inelastic x-ray scattering from collective atom...
TRANSCRIPT
theabdus salaminternational centre for theoretical physics
strada costiera, 11 - 34014 trieste italy - tel. +39 040 2240111 fax +39 040 224163 - [email protected] - www.ictp.trieste.it
united nationseducational, scientific
and culturalorganization
international atomicenergy agency
SCHOOL ON SYNCHROTRON RADIATION AND APPLICATIONSIn memory of J.C. Fuggle & L. Fonda
19 April - 21 May 2004
Miramare - Trieste, Italy
1561/22____________________________________________________________
Inelastic X-ray Scattering from
Collective Atom Dynamics
M. Krisch
Inelastic X-ray Scattering fromCollective Atom Dynamics
Michael Krisch
Introduction and Motivation
Inelastic neutron and x-ray scattering
IXS Instrumentation
High frequency collective dynamics of liquid water
Sound velocities in hcp-iron to 110 GPa
Elastic moduli in hcp-cobalt to 25 Gpa
Phonon dispersion in superconductors
European Synchrotron Radiation FacilityGrenoble, France
Aim of IXS (INS) Experiments
Study of phonon(-like) excitations in condensed matter.
Breakdown of the static lattice model
dynamical lattice model
• specific heat• thermal expansion• melting
• T-dependence of DC conductivity• thermal conductivity of insulators• sound transmission• superconductivity
Information obtained from IXS (INS) Experiments
• inter-atomic force constants• sound velocities• thermodynamic properties• dynamical instabilities (phonon softening)• electron-phonon coupling• relaxation phenomena….etc., etc.
X-rays and phonon studies ?
“When a crystal is irradiated with X-rays, the processes of photoelectric absorption and fluorescence are no doubt accompanied by absorption and emission of phonons. The energy changes involved are however so large compared with phonon energies that information about the phonon spectrum of the crystal cannot be obtained in this way.”
W. Cochran in Dynamics of atoms in crystals, (1973)
“…In general the resolution of such minute photon frequency is so difficult that one can only measure the total scattered radiation of all frequencies, … As a result of these considerations x-ray scattering is a far less powerful probe of the phonon spectrum than neutron scattering. ”
Ashcroft and Mermin in Solid State Physics, (1975)
∆E ≈ meV !!!Einc > 10 keV !!!Photon flux ???
• Energy transfer E = Eout – Ein (E<< Ein)
• Momentum transfer Q = kout - kin = 2k sin (ϑ/2) (kout≈kin≡k)
♦ Directional analysis of the scattered photons Q
♦ Energy analysis of the scattered photons E
Scattering kinematics
Ein, kin, εin
Eout , k
out , εout
E, Qϑ
X-ray inelastic cross section
( )∑=−j
jThX trArH ,21 2
0
Electron-photon interaction Hamiltonian
Double-differential cross section
( ) ( )∑ −−∑⋅=∂Ω∂
∂
FIif
j
rQiI EEEIeFP
kkr
Ej
,
2
212
2120
2δεεσ rr
rr
Thomson scattering cross section
(i) Adiabatic approximation:
(ii)
ne SSS =
nene FIFIII ==
The central approximations
For a mono-atomic system:
( ) ( ) ( )EQSQfkkr
E,2
212
2120
2 rrr εεσ⋅=
∂Ω∂∂
Dynamical structure factor
Atomic form factorThomson scattering cross section
The dynamical structure factor
Pair correlation function GP(r,t):GP(r,t) is the probability to find two different particles at positions Rl’(t=0) and Rl’(t), separated by the distance r and the time intervall t.
Dynamical structure factor S(Q,ω):Space and time Fourier transform of GP(r,t).
l l’
The dynamical structure factor
( ) ( ) ( ) ( )∫∫ −= trGrQirdtidtQS ,expexp21, 3 rrr
h
rω
πω
S(Q,ω) is the space and time Fourier transform of the pair correlation function G(r,t).
