contraction$16355$ - translation to ελληνικό
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contraction$16355$ - translation to ελληνικό

THE CONTRACTION OF LENGTH IN THE DIRECTION OF PROPAGATION
Lorentz–FitzGerald contraction hypothesis; Lorentz contraction; Fitzgerald–Lorentz contraction; FitzGerald–Lorentz Contraction; FitzGerald Lorentz Contraction; Lorentz-Fitzgerald Contraction; Lorentz Contraction; Lorentz-Fitzgerald contraction hypothesis; Lorentz-Fitzgerald contraction; Fitzgerald contraction; FitzGerald-Lorentz contraction; Lorentz-FitzGerald Contraction; Space contraction; Relativistic length contraction; Lorentz-FitzGerald contraction hypothesis; Fitzgerald-Lorentz contraction; FitzGerald-Lorentz Contraction; Lorenz contraction; Lorentz-FitzGerald contraction; FitzGerald contraction; Lorentz-FitzGeral contraction; Lorentz-FirtGerald contraction; Lorentz–Fitzgerald contraction; Lorentz–FitzGerald contraction; FitzGerald–Lorentz contraction; Fitz-Gerald contraction; Lorentz-Fitzgerald; Lorentz contraction hypothesis; Relativistic foreshortening
  • Minkowski diagram of Einstein's 1911 [[thought experiment]] on length contraction. Two rods of rest length <math>A' B' = A'' B'' = L_0</math> are moving with 0.6c in opposite directions, resulting in <math>A^\ast B^\ast <L_0</math>.
  • Formula on a wall in Leiden, Netherlands. Lorentz was chair of theoretical physics at the [[University of Leiden]] 1877-1910
  • ''Length contraction'': Three blue rods are at rest in S, and three red rods in S'. At the instant when the left ends of A and D attain the same position on the axis of x, the lengths of the rods shall be compared. In S the simultaneous positions of the left side of A and the right side of C are more distant than those of D and F. While in S' the simultaneous positions of the left side of D and the right side of F are more distant than those of A and C.
  • In special relativity, the observer measures events against an infinite latticework of synchronized clocks.
  • Wheels which travel at 9/10 the speed of light.  The speed of the top of a wheel is 0.994 c while the speed of the bottom is always zero. This is why the top is contracted relative to the bottom.
  • Cuboids in Euclidean and Minkowski spacetime

contraction      
n. συστολή, στένεμα, συναίρεση, συνηρημένη λέξη, σύσπαση
monetary policy         
  • United States Treasury bond]]
  • The [[Bank of Japan]], in Tokyo, established in 1882.
  • Banknotes with a face value of 5000 in different currencies. ([[United States dollar]], [[Central African CFA franc]], [[Japanese yen]], [[Italian lira]], and [[French franc]])
  • Jiaozi]], redeemable for 770 ''mò''.
  • Mechanics of open market operations: Demand-Supply model for reserves market
  • Gold certificate]]s were used as [[paper currency]] in the [[United States]] from 1882 to 1933. These certificates were freely convertible into [[gold coin]]s.
SUBCLASS OF THE ECONOMIC POLICY
Monetary policy of central banks; Central bank/Monetary policy; Monetary Policy; Contractionary monetary policy; Monetary regime; Expansionary monetary policy; Monetary expansion; Price policy; Monetray policy; Price level targeting; Monetary action; Money policy; Contractionary policies; Expansionary policies; Monetary management; Goal of monetary policy; Tight money policy; Tight credit; Unconventional monetary policy; Contractionary; Monetary contraction; Monetary policies; Interest rate targeting; Monetary policy credibility; History of monetary policy
νομισματική πολιτική

Ορισμός

Lorentz contraction

Βικιπαίδεια

Length contraction

Length contraction is the phenomenon that a moving object's length is measured to be shorter than its proper length, which is the length as measured in the object's own rest frame. It is also known as Lorentz contraction or Lorentz–FitzGerald contraction (after Hendrik Lorentz and George Francis FitzGerald) and is usually only noticeable at a substantial fraction of the speed of light. Length contraction is only in the direction in which the body is travelling. For standard objects, this effect is negligible at everyday speeds, and can be ignored for all regular purposes, only becoming significant as the object approaches the speed of light relative to the observer.