All-Electron Full-Potential Calculations at O(ASA) Speed A Fata Morgana?

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All-Electron Full-Potential Calculations at O(ASA) Speed A Fata Morgana? Center for Electronic Correlations and Magnetism Institute for Physics, University of Augsburg February 4, 2008

Outline 1 2 3

Outline 1 2 3

Outline 1 2 3

Outline 1 2 3

Back in the 1930 s... John C. Slater Full Potential { spherical symmetric near nuclei v σ (r) : flat outside the atomic cores

Back in the 1930 s... John C. Slater Full Potential { spherical symmetric near nuclei v σ (r) : flat outside the atomic cores Muffin-Tin Approximation { vσ MT spherical symmetric in spheres (r) = constant in interstitial region

Back in the 1930 s... Full Potential (FeS 2 ) Muffin-Tin Potential v / a.u. -4.5-4 -5.5-5 -6.5-6 -7.5-7 -8 0 10 20 30 40 50 0 50 40 30 20 10

Back in the 1930 s... Muffin-Tin Approximation distinguish: atomic regions Muffin-Tin Potential remainder

Back in the 1930 s... Muffin-Tin Approximation distinguish: atomic regions muffin-tin spheres v eff,σ (r) = v eff,σ ( r ) remainder Muffin-Tin Potential

Back in the 1930 s... Muffin-Tin Approximation distinguish: atomic regions muffin-tin spheres v eff,σ (r) = v eff,σ ( r ) remainder interstitial region v eff,σ (r) = 0 Muffin-Tin Potential

Back in the 1930 s... Partial Waves muffin-tin spheres v eff,σ (r) = v eff,σ ( r ) Muffin-Tin Potential interstitial region v eff,σ (r) = 0

Back in the 1930 s... Partial Waves muffin-tin spheres v eff,σ (r) = v eff,σ ( r ) solve radial Schrödinger equation numerically interstitial region v eff,σ (r) = 0 Muffin-Tin Potential

Back in the 1930 s... Partial Waves muffin-tin spheres v eff,σ (r) = v eff,σ ( r ) solve radial Schrödinger equation numerically interstitial region v eff,σ (r) = 0 exact solutions plane waves spherical waves Muffin-Tin Potential

Back in the 1930 s... Partial Waves muffin-tin spheres v eff,σ (r) = v eff,σ ( r ) solve radial Schrödinger equation numerically interstitial region v eff,σ (r) = 0 exact solutions plane waves spherical waves match at sphere surface ( augment ) Muffin-Tin Potential

Back in the 1930 s... Partial Waves muffin-tin spheres v eff,σ (r) = v eff,σ ( r ) solve radial Schrödinger equation numerically interstitial region v eff,σ (r) = 0 exact solutions plane waves spherical waves match at sphere surface ( augment ) Basis Functions matched partial waves augmented plane waves (APWs) muffin-tin orbitals (MTOs), augmented spherical waves (ASWs)

Back in the 1930 s... Wave Function expand in basis functions expansion coefficients from variational principle Basis Functions matched partial waves augmented plane waves (APWs) muffin-tin orbitals (MTOs), augmented spherical waves (ASWs)

Back in the 1930 s... Wave Function expand in basis functions expansion coefficients from variational principle Core States all-electron methods fully included orthogonal to partial waves Basis Functions matched partial waves augmented plane waves (APWs) muffin-tin orbitals (MTOs), augmented spherical waves (ASWs) used to describe valence states

Back in the 1930 s... Augmented Spherical Waves envelope functions augmented spherical waves A B A B r

Back in the 1970 s... Ole K. Andersen Linear Methods in Band Theory energy dependence of basis functions almost linear linearize (ϕ, ϕ) huge increase in computat. efficiency!

