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EGAS41 - Swansea University

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41 st EGAS CP 10 Gdańsk 2009<br />

IR luminescence of Xe 2 excimers produced in dense Xe gas by<br />

electron impact<br />

A.F. Borghesani 1,2 , G. Carugno 2<br />

1 Dept. of Physics, <strong>University</strong> of Padua, and CNISM unit<br />

2 Istituto Nazionale di Fisica Nucleare<br />

via Marzolo 8, I-35131 Padua, Italy<br />

∗ Corresponding author: borghesani@padova.infm.it,<br />

We discovered the emission of an infrared (IR) continuum centred at 1.3 µm (˜ν ≈ 7800<br />

cm −1 ) due to the decay of Xe 2 excimers produced in dense Xe gas excited by 70-keV<br />

electrons [1].<br />

0.5<br />

1.2<br />

0.4<br />

1<br />

7600<br />

Ar-Xe<br />

I (arb. un.)<br />

0.3<br />

0.2<br />

0.8<br />

0.6<br />

0.4<br />

7200<br />

6800<br />

0.1<br />

0.2<br />

6400<br />

Xe<br />

0.0<br />

0<br />

6000 7000 8000 9000 10000 11000<br />

<br />

~<br />

(cm -1 )<br />

0 1 2 3 4 5 6 7 8<br />

N (10 26 m 3 )<br />

Figure 1: Left: Xe 2 IR emission spectrum. Thick line: FC calculations. Right: Density dependence<br />

of the peak wavenumber in pure Xe gas and in an Xe–Ar mixture.<br />

In the left panel of Fig. 1 we show the spectrum for P = 0.1 MPa. The continuum<br />

is due to a bound–free transition between the 0 + u state related to the 6p( 1 D 2 ) atomic<br />

limit and the 0 + g dissociative one related to the 6s(3 P 1 ) limit. This assignment reproduces<br />

the spectrum shape by means of Franck–Condon calculations [2]. A unique feature of<br />

the spectrum is that the wavenumber of its peak ν m is red-shifted as the gas density<br />

N increases. In the right panel of Fig.1 ν m is plotted vs N for P ≤ 3.3 MPa in pure<br />

Xe gas and in an Ar-Xe mixture. The shift is explained by accounting for the dielectric<br />

properties of the gas and the quantum multiple scattering of the optically active electron<br />

whose wavefunction extends over many atoms [1].<br />

References<br />

[1] A.F. Borghesani, G. Bressi, G. Carugno, E. Conti, D. Iannuzzi, J. Chem. Phys. 115,<br />

6042 (2001)<br />

[2] A.F. Borghesani, G. Carugno, I. Mogentale, J. Phys. B: At. Mol. Opt. Phys. 40,<br />

4551 (2007)<br />

70

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