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o (1993 ACTA PHYSICA POLONICA A o 1

oceeigs o e I Ieaioa Scoo o Mageism iałowiea 9

MAGEIC OM ACO MEASUEMES Y OAISE EUO SCAEIG AICAIO O EAY EMIO SUECOUCOS

K.-U. NEUMANN AND K.R.A. ZIEBECK

eame o ysics ougooug Uiesiy o ecoogy ougooug E11 3U Gea iai

e eeimea ecique o si oaise euo scaeig as use i mageic om aco measuemes is esee A ioucio o e ieeaio a e cacuaio o mageic om acos a magei- aio esiies is gie e eeimea ecique o euo scaeig eoy as aie o easic si oaise scaeig eeimes is iey iouce e cacuaio o e mageic om aco a e mageia- io esiies ae cosiee o sime moe sysems suc as a coecio o ocaise mageic momes o a iiea eeco sysem e iscussio is iusae y a eeimea iesigaio o e mageic om aco i e eay emio suecoucos Ue13 a U3 Mageiaio esiy mas a mageic om acos ae esee a ei imicaios o oe ysica quaiies ae iey iscusse ACS umes 755+ 71+

1 Ioucio euo scaeig a i aicua si oaise euo scaeig is a oweu oo o e caaceiaio a iesigaio o ysica oeies o a aomic scae e cage euaiy a mageic ioe mome o e euo make i a iea oe o e iesigaio o mageic egees o eeom I aiio o usig euo scaeig o iesigaig eomea coece wi mageism (y eg esaisig e aue o mageicay oee saes eeimes may e eise o e caaceiaio o eais o eecoic wae ucios Suc a eeime is eaise we si oaise euos ae use o e eemiaio o e mageic om aco a o e mageiaio esiy Coay o secoscoic eciques wic ie eais o e wae ucio y a iesigaio o e eeimeay eemie ee sceme (eg e cysa ie ees o ocaise momes mageic om aco measuemes eee

(3 44 K.-U. Neumann, K.R.A. Ziebeck

to here are elastic measurements and therefore these measurements do not involve an energy transfer between and target. Consequently this method does not yield direct information on the energy eigenvalues of the Hamiltonian, that is the energy levels or band structure of the system under investigation. Instead a magnetic form factor investigation can be classified as an investigation of the real space properties of some electronic wave functions. This point will be discussed more fully below, and a clarification will be given as to what exactly is meant by "some electronic wave functions". The investigation of the magnetic form factor by spin polarised neutron scattering is therefore complementary to experiments such as de Haas—van Alphen measurements, which investigate the details in momentum space of energy levels and the Fermi surface. In order to be able to fully appreciate the potential of spin polarised neu- tron scattering for the investigation of magnetization densities and magnetic form factors a brief introduction is given to the experimental technique. First, the basic principles are reviewed of elastic nuclear and magnetic scattering, and a derivation is given for the description of a magnetic form factor measurement. Two simple models, a localised moment system and an itinerant model, are consid- ered, and for each of these model systems a magnetic form factor experiment is analysed. In the second section the theory is illustrated using the results of an ex- perimental investigation. A magnetic form factor measurement is considered which was carried out on the heavy fermion compounds UBe1 3 and UPt3. The exper- imental magnetization densities and form factors are presented and discussed in relation to the simple model systems mentioned above. Some consequences of the experimental findings are briefly discussed.

2. Mnt fr ftr rnt

Magnetic form factor measurements are usually carried out on single crystals employing spin polarised . The discussion here will be limited to the case of a paramagnetic material with a crystallographic structure which has a centre of inversion symmetry. An experimental determination of the magnetic form factor comprises of two different measurements. By using unpolarised neutrons, a first experiment establishes the details of the nuclear structure of the crystal under investigation. In a second experiment and by using spin polarised neutrons a quantity known as the flipping ratio is determined for a number of Bragg reflections. In order to establish the details of the nuclear structure it is important to carry out both experiments on the same single crystal and preferably also at the same temperature. The nuclear structure is determined by measuring the inte- grated intensity of Bragg reflections. A subsequent refinement of a crystallographic model and its comparison with the measured Bragg intensities is used to establish important parameters such as lattice site occupations and temperature factors. In this way the nuclear is determined precisely. In a second experiment the Bragg reflection is measured using spin polarised neutrons and with the crystal in an external magnetic field. Due to the presence of a magnetic field a ferromagnetic moment is induced in the paramagnet. As a result of Magnetic Form Factor Measurements ... 45 the induced ferromagnetic order magnetic Bragg scattering occurs. The magnetic scattering arises in addition to nuclear scattering. As both the magnetic and the nuclear unit cell have the same dimensions, magnetic and nuclear Bragg reflections are superimposed. It turns out that this superposition is more than a mere addition of nuclear and magnetic intensities. By using spin polarised neutrons it is possible to make use of an interference term in the scattering cross-section between nuclear and magnetic scattering. This combination of magnetic and nuclear scattering in the neutron scattering cross-section can be used to precisely determine a quantity known as the flipping ratio. The flipping ratio is a function of the magnetic and nuclear structure factors. If the nuclear structure factor is known, a measurement of the flipping ratio allows a very precise determination of the magnetic structure factor. The physical significance of the entities mentioned here will be discussed more fully below. A more detailed analysis of the theory of neutron scattering can be found in standard text books [1-4].

2.1. Nuclear scattering

For structure determination and for the measurement of the magnetic form factors it suffices to restrict the description of nuclear scattering of neutrons to elastic scattering only. In particular, it is only the integrated Bragg scattered in- tensity which is of relevance here. By definition the Bragg scattering is elastic scattering with no energy transfer between the crystal and the neutron. The dif- ferential neutron scattering cross-section can be written in the form

where ba is the scattering length of the atom i which is located at position k is the neutron scattering vector and dΩ is the infinitesimal solid angle into which the neutrons are scattered. The summation is carried out over all atoms in the crystal. Making use of the translational symmetry of the crystallographic structure, the summation in (1) may be separated into two partial sums

Here the index v sums over all unit cells of the crystal and the summation is carried out over all atoms within the unit cell v. The position of the atoms in each unit cell is given by IZV — IL„ and it is measured relative to the origin of the v-th unit cell as determined by 11 ,. A nuclear structure factor of the unit cell (k may be defined as

where the atomic position Ri is measured with respect to the origin of the unit cell. In general, (k will be a complex number. However, for a crystallographic K-U euma KA ieeck sucue wi a cee o iesio symmey e ucea sucue aco may e cose o e ea (y akig e oi o iesio symmey as e oigi o e ui ce eey aom a osiio i as is symmey eae aom ocae a —I= a wi e aom aig e same scaeig eg As a cosequece eey coiuio ie(ik • i i (3 is comie wi is come cougae i e(—ik • a i e summaio e imagiay as cace Iseig (3 io (1 a cayig ou e summaio oe a ui ces oe aies a

ee is e oa ume o ui ces i e cysa a δ(k — τ is e "ea ucio" wi r eig a ecioca aice eco e summaio is caie ou oe a ecioca aice ecos r us scaeig occus o scaeig ecos k wic coeso o a ecioca aice eco a wi a iesiy wic is eemie y e squae o e mouus o e ucea sucue aco (τ In acua eeimes e agg eecio wi o e suc a sa eak as iicae y e "ea ucio" i ( eak oaeig occus ue o e esouio o e isume a aso ue o same caaceisics (eg as gie y e saia ee o e coeey scaeig egios i e same owee e eais o e eak sae ae o o iees ee a ee is o ee o usue is oi ay ue e iegae agg iesiy o a agg eecio caaceise y is gie y

S(τ is a eecio eee scaig aco e scaeig eco eeece o S aises ue o e meo use o iegae e agg eaks e geomeic

coecio is kow as e oe coecio a i is eaiy eimiae om e measue iegae iesiies ee emais a oea scae aco wic is scaeig eco ieee e scae aco is ooioa o e oa ume o ui ces i e cysa eoig e ew scae aco (ae e eimiaio o e scaeig eco eeece y S e eeimeay eemie iegae iesiy o e agg eecio is gie y

U o a cosa e measue iesiies ae eeoe eemie y e squae o e ucea sucue aco owee o e esciio o e ucea sucue e aue o (τ is equie As oie ou aoe o sucues wi a iesio cee o symmey e ucea sucue aco may e cose ea us soig e ucea sucue euces o coosig o eac eecio e "coec" sig i e equaio

I is oie ou a soig e aoe ase oem o a eecios is equiae o e eemiaio o e aomic osiios i e ui ce is is so ecause aig oaie e sucue acos (τ o a suicie ume o Mageic σm acσ Measuemes 7

eecios e aomic osiios may e oaie y ouie iesio Wiig (3 i e om

i is see a e ucea sucue aco is oig ese u e ouie asom o e ieacio oeia wic i u is eemie y e osiios o e aoms a ei scaeig segs e aoe eiaio was caie ou usig some simiyig assumios e aice as ee ake as eec a e ema moio o e aoms as ee egece e emeaue moio a eo oi ucuaios ca e ake io accou y e susiuio wee W(k is e emeaue aco wic may e aisooic e ucio e(—W(kk is kow as e eye—Wae aco Oe eeimea acos suc as eicio a asoio coecios ae aso eaiy aie [5] a saa oceues eis o akig ese io accou []

