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Title: Phonons and Inelastic neutron and Xray Scattering


1
Phonons and Inelastic neutron and X-ray Scattering
  • Paolo Ghigna, Dipartimento di Chimica Fisica M.
    Rolla, Università di Pavia

2
Summary
  • The study of atomic dynamics in condensed matter
    at momentum transfers, Q, and energies, E,
    characteristic of collective motions is,
    traditionally, the domain of neutron
    spectroscopies.
  • The experimental observable is the dynamic
    structure factor S(Q,E), which is the space and
    time Fourier transform of the density-density
    correlation function.
  • Neutrons as probing particle are particularly
    suitable, since
  • the neutron-nucleus scattering cross-section is
    sufficiently weak to allow for a large
    penetration depth,
  • the energy of neutrons with wavelengths of the
    order of inter-particle distances is about 100
    meV, and therefore comparable to the energies of
    collective excitations associated to density
    fluctuations such as phonons, and
  • the momentum of the neutron allows to probe the
    whole dispersion scheme out to several Ã…-1, in
    contrast to inelastic light scattering techniques
    such as Brillouin and Raman scattering which can
    only determine acoustic and optic modes,
    respectively, at very small momentum transfers.

3
What is a phonon?
  • In physics, a phonon is a quantized mode of
    vibration occurring in a rigid crystal lattice,
    such as the atomic lattice of a solid. Phonon can
    also be used to describe an exitation of such a
    mode. The study of phonons is an important part
    of solid state physics, because phonons play an
    important role in many of the physical properties
    of solids, such as the thermal conductivity and
    the electrical conductivity. In particular, the
    properties of long-wavelength phonons gives rise
    to sound in solids -- hence the name phonon. In
    insulating solids, phonons are also the primary
    mechanism by which heat conduction takes place.
  • Phonons are a quantum mechanical version of a
    special type of vibrational motion, known as
    normal modes in classical mechanics, in which
    each part of a lattice oscillates with the same
    frequency. These normal modes are important
    because, according to a well-known result in
    classical mechanics, any arbitrary vibrational
    motion of a lattice can be considered as a
    superposition of normal modes with various
    frequencies in this sense, the normal modes are
    the elementary vibrations of the lattice.
    Although normal modes are wave-like phenomena in
    classical mechanics, they acquire certain
    particle-like properties when the lattice is
    analysed using quantum mechanics (see
    wave-particle duality.) They are then known as
    phonons. Phonons are bosons possessing zero spin.

4
X-rays as a probe of phonons
  • While it has been pointed out that X-rays can in
    principle as well be utilised to determine the
    S(Q,E), it was stressed that this would represent
    a formidable experimental challenge, mainly due
    to the fact that an X-ray instrument would have
    to provide an extremely high energy resolution.
    This is understood considering that photons with
    a wavelength of l0.1 nm have an energy of about
    12 keV. Therefore, the study of phonon
    excitations in condensed matter, which are in the
    meV region, requires a relative energy resolution
    of at least DE/E10-7.
  • On the other hand, there are situations where the
    use of photons has important advantages over
    neutrons. A specific case is based on the general
    consideration that it is not possible to study
    acoustic excitations propagating with a speed of
    sound vs using a probe particle with a speed v
    smaller than vs.
  • This limitation is not particularly relevant in
    neutron spectroscopy studies of crystalline
    samples. Here, the translation invariance allows
    to study the acoustic excitations in high order
    Brillouin zones, thus overcoming the above
    mentioned kinematic limit on phonon branches with
    steep dispersions.
  • On the contrary, the situation is very different
    for topologically disordered systems such as
    liquid, glasses and gases. In these systems, in
    fact, the absence of periodicity imposes that the
    acoustic excitations must be measured at small
    momentum transfers. Thermal neutrons have a
    velocity in the range of 1000 m/s, and only in
    disordered materials with a speed of sound
    smaller than this value (mainly fluids of heavy
    atoms and low density gases) the acoustic
    dynamics can be effectively investigated.
  • Another advantage of the inelastic X-ray
    technique arises from the fact that very small
    beam sizes of the order of a few tens of
    micrometers can be presently obtained at third
    generation synchrotron sources. This allows to
    study systems available only in small quantities
    down to a few 10-6 mm3 and/or their investigation
    in extreme thermodynamic conditions, such as very
    high pressure. These differences with respect to
    inelastic neutron scattering motivated the
    development of the very high resolution inelastic
    x-ray scattering (IXS) technique, and following
    the pioneering experiments in 1986, the IXS
    technique rapidly evolved. To date there are four
    instruments operational at the ESRF (2), APS (1)
    and Spring-8 (1), and several more under
    construction.

