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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 | |
| 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')
| -rw-r--r-- | physics/general relativity | 3 | ||||
| -rw-r--r-- | physics/gravitational waves | 6 | ||||
| -rw-r--r-- | physics/special relativity | 15 |
3 files changed, 15 insertions, 9 deletions
diff --git a/physics/general relativity b/physics/general relativity index 7521db5..7fc29eb 100644 --- a/physics/general relativity +++ b/physics/general relativity @@ -8,8 +8,9 @@ General Relativity .. note:: Most of this content is based on a 2002 Caltech course taught by Kip Thorn [PH237]_ -*See also `math/tensors </k/math/tensors>`_* +*See also `math/tensors </k/math/tensors>`__* +(no content) References ---------------- diff --git a/physics/gravitational waves b/physics/gravitational waves index ab7174e..5aa1744 100644 --- a/physics/gravitational waves +++ b/physics/gravitational waves @@ -38,9 +38,11 @@ Fifth term: current quadrupole Energy ---------------- -Quick calculation: for a source with mass M, size L, period P, the quadrupole moment $M_2 \approx M L^2$, h \approx 1/c^2 (Newtonian potential energy) ???? +Quick calculation: for a source with mass M, size L, period P, the quadrupole +moment :m:`$M_2 \approx M L^2$`, :m:`$h \approx 1/c^2` (Newtonian potential +energy) ???? -h on the order of $10^{-22}$ +h on the order of :m:`$10^{-22}$` Propagation ----------------- 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 |