| | '''Curvatures of spacetime''' is a set of 10 various curvatures that may be specified as components of a curvature tensor that describes the [[curvature of spacetime]] (the same thing as the [[curvature of 4-space]]). | | '''Curvatures of spacetime''' is a set of 10 various curvatures that may be specified as components of a curvature tensor that describes the [[curvature of spacetime]] (the same thing as the [[curvature of 4-space]]). |
| − | [[Curvature of spacetime]] (singular as opposed to plural "curvatures") is something that describes a fact that some 4-dimensional space is curved. It can't happen though in a stationary universe since the [[spacetime]] of stationary universe has to be flat (or [[Minkowski]], which is another word for the same thing). In particular '''curvatures of spacetime''' may describe the curvature of the common 3-dimenssional space (given by x,y,z vectors) being a part of this 4-dimensional spacetime (in this case given by t,x,y,z 4-vectors), which is a chance for messing things in astronomy when one says "[[curvature of space]]" but means the "[[curvature of spacetime]]" (that is then called simply [[curvature of 4-space]]) that has to be flat in stationary universe though having its non zero '''curvatures of spacetime''' adding to the flatness of whole [[spacetime]]. | + | [[Curvature of spacetime]] (singular as opposed to plural "curvatures") is something that describes a fact that some 4-dimensional space is curved. It can't happen though in a stationary universe since the [[spacetime]] of stationary universe has to be flat (or [[Minkowski]], which is another word for the same thing). In particular the '''curvatures of spacetime''' may describe the curvature of common 3-dimenssional space (given by x,y,z vectors) being a part of this 4-dimensional spacetime (in this case given by t,x,y,z 4-vectors), which is a chance for messing things in astronomy when one says the "[[curvature of space]]" but means the "[[curvature of spacetime]]" (that is then called simply the [[curvature of 4-space]]) that has to be flat in stationary universe though having its non zero '''curvatures of spacetime''' adding to the flatness of whole [[spacetime]]. |
| − | The 4-space has to be flat in stationary universe since parallel transport of 4-vectors along geodesic lines can't change the angles of those vectors for the reason of conservation of energy and momentum: the 4-vectors have to come back after the parallel transport being directd in the same direction and with the same magnitudes as before the transport by [[Noether theorem]]. To keep energy and momentum conserved there can't be any permanent changes in components of those vectors between ''"now"'' and ''"past"'' or ''"future"''. | + | The 4-space has to be flat in a stationary universe since parallel transport of 4-vectors along geodesic lines can't change the angles of those vectors for the reason of conservation of energy and momentum: the 4-vectors have to come back after the parallel transport being directd in the same direction and with the same magnitudes as before the transport by [[Noether theorem]]. To keep energy and momentum conserved there can't be any permanent changes in components of those vectors between the ''"now"'' and the ''"past"'' or the ''"future"''. |
| − | That's why it is often important to be aware of various subtleties of names used in physics not to violate suddenly the conservation of energy and/or momentum by requring "gravity to happen in a [[curved spacetime]]", while it is not required by any physical or geometrical law. | + | That's why it is often important to be aware of various subtleties of names used in physics not to violate suddenly the conservation of energy and/or momentum by requring "gravity to happen in the curved spacetime", while it is not required by any physical or geometrical law as [[Einsteinian gravitation]] might be happening just between particles interacting on a quantum level as described in the [[gravitation demystified]]. |