Back in the 1970 s... Ole K. Andersen Linear Methods in Band Theory energy dependence of basis functions almost linear linearize (ϕ, ϕ) huge increase in computat. efficiency! Linear Augmented Plane Wave (LAPW) muffin-tin approximation easy to implement good! full-potential at a low price basis functions from muffin-tin potential wave functions from full potential example: Wien2k large basis set ( 100 pw s/atom) bad!

Back in the 1970 s... Ole K. Andersen Linear Muffin-Tin Orbital (LMTO) based on spherical waves does not require crystalline periodicity natural interpretation of results difficult to implement bad! full-potential extension extremely difficult muffin-tin approximation (?) finite interstitial region large basis set: two functions per s-, p-, d-state still inefficient bad!

Back in the 1970 s... Ole K. Andersen Linear Muffin-Tin Orbital (LMTO) based on spherical waves does not require crystalline periodicity natural interpretation of results difficult to implement bad! full-potential extension extremely difficult muffin-tin approximation (?) finite interstitial region large basis set: two functions per s-, p-, d-state still inefficient bad!

Back in the 1970 s... Ole K. Andersen Linear Muffin-Tin Orbital (LMTO) based on spherical waves does not require crystalline periodicity natural interpretation of results atomic-sphere approximation (ASA) make spheres space-filling! interstitial region formally removed only numerical functions in spheres minimal basis set (s, p, d) very high computational efficiency O(ASA) speed!!! makes potential more realistic systematic error in total energy bad!

Back in the 1970 s... Ole K. Andersen Linear Muffin-Tin Orbital (LMTO) based on spherical waves does not require crystalline periodicity natural interpretation of results atomic-sphere approximation (ASA) make spheres space-filling! interstitial region formally removed only numerical functions in spheres minimal basis set (s, p, d) very high computational efficiency O(ASA) speed!!! makes potential more realistic systematic error in total energy bad!

Back in the 1970 s... Ole K. Andersen Linear Muffin-Tin Orbital (LMTO) based on spherical waves does not require crystalline periodicity natural interpretation of results atomic-sphere approximation (ASA) make spheres space-filling! interstitial region formally removed only numerical functions in spheres minimal basis set (s, p, d) very high computational efficiency O(ASA) speed!!! makes potential more realistic systematic error in total energy bad!

Iron Pyrite: FeS 2 Pyrite Pa 3 (T 6 h ) a = 5.4160 Å NaCl structure sublattices occupied by iron atoms sulfur pairs sulfur pairs 111 axes x S = 0.38484 rotated FeS 6 octahedra

FeS 2 : Structure Optimization ASW Version 2.2-16532.850-16532.900-16532.950 E (Ryd) -16533.000-16533.050-16533.100-16533.150-16533.200-16533.250 0.374 0.378 0.382 0.386 0.390 0.394 x S

Towards a Full-Potential Spherical-Wave Method Conclusions ASA (space-filling atomic spheres) O(ASA) speed systematic error in total energy non-overlapping muffin-tin spheres prerequisite for accurate total energies larger basis set inefficient

Towards a Full-Potential Spherical-Wave Method Conclusions ASA (space-filling atomic spheres) O(ASA) speed systematic error in total energy non-overlapping muffin-tin spheres prerequisite for accurate total energies larger basis set inefficient Requirements restore interstitial region go to non-overlapping muffin-tin spheres go beyond constant-potential approximation inside muffin-tin spheres non-spherical contributions

Towards a Full-Potential Spherical-Wave Method Conclusions ASA (space-filling atomic spheres) O(ASA) speed systematic error in total energy non-overlapping muffin-tin spheres prerequisite for accurate total energies larger basis set inefficient Requirements restore interstitial region go to non-overlapping muffin-tin spheres go beyond constant-potential approximation inside muffin-tin spheres non-spherical contributions

Towards a Full-Potential Spherical-Wave Method Guidelines interstitial quantities expanded in plane waves straightforward to implement inefficient interstitial quantities expanded in spherical waves elegant, no periodicity required efficient difficult to implement

