Melting of Iron at Earth’s core conditions from quantum Monte Carlo free energy calculations...
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Melting of Iron at Earth’s core conditions from quantum Monte Carlo free energy calculations
Department of Earth Sciences & Department of Physics and Astronomy,
Materials Simulation Laboratory & London Centre for Nanotechnology
University College London
Dario ALFÈ
• Birch (1952) - “The Core is iron alloyed with a small fraction of lighter elements”
2 4 6 8 10 12
4
6
8
10
Al Ti
Cr
Fe
Sn Ag
Mantle Core
V(km/s)
Density (g/cc)
• Nature of light element inferred from:
•Cosmochemistry
•Meteoritics
•Equations of state
Core composition
Temperature of the Earth’s core
• Exploit solid-liquid boundary
• Exploit core is mainly Fe• Melting temperature of Fe
Thermodynamic melting
F(V ,T ) = Fperf (V ,T) + Fharm(V ,T) + Fanharm(V ,T)
Fharm
(V ,T ) = 3kBT 1
Nq,s
ln 2sinhhωq,s(V ,T)
2kBT
⎛
⎝⎜
⎞
⎠⎟
⎡
⎣⎢⎢
⎤
⎦⎥⎥q,s
∑
The Helmholtz free energy
Solids: Low T
Phonons of Fe
F(V ,T ) = Fperf (V ,T) + Fharm(V ,T) + Fanharm(V ,T)
Fharm
(V ,T ) = 3kBT 1
Nq,s
ln 2sinhhωq,s(V ,T)
2kBT
⎛
⎝⎜
⎞
⎠⎟
⎡
⎣⎢⎢
⎤
⎦⎥⎥q,s
∑
The Helmholtz free energy
Solids:
Liquids:
F(V ,T ) = −kBT ln
1N!Λ3N
dR e−U (R)/kBT
V∫
Low THigh T
Fλ = −kBT ln
1N!Λ3N
dR e−Uλ (R)/kBT
V∫
U
ref, F
ref Uλ =(1−λ)Uref +λU
F − Fref = dλ
dFλ
dλ0
1
∫
dFλ
dλ=
dR ∂Uλ
∂λe−Uλ (R)/kBT
V∫
dR e−Uλ (R)/kBT
V∫
=∂Uλ
∂λλ
= U −Uref λ
Thermodynamic integration
F = Fref + dλ ⟨U0
1
∫ −Uref ⟩λ
Example: anharmonic free energy of solid Fe at ~350 GPa
F =Fharm+ dλ ⟨U
0
1
∫ −Uharm⟩λ F =Fharm+ dλ ⟨U
0
1
∫ −Uharm⟩λ =Fharm+ dtdλdt
U −Uharm( )λ0
T
∫
Improving the efficiency of TI
F = Fref + dλ ⟨U
0
1
∫ −Uref ⟩λ
F is independent on the choice of Uref , but for efficiency choose Uref such that:
⟨(U − Uref −⟨U −Uref ⟩)
2 ⟩
is minimum. For solid iron at Earth’s core conditions a good Uref is:
U
ref = c1Uharm + c2U IP
UIP=12
A
ri −rj
Bi≠j∑ ; B=5.86
U
harm =
12
uiαΦiα , jβujβiα , jβ∑
Improving the efficiency of TI (2)
U
ref = c1Uharm + c2U IP
At high temperature we find c1 = 0.2, c2 = 0.8
F independent on choice of Uref, but for efficiency choose Uref such that
is minimum.For liquid iron a good Uref is:
⟨(U − Uref −⟨U −Uref ⟩)
2 ⟩
Uref
=12
A
ri −rj
αi≠j∑
Free energy for liquid Fe:
F = Fref + dλ ⟨U
0
1
∫ −Uref ⟩λ
Liquid Fe
Uref
=12
A
ri −rj
Bi≠j∑
B=5.86
ΔT ≈100 K → ΔG ≈10 meV / atom
Size tests
0 0
1( )
2 H H Hp V V E E− = −
Hugoniot of Fe
Alfè, Price,Gillan, Nature, 401, 462 (1999); Phys. Rev. B, 64, 045123 (2001);
Phys. Rev. B, 65, 165118 (2002); J. Chem. Phys., 116, 6170 (2002)
The melting curve of Fe
NVE ensemble: for fixed V, if E is between solid and liquid values, simulation will give coexisting solid and liquid
Melting: coexistence of phases
QuickTime™ and aH.264 decompressor
are needed to see this picture.
