All non-condensing gases give similar
low temperature decrepitation peaks
Although much of the focus of Au exploration and acoustic decrepitation
is on the CO2 content of fluid inclusions, other gases such
as CH4 and N2 also give the same low temperature
decrepitation peaks as seen on CO2 rich samples. This is a
consequence of the fact that all these gases, above their critical
point temperatures, behave in accordance with the gas law, namely
PV=nRT. This behaviour is completely independent of the nature of the
gas species and only subject to variations due to the non-ideal
behaviour of some gases. However, at the temperatures and pressures
used in acoustic decrepitation analyses, these variations from
ideallity are very small and do not affect the results at all.
To demonstrate this, I have used the modified Redlich & Kwong
equation of state to calculate the behaviour of CO2, CH4
and N2 at 2 different molar volumes using a computer program
from Holloway, 1980. The results, plotted below, show that these
3 gases behave similarly and that decrepitation of inclusions
containing any of these gases, or mixtures of these gases, will all
develop high internal pressures and decrepitate at low temperatures, as
explained in the item: Why CO2 rich fluid
inclusions decrepitate at low temperatures. The small
differences between gases due to non-ideallity are of no consequence to
the acoustic decrepitation method.
Consequently, the acoustic
decrepitation method will work regardless of the presence of mixtures
of these gases or other gases above their critical
temperatures. The reason for using Molar Volume (the inverse of
density) in these calculations is that the gaseous components of fluid
inclusions formed at the same P-T conditions will have the same molar
volume, although their gas densities will differ. (This is a
consequence of the fact that 1 mole of any gas at STP occupies the same
volume.)