5
What is a phonon?
  • Due to the connections between atoms, the
    displacement of one or more atoms from their
    equilibrium positions will give rise to a set of
    vibration waves propagating through the lattice.
    One such wave is shown in the figure below. The
    amplitude of the wave is given by the
    displacements of the atoms from their equilibrium
    positions. The wavelength ? is marked.
  • It should be noted that there is a minimum
    possible wavelength, given by the equilibrium
    separation a between atoms. As we shall see in
    the following sections, any wavelength shorter
    than this can be mapped onto a wavelength longer
    than a.
  • Not every possible lattice vibration has a
    well-defined wavelength and frequency. However,
    the normal modes (which, as we mentioned in the
    introduction, are the elementary building-blocks
    of lattice vibrations) do possess well-defined
    wavelengths and frequencies. We will now examine
    these normal modes in some detail.

6
Inelastic Scattering
  • We will consider inelastic scattering where there
    is a change in the energy of the scattered beam
    with respect to the incident beam due to
    interactions of the incident wave with the
    sample.
  • This has proved to be a fruitful area of
    investigation, particularly with neutrons where
    the energy of thermalised neutrons is comparable
    to that of phonons. This was recently recognised
    in the award of the 1995 Nobel Prize in Physics.

7
Optical, Acoustic, Transverse, Longitudinal Phonon
  • In real solids, there are two types of phonons
    "acoustic" phonons and "optical" phonons.
    "Acoustic phonons", which are the phonons
    described above, have frequencies that become
    small at the long wavelengths, and correspond to
    sound waves in the lattice. Longitudinal and
    transverse acoustic phonons are often abbreviated
    as LA and TA phonons, respectively.
  • "Optical phonons," which arise in crystals that
    have more than one atom in the unit cell, always
    have some minimum frequency of vibration, even
    when their wavelength is large. They are called
    "optical" because in ionic crystals (like sodium
    chloride) they are excited very easily by light
    (in fact, infrared radiation). This is because
    they correspond to a mode of vibration where
    positive and negative ions at adjacent lattice
    sites swing against each other, creating a
    time-varying electrical dipole moment. Optical
    phonons that interact in this way with light are
    called infrared active. Optical phonons which are
    Raman active can also interact indirectly with
    light, through Raman scattering. Optical phonons
    are often abbreviated as LO and TO phonons, for
    the longitudinal and transverse varieties
    respectively.

8
High Energy X-ray Inelastic Scattering
  • Ever since the epoch-making DuMond experiments on
    beryllium, which provided the first evidence for
    the validity of Fermi-Dirac as opposed to
    Maxwell-Boltzmann electron momentum
    distributions, inelastic x-ray scattering has
    been established as a probe of the ground state
    properties of electrons in solids.
  • Inelastic scattering refers to a number of
    interactions between x-rays and atoms in which
    the energy of the scattered photon is less than
    that of the incident one. The term high energy
    indicates the relative magnitude of the incident
    photon energy in comparison to the electron
    binding energy.
  • Amongst the effects are the Compton effect,
    plasmon scattering (or collective excitation),
    x-ray Raman, x-ray resonant Raman and phonon
    scattering. In a typical scattering experiment an
    incident beam of photons of energy hn1 and
    wavevector k1 is scattered by the sample into a
    beam of photons of average energy hn2 and
    wavevector k2. The spectral distribution then
    provides information about the electronic
    structure of the sample.
  • One advantage of this type of experiment is that
    the scattering probe is a quasi-particle of
    energy hn h(n1-n2 ) and momentum (h/2p)k
    (h/2p)(k1-k2) and the functional dependence
    between k and w is multi-valued and can be
    tuned appropriately to study a desired
    interaction. Large momentum transfers correspond
    to Compton scattering providing information on
    the ground state momentum of the individual
    electrons.