2.2. Magnetic scattering I comaiso o ucea scaeig o wic e ieacio oeia e- wee euo a uceus is eemie y e ucea oce mageic scae- ig o euos is ase o a eiey iee ieacio mecaism Mageic euo scaeig eee o ee aises ue o a eecomageic ieacio e- wee e mageic ioe momes o e euo a ose o e eecos A ioucio a a comee eiaio o e asic omuae o mageic euo scaeig ca e ou i saa e ooks o euo scaeig [1 ] ee e iees is ocuse o easic mageic scaeig oy wi e mag- eic sucue eig esice o eomageic oe o e uose o cayig ou e euo scaeig eeime i is immaeia wee e eomageic oe is iisic o wee i as ee iuce y e aicaio o a eea mageic ie A moe eaie aaysis (as gie eg i [1 ] sows a e seg o e euo—eeco mageic mome ieacio is eemie y e ouc o e gyomageic aio o e euo -y (-y = —1913 a e cassica eeco aius wi = 175 1 -15 m e ouc M = γr0 = —539 1 -15 m eies a mageic scaeig eg M wic oies e ui o measuig e seg o mageic momes i mageic euo scaeig eeimes ee- oe i e oowig e mageic momes µ wi aways e measue i uis o M I is aso imoa o oe ee a e magiue o M is comaae wi yica magiues o ucea scaeig egs o a eomageicay oee sae e ce imesios as eie y e cemica ui ceł ae o cage ece y summig oe e same aoms as i (3 a mageic sucue aco o e ui ce may e eie as 48 K.-U. Neumann, K.R.A. Ziebeck

Here µi is the located on the i-th atom, and fi(k) is the atomic magnetic form factor of the atom. The form factor i is normalised according to

The magnetic structure factor as defined in (10) is a vector quantity. The overall strength of the magnetic neutron scattering is determined by the sizes of the mag- netic moments. Atoms with no magnetic moment, µ i = 0, will not contribute to the magnetic scattering. An additional scattering vector dependence is introduced into the structure factor due to the magnetic form factor. In general, the magnetic form factor tends to decrease with increasing magnitude of the scattering vector. As a consequence, the magnetic scattering diminishes for increasing scattering an- gles. This is in contrast to nuclear scattering for which the equivalent nuclear form factor is independent of the scattering vector and equal to one. Similarly to the case of the structure factor for nuclear scattering the mag- netic structure factor can be expressed as the Fourier transform of the interaction potential. For magnetic scattering the interaction potential is given by the mag- netization density within the unit cell

where M(r) is the position dependent magnetization. M(r) is a periodic function which has the periodicity of the nuclear lattice for a ferromagnetically ordered state. For a magnetization distribution which is given as the superposition of lo- calised atomic magnetic moments located at ri within the unit cell the magneti- zation density is given by

In this case the magnetic structure factor in (12) reduces to

A comparison with (10) yields the atomic form factor in the form

as the Fourier transform of the real space atomic magnetization mi(r). The total magnetic moment µ i is defined as the integral of mi(r) according to

This definition together with (15) ensures the normalization of the atomic form factor as defined in (11). For localised moments the integration in (14) and (15) is carried out over the whole of the three-dimensional space. All the various magnetic contributions of each individual atom are subsumed within mi. In general, mi is composed of several magnetic moments, including spin and orbital magnetic contributions and, if necessary, a core polarization as well. For the case of itinerant electron magnetism, for which the electronic wave functions are sufficiently delocalised, the general form (12) has to be used for Mageic σm aco Measuemes 49 the description of the magnetic structure factor. In general, it is not possible to uniquely allocate a given magnetization density to an individual atom, and the notion of a magnetic moment located on an atom loses its meaning. It is only meaiguł o ak aou e oa mageic mome e ui ce Mo with the total magnetic moment being defined as

Obviously for the case of localised magnetic moments Mo is determined by the sum over all magnetic moments in the unit cell. In this way the magnetic structure factor may be defined for both, localised as well as itinerant electron magnetism. However, for neutron scattering additional complications arise due to the vector form of the magnetic structure factor as compared to an equivalent scalar quantity for nuclear scattering. It turns out [1, 2, 4] that only those components of FM(k) which are per- pendicular to the scattering vector k may give rise to magnetic neutron scattering. The components which are active in the scattering process are defined as

In order'to combine the magnetic scattering contribution as defined by the vector in (18) with the nuclear scattering part as described by the scalar quantity FN(r) the vector FM(k) has to be reduced to a scalar. A more detailed analysis shows that it is the scalar product of F┴M(k)Pwithof the the neutron polarization vector beam that is needed for the neutron scattering cross-section. The scalar magnetic structure factor is defined as

For perfect polarization of the neutron beam P is a unit vector, the direction of which indicates the polarization direction. For a partial polarization of the neutron beam |P| is defined as

with n1, n↓, being the number of spin up or spin down neutrons in the beam. F, F(k) ┴M is the entity which plays the equivalent role to the nuclear structure factor in the formula for the scattering cross-section. For this reason F 1 ( k will be referred to as the magnetic structure factor. (This should not be confused with Fas M(k)┴ defined in (10).) Considering only magnetic scattering, the differential cross-section is determined as

where τM is a vector of the magnetic lattice and NM is given by the number of magnetic unit cells in the sample. For ferromagnetic order the chemical and magnetic unit cells are identical. Consequently N11 and τM have the same values as their nuclear counterparts. 50 K.-U. Neumann, K.R.A. Ziebeck

With nuclear and magnetic scattering present both contributions have to be combined. There are the two possibilities of either combining the intensities of nuclear and magnetic scattering or of adding the structure factors first and then inserting the sum into the formula for the differential cross-section. For the first possibility the intensities are summed by adding (4) and (20). This corresponds to an incoherent superposition of the scattered waves from the nuclear and the magnetic subsystems of the target. Here, however, nuclear and ferromagnetic scattering is considered which is superimposed on the same Bragg reflection. Under these conditions it is the sum of the nuclear and the magnetic structure factors as determined by (3), (14) and (19), which has to be evaluated. The underlying assumption is one of a coherent superposition of nuclear and mag- netic scattering contributions. The sum has to be inserted into the expression for the differential cross-section. Assuming perfect polarization of the neutron beam one arrives at

for a neutron spin polarization parallel (a) and antiparallel (b) to the external magnetic field direction. For a partially polarised neutron beam the cross-section is an average of (22a) and (22b) with the weighing factors determined by the proportion of spin up and spin down neutrons in the neutron beam. For this case the cross-section takes the form

The direction of is taken to be parallel to the direction of the external magnetic field. This form of the differential neutron scattering cross-section differs by the presence of an interference term between nuclear and magnetic scattering from the cross-section obtained for an incoherent superposition of the nuclear and magnetic intensities. The incoherent superposition is realized for an unpolarised neutron ex- periment, for which the magnitude of is equal to zero. In this case the differential cross-section takes the form

It is the presence of the interference term between nuclear and magnetic scattering which forms the basis of magnetic form factor measurements. It depends on the polarization of the neutron beam through in (23) or through the change of sign of I in (22a) and (22b). In the next section it will be discussed how this interference is exploited experimentally and how it can be utilised for the investigation of details of the magnetization on an atomic level. Magnetic Form Factor Measurements ... 51

2.3. Experimental e quaiies wic ae o e eemie y eeime ae e ucea a mageic sucue acos ese ae measue i seaae eeimes a y usig uoaise a oaise euos eseciey e measueme o e ucea sucue aco is equiae o a sucue eemiaio eeime I e eeime e iegae agg iesiy is eemie o a ume o agg eecios As iscusse aoe i Sec 1 a sucua moeł may e use o eie e ee aamees o a moe sucue us oaiig e ucea sucue acos FN (r) o a agg eecios use i e eieme e ucea sucue aco ogee wi oe eeimea eiies suc as aice aamee ec ae assume kow we e si oaise euo eeime is caie ou o e eemiaio o e mageic om aco a sige cysa o e ma- eia ue iesigaio is oieae i a eea mageic ie i suc a way a e mageic mome is aog e mageic ie iecio is ecessiaes a e mageic ie is iece aae o a easy ais o mageiaio I o- e o maimie e mageic siga (see (1 i is eeae o aig e mageic ie eeicua o e scaeig ae (wic is eie as e ae sae y e wae ecos o e icomig a scaee euos wi e scaeig eco eig e ieece o ese wo ecos Si oaise euos ae use i e om aco measueme owee o oaiaio aaysis is eee ae e euos ae agg scaee y e same ue iesigaio o a gie agg eecio r a assumig a eec euo si oa- iaio e ieeia euo scaeig coss-secios ae eemie o e

e iegae iesiies o is agg eecio ae gie y

ee eoes a euo si oaiaio aae o e aie mageic ie wie I iicaes a aiaae euo si oaiaio y usig eie e ieeia coss-secio o e iegae agg iesiy e iig aio R(τ ) is eie as