The pair correlation function
G(r,t) is the probability to find two different particles at positions Rl’(t=0) and Rl(t), and separated by the distance r and the time intervall t.
Q ≈ 2π/ξ ξ is a characteristic length
ω = E/h ≈ 2π/τ τ is a characteristic (relaxation) time
( ) ( )( ) ( )( )∑ −+−∫='.
'3 '0''1,
llll tRrrRrrd
NtrG
rrrrrrr δδ
IXS versus INS
• no correlation between momentum- and energy transfer• ∆E/E = 10-7 to 10-8
• Cross section ~ Z2 (for small Q) • Cross section is dominated by photoelectric absorption (~ λ3Z4)• no incoherent scattering• small beams: 100 µm or smaller
( )EQSkkb
E,
212
2 r=
Ω∂∂∂ σ
INS
• strong correlation between momentum- and energy transfer• ∆E/E = 10-1 to 10-2
• Cross section ~ b2
• Weak absorption => multiple scattering• incoherent scattering contributions• large beams: several cm
IXS ( ) ( ) ( )EQSQfkkr
E,2
21212
0
2 rrr εεσ⋅=
Ω∂∂∂
IXS versus INS: scattering kinematics
λ1 = 1 Å => E1 = 12398 eV E = some meV E1 ≈ E2
λ1 = 1 Å => E1 = 82 meV E = some meV E1 ≠ E2
Energy Transfer:
Neutrons:
X-rays:
=> moderate energy resolution: E/E1 = 0.05
=> extremely high energy resolution: E/E1 = 10-7
IXS versus INS: scattering kinematics
MomentumTransfer:
Neutrons:
X-rays:
=> strong coupling between E and Q inaccessible E-Q region
=> Q only controlled by scattering angle ϑ
( )ϑcos2 2122
21 kkkkQ −+=
( )2sin2 1 ϑkQ =
10-3 10-2 10-1 100 101 10210-4
10-3
10-2
10-1
100
101
102
ILL-BRISP
INS
IXS
IN5
FP (S
ande
rcoc
k) (1
990)
DM
DP
(198
5)H
IRES
UV
prot
otyp
e (2
000)
V=500 m
/sV=7000
m/s
BLS
E (
meV
)
Q ( nm-1)
The Q-E Space of phonon spectroscopies
IXS has advantages in disordered systems with a high speed of sound (vg = Ε/Q)
Where do X-rays complement neutrons?
• In disordered systems with a high speed of sound (vg = E/Q).
Kinematic limitations for INS
• Samples (only available) in small quantities.- novel (exotic) materials (MgB2, …..)- samples under very high pressures
Neutron beams: several cm => signal lossSR beams: 10 - 100 µm, tµ = 10 -100 µm
large high pressure cell => P < 100 kbarDiamond anvil cell => P > 1 Mbar
Cou
nts
per 2
min
utes
Experimental principle
Monochromator
Analyser
Sample
Detector
30 m 40 m 50 m 60 m 70 m
-0.05 m
0.00 m
0.05 m
0.10 m
0.15 m
0.20 m
A
Side View
BCA
BC
FED
0.0 m
0.4 m
0.8 m
1.2 m
Top viewED, F
Beamline Layout ID16 and ID28 at the ESRF
• The x-ray source• High heatload premonochromator (A)• Main monochromator (B)• Focusing mirror (C)• Sample (D)• Analyser (E)• Detector (F)
High Energy Resolution Monochromator
• Silicon (n,n,n) at θB = 89.98°• ωD=∆E/E tan(θB) > sz’, sx’
Reflection Energy [eV] DE [meV] DE/E(7 7 7) 13840 5.3 3.8·10-7
(8 8 8 ) 15817 4.4 2.8·10-7
(9 9 9) 17794 2.2 1.2·10-7
(11 11 11) 21747 1.02 4.7·10-8
(12 12 12) 23725 0.73 3.0·10-8
(13 13 13) 25703 0.5 2.0·10-8
Energy Analysis: The Crystal Analyser
Requirements:
• Perfect single crystal properties (as HR mono)• Collect some solid angle (∆Qapp; flux)
Solution:
• Spherical crystal in Rowland Geometry (∆θ = 0)- R = 2.5 (6.5; 11.5) m- elastic deformation => ∆E/E =
• Approximation to sphere by 10000 0.6x0.6x3 mm3 cubes- preservation single crystal properties- θB = 89.98° to minimise cube size contribution to ∆E/E
-6 -4 -2 0 2 4 60
100
200
300
400
500
600
2f)Si(13,13,13)E = 25702 eV∆E = 0.87 ± 0.04 meV∆E/E =3.4·10-8
Inte
nsity
(a.u
.)
