MAGMOM: Difference between revisions

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{{TAGDEF|MAGMOM|[real array]}}
{{TAGDEF|MAGMOM|[real array]}}
{{DEF|MAGMOM|NIONS * 1.0|for {{TAG|ISPIN}}{{=}}2|3 * NIONS * 1.0 |for non-collinear magnetic systems ({{TAG|LNONCOLLINEAR}}{{=}}.T.)}}
{{DEF|MAGMOM|NIONS * 1.0|for {{TAG|ISPIN}}{{=}}2|3 * NIONS * 1.0 |for noncollinear magnetic systems ({{TAG|LNONCOLLINEAR}}{{=}}.TRUE.)}}


Description: {{TAG|MAGMOM}} Specifies the initial magnetic moment for each atom, if and only if {{TAG|ICHARG}}=2, or if  {{TAG|ICHARG}}=1 and the {{TAG|CHGCAR}} file contains no magnetisation density
Description: Initial magnetic moment for each atom if no magnetization density is present. Considered when symmetry is determined.
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If one is searching for a spin polarised (ferro- or antiferromagnetic) solution,
it is usually safest to start from larger local magnetic moments, because in
some cases, the default values might not be sufficiently big.
A safe default is usually the experimental magnetic moment multiplied by
1.2 or 1.5. It is important to emphasize that the {{TAG|MAGMOM}} tag is
used ''only'', if
the {{TAG|CHGCAR}} file holds no information on the magnetisation density, ''and''
if the initial charge density is not calculated from the wavefunctions supplied in
the {{TAG|WAVECAR}} file.
This means that the {{TAG|MAGMOM}} tag is useful for two kind of calculations


*Calculations starting from scratch with no {{TAG|WAVECAR}} and {{TAG|CHGCAR}} file.
* For a '''magnetic calculation from scratch''' ({{TAG|ISTART}}=0), {{TAG|MAGMOM}} specifies (i) the initial on-site magnetic moment for each atom, and (ii) lowers the symmetry of the system (as of VASP.4.4.4). A magnetic calculation could be either a spin-polarized calculation ({{TAG|ISPIN}}=2) or noncollinear calculation ({{TAG|LNONCOLLINEAR}}=T). If the {{TAG|MAGMOM}} line breaks a symmetry of the crystal, the corresponding symmetry operation is removed and not applied during the symmetrization of, e.g., charges and forces.


*Calculations starting from  a ''non magnetic'' {{TAG|WAVECAR}} and {{TAG|CHGCAR}} file ({{TAG|ICHARG}}=1).
* When '''restarting a magnetic calculation''', {{TAG|MAGMOM}} is only used to determine the symmetry of the system and not to set the on-site magnetic moment. Therefore, if you remove the {{TAG|MAGMOM}} tag before restarting from a converged {{FILE|WAVECAR}} or {{FILE|CHGCAR}}, the magnetization is likely to be symmetrized away.


Often such calculations converge more reliably to the desired magnetic
* {{TAG|MAGMOM}} also specifies the initial on-site magnetic moments when a '''magnetic calculation''' ({{TAG|ISPIN}}=2 or {{TAG|LNONCOLLINEAR}}=T) is '''started from a non-spin-polarized calculation''' ({{TAG|ISPIN}}=1 and {{TAG|LNONCOLLINEAR}}=F). This implies restarting with {{TAG|ICHARG}}=1 while the {{TAG|CHGCAR}} file contains no magnetization density. Starting magnetic calculations from a non-spin-polarized calculation can improve convergence.
configuration than calculations of the first kind. Hence, if you have
The {{TAG|I_CONSTRAINED_M}} tag can constrain the on-site magnetic moments.
problems to converge to a desired magnetic solution, try to calculate
{{NB|tip|To converge to the magnetic ground state, we recommend setting the magnetic moments slightly larger than the expected values, e.g., using the experimental magnetic moment multiplied by 1.2 or 1.5.|}}
first the non magnetic groundstate, and continue from the generated
{{NB|important|The final magnetic state strongly depends on the initial values for {{TAG|MAGMOM}}.{{Cite|huebsch:prx:11}} This is true even if no symmetry is used ({{TAG|ISYM}}{{=}}-1), because of the many local minima that most exchange-correlation functionals have within spin-density-functional theory.|}}
{{TAG|WAVECAR}} and {{TAG|CHGCAR}} file. For the continuation job, you need to set
== Format and basis ==
{{TAG|ISPIN}} {{=}} 2
{{TAG|ICHARG}} {{=}} 1  
in the {{TAG|INCAR}} file.