Towards a Full-Potential Spherical-Wave Method Guidelines interstitial quantities expanded in plane waves straightforward to implement inefficient interstitial quantities expanded in spherical waves elegant, no periodicity required efficient difficult to implement

ASW Method Characteristics similar to LMTO different linearization scheme different interstitial energy different implementations

ASW Method Characteristics similar to LMTO different linearization scheme different interstitial energy different implementations 0th Generation (Williams, Kübler, Gelatt, 1970s) PRB 19, 6094 (1979)

ASW Method Characteristics similar to LMTO different linearization scheme different interstitial energy different implementations 1st Generation (VE, 1990s) IJQC 77, 1007 (2000) completely new, monolithic implementation new algorithms improved accuracy, numerical stability much improved functionality, usability, and portability xanderson convergence acceleration scheme all LDA-parametrizations, most GGA-schemes still based on atomic-sphere approximation

ASW Method: Basic Formalism Wave Function Expanded in Basis Functions ψ σ (r) = Lκi c Lκiσ H Lκσ (r i) c Lκiσ determined variationally

ASW Method: Basic Formalism Wave Function Expanded in Basis Functions ψ σ (r) = Lκi c Lκiσ H Lκσ (r i) c Lκiσ determined variationally Augmented Spherical Wave H HLκσ Lκ I (r i) (r i) = H Lκσ (r i ) J L j L κσ(r j )B L Lκ interstitial region on-centre sphere i off-centre spheres j B L Lκ(R j R i ): structure constants ASW classified by atomic site R i, L = (l, m), decay κ, spin σ

ASW Method: Basic Formalism Augmented Spherical Waves envelope functions augmented spherical waves A B A B r

ASW Method: Basic Formalism Envelope Functions H I Lκ (r i) := iκ l+1 h (1) l (κr i )Y L (ˆr i ) h (1) l (κr i ): spherical Hankel function

ASW Method: Basic Formalism Envelope Functions H I Lκ (r i) := iκ l+1 h (1) l (κr i )Y L (ˆr i ) h (1) l (κr i ): spherical Hankel function Augmented Functions H Lκσ (r i ) := h lκσ (r i )Y L (ˆr i ) J L κσ(r j ) := j l κσ(r j )Y L (ˆr j ) h, j: numerical solutions of radial Kohn-Sham equation boundary conditions from envelope functions correspond to ϕ and ϕ of LMTO

ASW Method: Further Reading

Outline 1 2 3

Basic Principles Steps to be Taken remove total energy error due to overlap of atomic spheres reintroduce non-overlapping muffin-tin spheres restore interstitial region

Basic Principles Steps to be Taken remove total energy error due to overlap of atomic spheres reintroduce non-overlapping muffin-tin spheres restore interstitial region find representation of electron density and full potential inside muffin-tin spheres in the interstitial region

Basic Principles Steps to be Taken remove total energy error due to overlap of atomic spheres reintroduce non-overlapping muffin-tin spheres restore interstitial region find representation of electron density and full potential find representation of products of the wave function inside muffin-tin spheres in the interstitial region

Basic Principles Steps to be Taken remove total energy error due to overlap of atomic spheres reintroduce non-overlapping muffin-tin spheres restore interstitial region find representation of electron density and full potential find representation of products of the wave function find representation of products of the basis functions inside muffin-tin spheres in the interstitial region

Basic Principles Steps to be Taken remove total energy error due to overlap of atomic spheres reintroduce non-overlapping muffin-tin spheres restore interstitial region find representation of electron density and full potential find representation of products of the wave function find representation of products of the basis functions inside muffin-tin spheres use spherical-harmonics expansions in the interstitial region

Basic Principles Steps to be Taken remove total energy error due to overlap of atomic spheres reintroduce non-overlapping muffin-tin spheres restore interstitial region find representation of electron density and full potential find representation of products of the wave function find representation of products of the basis functions inside muffin-tin spheres use spherical-harmonics expansions in the interstitial region no exact spherical-wave representation available!

