The Restless Universe Applications of Gravitational N-Body Dynamics to Planetary Stellar and Galactic Systems
The Restless Universe: Applications of Gravitational N-Body Dynamics to Planetary Stellar and Galactic Systems stimulates the cross-fertilization of ideas, methods, and applications among the different communities who work in the gravitational N-body problem arena, across diverse fields of astrophysics. The chapters and topics cover three broad the
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Aarseth algorithm Ap.J approximation asteroid belt asteroids Astron axis behaviour binary body problem celestial central configuration chaotic choreographies cluster codes coefficients collision collisionless component computed consider coordinates corresponding cosmological curves dark matter defined density differential equations disk distance distribution dynamics eccentricity elliptical energy equations of motion escape eulerian evolution example Farinella Figure fluid Fourier frequencies Froeschlé function galactic galaxy gravitational grid halo Hamiltonian system Henri Poincaré initial conditions instability integral iterative linear Lyapunov Lyapunov exponents mass method MNRAS N-body simulations numerical observed obtained orbits parameters particles peculiar velocity perturbation phase space physical planetesimal planets Poincaré points Poisson equation polynomial potential radial redshift surveys region resonance scale Section secular resonances semimajor semimajor axis solar system solution stable stars stellar structure surface techniques theorem theory torus Trojan Trojan asteroids variables variational equations vector Vokrouhlicky Yarkovsky effect