F. Cataldo, V. Kanazirev / Polyhedron 62 (2013) 42–50
43
still the possibility of mercury diacetylide or mercury alkynides
formation under given process conditions. Therefore, there is the
need to know better the safety and the explosive properties posed
by these organomercury compounds.
at room temperature. The yellow–white powder obtained the next
day was used for further characterization by infrared spectroscopy
and DSC thermal analysis.
A number of mercury aryl- and alkylacetylides have been well
studied since they were employed for the isolation and identifica-
tion of alkynes before the advent of the spectroscopy for the same
purposes [18–23]. Mercury alkynides have also been used to syn-
thesize other organomercury compounds and to study the relative
reaction kinetics [24–27]. There are also reports about the hazards
in handling such compounds [28]. For example, the bis(alkynyl)
mercurial (i-Pr–C„C)2Hg was found to be easily explosive [28]
and the hazard in handling copper and silver acetylides was as-
sessed very recently [7,29].
It is important to underline that the research on transition
metal acetylides is flourishing as demonstrated by the very recent
review on homoleptic acetylides [30], which also include mercury-
based derivatives. The interest in complex metal acetylides resides
in the potential application of these species as luminescent mate-
rials or as molecular components in microelectronics [31–34].
Thus, assessing the potential hazard in handling metal alkynides
is very important as a necessary step in any application. In the
present work we are focusing on the simplest mercury alkynide:
mercury diacetylide.
2.2. Synthesis of mercury diacetylide Hg(C„C–H)2 from HgCI2
Mercury dichloride (HgCl2, 650 mg) was completely dissolved
by stirring in 35 ml of distilled water inside a gas washing bottle.
The pH of the resulting solution was 4.5. The passage of a stream
of acetylene did not produce any precipitate. 4.5 g of KI were then
added in one shot. The precipitation of red HgI2 was briefly ob-
served before it dissolved quickly in the excess KI, yielding a trans-
parent and homogeneous solution. The pH of this solution was 7.0,
neutral. A stream of acetylene was then passed through this solu-
tion, but once again no precipitate formation was observed. 50 mg
of sodium hydroxide (NaOH) were then dissolved into the solution
and acetylene was again passed through the solution, yielding an
abundant precipitate of mercury diacetylide. The precipitate was
collected and washed as described in the previous Section 2.1;
the diacetylide yield was about 410 mg.
3. Results and discussion
3.1. Properties, infrared and UV spectra of mercury acetylide
2. Experimental
As mentioned in the introduction, mercury diacetylide was re-
ported in the old literature at the end of the 19th and at the begin-
ning of the 20th century. We have selected the most effective
experimental conditions which are known to produce mercury
diacetylide. These conditions require the use of complex mercury
HgI2 and HgCl2 were purchased from Sigma–Aldrich and used
as received. All the other reagents and solvents were analytical
grade materials obtained from Sigma–Aldrich or from Fluka. The
FT-IR spectra were recorded on a Nicolet 6700 spectrometer from
Thermo-Scientific. The mid infrared spectra were recorded in the
transmittance mode with the samples embedded in a KBr pellet
or in the reflectance mode using a ZnSe crystal and a horizontal
attenuated total reflectance attachment. The far infrared spectra
were obtained on the same spectrometer using the samples in
CsI pellets. The thermogravimetric analysis of the samples was per-
formed on a Linseis TGA model L-81 + DTA at a heating rate of
10 °C/min under a nitrogen flow (20 L/h). The combined TGA–FT-
IR analysis was performed by connecting the TGA apparatus with
a transfer line to the FT-IR gas cell of 10 cm path length and
equipped with BaF2 windows. The differential scanning calorime-
try (DSC) study was performed on a Mettler-Toledo DSC-1 Star
System. Different heating rates were used, as stated in the text,
and the samples were heated under a nitrogen flow of 3 L/h using
either a conventional aluminum pan with a hole or completely
sealed medium pressure stainless steel crucibles. In both cases
the sample size was 5 mg.
2ꢀ
salts, such as HgI4 and Hg(CN)42ꢀ, in a weakly alkaline medium
[13–15]. The passage of acetylene through such solutions causes
the formation of
a white–yellow precipitate described as
(–Hg–C„C–)x by Aylett [14], suggesting a polymeric nature to this
compound, which is reported to be insoluble in any common sol-
vent, has a density of 5.3 g/ml and is explosive.
In Section 2.1 we have produced a whitish precipitate by pass-
ing acetylene through an alkaline solution of K2HgI2 and in
Section 2.2 it was shown that a mercury diacetylide precipitate
occurs only when NaOH was added to the solution (basic condi-
tions). Neither passing acetylene through a slightly acidic solution
of HgCl2 nor through a derived solution of K2HgI2 prepared by add-
ing KI in excess to HgCl2 resulted in Hg diacetylide.
The chemical structure of mercury diacetylide can be easily
understood from its FT-IR spectrum, reported in Fig. 1. The spec-
trum shows a very sharp and clear acetylenic H–C„C– stretching
at 3280 cmꢀ1, while the bending of the same moiety occurs at
670 and 637 cmꢀ1. On the other hand the triple bond stretching
2.1. Synthesis of mercury diacetylide Hg(C„C–H)2 from HgI2
is located at 2013 cmꢀ1
.
Concerning the C–Hg–C bond stretching, literature [35] reports
the asymmetric stretching of the linear molecule dimethylmercury
at 538 cmꢀ1, the symmetric stretching at 515 cmꢀ1 and the bend-
ing at 160 cmꢀ1. In the case of diethylmercury, the asymmetric
Mercury diiodide (HgI2, 760 mg) was suspended by magnetic
stirring in 40 ml of distilled water and then potassium iodide (KI,
2.5 g) and potassium hydroxide (KOH, 186 mg) were added simul-
taneously under stirring. There was a gradual dissolution of HgI2,
which otherwise is insoluble. Once the solution was homogeneous,
it was transferred into a gas washing bottle and acetylene was bub-
bled with continuous magnetic stirring. Mercury diacetylide
started to precipitate immediately as soon as acetylene was passed
into the solution. The precipitate was whitish-yellow and could be
collected by filtration through filter paper, grade ‘‘Analitica A’’.
Once the filtration was completed, the filtrate was washed twice
with distilled water and then dried in air. The total yield was
380 mg. About 20 mg of the wet mercury diacetylide were trans-
ferred with a spatula into a small agate mortar to dry overnight
C–Hg–C stretching occurs at 515 cmꢀ1
, the symmetric at
488 cmꢀ1 and the skeletal bending Hg–C@C at 267 cmꢀ1, while
the C–Hg–C bending appears at 140 cmꢀ1. The C–Hg–C bond
stretching in divinylmercury H2C@CH–Hg–HC@CH2 occurs at 541
and 513 cmꢀ1. Since for the elements P and Ge the passage from
the divinyl derivatives to the diethynyl derivatives implies a shift
to lower wavenumbers of the carbon–metal stretching band by
Dm
= 70 to 80 cmꢀ1 [35], the asymmetric C–Hg–C bond stretching
in mercury diacetylide is expected at 464 cmꢀ1 and the symmetric
stretching at 435 cmꢀ1, as indeed is seen in Fig. 1. The other three
bands in the far infrared portion of the spectrum of Fig. 1 are