Galaxy Rotation Curves in Covariant Horava-Lifshitz Gravity
classification
✦ hep-th
gr-qchep-ph
keywords
covariantgravityhorava-lifshitzcurvesdescriptiongalaxyrotationsolutions
pith:VMO5KUVT Add to your LaTeX paper
What is a Pith Number?\usepackage{pith}
\pithnumber{VMO5KUVT}
Prints a linked pith:VMO5KUVT badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more
read the original abstract
Using the multiplicity of solutions for the projectable case of the covariant extension of Horava-Lifshitz Gravity, we show that an appropriate choice for the auxiliary field allows for an effective description of galaxy rotation curves. This description is based on static and spherically symmetric solutions of covariant Horava-Lifshitz Gravity and does not require Dark Matter.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.