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Vor 2 Tagen · Timelike geodesic incompleteness has the physical interpretation that there exists observers at rest who, after a finite proper time, reach the “end” of spacetime. Similarly, bounded acceleration incompleteness has the same interpretation for observers that may be accelerated. Null geodesic incompleteness is more difficult to interpret, given that the affine parameter of a null geodesic ...
Vor 3 Tagen · Proper reference frames for timelike helices. In case all three Frenet–Serret curvatures are constant, the corresponding worldlines are identical to those that follow from the Killing motions in flat spacetime.
Vor 4 Tagen · 1962 – Hermann Bondi, M. G. van der Burg, A. W. Metzner, and Rainer K. Sachs introduce the asymptotic symmetry group of asymptotically flat, Lorentzian spacetimes at null (i.e., light-like) infinity. 1963 – Roy Kerr discovers the Kerr vacuum solution of Einstein's field equations,
Exploring the possibilities humanity can achieve, creating closed timelike curves presents an intriguing opportunity. By performing quantum computing inside a closed timelike curve, a calculation can be completed at the moment it begins. Looping this process to infinity provides the calculative potential to create the most powerful AGI.
Vor 2 Tagen · The Absolute Infinite ( symbol: Ω) is an extension of the ultimate idea of infinity that is bigger than any other conceivable or inconceivable quantity, either finite or transfinite. The Absolute Infinite can be viewed generally as a maximal concept that transcends and encompasses all infinities.
Vor 4 Tagen · Infinity is used to describe quantities which go on forever without end. Common visualizations of infinity include. the length of a line (or ray) that extends forever; the amount of time it would take one to constantly travel along a circle; the number of digits in an irrational number, most notably. \pi π;
Vor 22 Stunden · Around the time of alignment, extreme gravitational lensing of the galaxy is observed. A black hole is a region of spacetime where gravity is so strong that nothing, including light and other electromagnetic waves, is capable of possessing enough energy to escape it. [2] Einstein 's theory of general relativity predicts that a sufficiently ...
