flat spacetime造句

• In flat spacetime, this means that the velocity is constant.
• A straight line is a nonaccelerating worldline in flat spacetime.
• The above equations are valid in flat spacetime.
• Where K _ 0 is the extrinsic curvature of the boundary imbedded flat spacetime.
• Although we still have, in flat spacetime;
• Again in flat spacetime, this translates to;
• Let us evaluate this for flat spacetime.
• In the context of an asymptotically flat spacetime, the boundary conditions are given at infinity.
• Here D is the covector derivative in any spacetime and reduces to \ bigtriangledown in flat spacetime.
• Lorentz metric, reserved for-dimensional flat spacetime with the remaining ambiguity only being the signature convention.
• Such time dilation appears in the Rindler coordinates, attached to a uniformly accelerating particle in a flat spacetime.
• In the free-fall frame the Maxwell equations have their usual, flat spacetime form for the falling observer.
• The first term in \ beta ^ \ Phi is just the anomaly of the bosonic string theory in a flat spacetime.
• In 1997 and 1998, two papers by Don Colladay and Alan Kosteleck?gave birth to the minimal SME in flat spacetime.
• Maxwell's equations in curved spacetime can be obtained by replacing the derivatives in the equations in flat spacetime with covariant derivatives.
• Now this consensus is about Feynman being for flat spacetime ( like Narlikar ) in which curvature of space compensate for time dilations.
• Note that the Einstein group approaches but never reaches the Poincare group as the flat spacetime ( special relativity limit ) is approached.
• In flat spacetime and linear coordinatization, " differences " in coordinates,, can be treated as a contravariant vector.
• In the absence of any ( large ) energy-momentum density-flux GR predicts a flat spacetime AKA Minkowski space-time.
• Special relativity is restricted to flat spacetime, " i . e . ", to all phenomena without significant influence of gravitation.