From Wave Functions to Electron Density Density inside MT-Spheres (Al) ρ v / a.u. 0.06 0.05 0.04 0.03 0.02 0.01 0 0 10 20 30 40 50 0 50 40 30 20 10

From Wave Functions to Electron Density Products of Basis Functions in Interstitial Region p I (r) = n d n F n (r) d 3 r F n (r)pi (r) = n d n d 3 r F n (r)f n(r)

From Wave Functions to Electron Density Products of Basis Functions in Interstitial Region p I (r) = n d n F n (r) d 3 r F n (r)pi (r) = n d n d 3 r F n (r)f n(r) F n (r): plane waves integrals exact inefficient Weyrich 1988, Blöchl 1989, VE 1991, Savrasov 1992, Methfessel 2000

From Wave Functions to Electron Density Products of Basis Functions in Interstitial Region p I (r) = n d n F n (r) d 3 r F n (r)pi (r) = n d n d 3 r F n (r)f n(r) F n (r): spherical waves would be efficient integrals not known analytically Springborg/Andersen 1987, Methfessel 1988, VE 2002, VE 2006

From Wave Functions to Electron Density Interstitial Products of Basis Functions expand in atom-centered spherical waves (Hankel functions): p I (r) := ( H Lκ 1 σ (r i) ) H L κ 2 σ (r j)! = n H L κ 2 σ (r j): orbital basis set (obs) H Kη (r n ): product basis set (pbs) Kη d Lκ 1iL κ 2 j Kηnσ H Kη (r n ) coefficients from projection P: [ ] P p I (r) = P [( HLκ 1 σ (r i) ) H L κ 2 σ (r j) ] = d Lκ 1iL κ 2 j Kηnσ P [ H Kη (r n ) ] n Kη

From Wave Functions to Electron Density Interstitial Products of Basis Functions expand in atom-centered spherical waves (Hankel functions): p I (r) := ( H Lκ 1 σ (r i) ) H L κ 2 σ (r j)! = n H L κ 2 σ (r j): orbital basis set (obs) H Kη (r n ): product basis set (pbs) Kη d Lκ 1iL κ 2 j Kηnσ H Kη (r n ) coefficients from projection P: [ ] P p I (r) = P [( HLκ 1 σ (r i) ) H L κ 2 σ (r j) ] = d Lκ 1iL κ 2 j Kηnσ P [ H Kη (r n ) ] n Kη

From Wave Functions to Electron Density Interstitial Products of Basis Functions projection P: P [( H Lκ 1 σ (r i) ) H L κ 2 σ (r j) ] = n Kη d Lκ 1iL κ 2 j Kηnσ P [ H Kη (r n ) ]

From Wave Functions to Electron Density Interstitial Products of Basis Functions projection P: P [( H Lκ 1 σ (r i) ) H L κ 2 σ (r j) ] = n Kη d Lκ 1iL κ 2 j Kηnσ P [ H Kη (r n ) ] Springborg/Andersen 1987 integrate over interstitial region, use one-center expansions P K η n... ˆ= Ω I d 3 r H K η (r n )...

From Wave Functions to Electron Density Interstitial Products of Basis Functions projection P: P [( H Lκ 1 σ (r i) ) H L κ 2 σ (r j) ] = n Kη d Lκ 1iL κ 2 j Kηnσ P [ H Kη (r n ) ] Methfessel 1988 match values and slopes at MT-sphere surfaces P K η n... ˆ= ( ) d 2ˆr η 1 Y K (ˆr)... r rn =s n

From Wave Functions to Electron Density Interstitial Products of Basis Functions projection P: P [( H Lκ 1 σ (r i) ) H L κ 2 σ (r j) ] = n Kη d Lκ 1iL κ 2 j Kηnσ P [ H Kη (r n ) ] VE 2002 integrate over interstitial region, use one-center expansions (interstitial shells between AS- and MT-spheres) P K η n... ˆ= d 3 r m HK η (r n )... m Ω m

