Formulation of the Post-Newtonian Equations of Motion of the Restricted Three Body Problem

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Applied Mathematics

ISSN Print: 2152-7385
ISSN Online: 2152-7393
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E-mail: am@scirp.org

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"Formulation of the Post-Newtonian Equations of Motion of the Restricted Three Body Problem"
written by Fawzy A. Abd El-Salam, Sobhy Abd El-Bar,
published by Applied Mathematics, Vol.2 No.2, 2011

has been cited by the following article(s):

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[1]	Photogravitational perturbations in the infinitesimal orbits around the libration points in the oblate RTBP
	2019

[2]	Combined effects of oblateness and photogravitational perturbations on the stability of the equilibrium points in the relativistic RTBP
	Canadian Journal of Physics, 2018

[3]	Periodic and Degenerate Orbits Around the Equilibrium Points in the Relativistic Restricted Three-Body Problem
	Iranian Journal of Science and Technology, Transactions A: Science, 2018

[4]	Perturbed location of [L. sub. 1] point in the photogravitational relativistic restricted three-body problem (R3BP) with oblate primaries
	Canadian Journal of Physics, 2015

[5]	On the equilibrium point L1 in the photogravitational oblate relativistic R3BP with application on Sun-planet systems
	The European Physical Journal Plus, 2015

[6]	On the equilibrium point L 1 in the photogravitational oblate relativistic R3BP with application on Sun-planet systems
	2015

[7]	Effect of Perturbations in the Coriolis and Centrifugal Forces on the Stability of L 4 in the Relativistic R3BP
	Journal of Astrophysics and Astronomy, 2014

[8]	Perturbed Location of L 1 point in the photogravitational Relativistic R3BP with Oblate Primaries
	Canadian Journal of Physics?ja, 2014

[9]	Relativistic Restricted Three Body Problem with Photo-gravitational Corrections to Triangular Equilibrium Points
	FAA El-Salam, SEA El-Bar, 2014

[10]	Effect of radiation pressure on the stability of L 4, 5 in the relativistic R3BP
	Astrophysics and Space Science, 2014

[11]	Relativistic restricted three body problem with oblatness and photo-gravitational corrections to triangular equilibrium points
	Astrophysics and Space Science, 2014

[12]	On the triangular equilibrium points in the photogravitational relativistic restricted three body problem
	Astrophysics and Space Science, 2014

[13]	Effect of radiation pressure on the stability of L 4,5 in the relativistic R3BP
	Astrophysics and Space Science, 2014

[14]	Determination of L3 Location in the Photogravitational Oblate Relativistic R3BP with Application on Sun-Planet Systems
	2014

[15]	Perturbed Location of L1 point in the photogravitational relativistic restricted three-body problem (R3BP) with oblate primaries
	2014

[16]	Determination of the Perturbed Locations of the Triangular Equilibrium Points in the Photo-Gravitational Relativistic Restricted Three Body Problem
	2013

[17]	Analytical and Semianalytical Treatment of the Collinear Points in the Photogravitational Relativistic RTBP
	Mathematical Problems in Engineering, 2013

[18]	Photo-Gravitational Effects in the Locations of the Collinear Points in the Relativistic Restricted Three Body Problem
	SEA El-Bar, M Radwan, FAA El-Salam - European Journal of Scientific Research, 2012

[19]	Study and Analysis of the Orbital and Physical Properties of 2010 TK 7
	Journal of Modern Physics, 2011

[20]	Study and Analysis of the Orbital and Physical Properties of 2010 TK7
	2011

[1]	Equilibrium Points and Networks of Periodic Orbits in the Pseudo-Newtonian Planar Circular Restricted Three-body Problem The Astronomical Journal, 2022 DOI:10.3847/1538-3881/ac31af

[2]	Equilibrium Points and Networks of Periodic Orbits in the Pseudo-Newtonian Planar Circular Restricted Three-body Problem The Astronomical Journal, 2022 DOI:10.3847/1538-3881/ac31af

[3]	Periodic and Degenerate Orbits Around the Equilibrium Points in the Relativistic Restricted Three-Body Problem Iranian Journal of Science and Technology, Transactions A: Science, 2018 DOI:10.1007/s40995-017-0394-7

[4]	Combined effects of oblateness and photogravitational perturbations on the stability of the equilibrium points in the relativistic RTBP Canadian Journal of Physics, 2018 DOI:10.1139/cjp-2018-0187

[5]	On the equilibrium point L1 in the photogravitational oblate relativistic R3BP with application on Sun-planet systems The European Physical Journal Plus, 2015 DOI:10.1140/epjp/i2015-15054-0

[6]	Perturbed Location ofL1point in the photogravitational relativistic restricted three-body problem (R3BP) with oblate primaries Canadian Journal of Physics, 2015 DOI:10.1139/cjp-2014-0346

[7]	Effect of Perturbations in the Coriolis and Centrifugal Forces on the Stability of L 4 in the Relativistic R3BP Journal of Astrophysics and Astronomy, 2014 DOI:10.1007/s12036-014-9307-8

[8]	Effect of radiation pressure on the stability of L 4,5 in the relativistic R3BP Astrophysics and Space Science, 2014 DOI:10.1007/s10509-014-1858-2

[9]	Relativistic restricted three body problem with oblatness and photo-gravitational corrections to triangular equilibrium points Astrophysics and Space Science, 2014 DOI:10.1007/s10509-014-1826-x

[10]	On the triangular equilibrium points in the photogravitational relativistic restricted three body problem Astrophysics and Space Science, 2014 DOI:10.1007/s10509-013-1629-5

[11]	Analytical and Semianalytical Treatment of the Collinear Points in the Photogravitational Relativistic RTBP Mathematical Problems in Engineering, 2013 DOI:10.1155/2013/794734

[12]	Study and Analysis of the Orbital and Physical Properties of 2010 TK₇ Journal of Modern Physics, 2011 DOI:10.4236/jmp.2011.211167

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