We apply kinetic field theory to non-linear cosmic structure formation. Kinetic decomposes the density into particles and follows their trajectories through phase space. assume that initial particle momenta are drawn from a Gaussian random field. place particular emphasis on late-time, asymptotic behaviour small spatial scales of low-order statistical measures for distribution in configuration ...

We study the spherical droplet problem in 3D Landau–de Gennes theory with finite temperature. By rigorously constructing biaxial–ring solutions and split–core–segment solutions, we theoretically confirm numerical results of Gartland–Mkaddem [15]. The structures disclinations are also addressed.