9
High Energy X-ray Inelastic Scattering
  • Intermediate and low momentum transfer are
    governed by the differential scattering cross
    section
  • where e (w,k) is the dynamic dielectric function
    and S(w,k), the dynamic structure factor provides
    information about the correlation of the valence
    electrons in space and time. For the core
    electrons x-ray Raman spectra provide information
    about the density of states near the Fermi energy
    and many body effects while x-ray resonant Raman
    and phonon inelastic scattering can provide
    details of the spin dependent momentum
    distribution

10
X-ray Inelastic Scattering
  • DuMond (in 1929!) developed from first
    principles, a relation between the electron
    momentum distribution I(p) of an isotropic
    ensemble of electrons and the spectrum of a
    monochromatic x-ray beam inelastically scattered
    by them. This relation
  • which leads to
  • DuMonds experimental spectra of Be were clearly
    most similar to (i) which was the first direct
    evidence for the validity of the Fermi-Dirac
    electron momentum distribution.

11
Inelastic Neutron Scattering
  • This is the principle technique for determining
    phonon dispersion curves and is of major
    importance in the study of phonons generally.
  • Thermal neutrons (i.e. those in the meV energy
    range) have both the right energy and wavevector
    to interact with phonons. This is in marked
    contrast to other probes such as infrared
    radiation (where the energy is similar but
    (h/2p)k is only a very small fraction of the
    Brillouin zone boundary, and hence only phonons
    with k?0 can be measured) or x-rays ( where
    (h/2p)k can be of the correct order but the
    energy is many orders of magnitude larger than
    that of phonons).
  • Note that a lattice vibration of angular
    vibration w connotes the movement of phonons,
    each with energy hn and crystal momentum (h/2p)k
    . Use of the term crystal momentum does not mean
    that ordinary momentum is transferred through the
    crystal at the corresponding rate, but crystal
    momentum is a conserved quantity in interactions
    involving the creation or annihilation of crystal
    phonons.

12
Inelastic Neutron Scattering
  • A neutron of velocity v has a wavevector and
    kinetic energy
  • Suppose that in either absorbing or creating a
    phonon, the energy and wavevector of the neutron
    are changed to E and Kn respectively. Then the
    angular frequency w and wavevector k of the
    phonon involved will be related by the
    conservation equations
  • The vector G is either zero or a reciprocal
    lattice vector and can be included since a phonon
    of wavevector k is identical to a phonon of any
    (kG). The positive signs in are for the creation
    of a phonon (Stokes process) and the negative
    signs for the annihilation (anti-Stokes) of a
    phonon.

13
Inelastic Neutron Scattering
14
Triple-axis spectrometer
  • The beam of neutrons is monochromated to the
    desired wavelength via Bragg reflection of a
    crystal monochromator. After the beam is
    scattered by the sample an analyser crystal is
    adjusted so that it Bragg reflects a defined
    energy of the scattered neutrons towards the
    detector.
  • In the triple-axis spectrometer the incident
    energy can be kept constant by keeping qM
    constant. The scattered energy is adjusted by
    changing qA, but the consequent change in ½k½
    can be compensated by simultaneously altering the
    scattering angle f to keep ½K½½k-k½ constant
    also the angle y of the sample can be varied so
    that K maintains its orientation with respect to
    the crystal axes. Thus by simultaneously changing
    the three angles qA, f and y, it is possible to
    investigate the variation of neutron count rate
    with the energy E of the scattered neutrons at
    fixed values of the incident neutron energy E and
    scattering vector K.

