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Michael N. Sullivan*, Jacob T. Stewart†, Michael C. Heaven*

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Presentation on theme: "Michael N. Sullivan*, Jacob T. Stewart†, Michael C. Heaven*"— Presentation transcript:

1 High-Resolution Electronic Spectroscopy of the Ultraviolet Bands of CaO
Michael N. Sullivan*, Jacob T. Stewart†, Michael C. Heaven* *Emory University, Dept. of Chemistry, Atlanta, GA 30322 †Connecticut College, Chemistry Department, New London, CT 06320

2 Motivation Demonstrate promise for cold molecular ions
Accurate potential energy surfaces Need spectroscopic data Challenges High density of states State interaction 1Pyka et al. Nature Comm., 4, 2291, 2013.

3 Previous Work First studied 1930’s2,3,4 Green and orange bands
Field and co-workers5,6,7 Low lying electronic states X 1Σ+, Aˈ1∏, a3∏, b3Σ+, A1Σ+ Bernath and co-workers – experimental8,9 Khalil et al. – theoretical10,11 Ground state assignment Pearson et al.12 UV bands Lagerqvist, Spectral congestion 10Khalil et al. Chem. Phys., 386, 50, 2011.

4 Experimental Setup

5 Ablation Source

6 Survey Spectra Frequency (cm-1) 30,000 30,500 31,000 31,500 32,000
32,500 33,000 Frequency (cm-1)

7 (νˈ,νˈ) Frequency (cm-1) 30,000 30,500 31,000 31,500 32,000 32,500
33,000 Frequency (cm-1)

8 32,460 32,480 32,500 32,520

9 32,460 32,480 32,500 32,520 Frequency (cm-1)

10 (νˈ,νˈ) ? Frequency (cm-1) 30,000 30,500 31,000 31,500 32,000 32,500
33,000 Frequency (cm-1)

11 Evidence of CaOH Interstellar clouds Low lying electronic levels
Strong ionic character Previously observed by Pereira and Levy14 D state characterized E and F states uncharacterized Closed shell OH- anion, and Ca+ cation (4s unpaired electron and closed shell argon core). Low lying electronic states ionic involving promotion of unpaired electrons to excited orbitals of Ca+. R. Pereria and D.H. Levy. J. Chem. Phys., 105, 9733, 1996.

12 Band origin – 29,869.59 cm-1 Bˈˈ- .4428 cm-1
CaO - C 1Σ+ ← X 1Σ+ (2,0) Band origin – 29, cm-1 Bˈˈ cm-1 Bˈ cm-1 CaOH – E 2Σ+ ← X 2Σ+ Band origin – 29, cm-1 Bˈˈ cm-1 Bˈ cm-1 Dˈˈ E-7 cm-1 Dˈ E-6 cm-1 TRot~ 150K

13 Molecular Constants CaO
B State (1∏) Vibrational Assignment ν0 9,0 30,299.54 0.3190 10,0 30,777.67 0.3163 11,0 31,252.21 0.3145 12,0 31,722 0.3107 13,0 32,186.54 0.3091 14,0 32,645.96 0.3081 15,0 33,101.23 0.3113 Note: Ground state rotational constants from Pearson et al.12 used in fits. Units in cm-1.

14 Molecular Constants CaO
C State (1Σ+) Vibrational Assignment ν0 Perturbation 2,0 29,869.59 0.3653 3,0 30,407.28 0.3620 4,0 30,938.15 0.3546 5,0 31,461.82 0.3540 6,0 31,977.67 0.3471 6,1 31,255.22 0.3497 7,0 32,496.26 0.3521 17 7,1 31,773.87 8,0 33,007.56 0.3437 8,1 32,285.11 0.3418 Note: Ground state rotational constants from Pearson et al.12 used in fits. Units in cm-1.

15 Molecular Constants CaO
D State (1Σ+) Vibrational Assignment ν0 Perturbation 0,0 32,036.99 0.3159 1,0 32,496.7 0.3087 17 1,1 31,774.32 2,0 32,955.18 0.3128 Note: Ground state rotational constants from Pearson et al.12 used in fits. Units in cm-1.

16 Summary Conclusions Future Work
Investigate neutral CaO using jet cooled techniques Extract rovibrational constants for B←X and C←X electronic bands Observed D←X band for the first time Future Work Assign transitions for E←X and F←X electronic band of CaOH Improved ablation source design Use experimental setup to performance double resonance microwave/millimeter studies of CaO

17 Acknowledgements Dr. Michael Heaven Dr. Jacob Stewart
Dr. Adrian Gardner Cody Anderson Heaven group Dr. Jiande Han Kyle Mascaritolo Joshua Bartlett Robert VanGundy Amanda Dermer

18 References A. Lagerqvist, Ark. Fys. 8, 83–95 (1954).
Pyka et al., Nature Comm., 4, 2291, 2013 P. C. Mahanti, Phys. Rev. 42, 609–621 (1932). P. H. Brodersen, Z. Phys. 79, 613–625 (1932). P. H. Brodersen, Z. Physik 104, 135–156 (1937). D.P. Baldwin, J.B. Norman, R.A. Soltz, A. Sur, R.W. Field, J. Mol. Spec. 139, 39 (1990). D.P. Baldwin,R.W. Field, J. Mol. Spec. 139, 68 (1990). D.P. Baldwin,R.W. Field, J. Mol. Spec. 139, 77 (1990). C. Focsa, A. Poclet, B. Pinchemel, R.J. Le Roy, P.F. Bernath, J. Mol. Spec. 203, 330 (2000). A. van Groenendael, M. Tudorie, C. Focsa, B. Pinchemel, P.F. Bernath, J. Mol. Spec. 234, 255 (2005). H. Khalil, V. Brites, F. Le Quéré, C. Léonard, Chem. Phys. 386, (2011). H. Khalil, F. Le Quéré, V. Brites, C. Léonard, J. Mol. Spec. 271, 1-9 (2012). R.A. Creswell, W.H. Hocking, E.F. Pearson, Chem. Phys. Lett. 48, (1977). A. Lagerqvist, Ark. Fys. 8, 83–95 (1954). R. Pereria and D.H. Levy. J. Chem. Phys., 105, 9733, 1996.


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