Pulse radiolysis of mercuric ion in aqueous solutions - The Journal of

Nov 1, 1973 - Shinichi Fujita, Hideo Horii, Setsuo Taniguchi. J. Phys. Chem. , 1973 ... Lisa Van Loon, Elizabeth Mader, and Susannah L. Scott. The Jou...
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S. Fujita, H. Horii, and S . Taniguchi

Pulse Radiolysis of Mercuric Ion in Aqueous Solutions S h i n ' i c h i F u j i t a , " H i d e a Horii, a n d Setsuo T a n i g u c h i Radiation Center of Osaka Prefecture, Shinke-cho, Sakai, Osaka, Japan Received May 23, 1973)

(Received January 24, 1973; Revised Manuscript

The pulse radiolysis method was used to study deaerated aqueous solutions of the mercuric ion in the wavelength range 220-300 nm. The transient mercurous ion gave two absorption maxima a t 225 and 250 nm with c255 = (1.4 f 0.1) X lo4 M - l sec-l. Stable mercurous ion, Hg22+, was formed uia an additional Hg+ HgO Hg(1I); HgO + step after the disproportionation reaction of the initial species: Hg+ Hg(I1) HgZ2+. The formation rate of HgZ2+ depended on the concentration of mercuric ion and the p H of the solution. The result was ascribed to the reaction of HgO with three partially hydrolyzed species of mercuric ion. Rate constants for the reactions were determined.

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Introduction The radiolysis of aqueous solutions of some metal ions gives various species in unstable valence states by the action of the transient primary products from water, such as OH radical, H radical, and hydrated electron. The technique of pulse radiolysis, as well known, is used to investigate the reaction processes of such short-lived species. By this method cadmium and zinc of group IIb metals have been investigated in detail; their monovalent states are strong reducers1 and show transient absorptions, due to charge transfer spectra, at about 310 nm.293 The chemistry of mercury differs from that of zinc and cadmium not only because of inherent peculiarities of the element but also because of the existence of the stable mercurous ion, HgZ2+, which is readily obtained by reduction of mercuric salts. According to H i g g i n ~ o n ,Hg22+ ~ dissociates to Hg+ at low concentrations and the absorption spectrum of the monomeric ion is entirely different from the charge transfer spectra for other group IIb metals. On the radiolysis of an aqueous solution of mercuric ion, the hydrated electron or H radical reduces the ion to form the mercurous ion. Recently, Faraggi and Amozig5 have reported that the transient Hg- shows an absorption maximum at 272 nm by the pulse technique. The present report sheds light on the chemical processes between stable and unstable mercurous ions by studies in the range 220-300 nm. The obtained spectrum of the transient species was fairly different from the result by Faraggi and Amozig. Another interesting result obtained is that the stable mercurous ion is produced by the bimolecular reaction of the zero-valent mercury with mercuric ion after disproportionation of the transient monovalent mercury. Experimental Section The electron beam was produced in a linear accelerator (High Voltage Engineering Co. ) giving 10-Mev electrons with a variable pulse width up to 5 psec; its peak current being about 0.4 A. The electron beam, spread by an aluminum plate 4 mm thick, entered the cell through a brass slit and fell on a brass collector. The current was monitored as voltage on a condenser with a digital voltmeter having a holding mechanism. The irradiation cell was 1.5 cm long, made of quartz having thermal end windows. The sample solution was reThe Journal of Physicai Chemistry, Vol. 77, No. 24, 1973

