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Relativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20 th WIEN2k Workshop PennStateUniversity – 2013 Xavier Rocquefelte Institut des Matériaux JeanRouxel (UMR 6502) Université de Nantes, FRANCE
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Page 1: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativistic effects&

Non-collinear magnetism

(WIEN2k / WIENncm)

20th WIEN2k WorkshopPennStateUniversity – 2013

Xavier RocquefelteInstitut des Matériaux Jean‐Rouxel (UMR 6502)

Université de Nantes, FRANCE

Page 2: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Talk constructed using the following documents:Slides of:

Robert Laskowski, Stefaan Cottenier, Peter Blaha and Georg Madsen

Books:- WIEN2k userguide, ISBN 3-9501031-1-2- Electronic Structure: Basic Theory and Practical Methods, Richard M. Martin ISBN 0 521 78285 6- Relativistic Electronic Structure Theory. Part 1. Fundamentals, Peter Schewerdtfeger, ISBN 0 444 51249 7

Notes of:- Pavel Novak (Calculation of spin-orbit coupling)

http://www.wien2k.at/reg_user/textbooks/- Robert Laskowski (Non-collinear magnetic version of WIEN2k package)

web:- http://www2.slac.stanford.edu/vvc/theory/relativity.html- wienlist digest - http://www.wien2k.at/reg_user/index.html- wikipedia …

20th WIEN2k WorkshopPennStateUniversity – 2013

Page 3: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Few words about Special Theory of Relativity

Light

Composed of photons (no mass)Speed of light = constant

c 137 au

Atomic units:ħ = me = e = 1

Page 4: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Few words about Special Theory of Relativity

Light Matter

Composed of photons (no mass)Speed of light = constant

c 137 au

Atomic units:ħ = me = e = 1

Speed ofmatter mass

v = f(mass)

mass = f(v)

Composed of atoms (mass)

Page 5: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Few words about Special Theory of Relativity

Light Matter

Composed of photons (no mass)

Lorentz Factor (measure of the relativistic effects)

Speed of light = constant

c 137 au

Atomic units:ħ = me = e = 1

Speed ofmatter mass

v = f(mass)

mass = f(v)

Momentum: p = mv = Mv

Total energy:

Relativistic mass: M = m (m: rest mass)1

1

12

cv

Composed of atoms (mass)

E2 = p2c2 + m2c4

E = mc2 = Mc2

Page 6: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

22.1

58.01

1

1

122

cve

Details for Au atom:

ccsve 58.013779)1(

Speed of the 1s electron (Bohr model):

+Zee-

Lorentz factor ()

123456789

10

0 20 40 60 80 100 120

c 137 au

H(1s)

Speed (v)

Au(1s)

« Non-relativistic » particle: = 1

1s electron of Au atom = relativistic particle

Definition of a relativistic particle (Bohr model)

au1)1(:H sve

au79)1(:Au sve

00003.1

22.1nZve

au1)1(:H sve

au79)1(:Au sve

00003.1

22.1nZve

Me(1s-Au) = 1.22me

Page 7: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativistic effects

Relativistic increase in the mass of an electron with its velocity (when ve c)

1) The mass-velocity correction

+Ze

Page 8: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativistic increase in the mass of an electron with its velocity (when ve c)

1) The mass-velocity correction

It has no classical relativistic analogueDue to small and irregular motions of an electron about its mean position (Zitterbewegung*)

2) The Darwin term

+Ze

Relativistic effects

*Analysis of Erwin Schrödinger of the wave packet solutions of the Dirac equation for relativisticelectrons in free space:The interference between positive and negative energy states produces whatappears to be a fluctuation (at the speed of light) of the position of an electron around the median.

Page 9: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativistic increase in the mass of an electron with its velocity (when ve c)

1) The mass-velocity correction

It has no classical relativistic analogueDue to small and irregular motions of an electron about its mean position (Zitterbewegung)

2) The Darwin term

It is the interaction of the spin magnetic moment (s) of an electron with the magnetic field induced by its own orbital motion (l)

3) The spin-orbit coupling

+Ze

Relativistic effects

Page 10: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativistic increase in the mass of an electron with its velocity (when ve c)

1) The mass-velocity correction

It has no classical relativistic analogueDue to small and irregular motions of an electron about its mean position (Zitterbewegung)

2) The Darwin term

It is the interaction of the spin magnetic moment (s) of an electron with the magnetic field induced by its own orbital motion (l)

3) The spin-orbit coupling

The change of the electrostatic potential induced by relativity is an indirect effect of the core electrons on the valence electrons

