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NUCLEAR HYPERFINE INTERACTION OF Fe IN CHLORO-HEMIN

R. Sharma, P. Mastoris

To cite this version:

R. Sharma, P. Mastoris. NUCLEAR HYPERFINE INTERACTION OF Fe IN CHLORO-HEMIN.

Journal de Physique Colloques, 1974, 35 (C6), pp.C6-359-C6-361. �10.1051/jphyscol:1974664�. �jpa- 00215821�

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JOURNAL DE PHYSIQUE Colloque C6, suppliment au no 12, Tome 35, Dtcembre 1974, page C6-359

NUCLEAR HYPERFINE INTERACTION OF Fe IN CHLORO-HEMIN

R. R. SHARMA

Department of Physics, University of Illinois, Chicago 911, U. S. A.

and

Theoretical Physics Division

Atomic Energy Research Establishment, Harwell, Oxfordshire, OX1 1 ORA, England and

P. MASTORIS (*)

Department of Physics, University of Illinois, Chicago 911, U. S. A.

Resume. - L'klatement nucleaire hyperfin de I'ion ferrique dans la chlorohemine a Bte 6tudiC theoriquement en calculant le gradient de champ Clectrique au noyau de fer ii l'aide d'orbitales moleculaires multielectroniques construites dans le cadre des atomes qui se recouvrent. On montre que pour arriver aux principales contributions il faut considber dans notre cas au moins les C1- voisins, quatre aiomes N et les huit atomes C les plus proches. La distorsion de la distribution de la charge du fer provient principalement des ligands chlore. La distorsion due aux atomes d'azote voisins produit des effets comparables et annule partiellement la contribution du chlore. Utilisant les donnees structurales de RX de Koenig, on a calcul6 l'klatement hyperfin nucleaire du fer dansla chlorohc5mine dfi aux effets de recouvrement et on a trouvb

+

0,44 mm/s ; le signe est correct et la valeur reprhente environ 57 % de la valeur exptrimentale,

+

0,78 mm/s, observk par Johnson, Gonser et Grant, Shulman et Wertheim.

Notre calcul montre que le recouvrement dii aux electrons 2pz des C les plus proches produit des effets importants sur l'kclatement hyperfin du fer. Ceci rkvele qu'il existe un fort lien direct entre l'ion fer et les plus proches C dans la chlorohemine. Les effets des dipoles induits sur le chlore et les azotes ont aussi 6t6 etudits par des mkthodes autocoherentes. En tenant compte de ces effets, l'kclate- ment est rtduit a

+

0,14 mrnls, si l'on prend pour la polarisation de C1- une valeur aussi 6levk que 2,9783. Par contre avec une faible polarisation de C1- (1 8 9 , la valeur calculk est remarquablement amelioree et devient

+

0,79 rnm/s, en accord avec les experiences.

Abstract. - The nuclear hyperfine splitting of ferric iron in chloro-hemin has been studied theoretically by estimating the electric field-griidient at the iron nucleus employing the multi-electron molecular orbitals constructed in the frame-work of the overlapping atoms. It is shown that one must take into account as least the neighbouring C1-, four N's and eight nearest C's in our case to arrive at the most dominant contributions. The distortion ofthe iron charge distribution due to the chlorine ligand has been found to produce the dominant effect. The distortion due to the neighbour- ing nitrogen atoms produce comparable effects and partly nullify the chlorine contribution. Using the Koenig's X-ray structure data, the calculated nuclear hyperfine splitting of Fe in chloro-hemin due to the overlap effects has been obtained to be

+

0.44 mm/s which is of correct sign and about 57 per cent of the experimental value

+

0.78 mm/s as observed by Johnson, Gonser and Grant, and Shulman and Wertheim.

Our calculations show that the overlap due to the 2pz electrons of the nearest C's produce impor- tant effects on the hyperfine splitting of Fe. This reveals that there exists a strong direct link between the iron ion and the nearest C's in chloro-hemin. The effects of the induced dipoles at chlorine and nitrogens have also been investigated by self-consistent methods. Inclusion of these effects reduce the splitting to

+

0.14 mm/s if the polarizability of Cl- is taken to be as large as 2.97 8 3whereas it improves the result drastically to

+

0.79 mm/s, in agreement with the experiments, if the polariza- bility of C1- is assumed to be small (1 83).

Hemoglobins and the related compounds have [l-81. Weissbluth and Maling [6] have interpreted the recently been studied extensively by several groups Mossbauer spectra of several derivatives of hemoglo- bin t o understand the qualitative features of the qua-

(*) Formerly P. Moutsos. drupole splitting. The theoretical investigation for the

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1974664

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C6-360 R. R. SHARMA asymmetry of the Mossbauer spectrum in chloro-

hemin has been investigated by Blume [2] and the Mossbauer isomer shift has been studied by Moutsos, Adams and Sharma

[a].