Alfè, Price,Gillan, Nature, 401, 462 (1999); Phys. Rev. B, 64, 045123 (2001);
Phys. Rev. B, 65, 165118 (2002); J. Chem. Phys., 116, 6170 (2002)
The melting curve of Fe
Free energy approach and Coexistence give same result (as they should !)
Thermodynamic integration, a perturbative approach:
F = Fref + dλ ⟨U0
1
∫ −Uref ⟩λ
U −Uref λ= U −Uref λ=0
+λ∂ U −Uref λ
∂λλ=0
+o(λ2 )
∂ U −Uref λ
∂λ=
∂∂λ
dR U −Uref( )e−Uλ (R)/kBT
V∫
dR e−Uλ (R)/kBT
V∫
⎧
⎨
⎪⎪
⎩
⎪⎪
⎫
⎬
⎪⎪
⎭
⎪⎪
=
−1
kBT
dR U −Uref( )2e−Uλ (R)/kBT
V∫
dR e−Uλ (R)/kBT
V∫
−dR U −Uref( ) e
−Uλ (R)/kBT
V∫
dR e−Uλ (R)/kBT
V∫
⎛
⎝
⎜⎜⎜⎜
⎞
⎠
⎟⎟⎟⎟
2⎧
⎨
⎪⎪
⎩
⎪⎪
⎫
⎬
⎪⎪
⎭
⎪⎪
=−1
kBTδΔUλ
2
λ
U −Uref λ
= U −Uref λ=0−
λkBT
δΔU02
0+o(λ2 )
δΔUλ =U −Uref − U −Uref λ
dλ
0
1
∫ U −Uref λ; U −Uref λ=0
−1
2kBTδΔU0
2
0
Only need to run simulations with one potential (the reference potential for example).
Melting of Fe from QMC:
Free energy corrections from DFT to QMC:
δTm =ΔG ls (Tm
ref )
Srefls
QMC on Fe, technical details
• CASINO code: R. J. Needs, M. D. Towler, N. D. Drummond, P. Lopez-Rios, CASINO user manual, version 2.0, University of Cambridge, 2006.
• DFT pseudopotential, 3s23p64s13d7 (16 electrons in valence)
• Single particle orbitals from PWSCF (plane waves), 150 Ry PW cutoff. Then expanded in B-splines.
ΨT (R) =exp[J (R)]D↑{φi (r j )}D
↓{φi (r j )}
(D. Alfè and M. J. Gillan, Phys. Rev. B, 70, 161101(R), (2004))
Blips
ψ n(r) = anj
j∑ Θ j (r)
Storing the coefficients: • avc(x,y,z,ib) [old]• avc(ib,x,y,z) [new]
New is faster on large systems, but slower on small systems (cutoff ~ 250 electrons)
Solid (h.c.p.) Fe, finite size Ester Sola
Solid Fe, equation of state at 300 K
QMC correction to the DFT Fe melting curve
δTm =ΔG ls (Tm
ref )
Srefls = 500 ± 200
ΔG ls (Tmref ) = 0.05 ± 0.02 eV/atom
QMC correction to the DFT Fe melting curve
δTm =ΔG ls (Tm
ref )
Srefls = 500 ± 250
ΔG ls (Tmref ) = 0.05 ± 0.025 eV/atom
Conclusions
• Melting temperature of Fe at 330 GPa = 6800 +- 400 K
• Melting point depression due to impurities ~ 800 K
• Probable temperature of the Earth’s core is ~ 6000 K