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Author Topic: Project Update  (Read 65266 times)
chooka03
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« Reply #45 on: March 06, 2019, 11:06:17 AM »

I saw that! Great news.
The team has been having a Universe@Home party lately! I have other priorities for the time being.

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Dataman
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Madness Takes Its Toll - Have Exact Change Ready


« Reply #46 on: April 20, 2019, 12:16:23 AM »

More from the project:

Sorry for late notification!

Another research on the famous GW170817 source, which used data obtained from the Universe@Home project, have been published last year. In this study, it was shown that the merger rates of double neutron stars (calculated from one direct observation) stay in contradiction with these inferred from the observations of double pulsars in our Galaxy. The reason behind this tension is the delay time distribution which favours short delays. The study highlights the problem that scientist encounter trying to connect evolutionary predictions and the observations of the first double neutron star merger.

The original paper can be found here:
http://adsabs.harvard.edu/abs/2018arXiv181210065B

 Boinc@Aussie
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