Eeimeay i is easie a ase o measue e eaie iesiies o si u a si ow euos a oy oe oi o e agg eecio (wic i e eeime is ou o e oaee o a Gaussia eak sae comae o 52 K-U. Neumann, K.R.A. Ziebeck a "ea ucio" iicae i e aoe omuae isea o aig o oai e iegae iesiies o o euo si oieaios eeoe i e eeime e cysa is se so as o maimie e couig ae o a gie agg eecio a e eaie couig aes ae measue as eemie y (5a a (5 o e ee a e saes o e ucea a mageic agg eecios ae ieica (τ oes o ee o ow e aio is eie wee y usig e aio o e iegae iesiies o y uiiig e aio a oy oe oi o e agg eecio As iscusse i eai esewee [5] oe eeimea acos ae eaiy icue i e eiiio o e iig aio akig io accou a aia oaiaio o e euo eam e eiciecy e o e euo si ie a e age O ewee mageic mome iecio a scaeig eco e iig aio akes e om

euig o e eessio o e iig aio as gie i (7 e equaio is eaiy iee o yie e aio o e mageic o ucea sucue acos as a ucio o e iig aio

e amiguiy gie y e ± √(τ em i (9 is eae o e amiguiy o wiig (τ i (7 eie i ems o ┴Mτo/( y usig e iese aio (τ /┴MτI( is e equiae o e quesio┴Mτis(/( o wee ( age o smae a oe I a acua eeime is oes geeay o ese a oem ecause a coice ca e mae o ysica gous A is oi i is wo sessig agai a e kowege o e ucea sucue aco is ia o e eemiaio o ┴Mτ( e uceaiy i e mageic sucue aco is isy eemie y e eeimea eo i e measueme o e iig aio (τ u secoy aso a moe imoay y e uceaiy i e ucea sucue aco As see om (9 e mageic sucue aco is measue i uis o e ucea oe a cosequey ay sysemaic eo i e eemiaio o e ucea sucue aco (as gie y e egec o emeaue acos asoio eicio ec wi iuece e accuacy o e mageic sucue aco Some aicua eaues o e iig aio ae wo oig I is is o a a quaiy wic is ieee o a scaig aco y akig e aio i (7 e scaig acos ae cacee uemoe i is a ucio oy o e ucea a e mageic sucue acos o aeciae e sigiicace o is saeme cosie e case o weak eomageic oe caaceise y

We eaig┴M τ /( (7 o eaig oe i τ e iig aio is gie y Mageic σm aco Measuemes 53

The deviation of the flipping ratio from one is a direct measure of the magnitude of Fili as measured in units of the nuclear structure factor. As FN(r) is known from a previous structure determination experiment the deviation of the flipping ratio from one immediately yields the value of F ┴Mτbothmagnitude(It(): and itsphase! ( ) should be stressed again that only centrosymmetric structures are considered here. For such structures the phase degree of freedom of the structure factors reduces to a choice of a ± sign in front of the wave function.) In these respects the measurement of the flipping ratio is unusual. It ren- ders possible an absolute measurement without the necessity of a normalization. Furthermore, it allows for a simultaneous determination of the amplitude and the phase of the magnetic scattering contribution. The physical origin of this can be ace ack o e esece o e ieeece em i e ieeiał euo scaeig coss-secio As e ieeece em is ooioa o e ouc o e ucea a mageic sucue acos e ase o e mageic scaeig ca e eae o e ase o e ucea sucue aco e ase oem o e ucea sucue aco (wic is e key quesio o ay sucue ee- miaio as ee soe a e ase is aeay eemie (u o a oea ase aco commo o a eecios us e kowege o e ase o e ucea sucue aco ca e use o eac e iomaio o e ase o e mageic sucue aco It is also worth pointing out that due to the interference term the sensitivity is significantly increased. While for an experiment employing unpolarised neutrons and with ferromagnetic order present in the sample the scattered intensity is given by

for an experiment carried out with spin polarised neutrons the intensity change is determined to be given by

For a ratio of F┴M /(τ = 0.1, the changeτ of intensity, δI/I may be compared with and normalized to the intensity I of an identical sample without magnetic order. For an unpolarised neutron experiment δI/I is of order 1%, while a value of . order 20% is found for 81/I for the spin polarised neutron scattering experiment. This increased sensitivity in spin polarised neutron scattering experiments allows for a more accurate determination of the magnetic scattering contribution and, finally, also of the magnetic structure factor. Thus, a measurement of the flipping ratios yields accurate values of the magnetic structure factors. As an experimentally determined entity the magnetic structure factors are model independent. However, the collection of values of mag- netic structure factors is not very revealing if presented on its own and in tabular form. It is more informative to consider the Fourier transform of the magnetic structure factors. As pointed out above the magnetic structure factors are determined by the Fourier transformation of the magnetic interaction potential. According to (12) 54 K.-U. Neumann, K.R.A. Ziebeck

e mageic sucue aco M(τ is eemie y

The inverse transformation is given by

wi eig e oume o e ui ce e summaio is caie ou oe ał ecioca aice ecos τ e mageic sucue acos ae e ouie coei- cies i e seies (3 e ouie asom ack io ea sace wi eeoe construct a picture of the real space interaction potential, which amounts here to the magnetization density distribution. In this manner a map of the magnetization density may be constructed and presented in real space as either a cut through the unit cell or as a projection. In order to be able to perform the Fourier transformation by using the exper- imentally determined magnetic structure factors an infinite number of the Fourier components in (34) has to be known. Experimentally this presents a problem, as only a finite number of coefficients can be determined. A Fourier series is an infinite series and it is only complete if all coefficients of the infinite series are included. Therefore, constructing a magnetization map by using a finite subset of coeffi- cients will result in "incomplete" and thus erroneous magnetization density maps. However, it turns out that a magnetization density map constructed by using a finite set of coefficients in (34) may still be meaningful and yields a magnetization density with the important features present. In order to understand the limitations imposed by the finite number of magnetic structure factors and to appreciate the significance of magnetization density maps a more detailed discussion of some of the relevant aspects is helpful. A discussion relating to these questions has been given by Moon [7]. A reflection which is not measurable by neutrons is the Bragg reflection coesoig o τ = O owee o is ecioca aice eco e eiiio of the magnetic structure factor in (12) reduces to the evaluation of the total magnetic moment in the unit cell as given in (17). While this reflection is not accessible in the neutron scattering experiment, its value may be obtained by magnetization measurements using conventional magnetometers. Its inclusion in the Fourier series and in a magnetization density map adds a scattering vector independent contribution. This Fourier coefficient may thus be considered to fix the zero level in the magnetization density map. A moe seious imiaio is e ue cu-o i Iτ i e summaio o e Fourier series. Denote by k, the magnitude of the scattering vector τ beyond which no more experimental values of Fi 1 ( are available. k, is taken to characterise the upper limit of the cut-off in the Fourier series. The coefficients belonging to τ > kc give rise to fast oscillating contributions in the unit cell. These components are needed for the description of the finer details in the magnetization density in real space. By not including these magnetic structure factors in (34) these details are lost. This loss of detailed structure corresponds to a picture where in the Mnt r tr Mrnt 55 perfect real space magnetization density (which is obtained by including all Fourier coefficients in (34)) a local average is carried out over a small volume element so as to eliminate the fast oscillating contributions within this volume element. In order to estimate the dimension of the volume element and to be able to relate it to k, the following procedure may be used (it suffices to consider the one-dimensional case). The magnitude of the cut-off wave vector kc defines a characteristic length in reciprocal space. Let r, be a characteristic length in real space. A reasonable estimate for the interval of average [0, c] will be given by a value of r, for which the phase factor exp(ik • undergoes several (but at least one) oscillation(s) as r is varied within the limits of the averaging interval and for a scattering vector k > kc . This criterion results in a definition of r, given by k, • r, = 2a. Writing kc in terms of a cut-off scattering angle with a eig e neutron wavelength employed_ _ in the ex )eriment, the interval of average is defined as For the two- or three-dimensional cases the volume of average may be taken to be a square or a cube with the linear dimensions de. fined by F Thus carrying out a Fourier transform on a limited set of wrier coefficients may still yield a correct magnetization density which, however, is deprived of some details in its structure. The experimentally determined magnetization densities are therefore not sensitive on a length scale defined by r c , with the fine structure being smeared out over the average volume. The coefficients which remain in (34) are all those Fourier components which belong to scattering vectors τ with τ k,. It is obvious that within this limited range the set of coefficients must be complete, or at least as complete as possible, for a meaningful magnetization picture to emerge from the Fourier transformation. As the various Fourier components in (34) are linearly independent a "missing component" in the series cannot be compensated by other ones. A magnetization density map will be severely distorted when constructed with an incomplete finite series with some coefficients missing for a with |n < kc . An example of a magnetization density map with a missing component will be given below. So far the discussion has been restricted to a paramagnetic material with a centrosymmetric crystallographic structure, and the procedures of a magnetic form factor measurement have been developed within this restriction. In order to complete this section, a brief discussion is given of the problems which arise when these restrictions are lifted. First, consider a magnetically ordered state of the sample. A brief but very instructive introduction to the investigation of magnetic order by neutron scatter- ing has been given by Brown [8]. The crystallographic structure is still required to be centrosymmetric. For a ferromagnetically ordered sample a magnetic field is not needed for inducing magnetic moments or aligning disordered ones, because long-range ferromagnetic order is assumed present. However, in order to define a unique direction of the magnetic moment, and thus Fe(τ an external magnetic field has to be applied. This is true even in the case of strong magnetic anisotropy, which tends to align the moments along a given crystallographic axis. Under these cicumsaces e eeał mageic ie as o emoe e egeeacy coece wi e omai sucue i e mageicay oee sae Oy i e woe si- 5 K.-U. Neumann, K.R.A. Ziebeck ge cysa is aso caaceise y oy oe mageic omai e aoimaios o ay i e eiaio o e iig aio i (7 I as aeay ee oie ou aoe a i e case o mageic aisooy e eea mageic ie mus e aie aae o a easy ais o mageiaio A ese ecauios ae o e ake i oe o uiquey eie e iecio o mageic momes i e cysa ue iesigaio o e case o a aieomageicay oee sucue e measueme • o e mageic om aco is comicae ue o seea acos o may a- ieomageic sucues e mageic oe cages e sie o e ui ce As a esu mageic a ucea agg eecios occu a iee ois i ecioca sace o a mageic om aco measueme owee e esece o ucea a mageic scaeig is eee a e same ecioca aice oi I a ucea ecioca aice eco τucea oes o coicie wi a τmageic e ucea-mageic ieeece em wi e ase om e easic euo scaeig coss-secio us a ieeece em i e easic euo scae- ig coss-secio wi e ase o aieomageic sucues wi a icease ui ce oume ue o e mageic oe is oes aso icue moe comi- cae mageic sucue suc as icommesuae o eica oes eeoe oy e case o a aieomage wiou a icease ui ceł ees o e cosiee ue Suc a aieomageic oe occus o eame i a cc sucue wee e mageic aoms a osiios ( a (1/ 1/ 1/ ae ei mageic momes aige aiaae wi esec o oe aoe e aious cases o mageic oeig ae es escie wi e e o e ime iesio oeao Ot . We acig o a mageic mome M is oeao eeses e mome iecio accoig o

