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NEWTONIAN AND NON-NEWTONIAN LIMITS OF THE STATIONARY GRAVITATIONAL FIELDS
Proceedings of the Academy of Sciences of the Estonian SSR. Physics. Mathematics, 1975 openaire +1 more source
A computational model for retinal haemodynamics under gravitational and postural variations. [PDF]
J PhysiolNigro M, Montanino A, Soudah E.
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One-Dimensional Relativistic Self-Gravitating Systems. [PDF]
Entropy (Basel)Mann RB.
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Exploring irradiated granular flows with rapid heating for concentrated solar thermal energy collection and storage. [PDF]
iScienceJeong SY +3 more
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Isotropic fluid structures and role of non-metricity on their dynamics governed by an electric charge: A theoretical study. [PDF]
PLoS OneNaseer T +4 more
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Propagation of Newtonian gravitation derived by the elastic energy
Physics Essays, 2022The Earth is compressed by its own Newtonian gravitation. The pressure is generated inside the Earth for this compression. The pressure distribution is expressed using the Adams‐Williamson equation (AWE).
Noboru Kohiyama
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Newtonian gravitation derived by the elastic energy in the Earth’s interior
Physics Essays, 2022The pressure distribution in the Earth’s interior is expressed using the Adams‐Williamson equation. The elastic energy is stored inside the Earth by the pressure. The Newtonian gravitation is expressed by this energy.
Noboru Kohiyama
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The Physical and Mathematical Foundations of the Theory of Relativity, 2019
Antonio Romano, Mario Mango Furnari
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Antonio Romano, Mario Mango Furnari
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, 2016
Einstein’s field equations relate space-time geometry to matter and energy distribution. These tensorial equations are so unwieldy that solutions are only known in some very specific cases. A semi-relativistic approximation is desirable: One where space-time may still be considered as flat, but where Newton’s equations (where gravity acts ...
Erik I. Verriest
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Einstein’s field equations relate space-time geometry to matter and energy distribution. These tensorial equations are so unwieldy that solutions are only known in some very specific cases. A semi-relativistic approximation is desirable: One where space-time may still be considered as flat, but where Newton’s equations (where gravity acts ...
Erik I. Verriest
semanticscholar +2 more sources
Discrete Newtonian gravitation and the three-body problem
Foundations of Physics, 1974D. Greenspan
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