From Wave Functions to Electron Density Interstitial Products of Basis Functions projection P: P [( H Lκ 1 σ (r i) ) H L κ 2 σ (r j) ] = n experience Kη product basis set almost overcomplete d Lκ 1iL κ 2 j Kηnσ P [ H Kη (r n ) ] value/slope (Methfessel) matching most stable

From Wave Functions to Electron Density Density from Value/Slope Matching at MT-Radii (Al) ρ v / a.u. ρ v / a.u. 0.06 0.05 0.04 0.03 0.02 0.01 0 0 10 20 30 40 50 0 50 40 30 20 10 0.06 0.05 0.04 0.03 0.02 0.01 0 0 10 20 30 40 50 0 50 40 30 20 10

From Electron Density to Full Potential Inside Muffin-Tin Spheres density, Hartree-potential and xc-potential numerically Interstitial Region density from value/slope matching Hartree-potential analytically xc-potential from value/slope matching

From Electron Density to Full Potential Inside Muffin-Tin Spheres density, Hartree-potential and xc-potential numerically Interstitial Region density from value/slope matching Hartree-potential analytically xc-potential from value/slope matching

From Full Potential to Basis Functions Previous Approaches project full potential to muffin-tin potential construct basis functions from muffin-tin potential no minimal basis set! (large basis set!) Present Approach project full potential to ASA potential construct basis functions from ASA potential minimal basis set! future use spheres larger than space-filling remove linearization error

From Full Potential to Basis Functions Previous Approaches project full potential to muffin-tin potential construct basis functions from muffin-tin potential no minimal basis set! (large basis set!) Present Approach project full potential to ASA potential construct basis functions from ASA potential minimal basis set! future use spheres larger than space-filling remove linearization error

Comparison of Approaches Ole K. Andersen ASA geometry used for basis functions minimal basis set ASA geometry used for density and potential error in total energy good! bad!

Comparison of Approaches Ole K. Andersen ASA geometry used for basis functions minimal basis set ASA geometry used for density and potential error in total energy Michael S. Methfessel MT geometry used for density and potential accurate total energy MT geometry used for basis functions large basis set good! bad! good! bad!

Comparison of Approaches Ole K. Andersen ASA geometry used for basis functions ASA geometry used for density and potential Michael S. Methfessel MT geometry used for density and potential MT geometry used for basis functions present approach ASA geometry used for basis functions minimal basis set O(ASA) speed MT geometry used for density and potential accurate total energy good! bad! good! bad! great! great!

Implementation 2nd Generation ASW (VE, 2000s) based on 1st generation code full-potential ASW method at O(ASA) speed! electron densities, spin densities electric field gradients elastic properties, phonon spectra optical properties based on linear-response theory direct calculation of Rσ and Iσ no Kramers-Kronig relations needed LDA+U method all flavours for double-counting terms (AMF, FLL, DFT)

Implementation 2nd Generation ASW (VE, 2000s) based on 1st generation code full-potential ASW method at O(ASA) speed! electron densities, spin densities electric field gradients elastic properties, phonon spectra optical properties based on linear-response theory direct calculation of Rσ and Iσ no Kramers-Kronig relations needed LDA+U method all flavours for double-counting terms (AMF, FLL, DFT)

Implementation 2nd Generation ASW (VE, 2000s) based on 1st generation code full-potential ASW method at O(ASA) speed! electron densities, spin densities electric field gradients elastic properties, phonon spectra optical properties based on linear-response theory direct calculation of Rσ and Iσ no Kramers-Kronig relations needed LDA+U method all flavours for double-counting terms (AMF, FLL, DFT)

