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HAL Id: jpa-00224333

https://hal.archives-ouvertes.fr/jpa-00224333

Submitted on 1 Jan 1984

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NEW PHASES AND CHEMICAL REACTIONS IN SOLID CO UNDER PRESSURE

R. Mills, D. Schiferl, A. Katz, B. Olinger

To cite this version:

R. Mills, D. Schiferl, A. Katz, B. Olinger. NEW PHASES AND CHEMICAL REACTIONS IN SOLID CO UNDER PRESSURE. Journal de Physique Colloques, 1984, 45 (C8), pp.C8-187-C8-190.

�10.1051/jphyscol:1984833�. �jpa-00224333�

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NEW P H A S E S A N D C H E M I C A L R E A C T I O N S IN S O L I D C O UNDER P R E S S U R E * R.L. Mills, D. Schiferl, A.I. Katz and B.W. Olinger

Los Alamos national Laboratory, Los Alamos, ISM 87545, U.S.A.

Résumé - Nous avons déterminé le diagramme de phase du monoxyde de carbone par diffraction des rayons X et spectroscople Raroan, de 15 â 297 K et i des pressions de 1.0 â 10.0 GPa. A basse température et au voisinage de 3.4 GPa, la phase connue a (groupe d'espace P2]3) se transforme en une phase nouvelle G (de structure Inconnue), au lieu de la phase prévue t (PAj/renra).

Nous avons trouvé une transformation de C0 - $ (groupe d'espace P&3/ramc) en une phase nouvelle i (Pm3n), au voisinage de 5.2 GPa, à la température ambiante. Au-dessus de 4.6 GPa et 80 K, environ, lorsque Irradié par lumière visible laser, C0 subit une réaction photochimique. Cette ten- dance à réagir peut être associée avec la formation d'un polymère jaune qui subsiste jusqu' à" pression nulle. Des mesures ESCA Indiquent que le poly- mère est composé de sous-oxyde de carbone ^ ( ^ x -

Abstract - The phase diagram of solid carbon monoxide was determined by x-ray diffraction and Raman spectroscopy from 15 to 297 K at pressures from 1.0 to 10.0 GPa. At low temperature a transition occurs near 3.4 GPa from the known a-phase (space group P2i3) to a new c-phase (structure unknown), rather than to the predicted ir-phase (P42/mnm). A transformation from p-CO (space group P63/mmc) Into a new 4-phase (Pm3ti) was found near 5.2 GPa at room temperature. Above about 4.6 GPa and 80 K, CO reacts photochemically when irradiated with visible laser light. The photoreac- tlvlty may be associated with the formation of a yellow polymer, which can be recovered at zero pressure. ESCA measurements Indicate that the polymer Is composed of carbon suboxide (C3Q2)x*

I. INTRODUCTION

The gases CO and N? are close molecular analogues. At low pressure they condense Into liquids with almost identical molar volumes and freeze Into solids with simi- lar crystal structures. Recently [1] the phase diagram of t*2 was determined by Raman spectroscopy from 16 to 300 K at pressures to 52 GPa. The present study was carried out to establish the P-T diagram of the solid phases of CO over the range 15-300 K and 1.0 - 10.0 GPa using x-ray diffraction and Raman spectroscopy. Al- though we find similarities in the physical structures of the high-pressure forms of solid CO and N;, there are striking differences in chemical behavior. Above about 4.6 GPa and 80 K, CO forms a yellow solid that can be recovered at zero pres- sure. Chemical analysis Indicates that the solid may be a mixture of (C302)

x

and other products resulting from chemical dlsproportionation [2].

II. EXPERIMENTAL APPARATUS AND PROCEDURE

Raman spectra were measured in a Merrlll-Bassett [3] cell, loaded with 99.95% pure liquid CO by the indium-dam technique [4]. Cell temperatures from 15 to 300 K were controlled to + 1 K by a helium-flow eryostat. We calculated pressures using the frequency shift of laser-induced fluorescence from ruby powder In the cell [1,5,6].

Both the ruby fluorescence and Raman spectra were measured with a Spex 1403 spec- trometer using K r

+

15454-cm

-1

laser radiation.