I aiio o e ime iesio oeao i i is oy e symmey eeme o e iesio i sace I, wic is eee ou o a e symmey eemes wic caaceise e cysaogaic sucue Sace iesio oes o cage e oieaio o e mageic mome M. (is is ue o e ac a e si a o e mageic mome is o coue o e saia cooiaes wie e oia a o M is ooioa o e seuoeco r p, wee r is e osiio o e eeco ue cosieaio a p is is iea momeum e eco ouc r p oes o cage is oieaio we ace uo y I.) o eomageic oe a some aieomages e iesio symmey oeao is o comie wi e ime iesio As a cosequece ay aom a osiio i as a equiae aom ocae a —Ri. us gouig ose aoms ogee wic ae eae y iesio symmey; ei coiuio o e mageic sucue aco is ou o e ooioa o

As see om (3 ue e aoe assumios e mageic sucue aco is a eał quaiy (is was assume aoe a sae wiou oo o e mageic sucue aco o e aamage i a eea mageic ie Magnetic Form Factor Measurements ... 57

If, however, the antiferromagnetic state is characterised by a combination of operators as given by the product of space inversion times time inversion symmetry operator; the magnetic moment of the symmetry related atom is reversed. This results in a magnetic structure factor proportional to

This magnetic structure factor is purely imaginary. It is phase shifted by 90° with respect to the nuclear structure factor. As a consequence of this phase shift the flipping ratio as defined in (27) is identically equal to one. Denoting the real and imaginary part of the structure factor by Re and Inn, respectively, and under the assumption as stated above that the structure factors are given by

The flipping ratio as defined in (27) is equal to one for all reflections τ because the identity

is fulfilled for all Bragg reflections. Therefore no (τ≠1 reflection may be found for an antiferromagnetic structure which combines the space inversion element with time inversion. However, for a structure for which the space inversion element is a proper symmetry element both the nuclear and magnetic structure factors are real quan- tities. This is the case for a ferromagnetic and some types of antiferromagnetic structure, for which the assumptions leading to (36) are true. Only for these struc- tures a measurement of the flipping ratio is a possibility. However, in addition to the structural requirements which have to be fulfilled for a nonzero flipping ratio to occur, a further complication arises due to the presence of magnetic domains in the sample. For most magnetic structures and including a coupling to the lattice a small number of magnetic domains is possible. It suffices here to restrict the discussion to two domains, which are related to one another by time inversion symmetry. Such a pair of magnetic domains is always possible. It is appropriate to denote these domains as a 0° and a 180° domain, because the 180° domain is obtained from the 0° domain by an inversion of all magnetic moment directions. It may also be described as obtaining the 180° domain from the 0° one by the action of O ► on the 0° domain. Both domains are energetically degenerate. It may therefore be expected that the two domains occur with the same probability in a sample. Therefore, the magnetic structure factor of the whole sample has to be obtained by averaging over the various magnetic domains. This average, however, will result in a zero average magnetic structure factor. With the definition of the magnetic structure factor as given in (12) and by using an obvious notation to identify the structure factors for the various magnetic domains one obtains 5 K.-U. Neumann, K.R.A. Ziebeck

e mageic sucue aco is a eco e iecio o wic is eemie y e iecio o e mageic momes As e mageic mome iecio is eese y goig om oe omai o e oe e mageic sucue aco cages sig eeoe a eo aeage mageic sucue aco esus o ay same wi equa amous o mageic omais ese wic ae eae y ime iesio symmey is agume aies equay we o a eomageicay as we as a aieomageicay oee sucue I oe o emoe e egeeacy o e ° a 1° mageic omais a mageic ie as o e aie o a eomageicay oee same i suices o ay a omogeeous eea mageic ie is ie emoes e egeeacy o e mageic omais a i o suicie seg i may saiie a sige mageic omai i e woe cysa o a aieomage e aie mageic ie as o ae e mouaio o e aieomageic sucue i oe o emoe e egeeacy e wae eco o e mageic mouaio is o e oe o agsoms a a ese o eeay aie mageic ies ae aaiae wi suc so waeegs Oe eeimeay cooe aamees suc as essue o o eak ime iesio symmey a ey ae eeoe o caae o emoig e egeeacy o e mageic omais us oe is e wi e cocusio a o a aieomageic sucue a iig aio may e osee o ceai sucues a ue e coiio o a imaace o mageic omais wic ae eae y ime iesio symmey e aoe iscussio as iusae e comeiy o e agume a i as oe ou e eeimea iicuies wic ae o e oecome o wisaig ese oems measuemes o e iig aio i a aieomageic sucue ae successuy ee caie ou [9] e ieese eae is eee o e oigia uicaios o a eaie iscussio o aious asecs o e eeime o a aieomageicay oee susace a eea mageic ie may e aie o iuce a eomageic comoe is may e aciee y iig e mageic momes ou o ei aiaae aigme io e iecio o e eea mageic ie eey ceaig a eomageic comoe is siuaio is iusae i ig 1 e eomageic comoe o e mageic sucue is caaceise y a wae eco k = wie e aieomageic comoe is escie y a wae eco q. I is oy e k comoe wic coues o a aie mageic ie e coiuios o o wae ecos may e ecoue a cosiee seaaey o e eomageic comoe e eoy aies as eeoe aoe o e aieomageic comoe a ose comicaios aise wic ae ee cosiee i e eaie iscussio I e eeime oe accou as o e ake o o mageic comoes us i a om aco measueme o a aieomageic cysa (wic oes o icease e imesios o ui ce y oeig aieomageicay a wic is ace i a eea mageic ie i is oy e eomageic comoe wic coiues o e ieeece em owee ue accou as o e ake o e aieomageic scaeig coiuio o e oa iesiy o e agg eak Mageic σm aco Measuemes 59

o cysaogaic sucues wic o o ossess a cee o iesio symmey e ucea a mageic sucue acos ae come quaiies is imies a łage ume o comoes o ei caaceiaio Oe com- e ume o equiaey wo ea umes o caaceise ea a imagi- ay as ae eee as comae o oy oe ea ume a a sig i e case o ceosymmeic sucues e geeaiaio o e aoe eiaio o o-ceosymmeic sucues wi esu i moe comicae eessios [5] eoig e eał a imagiay as y a " eseciey a oig e scaeig eco eeece o e ucios e iig aio akes e om

Wie e ucea sucue aco Fi + iFN" is kow i suices o oe a a sige measueme o oy oe iig aio e agg eecio is o suicie o eacig e come quaiy ┴M(τA seco measueme is eee o wic e eeał mageic ie iecio o e oieaio o e cysał is eese As oie ou aoe e ea a o e sucue aco is eae o a a o e mageiaio wic is symmeic wi esec o e iesio oea- o e imagiay a o e oe a is aisymmeic ue sace iesio I e eea mageic ie iecio is eese e ea a o e mageic sucue aco wi o cage is sig wie e imagiay a wi us e- esig e eea ie iecio wi yie a iig aio gie y

o a o-ceosymmeic sucue e iig aio is iee o e wo co- 60 K.-U. Neumann, K.R.A. Ziebeck figurations of the magnetic field. These two measurements are in general sufficient to determine both the real and the imaginary part of the magnetic structure fac- tor. For a centrosymmetric structure the second setup will yield the same flipping ratio as the first measurement.