4) Indirect relativistic effect

+Zeffe

Relativistic effects

Page 11: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

One electron radial Schrödinger equation

VHS

2

21

V

mH

eS

22

2

HARTREE ATOMIC UNITS INTERNATIONAL UNITS

Atomic units:ħ = me = e = 11/(40) = 1

c = 1/ 137 au

Page 12: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

One electron radial Schrödinger equation

VHS

2

21

V

mH

eS

22

2

rZV

rZeV

0

2

4

INTERNATIONAL UNITS

In a spherically symmetric potential

Atomic units:ħ = me = e = 11/(40) = 1

c = 1/ 137 au

,,,,, mllnmln YrR

2

2

2222

22

sin1sin

sin11

rrrr

rr

HARTREE ATOMIC UNITS

Page 13: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

One electron radial Schrödinger equation

VHS

2

21

lnln

e

ln

e

RRrll

mV

drdR

rdrd

rm ,,2

2,2

2

2

12

12

In a spherically symmetric potential

V

mH

eS

22

2

rZV

rZeV

0

2

4

lnln

ln RRr

llVdr

dRr

drd

r ,,2,2

2 2

121

INTERNATIONAL UNITS

,,,,, mllnmln YrR

2

2

2222

22

sin1sin

sin11

rrrr

rr

HARTREE ATOMIC UNITS

Page 14: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Dirac Hamiltonian: a brief description

Dirac relativistic Hamiltonian provides a quantum mechanical description of electrons, consistent with the theory of special relativity.

DH with

E2 = p2c2 + m2c4

VcmpcH eD 2

Page 15: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Dirac Hamiltonian: a brief description

Dirac relativistic Hamiltonian provides a quantum mechanical description of electrons, consistent with the theory of special relativity.

00

k

kk

10

01k

0110

1

00

2 ii

10

013

(22) Pauli spin matrices

Momentum operator Rest mass

Electrostatic potential

VcmpcH eD 2

(22) unit and zero matrices

DH with

E2 = p2c2 + m2c4

Page 16: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Dirac equation: HD and are 4-dimensional

and are time-independent two-component spinors describing the spatial and spin-1/2 degrees of freedom

is a four-component single-particle wave function that describes spin-1/2 particles.

4

3

2

1

4

3

2

1

DH

spin up

spin down

Largecomponents ()

Smallcomponents ()

In case of electrons:

Leads to a set of coupled equations for and :

2cmVpc e

2cmVpc e

factor 1/(mec2)

Page 17: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Dirac equation: HD and are 4-dimensional

For a free particle (i.e. V = 0):

0

0ˆˆˆ0ˆˆˆˆˆˆ0

ˆˆˆ0

4

3

2

1

2

2

2

2

cmppipcmpipp

ppipcmpippcm

ezyz

eyzz

zyze

yxze

000,2

cme

00

0

,2 cme

Particles: up & down

0

00

,2

cme

000

,2cme

Antiparticles: up & down

Solution in the slow particle limit (p=0)

Non-relativistic limit decouples 1 from 2

and 3 from 4

Page 18: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Dirac equation: HD and are 4-dimensional

For a free particle (i.e. V = 0):

0

0ˆˆˆ0ˆˆˆˆˆˆ0

ˆˆˆ0

4

3

2

1

2

2

2

2

cmppipcmpipp

ppipcmpippcm

ezyz

eyzz

zyze

yxze

000,2

cme

00

0

,2 cme

Particles: up & down

0

00

,2

cme

000

,2cme

Antiparticles: up & down

Solution in the slow particle limit (p=0)

Non-relativistic limit decouples 1 from 2

and 3 from 4

For a spherical potential V(r):

n

n

rfirg gn and fn are Radial functions

Y are angular-spin functions

2slj

21 js

1,1 s

Page 19: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Dirac equation in a spherical potential

The resulting equations for the radial functions (gn and fn) are simplified if we define:

2' cme 22

'c

rVmrM ee

Energy: Radially varying mass:

For a spherical potential V(r):

Page 20: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Dirac equation in a spherical potential

The resulting equations for the radial functions (gn and fn) are simplified if we define:

2' cme 22

'c

rVmrM ee

Energy: Radially varying mass:

Then the coupled equations can be written in the form of the radial eq.:

Darwin term

Spin-orbit coupling

11 llNote that:

For a spherical potential V(r):

Mass-velocity effect

nn

e

n

en

e

n

e

ggrdr

dVcMdr

dgdrdV

cMg

rll

MV

drdgr

drd

rM'1

441

21

2 22

2

22

2

2

22

2

2

lnln

e

ln

e

RRrll

mV

drdR

rdrd

rm ,,2

2,2

2

2

12

12

One electron radial Schrödinger equation in a spherical potential

Page 21: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Dirac equation in a spherical potential

The resulting equations for the radial functions (gn and fn) are simplified if we define:

2' cme 22

'c

rVmrM ee

Energy: Radially varying mass:

nn

e

n

en

e

n

e

ggrdr

dVcMdr

dgdrdV

cMg

rll

MV

drdgr

drd

rM'1

441

21

2 22

2

22

2

2

22

2

2

nnnk f

rgV

cdrdf 1'1

Then the coupled equations can be written in the form of the radial eq.:

and Darwin term

Spin-orbit coupling

11 llNote that:

For a spherical potential V(r):

Due to spin-orbit coupling, is not an eigenfunction of spin (s) and angular orbital moment (l). Instead the good quantum numbers are j and

