Examples of using Spacetime in English and their translations into Slovak
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fundamentally, a"shortcut" through spacetime.
objects travel along the path of these bends in spacetime.
One example of a great speaker is Neil deGrasse Tyson in the documentary series, Cosmos: A Spacetime Odyssey.
a villa in the south of France, the spacetime that intersects your local universe can be modified by you.
it was evidence that spacetime itself had been perturbed.
If tabbed browsing arranges your information in one axis along the tab bar, SpaceTime uses three axes.
Physical objects in spacetime are described by worldlines(if the object is a point particle)
In general relativity, an event horizon is a boundary in spacetime beyond which events cannot affect an outside observer.
This small value for the beta function means that currently the spacetime rainbow is very narrow
transformed the way scientists regard the universe with the development of his theory of spacetime.
Furthermore, the absence of potential energy in the“critical dimension” explains why flat spacetime solutions are possible.
Consequently, the quantum theory describing the low energy limit is a theory that describes the dynamics of these points moving in spacetime, rather than strings.
This little value for the beta function usually means that currently, the spacetime rainbow is extremely narrow and can't be detected experimentally.
An event horizon is, in general relativity, a boundary in spacetime beyond which events cannot affect an outside observer.
older criticism of string theory is that it is background-dependent- string theory describes perturbative expansions about fixed spacetime backgrounds.
In general relativity, an absolute horizon is a boundary in spacetime, defined with respect to the external universe, inside which events cannot affect an external observer.
Consequently, the quantum theory describing the low energy limit is a theory that describes the dynamics of particles moving in spacetime, rather than strings.
an event horizon is a boundary in spacetime beyond which events can never affect an outside observer.
Calculations have also shown that each theory requires more than the normal four spacetime dimensions(although all extra dimensions are in fact spatial.).
Spacetime diagram showing a uniformly accelerated particle,