Timelike bound orbits in JMN-1 naked singularity spacetimes can precess opposite to the direction of particle motion when 0<M0<1/3, unlike Schwarzschild orbits, with precession factor m=sqrt(2-3M0).
Con- sequently, the nature of the orbits also changes across M0 = 1
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
gr-qc 1years
2019 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Timelike geodesics in Naked Singularity and Black Hole Spacetimes
Timelike bound orbits in JMN-1 naked singularity spacetimes can precess opposite to the direction of particle motion when 0<M0<1/3, unlike Schwarzschild orbits, with precession factor m=sqrt(2-3M0).