Energy (meV)
The Analyser in real life
Best Resolution so far obtained:
HR Mono: Energy Scans via Temperature Scans
λ = 2·d(T) sinθB∆d/d = -α(T)·∆T (α=2.58·10-6 at RT)
• Temperature controlled by AC Thermometer bridge∆Tmin = 0.25 mK∆Ttyp = 3, 5, 10, 15 mK/minute
The IXS spectrometers (schematics)
Side view
θsTop view
6.5 m
Q = 4π/λ·sin(θs/2)
detector analysers
sample
3 mm
5-Analyser Assembly
Analyser crystal
T-control mount
Goniometry (ath,achi)
0
100
200
300
400fit.outQ = 2 nm-1
T = 171 K
Glycerol
1
BG = 5.74086 +/- 0.43727SL = 0.17173 +/- 0.04063ZR = (-0.05627) +/- 0.01126PC = 811.0458 +/- 17.41197GC = 0.05275 +/- 0.01182PL = 172.9469 +/- 11.99725OL = 4.03667 +/- 0.04203GL = 0.11458 +/- 0.09244
VL = 3075.943 +/- 32.0274Ianel / Iel = 0.21379
χ2 = 116.1882
µχ
2 = 96 σ
χ2 = 13.85641
Inte
nsity
( c
ount
s )
-20 -15 -10 -5 0 5 10 15 200
50
100
2
Energy ( meV )
-0.10 -0.05 0.00 0.05 0.10
-0.10
-0.05
0.00
0.05
0.10 3
∆ΓL
∆ΩL
-0.10 -0.05 0.00 0.05 0.10
-10
-5
0
5
10 4
∆P C
∆P L
∆ΩL
-0.10 -0.05 0.00 0.05 0.10-0.015
-0.010
-0.005
0.000
0.005
0.010
0.015
5
∆ΩL
∆ΓC
-0.10 -0.05 0.00 0.05 0.10
-15
-10
-5
0
5
10
15 6
∆ΩL
-20 -15 -10 -5 0 5 10 15 20
-2
0
27
Example of IXS spectrum and of data analysis
Si(11,11,11)∆E = 1.5 meV at 21747 eV8 hours accumulation
Data Analysis:Damped Harmonic Oscillator
0.36° -0.36°
The high-frequency dynamics of liquid water
1993 - 2004
Some key references:
J. Teixeira et al.; Phys. Rev. Lett. 54, 2681 (1985)G. Ruocco and F. Sette; J.Phys.: Condens.Matter 11, R259 (1999)M. Krisch et al.; Phys. Rev. Lett. 89, 125502 (2002)
INS and Molecular Dynamics Results(as of 1993)
Origin and nature of these two excitations?
0 2 4 6 8 10 120
10
20 MD Rahman et al. [9] " INS Bosi et al. [10] INS Teixeira et al. [11]
E (
meV
)
Q ( nm-1 )
IXS results with ∆E = 5 meV
Damped harmonic oscillator
( ) ( )[ ] ( ) ( ) ( )
( )[ ] ( ) 22222
21,
ωω
ωωωQQ
QQQInQFΓ+−Ω
ΩΓ+=
Dispersion relation for water at 5º C
• Confirmation of the existence of the “fast sound”.• Excitation involves the center of mass of the molecule.
No clear evidence for low energy excitations!
