"Greg Egan - Foundations 1 - Special Relativity" - читать интересную книгу автора (Egan Greg) =
OP2 / OP2 = = 1 The notation тАЬ(x,y)тАЭ beside the point P is a reminder that points can be referred to by their x- and y-coordinates, written as an ordered pair. The arrow drawn from O to P is a reminder that every point can be thought of as defining a vector from the origin to the point. The advantage of dealing with vectors, rather than just points in space, is that the same geometry can then be applied to other vectors, like velocity and acceleration. To make it easier to carry things over from Euclidean geometry to spacetime geometry, it will help to restate some of these familiar ideas in slightly different language. In both Euclidean and spacetime geometry, there's a formula for taking two vectors and calculating a number from them which depends on the length of the vectors and the angle between them. This formula is known as the metric for the geometry. (You might also have come across it as the тАЬdot productтАЭ of two vectors.) It's usually written as g: g[(x,y),(u,w)] = xu + yw (1) Eqn (1) defines the Euclidean metric. Eqns (2a)-(2c) demonstrate some of its properties: it's symmetric (swapping the two vectors leaves the value unchanged), and it's linear (its value is simply multiplied and added as shown, if you apply it to a vector g[(u,w),(x,y)] = ux + wy = xu + yw = g[(x,y),(u,w)] (2a) g[a(x,y),(u,w)] = g[(ax,ay),(u,w)] = axu + ayw = a (xu + yw) = a g[(x,y),(u,w)] (2b) g[(x,y)+(p,q),(u,w)] = g[(x+p,y+q),(u,w)] = (x+p)u + (y+q)w = (xu + yw) + (pu + qw) = g[(x,y),(u,w)] + g[(p,q),(u,w)] (2c) Egan: "Foundations 1"/p.6 Eqn (3) is just a restatement of Pythagoras's theorem; the notation |(x,y)| means the length of the vector (x,y) тАФ also referred to as its magnitude тАФ or if you prefer to think in terms of the coordinates of a point, |(x,y)| is the distance from the origin (0,0) to the point (x,y). |(x,y)|2 = g[(x,y),(x,y)] |
|
|