Maxsus çağıştırmalılıq teoriäse: юрамалар арасында аерма

Контент бетерелгән Контент өстәлгән
Юл номеры - 46:
İkençe Postulatnı anıñ üzeneñ tögelräk yuraması qullanırğa bula. Fäza-waqıt intervalı inertsial başlap sanaw sistemlären alışqaç, invariant bulıp qala. Berar nindi ''A'' häm ''B'' waqiğalar öçen:
:<math> c^2 (s-t)^2 - (x_1-y_1)^2 - (x_2-y_2)^2 - (x_3-y_3)^2 = c^2 (s'-t')^2 - (x'_1-y'_1)^2 - (x'_2-y'_2)^2 - (x'_3-y'_3)^2</math>
ide. Başlap sanaw sistemeläre arasında transformasiäları öçen qanunnar çağıştıru bu qanun qullanırğa bula; [[Lorentz transformasiälärıtransformasiäläre]]n qara.
 
[[Pseudo-Rieman küptabaqlı fäzası]]n qullanğaç, Postulatlarnıñ matematik küzallawı qısqarala.<!--The postulates of special relativity can be expressed very succinctly using the mathematical language of [[pseudo-Riemannian manifold]]s. The second postulate is then an assertion that the four-dimensional spacetime ''M'' is a pseudo-Riemannian manifold equipped with a Lorentzian metric ''g'' of signature (3,1), which is given by the flat [[Minkowski metric]] when measured in each inertial reference frame. This metric is viewed as one of the physical quantities of the theory, thus it transforms in a certain manner when the frame of reference is changed, and it can be legitimately used in describing the laws of physics. The first postulate is an assertion that the laws of physics are invariant when represented in any frame of reference for which ''g'' is given by the Minkowski metric. One advantage of this formulation is that it is now easy to compare special relativity with [[general relativity]], in which the same two postulates hold but the assumption that the metric is required to be Minkowski is dropped.-->