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Energies and angular momenta of periodic Schwarzschild geodesics

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arxiv 2401.13894 v1 pith:46B5RYQZ submitted 2024-01-25 gr-qc hep-th

classification gr-qchep-th
keywords periodicorbitorbitscircularlimitnumberwhirlaccording
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abstract

We consider physical parameters of Levin and Perez-Giz's `periodic table of orbits' around the Schwarzschild black hole, where each periodic orbit is classified according to three integers $(z,w,v)$. In particular, we chart its distribution in terms of its angular momenta $L$ and energy $E$. In the $(L,E)$-parameter space, the set of all periodic orbits can be partitioned into domains according to their whirl number $w$, where the limit of infinite $w$ approaches the branch of unstable circular orbits. Within each domain of a given whirl number $w$, the infinite zoom limit $\lim_{z\rightarrow\infty}(z,w,v)$ converges to the common boundary with the adjacent domain of whirl number $w-1$. The distribution of the periodic orbit branches can also be inferred from perturbing stable circular orbits, using the fact that every stable circular orbit is the zero-eccentricity limit of some periodic orbit, or arbitrarily close to one.

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Cited by 2 Pith papers

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  1. Periodic orbits of neutral test particles in Reissner-Nordstr\"{o}m naked singularities

    gr-qc 2025-02 conditional novelty 6.0 of 10

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  2. Rational Orbits and Gravitational Waves in Static Spherical Spacetimes: An Open-Source Numerical Framework

    gr-qc 2026-06 conditional novelty 5.0 of 10

    Open-source numerical package for rational orbits and gravitational waves in static spherically symmetric spacetimes, validated on Schwarzschild and applied to an IMBH-Sgr A* EMRI.

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