Outline 1 2 3

Electronic Structure of BaTiO 3 Wien2k VASP 5 Energy (ev) 0 4.62 ev 5 R X G M R G

Electronic Structure of BaTiO 3 Wien2k ASW Version 2.2 6 4 (E - E V ) (ev) 2 0-2 -4-6 R X Γ M R Γ

Electronic Structure of BaTiO 3 Wien2k FPASW Version 2.3 6 4 (E - E V ) (ev) 2 0-2 -4-6 R X Γ M R Γ New! much better agreement with other full-potential codes (valence-band width, valence states at M-point)

Fermi Surface of MoO 2 ASW Version 1.9 FPASW Version 2.3 2 2 1 1 (E - E F ) (ev) 0 (E - E F ) (ev) 0-1 -1-2 -2 Γ Y C Z Γ A E Z Γ B D Z Γ Y C Z Γ A E Z Γ B D Z New! no hole pocket near Z-point much better agreement with ARPES, de Haas-van Alphen

Iron Pyrite: FeS 2 Pyrite Pa 3 (T 6 h ) a = 5.4160 Å NaCl structure sublattices occupied by iron atoms sulfur pairs sulfur pairs 111 axes x S = 0.38484 rotated FeS 6 octahedra

FeS 2 : Partial Densities of States DOS (1/eV) 40 35 30 25 20 15 10 Fe 3d S 3s S 3p Relevant states Fe 3d S 3s S 3p 5 0-15 -10-5 0 5 (E - E V ) (ev)

FeS 2 : Partial Densities of States 8 DOS (1/eV) 7 6 5 4 3 2 Fe 3d t 2g Fe 3d e g Crystal field splitting Fe 3d in octahedron: t 2g and e g states without rotation 1 with rotation 0-8 -6-4 -2 0 2 4 6 (E - E V ) (ev)

FeS 2 : Partial Densities of States 8 DOS (1/eV) 7 6 5 4 3 2 Fe 3d t 2g Fe 3d e g Crystal field splitting Fe 3d in octahedron: t 2g and e g states without rotation 1 with rotation 0-8 -6-4 -2 0 2 4 6 (E - E V ) (ev)

FeS 2 : Partial Densities of States 2 DOS (1/eV) 1.5 1 0.5 0 S 3p x, 3p y S 3p z -8-6 -4-2 0 2 4 6 (E - E V ) (ev) Crystal field splitting S 3p: p x /p y vs. p z states without rotation with rotation: z axis 111

FeS 2 : Partial Densities of States 2 DOS (1/eV) 1.5 1 0.5 0 S 3p x, 3p y S 3p z -8-6 -4-2 0 2 4 6 (E - E V ) (ev) Crystal field splitting S 3p: p x /p y vs. p z states without rotation with rotation: z axis 111

FeS 2 : Density and Laplacian Valence Electron Density ρ v / a.u. 0.25 0.2 0.15 0.1 0.05 0 0 10 20 30 40 50 0 50 40 30 20 10

FeS 2 : Density and Laplacian Valence Electron Density Laplacian of Electron Density ρ v / a.u. - 2 ρ / a.u. 0.25 0.2 0.15 0.1 0.05 0 0 10 20 30 40 50 0 50 40 30 20 10 0.3 0.2 0.1-0.1 0-0.2-0.3 0 10 20 30 40 50 0 50 40 30 20 10 New! topological analysis (Bader analysis)

FeS 2 : Equilibrium Volume and Bulk Modulus -16532.600-16532.650-16532.700 V 0 = 1056.15 a B 3 E 0 = -16532.904060 Ryd B 0 = 170.94 GPa E (Ryd) -16532.750-16532.800-16532.850-16532.900-16532.950 850 900 950 1000 1050 1100 1150 1200 3 V (a B )