No approximation have been made

so far

Page 22: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Dirac equation in a spherical potential

Scalar relativistic approximation

Approximation that the spin-orbit term is small neglect SOC in radial functions (and treat it by perturbation theory)

nln gg ~ nln ff ~

nl

nl

enl

e

nl

e

gdrgd

drdV

cMg

rll

MV

drgdr

drd

rM~'

~

4~1

2

~12 22

2

2

22

2

2

drgd

cMf nl

enl

~

2~

and with the normalization condition: 1 ~~ 222 drrfg nlnl

No SOC Approximate radial functions:

Page 23: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Dirac equation in a spherical potential

Scalar relativistic approximation

Approximation that the spin-orbit term is small neglect SOC in radial functions (and treat it by perturbation theory)

nln gg ~ nln ff ~

nl

nl

enl

e

nl

e

gdrgd

drdV

cMg

rll

MV

drgdr

drd

rM~'

~

4~1

2

~12 22

2

2

22

2

2

drgd

cMf nl

enl

~

2~

and with the normalization condition: 1 ~~ 222 drrfg nlnl

No SOC Approximate radial functions:

The four-component wave function is now written as:

Inclusion of the spin-orbit coupling in “second variation” (on the large component only)

lmnl

lmnl

rfirg

~~~SOHH

with

0001

4 22

2 ldrdV

rcMH

eSO

is a pure spin state

is a mixture of up and down spin states

Page 24: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativistic effects in a solid

For a molecule or a solid:

Relativistic effects originate deep inside the core.

It is then sufficient to solve the relativistic equations in a spherical atomic geometry (inside the atomic spheres of WIEN2k).

Justify an implementation of the relativistic effects only inside the muffin-tin atomic spheres

Page 25: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

SOC: Spin orbit coupling

Implementation in WIEN2k

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

Coreelectrons

Coreelectrons

Valence electronsValence electrons

« Fully » relativistic

Spin-compensated Dirac equation

Scalar relativistic (no SOC)

Possibility to add SOC(2nd variational)

Page 26: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Interstitial RegionInterstitial Region

Valence electronsValence electrons

Not relativistic

SOC: Spin orbit coupling

Implementation in WIEN2k

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

Coreelectrons

Coreelectrons

Valence electronsValence electrons

« Fully » relativistic

Spin-compensated Dirac equation

Scalar relativistic (no SOC)

Possibility to add SOC(2nd variational)

Page 27: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Implementation in WIEN2k: core electrons

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

CoreelectronsCore

electrons

« Fully »relativistic

Spin-compensatedDirac equation

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

CoreelectronsCore

electrons

« Fully »relativistic

Spin-compensatedDirac equation

17 0.00 0 1,-1,2 ( n,,occup)2,-1,2 ( n,,occup)2, 1,2 ( n,,occup)2,-2,4 ( n,,occup)3,-1,2 ( n,,occup)3, 1,2 ( n,,occup)3,-2,4 ( n,,occup)3, 2,4 ( n,,occup)3,-3,6 ( n,,occup)4,-1,2 ( n,,occup)4, 1,2 ( n,,occup)4,-2,4 ( n,,occup)4, 2,4 ( n,,occup)4,-3,6 ( n,,occup)5,-1,2 ( n,,occup)4, 3,6 ( n,,occup)4,-4,8 ( n,,occup)0

case.inc for Au atom

s 0 1/2 -1 2

p 1 3/21/2 1 -2 2 4

d 2 5/23/2 2 -3 4 6

f 3 7/25/2 3 -4 6 8

l s=+1

j=l+s/2 =-s(j+1/2) occupation

s=-1 s=+1s=-1 s=+1s=-1

For spin-polarized potential,spin up and spin down are calculated separately, the density is averaged according to the occupation number

specified in case.inc file.

Core states: fully occupied spin-compensated Dirac

equation (include SOC)

Page 28: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

1s1/2 2s1/2

2p1/2 2p3/2 3s1/2

3p1/2

3p3/2

3d3/2 3d5/2 4s1/2

4p1/2

4p3/2

4d3/2

4d5/2

5s1/2

4f5/2 4f7/2

Implementation in WIEN2k: core electrons

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

CoreelectronsCore

electrons

« Fully »relativistic

Spin-compensatedDirac equation

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

CoreelectronsCore

electrons

« Fully »relativistic

Spin-compensatedDirac equation

17 0.00 0 1,-1,2 ( n,,occup)2,-1,2 ( n,,occup)2, 1,2 ( n,,occup)2,-2,4 ( n,,occup)3,-1,2 ( n,,occup)3, 1,2 ( n,,occup)3,-2,4 ( n,,occup)3, 2,4 ( n,,occup)3,-3,6 ( n,,occup)4,-1,2 ( n,,occup)4, 1,2 ( n,,occup)4,-2,4 ( n,,occup)4, 2,4 ( n,,occup)4,-3,6 ( n,,occup)5,-1,2 ( n,,occup)4, 3,6 ( n,,occup)4,-4,8 ( n,,occup)0

