The Physics of Einstein: Black Holes, Time Travel, Distant Starlight, E=mc^2 by Jason Lisle

The Physics of Einstein: Black Holes, Time Travel, Distant Starlight, E=mc^2 by Jason Lisle

Author:Jason Lisle [Lisle, Jason]
Language: eng
Format: epub, mobi
Publisher: Biblical Science Institute
Published: 2018-12-01T16:00:00+00:00


Here, the total energy has been divided into two components. The first component (m0c2) does not change with velocity. So it must be the potential energy of the object. We can also call this the “rest energy” of the object, which naturally corresponds to its rest mass. The second component ((γ-1)m0c2) does depend on velocity, and goes to zero when velocity is zero. Therefore, it must be the kinetic energy (K).

The total energy can then be written as the sum of the potential energy plus kinetic energy:



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