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The methodology used in Timelapse of the Entire Universe.. In 2012, a short, one-and-a-half-minute film by Boswell, Our Story in 1 Minute, is published.It is a shorter version of Timelapse of the Entire Universe, specifically in one minute and 29 seconds, and used closed captions to evoke reflection on humanity.
The soundtrack's first track, "Sun Mother," uses a 120 beats per minute rhythm, increasing as the time evolves to "highlight the accelerating rate of [the time-lapse]." The music's timing is also taken into consideration, saying that "It was important to me to have moments where the music, visuals, and sound effects could breathe, and the ...
This is the point at which it has been hypothesized that the known laws of gravity cease to be valid. [11] There are competing theories as to what occurs at this point. For example loop quantum gravity predicts that a Planck star would form. Regardless, it is argued that gravitational collapse ceases at that stage and a singularity, therefore ...
Regions of higher density collapsed more rapidly under gravity, eventually resulting in the large-scale, foam-like structure or "cosmic web" of voids and galaxy filaments seen today. Voids located in high-density environments are smaller than voids situated in low-density spaces of the universe. [3]
where is the lapse function encoding the proper time evolution, is the shift vector, encoding how spatial coordinates change between hypersurfaces. g i j {\displaystyle g_{ij}} is the emergent 3D spatial metric on each hypersurface.
Gravitational time dilation is a form of time dilation, an actual difference of elapsed time between two events, as measured by observers situated at varying distances from a gravitating mass. The lower the gravitational potential (the closer the clock is to the source of gravitation), the slower time passes, speeding up as the gravitational ...
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The gravity g′ at depth d is given by g′ = g(1 − d/R) where g is acceleration due to gravity on the surface of the Earth, d is depth and R is the radius of the Earth. If the density decreased linearly with increasing radius from a density ρ 0 at the center to ρ 1 at the surface, then ρ ( r ) = ρ 0 − ( ρ 0 − ρ 1 ) r / R , and the ...