case.inc for Au atom

s 0 1/2 -1 2

p 1 3/21/2 1 -2 2 4

d 2 5/23/2 2 -3 4 6

f 3 7/25/2 3 -4 6 8

l s=+1

j=l+s/2 =-s(j+1/2) occupation

s=-1 s=+1s=-1 s=+1s=-1

For spin-polarized potential,spin up and spin down are calculated separately, the density is averaged according to the occupation number

specified in case.inc file.

Core states: fully occupied spin-compensated Dirac

equation (include SOC)

Page 29: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Implementation in WIEN2k: valence electrons

Valence electrons INSIDE atomic spheres are treated within scalar relativistic approximation [1] if RELA

is specified in case.struct file (by default).

[1] Koelling and Harmon, J. Phys. C (1977)

TitleF LATTICE,NONEQUIV.ATOMS: 1 225 Fm-3mMODE OF CALC=RELA unit=bohr

7.670000 7.670000 7.670000 90.000000 90.000000 90.000000ATOM 1: X=0.00000000 Y=0.00000000 Z=0.00000000

MULT= 1 ISPLIT= 2Au1 NPT= 781 R0=0.00000500 RMT= 2.6000 Z: 79.0LOCAL ROT MATRIX: 1.0000000 0.0000000 0.0000000

0.0000000 1.0000000 0.00000000.0000000 0.0000000 1.0000000

48 NUMBER OF SYMMETRY OPERATIONS

no dependency of the wave function, (n,l,s) are still good quantum numbers

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

Valence electronsValence electrons

Scalar relativistic(no SOC)

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

Valence electronsValence electrons

Scalar relativistic(no SOC)

all relativistic effects are included except SOC small component enters normalization and calculation of charge inside spheres augmentation with large component only SOC can be included in « second variation »

Valence electrons in interstitial region are treated classically

Page 30: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Implementation in WIEN2k: valence electrons

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

Valence electronsValence electrons

Scalar relativistic(no SOC)

Possibility to add SOC(2nd variational)

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

Valence electronsValence electrons

Scalar relativistic(no SOC)

Possibility to add SOC(2nd variational)

SOC is added in a second variation (lapwso):

- First diagonalization (lapw1):- Second diagonalization (lapwso):

1111 H SOHH1

The second equation is expanded in the basis of first eigenvectors (1)

jiN

i

iSO

jjij H 11111

sum include both up/down spin states N is much smaller than the basis size in lapw1

Page 31: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Implementation in WIEN2k: valence electrons

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

Valence electronsValence electrons

Scalar relativistic(no SOC)

Possibility to add SOC(2nd variational)

Atomic sphere (RMT) RegionAtomic sphere (RMT) Region

Valence electronsValence electrons

Scalar relativistic(no SOC)

Possibility to add SOC(2nd variational)

SOC is added in a second variation (lapwso):

- First diagonalization (lapw1):- Second diagonalization (lapwso):

1111 H SOHH1

The second equation is expanded in the basis of first eigenvectors (1)

jiN

i

iSO

jjij H 11111

sum include both up/down spin states N is much smaller than the basis size in lapw1

SOC is active only inside atomic spheres, only spherical potential (VMT) is taken into account, in the polarized case spin up and down parts are averaged.

Eigenstates are not pure spin states, SOC mixes up and down spin states

Off-diagonal term of the spin-density matrix is ignored. It means that in each SCF cycle the magnetization is projected on the chosen direction (from case.inso)

VMT: Muffin-tin potential (spherically symmetric)

Page 32: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Controlling spin-orbit coupling in WIEN2k

Do a regular scalar-relativistic “scf” calculation

save_lapw

initso_lapw

WFFIL4 1 0 llmax,ipr,kpot-10.0000 1.50000 emin,emax (output energy window)0. 0. 1. direction of magnetization (lattice vectors)

NX number of atoms for which RLO is addedNX1 -4.97 0.0005 atom number,e-lo,de (case.in1), repeat NX times0 0 0 0 0 number of atoms for which SO is switch off; atoms

case.inso:

case.in1(c):(…)2 0.30 0.005 CONT 1 0 0.30 0.000 CONT 1

K-VECTORS FROM UNIT:4 -9.0 4.5 65 emin/emax/nband

symmetso (for spin-polarized calculations only)

run(sp)_lapw -so -so switch specifies that scf cycles will include SOC

Page 33: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Controlling spin-orbit coupling in WIEN2k

