Abstract
We investigate the static and spherically symmetric solutions of Einstein’s equationsfor a scalar field with a non-canonical kinetic term, assumed to provide boththe dark matter and dark energy components of the Universe. In particular,we give a prescription to obtain solutions (dark halos) whose rotation curvevc(r) is in good agreement with observational data. We show that there exist suitable scalar fieldLagrangians that allow us to describe the cosmological background evolution and the staticsolutions with a single dark fluid.
Sign-in/Register to access full text options 
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 callDisclaimer: 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.
