asymptotically$5581$ - significado y definición. Qué es asymptotically$5581$
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Qué (quién) es asymptotically$5581$ - definición

Asymptotically flat; Asymptotic flatness; Asymptotically simple spacetime

Asymptotically flat spacetime         
An asymptotically flat spacetime is a Lorentzian manifold in which, roughly speaking, the curvature vanishes at large distances from some region, so that at large distances, the geometry becomes indistinguishable from that of Minkowski spacetime.
Asymptotically optimal algorithm         
ALGORITHM THAT IS AT MOST A CONSTANT FACTOR WORSE THAN THE BEST POSSIBLE ALGORITHM FOR LARGE INPUT SIZES
Asymptotic optimality; Asymptotically optimal; Asymptotically faster algorithm
In computer science, an algorithm is said to be asymptotically optimal if, roughly speaking, for large inputs it performs at worst a constant factor (independent of the input size) worse than the best possible algorithm. It is a term commonly encountered in computer science research as a result of widespread use of big-O notation.
Asymptotic freedom         
PHENOMENON IN CERTAIN QUANTUM SYSTEMS IN WHICH THE COUPLING CONSTANT BECOMES SMALL AT HIGH ENERGY SCALES
Asymptotically free
In quantum field theory, asymptotic freedom is a property of some gauge theories that causes interactions between particles to become asymptotically weaker as the energy scale increases and the corresponding length scale decreases.

Wikipedia

Asymptotically flat spacetime

An asymptotically flat spacetime is a Lorentzian manifold in which, roughly speaking, the curvature vanishes at large distances from some region, so that at large distances, the geometry becomes indistinguishable from that of Minkowski spacetime.

While this notion makes sense for any Lorentzian manifold, it is most often applied to a spacetime standing as a solution to the field equations of some metric theory of gravitation, particularly general relativity. In this case, we can say that an asymptotically flat spacetime is one in which the gravitational field, as well as any matter or other fields which may be present, become negligible in magnitude at large distances from some region. In particular, in an asymptotically flat vacuum solution, the gravitational field (curvature) becomes negligible at large distances from the source of the field (typically some isolated massive object such as a star).