Starting from VASP.4.4.4, VASP also determines whether the magnetic moments supplied in
* For a spin-polarized calculation ({{TAG|ISPIN}}=2), {{TAG|MAGMOM}} is a list of NIONS positive or negative values that specify the magnitude and relative orientation of the magnetization on each ion. The on-site magnetic moments have no direction in real space, i.e., no orientation in the lattice.
the {{TAG|MAGMOM}} line break the symmetry. If they do, the corresponding symmetry operations are removed
 
and not applied during the symmetrization of charges and forces. This means that antiferromagnetic (AFM) calculations can be performed by
* For noncollinear calculation ({{TAG|LNONCOLLINEAR}}=T), the on-site magnetic moment is specified by three components for each ion. Without spin-orbit coupling ({{TAG|LSORBIT}}=False), the total energy depends only on the relative direction of the on-site magnetic moments. Hence, you can give the desired magnetic structure in Cartesian coordinates without considering how the lattice matrix or {{TAG|SAXIS}} is defined.
specifying anti-parallel magnetic moments for the atoms in the cell: The most simple {{TAG|POSCAR}}-file for a bcc-cell with AFM spin alignment  
 
would be
* With spin-orbit coupling ({{TAG|LSORBIT}}=True), the three components must be specified in the basis of spinor space that is defined by {{TAG|SAXIS}}. The default is <math>\sigma_1=\hat x</math>, <math>\sigma_2 =\hat y</math>, <math>\sigma_3 = \hat z</math>, such that {{TAG|MAGMOM}} can be given in Cartesian coordinates. The orientation of {{TAG|MAGMOM}} with respect to the lattice only matters if spin-orbit coupling is included ({{TAG|LSORBIT}}). 
AF
 
  2.8000
== Examples ==
 
* The most simple input for a bcc cell with AFM spin alignment would be the following.
 
:{{TAG|POSCAR}} file:
  AFM
   2.80000
   2.80000
   1.00000  .00000  .00000
   1.00000  .00000  .00000
Line 40: Line 32:
   .00000  .00000  1.00000
   .00000  .00000  1.00000
   1 1
   1 1
  Carthesian
  Cartesian
   .00000  .00000  .00000
   .00000  .00000  .00000
   .50000  .50000  .50000
   .50000  .50000  .50000
with  
:with  
   {{TAG|ISPIN}} = 2
   {{TAG|ISPIN}} = 2
   {{TAG|MAGMOM}} = 1.0 -1.0
   {{TAG|MAGMOM}} = 1.0 -1.0
specified in {{TAG|INCAR}}.
:specified in {{FILE|INCAR}}. In a perfectly AFM ordered cell, the total net magnetisation is zero, but the local magnetic moments can be written to the {{FILE|OUTCAR}} file by setting {{TAG|LORBIT}} tag (and if {{TAG|LORBIT}}<10 , the {{TAG|RWIGS}} tag in addition) in the {{FILE|INCAR}} file.
In a perfectly AFM ordered cell, the total net magnetisation
is zero as a matter of fact, but it is possible to determine the local magnetic moments by using the {{TAG|LORBIT}} tag (and if {{TAG|LORBIT}}<10 , the {{TAG|RWIGS}}-tag in addition).


In the case of spin-orbit coupling ({{TAG|LSORBIT}}) the 3D-orientation of the magnetic moments has to be given with respect to the spin-quantisation axis {{TAG|SAXIS}}.
* If you have problems converging to a desired magnetic solution, try to calculate first the non-magnetic ground state and continue from the generated {{TAG|WAVECAR}} and {{TAG|CHGCAR}}. To restart, e.g., a calculation with two atoms that have equally large and antiferromagnetically coupled on-site magnetic moments, you need to set the following in the {{TAG|INCAR}} file:
{{TAG|ICHARG}} = 1
{{TAG|ISPIN}} = 2
{{TAG|MAGMOM}} = m -m
:or for a noncollinear
{{TAG|ICHARG}} = 1
{{TAG|LNONCOLLINEAR}} = T
{{TAG|MAGMOM}} = 0 0 m  0 0 -m


* For systems containing many atoms, {{TAG|MAGMOM}} input on a single line can be hard to read, especially in the noncollinear case. It is possible to provide {{TAG|INCAR}} input on [[INCAR#Format|multiple lines]] using backslashes ('''\''') as linebreaks. E.g. for a noncollinear system with AFM alignment and 16 atoms (the first 8 of them magnetic), the multi-line input could look like this:
{{TAG|MAGMOM}} =  3.0  2.0  1.0 \
          -3.0 -2.0 -1.0 \
          3.0  2.0  1.0 \
          -3.0 -2.0 -1.0 \
          3.0  2.0  1.0 \
          -3.0 -2.0 -1.0 \
          3.0  2.0  1.0 \
          -3.0 -2.0 -1.0 \
          24*0.0


== Related Tags and Sections ==
== Related Tags and Sections ==
{{TAG|ISPIN}},
{{TAG|ISPIN}},
{{TAG|ICHARG}},
{{TAG|LNONCOLLINEAR}}, {{TAG|LSORBIT}}, {{TAG|SAXIS}},
{{TAG|LNONCOLLINEAR}}, {{TAG|LSORBIT}}, {{TAG|SAXIS}},
{{TAG|LORBIT}}, {{TAG|RWIGS}}
{{TAG|LORBIT}},
{{TAG|I_CONSTRAINED_M}}


{{sc|MAGMOM|Examples|Examples that use this tag}}
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[[The_VASP_Manual|Contents]]


[[Category:INCAR]][[Category:Magnetism]]
[[Category:INCAR tag]][[Category:Magnetism]][[Category:Symmetry]]

Latest revision as of 10:15, 17 October 2024

MAGMOM = [real array] 

Default: MAGMOM = NIONS * 1.0 for ISPIN=2
= 3 * NIONS * 1.0 for noncollinear magnetic systems (LNONCOLLINEAR=.TRUE.)