The w2web interface is helping you

Non-spin polarized case

Page 34: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Controlling spin-orbit coupling in WIEN2k

The w2web interface is helping you

Spin polarized case

Page 35: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativistic effects in the solid: Illustration

LDA overbinding (7%)

No difference NREL/SREL

Bulk modulus:- NREL: 131.4 GPa- SREL: 131.5 GPa- Exp.: 130 GPa

hcp-BeZ = 4

Page 36: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativistic effects in the solid: Illustration

LDA overbinding (7%)

No difference NREL/SREL

Bulk modulus:- NREL: 131.4 GPa- SREL: 131.5 GPa- Exp.: 130 GPa

LDA overbinding (2%)

Clear difference NREL/SREL

Bulk modulus:- NREL: 344 GPa- SREL: 447 GPa- Exp.: 462 GPa

hcp-BeZ = 4

hcp-OsZ = 76

Page 37: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativistic effects in the solid: Illustration

Scalar-relativistic (SREL):- LDA overbinding (2%)- Bulk modulus: 447 GPa

+ spin-orbit coupling (SREL+SO):- LDA overbinding (1%)- Bulk modulus: 436 GPa

Exp. Bulk modulus: 462 GPa

hcp-BeZ = 4

hcp-OsZ = 76

Page 38: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Zansr 0

2

)1( bohr 10 cm

ae

bohr 013.0791)1( sr

r2 (e/bohr)

0.00r (bohr)

0.01 0.02 0.03 0.04 0.05 0.060

10

20

30

40

50Non relativistic (l=0)

r2 (e/bohr)

0.00r (bohr)

0.01 0.02 0.03 0.04 0.05 0.060

10

20

30

40

50Non relativistic (l=0)

r2 (e/bohr)

0.00r (bohr)

0.01 0.02 0.03 0.04 0.05 0.060

10

20

30

40

50

Radius of the 1s orbit (Bohr model):

+Zee-

Atomic units:ħ = me = e = 1

c = 1/ 137 au

AND

Au 1s

(1) Relativistic orbital contraction

Page 39: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

00

acM

RELAae

ee mmM 22.1

Zansr 0

2

)1( bohr 10 mc

a

bohr 013.0791)1( sr

r2 (e/bohr)

0.00r (bohr)

0.01 0.02 0.03 0.04 0.05 0.060

10

20

30

40

50Non relativistic (l=0)Relativistic (=-1)

r2 (e/bohr)

0.00r (bohr)

0.01 0.02 0.03 0.04 0.05 0.060

10

20

30

40

50Non relativistic (l=0)Relativistic (=-1)

r2 (e/bohr)

0.00r (bohr)

0.01 0.02 0.03 0.04 0.05 0.060

10

20

30

40

50Non relativistic (l=0)Relativistic (=-1)Relativistic (=-1)

20% Orbitalcontraction

Radius of the 1s orbit (Bohr model):

+Zee-

AND

In Au atom, the relativistic mass (M) of the 1s electron is 22% larger than

the rest mass (m)

bohr010.022.11

791)1( 0

2

a

Znsr

Au 1s

(1) Relativistic orbital contraction

Page 40: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

0 2 4 60.0

0.1

0.2

0.3

0.4

0.5r2 (e/bohr)

r (bohr)

Non relativistic (l=0)Relativistic (=-1)

0 2 4 60.0

0.1

0.2

0.3

0.4

0.5r2 (e/bohr)

r (bohr)

Non relativistic (l=0)Relativistic (=-1)Relativistic (=-1)

Orbitalcontraction

Au 6s

ns orbitals (with n > 1) contract due to orthogonality to 1s

0046.1

096.01

1

1

122

cve

cnZsve 096.017.13

679)6(

Direct relativistic effect (mass enhancement) contraction of 0.46% only

(1) Relativistic orbital contraction

However, the relativistic contraction of the 6s orbital is large (>20%)

Page 41: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

-40

-30

-20

-10

0

10

20

Relativisticcorrection (%)

1s 2s 4s3s 5s 6s

NRELA

NRELARELA

EEE

r2 (e/bohr)

0.00r (bohr)

0.01 0.02 0.03 0.04 0.05 0.060

10

20

30

40

50

Orbitalcontraction

Non relativistic (l=0)Relativistic (=-1)

Au 1s0 2 4 6

0.0

0.1

0.2

0.3

0.4

0.5r2 (e/bohr)

r (bohr)

r2 (e/bohr)

r ( )

Orbitalcontraction

Non relativistic (l=0)Relativistic (=-1)

Au 6s

(1) Orbital Contraction: Effect on the energy

Page 42: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

(2) Spin-Orbit splitting of p states

1.0

r2 (e/bohr)

r (bohr)0.0 0.5 1.5 2.0

r2 (e/bohr)

r (bohr)2.5

Non relativistic (l=1)Non relativistic (l=1)

Au 5p

0.0

0.1

0.2

0.3

0.5

0.7

0.6

0.4

Page 43: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

(2) Spin-Orbit splitting of p states

l=1

E

j=3/2 (=-2)

orbital moment

spin

+e-e

j=1+1/2=3/2

Spin-orbit splitting of l-quantum number

r2 (e/bohr)r2 (e/bohr)Non relativistic (l=1)Relativistic (=-2)Non relativistic (l=1)Relativistic (=-2)

Au 5p

p3/2 (=-2): nearly same behavior than non-relativistic p-state

1.0r (bohr)

0.0 0.5 1.5 2.0r (bohr)

2.50.0

0.1

0.2

0.3

0.5

0.7

0.6

0.4

Page 44: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

(2) Spin-Orbit splitting of p states

l=1

E

j=1/2 (=1)

spin

orbital moment

+e -e

j=1-1/2=1/2

Spin-orbit splitting of l-quantum number

