BEXT: Difference between revisions
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{{DISPLAYTITLE:BEXT}} | {{DISPLAYTITLE:BEXT}} | ||
{{TAGDEF|BEXT|[real | {{TAGDEF|BEXT|[real] ( [real] [real] )}} | ||
{{DEF|BEXT|0.0|if {{TAG|ISPIN}}{{=}}2|3*0.0|if {{TAG|LNONCOLLINEAR}}{{=}}.TRUE.| N/A | else}} | {{DEF|BEXT|0.0|if {{TAG|ISPIN}}{{=}}2|3*0.0|if {{TAG|LNONCOLLINEAR}}{{=}}.TRUE.| N/A | else}} | ||
Description: | Description: Specifies an external magnetic field in eV. | ||
---- | ---- | ||
{{TAG|BEXT}} tag sets an external magnetic field that acts on the electrons in a Zeeman-like manner. | |||
An additional potential of the following form carries this interaction: | |||
* For {{TAG|ISPIN}} = 2: | * For spin-polarized calculations ({{TAG|ISPIN}} = 2): | ||
:<math> | :<math> | ||
V^{\uparrow} = V^{\uparrow} + B_{\rm ext} | V^{\uparrow} = V^{\uparrow} + B_{\rm ext} | ||
Line 19: | Line 19: | ||
:and <math>B_{\rm ext}</math> = {{TAG|BEXT}} (in eV). | :and <math>B_{\rm ext}</math> = {{TAG|BEXT}} (in eV). | ||
* For {{TAG|LNONCOLLINEAR}} = .TRUE.: | * For noncollinear calculations ({{TAG|LNONCOLLINEAR}} = .TRUE.): | ||
:<math> | :<math> | ||
V_{\alpha\beta} = V_{\alpha\beta} + \ | V_{\alpha\beta} = V_{\alpha\beta} + \mathbf{B}_{\rm ext} \cdot \mathbf{\sigma}_{\alpha \beta} | ||
</math> | </math> | ||
:where <math> | :where <math>\mathbf{B}_{\rm ext}=({B}^1_{\rm ext}, {B}^2_{\rm ext}, {B}^3_{\rm ext})^T</math> is given by | ||
{{CB|{{TAGBL|BEXT}} {{=}} B1 B2 B3 ! in eV|:}} | |||
:and <math>\mathbf{\sigma}</math> is the vector of Pauli matrices ({{TAG|SAXIS}}, default: <math>\sigma_1=\hat x</math>, <math>\sigma_2 =\hat y</math>, <math>\sigma_3 = \hat z</math>). | |||
The effect of the above is most easily understood for the collinear case ({{TAG|ISPIN}}=2): | |||
The eigenenergies of spin-up states are raised by <math>B_{\rm ext}</math> eV, whereas the eigenenergies of spin-down states are lowered by the same amount. The total energy changes by: | |||
::<math>\Delta E = (n^{\uparrow} - n^{\downarrow}) B_{\rm ext} | ::<math>\Delta E = (n^{\uparrow} - n^{\downarrow}) B_{\rm ext} | ||
</math> eV | </math> eV | ||
where <math>n^{\uparrow}</math> and <math>n^{\downarrow}</math> are the number of up- and down-spin electrons in the system. | |||
{{TAG|BEXT}} is applied during the self-consistent [[electronic minimization]] and effectively shifts the eigenenergies of the spin-up and spin-down states w.r.t. each other at each step. Consequently, the electrons redistribute (changing the occupancies) ''and'' the density changes. The change in the density (,e.g., charge density and magnetization) also affects the scf potential and KS orbitals. For a rigid-band Zeeman splitting, converge the charge density with {{TAG|BEXT}}=0 and restart with {{TAG|BEXT}}<math>\neq</math>0 and fixed charge density ({{TAG|ICHARG}}=11). | |||
== Units == | |||
For an applied magnetic field <math>B_0</math>, the energy difference between two Zeeman-splitted electronic states is given by: | |||
:<math> | :<math> | ||
\hbar \omega = g_e \mu_B B_0 | \hbar \omega = g_e \mu_B B_0, | ||
</math> | </math> | ||
where <math>\mu_B</math> is the Bohr magneton and <math>g_e</math> is the electron ''g''-factor. | where <math>\mu_B</math> is the Bohr magneton and <math>g_e</math> is the electron spin ''g''-factor. | ||
For {{TAG|ISPIN}}=2, | For {{TAG|ISPIN}}=2, rigid-band Zeeman-splitted states imply: | ||
:<math> | :<math> | ||
V^{\uparrow} - V^{\downarrow} = 2 B_{\rm ext} | V^{\uparrow} - V^{\downarrow} = 2 B_{\rm ext} | ||
Line 56: | Line 59: | ||
{{TAG|ISPIN}}, | {{TAG|ISPIN}}, | ||
{{TAG|LNONCOLLINEAR}} | {{TAG|LNONCOLLINEAR}}, | ||
{{TAG|SAXIS}} | |||
---- | ---- | ||
[[Category:INCAR tag]] [[Category:Magnetism]] | [[Category:INCAR tag]] [[Category:Magnetism]] |
Latest revision as of 13:45, 27 June 2024
BEXT = [real] ( [real] [real] )
Default: BEXT | = 0.0 | if ISPIN=2 |
= 3*0.0 | if LNONCOLLINEAR=.TRUE. | |
= N/A | else |
Description: Specifies an external magnetic field in eV.
BEXT tag sets an external magnetic field that acts on the electrons in a Zeeman-like manner. An additional potential of the following form carries this interaction:
- For spin-polarized calculations (ISPIN = 2):
- and = BEXT (in eV).
- For noncollinear calculations (LNONCOLLINEAR = .TRUE.):
- where is given by
- BEXT = B1 B2 B3 ! in eV
- and is the vector of Pauli matrices (SAXIS, default: , , ).
The effect of the above is most easily understood for the collinear case (ISPIN=2): The eigenenergies of spin-up states are raised by eV, whereas the eigenenergies of spin-down states are lowered by the same amount. The total energy changes by:
- eV
where and are the number of up- and down-spin electrons in the system.
BEXT is applied during the self-consistent electronic minimization and effectively shifts the eigenenergies of the spin-up and spin-down states w.r.t. each other at each step. Consequently, the electrons redistribute (changing the occupancies) and the density changes. The change in the density (,e.g., charge density and magnetization) also affects the scf potential and KS orbitals. For a rigid-band Zeeman splitting, converge the charge density with BEXT=0 and restart with BEXT0 and fixed charge density (ICHARG=11).
Units
For an applied magnetic field , the energy difference between two Zeeman-splitted electronic states is given by:
where is the Bohr magneton and is the electron spin g-factor.
For ISPIN=2, rigid-band Zeeman-splitted states imply:
This leads to the following relationship between our definition of (in eV) and the magnetic field (in T):
where = 5.788 381 8060 x 10-5 eV T-1, and = 2.002 319 304 362 56.