The calculations of the nuclear hyperfine splitting of Fe in chloro-hemin has been made by Han, Rettig, Ikenberry and Das [7] using the extended Hiickel approximation. The hyperfine splitting, calculated by Han et al., has been found to be of opposite sign compared to the experimental result [3-51 and thus require further theoretical study.

We intend to inform an estimate of the nuclear hyperfine splittings of Fe5'" in chlorohemin by extend- ing the method used by one of us [9, 101 for evaluat- ing the electric field-gradients(EFGs) in nonmetals. The multi-electron wave functions have been constructed in accordance with the Hund-Mulliken-Van Vleck [I I ] molecular orbital linear combination of the atomic orbitals involving overlap effects. The case of hemin is difficult in the sense that many more atoms (and electrons) surrounding the Fe are required to be taken into account than just the ligands to obtain the molecular orbitals. We show that the calculated splitting due to the overlap effects is of right sign and right order of magnitude in view of the experimental observations made by Johnson [3], Gonser and Grants [4] and Shulman and Wertheim [5].

The susceptibility and paramagnetic resonance mea- surements [12] have established that the Fe3+ ion in chloro-hemin carries the high spin S =

3.

This directs us to take the ls2, 2s2, 2p6, 3s2, 3p6, 3d5 electrons on the Fe3+ ion in forming the molecular orbitals. Also, we take 3s2 and 3p6 orbitals of C1-, 2s2 and 2p3 orbitals of N and 2s2 and 2p2 orbitals of C in the linear combination of atomic orbitals to construct the mole- cular orbitals. As will be clear later, it is required to take account of only the neighbouring C1-, four N's and eight nearest C's in our case to obtain the most important contributions. The one-electron molecular orbitals $i are the antibonding (ab) and bonding (b) orbitals given by [9, 101

where a designates the quantum numbers n' L' M' of Fe3 + orbitals and P(g) the quantum numbers nLM of the orbitals of the neighbouring atoms located at the site g. The parameters Sg,B(s),a are the matrix elements

< xgJc!

1

$2 >

and Na is the normalization constant.

Form~ng the many-electron wavefunction in the Hartree-Fock approximation as a Slater determinant of one electron molecular orbitals, the EFG due to the electrons is given by

q,, = e

1

zi

<

$i

1

(3 cos2 Oi - 1)lr;

1

I(/i

>

(2)

i

where e is the electron charge (including sign) and zi is the number of electrons in the molecular orbital $i.

Incorporating the effects of the Sternheimer shielding

and taking account of the charges on the nuclei of the surrounding atoms under consideration, the total contribution to the EFG (denoted by q) may be written as 19, 10, 131

where (1 - R) and (1 - y,) are the Sternheimer shielding factors ; q;, q:, and q: are the (( local D, non- local n and (( distant )) contributions arising from the antibonding orbitals whereas qib is the (distant) contri- bution due to the bonding orbitals ; q6 is the contribution from the nuclei of the surrounding atoms under consi- deration. The expressions for q;, etc., in eq. (3) are similar to those obtained in ref, [13] except that they are more involved since many more atoms contribute to the results than just the nearest neighbours.

As for the calculations we have restricted (as mentioned above) the surrounding atoms to the C1-, the four N's and the eight nearest C's in order that the caIculations remain manageable and still give the dominant contributions. The required atomic wave- functions of Fe3 +, C1-, N and C taken for our calcula- tions are those of Clementi [14]. The overlap and two- center integrals involved in the local, etc., expressions are evaluated by making use of a general expression [15]

of the Lowdins a-function.

The calculated EFG components have been tabu- lated in Table I using the X-ray structure parameters of Koenig [16] ; the contributions arising from various Fe-orbitals are separately shown (whenever possible) for the four neighbouring N's, Cl- and eight nearest C's for the purposes of comparison. The most domi- nant contribution comes from the N's, next from CI- and from C's. Other atoms in hemin are farther away and give only a small contribution.

Taking 1-R=0.68 [17] and 1-y,=lOxl4 [la], we obtain the total EFG as q = f7.189 x 1014 esu which yields the quadrupole splitting

(using Q =

+

0.20 [SO] b for Fe) which is of correct sign and about 57 per cent of the experimental result [3-51

+

0.78 f 0.03 mm/s. Our results may also be compared with the previously calculated value [7]

using the extended Hiickel approximation Consi- dering the approximate nature of our starting wave- functions, the agreement with the experiment is remarkably good. Our rough estimates indicate that further improvements may be made if one also includes the contributions from the other neighbouring atoms.

Since in hemin the iron is in the state Fe3+ and the chlorine in the state C1- it is expected that these ions will induce the polarizations in the system. Thus, it is worthwhile to consider the effects of the induced

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NUCLEAR HYPERFINE INTERACTION OF Fe IN CHLORO-HEMIN C6-361

dipoles at C1- and nearest nitrogens no the electric field-gradient at iron. We use the self consistent method of calculating [I91 the induced dipoles on C1- and four nitrogens neglecting the induced dipoles on the remaining atoms. We find that for the polariza- bility values, a(N) = 1.13

A3

and a(CIF) = 2.97

A3

the splitting reduces to

+

0.14 mm/s, retaining the correct sign. If, however, a(C1-) is taken as 1

A3

while keeping a ( N ) constant (1.13

A3)

one obtains the splitting as

+

0.79 mm/s, in agreement with the experimental value. Though it is difficult to say what value of a(C1-) is appropriate for hemin, it looks that the value 2.97

A3

for a(ClP) is somewhat large and, therefore, good agreement with the reduced value of u(C1-) is encouraging.

