Halo Spacetime
classification
🌌 astro-ph
gr-qc
keywords
theorynewtonianasymptoticallyconstantcurvesdensityeinsteinfluid
read the original abstract
It is shown that constant galactic rotation curves require a logarithmic potential in both newtonian and relativistic theory. In newtonian theory the density vanishes asymptotically, but there are a variety of possibilities for perfect fluid einstein theory.
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