Physical Field Theory

In this chapter we will describe physical field equations used in Agros2D.

Electrostatic

Electrostatic field can be described by Poisson partial differential equation

\div \varepsilon\, \grad \varphi = \rho,

where \varepsilon is permittivity of the material, \varphi is electrical scalar potential and \rho is subdomain charge density. Electric field can be written as

\vec{E} = - \grad \varphi

and electric displacement is

\vec{D} = \varepsilon \vec{E}.

Maxwell stress tensor:

\vec{S}_\mathrm{M} = \vec{E} \otimes \vec{D} - \frac{1}{2} \vec{E} \vec{D} \cdot \delta

Boundary conditions

  • Dirichlet BC

    Scalar potential \varphi = f on the boundary is known.

  • Neumann BC

    Surface charge density D_\mathrm{n} = g on the boundary is known.

Boundary integrals

Charge:

Q = \int_S D_\mathrm{n} \dif S = \int_S \varepsilon \frac{\partial \varphi}{\partial n} \dif S\,\,\,\mathrm{(C)}

Subdomain integrals

Energy:

W_\mathrm{e} = \int_V \frac{1}{2} \vec{E} \vec{D} \dif V\,\,\,\mathrm{(J)}

Maxwell force:

\vec{F}_\mathrm{M} = \int_S \vec{S}_\mathrm{M} \dif S = \int_V \div \vec{S}_\mathrm{M} \dif V\,\,\,\mathrm{(N)}

Current Field

Current field can be described by Laplace partial differential equation

\div \sigma\, \grad \varphi = 0,

where \sigma is electric conductivity of the material and \varphi is electrical scalar potential. Electric field can be written as

\vec{E} = - \grad \varphi

and electric current density is

\vec{J} = \sigma \vec{E}.

Boundary conditions

  • Dirichlet BC

    Scalar potential \varphi = f on the boundary is known.

  • Neumann BC

    Current density J_\mathrm{n} = \sigma \frac{\partial \varphi}{\partial n} = g on the boundary is known.

Boundary integrals

Current:

I = \int_S J_\mathrm{n} \dif S = \int_S \sigma \frac{\partial \varphi}{\partial n} \dif S\,\,\,\mathrm{(A)}

General Magnetic Field

General magnetic field can be desribed by partial differential equation

\curl \frac{1}{\mu}\, \left( \curl \vec{A} - \vec{B}_\mathrm{r} \right) + \sigma \vec{v} \times \curl \vec{A} + \sigma \frac{\partial \vec{A}}{\partial t} = \vec{J}_\mathrm{ext},

where \mu is permeability of the material, \vec{A} = ( A_z\,\mathrm{or}\,A_{\varphi} ) is component of the magnetic vector potential, \vec{B}_\mathrm{r} is remanent flux density, \vec{v} is velocity, \sigma is electric conductivity and finally J_\mathrm{ext} = ( \vec{J}_z\,\mathrm{or}\,J_{\varphi} ) is component of source current density. Magnetic flux density is given by form

\vec{B} = \curl \vec{A},

magnetic field is

\vec{H} = \frac{\vec{B}}{\mu},

eddy current density is

J_\mathrm{trans} = \sigma \frac{\partial \vec{A}}{\partial t},

velocity current density is

J_\mathrm{vel} = \sigma \vec{v} \times \vec{B} = \sigma \vec{v} \times \curl \vec{A},

and total current density is

J_\mathrm{tot} = J_\mathrm{ext} + J_\mathrm{trans} + J_\mathrm{vel}.

Maxwell stress tensor:

\mat{S}_\mathrm{M} = \vec{H} \otimes \vec{B} - \frac{1}{2} \vec{H} \vec{B} \cdot \mat{I}

Boundary conditions

  • Dirichlet BC

    Component of the magnetic vector potential A = f on the boundary is known.

  • Neumann BC

    Normal derivative of magnetic vector potential \frac{\partial A}{\partial n} = g on the boundary is known.

Subdomain integrals

External current:

I_\mathrm{ext} = \int_V J_\mathrm{ext} \dif V\,\,\,\mathrm{(A)}

Eddy current:

I_\mathrm{trans} = \int_V J_\mathrm{trans} \dif V\,\,\,\mathrm{(A)}

Velocity current:

I_\mathrm{vel} = \int_V J_\mathrm{vel} \dif V\,\,\,\mathrm{(A)}

Total current:

I_\mathrm{tot} = I_\mathrm{ext} + I_\mathrm{trans} + I_\mathrm{vel}

Power losses:

P_\mathrm{j} = \int_V \frac{J_\mathrm{tot}^2}{\sigma} \dif V\,\,\,\mathrm{(W)}

Energy:

W_\mathrm{m} = \int_V \frac{1}{2} \vec{H} \vec{B} \dif V\,\,\,\mathrm{(J)}

Lorentz force:

\vec{F} = \int_V J_\mathrm{tot} \times \vec{B} \dif V = \int_V J_\mathrm{tot} \times \curl \vec{A} \dif V\,\,\,\mathrm{(N)}

Maxwell force:

\vec{F}_\mathrm{M} = \oint_S \mat{S}_\mathrm{M} \dif S \,\,\,\mathrm{(N)}

Torque (planar arrangement only):

T_\mathrm{z} = \int_V \vec{r} \times \vec{F} \dif V\,\,\,\mathrm{(Nm)}

Harmonic Magnetic Field

Harmonic magnetic field can be described by partial differential equation

\curl \frac{1}{\mu}\, \left( \curl \vecfaz{A} - \vec{B}_\mathrm{r} \right) + \sigma \vec{v} \times \curl \vecfaz{A} + \mj \omega \sigma \vecfaz{A} = \vecfaz{J}_\mathrm{ext},

where \mu is permeability of the material, \faz{A} = ( \faz{A}_z\,\mathrm{or}\,\faz{A}_{\varphi} ) is component of the magnetic vector potential, \omega = 2 \pi f is frequency, \sigma is electric conductivity, \vec{v} is velocity and finally \faz{J}_\mathrm{ext} = ( \faz{J}_z\,\mathrm{or}\,\faz{J}_{\varphi} ) is component of source current density. Magnetic flux density is given by form

\vecfaz{B} = \curl \vecfaz{A},

magnetic field is

\vecfaz{H} = \frac{\vecfaz{B}}{\mu},

eddy current density is

\vecfaz{J}_\mathrm{trans} = \mj \omega \sigma \vecfaz{A},

velocity current density is

\vecfaz{J}_\mathrm{vel} = \sigma \vec{v} \times \vecfaz{B} = \sigma \vec{v} \times \curl \vecfaz{A},

and total current density is

\vecfaz{J}_\mathrm{tot} = \vecfaz{J}_\mathrm{ext} + \vecfaz{J}_\mathrm{trans} + \vecfaz{J}_\mathrm{vel}.

Boundary conditions

  • Dirichlet BC

    Component of the magnetic vector potential \faz{A} = \faz{f} on the boundary is known.

  • Neumann BC

    Normal derivative of magnetic vector potential \frac{\partial \faz{A}}{\partial n} = \faz{g} on the boundary is known.

Subdomain integrals

External current:

\faz{I}_\mathrm{ext} = \int_S \vecfaz{J}_\mathrm{ext} \dif S\,\,\,\mathrm{(A)}

Eddy current:

\faz{I}_\mathrm{trans} = \int_S \vecfaz{J}_\mathrm{trans} \dif S\,\,\,\mathrm{(A)}

Velocity current:

\faz{I}_\mathrm{vel} = \int_S \vecfaz{J}_\mathrm{vel} \dif S\,\,\,\mathrm{(A)}

Total current:

\faz{I}_\mathrm{tot} = \faz{I}_\mathrm{ext} + \faz{I}_\mathrm{trans} + \faz{I}_\mathrm{vel}

Power losses:

P = \int_V \frac{\left( \vecfaz{J}_\mathrm{tot} \cdot \vecfaz{J}_\mathrm{tot}^* \right)}{\sigma} \dif V\,\,\,\mathrm{(W)}

Lorentz force:

F_\mathrm{L} = \int_V \vecfaz{J}_\mathrm{tot} \times \vecfaz{B} \dif V\,\,\,\mathrm{(N)}

Average energy:

W_\mathrm{m} = \int_V \frac{1}{2} \vecfaz{H} \vecfaz{B} \dif V\,\,\,\mathrm{(N)}

Heat Transfer

Heat transfer can be described by partial differential equation

\div \lambda\, \grad T - \rho c_\mathrm{p} \frac{\partial T}{\partial t} = -w,

where \lambda is thermal conductivity, T is temperature, \rho is density, c_\mathrm{p} is specific heat and finally w is source of the inner heat (eddy current, chemical source, ...). Term with partial derivative is in steady-state analysis neglected. Thermal flux can be written as

\vec{F} = \lambda\, \grad T

and temperature gradient is

\vec{G} = \grad T.

Boundary conditions

  • Dirichlet BC

    Temperature T = f on the boundary is known.

  • Neumann BC

    Thermal heat flux q = - \lambda \frac{\partial T}{\partial n} on the boundary is known.

  • Mixed BC

    Thermal heat flux due to convection into the environment q = - \lambda \frac{\partial T}{\partial n} = \alpha \left( T - T_{\mathrm{ext}}\right) on the boundary is known.

Boundary integrals

Average temperature:

T_\mathrm{avg} = \frac{1}{S} \int_S T \dif S\,\,\,\mathrm{(deg.)}

Heat flux:

F = \int_S \lambda \frac{\partial T}{\partial n} \dif S\,\,\,\mathrm{(W)}

Subdomain integrals

Average temperature:

T_\mathrm{avg} = \frac{1}{V} \int_V T \dif V\,\,\,\mathrm{(deg.)}