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Showing 1 to 10 of 10 for “"Gravitational perturbations"”.

  1. Interstellar Gravitational Perturbations of Cometary Orbits

    Made available in DSpace on 2014-12-12T00:17:47Z (GMT). No. of bitstreams: 1 7212154.pdf: 2691518 bytes, checksum: 30ec6fe43239395eef63314798ecafec (MD5) Previous issue date: 1971

    uiuc Repository record for Interstellar Gravitational Perturbations of Cometary Orbits (opens in a new tab)

  2. Modeling and Characterization of Structural, Thermophysical, and Dynamical Evolutions of Small Bodies in the Solar System

    … of asteroids, a key factor giving rise to non-gravitational perturbations on their dynamics. Finally, the work extends to binary asteroid systems, coupling detailed shape models with full two-body gravitational dynamics and thermal torque modeling to quantify the effects of both impact-induced …

    gatech Repository record for Modeling and Characterization of Structural, Thermophysical, and Dynamical Evolutions of Small Bodies in the Solar System (opens in a new tab)

  3. Dust in circumstellar disks

    … the inner disks is most likely the result of the gravitational influence of a large planet and/or a lack of dust-producing minor bodies in the dust-free region. Finally, I describe a numerical model to simulate the dynamical evolution of dust particles in debris disks, taking into account the …

    heid-diss Repository record for Dust in circumstellar disks (opens in a new tab)

  4. The influence of planetary and stellar companions on debris discs

    … (SED) modelling or direct imaging of the dust. Gravitational perturbations in a system containing planets or multiple stars can influence the evolution of a disc and leave observable signatures in the disc’s structure, potentially allowing the inference of companions which are not directly …

    cambridge Repository record for The influence of planetary and stellar companions on debris discs (opens in a new tab)

  5. Leveraging numerical relativity formulations for perturbative analysis: applications to quasinormal modes in general relativity

    … the simulation of compact object mergers, gravitational col-lapse, and other nonlinear phenomena. At the same time, perturbation theory provides a powerful analytical framework for understanding small deviations from equilibrium configurations, offering insights into gravitational wave …

    cape-town Repository record for Leveraging numerical relativity formulations for perturbative analysis: applications to quasinormal modes in general relativity (opens in a new tab)

  6. The Effects of Fractal Molecular Clouds on the Dynamical Evolution of Oort Cloud Comets

    … interesting because it contains a record of the gravitational perturbations suffered by the solar system over its lifetime. Here, we investigate the effects of a particular class of perturbing objects - enormous complexes of molecular gas called giant molecular clouds (GMCs). Recent evidence has …

    queens Repository record for The Effects of Fractal Molecular Clouds on the Dynamical Evolution of Oort Cloud Comets (opens in a new tab)

  7. Solar radiation pressure, drag and gravitational effects on a dust particle in Earth orbit

    … by numerical integration. One of the predominant perturbations on particle orbits is the solar radiation pressure (SRP), which is defined as the pressure exerted by the photons constituting the light from the Sun. Colombo et. al studied the orbital dynamics of ``smart-dust'' under the effects of …

    uiuc Repository record for Solar radiation pressure, drag and gravitational effects on a dust particle in Earth orbit (opens in a new tab)

  8. The imprint of scalar clouds around Kerr black holes: hairy solutions and weak cosmic censorship

    … of gauge allowed us to decouple the scalar field perturbations form the gravitational sector and perform the analysis by looking at the quasinormal mode spectrum of the hairy solutions. When the scalar field is real, these stationary hairy solutions do not exist, but scalar clouds still form …

    cambridge Repository record for The imprint of scalar clouds around Kerr black holes: hairy solutions and weak cosmic censorship (opens in a new tab)

  9. Frequency space analysis in General Relativity

    … and half-integer s, describes the dynamics of perturbations of Kerr black holes in the linearized setting. We begin by showing that the Teukolsky equation is modally stable, i.e. that it admits no exponentially growing or bounded but non-decaying separable solutions. This result is novel for …

    cambridge Repository record for Frequency space analysis in General Relativity (opens in a new tab)

  10. Natural and perturbed dynamics about Trojan bodies

    … is adopted far from the asteroid1, where the gravitational perturbations of the Sun and Jupiter are dominant while the inhomogeneities of the asteroid are negligible. Low-thrust propulsion perturbations are incorporated into this model. The possibility to determine the range of validity of …

    strathclyde Repository record for Natural and perturbed dynamics about Trojan bodies (opens in a new tab)