r2 (e/bohr)r2 (e/bohr)Non relativistic (l=1)

Relativistic (=1)

Non relativistic (l=1)

Relativistic (=1)

Au 5p

p1/2 (=1): markedly different behavior than non-relativistic p-state g=1 is non-zero at nucleus

1.0r (bohr)

0.0 0.5 1.5 2.0r (bohr)

2.50.0

0.1

0.2

0.3

0.5

0.7

0.6

0.4

Page 45: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

(2) Spin-Orbit splitting of p states

l=1

E

j=3/2

j=1/2 (=1)

(=-2)

orbital moment

spin

spin

orbital moment

+e-e

+e -e

j=1+1/2=3/2 j=1-1/2=1/2

Ej=3/2 Ej=1/2

Spin-orbit splitting of l-quantum number

r2 (e/bohr)r2 (e/bohr)Non relativistic (l=1)Relativistic (=-2)Relativistic (=1)

Non relativistic (l=1)Relativistic (=-2)Relativistic (=1)

Au 5p

p1/2 (=1): markedly different behavior than non-relativistic p-state g=1 is non-zero at nucleus

1.0r (bohr)

0.0 0.5 1.5 2.0r (bohr)

2.50.0

0.1

0.2

0.3

0.5

0.7

0.6

0.4

Page 46: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

-40

-30

-20

-10

0

10

20

Relativisticcorrection (%)

2p1/2 2p3/2

3p1/2 3p3/2 4p1/2 4p3/2 5p1/2 5p3/2

NRELA

NRELARELA

EEE

=1 =-2

(2) Spin-Orbit splitting of p states

Scalar-relativistic p-orbital is similar to p3/2 wave function, but does not contain p1/2 radial basis function

r2 (e/bohr)r2 (e/bohr)Non relativistic (l=1)Relativistic (=-2)Relativistic (=1)

Non relativistic (l=1)Relativistic (=-2)Relativistic (=1)

Au 5p

1.0r (bohr)

0.0 0.5 1.5 2.0r (bohr)

2.50.0

0.1

0.2

0.3

0.5

0.7

0.6

0.4

Page 47: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

(3) Orbital expansion: Au(d) states

Higher l-quantum number states expand due to better shielding of nucleus charge from contracted s-states

-e

+Ze-e

-e

Non-relativistic (NREL)

Page 48: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

(3) Orbital expansion: Au(d) states

Higher l-quantum number states expand due to better shielding of nucleus charge from contracted s-states

-e

+Ze-e

-e

Non-relativistic (NREL)

-e

+Zeff1e

Zeff1 = Z-(NREL)

Page 49: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

(3) Orbital expansion: Au(d) states

Higher l-quantum number states expand due to better shielding of nucleus charge from contracted s-states

+Ze-e

-e

+Ze -e

-e

-e

+Zeff1e +Zeff2e

Zeff2 = Z-(REL)

Non-relativistic (NREL) Relativistic (REL)

Zeff1 = Z-(NREL) Zeff1 > Zeff2

-e-e

-e

Page 50: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

(3) Orbital expansion: Au(d) states

Higher l-quantum number states expand due to better shielding of nucleus charge from contracted s-states

-e

+Ze-e

-e

-e

+Ze -e

-e

-e

+Zeff1e +Zeff2e

-e

Zeff2 = Z-(REL)

Non-relativistic (NREL) Relativistic (REL)

Indirect relativistic effect

Zeff1 > Zeff2Zeff1 = Z-(NREL)

Page 51: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

-40

-30

-20

-10

0

10

20

Relativisticcorrection (%)

3d3/2 3d5/2 4d3/2 4d5/2

5d3/2 5d5/2

4f5/2 4f7/2

NRELA

NRELARELA

EEE

0 1 2 30.0

0.1

0.2

0.3

0.4r2 (e/bohr)

r (bohr)

Non relativistic (l=2)Relativistic (=2)Relativistic (=-3)

40 1 2 30.0

0.1

0.2

0.3

0.4r2 (e/bohr)

r (bohr)

Non relativistic (l=2)Relativistic (=2)Relativistic (=-3)

40.0 0.1 0.2 0.30

1

2

3

4r2 (e/bohr)

r (bohr)

Non relativistic (l=2)Relativistic (=2)Relativistic (=-3)

0.40.0 0.1 0.2 0.30

1

2

3

4r2 (e/bohr)

r (bohr)

Non relativistic (l=2)Relativistic (=2)Relativistic (=-3)

0.4

=2 =-3

=3 =-4

Orbitalexpansion

(3) Orbital expansion: Au(d) states

Au 3d Au 5d

Page 52: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

-40

-30

-20

-10

0

10

20

Relativisticcorrection (%)

1s 2s 4s2p1/2 2p3/2

3d3/2 3d5/2

3s3p1/2 3p3/2

5s 6s4p1/2 4p3/2 5p1/2 5p3/2

4d3/2 4d5/2

5d3/2 5d5/2

4f5/2 4f7/2

NRELA

NRELARELA

EEE

Relativistic effects on the Au energy levels

Page 53: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Atomic spectra of gold

SO splitting

SO splitting

Page 54: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Ag – Au: the differences (DOS & optical prop.)

Ag Au

Page 55: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativistic semicore states: p1/2 orbitals

Electronic structure of fcc Th, SOC with 6p1/2 local orbital

J.Kuneš, P.Novak, R.Schmid, P.Blaha, K.Schwarz, Phys.Rev.B. 64, 153102 (2001)

6p1/2

6p1/2

6p3/2

6p3/2

Energy vs. basis size DOS with and without p1/2

p1/2 included

p1/2 not included

Page 56: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

SOC in magnetic systems