0 2 4 6 8 10 120
5
10
15
20
25
D2O INS Teixeira et al. [11] H
2O IXS Sette et al. [31]
E (m
eV)
Q (nm-1)
IXS results with ∆E = 1.5 meV
-10 0 10 20
E (meV)
E (meV)
Q=10.0 nm-1
Q=4.0 nm-1
Inte
nsity
( a
rb. u
nits
)
Energy (meV)
-5 0 5 10
-5 0 5 10
-5 0 5 10
0.5
0.5
0.5
0.0
0.0
0.0
0.5
0.0
Q=2.5 nm-1
2.0 nm-1
1.5 nm-1
1.0 nm-1
Inte
nsity
(ar
b. u
nits)
Energy (meV)
Complete dispersion relation for water at 5º C
• Existence of two sounds: v0 = 1500 m/s and v∞ = 3200 m/s• The “fast sound” is the continuation of the “hydrodynamic” sound. • The low energy mode only visible once the “fast sound” value is reached.
0 2 4 6 80
5
10
15
20
0 1 2 3 40
2
4
6
8
Ω (Q
) (m
eV)
Q (nm-1)
vinf=3200 m/s
v0 = 1500 m/s
Signature of a structural relaxation process (“fast” α-relaxation)
Low-frequency viscous regime (Ωτ << 1): liquid-like responsehigh-frequency elastic regime (Ωτ >> 1): solid-like response
Ωτ ≈ 1: Coupling of the phonon-like excitations with structural rearrangements.
E ≈ 3.3 meV τ = h/E = 1.3 psQ = 2 nm-1 ξ = 3.1 nm
Time and length scale can be associated withthe formation and breaking of hydrogen bond networks.
Q = 4 nm-1
-10 0 10
0.0
0.5
1.0
1.5
Intn
esit
y (
cou
nt /
s )
T = 314 K0.0
0.5
1.0
1.5
2.0
2.5Q = 2 nm-1
Energy ( meV )
T = 266 K
-10 -5 0 5 100.0
0.5
1.0
1.5
2.0 T = 413 K 0 2 4 6 8 10 12 140
5
10
15
20
25 T = 278 K T = 373 K T = 493 K
Ener
gy (
meV
)
Q ( nm-1 )
Fast sound transition as a function of T
Relaxation time τ(T) from: Ωtrans(T) τ=1
2,0 2,5 3,0 3,5 4,0
10-1
100
- Arrhenius behavior: ∆E = 2.3 + 0.2 kcal / mole
- Hydrogen bond in water : EHB
= 5 kcal / mole
∆E = 2.3 + 0.2 kcal / mole
IXS (const Q) IXS (const T)
333 250500
τ (
ps )
1000 / T ( K-1 )
-15 -10 -5 0 5 10 150
50
100
150
T=277 KP=3.8 kBar
2 nm -1
Energy ( meV )
0
50
100
150
3 nm -1
0
50
100
150
4 nm -1
0
50
100
150
5 nm -1
0
100
200
300In
tens
ity
( nor
mal
ized
uni
ts )
Q = 6 nm -10 2 4 6 8
0
5
10
15
20v=3320 (40) m/s Ω(Q) (meV)
Q (nm-1)
Large volume cellV = 20 mm3
∆E=1.5 meV, Si (11,11,11)
-25 -20 -15 -10 -5 0 5 10 15 20 250
20
40
60
T=297 KP=7.9 kBar
3 nm -1
Energy ( meV )
010203040
4 nm -1
0
20
40
60
5 nm -1
0
20
40
60
6 nm -1
0
50
100
150
Inte
nsity
( n
orm
aliz
ed u
nits
)
Q = 8 nm -10 2 4 6 805101520
25v=3540 (60) m/s Ω(Q) (meV)
Q (nm-1)
Diamond anvil cellV = 0.04 mm3
∆E=3.0 meV, Si (9,9,9)
Water under pressure
Density dependence of sound velocity
• cIXS and c0 approach each other.• cIXS shows anomalous behavior at density, ρ~1.12 gcm-3
1,01,0 1,2 1,4
2
3
4
cIXS
T=277 K c
IXS T=297 K
cIXS
T=410 K c
0 T=277 K
c0 T=297 K
c0 T=410 K
Soun
d ve
loci
ty (k
m/s
)
Density (g/cm3)
• LVC
• DAC
1,0 1,1 1,2 1,3 1,4 1,5 1,61
2
3
4
5
(vix
s/v0)2
ρ [g/cm3]
• Decreasing role of H-bond network for water dynamics.• Water becomes a simple liquid.• ρ = 1.12 g/cm3 seems to mark transition region.
