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SRC Users' Meeting - Synchrotron Radiation Center - University of ...

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FIELD IONIZATION OF CH 3 I IN SUPERCRITICAL AR<br />

C. M. Evans 1 and G. L. Findley 2<br />

1 Department <strong>of</strong> Chemistry and Biochemistry, Queens College – CUNY,<br />

65-30 Kissena Blvd, Flushing, NY 11367<br />

2 Department <strong>of</strong> Chemistry, <strong>University</strong> <strong>of</strong> Louisiana at Monroe,<br />

Monroe, LA 71209<br />

Supercritical fluids have recently been shown to improve rates and modify product ratios<br />

<strong>of</strong> chemical reactions, to vary chemical shifts in NMR, and to alter lifetimes and energies <strong>of</strong><br />

molecular vibrational states. However, the detailed nature <strong>of</strong> the molecule (i.e., dopant)/fluid<br />

(i.e., perturber) interactions that lead to these effects is not well understood. In recent studies <strong>of</strong><br />

the density dependence <strong>of</strong> solvatochromic shifts <strong>of</strong> vibrational and UV-visible absorption bands,<br />

an increase in the energy shift near the critical density along the critical isotherm <strong>of</strong> the perturber<br />

was observed (cf. Fig. 1). In measurements <strong>of</strong> the field ionization <strong>of</strong> high-n CH 3 I Rydberg states<br />

in supercritical argon, we observed a decrease in the shift near the critical density along the<br />

critical isotherm (cf. Fig. 2). Such a dramatic difference in behavior is striking. The densitydependent<br />

shift <strong>of</strong> the dopant ionization energy in dense media can be written as a sum <strong>of</strong><br />

contributions, = w 0 (P) + V 0 (P), where w 0 is the shift due to the average polarization <strong>of</strong> the<br />

perturber by the ionic core, V 0 is the quasi-free electron energy in the perturbing medium and P<br />

is the perturber number density. Our preliminary analysis suggests that while w 0 shifts in a<br />

manner similar to the vibrational and UV-visible band shifts, V 0 does not. Thus, the difference in<br />

behavior between the shift <strong>of</strong> high-n Rydberg states and <strong>of</strong> vibrational (or UV-visible) absorption<br />

bands is due to the interaction <strong>of</strong> the quasi-free electron with the perturbing medium.<br />

This work was conducted at <strong>SRC</strong> (NSF DMR-0084402) and was supported by a grant from<br />

the Louisiana Board <strong>of</strong> Regents Support Fund (LEQSF (1997-00)-RD-A-14).<br />

1996<br />

0.0<br />

1994<br />

-0.2<br />

line position (cm )<br />

-1<br />

1992<br />

1990<br />

1988<br />

(eV)<br />

-0.4<br />

-0.6<br />

1986<br />

-0.8<br />

1984<br />

0 2 4 6 8 10 12 14 16 18<br />

density (mol/L)<br />

Fig. 1. Infrared absorption line peak position <strong>of</strong> the T 1u<br />

asymmetric CO stretching mode <strong>of</strong> W(CO) 6 in CO 2 vs<br />

CO 2 density at (!) the critical temperature <strong>of</strong> 33C and<br />

() 50C. The lines provide a visual aid. (Modified<br />

from R.S. Urdahl, D. J. Myers, K. D. Rector, P. H.<br />

Davis, B. J. Cherayil and M. D. Fayer, J. Chem. Phys<br />

107, 3747 (1997).)<br />

-1.0<br />

0<br />

5<br />

10<br />

15<br />

Ar<br />

(10 21 cm -3 )<br />

Fig. 2. Ionization potential <strong>of</strong> CH 3 I in argon<br />

plotted as a function <strong>of</strong> argon number density Ar.<br />

() -114C; () -118C; () various lower<br />

temperatures other than the critical temperature;<br />

() the critical temperature <strong>of</strong> -122C. The lines<br />

provide a visual aid. (C. M. Evans and G. L.<br />

Findley, to be published.)<br />

20<br />

25

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