[docs]
class VlasovMaxwellOneSpecies(StruphyModel):
"""Vlasov-Maxwell equations for one kinetic species.
Parameters
----------
base_units: BaseUnits
Base units for normalization (default: BaseUnits())
charge_number: int
Charge number (in units of the positive elementary charge) of the species (default: 1)
mass_number: float
Mass number (in units of Proton mass) of the species (default: 1.0)
alpha: float, optional
Dimensionless parameter: plasma frequency / cyclotron frequency. If None, computed from units and charge/mass numbers.
epsilon: float, optional
Normalized cyclotron period: 1 / (cyclotron frequency × time unit). If None, computed from units and charge/mass numbers.
measure_gauss_law: bool
Whether to track the Gauss-law error as a scalar quantity (default: False)
"""
@classmethod
def model_type(cls) -> LiteralOptions.ModelTypes:
return "Kinetic"
## species
class EMFields(FieldSpecies):
def __init__(self):
self.e_field = FEECVariable(space="Hcurl")
self.b_field = FEECVariable(space="Hdiv")
self.phi = FEECVariable(space="H1")
self.init_variables()
class KineticIons(ParticleSpecies):
def __init__(
self,
charge_number: int = 1,
mass_number: float = 1.0,
alpha: float = None,
epsilon: float = None,
):
self.var = PICVariable(space="Particles6D")
self.init_variables(
charge_number=charge_number,
mass_number=mass_number,
alpha=alpha,
epsilon=epsilon,
)
## propagators
class Propagators:
def __init__(
self,
b2_var: FEECVariable = None,
):
self.maxwell = MaxwellWeakAmpere()
self.push_eta = PushEta()
self.push_vxb = PushVxB(b2_var=b2_var)
self.coupling_va = VlasovAmpereCoupling()
## abstract methods
def __init__(
self,
base_units: BaseUnits = BaseUnits(),
charge_number: int = 1,
mass_number: float = 1.0,
alpha: float = None,
epsilon: float = None,
measure_gauss_law: bool = False,
):
# 0. store input parameters
self.params = copy.deepcopy(locals())
# 1. instantiate all species
self.em_fields = self.EMFields()
self.kinetic_ions = self.KineticIons(
charge_number,
mass_number,
alpha,
epsilon,
)
# 2. derive units (must be done after instantiating species to access charge and mass numbers)
self.setup_equation_params(base_units=base_units)
# 3. instantiate all propagators
self.propagators = self.Propagators(b2_var=self.em_fields.b_field)
# 4. assign variables to propagators
self.propagators.maxwell.variables.e = self.em_fields.e_field
self.propagators.maxwell.variables.b = self.em_fields.b_field
self.propagators.push_eta.variables.var = self.kinetic_ions.var
self.propagators.push_vxb.variables.ions = self.kinetic_ions.var
self.propagators.coupling_va.variables.e = self.em_fields.e_field
self.propagators.coupling_va.variables.ions = self.kinetic_ions.var
# 5. define scalars to be tracked during simulation
electric_energy = BilinearEnergyFEEC(self.em_fields.e_field)
magnetic_energy = BilinearEnergyFEEC(self.em_fields.b_field)
particle_energy = KineticEnergyPIC(
self.kinetic_ions.var,
normalization=self.kinetic_ions.equation_params.alpha**2,
)
scalars_dict = {
"en_E": electric_energy,
"en_B": magnetic_energy,
"en_f": particle_energy,
"en_tot": electric_energy + magnetic_energy + particle_energy,
}
if measure_gauss_law:
scalars_dict["gauss_error"] = FunctionScalarPIC(self.calculate_gauss_error, self.kinetic_ions.var)
self.scalars = Scalars(**scalars_dict)
# initial Poisson (not a propagator used in time stepping)
alpha = self.kinetic_ions.equation_params.alpha
epsilon = self.kinetic_ions.equation_params.epsilon
particles_to_grid = ParticlesToGrid(
self.kinetic_ions.var,
"H1",
Pyccelkernel(accum_kernels.charge_density_0form),
)
self.initial_poisson = PoissonSolve(
rho=particles_to_grid,
rho_coeffs=alpha**2 / epsilon,
)
self.initial_poisson.variables.phi = self.em_fields.phi
# property to measure violation of gauss law from control variate
self.measure_gauss_law = measure_gauss_law
@property
def bulk_species(self):
return self.kinetic_ions
@property
def velocity_scale(self):
return "light"
def allocate_helpers(self):
"""Solve initial Poisson equation.
:meta private:
"""
self._tmp = xp.empty(1, dtype=float)
particles = self.kinetic_ions.var.particles
if self.measure_gauss_law:
self.op = Propagator.derham.grad.T @ Propagator.mass_ops.M1
self.subcom_residual = xp.empty(shape=particles.mpi_size, dtype=float)
self.intercom_residual = xp.empty(shape=particles.num_clones, dtype=float)
logger.info("\nINITIAL POISSON SOLVE:")
# use control variate method (reset weights after Poisson solve)
particles.update_weights()
self.initial_poisson.allocate()
# keep the AccumulatorVector built by the propagator for the Gauss-law diagnostic below
self.charge_accum = self.initial_poisson.sources[0]
# Solve with dt=1. and compute electric field
logger.info("Solving initial Poisson problem...")
self.initial_poisson(1.0)
phi = self.initial_poisson.variables.phi.spline.vector
Propagator.derham.grad.dot(-phi, out=self.em_fields.e_field.spline.vector)
logger.info("... Done.")
# reset particle weights
particles.weights = particles.weights_at_t0.copy()
def calculate_gauss_error(self):
# control variate method
particles = self.kinetic_ions.var.particles
particles.update_weights()
self.charge_accum()
rhs = self.charge_accum.vectors[0]
# reset particle weights
particles.weights = particles.weights_at_t0.copy()
# non control variate method
e = self.em_fields.e_field.spline.vector
lhs = self.op.dot(e)
# calculate local residual of local MPI rank
loc_residual = xp.max(xp.abs(lhs.toarray() - rhs.toarray()))
# logger.info(f"{MPI.COMM_WORLD.Get_rank() = }, {xp.max(xp.abs(lhs.toarray())) = }")
# logger.info(f"{MPI.COMM_WORLD.Get_rank() = }, {xp.max(xp.abs(rhs.toarray())) = }")
# logger.info(f"{loc_residual = }")
# return the maximum residual across all MPI rank
particles._gather_scalar_in_subcomm_array(scalar=loc_residual, out=self.subcom_residual)
particles._gather_scalar_in_intercomm_array(scalar=loc_residual, out=self.intercom_residual)
return xp.max([xp.max(self.subcom_residual), xp.max(self.intercom_residual)])
## default parameters
def generate_default_parameter_file(self, path=None, prompt=True):
params_path = super().generate_default_parameter_file(path=path, prompt=prompt)
new_file = []
with open(params_path, "r") as f:
for line in f:
if "coupling_va.Options" in line:
new_file += [line]
new_file += ["model.initial_poisson.options = model.initial_poisson.Options()\n"]
elif "saving_params = " in line:
new_file += ["\nbinplot = BinningPlot(slice='e1', n_bins=128, ranges=(0.0, 1.0))\n"]
new_file += ["saving_params = SavingParameters(binning_plots=(binplot,))\n\n"]
elif "VlasovMaxwellOneSpecies()" in line:
new_file += ["\nmodel = VlasovMaxwellOneSpecies(measure_gauss_law=True)\n"]
else:
new_file += [line]
with open(params_path, "w") as f:
for line in new_file:
f.write(line)
[docs]
@classmethod
def doc_pde(cls):
r"""**PDEs solved by model:**
Vlasov equation:
.. math::
\frac{\partial f}{\partial t} + \mathbf{v} \cdot \nabla f + \frac{1}{\varepsilon} \left( \mathbf{E} + \mathbf{v} \times \left( \mathbf{B} + \mathbf{B}_0 \right) \right) \cdot \frac{\partial f}{\partial \mathbf{v}} = 0
Ampère's law:
.. math::
-\frac{\partial \mathbf{E}}{\partial t} + \nabla \times \mathbf{B} = \frac{\alpha^2}{\varepsilon} \int_{\mathbb{R}^3} \mathbf{v} f \, \text{d}^3 \mathbf{v}
Faraday's law:
.. math::
\frac{\partial \mathbf{B}}{\partial t} + \nabla \times \mathbf{E} = 0
where :math:`Z=-1` and :math:`A=1/1836` for electrons.
At initial time the weak Poisson equation is solved once to weakly satisfy Gauss' law,
.. math::
\int_{\Omega} \nabla \psi^{\top} \cdot \nabla \phi \, \textrm{d} \mathbf{x} &= \frac{\alpha^2}{\varepsilon} \int_{\Omega} \int_{\mathbb{R}^3} \psi \, (f - f_0) \, \text{d}^3 \mathbf{v} \, \textrm{d} \mathbf{x} \qquad \forall \ \psi \in H^1
\\[2mm]
\mathbf{E}(t=0) &= -\nabla \phi(t=0)
Moreover, it is assumed that
.. math::
\nabla \times \mathbf{B}_0 = \frac{\alpha^2}{\varepsilon} \int_{\mathbb{R}^3} \mathbf{v} f_0 \, \text{d}^3 \mathbf{v}
where :math:`\mathbf{B}_0` is the static equilibrium magnetic field.
"""
[docs]
@classmethod
def doc_normalization(cls):
r"""The model uses the light speed as reference velocity:
.. math::
\hat v = c,\qquad \hat E = \hat B \hat v,\qquad \hat\phi = \hat E \hat x.
The species parameters are :math:`\alpha=\hat\Omega_p/\hat\Omega_c` and
:math:`\varepsilon=1/(\hat\Omega_c\hat t)`."""
[docs]
@classmethod
def doc_scalar_quantities(cls):
r"""**The following scalars are tracked during simulation:**
- Electric field energy: ``en_E``
- Magnetic field energy: ``en_B``
- Particle kinetic energy: ``en_f``
- Total energy: ``en_tot``
- Optional Gauss-law diagnostic: ``gauss_error``"""
[docs]
@classmethod
def doc_discretization(cls):
"""Time integration is performed by the following propagators (in sequence):
1. :class:`~struphy.propagators.maxwell_weak_ampere.MaxwellWeakAmpere`
2. :class:`~struphy.propagators.push_eta.PushEta`
3. :class:`~struphy.propagators.push_vxb.PushVxB`
4. :class:`~struphy.propagators.vlasov_ampere_coupling.VlasovAmpereCoupling`
"""
doc = rf"""**1. propagators.maxwell.Maxwell:**
{MaxwellWeakAmpere.__doc__}
**2. PushEta:**
{PushEta.__doc__}
**3. PushVxB:**
{PushVxB.__doc__}
**4. VlasovAmpereCoupling:**
{VlasovAmpereCoupling.__doc__}
"""
return doc
[docs]
@classmethod
def doc_long_description(cls):
r"""VlasovMaxwellOneSpecies is the fully electromagnetic one-species PIC
model in Struphy. It evolves particles and fields self-consistently and
supports an optional control-variate formulation for the field coupling."""
[docs]
@classmethod
def doc_examples(cls):
r"""Create and initialize a Vlasov-Maxwell model:
.. code-block:: python
from struphy.models import VlasovMaxwellOneSpecies
model = VlasovMaxwellOneSpecies()
model.em_fields.e_field
model.em_fields.b_field
model.kinetic_ions.var
"""
[docs]
@classmethod
def doc_use_cases(cls):
r"""This model is appropriate for:
- self-consistent electromagnetic kinetic simulations
- one-species PIC benchmarks
- wave-particle interaction studies with evolving magnetic fields
- verification of the full Vlasov-Maxwell splitting"""
[docs]
@classmethod
def doc_cannot_be_used_for(cls):
r"""This model is not suitable for:
- multi-species plasma dynamics without extension
- collisional kinetic closures
- reduced electrostatic-only models where magnetic evolution is unnecessary
- linearized delta-f studies that should use the dedicated linear models"""
