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| author | bnewbold <bnewbold@eta.mit.edu> | 2009-02-03 06:08:09 -0500 | 
|---|---|---|
| committer | bnewbold <bnewbold@eta.mit.edu> | 2009-02-03 06:08:09 -0500 | 
| commit | b053ffbd7f1dc1a28098c1a68d44d92d0f449cfc (patch) | |
| tree | 1c232af203814323aac7617575ef6c2756114f04 /physics/special relativity | |
| parent | 95a9589201696dfe00a9219e5c2586bfec15339b (diff) | |
| parent | 838e1b2d55f39113fffe0f998cb1011b57747691 (diff) | |
| download | knowledge-b053ffbd7f1dc1a28098c1a68d44d92d0f449cfc.tar.gz knowledge-b053ffbd7f1dc1a28098c1a68d44d92d0f449cfc.zip  | |
Merge branch 'master' of ssh://bnewbold@animus.robocracy.org/srv/git/knowledge
Diffstat (limited to 'physics/special relativity')
| -rw-r--r-- | physics/special relativity | 15 | 
1 files changed, 9 insertions, 6 deletions
diff --git a/physics/special relativity b/physics/special relativity index 41bf4b8..37fd3e9 100644 --- a/physics/special relativity +++ b/physics/special relativity @@ -8,7 +8,7 @@ Special Relativity  .. note:: Most of this content is based on a 2002 Caltech course taught by      Kip Thorn [PH237]_ -*See also `physics/general relativity</k/physics/generalrelativity/>`_* +*See also `physics/general relativity</k/physics/generalrelativity/>`__*  As opposed to general relativity, special relativity takes place in a *flat*  Minkowski space time: a 4-space with three spatial dimensions and one time @@ -17,22 +17,25 @@ dimension.  +----------------+--------------------+  | Index notation | Variable | Type    |  +----------------+--------------------+ -| `$x^\0`:m:     | `$t$`:m: | Time    | -| `$x^\1`:m:     | `$x$`:m: | Spatial | -| `$x^\2`:m:     | `$y$`:m: | Spatial | -| `$x^\3`:m:     | `$z$`:m: | Spatial | +| `$x^0$`:m:     | `$t$`:m: | Time    | +| `$x^1$`:m:     | `$x$`:m: | Spatial | +| `$x^2$`:m:     | `$y$`:m: | Spatial | +| `$x^3$`:m:     | `$z$`:m: | Spatial |  +----------------+--------------------+  Separations  ------------- -The separation `$(\Delta s)^2`:m: between two events in space time, in a given +The separation `$(\Delta s)^2$`:m: between two events in space time, in a given  Lorentzian/inertial frame, is defined  as:  :m:`$$ (\Delta s)^2 \equiv -(\Delta t)^2 + (\Delta x)^2 + (\Delta y)^2 + (\Delta z)^2 $$` +  or +  :m:`$$ (\Delta s)^2 \equiv -(\Delta x^0)^2 + \sum_{i,j} \delta_{ij} \Delta x^i \Delta x^j$$` +  where :m:`$\delta_{ij}$` is the Kronecker delta (unity or 1 when   :m:`$i=j$`; zero otherwise), and the indices i and j are over the spatial  dimensions 1,2,3 (corresponding to x,y,z). It can be shown that this separation  | 
