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CALIFORNIA INSTITUTE OF TECHNOLOGY TIME DOMAIN TERAHERTZ SPECTROSCOPY OF POLYCYCLIC AROMATIC HYDROCARBONS Brandon Carroll  Marco A. Allodi  Sergio Ioppolo.

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Presentation on theme: "CALIFORNIA INSTITUTE OF TECHNOLOGY TIME DOMAIN TERAHERTZ SPECTROSCOPY OF POLYCYCLIC AROMATIC HYDROCARBONS Brandon Carroll  Marco A. Allodi  Sergio Ioppolo."— Presentation transcript:

1 CALIFORNIA INSTITUTE OF TECHNOLOGY TIME DOMAIN TERAHERTZ SPECTROSCOPY OF POLYCYCLIC AROMATIC HYDROCARBONS Brandon Carroll  Marco A. Allodi  Sergio Ioppolo  Ian A. Finneran  Brett A. McGuire  Xander de Vries  Geoffrey A. Blake

2 Polycyclic Aromatic Hydrocarbons (PAHs) Nearly any combination of aromatic rings Stable with a wide variety of charge states, electronic states, and hydrogenation Highly photostable and functionalizable INTRODUCTION

3 Bands at 3.3 μ m 6- 9 μ m and 11-15 μ m consistently appear together, however their relative intensities vary widely Transitions due to sp 2 hybridized (aromatic) carbonaceous species No one species can explain the observed variations in intensity or line shape/width UIRS

4 FAR INFRARED PAH EMISSION Boersma et al. ApJ 729 64, (2011)

5 SPECTRAL COVERAGE

6 EXPERIMENTAL SETUP

7 ANTHRACENE PELLETS

8 Three simple PAHs Crystalline samples Polyethylene substrate 0.3 THz – 8 THz Multiple temperatures –10 K, 37.5 K, 75 K, 150 K, 300K SPECTRA

9 NAPHTHALENE 4.9 THz

10 NAPHTHALENE 5.2 THz

11 NAPHTHALENE Frequency (cm -1 ) 267 200133 67 0

12 NAPHTHALENE Frequency (cm -1 ) 267 200 67 0 Frequency (THz)

13 ANTHRACENE 2.5 THz

14 ANTHRACENE 3.3 THz

15 ANTHRACENE 7.0 THz

16 ANTHRACENE Frequency (cm -1 ) 267 200 67 0 Frequency (THz)

17 ANTHRACENE Frequency (cm -1 ) 267 200 67 0 Frequency (THz)

18 PYRENE 2.7 THz

19 PYRENE 5.7 THz

20 PYRENE Frequency (cm -1 ) 267 200 67 0 Frequency (THz)

21 PYRENE Frequency (cm -1 ) 267 200 67 0 Frequency (THz)

22 CONCLUSION AND FUTURE DIRECTIONS Initial spectra a promising Crystalline samples are promising, but complex Simple ab initio is a good start, but not complete

23 Si substrate Optical constants Lattice vibrations Additional species Matrix isolation CONCLUSION AND FUTURE DIRECTIONS Initial spectra a promising Crystalline samples are promising, but complex Simple ab initio is a good start, but not complete

24 ACKNOWLEDGEMENTS Blake Lab: -Jacob Good - Nate Crockett -Masha Klescheva -Coco Zhang -Dana Anderson -Katherine Kaufman -Alex Lockwood


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