SOC couples magnetic moment to the lattice

Symmetry operations acts in real and spin space

direction of the exchange field matters (input in case.inso)

number of symmetry operations may be reduced (reflections act differently on spins than on positions)

time inversion is not symmetry operation (do not add an inversion for klist)

initso_lapw (must be executed) detects new symmetry setting

[100] [010] [001] [110]

1

mx

my

2z

A A A A

A B B -

B A B -B B A B

Direction of magnetization

Page 57: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativity in WIEN2k: Summary

WIEN2k offers several levels of treating relativity:non-relativistic: select NREL in case.struct (not recommended)

standard: fully-relativistic core, scalar-relativistic valence

mass-velocity and Darwin s-shift, no spin-orbit interaction

”fully”-relativistic:

adding SO in “second variation” (using previous eigenstates as basis)

adding p1/2 LOs to increase accuracy (caution!!!)

x lapw1 (increase E-max for more eigenvalues, to havex lapwso basis for lapwso)

x lapw2 –so -c SO ALWAYS needs complex lapw2 version

Non-magnetic systems:

SO does NOT reduce symmetry. initso_lapw just generates case.inso and case.in2c.

Magnetic systems:

symmetso dedects proper symmetry and rewrites case.struct/in*/clm*

Page 58: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

ATOMIC STRUCTURE OF CuO

CuO4 square planar

Cu

O

CuO interlude

Page 59: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

ATOMIC STRUCTURE OF CuO

CuO2 ribbons

Cu

O

CuO interlude

Page 60: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

ATOMIC STRUCTURE OF CuO

Oxygen 4-fold coordinated

Cu

O

CuO interlude

Page 61: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

ATOMIC STRUCTURE OF CuO

Monoclinic 3D atomic structure

Cu

O

CuO interlude

Page 62: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

MAGNETIC STRUCTURE OF CuO

Cu

O

CuO interlude

Page 63: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

MAGNETIC STRUCTURE OF CuO

Cu

O

c

a

+

+

+‐

‐ ‐

CuO interlude

Page 64: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

AFM interactions along [1 0 -1]

FM interactions along [1 0 1]

LOW-TEMPERATURE MAGNETIC STRUCTURE OF CuO FROMSINGLE-CRYSTAL NEUTRON DIFFRACTION[1]

O

Cu

Cu

[1] J.B. Forsyth et al., J. Phys. C: Solid State Phys. 21 (1988) 2917

+

+

+

‐ + ‐

‐ +

+

+

+

CuO interlude

Magnetic moments are along the [0 1 0] direction

a

c

Page 65: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

[1] X. Rocquefelte, P. Blaha, K. Schwarz, S. Kumar, J. van den Brink, Nature Comm., Accepted

CuO interlude

Estimation of the Magneto-crystalline Anisotropy Energy (MAE) of CuO

Allows to define the magnetization easy and hard axes

Here we have considered the following expression:

MAE = E[u v w] – E[0 1 0]

E[uvw] is the energy deduced from spin-orbit calculations with the magnetization along the [uvw]

crystallographic direction

Page 66: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Relativistic effects&

Non-collinear magnetism

(WIEN2k / WIENncm)

Xavier RocquefelteInstitut des Matériaux Jean‐Rouxel (UMR 6502)

Université de Nantes, FRANCE

20th WIEN2k WorkshopPennStateUniversity – 2013

Page 67: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Pauli Hamiltonian for magnetic systems

...2

22

lBVm

H effBeffe

P

2x2 matrix in spin space, due to Pauli spin operators

0110

1

00

2 ii

10

013

(22) Pauli spin matrices

Page 68: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Pauli Hamiltonian for magnetic systems

...2

22

lBVm

H effBeffe

P

2x2 matrix in spin space, due to Pauli spin operators

Wave function is a 2-component vector (spinor) – It corresponds to the large components of the dirac wave function (small components are neglected)

2

1

2

1 PH spin upspin down

0110

1

00

2 ii

10

013

(22) Pauli spin matrices

Page 69: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Pauli Hamiltonian for magnetic systems

...2

22

lBVm

H effBeffe

P

2x2 matrix in spin space, due to Pauli spin operators

Effective electrostatic potential

Effective magnetic field

xcHexteff VVVV xcexteff BBB

Exchange-correlation potential

Exchange-correlation field

Page 70: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Pauli Hamiltonian for magnetic systems

...2

22

lBVm

H effBeffe

P

2x2 matrix in spin space, due to Pauli spin operators