Pressure dependence of vIXS/v0
Geophysical applications of IXS
Jephcoat/RefsonNature 413,28 (2001)
• Earth’s shells• Earth’s composition• Earth’s dynamics
PHASE DIAGRAM OF IRONhcp –iron: the main constituent of Earth’s inner core
Determination of sound velocities• Comparison with seismic results• constraining compositional models • texturing mechanisms
Gasket
Sample
RubyDiamond anvil cell (DAC) techniques
1200 1250 1300 1350 1400 1450 1500 1550 16000
5000
10000
15000
20000
25000
30000
R2
R1
D
Inte
nsità
(u.
a.)
∆ν (cm-1)
Pressure measurement by frequency shift of ruby fluorescence
0 100 200 300 4000
100
200
300
400
500
Righa R1
∆ν
Hydrostatic - - -
Non Hydrostatic ........
dP/dν=1.3177 Kbar/cm-1
dν/dP=0.7589 cm-1/Kbarν(P=0)=14405 cm-1
∆P (K
bar)
polycrystalline ε (hcp)-iron
10 20 30 40 50
Inte
nsity
[a.u
.]
Energy [meV]
hcp iron at 28 GPa
0
10
20
30
40
50
60
0 2 4 6 8 10 12 14En
ergy
[meV
]Q [nm-1]
G. Fiquet, J. Badro, F. Guyot, H. Requardt and M. Krisch; Science 291, 468 (2001)
( )2/1
maxcos1 ⎥
⎦
⎤⎢⎣
⎡∑ ⎟⎟
⎠
⎞⎜⎜⎝
⎛⎟⎟⎠
⎞⎜⎜⎝
⎛−⋅=
n QQnIQE π
(C*)
• ∆E = 5.5 meV at 15816 eV• focal size: 250 x 70 µm2 (FWHM)
ID 28
VP and VS as a function of density
9000 10000 11000 12000 13000
4000
6000
8000
10000
12000 IXS PREM
VS
VP
S
ound
Vel
ocity
[m/s
]
Density [Kg/m3]
ρ
ρ
/
/34
2
2
Gv
GKv
s
p
=
⎟⎠⎞
⎜⎝⎛ +=
D. Antonangeli et al; submitted to Earth and Planetary Science Letters (2004)
9000 10000 11000 12000 13000
4000
6000
8000
10000
12000
PREM NRIXS XRD Shock US PREM XRD
VS
VP
Soun
d Ve
loci
ty [m
/s]
Density [Kg/m3]
Comparison with other experimental techniques
• Good agreement between very different experimental techniques.- stringent test for theoretical approaches
• Shock results yield systematically lower VP’s.- VP(ρ,T)- Evidence that ε-iron VP too low w/r to PREM
different iron phase?presence of light elements?