15
Phonon dispersion curves
  • The technique can thus be applied to measuring
    the phonon frequencies as a function of
    wavevector throughout the Brillouin zone of the
    material. The figures display the results for two
    f.c.c metals and for f.c.c silicon which has two
    atoms in the basis and thus displays both
    acoustic and optic branches in the Brillouin zone

16
Comparison IXS versus INS
  • Similarities and differences between the IXS and
    INS cross section are summarised below
  • Q - E limitation for INS
  • Small beam size for IXS
  • X-rays couple to the electrons of the system with
    a cross-section proportional to the square of the
    classical electron radius, ro2.82x10-13 cm, i.e.
    with a strength comparable to the neutron-nucleus
    scattering cross-section b.
  • The IXS cross section is proportional to fj(Q)2.
    In the limit Q?0, the form factor is equal to the
    number of electrons in the scattering atom, Z
    for increasing values of Q, the form factor
    decays with decay constants of the order of the
    inverse of the atomic wavefunction dimensions of
    the electrons in the atom.
  • The total absorption cross-section of X-rays
    above 10 keV energy is limited in almost all
    cases (Zgt4) by the photoelectric absorption
    process, and not by the Thomson scattering
    process. The photoelectric absorption, whose
    cross-section is roughly proportional to Z4,
    determines therefore the actual sample size along
    the scattering path. Consequently the Thomson
    scattering channel is not very efficient for
    system with high Z in spite of the Z2 dependence
    of its cross-section.
  • As a consequence, multiple scattering processes
    can in general be neglected
  • The magnetic cross section is negligible for IXS,
    whereas it is comparable to the nuclear cross
    section for neutrons.
  • The IXS cross section is highly coherent
  • The shape of the IXS instrumental energy
    resolution is not Gaussian as it is for a neutron
    triple-axis spectrometer, but Lorentzian.

17
General optical lay-out
  • The optical lay-out is based on the triple-axis
    principle, composed of the very high energy
    resolution monochromator (first axis), the sample
    goniometry (second axis) and the crystal analyser
    (third axis). The figure below shows a schematic
    view of the optics and the distances involved.
    Due to the backscattering geometry the beamline
    is fairly long in order to acquire a sufficient
    beam offset between the incident photon beam from
    the X-ray source and the focused very high-energy
    resolution beam at the sample position

18
Backscattering monochromator
  • The main monochromator consists of a flat perfect
    single crystal, operating at a Bragg angle of
    89.98º and utilising the silicon (n,n,n,)
    reflection orders. This close-to-exact-backscatter
    ing configuration insures that the spectral
    angular acceptance, the so-called Darwin width,
    is larger than the x-ray beam divergence, and
    therefore that all the photons within the desired
    energy bandwidth are transmitted. The crystal is
    temperature controlled in the mK region by a high
    precision platinum 100W (Pt100) thermometer
    bridge in closed-loop operation with a PID
    controlled heater unit. The complete electronic
    unit was purchased from Automatic Systems
    Laboratory (Milton Keynes, England).
  • The energy scans are performed by varying the
    temperature of the monochromator and keeping the
    temperature of the analyzer fixed.

19
Very high energy resolution spherical crystal
analyzer
  • Although the required energy resolution is the
    same for the monochromator and the analyser,
    there is a big difference concerning their
    angular acceptance. The spatial angular
    acceptance of the monochromator should be
    compatible with the divergence of the synchrotron
    beam, whereas the analyser must have a much
    larger angular acceptance, which is only
    restricted by the required Q resolution. An
    angular acceptance up to 4x10mrad2 is an adequate
    compromise of Q-resolution and signal
    maximisation. These constraints necessitate
    focusing optics. Since it is not possible to
    elastically bend a crystal without introducing
    important elastic deformations, which in turn
    deteriorate the intrinsic energy resolution, one
    has to position small, unperturbed crystals onto
    a spherical substrate with a radius, fulfilling
    the Rowland condition. This polygonal
    approximation to the spherical shape yields the
    intrinsic energy resolution, provided the
    individual crystals are unperturbed and the
    geometrical contribution of the cube size to the
    energy resolution is negligible. The solution
    realised at the ESRF consists of gluing 12000
    small crystals of 0.6x0.6x3 mm3 size onto a
    spherical silicon substrate. This procedure,
    yield very good results, and provided the record
    energy resolution of 0.9 meV, utilising the
    silicon (13,13,13) reflection order at 25704 eV.
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