*Although this paper was not actually presented at this session, it was sent for re- view prior to the Meeting and recommended for publication by the Conference Committee.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1984833

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C8-188

JOURNAL

DE PHYSIQUE

Our x-ray studies of solid CO were carried out in a Be gasket clamped between tungsten-carbide anvils in a hydraulic press [l]. A collimated beam of Cu

KQ

radiation was directed through the gasket, and the diffracted x rays were photo- graphed with a 114.6-mn diam. powder camera. W e attained temperatures between 1 0 0 and 300

K

by circulating liquid nitrogen through the press platens. Pressures were determined from diffraction lines of in situ NaF, the compression of which is known from shockwave experiments [a].

In order t o synthesize a sufficient amount of CO-disproportionation product for chemical analysis, we modified the x-ray apparatus by incorporating a larger volume gasket ( ~ 0 . 5 mn3) made of BeCu, stainless steel, or Inconel. The anvils and gasket were also enclosed by a metal bellows, equipped with a capillary line and sealed against the platens with indium rings. This arrangement allowed the gasket to be filled with liquid CO before pressurization and t o be emptied into a mass spectrometer for analysis of product after pressurization. Pressures were applied for up t o 1 0 0 h, while the platens and cell were electrically heated t o 345 K.

111. RESULTS AND DISCUSSION

Raman spectra, characteristic of the vibron regions of

a-,

p-,

6-,

and c-CO and of the lattice-mode regions of a-CO and C-CO, along with the Raman frequencies as a function of pressure have already been published 121. From our present extension of this work we can now construct t h e phase diagram for CO. shown in Fig. 1. The open symbols represent Raman observations and the closed ones represent corroberat- ing x-ray data. Coincident symbols in Fig. 1 signify phase boundaries. The space groups of the various crystal phases have been reported as a-CO (P213) [93, p-CO (P63/mnc) [10,11], and a-CO (Pm3n) [2]. Our results confirm these structures. The

Q,

p, and

6

forms have analogues in the N2 phase diagram [I], which exhibits an additional

y

phase (P42/mnm) [12,13], not seen in CO, possibly because of its much larger quadrupole interaction energy [14].

Our calculated and observed interplanar spacings, and observed intensities for c-CO at 6.9 GPa and 1 0 0

K

are given in Table I. The diffraction pattern can be indexed as rhombohedral with a = 5.96 A and

a =

85.1°. If it is assumed that there are eight CO molecules per primitive unit cell, the molar volume has the reasonable value 16.0 cm3. The structure appears t o be a small rhombohedral distortion of cubic 6-CO (Pm3n). The three strongest diffraction lines in the cubic (Pm3n) structure of 6-CO o r 6-N2 are the (ZOO), (201). and (211), while the other low- index powder diffraction lines are unobservable. This situation carrjgs over t o rhombohedra1 C-CO where the (200); (201), (201); (211). (211). and (211) are the first strong lines. The space group cannot be uniquely determined from the present data, but it is most likely R3c if the molecules exhJbit head-to-tail order or R3c

if they are disordered.

Table I. Calculated and observed interplanar spacings and reflected intensities for C-CO at 6.9 GPa and 100 K.

hkl

(

rhomb.

)

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Fig. 1. Phase diagram o f condensed

CO.

Open symbols, Raman observations;

closed symbols, x-ray determinations; c i r c l e , a-CO (P213);

hexagon, $-CO (P63/mnc); square, 8-CO (Pm3n); t r i a n g l e ,

C-CO

( R ~ c ) ? ; s o l i d l i n e , e s t a b l i s h e d phase l i n e ; dashed l i n e , estimated phase l i n e ; cross hatch, r e g i o n where b o t h B-CO and a-CO were observed. Coincident p o i n t s i n d i c a t e c o e x i s t i n g phases.

When CO i s pressurized above about 4.6 GPa a t temperatures g r e a t e r than 80 K, chem- i c a l d i s p r o p o r t i o n a t i o n can occur. r e s u l t i n g i n a s o l i d product t h a t p e r s i s t s when t h e pressure i s removed. I n d u c t i o n o f t h e chemical r e a c t i o n depends on tempera- t u r e , elapsed time, and exposure t o v i s i b l e l a s e r l i g h t o r x rays. These f a c t o r s a l s o a f f e c t t h e c o l o r o f t h e s o l i d , which v a r i e s from l i g h t y e l l o w t o dark red, and i t s consistency, which v a r i e s from f i n e - g r a i n e d t o caramel-like. A l l o f t h e sam- p l e s appeared q u i t e porous and, indeed, t h e t o t a l amount o f s o l i d produced c o r r e - sponded t o o n l y about 5-10% o f t h e i n i t i a l

CO

charge. The s o l i d samples were solu- b l e i n water, acetone, and a l c o h o l and were degraded by a i r and l i g h t .

