This is a project which is currently making use of HPC facilities at Newcastle University. It is active.
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Numerical modelling the hypothesis dark matter candidate with ultralight mass, featuring quantum wavy features. We attempt to update the model with the state of the art numerical methods, such as considering the role of self coupling and temperatures.
The numerical scripts will be developed in MATLAB, JULIA and Python, using existed or in-house packages. We will consider RK4 and time-splitting methods for the time propagation and use FFT packages to solve the kinetic and gravitational potential of the FDM model