# Kinetic-fluid Hybrid Model

Many problems in plasma physics fall in a class where both electron kinetics and electromagnetic waves do not play a critical role in the solution. Examples of such situations include the study of collisionless magnetic reconnection and instabilities driven by ion temperature anisotropy, to mention only two. For these kinds of problems the computational cost of resolving the electron dynamics can be avoided by modeling the electrons as a neutralizing fluid rather than kinetic particles. By further using Ohm’s law to compute the electric field rather than evolving it with the Maxwell-Faraday equation, light waves can be stepped over. The simulation resolution can then be set by the ion time and length scales (commonly the ion cyclotron period \(1/\Omega_i\) and ion skin depth \(l_i\), respectively), which can reduce the total simulation time drastically compared to a simulation that has to resolve the electron Debye length and CFL-condition based on the speed of light.

Many authors have described variations of the kinetic ion & fluid electron model,
generally referred to as particle-fluid hybrid or just hybrid-PIC models. The implementation
in WarpX follows the outline from Winske *et al.* [1].
This description follows mostly from that reference.

## Model

The basic justification for the hybrid model is that the system to which it is applied is dominated by ion kinetics, with ions moving much slower than electrons and photons. In this scenario two critical approximations can be made, namely, neutrality (\(n_e=n_i\)) and the Maxwell-Ampere equation can be simplified by neglecting the displacement current term [2], giving,

\[\mu_0\vec{J} = \vec{\nabla}\times\vec{B},\]

where \(\vec{J} = \sum_{s\neq e}\vec{J}_s + \vec{J}_e + \vec{J}_{ext}\) is the total electrical current, i.e. the sum of electron and ion currents as well as any external current (not captured through plasma particles). Since ions are treated in the regular PIC manner, the ion current, \(\sum_{s\neq e}\vec{J}_s\), is known during a simulation. Therefore, given the magnetic field, the electron current can be calculated.

The electron momentum transport equation (obtained from multiplying the Vlasov equation by mass and integrating over velocity), also called the generalized Ohm’s law, is given by:

\[en_e\vec{E} = \frac{m}{e}\frac{\partial \vec{J}_e}{\partial t} + \frac{m}{e^2}\left( \vec{U}_e\cdot\nabla \right) \vec{J}_e - \nabla\cdot {\overleftrightarrow P}_e - \vec{J}_e\times\vec{B}+\vec{R}_e\]

where \(\vec{U}_e = \vec{J}_e/(en_e)\) is the electron fluid velocity, \({\overleftrightarrow P}_e\) is the electron pressure tensor and \(\vec{R}_e\) is the drag force due to collisions between electrons and ions. Applying the above momentum equation to the Maxwell-Faraday equation (\(\frac{\partial\vec{B}}{\partial t} = -\nabla\times\vec{E}\)) and substituting in \(\vec{J}\) calculated from the Maxwell-Ampere equation, gives,

\[\frac{\partial\vec{J}_e}{\partial t} = -\frac{1}{\mu_0}\nabla\times\left(\nabla\times\vec{E}\right) - \frac{\partial\vec{J}_{ext}}{\partial t} - \sum_{s\neq e}\frac{\partial\vec{J}_s}{\partial t}.\]

Plugging this back into the generalized Ohm’ law gives:

\[\begin{split}\left(en_e +\frac{m}{e\mu_0}\nabla\times\nabla\times\right)\vec{E} =& - \frac{m}{e}\left( \frac{\partial\vec{J}_{ext}}{\partial t} + \sum_{s\neq e}\frac{\partial\vec{J}_s}{\partial t} \right) \\ &+ \frac{m}{e^2}\left( \vec{U}_e\cdot\nabla \right) \vec{J}_e - \nabla\cdot {\overleftrightarrow P}_e - \vec{J}_e\times\vec{B}+\vec{R}_e.\end{split}\]

If we now further assume electrons are inertialess (i.e. \(m=0\)), the above equation simplifies to,

\[en_e\vec{E} = -\vec{J}_e\times\vec{B}-\nabla\cdot{\overleftrightarrow P}_e+\vec{R}_e.\]

Making the further simplifying assumptions that the electron pressure is isotropic and that the electron drag term can be written as a simple resistance i.e. \(\vec{R}_e = en_e\vec{\eta}\cdot\vec{J}\), brings us to the implemented form of Ohm’s law:

\[\vec{E} = -\frac{1}{en_e}\left( \vec{J}_e\times\vec{B} + \nabla P_e \right)+\vec{\eta}\cdot\vec{J}.\]

Lastly, if an electron temperature is given from which the electron pressure can be calculated, the model is fully constrained and can be evolved given initial conditions.

## Implementation details

Note

Various verification tests of the hybrid model implementation can be found in the examples section.

The kinetic-fluid hybrid extension mostly uses the same routines as the standard electromagnetic
PIC algorithm with the only exception that the E-field is calculated from the
above equation rather than it being updated from the full Maxwell-Ampere equation. The
function `WarpX::HybridPICEvolveFields()`

handles the logic to update the E&M fields
when the “hybridPIC” model is used. This function is executed after particle pushing
and deposition (charge and current density) has been completed. Therefore, based
on the usual time-staggering in the PIC algorithm, when `HybridPICEvolveFields()`

is called
at timestep \(t=t_n\), the quantities \(\rho^n\), \(\rho^{n+1}\), \(\vec{J}_i^{n-1/2}\)
and \(\vec{J}_i^{n+1/2}\) are all known.

### Field update

The field update is done in three steps as described below.

#### First half step

Firstly the E-field at \(t=t_n\) is calculated for which the current density needs to
be interpolated to the correct time, using \(\vec{J}_i^n = 1/2(\vec{J}_i^{n-1/2}+ \vec{J}_i^{n+1/2})\).
The electron pressure is simply calculated using \(\rho^n\) and the B-field is also already
known at the correct time since it was calculated for \(t=t_n\) at the end of the last step.
Once \(\vec{E}^n\) is calculated, it is used to push \(\vec{B}^n\) forward in time
(using the Maxwell-Faraday equation, i.e. the same as in the regular PIC routine with `WarpX::EvolveB()`

)
to \(\vec{B}^{n+1/2}\).

#### Second half step

Next, the E-field is recalculated to get \(\vec{E}^{n+1/2}\). This is done using the known fields \(\vec{B}^{n+1/2}\), \(\vec{J}_i^{n+1/2}\) and interpolated charge density \(\rho^{n+1/2}=1/2(\rho^n+\rho^{n+1})\) (which is also used to calculate the electron pressure). Similarly as before, the B-field is then pushed forward to get \(\vec{B}^{n+1}\) using the newly calculated \(\vec{E}^{n+1/2}\) field.

#### Extrapolation step

Obtaining the E-field at timestep \(t=t_{n+1}\) is a well documented issue for the hybrid model. Currently the approach in WarpX is to simply extrapolate \(\vec{J}_i\) foward in time, using

\[\vec{J}_i^{n+1} = \frac{3}{2}\vec{J}_i^{n+1/2} - \frac{1}{2}\vec{J}_i^{n-1/2}.\]

With this extrapolation all fields required to calculate \(\vec{E}^{n+1}\) are known and the simulation can proceed.

### Sub-stepping

It is also well known that hybrid PIC routines require the B-field to be updated with a smaller timestep than needed for the particles. The update steps as outlined above are therefore wrapped in loops that enable the B-field to be sub-stepped. The exact number of sub-steps used can be specified by the user through a runtime simulation parameter (see input parameters section).

### Electron pressure

The electron pressure is assumed to be a scalar quantity and calculated using the given input parameters, \(T_{e0}\), \(n_0\) and \(\gamma\) using

\[P_e = n_0T_{e0}\left( \frac{n_e}{n_0} \right)^\gamma.\]

The isothermal limit is given by \(\gamma = 1\) while \(\gamma = 5/3\) (default) produces the adiabatic limit.

D. Winske, Homa Karimabadi, Ari Le, N. Omidi, Vadim Roytershteyn, and Adam Stanier. Hybrid codes (massless electron fluid). 2022. arXiv:2204.01676.

CLAIR W. NIELSON and H. RALPH LEWIS. Particle-code models in the nonradiative limit. In JOHN KILLEEN, editor, *Controlled Fusion*, volume 16 of Methods in Computational Physics: Advances in Research and Applications, pages 367–388. Elsevier, 1976. doi:https://doi.org/10.1016/B978-0-12-460816-0.50015-4.