Test particle motion in the cyclotron resonance regime

1991 ◽  
Vol 3 (11) ◽  
pp. 2994-3012 ◽  
Author(s):  
Gregory P. Ginet ◽  
Jay M. Albert
Keyword(s):  
Test Particle ◽  
Particle Motion ◽  
Cyclotron Resonance ◽  
Resonance Regime

scholarly journals Planetary perturbation equations based on relativistic Keplerian motion

1986 ◽  
Vol 114 ◽  
pp. 41-52
Author(s):  
Neil Ashby
Keyword(s):  
Test Particle ◽  
Particle Motion ◽  
Elliptic Functions ◽  
Orbital Elements ◽  
Keplerian Motion ◽  
Jacobian Elliptic Functions ◽  
Planetary Perturbation ◽  
Geodesic Equations ◽  
Bound Test ◽  
Perturbation Equations

Solutions of the geodesic equations for bound test particle motion in a Schwarzschild field are expressed using Jacobian elliptic functions. Keplerian orbital elements are identified and related to a set of canonical constants. Relativistic Lagrange planetary perturbation equations are derived.

scholarly journals Effect of radiation flux on test-particle motion in the Vaidya spacetime

2011 ◽  
Vol 28 (24) ◽  
pp. 245019 ◽  
Author(s):  
Donato Bini ◽  
Andrea Geralico ◽  
Robert T Jantzen ◽  
Oldřich Semerák
Keyword(s):  
Test Particle ◽  
Particle Motion ◽  
Radiation Flux

scholarly journals Test particle motion in a gravitational plane wave collision background

2003 ◽  
Vol 20 (2) ◽  
pp. 341-350 ◽  
Author(s):  
Donato Bini ◽  
Gianluca Cruciani ◽  
Andrea Lunari
Keyword(s):  
Plane Wave ◽  
Test Particle ◽  
Particle Motion ◽  
Wave Collision

Test Particle Motion around an Oblate Planet

Icarus ◽  
1994 ◽  
Vol 107 (1) ◽  
pp. 129-141 ◽  
Author(s):  
Nicole Borderies-Rappaport ◽  
Pierre-Yves Longaretti
Keyword(s):  
Test Particle ◽  
Particle Motion ◽  
Oblate Planet

scholarly journals Trajectory around a spherically symmetric non-rotating black hole

2011 ◽  
Vol 89 (6) ◽  
pp. 689-695 ◽  
Author(s):  
Sumanta Chakraborty ◽  
Subenoy Chakraborty
Keyword(s):  
Black Hole ◽  
Gravitational Field ◽  
Gravitational Potential ◽  
Test Particle ◽  
Effective Potential ◽  
Particle Motion ◽  
Spherically Symmetric ◽  
Rotating Black Hole

The trajectory of a test particle or a photon around a general spherical black hole is studied, and bending of the light trajectory is investigated. A pseudo-Newtonian gravitational potential describing the gravitational field of the black hole is determined and is compared with the related effective potential for test particle motion. As an example, results are presented for a Reissner–Nordström black hole.

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