+

-

+

freshed from a Pyrex stock bottle of 0.5-1 1. by combination of argon and a magnetic valve. The analytical system consisted of a 150-W D2 lamp, three lenses, a mirror, a Bosch and Lomb grating monochrometer, and a 1P28 photomultiplier tube. This combination gave only a little scattered light of lower wavelength, which was about 5.5% a t 220 nm and less a t longer wavelength. The water used throughout this work was triply distilled. The aqueous solutions of mercuric ion were prepared from two sources: mercuric perchlorate and usually mercuric oxide with perchloric acid. The solutions were deaerated by bubbling with argon for longer than 2 hr. All materials were used without further purification from the commercial sources. Only nitrous oxide was specially ordered ( 0 2 < 0.1%). The determination of the concentration of mercuric ion was carried out spectrophotometrically as its EDTA complex in acidic solution a t 247 nm where the complex has an absorption maximum with 6 = (2.28 f 0.05) X lo3 M-1 cm -1. The dosimetry was carried out by means of 0.1 M KCNS solutions saturated with oxygen using the reported ~ - M - I cm-I and G = 2.8.6 value of C ~ ? ~ ( C N S=)7600 Results Pulse radiolysis of deaerated aqueous solutions of mercuric ion yielded a transient species, Hg+, with two absorption maxima a t 225 and 250 nm. Figure 1 shows the spectrum 2 psec after the pulse and its change with time in a 50 pM HgO solution at pH 4.3. The half-lives of the absorptions a t two peaks were identical within experimental errors and were inversely proportional to the initial absorption. Similar results were obtained in the solution of perchlorate salt. After the initial species has decayed, another absorption, which has a peak at 236 nm and can be assigned to a stable mercurous ion, HgZ2+, appears and reaches constancy within a few milliseconds. The permanent absorption was formed faster in solutions of higher concentration of mercuric ion or of lower pH. Figure 2 shows the typical synchroscopic traces of absorptions a t 236 nm. Decay of the initial species and formation of the stable mercurous ion are not simultaneous. Essentially similar results were obtained with the addition of tertbutyl alcohol, although the spectrum of its radical over-

Pulse Radiolysis 01 Mercuric Ion in Aqueous Solutions

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0.10

-

>. ._

F 0

m

-

E .'p 0.05

Figure 2. Synchroscapic lrace5 at 236 nm Obtained in a deaerated aqueous solution of 50 p M of mercuric ion. pH 4.3: pulse doses, 1420 rads/pulse; ordinates. 4.4%/cm for (a) and (b); abscissa, (a) 2Opsec/division. (b) 1 msec/division.

0

OM) 200

250

3 w

Wove l q t h ( n m ) Figure 1. Spectrum and its change with time after a pulse in a deaerated aqueous Solution of 50 pM HgO at pH 4.3: average 2 psec. (.....) 15 met, (-.-) dose, 2700 rads/pulse: (-) 50 psec. (-..-I 1550 psec. (--.I 500 psec. (- -) 3 msec.