ESCA ( E l e c t r o n Spectroscopy f o r Chemical Analysis) measurements showed t h a t t h e s o l i d product contained carboxylated carbon atoms and g r a p h i t i c carbon atoms. On t h i s basis, and from t h e s i m i l a r i t y o f o u r product t o poly-carbon-suboxide ( C 3 0 ~ ) ~ prepared chemically a t 1 bar [15-191, we b e l i e v e t h a t we have synthesized t h i s m a t e r i a l from

CO

alone under pressure. It was f i r s t assumed t h a t

CO

might undergo chemical d i s p r o p o r t i o n a t i o n i n t h e pressure c e l l according t o

4

CO +

P C3O2 + C02,

and ( 1 )

X

c302

+

(C302)x - (2)

However, mass spectrometric a n a l y s i s o f t h e gas released from t h e c e l l a f t e r pres-

s u r i z a t i o n showed o n l y unreacted

CO,

w i t h no t r a c e o f C02. Furthermore, x-ray

d i f f r a c t i o n photographs o f t h e s o l i d gave a sharp p a t t e r n which must be associated

w i t h a second, c r y s t a l l i n e product.

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C8-190

J O U R N A L D E PHYSIQUE

We now speculate t h a t t h e r e a c t i o n may proceed as 5

CO

P

+

C3O2

4.

C2O3

f o l l o w e d by p o l y m e r i z a t i o n o f C3O2 and p o s s i b l y by

where (C203)2 i s a dimer o f o x a l i c anhydride. A d d i t i o n a l s t u d i e s aimed a t measur- i n g f a r I R absorption, x-ray s t r u c t u r e , e l e c t r o n s p i n concentration, and decomposition products a r e c u r r e n t l y underway.

REFERENCES

[ 1 1 BUCHSBAUM, S., MILLS, R. L. and SCHIFERL, D., J. Phys. Chem. 88 (1984) 2522.

[ 21 KATZ, A. I., SCHIFERL, D. and MILLS, R. L., J. Phys. Chem. 88 (1984) 3176.

[ 31 MERRILL. L. and BASSETT. W. A., Rev. Sci. Instrum. 45 (1974) 290.

[ 41 MILLS. R. L., LIEBENBERG. D. H.. BRONSON.

J. C. and

SCHMIDT,

L. C.,

Rev.

S c i . Instrum. 2 (1981) 891.

[ 53 FORMAN, R. A., PIERMARINI,

G.

J., BARNETT, J. D. and BLOCK, S., Science 176

(1972) 284.

[ 61 BARNETT, J. D.. BLOCK. S. and PIERMARINI, 6. J., Rev. Sci. Instrum. fi

(1973) 1.

[ 73 OLINGER, B. W.. MILLS, R. L. and ROOF, R. B.. J. Chem. Phys., t o be published.

[ B] CARTER, W. J . . High-Temp. High-Press. 5 (1973) 313.

[ 93 ANDERSON, A., SUN, T. S. and DONKERSLOOT, M.

C.

A., Can. J. Phys. 48 (1970) 2265.

[ I 0 1 VEGARD, L., Z. Phys. 88 (1934) 235.

[ll] CRDMER, D. T., SCHIFERL, D., LESAR, R. and MILLS, R. L.. Acta Cryst. C 39

(1983) 1146.

1123 MILLS, R. L. and SCHUCH, A. F., Phys. Rev. L e t t . 23 (1969) 1154.

[13] SCHUCH, A. F. and MILLS, R. L., J. Chem. Phys. 52 (1970) 6000.

1141 RAICH, J.

C.

and MILLS, R. L., J. Chem. Phys. 55 (1971) 1811.

[15] SMITH. R. N., YOUNG. D. A.. SMITH, E. N. and CARTER. C.

C.,

Inorg. Chem. 2

(1963) 829.

[16] BLAKE. A. R., EELES, W. T. and JENNINGS, P. P., Trans. Far. Soc. @ (1964) 691.

1171 GELIUS. U., ALLAN, C. J., ALLISON, D. A., SIEGBAHN. H. and SIEGBAHN, K., Chem. Phys. L e t t . 11 (1971) 224.

[ I 8 1 SNOW, A. W., HAUBENSTOCK, H. and YANG, N.-L., Macromolecules 11 (1978) 77.

[19] YANG, N.-L., SNOW, A. and HAUBENSTOCK, H., Polymer P r e p r i n t s 22 (1981) 52.

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