Effective electrostatic potential

Effective magnetic field

Spin-orbit coupling

drdV

rcM e

12 22

2

xcHexteff VVVV xcexteff BBB

Exchange-correlation potential

Exchange-correlation field

Many-body effects which are defined within DFT LDA or GGA

Page 71: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Exchange and correlation

From DFT exchange correlation energy:

3 , , drmrrmrE homxcxc

Local function of the electronic density () and the magnetic moment (m)

Definition of Vxc and Bxc (functional derivatives):

mEV xc

xc

, m

mEB xcxc

,

LDA expression for Vxc and Bxc:

mmV

homxchom

xcxc

,, m

mmB

homxc

xc ˆ,

Bxc is parallel to the magnetization density vector (m)^

Page 72: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Non-collinear magnetism

Direction of magnetization vary in space, thus spin-orbit term is present

...2

22

lBVm

H effBeffe

P

...2

...2

22

22

zBeffe

yxB

yxBzBeffe

BVm

iBB

iBBBVm

Non-collinear magnetic moments

2

1

1 and 2 are non-zero

Solutions are non-pure spinors

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Collinear magnetism

Magnetization in z-direction / spin-orbit is not present

...2

22

lBVm

H effBeffe

P

...2

0

0...2

22

22

zBeffe

zBeffe

BVm

BVm

Collinear magnetic moments

Solutions are pure spinors

0

1

2

0

Non-degenerate energies

Page 74: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Non-magnetic calculation

No magnetization present, Bx = By = Bz = 0 and no spin-orbit coupling

...2

22

lBVm

H effBeffe

P

effe

effe

Vm

Vm

22

22

20

02

0

0

Solutions are pure spinors

Degenerate spin solutions

Page 75: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Magnetism and WIEN2k

Wien2k can only handle collinear or non-magnetic cases

run_lapw script:

x lapw0x lapw1x lapw2x lcorex mixer

non-magnetic case

m = n – n = 0

run_lapw script:

x lapw0x lapw1 –upx lapw1 -dnx lapw2 –upx lapw2 -dnx lcore –upx lcore -dnx mixer

magnetic case

m = n – n 0DOS

EF

DOS

EF

Page 76: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Magnetism and WIEN2k

Spin-polarized calculations

runsp_lapw script (unconstrained magnetic calc.)

runfsm_lapw -m value (constrained moment calc.)

runafm_lapw (constrained anti-ferromagnetic calculation)

spin-orbit coupling can be included in second variational step

never mix polarized and non-polarized calculations in one case directory !!!

Page 77: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Non-collinear magnetism

code based on Wien2k (available for Wien2k users)

In case of non-collinear spin arrangements WIENncm (WIEN2k clone) has to be used:

structure and usage philosophy similar to Wien2k independent source tree, independent installation

WIENncm properties:

real and spin symmetry (simplifies SCF, less k-points)

constrained or unconstrained calculations (optimizes magnetic moments)

SOC in first variational step, LDA+U

Spin spirals

Page 78: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

Non-collinear magnetism

For non-collinear magnetic systems, both spin channels have to be considered simultaneously

runncm_lapw script:

xncm lapw0xncm lapw1xncm lapw2xncm lcorexncm mixer

Relation between spin density matrix and magnetization

mz = n – n 0

mx = ½(n + n) 0

my = i½(n - n) 0

DOS

EF

Page 79: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

WienNCM: Spin spirals

Transverse spin wave

qR

R cos , sinsin , cos nnn RqRqmm

spin-spiral is defined by a vector q given in reciprocal space and an angle between magnetic moment and rotation axis.

Rotation axis is arbitrary (no SOC) – fixed as z-axis in WIENNCM

Translational symmetry is lost !

But WIENncm is using the generalized Bloch theorem. The calculation of spin waves only requires one unit cell for even incommensurate modulation q vector.

Page 80: Relativistic effects Non-collinear magnetism …susi.theochem.tuwien.ac.at/.../Relativity-NCM.pdfRelativistic effects & Non-collinear magnetism (WIEN2k / WIENncm) 20th WIEN2k Workshop

WienNCM: Usage

1. Generate the atomic and magnetic structures

2. Run initncm (initialization script)

3. Run the NCM calculation:

Create atomic structure

Create magnetic structure

See utility programs: ncmsymmetry, polarangles, …

xncm (WIENncm version of x script)

runncm (WIENncm version of run script)

More information on the manual (Robert Laskowski)

[email protected]


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