lapped. However, little ahsorption appeared in the solution saturated with nitrous oxide. In a solution of 1 m M HgO a t pH 2 the spectrum of the transient species was similar t o that in Figure 1. However, the ahsorption yield of the transient a t a fixed dose increased markedly compared with that obtained in the solution of 50 p M at pH 4.3. Also in the presence of tert-butyl alcohol, the yield increased with increase in the concentration of HgZ+ up to a few millimoles per liter. The dependencies were similar 0 between the ahsorptions o f t h e transient at 255 nm and of 0 20 40 60 80 stable mercurous ion a t 236 nm. The contribution from tTime, psec BuOH radical to the observed ahsorption was negligible a t 255 nm.? Both yields reach constant values a t above 10 Figure 3. Test 01 second-order rate law for t h e decay 01 transient absorption at 255 nm in the presence 01 2 mM tert-butyl m M of mercuric ion. The Hg+ yield is reduced a t low conalcohol: ( 0 ) 1/D. 50 p M HgO at pH 4.3; dose, (upper) 1800 centrations of mercuric ion by the competion of H radical rads/pulse. (lower) 2800 rads/Pulse: ( 0 ) l/D', 1 mM HgO at recombination. Then, the product G values should he PH 2.0; dose. (upper) 1800 radslpulse. (lower) 2800 rads/ equal to that of H radical a t 10 m M mercuric ion. Taking pulse, where D' = D o ( D - D , ) / ( D o - D - ) . G(H) = 3.2, each molar extinction coefficient is calculated to he cZJ5(Hg+) = (1.4 i 0.1) x lo', ~ ~ 3 ~ ( H g = 2 ~ + TABLE ) I: Decay Rate Constants 01 Hgt in Solutions 01 50 pM (2.4 i 0.2) X M lWM-' cm-', where the molecular yield of HgO at pH 4.3 and 1 mM HgO at pH 2.0 with Various Hgz2+ is half of that OS the transient according to the stoiConcentrations 01 NaCIOI chiometrical relation. Figure 3 shows that the plots of ] / I ) us. time after the end of the pulse fall into a good linear line in a 50 p M HgO solution of pH 4.3. The slope of the lines equals 2 k l t l 4.3 50uM 0 3.9 f 0.2 5.2 f 0.5 where k is the second-order rate constant, t is the molar 0.15 5.1 f 0.2 extinction coefficient, and 1 is the light path length in the 2.0 1.0mM 0 3.9 f 0.3 4.9 f 0.5 irradiation cell. In a 1.0 m M HgO solution of pH 2.0, the 0.03 4.2 f 0.3 linearity was not as good due to the fast Sormation of sta0.08 4.8 f 0.3 ble mercurous ions. In this case, the results were improved by plotting I j D ' . where I)' = I I o ( l ) - I ) J / ( L k error and increases with increase in innic strength. 2ko in the last column shows the rate constant a t zero ionic Del. on an assumption that Hg+ ions recombine simultaneously to form Hgz2'. I)' represents the optical density strength. by plotting log 2h/t as a Sunction OS P " ~ / ( 1 + of the pure transient species. The improved slopes are also p l ' * ) , multiplied hyr. shown in Figure 3. Table I lists the results in hoth pH soThe formation of the stable mercurous inn oheyed the lutions containing various concentration of sodium perfirst-order rate law in the absence of tert-butyl alcohol, chlorates. The second-order rate of' decay OS the transient the radical of which was effective to snme extent in ahat each pH approximately equals within experimental sorption a t 236 nm. When the formatinn of Hgz2' was relThe J ~ u r n a l o l P h y ~ i c a ChemiSBy. l VoI. 77, No. 24. 1973

S. Fujita, H . Horii, and S.Taniguchi

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Rates of Formation of Hg*’+ at 236 n m , Abundance Ratios of the Mercuric Ion in the Three Hydrolyzed Forms, and the Resulting Rate Constants of the Respective Components

TABLE I I :

.~

Pt-

Rates of formation X 10-3sec-1

[HgOIza P M

4.0

59

3.5

36 16 36

3.6 f 0.3 2.5 f 0.2 1.2 f 0.1

5.9 f 0.5 2.5 f 0.2 6.8 f 0.7

15 3.0

16

01

P

r

0.67 =k 0.07

0.019

0.038

0.943

1.66 f 0.7

0.150

0.095

0.755

iz 0.4

0.588

0.118

0.298

kpH x

4.2

M - ’ sec-1

k, = 5.9 X lo8, k o = 5.0 X IO8, k, 5 5 X l o 7 A / - ’

sec-’

Corrected vaiues with consumption by eaq- and ti radical.

-1.5

-3.5

I - \



0

1 .0

0.5

T i m e , ms

Figure 4. First-order formation of Hg2*+ at 236 nm in the absence of tert-butyl alcohol, average dose, 1250 rads/pulse: ( @ ) 36 pM HgO at pH 4.0; ( 0 )36 gM HgO at pH 3.5; ( A ) 16 g M HgO at pH 3.0. atively slow. the linearity of the plots of log ( D , - D ) cs t was satisfactory in a considerable range of time except in a n earlier stage (Figure 4). The apparent rate of formation calculated from the slope appeared t o vary along an S-type curve against p H ( p K 3 . 5 ) in the 50 Ji4 HgO solution. Even a t this concentration, however, the linearities of the plots were poor a t low pH’s due to the fast formation of HgZ2+. Therefore, the rates at low pH’s were determined in the more diluted solutions of HgO. The results at three pH’s were listed in Table 11.

