Journal of Applied Mathematics and Physics

Volume 12, Issue 4 (April 2024)

ISSN Print: 2327-4352   ISSN Online: 2327-4379

Google-based Impact Factor: 0.70  Citations  

Black Hole Singularities and Planetary Formation

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DOI: 10.4236/jamp.2024.124067    34 Downloads   200 Views  
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ABSTRACT

The goal of this research is to explore the effects of black hole singularities. Methodology is to start with large objects like galaxies and continue to smaller objects within our solar neighbourhood. High-redshift observations from the James Webb Space Telescope reveal that distant galaxies and their central black holes formed shortly after the Big Bang. An innovation about the speed of light explains how supermassive black holes could have formed primordially. Predictions of Hawking radiation include the possibility of black holes contributing to the energy of stars such as the Sun. Black holes have also been suggested as a source of radiation and magnetic fields in giant planets. Observations of Enceladus raise the possibility that this moon and other objects near Saturn’s Rings contain small singularities. Extrapolations of this methodology indicate that black holes could exist within solar system bodies including planets. Extended discussion describes how their presence could explain mysteries of internal heat, planetary magnetic fields, and processes of solar system formation.

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Riofrio, L. (2024) Black Hole Singularities and Planetary Formation. Journal of Applied Mathematics and Physics, 12, 1079-1088. doi: 10.4236/jamp.2024.124067.

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