. Mnt fr ftr lltn fr pl dl t

In the previous section the magnetic form factor measurements have been considered from an experimental point of view. The magnetic structure factors and their Fourier transform in the form of magnetization density maps are the experimentally determined quantities. In order to fully interpret the experimental observation an attempt has to be made to quantitatively describe magnetization densities or magnetic structure factors. By using a model, parameters have to be obtained from observation for a description of the magnetization on an atomic level. For the most general case the theory will be complicated, and the interested reader is referred to the literature for details of some theoretical aspects of neutron magnetic form factors (Harmon [10]). It will also not be attempted here to derive the full expressions for the magnetization in real space or of the wave vector de- pendent susceptibility (see e.g. Oh et.al. [11], Cooke et al. [12]). Rather in order to illustrate the power of magnetic form factor measurements in this section atten- tion will be focused on some simple model systems. The first case is characterised by delocalised or itinerant , while a second model system is one with a collection of localised and atomic-like magnetic moments. The theoretical evaluation of M(r) necessitates the calculation of matrix elements of the form where |W) is the many-electron wave function of the crystal under investigation. Operators will here and henceforth be denoted by a — sign in order to distinguish the operator from its expectation value. Depending on the form of the operator it may be more convenient to present the wave function either in momentum space or in position space. These Hilbert spaces are defined such that the state vectors of the Hilbert space are either eigen- saes o e łiea momeum oeao wi or of the position operator r as given by

The momentum space and the position space are assumed to be complete

and the state vectors normalised Mageic σm aco Measuemes 1

e asomaio wic yies 11 as eie a eeseaio i momeum o i osiio sace is gie y

wi e ucios u(k a u( eig gie as

Wii u(k a u( is coaie e iomaio coece wi e occuaio o e aious ees o eegy as o e soi o a comee esciio o e quaum mecaica sae o e sae ecos a e ucios u(k a u( ae o icue a ie σ• o eoe e eecoic si egee o eeom e ucios u(k a u( ae o ieee om oe aoe e asomaio o u(k om a momeum sace eeseaio o a osiio sace eeseaio is aciee y a ouie asom o e mageiaio oeao M( a seaaio is ossie o e oa mageic mome oeao io a si a a oia coiuio accoig o

o e si a e oia coiuio o e mageiaio oeao ae a osiio eeece gie y

o some mageic maeias e oia comoe is eo is may e e case eie o a mageic mome wi = O (wi M ± a G3+ eig eames o i may aise ue o e quecig o e oia mome ue o cysaie eecic ies Eames o e ae ae ou amog e 3 eemes a ei aoys Ue ese coiios oy e si a o e mageic mome s oeao is acie e oeao o e si esiy M ( is eie as

e summaio is caie ou oe a eecos i e cysa e si oeao S is eemie as

wee ś↑ a ś↓ ae oeaos wic isiguis ewee si u a si ow saes o e i- eecos accoig o

ee I a I 1 eoe e si sae o a sige eeco e eco is a ui eco wic eies e ais o quaiaio i e sysem a a uique iecio wi esec o wic e eeco sis ae eie u o ow K-U Neumann, K.R.A. Ziebeck

Usig e aoe eiiios a asomig o a osiio sace eese- aio e mai eeme (5 is eauae o

e mai eeme (Ms(" is eaiy eauae wi e esu

O iseig (5 io (55 a iegaig e mai eeme o e magei- aio akes e om

e ysica sigiicace o is esu ca e mae ee moe asae we e si aiae is aome om S o e ucio ui( is is aciee i a simia mae as aoe i (53 y seaaig e si u a si ow as o ui(r) wi e iseio o a si ie e mageiaio esiy ca e wie i e om

e a eoes e aeage si u/si ow esiy o e eecos i e same wi e aeage eig oaie y cayig ou Ei a summig oe ał eeco coiuios is esu shows a e mageiaio esiy i ea sace is eemie y e esiies u ↑↓(1 o si u a si ow eecos A e mageiaio aises a osiio r i e esiy o si u eecos is iee om e oe o si ow eecos a is ocaio i e cysa Wii is esciio o mageic coiuio aises o comeey ie as o aomic oias us oy ose eecoic wae ucios may coiue o e mageiaio esiy wic eog o aiay ie eecoic as o ocaise ees a wic may gie ise o a e mageic mome As a secia case a as a iusaio o e iscussio gie aoe eecos ae cosiee i a soi wi ei wae ucios eig gie y ose o ee eecos e quaum ume k o ese eecos is a goo quaum ume yieig e ee eeco wae ucio i momeum sace I is eeoe ao- iae o e-eauae e mai eeme o e mageiaio esiy i eciocał sace a y makig use o e iea momeum eeseaio o W Accoig o (1 e ouie asom o e mageiaio esiy i ea sace is e mageic sucue aco us Mageic σm acσ Measuemes 3

e ie S o e mageic sucue aco iicaes a i is oy e si a o e oa mageiaio wic is icue Wi e e o e com- eeess eaio ( e mai eeme (kMs(k" may e eae o e mai eeme i osiio sace as gie i (5

e mai eeme ome y e comiaio o a iea momeum a a a osiio ke eco is gie y

Iseig (5 ( a (1 io (59 a makig use o e "ea ucio" i e om

e mageic sucue aco akes e om

I eici om a icuig e si u a si ow oaio o u(k e aoe equaio may e wie as

Equaios (3 a ( ae coouio iegas a oig ese u e ouie asoms o (57 a (5 e mageic sucue aco as gie i ( is si geeay ai a o ye esice o e case o ee eecos • e iegaio i ( ecomes aicuay sime o e case o ee eec- os ei wae ucio is gie y ae waes wi u(k equa o a cosa e cosa equas oe o a occuie saes wie e ucio u(k is equał o eo o k saes wic ae o occuie e eegy isesio o ee eecos is gie y a aaoa wi egeeae eegy as o si u a si ow eecos I oe o ae a oeo mageic sucue aco a a e eomageic mome e eegy as o si u a si ow eecos mus e isace i eegy is is iusae i ig e iig o e egeeacy may e eie ue o a eea mageic ie o ue o a iisic eomageic isaiiy o e coucio eeco a e emi suace is assume o e a see o o si u a si ow eecos wi e emi wae ecos gie y a eseciey K.-U. Neumann, K.R.A. Ziebeck

e ucio ut (k — k') (ul(k — k')) as a oeo aue (≡ 1 i a see o aius kF (kF). e cee o e see is ocae a k. us e coouio iega ( euces o e iegaio o e iesecio o wo sees o equa aii a wi ei cees a isace k aa is siuaio is iusae i ig 3 Usig ese geomeic agumes a eoig k yek iega is Magnetic Form Factor Measurements ... 65

The spin down integral can be evaluated in an identical manner, and the magnetic structure factor is obtained by the subtraction of the results of the integration for spin up and spin down electrons. K.-U. Neumann, K.R.A. Ziebeck

