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Static Orbits in Rotating Spacetimes.

Lucas G Collodel1, Burkhard Kleihaus1, Jutta Kunz1

  • 1Institut für Physik, Universität Oldenburg, Postfach 2503, D-26111 Oldenburg, Germany.

Physical Review Letters
|June 5, 2018
PubMed
Summary
This summary is machine-generated.

Researchers found static orbits in rotating spacetimes where particles remain at rest. These stable orbits exist in the equatorial plane for various exotic objects like boson stars and wormholes.

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Area of Science:

  • Theoretical Physics
  • General Relativity
  • Astrophysics

Background:

  • Axisymmetric rotating spacetimes are solutions to Einstein's field equations.
  • Understanding particle orbits in these spacetimes is crucial for testing theories of gravity.

Purpose of the Study:

  • To identify conditions for static particle orbits in the equatorial plane of rotating spacetimes.
  • To explore the occurrence of such orbits in specific astrophysical objects.

Main Methods:

  • Analytical investigation of spacetime geometry.
  • Examination of particle motion equations in curved spacetime.

Main Results:

  • Demonstrated the existence of a ring of static orbits in the equatorial plane under specific conditions.
  • Illustrated these orbits for boson stars, wormholes, hairy black holes, and Kerr-Newman solutions.

Conclusions:

  • Static orbits can exist in rotating spacetimes, challenging previous assumptions.
  • These findings have implications for the study of compact objects and gravitational physics.