At yesterdays RAS General meeting there was an interesting lecture on Cosmology – by Professor Andrew Liddle (Sussex): Titled The Universe, Darkly one of the interesting points he made is that the information we have on the existence of dark matter is from the galaxy surveys and gravitational lensing that are typically at a redshift of 1 or so and are therefore a reasonable time in the past. You need to go back this far to get a large enough volume of space to see the effects.
There is also a constraint on dark matter imposed by the CMB.
The interesting thing is that if you join these two constraints using equations used to predict the evolution of dark matter when you run the equations forward it is possible their is no dark matter now or equally rather more than was in the past. The problem is that observations of the local universe ( a few million Parsecs !) do not contain enough volume or distance for the effects of dark matter to be seen. The reason there appears to be less dark matter in the relatively local galaxies we can measure the rotation curves of could be that dark matter is decaying and has at the present epoch almost disappeared.
This could explain why the dark matter detectors have not found it and why there is no evidence for dark matter in the Solar System.
A similar argument can be used for dark energy but the constraints due to observations of SN are even wider.
Comments ?
John Murrell
Astronomer Without Portfolio
Website www.JohnMurrell.org.uk
Is my posting below related to this news release ? http://www.ras.org.uk/news-and-press/219-news-2012/2187-cosmic-gdp-crashes-97-as-star-formation-slumps
If dark matter is required for galaxy formation what impact does it have on star formation rates ??
Am I jumping to unwarranted associations ?
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Mike,
The estimates of dark matter at around Z=1 are from the SDSS and the other similar survey I have forgotten at present.
The rotation curves of nearby galaxies show less dark matter than that predicted from the CMB & Big Bang – you need to go for clusters of galaxies at large distances to see the most dark matter.
As for our galaxy I don’t think we have a rotation curve – from where we are it is difficult enough to get the arm structure right let alone work out the rotation curve.
As for the local dark matter there appears to be little agreement – some papers state there is no evidence but others state there is. The dark matter detectors have so far drawn a blank with the possible exception of one disputed result. However Dark Matter may not be WIMPs which is what I think the detectors are looking for.
Perhaps we should invite Andrew Liddle to speak to the CAS ?
Hi Tony,
I heard the Barbara Becker talk and thought it was very good.
When it came to question time it was obvious from the way she answered that she had done a great deal of research and knew the subject intimately.
Regards
Brian
From: alta...@googlegroups.com [mailto:alta...@googlegroups.com] On Behalf Of Tony Angel
Sent: 11 November 2012 23:49
To: alta...@googlegroups.com
John
The link below leads to a BBC report concerning the failure to find evidence of WIMPs at LHC http://www.BBC.co.UK/news/science-environment-20300100
Mike
Mike,
The failure to find WIMPs at the LHC shakes people’s faith in Super Symmetry as was said in the article Super Symmetry is not dead but it is in hospital !
I believe the LHC should create the WIMPs so even if they have died out there should still be some in the LHCb data.
As Tony said it was Zwicky who identified the need for dark matter to hold the coma cluster together – that gets a mention the review of his biography in the November Astronomy Now. The coma cluster is some 320 M light years away. The value of Omega for the cluster appears to be about 0.1 i.e. 1/10 of the value for the Universe as a whole.
Have a look at the article in Astronomy at http://astronomy.com/News-Observing/News/2012/11/Astronomers measure the universes deceleration before dark energy took over.aspx
It is a pity that the expansion graph does not have a vertical scale or even a zero point ! Is drawing the curve they have chosen consistent with the data points ?