Generating Moving Field Initial Conditions with Spatially Varying Boost

Generating Moving Field Initial Conditions with Spatially Varying Boost
Siyang Ling
arXiv:2506.23020v1 Announce Type: cross
Abstract: We introduce a novel class of algorithms, the “spatially varying boost”, for generating dynamical field initial conditions with prescribed bulk velocities. Given (non-moving) initial field data, the algorithm generates new initial data with the given velocity profile by performing local Lorentz boosts. This algorithm is generic, with no restriction on the type of the field, the equation of motion, and can endow fields with ultra-relativistic velocities. This algorithm enables new simulations in different branches of physics, including cosmology and condensed matter physics. For demonstration, we used this algorithm to (1) boost two Sine-Gordon solitons to ultra-relativistic speeds for subsequent collision, (2) generate a relativistic transverse Proca field with random velocities, and (3) set up a spin-$1$ Schr”{o}dinger-Poisson field with velocity and density perturbations consistent with dark matter in matter dominated universe.arXiv:2506.23020v1 Announce Type: cross
Abstract: We introduce a novel class of algorithms, the “spatially varying boost”, for generating dynamical field initial conditions with prescribed bulk velocities. Given (non-moving) initial field data, the algorithm generates new initial data with the given velocity profile by performing local Lorentz boosts. This algorithm is generic, with no restriction on the type of the field, the equation of motion, and can endow fields with ultra-relativistic velocities. This algorithm enables new simulations in different branches of physics, including cosmology and condensed matter physics. For demonstration, we used this algorithm to (1) boost two Sine-Gordon solitons to ultra-relativistic speeds for subsequent collision, (2) generate a relativistic transverse Proca field with random velocities, and (3) set up a spin-$1$ Schr”{o}dinger-Poisson field with velocity and density perturbations consistent with dark matter in matter dominated universe.