FeS 2 : Equilibrium Volume and Bulk Modulus Lattice Constant 10.28 NCPP Zeng and Holzwarth 94 10.02 FPLO Opahle et al. 99 10.17 CRYSTAL98 Muscat et al. 02 9.92 CASTEP Muscat et al. 02 10.18 FPASW present work 10.23 exp. Finklea et al. 76 10.22 exp. Will et al. 84 10.23 exp. Stevens et al. 91

FeS 2 : Equilibrium Volume and Bulk Modulus Bulk Modulus 187 LMTO Nguyen-Manh et al. 98 185 FPLO Opahle et al. 99 209 CRYSTAL98 Muscat et al. 02 208 CASTEP Muscat et al. 02 171 FPASW present work 148 exp. Drickamer et al. 66 118 exp. Will et al. 84 215 exp. Chattopadhyay and von Schnering 85 157 exp. Fujii et al. 86 143 exp. Jephcoat and Olson 87 162 exp. Ahrens and Jeanloz 87 145 exp. Blachnik et al. 98

FeS 2 : From Atoms to the Solid -16532.600-16532.650-16532.700 V 0 = 1056.15 a B 3 E 0 = -16532.904060 Ryd B 0 = 170.94 GPa E (Ryd) -16532.750-16532.800-16532.850-16532.900-16532.950 850 900 950 1000 1050 1100 1150 1200 3 V (a B )

FeS 2 : From Atoms to the Solid -16527-16528 -16529 E (Ryd) -16530-16531 -16532-16533 0 2000 4000 6000 8000 10000 12000 V (a B 3 )

FeS 2 : Structure Optimization ASW Version 2.2 E (Ryd) -16532.850-16532.900-16532.950-16533.000-16533.050-16533.100-16533.150-16533.200-16533.250 0.374 0.378 0.382 0.386 0.390 0.394 x S

FeS 2 : Structure Optimization ASW Version 2.2 FPASW Version 2.3 E (Ryd) -16532.850-16532.900-16532.950-16533.000-16533.050-16533.100-16533.150-16533.200-16533.250 0.374 0.378 0.382 0.386 0.390 0.394 x S E (Ryd) -16532.850-16532.860-16532.870-16532.880-16532.890-16532.900-16532.910 0.374 0.378 0.382 0.386 0.390 0.394 x S

FeS 2 : Structure Optimization Sulfur Position 0.378 NCPP Zeng and Holzwarth 94 0.377 FPLO Opahle et al. 99 0.378 CRYSTAL98 Muscat et al. 02 0.382 CASTEP Muscat et al. 02 0.382 FPASW present work 0.386 exp. Finklea et al. 76 0.386 exp. Will et al. 84 0.385 exp. Stevens et al. 91

Phase Stability in Silicon ASW Version 2.2-578.000-578.020-578.040 E (Ryd) -578.060-578.080-578.100 dia hex β-tin sc bcc fcc 80 90 100 110 120 130 140 150 160 170 3 V (a B ) Bad β-tin structure most stable # nature (diamond structure)

Phase Stability in Silicon ASW Version 2.2 FPASW Version 2.4 E (Ryd) -578.000-578.020-578.040-578.060 E (Ryd) -578.010-578.015-578.020-578.025-578.030-578.035-578.040 dia hex β-tin sc bcc fcc -578.080-578.100 dia hex β-tin sc bcc fcc 80 90 100 110 120 130 140 150 160 170 3 V (a B ) -578.045-578.050-578.055-578.060 80 90 100 110 120 130 140 150 160 170 3 V (a B ) New! diamond structure most stable pressure induced phase transition to β-tin structure

LTO(Γ)-Phonon in Silicon ASW Version 2.2-1156.0691 Si fcc -1156.0692-1156.0693 E (Ryd) -1156.0694-1156.0695-1156.0696-1156.0697-1156.0698 0.118 0.12 0.122 0.124 0.126 0.128 0.13 0.132 x Si Bad no stable Si position # nature