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Discussion In order to explain the appearance of the transient mercurous ion, the following reactions were taken into consideration, based on the scavenger effects. H,O --+ e,,-, H. OH, other stable products (1) eaq-

H e,-

OH

The unstable monovalent cations of some other metals have been reported to have charge transfer spectra a t about 300 nm.2y3 The transient mercurous ion seems to be unique in the spectrum and its large absorption coefficients a t the maxima. Our result of the absorption maximum is not consistent with Faraggi and A m ~ z i g They .~ have reported that the maximum is situated a t 272 nm. We have also obtained the same result in 1 mM mercuric perchlorate solution using a xenon lamp as the light s o u r ~ eThe . ~ difference might arise from the presence of much scattered light when the xenon lamp is used a t short wavelength settings of the monochromator. According to H i g g i n ~ o nHg+ , ~ has a n absorption spectrum rising monotonously from 250 nm to the shorter wavelength and its absorption coefficient is a t most 3 x 103 M - 1 cm-1 even a t 225 nm. The transient species observed here might be alternatively assigned to HgHZ-. which has been proposed in matrix experiments by esr,lO though the matrix is extremely acidic. However, the slope of the plots, ~ to be rather smaller log 2k us. p I i a ( 1 1 . ~ ~ ’ is~ )calculated than $1, even in the solution of p H 2.0. This result suggests t h a t the transient carries a single charge with it, based on the Debye-Bronsted theory. Thus, the transient may be assigned most likely to Hg+. The analysis of the second-order rate of decay is expected to be complicated because the absorption of HgZ2+ intervenes a t the rates according to the concentration of HgO and the pH of the solution. Thus, two simple conditions were chosen to determine the rate: (1) a solution of 50 piM HgO at pM 4.3, where the formation rate of HgZ2+ is slow (The pH (4.3) was chosen since the solution of mercuric perchlorate shows that the p H in that concentration would be due to hydrolysis.); (2) a solution of 1 m M HgO a t p H 2.0, where it would be assumed that HgZ2+ forms instantaneously after the transient has decayed. In this case, D’ was used instead of D (the apparent optical density), where D’ = Do(D - Dm)/(Do D m ) . Good agreement with the rates of decay between the two solutions suggests that the transient sbsorptions in both solutions originate from the same species, Hg+. In high pH solutions of HgQ the stable mercurous ion does not appear immediately after the decay of the transient as seen in Figure 1 and 2. However, it was concluded that the transient finally becomes Hg? after one or more steps, because both yields (transient Hg+ and Hgz2+) depended similarly on the concentration of mercuric ion. The dependencies can be interpreted by the competition of the reaction 311 with the recombination reaction of H radicals.12 Thus, the following reaction mechanism is assumed for the formation process of Hg22+. The transient may disproportionate to form zero valent mercury, HgO,

+

+

+ Hg(I1) + Hg(I1)

N,O

t-BuOH

-+

-+

--j

Hg’

(2)

Hg’

(3 )

+

X2 OH f OHt-BuOH radical H,O

+

(4)

(5)

In p H 2 solutions reaction 3 plays the important part. since eaq- reacts with H- to form the H radical. ea“- -t H’ -+ H (6) The reaction of the H radical with t-BuOH can be neglected. * In the absence of t-BuOH most of the OH radicals must be consumed by their recombination reaction; some would oxidize the transient. The Journal of Physical Chemistry, Voi. 77, No. 24, 1973

+

Pulse Radiolysis of Mercuric i o n in Aqueous Solutions

and mercuric ion. Later, HgO may react with Hg(I1) to form the stable mercurous ion. HgO

+

Hg(I1)

(7)

*

Hg,2+

(8)

Hgo

2Hg'

--+

+

Hg(I1)

Equation 8 is a well-known equilibrium reaction (log K8 = 1.92 at 25")l3 when an aqueous solution of mercuric ion contacts with liquid mercury. Further support of the mechanism is presented by two facts of the formation rate of HgZz+: the p H dependency and the linear proprotionality to the concentration of mercuric ion (Table 11). It should be noted that the formation rate is not shown correctly at the low pH region since it becomes fast and the apparent rate is affected by the decay of the transient. Therefore, the values obtained in more diluted solutions are listed in Table 11. The pH dependency of the formation rate may come from the fact that Hg(I1) has three conjugate forms, according to the pH.14 Hg2+

