Vir: Wikipedia. Strani: Poglavjih: Albert Einstein, Enrico Fermi, Posebna teorija relativnosti, Splošna teorija relativnosti, Eugene Paul Wigner, Richard Phillips. Teorija relativnosti [trda vezava]. Authors: translation (Einstein) and afterword Matjaž Ličer translation Albert Einstein in rojstvo sodobne relativistične fizike. Vir: Wikipedia. Strani: Poglavjih: Albert Einstein, Enrico Fermi, Posebna teorija relativnosti, Splo na teorija relativnosti, Eugene Paul Wigner, Richard Phillips.
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Attempts to generalize ordinary quantum field theories, used in elementary particle physics to describe fundamental interactions, so as to include gravity have led to serious problems. Given both Einstein’s equations and suitable equations for the properties of matter, such a solution consists of a specific semi-Riemannian manifold usually defined by giving the metric in specific coordinatesand specific matter fields defined on that manifold. Measurement of de Sitter geodetic precession rate for lunar perigee”, Physical Review Letters58 Prema Bellu, kvantna nelokalnost time je ustanovljena, dok drugi u tome vide teorijx determinizma.
Krucijalno pitanje koje bi on pitao, dok je odvagivao neke od elemenata teorije bilo relativnsoti Given the difficulty of finding exact solutions, Einstein’s field equations are also solved frequently by numerical integration on a einsteon, or by considering small perturbations of exact solutions.
This structure can be displayed using Penrose—Carter diagrams in which infinitely large regions of space and infinite time intervals are shrunk ” compactified ” so as to fit onto a finite map, while light still travels along diagonals as in standard spacetime diagrams. In the field of numerical relativitypowerful computers are employed to simulate the geometry of spacetime and to solve Einstein’s equations for interesting situations such as two colliding black holes.
In modern parlance, their paths are geodesicsstraight world lines in curved spacetime. For example, it implies the existence of black holes—regions of space in which space and time are distorted in such a way that nothing, not even light, can escape—as an end-state for massive stars.
As thermodynamical objects with non-zero temperature, black holes should emit thermal radiation. Einstein umire u 1: As it is constructed using tensors, general relativity exhibits general covariance: Compile a new entry. Using global geometry, later studies have revealed more general properties of black holes. However, for weak fields, a linear approximation can be made. Equivalence principle Riemannian geometry Penrose diagram Geodesics Mach’s principle.
This suggests the definition of a new class of inertial motion, namely that of objects in free fall under the influence of gravity.
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AndrewsScotland, May, The theory is successful in that one mode will always correspond to a gravitonthe messenger particle of gravity, e. You will find the translations found for all senses of the headword under the tab “Usage Examples”. The entry has been added to your favourites. Mathematics of general relativity and Physical theories modified by general relativity. Whenever the ratio of an object’s mass to relativbosti radius becomes sufficiently large, general relativity predicts the formation of a black hole, a region of space from which nothing, not even light, can escape.
Waldch. At its core are Einstein’s equationswhich describe the relation between the geometry of a four-dimensional pseudo-Riemannian manifold representing spacetime, and the energy—momentum contained in that spacetime.
Ovaj rad predstavlja uvod u posebnu teoriju relativnostikao teoriju vremenaprostoramase i energijekoja je u suglasnosti sa teorijom elektromagnetizmaali ne opisuje pojavu gravitacije.
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You can jump the queue or expand by hand Havas, P. Relativity 3http: Soon after publishing the special theory of relativity inEinstein started thinking about how to incorporate gravity into his new relativistic framework.
How can I copy translations to the vocabulary trainer? This new class of preferred motions, too, defines a geometry of space and time—in mathematical terms, it is the geodesic motion associated with a specific connection which depends on the gradient of the gravitational potential.
Due to its general covariance, Einstein’s theory is teodija sufficient by itself to determine the time evolution of the metric tensor.
Such effects are known as gravitational lensing. Relativity 5DOI: Astronomical observations of the cosmological expansion rate allow the total amount of matter in the universe to be estimated, although the nature of that matter remains mysterious in part.
These are one of several analogies between weak-field gravity and electromagnetism in that, they are analogous to electromagnetic waves. Reactivation will enable you to use alebrt vocabulary trainer and any other programs. Assuming that the equivalence principle holds,  gravity influences the passage of time.
This is most extreme for rotating black holes where, for any object entering a zone known as the ergosphererotation is inevitable.