• Strong temperature effect on VS- partial melting of the core?- strong T-dependence of shear modulus G close to melting
(confirmed by calculations: Laio et al.; Science 287, 1027, 2000)
Conclusions
single crystals:
Limitations of polycrystals- orientationally averaged sound velocities
- no transverse modes
- all elastic moduli (constants)
hcp-Co
hcp-Co five independent elastic moduli: C11, C33, C44, C12, C13
3321
33 1 )001( C
CVLA →⎟⎟
⎠
⎞⎜⎜⎝
⎛=→
ρ
1121
11 1 )100( C
CVLA →⎟⎟
⎠
⎞⎜⎜⎝
⎛=→
ρ
( )12116621
66100 2
1 1 )110( CCCCV
LA −=→⎟⎟⎠
⎞⎜⎜⎝
⎛=→
ρ
4421
44001 1 )110( C
CVTA →⎟⎟
⎠
⎞⎜⎜⎝
⎛=→
ρ
( ) 131312443311 ,,,,f )101( CCCCCCLA →→
hcp-cobalt as an analogue to hcp-ironThesis work of Daniele Antonangeli
-5 0 5 10 15 20 25 3 0
300
350
400
450
500
550
600
elastic constan t: C33
δC33
/δP= 7.85 +/- 0.36 C33(P =0)= 339 +/-6 GPa
u ltrasonic measurements
Ela
stic
con
stan
ts (
GP
a)
P (GPa)
-5 0 5 10 15 2 0 25 30
70
80
90
100
110
120
130
elastic constant: C44
δC4 4/δP= 1.58 +/-0.18 C44(P=0)= 78 +/-2 GPa
ultra sonic mea sure ments
Ela
stic
cons
tant
(GPa
)
P (GPa)
-5 0 5 10 15 2 0 25 30
60
70
80
90
100
110
120
130
140
150
elastic constant: C 66
δC66
/δP= 2.6 +/- 0.2 C
66(P=0)= 71 +/-1 GPa
ultra sonic me asure men ts
Ela
stic
con
stan
t (G
Pa)
P (GPa)
-5 0 5 10 15 2 0 25 30260
280
300
320
340
360
380
400
420
440
460
480
elastic constant: C11
δC11/δP= 5.32 +/-0.3 7 C
11(P=0)= 29 4 + /-2 GPa
ultra sonic me asure men ts
Ela
stic
con
stan
t (G
Pa)
P (GPa)
0 10 20 30 40 50 60 70 80 9 0
6.2
6.4
6.6
6.8
7.0
7.2 P~ 14 GPa (V=7 0.0 Bohr3) IX S m easurem ents confid ence level (2 σ ) Steinle-Neum ann GGA Steinle-Neum ann LDA
ac
soun
d ve
loci
ty (K
m/s
)
direc tion respect c- axes (degree)
Ref.:Steinle-Neumann et al., Phys. Rev. B, 60, 791, (1999)
Comparison of IXS with theory
Phonon dispersion in Nd1.86Ce0.14CuO4+δ
M. D’Astuto et al.; Phys. Rev. Lett. 88, 167002 (2002)
Electron-phonon coupling in electron-doped high Tc superconducting cuprates?
Explanation of particle-hole asymmetry
Z.-X. Shen (2001)
Angle-resolved photoemission studies: Discontinuity in the quasi-particle dispersion.INS on hole-doped systems (La1.85Sr0.15CuO4): Anomalous softening of LO phonons.
Doping x
• Renormalisation of the highest LO branch with respect to undoped compound.• Anomalous softening of the highest LO branch.
=>Strong evidence for e-ph coupling as well in electron doped cuprates.
T = 15 KV = 5·10-3 mm3
Phonon dispersion in MgB2A. Shukla et al.; Phys. Rev. Lett. 90, 095506 (2003)
A selection of other investigated Systems
Liquids and glasses
- Teflon, Polyethylene (high presssure)- Na, Si, Ge, Sn (high temperature)- SiO2, aSi- H2, D2- glycerol, polybutadiene, salol,…….- water
Polycrystals- Ice IX, XII- Fe, FeS, FeO, FeSi (high pressure)
Single crystals
- Ice VI,VII; CH4-H2O (high pressure)- Co, Zn,Ta,Mo (high pressure)- SrTiO3 (high pressure)- SmS (high pressure) - C12,C13,GaN, SiC (ZB), ZnMgY- NbSe3, Pu- Nd1.86Ce0.14CuO4+δ, LaSrCuO4, HgBa2CuO4