K, Kb 7 HgOH' -H+-

Hg(OH),

+

[HgOH']

-I- [Hg(OH),I = ( a + P + Y)[H~(II)IT

then, d [ H g 3 + ] / d t = ( k o a + k s p + k,-y)[Hg(II)]TIHgo]. The apparent rate constant of formation of Hgzz+ at a given pH value, k p H , is expressed as

k,PH = k,&

+

kaP

+

H

+

Hg,'+

--+

Hg,'

+ H+

(10)

A small part of the H radicals or hydrated electrons might be able to react with the product, Hgzz+.

(9)

where K , = 10-3.7, Kb = 10-2.6. From equilibrium 9, the total concentration, [Hg(II)]T, is the sum of the three components [Hg(II)], = [Hg2+]

HgZ+ is also complexed with water molecules, The larger value of k , than that of kr is compatible with the general concept that a metal ion makes a more stable complex with a ligand having opposite charge. It is interesting that even Hg(0H)z reacts with HgO at such a rate, while dissolved mercuric oxide does not react with metallic mercury in a neutral solution. We are also studying neutral solutions by the pulse technique and find that Hg22f is not observed but a species having another spectrum is found just after the decay of a transient species. More detailed information will be expected from the successive investigation. Figure 1 also reveals that an absorption appears at 285 nm that reaches maximum in a few tens of psec after the pulse, and then decays. It may correspond to Hgz+ proposed by Faraggi, et aL5

k,Y

The respective rate constants for the three forms of Hg(I1) were resolved from the ternary simultaneous equations which are obtained from the values in Table 11. The abundance ratios ( a , p. and y) were calculated from K , and Kb a t the respective pH. All values used and the resulting rate constants are listed in Table 11. These results suggest that the rate is determined by the exchange process between a ligand and a mercury nucleus, considering that

References and Notes D. Meyerstein and W.A. Mulac, J. Phys. Chem., 72, 784 (1968). G. E. Adams, J. H. Baxendale. and J. W.Boag, Proc. Chem. SOC., 241 (1963). J . H. Baxendale, E. M. Fielden, and J. P. Keene, Proc. Roy. Soc., Ser. A, 286,320 (1965). W.C. Higginson, J. Chem. SOC.,1438 (1951). M. Faraggi and A. Amozig, Int. J. Radial. Phys. Chem., 4, 353 (1972). J. H. Baxendale, P. L. T. Bevan, and D. A. Scott, Trans. Faraday Soc., 64, 2389 (1968). (a) A. Appieby, G. Scholes, and M. Simic, J. Amer. Chem. Soc., 85, 3891 (1963); (b) J. Rabani, J. Phys. Chem., 66, 361 (1962); J. Chem. Phys., 37, 1865 (1962); (c) A. Appleby, J. Amer. Chem. Soc., 67, 1610 (1963). M. Simic, P. Neta, and E. Hayon, J. Phys. Chem., 73, 3794 (1969). S. Fujita, H. Horii, and S. Taniguchi, Proc. Congr. Radiat. Chem., 74th, 56 (1971). R . J . Booth, H. C. Starkie, and M. C. R . Symons, J. Chem. SOC.A, 3198 (1971). (a) E. Hayon and M. Moreau. J. Chim. Phys., 62, 391 (1965); (b) M. Faraggi and J. Desalos, Int. J. Radiat. Phys. Chem., 1, 335 (1969). M. S. Matheson, Radiat. Res. Suppl., 4, 1 (1964). H. L. Roberts, Advan. lnorg. Chem. Radiochem., 11,337 (1968). S. Hietanen and L. G. Sillen, Acta Chem. Scand., 6, 747 (1952).

The Journal of Physical Chemistry, Vol. 77, No. 24, 7973