Benjamin McCall and Takeshi Oka University of Chicago Therese R. Huet Universite de Lille
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Benjamin McCall and Takeshi Oka
University of Chicago
Therese R. HuetUniversite de Lille
James K. G. WatsonNational Research Council of Canada
Overtone and Combination Band Spectroscopy of H3
+
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About H3+
No electronic spectrum
Equilateral triangle configuration no allowed rotational spectrum
2y
2x
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Importance of H3+
* Dominant ion in H2-dominated plasmas
* 2 fundamental seen in emission on Jupiter
* 2 seen in absorption in interstellar medium
* As simplest polyatomic molecule, it is a benchmark for ab initio theory
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Why Study High Energy H3+?
* 22 band discovered on Jupiter, higher bands may be observable
* Emission from hot astronomical objects (planetary nebulae?)
NGC 6543. Balick AJ 94, 671 (1987)
* Refinement of theoretical understanding
* Breaking the barrier to linearity
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H3+ Vibrational Bands
1
1/270
1/840
1/4800
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Experimental Technique
Diode Laser
Spectrum Analyzer
Reference Cell
Detector
Discharge Cell
Autobalancing Detector
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New Focus Diode Laser
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Plasma Conditions
HHHH
eeHeH
322
22
* p(H2) ~ 0.5 Torr
* ~5 kV @ 6 kHz, 150 mA
* liquid-N2 cooling
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New Focus “Nirvana” Detector
“Autobalancing” detector outputs (S - g*R), where the gain ‘g’ is such that <(S - g*R)> = 0
at a user-selectable bandwidth
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Theoretical Predictions
Watson
Neale, Miller,& Tennyson
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Predictions for 1+220
Watson
Neale, Miller,& Tennyson
1+220 band is forbidden!
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Lines Studied to Date
Q(1,0)
R(3,3)
R(1,1)-
P(3,3)
R(2,2) 3
R(1,0)
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Representative Spectrum
NW
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H2 Rydberg Transitions
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Summary of Detections
Observed Assignment Watson Neale(cm-1) (J’G’U’)(JK) [O-W] [O-N]
7785.76 (1,3,2)(1,0) 7785.340 7786.009[0.420] [-0.249]
7789.88 (4,6,2)(3,3) 7790.025 7790.156[-0.145] [-0.276]
7822.38 (3,2,3)(2,2) 7822.250 7822.645[32
3] [0.127] [-0.268]
7826.74 (2,0,2)(3,3) 7826.679 7827.115[0.062] [-0.374]
7850.97 (2,4,2)(1,1) 7850.677 7851.250[0.291] [-0.282]
7970.42 (2,3,2)(1,0) 7970.124 7970.698[0.296] [-0.278]
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Future Work
* Complete scan of 1+222 band
(expect ~ 30 lines)
* Comparison of observed linesand theoretical predictions
* 42 band (Ti::Sapph laser)
* 52 band? (Ti::Sapph)
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1+222 Band Intensities