e mageic sucue aco may e cacuae o e wo cases o com- ee a aia mageic oaiaio o e eecos as iusae i ig e esuig mageic sucue acos ae iusae i ig wee e scaeig eco eeece is oe o e mageic sucue aco omaise o oe a eo scaeig eco y iiig FsM(k) y e oa mageic mome e esus o e iegaio i ( sows a e coiuio o e ee eeco mageiaio o e mageic sucue aco is imie o ow scaeig ecos A ue imi o e coiuio may e oaie om ( y cosi- eig e uy oaise sae o scaeig ecos k wi k > ma(k↑k↓e) mageic sucue aco is eo o ee eecos A yica aue o e emi wae eco may e cose o e A is esus i a esimae o 1/π o e ue cu-o i si /a o a ee eeco coiuio o a aiay oaise sae e ue cu-o wi e euce aoiaey e mageic sucue aco o ee eecos may e use o esimae e coiuio o coucio eecos Wie coucio eecos i ea sois ae eocaise ey may o e eiey ee (a is ae a u(k) as gie aoe u e ee eeco icue may see as a easoae guie o esimae ei coiuio o e mageic sucue aco I "ea" sois a akig ae ea aoys as a eame e mai a o e mageiaio is caie y ocaise mageic momes wic oigiae om -eecos A oaiaio o e coucio eecos wi gie ise o a smał aiioa mageic mome wic wi cage e aue o e oa mageic mome i e ui ce a iuece e is ew agg eecios e oa -eeco mome oaie y a eaoaio o e mageic om acos o mageic sucue acos o ige scaeig ecos o owe k aues oes o aways agee wi e oa mageic mome as oaie y mageiaio measuemes e ieece is usuay aiue o a coucio eeco oa- iaio As ei coiuio is coie o ow scaeig ecos i is someimes aoimae y a "ea ucio" ee ae oy ew agg eecios wii e age o a oeo ee eecio mageic sucue aco us e eaie om o e mageic sucue aco is o eaiy iesigae eeimeay y usig e ecique iscusse ee I is oy ue o a eiaio o a ew mageic sucue acos om ei eaoae aues a ow asoue scaeig ecos (a mos sigiicay a k = a e coucio eeco oaiaio may e eece A aoimaio y some we ocaise a aow ucio ce- e a eo scaeig eco seems o e aequae o aciee cosisecy wi oseaio I is a geea eaue o e ouie asom a a ocaise coiuio i oe sace wi esu i a ouie asom wic as a eocaise caace e iese is aso coec As o e case o ee eecos ei wae ucio is eocaise i ea sace us giig ise o a say eake mageic sucue aco I oe o ae a mageic sucue aco wic is moe eee i ecioca sace e souce o mageiaio esiy mus e moe ocaise i eał sace e oe eeme comae o e comeey eocaise a ee eecos Mageic σm aco Measuemes 7 is gie y comeey ocaise eecos Suc cases ae eaie i ae ea a aciie meas a ei aoys e -eeco wae ucios ae weł ocaise wii e eeco cou o e ee aom wi a aius o e -eeco wae ucio wic is muc smae a e aii o e oue s o p eecos us i aoms wi a aiay ie -eeco se ae aoye io a soi ei -eeco wae ucios o o oea a ey emai o a age egee aomic-ike ow- ee comicaios aise ue o a ieacio wi coucio eecos esuig i a ic secum o ysica oeies icuig iemeiae aecy a eay emio eaiou o e uose o aaysig mageic om aco measuemes owee e mos imoa eaue is e ocaiaio o ose eecos wic gie ise o e mageiaio i e ui ce Wi e eame o -eeco sysems i mi i is o e eece a e mageiaio o -eecos ca e uiquey a uamiguousy assige o a ceai aom e oea iega is sma ewee -eeco wae ucios ocae o eigouig aoms a e iega may e aoimae y eo o e uose o cacuaig e mageiaio esiy I suices o cosie oy e ocaise coiuios o e mageiaio esiy wi a wae ucio Ψ o e woe cysa gie i a ig iig aoima- io o simiciy i is assume a oy oe aom e ui ce is coiuig o e ocaise mageiaio esiy Wii a a icue e -eecos wi gie ise o a aow a is -eeco a wi e caaceise y oy a ey moes isesio ue o e smaess o e wae ucio oea ewee -eeco aoms o eigouig aice sies o ea sois e isesio o e -eeco a is maiy ue o e yiiaio wi coucio eecos I oe o simiy e esciio oy oe a wi e cosiee e wae ucio Ψ as o ake ue accou o e ocaiaio a a e same ime aso o e equieme o e oc eoem o wae ucios i a eioic aice o a ocaise mome sysem i a ig iig aoimaio e sae eco o e woe cysa may e eae as

usig e comee a oooma asis se o oc sae ecos Ψ(k As oie ou aoe oy oe a wi e cosiee as a cosequece o wic e a ie wi e ie e asomaio o a oc sae eco o a eco i osiio sace eeseaio is gie y

u (k, is a eioic ucio wi e eioiciy o e aice o e case o oe mageic aom e ui ce a wii a ig iig aoimaio e ucio u (k, akes e om

e ucio Φ(—i is a wae ucio wic is assume o escie e ocaise coiuio aisig om e i- aom ocae a 11 i is a aice eco o e K.-U. Neumann, K.R.A. Ziebeck cysaogaic aice e ume N is equa o e ume o ui ces i e cysa wic o e coiios seciie aoe is equiae o e ume o mageic aoms i e cysa e oea is assume egigie wi

I is oe assume a (i is gie i ems o wae ucios wic ae ca- aceisic o e ee aom I may e comose o seea as accoig o

wi a ucios α( o e easio eig ocae a e osiio o e i- aom is aows e iig o egeeacy o a aom i a cysaie eiome as comae o a ee aom o e ake io accou o -eeco sysems e eucio i symmey is e egeeacy o e ees e eegy ees si io cysaie eecic ie ees wi e egeeacies o e ees eig eemie y e oi symmey o e aomic osiio ee owee e siig o e -eeco a o -eeco ees wi o e cosiee ue e mai eeme o e mageiaio esiy i ea sace is gie y

I (71 e mageiaio oeao icues e si a oia coiuio Wi e sae eco as seciie aoe i ( e mai eeme o e mageiaio akes e om

Iseig e mai eeme un(k, i ( io e aoe omua M(r) akes e om

ecause o e assumio o egigie oea ewee eigouig aice sies e summaio oe e ie j wi oy gie a coiuio o e em i = j.

us (73 may e wie as Mageic om acσ Measuemes 9

Wi a si o e oigi y i (ie y a aiae asomaio — i → a wi e e o e "ea ucio"

e mageiaio esiy i ea sace is iay oaie as

e aco kα (k 2 is oig ese u a occuaio aco wic i ea sace coesos o a aeage occuaio o e ee o ees icue i Φ((M( yiese emaiig e mageiaio aco esiy i ems o e wae ucio wic escies e ocaise coiuio e occuaio aco may e asoe io Φ( wic e coesos o a wae ucio comose o a sum oe a occuie saes wi weigig acos accoig o e occuaio o e aious ees As oie ou aoe a equey use aoimaio is o ake e uc- ios Φ( o e gie y ose o a ee aom is is e easo wy ee aom om acos ae so oe emoye o a eaaio o mageiaio esiy measuemes I is wo ecaig e eiiio o e mageic om aco (k as gie i (15 wee (k was eie as e ouie asom o e mageia- io esiy o a sige aom e esus o cacuaios o aomic mageic om acos o ae ea a aciie aoms ae ee auae i e ieaue o o oeaiisic [13] a eaiisic [1] cacuaios us e cacuaio o e mageiaio esiy i ea sace as ee euce o e cacuaio o e mageiaio esiy o a ee aom o si a oia coiuios o e mageiaio ae moe eaiy cacuae o e ee aom comae o a eemiaio y a a sucue cacuaio Oe ieacios suc as si—oi couig a cysa ie ieacios wi e cysaie eiome may aso e icue aicuay o e ieacios wic gie ise o e cysaie eecic ies i is a aaage a o ocaise a aomic-ike wae ucios i is ossie o seaae e wae ucio io a agua a a aia a y asomig o seica cooiaes e wae ucio Φ(r) may e wie i e om /( = R(r) Y(υ, ). e agua a o e wae ucio is eaiy eae oougy akig io accou e emoa o seica symmey a e iig o egeeacies i e cysa Gou eoy eics e siig a e ee egeeacies e emaiig mai eemes wic ae o ie y symmey cosieaios ae commoy ake as ee aamees o e ie y comaiso wi eeimes A comee eiaio o e maemaics is gie i [15 1] a i oesey [] e case o cysa ies as ee cosiee y oucee [17] e aia a o e wae ucio is o eemie y symmey aoe u i is a ae comicae ucio o Is u a saisacoy eemiaio equies a uł scae eaiisic cacuaio o e ee aom o go eyo is aoimaio ecessiaes a uł scae a sucue cacuaio is owee is oe o easie a e aia eeece o a ee aom cacuaio is use o comaiso wi eeime 70 K.-U. Neumann, K.R.A. Ziebeck

The problem of calculating the magnetization density in the unit cell has thus been reduced to the calculation of the magnetization of a single atom. Under the assumption that it is adequate to treat the atom in the crystal essentially in the same manner as a free atom all the standard procedures of spectroscopy may be applied. While the mathematical procedure may be involved it is nevertheless straightforward. A complete exposition of the physics of spectroscopy is given in the book by Condon and Odabasi [18], and it should be consulted in addition to the references. cited above. After the discussion of the calculation of the magnetization density in real space an experimental investigation will be considered in the next section. Exper- imental results are presented and the magnetization densities are interpreted and discussed in relation to the models of localised and itinerant electron magnetization densities.

4. Experimental investigation

The investigation of the magnetic form factor and the magnetization densi- ties in a solid commences with a proper characterization of the nuclear structure. Therefore, the first part of this section will be concerned with the determination of the nuclear structure as defined by the identification of the atomic positions. In the second part data will be presented of the magnetic form factor and magnetization density, and an interpretation will be given of the observation. Two substances will be considered here, UBe13 and UPt3, with both com- pounds belonging to the group of heavy fermion superconductors. The properties of heavy fermion systems are of interest in themselves, and their investigation is currently a very active field of research. However, the physical properties of heavy fermions are not of primary interest here, but rather attention is focused on their magnetic form factors only. Therefore, out of the rich spectrum of heavy fermion properties it is only the static magnetic characteristics as seen in an investigation of the magnetization densities which are of interest here.

