Results 221 to 230 of about 32,266 (262)

Sedimentation of Brownian Particles in a Gravitational Potential

Journal of Statistical Physics, 2002
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The Gravitational Potential

2021
James M. Longuski, Felix R. Hoots, George E. Pollock IV   +2 more
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Temperature and Gravitational Potential

1994
It is argued that thermal equilibrium of spatially extended systems is characterized by the presence of a “global” temperature, but that there also exists a “local” temperature, which is sensitive to the value of the gravitational potential. It is further asserted that thermometers read out the local temperature.
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Electromagnetic and gravitational Hertz potentials

Journal of Mathematical Physics, 1978
With generality of complex relativity, the classical theory of the electromagnetic Hertz potentials is outlined in terms of spinors and forms. Particularly interesting are D (0,1) and D (1,0) null Hertz potentials. Then, a new spinorial approach to heavens (ℋ spaces) is proposed, which reveals in their structure the presence of the left null ...
Jerzy F. Plebański, Ivor Robinson
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Gravitational Potential

2022
Elena Bannikova, Massimo Capaccioli
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Earth Satellites and the Gravitational Potential

Nature Physical Science, 1972
ANALYSIS of the orbit of the artificial Earth satellite Ariel 3 (1967-42A) at the Royal Aircraft Establishment1 has shown that useful determinations of the 15th-order harmonics of the Earth's gravitational potential can be made if the analysis is carried out for the period when the orbit passes through resonance with these harmonics. Several satellites
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Challenges and opportunities of gravitational-wave searches at MHz to GHz frequencies

Living Reviews in Relativity, 2021
O D Aguiar, G Cella, Valerie Domcke
exaly  

Gravitational and electric potential

2022
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Parameter estimation with gravitational waves

Reviews of Modern Physics, 2022
N Christensen, Renate Meyer
exaly  

The Eulerian Perturbation of the Gravitational Potential

2010
Attention is paid to the Eulerian perturbation of the gravitational potential. A solution for it is derived by integration of Poisson’s perturbed second-order differential equation, successively, in terms of the distribution of the Eulerian perturbation of the mass density and the distribution of the components of the Lagrangian displacement throughout
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