has been cited by the following article(s):
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[1]
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A numerical method for computing optimum radii of host stars and orbits of planets, with application to Kepler-11, Kepler-90, Kepler-215, HD 10180, HD 34445 and …
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International Journal of Modern Physics C,
2021 |
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[2]
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A numerical method for computing optimum radii of host stars and orbits of planets, with application to Kepler-11, Kepler-90, Kepler-215, HD 10180, HD 34445, and …
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2020 |
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[3]
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Gravitational quantization of exoplanet orbits: The system TRAPPIST-1
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2017 |
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[4]
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Gravitational quantization of exoplanet orbits in HD 10180, Kepler-32, Kepler-33, Kepler-102, and Kepler-186
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arXiv preprint arXiv:1506.06344,
2015 |
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[5]
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Numerical results of the Global Polytropic Model for the orbits of 15 planetary systems
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2015 |
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[6]
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Numerical results of the Global Polytropic Model for the exoplanet orbits of 15 systems
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2015 |
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[7]
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Gravitational quantization of exoplanet orbits in HD 40307, $\ mu $ Ara, Kepler-26, Kepler-62, and Kepler-275: Comparing predicted orbits
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arXiv preprint arXiv:1501.04189,
2015 |
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[8]
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Gravitational quantization of exoplanet orbits in HD 40307, Ara, Kepler-26, Kepler-62, and Kepler-275: Comparing predicted orbits
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2015 |
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[9]
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Gravitational quantization of exoplanet orbits in 55 Cnc, $\ upsilon $ And, Kepler-11, Kepler-20, and Kepler-90
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arXiv preprint arXiv:1411.5390,
2014 |
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[10]
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Gravitational quantization of satellite orbits in the giant planets
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arXiv preprint arXiv:1410.5844,
2014 |
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[11]
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Gravitational quantization of exoplanet orbits in 55 Cnc, And, Kepler-11, Kepler-20, and Kepler-90
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2014 |
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[1]
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A numerical method for computing optimum radii of host stars and orbits of planets, with application to Kepler-11, Kepler-90, Kepler-215, HD 10180, HD 34445 and TRAPPIST-1
International Journal of Modern Physics C,
2021
DOI:10.1142/S0129183121500285
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