Description: Initial magnetic moment for each atom if no magnetization density is present. Considered when symmetry is determined.


  • For a magnetic calculation from scratch (ISTART=0), MAGMOM specifies (i) the initial on-site magnetic moment for each atom, and (ii) lowers the symmetry of the system (as of VASP.4.4.4). A magnetic calculation could be either a spin-polarized calculation (ISPIN=2) or noncollinear calculation (LNONCOLLINEAR=T). If the MAGMOM line breaks a symmetry of the crystal, the corresponding symmetry operation is removed and not applied during the symmetrization of, e.g., charges and forces.
  • When restarting a magnetic calculation, MAGMOM is only used to determine the symmetry of the system and not to set the on-site magnetic moment. Therefore, if you remove the MAGMOM tag before restarting from a converged WAVECAR or CHGCAR, the magnetization is likely to be symmetrized away.
  • MAGMOM also specifies the initial on-site magnetic moments when a magnetic calculation (ISPIN=2 or LNONCOLLINEAR=T) is started from a non-spin-polarized calculation (ISPIN=1 and LNONCOLLINEAR=F). This implies restarting with ICHARG=1 while the CHGCAR file contains no magnetization density. Starting magnetic calculations from a non-spin-polarized calculation can improve convergence.

The I_CONSTRAINED_M tag can constrain the on-site magnetic moments.

Tip: To converge to the magnetic ground state, we recommend setting the magnetic moments slightly larger than the expected values, e.g., using the experimental magnetic moment multiplied by 1.2 or 1.5.
Important: The final magnetic state strongly depends on the initial values for MAGMOM.[1] This is true even if no symmetry is used (ISYM=-1), because of the many local minima that most exchange-correlation functionals have within spin-density-functional theory.

Format and basis

  • For a spin-polarized calculation (ISPIN=2), MAGMOM is a list of NIONS positive or negative values that specify the magnitude and relative orientation of the magnetization on each ion. The on-site magnetic moments have no direction in real space, i.e., no orientation in the lattice.
  • For noncollinear calculation (LNONCOLLINEAR=T), the on-site magnetic moment is specified by three components for each ion. Without spin-orbit coupling (LSORBIT=False), the total energy depends only on the relative direction of the on-site magnetic moments. Hence, you can give the desired magnetic structure in Cartesian coordinates without considering how the lattice matrix or SAXIS is defined.
  • With spin-orbit coupling (LSORBIT=True), the three components must be specified in the basis of spinor space that is defined by SAXIS. The default is , , , such that MAGMOM can be given in Cartesian coordinates. The orientation of MAGMOM with respect to the lattice only matters if spin-orbit coupling is included (LSORBIT).

Examples

  • The most simple input for a bcc cell with AFM spin alignment would be the following.
POSCAR file:
AFM
 2.80000
 1.00000   .00000   .00000
  .00000  1.00000   .00000
  .00000   .00000  1.00000
 1 1
Cartesian
  .00000   .00000   .00000
  .50000   .50000   .50000
with
 ISPIN = 2
 MAGMOM = 1.0 -1.0
specified in INCAR. In a perfectly AFM ordered cell, the total net magnetisation is zero, but the local magnetic moments can be written to the OUTCAR file by setting LORBIT tag (and if LORBIT<10 , the RWIGS tag in addition) in the INCAR file.
  • If you have problems converging to a desired magnetic solution, try to calculate first the non-magnetic ground state and continue from the generated WAVECAR and CHGCAR. To restart, e.g., a calculation with two atoms that have equally large and antiferromagnetically coupled on-site magnetic moments, you need to set the following in the INCAR file:
ICHARG = 1 
ISPIN = 2 
MAGMOM = m -m
or for a noncollinear
ICHARG = 1
LNONCOLLINEAR = T
MAGMOM = 0 0 m  0 0 -m
  • For systems containing many atoms, MAGMOM input on a single line can be hard to read, especially in the noncollinear case. It is possible to provide INCAR input on multiple lines using backslashes (\) as linebreaks. E.g. for a noncollinear system with AFM alignment and 16 atoms (the first 8 of them magnetic), the multi-line input could look like this:
MAGMOM =  3.0  2.0  1.0 \
         -3.0 -2.0 -1.0 \
          3.0  2.0  1.0 \
         -3.0 -2.0 -1.0 \
          3.0  2.0  1.0 \
         -3.0 -2.0 -1.0 \
          3.0  2.0  1.0 \
         -3.0 -2.0 -1.0 \
          24*0.0

Related Tags and Sections

ISPIN, LNONCOLLINEAR, LSORBIT, SAXIS, LORBIT, I_CONSTRAINED_M

Examples that use this tag