitted] since [formula omitted] is not very sensitive to [formula omitted]
  • 112
    • 85038192651 scopus 로고    scopus 로고
    • Here the quantity [formula omitted] is small, so that the harmonic approximation is accurate enough for present purposes.
  • 115
    • 85038185257 scopus 로고    scopus 로고
    • 57 on iodine in argon, and this system has been attributed to a molecule IN.
    • Elliott, A.1
  • 117
    • 85038185572 scopus 로고    scopus 로고
    • With respect to expected shortcutting into excited atoms, see the last paragraph of Sec. III.
  • 118
    • 85038187789 scopus 로고    scopus 로고
    • According to a calculation by N. S. Ham (see Ref. 37, footnote on p. 756), [formula omitted] is [formula omitted] and [formula omitted] so that [formula omitted] would be [formula omitted] and [formula omitted] and for [formula omitted] and [formula omitted] there is a 9.5percent; mixing.


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