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| author | bnewbold <bnewbold@robocracy.org> | 2016-06-11 18:55:15 -0400 |
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| committer | bnewbold <bnewbold@robocracy.org> | 2016-06-11 19:01:12 -0400 |
| commit | 73884c965a489f53edfcf23ec4050ad0248685ce (patch) | |
| tree | 0f1ddb66393077d0284fbeb9e1fe839535c8dd21 /physics/LIGO.page | |
| parent | 2632bfadcfa505a4d5b31f5cb63495e3dec4a57b (diff) | |
| download | knowledge-73884c965a489f53edfcf23ec4050ad0248685ce.tar.gz knowledge-73884c965a489f53edfcf23ec4050ad0248685ce.zip | |
tweak physics syntax
Diffstat (limited to 'physics/LIGO.page')
| -rw-r--r-- | physics/LIGO.page | 15 |
1 files changed, 7 insertions, 8 deletions
diff --git a/physics/LIGO.page b/physics/LIGO.page index 2e86d5f..b7ba600 100644 --- a/physics/LIGO.page +++ b/physics/LIGO.page @@ -1,18 +1,12 @@ --- -format: rst -categories: physics toc: no +title: LIGO: Laser Interferometer Gravitational Observatory ... -======================================================================= -LIGO: Laser Interferometer Gravitational Observatory -======================================================================= - .. warning:: This is a rough work in progress!! Likely to be factual errors, poor grammar, etc. -.. note:: Most of this content is based on a 2002 Caltech course taught by - Kip Thorn [PH237]_ +.. note: Most of this content is based on a 2002 Caltech course taught by Kip Thorn [PH237] Noise Sources ~~~~~~~~~~~~~~~~~~~~~~ @@ -53,3 +47,8 @@ This technique requires known, theoretically derived waveforms (within phase/amplitude). There are other methods when we don't have good guesses about the waveform we are looking for... +References +---------------- + +[PH237]: **Gravitational Waves** (aka ph237), a course taught by Kip Thorne at Caltech in 2002. See http://elmer.tapir.caltech.edu/ph237/ for notes and lecture videos. + |