Timeline for What is the uncertainty in the one solar mass radiated away as pure energy? (Gravitational waves)
Current License: CC BY-SA 3.0
4 events
| when toggle format | what | by | license | comment | |
|---|---|---|---|---|---|
| Jun 17, 2016 at 17:02 | history | edited | ProfRob | CC BY-SA 3.0 |
added 51 characters in body
|
| Jun 17, 2016 at 16:37 | vote | accept | uhoh | ||
| Jun 17, 2016 at 16:36 | comment | added | uhoh | OK great - it's late here so I will read in the morning. It seems that your are saying that the mass-loss with it's uncertainty is $1.0^{+0.1}_{-0.2}M_{\odot}$ , which is definitely an answer to the question. I understand what you are saying about the correlations, and so in a 3D plot of probability shells vs $m_1, m_2, \text{and } \Delta M$ will be narrower in the $\Delta M$ (mass loss) direction than either of the other two. Looking forward to one ore more cups of coffee and a nice morning read. Thanks!! | |
| Jun 17, 2016 at 16:07 | history | answered | ProfRob | CC BY-SA 3.0 |