Abstract

We consider radial solutions to the Schrodinger--Poisson system in three dimensions with an external smooth potential with Coulomb-like decay. Such a system can be viewed as a model for the interaction of dark matter with a bright matter background in the nonrelativistic limit. We find that there are infinitely many critical points of the Hamiltonian, subject to fixed mass, and that these bifurcate from solutions to the associated linear problem at zero mass. As a result, each branch has a different topological character defined by the number of zeros of the radial states. We construct numerical approximations to these nonlinear states along the first several branches. The solution branches can be continued, numerically, to large mass values, where they become asymptotic, under a rescaling, to those of the Schrodinger--Poisson problem with no external potential. Our numerical computations indicate that the ground state is orbitally stable, while the excited states are linearly unstable for sufficiently la...

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.