relativistic correction
1relativistic correction — reliatyvistinė pataisa statusas T sritis fizika atitikmenys: angl. relativistic correction; relativity correction vok. relativistische Korrektion, f; Relativitätskorrektion, f rus. релятивистская поправка, f pranc. correction relativiste, f …
2Relativistic Precession — The special and general theories of relativity give three types of corrections to the Newtonian precession, of a gyroscope near a large mass such as the earth. They are: * Thomas precession a special relativistic correction accounting for the… …
3correction relativiste — reliatyvistinė pataisa statusas T sritis fizika atitikmenys: angl. relativistic correction; relativity correction vok. relativistische Korrektion, f; Relativitätskorrektion, f rus. релятивистская поправка, f pranc. correction relativiste, f …
4Relativistic beaming — Doppler beaming redirects here. For other uses named for Christian Doppler, see Doppler (disambiguation). Only a single jet is visible in M87. Two jets are visib …
5relativity correction — reliatyvistinė pataisa statusas T sritis fizika atitikmenys: angl. relativistic correction; relativity correction vok. relativistische Korrektion, f; Relativitätskorrektion, f rus. релятивистская поправка, f pranc. correction relativiste, f …
6Fine structure — Interference fringes, showing fine structure (splitting) of a cooled deuterium source, viewed through a Fabry Pérot étalon. In atomic physics, the fine structure describes the splitting of the spectral lines of atoms due to first order… …
7Thomas precession — In physics the Thomas precession, named after Llewellyn Thomas, is a special relativistic correction to the precession of a gyroscope in a rotating non inertial frame. It can be understood as a consequence of the fact that the space of velocities …
8Redshift — This article is about the astronomical phenomenon. For other uses, see Redshift (disambiguation). Physical cosmology …
9Precession — For other uses, see Precession (disambiguation). Precession of a gyroscope Precession is a change in the orientation of the rotation axis of a rotating body. It can be defined as a change in direction of the rotation axis in which the second… …
101s Slater-type function — A normalized 1s Slater type function is a function which has the form:psi {1s}(zeta, mathbf{r R}) = left(frac{zeta^3}{pi} ight)^{1 over 2} , e^{ zeta |mathbf{r R}. [cite book last = Attila Szabo and Neil S. Ostlund first = title = Modern Quantum… …