$.1. Nuclear structure of UBe13 and UPt3

The crystallographic structure of UBe13 and UPt3 is cubic and hexagonal, respectively. The crystallographic space groups proposed in the literature [19] are given as Fm3m for UBe13 and P63/mmc for UPt3. These structures have been confirmed in a detailed neutron scattering experiment, and the free parameters have been determined experimentally for these structures as given by the positional parameters of one Be atom position in UBe13 and the position of the Pt atom in the unit cell of UPt3. Additional information was obtained in these experiments with regard to temperature factors, absorption and extinction. The nuclear structure of UBe13 is presented in Fig. 5 as a projection of the atomic positions onto one of the cubic faces. Each unit cell contains 8 formula units, with 8 U atoms and 104 Be atoms on two crystallographically different positions. Denoting the two Be sites by Bel and Bell, there are 8 BeI and 96 BeII atoms shown in the projection. For clarity a projection is shown in Fig. 5b which contains Mageic σm aco Measuemes 71

only the U atom positions. The uranium and BeI atoms each form a simple cubic sublattice within the UBe13 structure. For the projections shown in Fig. 5b there are two U atoms being projected down onto each uranium site. It is worth pointing out some of the features of the projection of the nuclear density in Fig. 5. First of all, it is a map in real space of the neutron—nuclei in- teraction potential. It is obtained by a Fourier transformation using the nuclear structure factors in a manner identical to the procedures described above for the magnetization density. The nuclear density is seen to be smeared out over a small region with the centre of the density being located at the position of the atom. This smearing is a consequence of the finite Fourier series which has been used to obtain the nuclear density. The "real" interaction potential is a "delta function" when a standard description of the interaction potential is used with the Fermi approximation. Thus, the finite width in the nuclear density map is entirely due 72 K.-U. Neumann, K.R.A. Ziebeck

o e ume o e ouie coeicies use i e ouie iesio I oe o aow a comaiso wi e mageiaio esiy ma e same cu-o is use i e ouie seies as wi e use ae i e cosucio o e mageia- io esiy I suyig e oecio o e ucea esiy i sou aso e ake io accou a e ucea esiy is measue y e seg o e euo— uceus ieacio e seg o e ieacio oeia is aam- eeie y e euo scaeig egs bu a bBe [20]. owee ue o ey simia aues o e scaeig egs o U a e (bu = 1 1 -15 m bBe = 7.79 x 10' 15 m i is iicu o isiguis e U a e aom osiios om e aues o e coou ees i ig 5 o U3 e ucea sucue is sow i ig as a ee-imesioa icue igue 7 sows e osiio o e U a aom o wo cus oug Mageic σm acσ Measuemes 73

e ui ce e ui ce o U 3 coais wo omua uis wi e aoms ocae i wo eagoa aes wi z = 1/ a z = 3/ a as sow i ig 7 o aes ae eae o oe aoe y cees o iesio symmey wic ae ocae a e oigi o e ui ce ( a a e osiio (5 5 5 o ucea sucues ae ceosymmeic as a cosequece o wic e ucea sucue acos ca e cose ea eeoe e ase aco o e ucea (a aso o e (eo- mageic sucue aco is gie y eie +1 o —1 o maeias ae aamageic i e emeaue age iesigae i e om aco measueme o U3 aieomageic oe is eoe o occu a aoimaey 5 K wi a ouig o e ui ce is owee wi o ieee wi e om aco measuemes a eeoe e aieomageic oe o U3 wi o e usue ue

4.2. Mageic σm acσ measuemes i Ue13 a U3 I e si oaise euo scaeig eeime e sames wee ace i a mageic ie o esa o e Ue13 same e mageic ie iecio was aae o e cysaogaic [1 1 ] iecio wie o U3 e mageic ie was aog [ 1 ] o U3 is coesos o a coiguaio wee e ie is i e eagoa ae a eeicua o e mageicay a iecio wic is ou o e gie y e cysaogaic c-ais e iig aios o a ume o e agg eecios ae ee measue a emeaues o 1 K o Ue13 a o 5 K a 3 K o U3 As e iig aios o U3 i o ay wi emeaue e wo aa ses wee mege i oe o imoe saisics I e si oaise euo scaeig eeimes e iig aios ae ee oaie o a measuae agg eecios wi aues o e scaeig ecos caaceise y si Θ/λ 5 Ǻ-1 I oe o ese e aa i a cocise a meaigu mae oe may assume a e mageiaio aises oy om e 5 eecos ocae o e uaium aom ue o e simiciy o e sucues o o Ue13 a U3 i is ossie o euce e mageic sucue aco o e mageic om aco o e uaium aom Wii is moeł o oy akig io accou e 5-eeco mageiaio a y usig (1 a (15 e mageic sucue aco ca e wie as

ee e summaio is caie ou oe a uaium aoms wi ei osi- ios gie y i wii e ui ce Accoig o e assumio mae aoe a oe aoms i e ui ce o o coiue o e mageiaio a ee- oe ey ee o e icue i e summaio i (77 Moeoe a uaium aoms ae o cysaogaicay equiae osiios a ei iuce mageic momes ae a equa us wi

e mageic om aco euces o 7 K.-U. Neumann, K.R.A. Ziebeck

e aco ∑ eτi is a kow eiy as a e aamees suc as aomic osiios ae kow us is aco may eaiy e emoe om (79 eey e mageic sucue aco is euce o e mageic om aco o e uaium aom muiie y a cosa e muiicaie aco i o o e mageic om aco is equa o e oa eomageic mome ocae o e -uaium aom e mageic om aco o e uaium aom is e ouie asom o e aomic mageiaio esiy ese esiies ae ee cacuae o e aious saes o ioiaio o e ee uaium aom a e eea ucios ae ee auae i e ieaue [1] Assumig a ee 5-eecos ae ese o e uaium aom a a cysa ie siigs a yiiaio eecs ca e egece e mageiaio esiy o e uaium aom eais is seica symmey wii e cysaie eiome A mageic om aco wic is eauae ue ese assumios is kow as a om aco i ioe aoimaio Usig e ioe aoimaio o e 5-eeco mageiaio ee e- mais oy oe ee aamee o e eemie y comaiso wi eeime e ukow eiy is gie y e sie o e mageic mome ocae o e • uaium aom Wie e sauaio mageic mome o is coiguaio ca e cacuae e mageic mome aige y e eea mageic ie a a e eea emeaue may e susaiay iee om e oa magnetic mome o e aom us wi e assumio o a ocaise mageiaio esiy cee o e Uaium aom a wii a ioe aoimaio o e mageiaio isiuio a oe-aamee i as o e caie ou e esus o suc a iig oceue ae sow i ig a ig 9 e coiuous ie coesos o e mageic om aco o e uaium aom wie e aa ois ae gie y e measuemes o Ue 13 a U3 Wie e eeimeał aues o e mageic om aco o Ue 13 ae saisacoiy eouce y a om aco o e Uaium aom i ioe aoimaio e coesoig aa ois o U 3 sow a sigiica scae aou e cue o a seicay symmeic mageiaio isiuio I oe o imoe e ageeme ewee cacuaio a oseaio o U3 oe may y o ea e coiio o a seicay symmeic mageiaio isiuio a moe e om aco wii a cysa ie moe owee ee wii is ess sige moe e ageeme o a imoe moe cacuaio a eeimea oseaio is oo I us ou a e scae o e aa - ois i ig 9 is oo aie o aow moeig usig oy a uranium aom mageiaio I oe o oai moe isig io e easo o suc a isceacy a o e ae o ieiy e aious coiuios o e mageiaio i is iomaie o suy e mageiaio esiy i ea sace Usig e measue mageic sucue acos i e ouie seies e ea sace mageiaio esiies ae ee cosuce o o Ue13 a U 3 e mageiaio esiy i Ue13 is sow i ig 1 as a oecio oo oe o e aces o e cuic ui ce e ume o e ouie coeicies a e oe coiios o oaiig e o ae e same as e oe o e oecio Magnetic Form Factor Measurements ... 75

o e ucea esiy i ig 5 I is see om e mageiaio oecio a a mageic esiy aises a e osiios o e uaium aoms o oe sucue o eai is isie wii e ui ce I aicua ee is o ocaise mageic coiuio cee a e e aom osiios is esu is o suisig i iew o e ac a e mageic om ac- o i i ig is a goo esciio o e eeimea aa e mageiaio esiy i ea sace is eeoe omiae y e 5-eeco mageiaio ow- ee o ow scaeig ecos a sysemaic eiaio is ou i ig ewee e osee aa ois a e cacuae om aco cue is eiaio a ow aues o si /a is aiue o a oaiaio o e coucio eecos As iscusse i some eai i Sec 3 e coucio eeco coiuio wi e say eake a τ = O a quicky a o eo as e sie o e scaeig eco iceases e ouie asom is o eece o sow sigiica sucue I oe o iusae e eecs o a icomee ouie seies a magei- aio esiy ma is cosuce wi oe comoe missig Suc a icue is sow i ig 11 wee e comoe coesoig o τ ( as ee 76 K-U. Neumann, K.R.A. Ziebeck

reduced by a factor of two. The nuclear structure factor of this reflection is acci- dentally very small, as a consequence of which it is experimentally more involved to obtain accurate values of the flipping ratio. This is due to experimental difficul- ties and uncertainties which arise in an accurate determination of the background contribution for weak reflections. For reflections with a low nuclear structure factor other contributions such as those due to multiple scattering may seriously influence the intensity of the Bragg reflection. Thus, the flipping ratio of a weak reflection may be systematically estimated as being either too low or too high. For a mag- netization density map which is constructed using this coefficient in the Fourier series the resulting magnetization density may show additional structure which arises from the difference between the correct and estimated magnetic structure factor. Figure 11 shows magnetization density for the magnetic structure factor Magnetic Form Factor Measurements ... 77

with the "correct" coefficient of the (2, 2, 0) reflection being multiplied by 0.5. This reflection and the ones obtained from it by the application of the symmetry elements of the structure contribute a term proportional to cos (4π/α(r + ry )) to the projection of the magnetization density. In order to see whether or not such structure in the magnetization density is a "reap' effect or whether it arises due to some missing or wrong Fourier com- ponents one may calculate the magnetization using a simple model such as the uranium 5f-electron magnetization only and employing the dipole approximation. is moeł may e e use o cosuc e mageiaio esiy i ea sace y a ouie asomaio a wi e same coeicies i e ouie as- om as use i e eeimea seies Suc a esiy ma sou e sow oy ocaise mageic coiuios Ay eiaio om is mus e aiue o a eec o e ouie seies Aeaiey oe may suy e ieece ma wic is oaie y ouie asomig e ieece o osee a cacu- ae mageic sucue acos o oceues eae o ieiy e oigi o e sucue wic is ou i e mageiaio esiy mas Figure 12 shows the magnetization density for UPt 3 as a cut through the unit cell at a height of z = 1/4. The positions of the atoms in this plane are indicated in Fig. 7. When studying the magnetization density of Fig. 12, the first impression 78 K.-U. Neumann, K.R.A. Ziebeck

is one of a complex magnetization distribution with various contributions which are located at different positions in the unit cell. Around the position of the uranium atom there is indeed a significant and weł ocaise mageiaio o e ou e aia ee o e 5-eeco wae ucios is cosise wi e iemos mageiaio isiuio owee i aiio o e mageiaio o e 5-eecos a mageiaio coiuio is ieiie wic aises om a 7s electrons of the uranium atom. The sym- metry of the 6d-electron wave functions is reduced due to the point symmetry of the uranium location. The threefold axis of rotation gives rise to the crystal field splitting of the 6d-electron levels. This is the reason for finding the three regions of positive magnetization density at a distance of ≈A1.2of the U atom position. Both the radial extent of the wave function and the fact that it is split into crys- tal field levels uniquely identify this magnetization distribution as arising from 6d electron. For s or p electrons no splitting is expected to occur for the site sym- metry of the uranium atom. The remaining negative magnetization distribution is attributed to a 7s-electron polarization, with the 7s-electron spin being orientated antiparallel to the direction of the 5f-electron magnetic moment. The remaining magnetization distribution in the unit cell arises due to a magnetic polarization of the platinum electrons. The Pt triangle within the unit cell is seen to carry a significant part of the magnetization density. The electrons have to be considered delocalised. The overlap between neighbouring Pt atom wave functions is significant, as a result of which the magnetization distribution is severely distorted. The appearance of the magnetization density does not any more resemble the one expected for atomic wave functions. In order to model the magnetization density for UPt 3 all those electronic con- Mageic σm acσ Measuemes 79 tributions identified above have to be included. The model of a localised moment magnetization can be modified to include the localised magnetization contributions of the uranium atom. It suffices to use free atom wave functions. For the mod- elling of the magnetization density within the triangles of Pt atoms the overlap of wave functions has to be included. This requires a band structure calculation. Until now, however, a theoretical prediction of the magnetization density in UPt3 based on the band structure calculation has not been reported in the literature. Bearing these comments in mind a model calculation has been carried out using free atom wave functions for both, uranium and platinum contributions. By using such a model the agreement with observation could be significantly improved. The agreement is considered fair, however, with the main shortcoming of such a calculation being given by the inability to adequately model the delocalised magnetization density around the Pt atoms.

5. Discussion

The results of the form factor measurement of UPt3 illustrate quite nicely the power of the technique of spin polarised neutron scattering. The magnetiza- tion density as presented in Fig. 12 reveals details of the electronic wave functions, their radial extent and the angular dependence. It is therefore a decisive test for any band structure calculation, whether or not such details. of the electronic wave function are reproduced by the calculation. It was pointed out in the introduc- tion that this type of measurement probes the ground state of the system. The perturbation which is introduced by the application of a magnetic field is of the order of 10 K. This energy is much smaller than the energies involved in typi- cal experiments in spectroscopy, or the accuracy of energy values obtained by a band structure calculation. For the purpose of comparing the magnetic form factor measurements with results of band structure calculations the ground state wave function may be used for the calculation of M(r). In general, band structure calculations are aimed at a determination of the eigenvalues of the hamiltonian of the system. This results in the energy spectrum as given by the band structure and the electronic density of states. In order to obtain good estimates for the energy eigenvalues of the system it is generally not required to have the exact wave function which is an eigenstate of the Hamiltonian. A method due to Ritz is a well known procedure in quantum mechanics whereby a trial wave function with some free parameters is used in a variational procedure to obtain estimates of energies for the system under investigation. Quite different wave functions may lead to very similar estimates for the energies. It is not essential to have the correct electronic wave function for obtaining good estimates for the band structure. However, for obtaining a complete solution of a quantum mechanical system the eigenfunctions have to be determined. In this respect a comparison of calcu- łae wae ucios wi e esus o mageic om aco measuemes ca e eu Si oaise euo scaeig eeimes ae caae o yieig ey eaie iomaio o e wae ucios o some eecos i e sysem I aiio o oiig a caege o a sucue cacuaios e mag- K.-U. Neumann, K.R.A. Ziebeck

eiaio esiies may yie quaiaie iomaio o e egee o ocaiaio o eecos i meas a o cemica oig i ioic comous A age um- e o sysems ae y ow ee iesigae wi is ecique e ieese eae is eee o a comiaio o eeeces o mageic om aco mea- suemes (oucee [1] wic coais a age ume o sysems wi aie ysica caaceisics e eaie ieeaio o eeimea esus aso ees o a age egee o e sysems wic ae cosiee ee oy e e- ame o a meaic sysem wi ocaise a eocaise eeco mageiaio coiuios as ee cosiee o a moe eaie iscussio e ieaue [-] may e cosue i aiio o e e ooks o euo scaeig [1-3]

Cocusios A ioucio as ee gie o e ecique o si oaise euo scaeig wi a aicaio o mageic om aco measuemes Some ee- imea quesios ae ee iscusse o e ieeaio o e mageiaio esiy wo moes ae ee cosiee a ocaise mome sysem a a eo- caise eeco sysem wi e eeco escie y ee eeco wae ucios e aious ois aise i ese iscussios ae ee iusae wi e eei- mea iesigaio o e eay emio sysems Ue13 a U3 ese sysems eii e u secum o eecoic mageiaio isiuios i meas o eecos wi ocaise caaceisics i icues coiuios om 5-eecos o e uaium aom wi e mageiaio aig seica symmey cysa ie si coiuios o -eecos a 7s-eeco mageiaio wi o a- gua eeece eocaise eeco coiuios ae ou i mageiaio esiy i ea sace e eeimea ecique o mageic om aco measuemes y eu- o scaeig is a oweu oo wic may yie eaie iomaio coceig eecoic wae ucios is iomaio is comemeay o oe eeime- a eciques wic iesigae e eegy secum a a sucue o e soi Mageic om aco measuemes ae aso a caege o eoy a a sucue cacuaios A cose comaiso o e mageiaio esiy i ea sace wi eecoic wae ucios oaie i a sucue cacuaio is igy esiae

eeeces

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[] ow C Maewma The Cambridge Crystallographic Subroutine Library (A collection of FORTRAN subroutines for the use in crystallography), Iea I eo I Geoe 199 [7] M Moo Int. J. Magn. 1 19 (1971 [] ow Physica B 137 31 (19 [9] aas A Aei S icka ow J. Appl. Phys. 3 11 (193; A Aei ow aas S icka Phys. Rev. Lett. 37 (19 [1] amo J. Phys. (France) C7 177 (19 [11] K O amo S iu SK Sia Phys. Rev. B 1 13 (197 [1] Cooke S iu A iu Phys. Rev. B 37 9 (19 [13] M ume A eema E Waso J. Chem. Phys. 37 15 (19 [1] A eema escau J. Magn. Magn. Mater. 1 11 (1979; C Sassis W eckma amo escau A eema Phys. Rev. B 15 39 (1977 [15] E aca J. Phys. C, Solid State Phys. 151 (1975 [1] E imme SW oesey Rep. Prog. Phys. 3 333 (199 • [17] oucee Gio Scweie J. Phys. (France) C7 199 (19 [1] EU Coo Oaasi Atomic Structure, Camige Uiesiy ess Cam- ige 19 [19] ias Cae Pearson's Handbook of Crystallographic Data for Inter- metallic Phases, Ameica Sociey o Meas Wiau (Swiea 195 [] Seas Thermal Neutron Scattering Lengths and Cross-Sections for Condensed Matter Research, Cak ie ucea a Cak ie (Caaa 19 [1] oucee A Compilation of Magnetic Form Factors and Magnetization Den- sities, euo iacio Commissio o e Iea Uio o Cysaogay I Geoe 19 [] Scweie i e [] 51 [3] Scweie i e [] 79 [] ow i e [] 73 [5] osy i e [] 791 [] M Moo J. Phys. (France) C7 17 (19