Timeline for Gravitational waves detector orientation
Current License: CC BY-SA 3.0
6 events
| when toggle format | what | by | license | comment | |
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| Jan 23, 2018 at 20:15 | vote | accept | CommunityBot | ||
| Jan 23, 2018 at 18:16 | comment | added | Mike | @mmeent That's only in practice. In principle — which is what we deal with here — there are no other sources of signal in the universe, so a two-mass system is perfectly fine. Save your practical details for engineering.SE! ;) | |
| Jan 23, 2018 at 15:17 | answer | added | Mike | timeline score: 1 | |
| Jan 23, 2018 at 15:15 | comment | added | TimRias | With just two masses it is almost impossible. You typically need three (or more) freefalling masses as in LIGO or LISA. | |
| Jan 23, 2018 at 15:06 | history | edited | user174295 | CC BY-SA 3.0 |
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| Jan 23, 2018 at 15:00 | history | asked | user174295 | CC BY-SA 3.0 |