LTO(Γ)-Phonon in Silicon ASW Version 2.2 FPASW Version 2.4-1156.0691 Si fcc -1156.1000 Si fcc -1156.0692-1156.1010-1156.0693-1156.1020 E (Ryd) -1156.0694-1156.0695 E (Ryd) -1156.1030-1156.1040-1156.0696-1156.1050-1156.0697-1156.1060-1156.0698 0.118 0.12 0.122 0.124 0.126 0.128 0.13 0.132-1156.1070 0.118 0.12 0.122 0.124 0.126 0.128 0.13 0.132 x Si x Si New! phonon frequency: f calc = 15.26 THz (f exp = 15.53 THz)

Structure Optimization in PdCoO 2 Delafossite Structure

Structure Optimization in PdCoO 2 Delafossite Structure Total energy surface -13.179778-13.179778-13.179778-13.179779-13.179779-13.179779-13.179779-13.179779 5.36 5.38 5.45.42 5.445.465.48 5.5 33.25 33.3 33.35 33.4 33.45 33.5 33.55 33.6 33.65 33.7 33.75 33.8

Structure Optimization in PdCoO 2 Structural Data experiment theory a = 2.83 Å c = 17.743 Å z O = 0.1112 a = 2.8767 Å c = 17.7019 Å z O = 0.1100 Total energy surface -13.179778-13.179778-13.179778-13.179779-13.179779-13.179779-13.179779-13.179779 5.36 5.38 5.45.42 5.445.465.48 5.5 33.25 33.3 33.35 33.4 33.45 33.5 33.55 33.6 33.65 33.7 33.75 33.8 VE, R. Frésard, A. Maignan, Chem. Mat. (2008), in press

Dielectric Functions of Corundum Imaginary Part FLAPW, Hosseini et al., 2005 FPLMTO, Ahuja et al., 2004 FPASW 0.6 0.5 Im ε xx Im ε zz 0.4 ε 0.3 0.2 0.1 0 0 5 10 15 20 25 30 E (ev)

Dielectric Functions of Corundum Real Part FLAPW, Hosseini et al., 2005 FPLMTO, Ahuja et al., 2004 FPASW 0.6 0.5 Re ε xx Re ε zz 0.4 0.3 ε 0.2 0.1 0-0.1 0 5 10 15 20 25 30 E (ev)

LDA+U-Calculations for Gadolinium DOS of ferromagnetic Gd 20 15 10 Energetics DOS (1/eV) 5 0-5 -10-15 Gd total Gd 4f (LDA+U) Gd 4f (LDA) E AF E FE LDA -1.601 LDA+U 8.425 (in mryd/atom) -20-10 -8-6 -4-2 0 2 4 6 (E - E F ) (ev)

Summary (Versions 2.3/2.4) ASA Geometry used for Basis Functions MT Geometry used for Density and Potential Accurate Total Energies O(ASA) Speed! Optical Properties implemented LDA+U-Method implemented What s Next? Forces? Automated Structure Optimization? Exact Exchange (EXX)? at O(ASA) speed?

Summary (Versions 2.3/2.4) ASA Geometry used for Basis Functions MT Geometry used for Density and Potential Accurate Total Energies O(ASA) Speed! Optical Properties implemented LDA+U-Method implemented What s Next? Forces? Automated Structure Optimization? Exact Exchange (EXX)? at O(ASA) speed?

Acknowledgments Darmstadt SFB 252 Stuttgart O. K. Andersen Augsburg T. Kopp, J. Mannhart, K.-H. Höck, W. Scherer Darmstadt J. Sticht Darmstadt P. C. Schmidt, M. Stephan

Acknowledgments Darmstadt SFB 252 Stuttgart O. K. Andersen Augsburg T. Kopp, J. Mannhart, K.-H. Höck, W. Scherer Darmstadt J. Sticht Darmstadt P. C. Schmidt, M. Stephan Cocoyoc Thank You for Your Attention!