Precise analysis of our results reveal that the distant

{( ati-bonding )) component of the field-gradient arising from nearest C's in hemin yield important contribution to the quadrupole splitting of Fe. This is interpreted as an evidence of a strong direct link between the iron ion and the neatest carbons in chloro-hemin.

It is important to remark that the effect of the 3p-orbitals of Fe is dominant (see Table I). In the previous calculations of EFG by Han et al. [7] in hemin such contributions gave zero result since the 3p-orbitals were isotropic in their model. We expect that our results will give impetus to the more detailed molecular orbital calculations (such as self-consistent Hartree-Fock calculations) in which the particular

emphasis will be placed on including the effects of 3p-iron orbitals.

Various separated electric-field-gradient components (in 1014 esu) at Fe-site in hemin due to the neighbouring four N's, C1- and the nearest eight C's. (( Primes )) denote the components without shielding effects. The total eZectric-jieZd-gradient q (in 1014 esu) is also given.

Field-gradient Fe-

Components orbital N C1- C

- - - -

3d 1.313 -0.664 0.171

4 ; 3p 21.755 -13.964 3.458

2~ 0.490 -0.344 0.082

q (total) 7.189

References

[l] GONSER, U., Proc. of the 2nd International Conference on the Mossbauer Effect, Ed. Cornpton, D . M. J, and Schoen, A. H. (John Wiley and Sons, 1962) p. 281 ;

EPSTEIN, L. M., J. Chem. Phys. 36 (1962) 2731 ;

GRANT, R. W., GONSER, U. and KREGZDE, J., Rev. Mod.

Phys. 56 N 12 (1964) 458 ;

BEARDEN, A. J., MOSS, T. H., CAUGHEY, W. S. and BEAU-

DREAU, C. A., Proc. Natl. Sci. U. S. 53 (1965) 1246 ; LANG, G. and MARSHALL, W., Proc. Phys. Soc. (London) 87

(1966) 3 ;

Moss, T., BEARDEN, A. J. and CAUGHEY, W. S., J. Chem.

Phys. 51 (1969) 2624.

[2] BLUME, M., Phys. Rev. Letters 18 (1967) 305.

[3] JOHNSON, C. E., Phys. Letters 21 (1966) 491.

[4] GONSER, U. and GRANTS, R. W., Bio. Phys. J. 5 (1967) 823.

[5] SHULMAN, R. G. and WERTHEIM, G. K., Rev. Mod. Phys. 36 (1964) 459.

[6] WEISSBLUTH, M. and MALING, J. E., J. Chem. Phys. 47 (1967) 4166.

[7] HAN, P. S., RETTIG, M. F., IKENBERRY, D . and DAS, T. P., Theoret. Chim. Acta (Berl.) 22 (1971) 261.

[8] Mou~sos, P., ADAMS, J., SHARMA, R. R., J. Chem. Phys. 60 (1974) 1447.

[9] SHARMA, R. R., Phys. Rev. Letters 25 (1970) 1622. See Also : TAYLOR, D . R., J. Chem. Phys. 48 (1968) 536 ;

SAWATZKY, G. A. and HUPKES, J., Phys. Rev. Letters 25 (1970) 100.

[lo] SHARMA, R. R., Phys. Rev. Letters 26 (1971) 563.

[ l l ] VAN VLECK, J. H., J. Chem. Phys. 3 (1935) 803,807.

[I21 PAULING, L. and CORYELL, C. D., Proc. Nut. Acad. Sci. 22 (1936) 159 ;

INGRAM, D . J. E. and BENNETT, J. E., Disc. Farad. Soc. 19 (1955) 140 ;

SCHOFFA, G., Nature 203 (1964) 640 ;

GRIFFITHS, J. S., Proc. Roy. Soc. A 235 (1956) 23.

[13] SHARMA, R. R., Phys. Rev. B 6 (1972) 4310.

[14] CLEMENTI, E., IBM J. Research Develop. 9 (1965) 2.

[I51 SHARMA, R. R., J. Math. Phys. 9 (1968) 505 ; LOWDIN, P. O., Advan. Phys. 5 (1956) 1.

[16] KOENIG, D. F., Acta Cryst. 18 (1965) 663.

[17] INGALLS, R., Phys. Rev. 133 (1964) A 787.

[18] STERNHEIMER, R. M., Phys. Rev. 130 (1963) 1423.

[19] SHARMA, R. R. and DAS, T. P., J. Chem. Phys. 41 (1964) 3581.

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