> On 27 Sep 2018, at 22:27, Brent Meeker <[email protected]> wrote:
> 
> The dark matter of a galaxy responsible for the flat rotation curve is 
> presumably in a cloud of spherical orbits around the galaxy.  It doesn't 
> collapse to a disk, as the visible matter does, because being dark it doesn't 
> radiate away energy via EM in collisions.  But it must still radiate 
> gravitational waves in collisions.  Are there estimates of how long this 
> would take to collapse dark matter to a disk?  Are there any galaxies we can 
> see which are old enough for this to have happened?


There are galaxies with strange shape that apparently nobody can explain, so 
perhaps …

Let me look for an example. Ah …  the Burçin Mutlu-Pakdil galaxy:

https://www.youtube.com/watch?v=uv5-hIif7BQ

Not sure how much hard it would be to detect a dark matter disk, but that 
should not be impossible. I would try this on those strange looking one.

Bruno



> 
> Brent
> 
> On 9/27/2018 5:00 AM, Philip Thrift wrote:
>> 
>> 
>> Someone to perhaps follow, doing #darkmatter theory:
>> 
>> Axel Maas <https://twitter.com/axelmaas>@axelmaas 
>> <https://twitter.com/axelmaas>
>> Professor for Theoretical Particle Physics at the University of Graz 
>> (Austria). Doing everything from low-energy QCD to beyond-the-standard-model 
>> #np3 <https://twitter.com/hashtag/np3?src=hash>
>> 
>> More                   
>> I have published a new blog entry on how a model, which we investigated for 
>> a very different purpose, may actually be a (perhaps even useful) 
>> #darkmatter <https://twitter.com/hashtag/darkmatter?src=hash> candidate, see 
>> https://axelmaas.blogspot.com/2018/09/unexpected-connections.html … 
>> <https://t.co/XBwoPUsEUP> #np3 <https://twitter.com/hashtag/np3?src=hash>
>> 
>> 
>> 
>> 
>> - pt
>> 
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