Ongenoemd mag ook niet blijven de semi-populaire verhandeling van de meester zelf, ” Over de speciale en algemene relativiteitstheorie”, Albert Einstein (Het. General Relativity (Algemene Relativiteitstheorie) (NS-TPM): RULES. Teacher: Tomislav Prokopec, office: BBG , tel. , email: . Einstein: mijn theorie / druk 9: over de speciale en de algemene relativiteitstheorie on *FREE* shipping on qualifying offers.
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This formula, too, is readily generalized to curved spacetime by replacing partial derivatives with their curved- manifold counterparts, covariant derivatives studied in differential geometry.
Categorie:Algemene relativiteitstheorie – Wikipedia
A thorough, book-length introduction including an introduction to the necessary mathematics Poisson Weinbergch. This is readily described by the expanding cosmological solutions relativiteitsheorie by Friedmann inwhich do not require a cosmological constant.
Gravitational lensing has developed into a tool of observational astronomy. Rindlersec.
Introduction History Mathematical formulation Tests. The best-known examples are black holes: For instance, by the second law of black hole mechanics, the area of the event horizon of a general black hole will never decrease with time, analogous to the entropy of a thermodynamic system.
A distant observer will determine that objects close to the mass get “dragged around”. De ricci-tensor relativiteotstheorie scalaire kromming kunnen eenduidig bepaald worden gegeven de metrische tensordus de einstein-tensor kan in principe expliciet uitgedrukt worden in termen van de metriek.
The solutions require extreme physical conditions unlikely ever to occur in practice, and it remains an open question whether further laws of physics will eliminate them completely. This limits relativiteitsthorie energy that can be extracted by classical means from a rotating black hole e.
Paispp. Detection of these waves is a major goal of current relativity-related research. Ordinary quantum field theorieswhich form the basis of modern elementary particle physics, are defined in flat Minkowski space, which is an excellent approximation when it comes to describing the behavior of microscopic particles in weak gravitational fields like those found on Earth. Gravitational redshift has been measured in the laboratory  and using astronomical observations.
If general relativity were considered to be one of the two pillars of modern physics, then quantum theory, the basis of understanding matter from elementary particles to solid relativieitstheorie physicswould be the other.
Aware of the importance of causal structure, Roger Penrose and others developed what is known as global geometry.
The demand for consistency between a quantum description of matter and a geometric description of spacetime,  as well as the appearance relativiteitstyeorie singularities where curvature length scales become microscopicindicate the need for a full theory of quantum gravity: On February 11,the Advanced LIGO team announced that they had directly detected gravitational waves from a pair of black holes merging.
De eenvoud van deze vergelijkingen, uitgedrukt met de einstein-tensor toont de diepe geometrische en fysische betekenis van het object aan. It must be combined with a coordinate conditionwhich is analogous to gauge fixing in other field algdmene.
Hulpmiddelen Links naar deze pagina Verwante wijzigingen Bestand uploaden Speciale pagina’s Permanente koppeling Paginagegevens Wikidata-item Deze pagina citeren. Assuming that the equivalence principle holds,  gravity influences the relativiteiystheorie of time.
As can be shown using simple thought experiments following the free-fall trajectories of different test particles, the result of transporting spacetime vectors that can denote a particle’s velocity time-like vectors will vary with relativireitstheorie particle’s trajectory; mathematically speaking, the Newtonian connection is not integrable. An early key article is Einsteincf.
Black hole Event horizon Singularity Two-body problem Gravitational waves: The Einstein field equations are nonlinear and very difficult to solve.
Translated into the language of spacetime: In modern parlance, their paths are relativiteitstheorlestraight world lines in curved spacetime. Quantum mechanics Quantum electrodynamics Quantum field theory Quantum gravity.
The theory is successful in that one mode will always correspond to a gravitonthe messenger particle of gravity, e. But as early asthe astrophysicist Karl Schwarzschild found the first non-trivial exact solution to the Einstein field equations, the Schwarzschild metric.
Bringing gravity into play, and assuming the universality of free fall, an analogous reasoning as in the previous section applies: Wikisource has original works on the topic: Although the bending of light can also be derived by extending the universality of free fall to light,  the angle of deflection resulting from such calculations is only half the value given by general relativity.
However, there are strong indications the relatigiteitstheorie is incomplete. Light cone World line Minkowski diagram Biquaternions Minkowski space.
Some remarks on the notions of general covariance and background independence”, Approaches to Fundamental PhysicsLecture Notes in Physics, Springer, General relativity generalizes special relativity and Newton’s law of universal gravitationproviding a unified description of gravity as a geometric property of space and timeor spacetime.
De einstein-tensor komt voor in het linkerlid van de einstein-vergelijkingen:. Such effects are known as algemehe lensing. General relativity GRalso known as the general theory of relativity or GTR is the geometric theory of gravitation published by Albert Einstein in and the current description of gravitation in modern physics.
The derivation outlined in the previous section contains all the information needed to define general relativity, describe its key properties, and address a question of crucial importance in physics, namely how the theory can be used for model-building. Kaluza—Klein theory Quantum gravity Supergravity. Consequently, we are now dealing with a curved generalization of Minkowski space. With this additional condition—the covariant divergence of the energy—momentum tensor, and hence of whatever is on the other side of the equation, is zero— the simplest set of equations are what are called Einstein’s field equations:.
Views Read Edit View history. This page was last edited on 21 Decemberat As it is constructed using tensors, general relativity exhibits general covariance: Equivalence principle Riemannian geometry Penrose diagram Geodesics Mach’s principle. Such calculations tacitly assume that the geometry of space is Euclideancf. De einstein-vergelijking van de algemene relativiteitstheorie geeft de evenredigheidsrelatie met de energie inclusief die vertegenwoordigd door rustmassa per volume-eenheid.
Giulini, DomenicoSpecial Relativity: