2001
DOI: 10.1021/jp003728a
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Multichannel Quantum Defect Theory (MQDT) Analysis of the (2 + 1‘) Mass Analyzed Threshold Ionization (MATI) Spectroscopy of NH3

Abstract: MATI spectra of NH 3 have been recorded using two-color (2 + 1′) multiphoton excitation via the B ˜and C ˜′ states and have been simulated using multichannel quantum defect theory. New vibrational bands in the MATI spectra are reported for intermediate levels up to ν 2 ) 6 in the B ˜state. The spectra obtained should in principle be identical to ZEKE spectra recorded under the same resolution. A good agreement between experiment and theory is obtained by using quantum defects determined previously from optical… Show more

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Cited by 25 publications
(44 citation statements)
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“…30,31 However, the observed ⌬K = 0 with l = odd transitions do not follow this atomiclike picture that assumes a predominant 2p z character for the nonbonding orbital. The observation of ⌬K = odd as well as l = odd transitions has been rationalized by Niu and White 14 and Dickinson et al 12,13 that l spoiling, i.e., p-d␦ mixing, in the process of photoionization of NH 3 is substantial because the photoelectron goes through the pyramidal potential at short range, resulting in both l = even and odd transitions. This interpretation could be problematic because the nuclear wave function in the ground state of NH 3 is located equally in both potential wells associated with the umbrella motion.…”
Section: Resultsmentioning
confidence: 85%
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“…30,31 However, the observed ⌬K = 0 with l = odd transitions do not follow this atomiclike picture that assumes a predominant 2p z character for the nonbonding orbital. The observation of ⌬K = odd as well as l = odd transitions has been rationalized by Niu and White 14 and Dickinson et al 12,13 that l spoiling, i.e., p-d␦ mixing, in the process of photoionization of NH 3 is substantial because the photoelectron goes through the pyramidal potential at short range, resulting in both l = even and odd transitions. This interpretation could be problematic because the nuclear wave function in the ground state of NH 3 is located equally in both potential wells associated with the umbrella motion.…”
Section: Resultsmentioning
confidence: 85%
“…Ammonia is also recognized as an astrophysical molecule, which has been found to exist in primitive planetary atmospheres, comets, and interstellar space. [1][2][3][4] Partly for this reason, NH 3 has been the subject of many previous photoionization and photoelectron measurements, [5][6][7][8][9][10][11][12][13][14][15] which have provided valuable energetic and spectroscopic information for NH 3 and its cation NH 3 + . From an experimental point of view, the relatively large rotational constants ͑Ϸ10 cm −1 ͒ of both NH 3 and NH 3 + represent an advantage, 11,16,17 making it easier to obtain fully rovibrationally resolved transitions in photoionization and photoelectron studies.…”
Section: Introductionmentioning
confidence: 99%
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“…m 2 þ m 3 [1][2][3]. At low resolution, the 14 NH þ 3 ion has been studied by photoelectron and photoionization spectroscopy [4][5][6][7][8][9][10][11][12][13][14][15]. Further, the infrared spectrum of NH þ 3 , trapped in a solid neon matrix, has been recorded [16].…”
Section: Introductionmentioning
confidence: 99%
“…The future clearly lies in more rigorous calculations based on quantum chemical input data and fully developed MQDT analyses. Several significant MQDT studies of the photoionization dynamics of other polyatomic molecules, including H 2 O and NH 3 (82)(83)(84)(85), have already been performed. Such studies have allowed the assignment of structure in the near-threshold photoionization spectra and in pulsed-field ionization spectra.…”
Section: Future Directionsmentioning
confidence: 99%