Galaxy motions -> hidden superstructure (DM)

  • Thread starter Nereid
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In summary: This is because the standard BB model predicts that the total mass in a cluster should be the same as the mass of the galaxies within it, and if there is more mass than that, then it should be orbiting at a distance where it can't gravitationally interact with the galaxies. But galaxies within a cluster will have been drawn in by the cluster's gravity, and so the extra mass must be in the form of dark matter. This is the explanation for the 'dark matter halos' around galaxies, and the fact that the amount of dark matter in a cluster is proportional to the mass of the clusters galaxies.
  • #71
Garth said:
They were not - indeed GPB is ideal for testing such alternatives - SCC and Moffat's non-symmetric gravitational theory (NGT) [see "Modified Gravitational Theory and the Gravity Probe-B Gyroscope Experiment" http://arxiv.org/abs/gr-qc/0405091] .
Good to hear.
The question how would a non-GR outcome of the experiment be interpreted should it occur?
Indeed! It should be an exciting time, should it not?
1. The space-borne interferometer to test whether photons and particles fall 'at the same rate': "Self Creation Cosmology An Alternative Gravitational Theory" http://arXiv:gr-qc/0405094 Section 7.1 pg 17.
I'd be interested to hear whether you think the proposals in Cosmic Visions (or the NASA equivalent) will cover this.
2. The deep-space Casimir force experiment to test whether there is a cut off of the Casimir force at great distances from the Sun. (ibid)
AFAIK, there are no deep space experiments planned, by anyone, for any purpose :cry: (unless you count the Pluto-Kuiper Express, which is all but dead, no?)
The truncated LIGO type interferometer, to test the same question as 1 above.
To what extent would LISA be able to serve as an alternative? What about the resonant mass gravity wave detectors?
I can partly understand Nereid's puzzlement over the statement. However I would like to point out that, apart from a motley collection of such as myself who might be called 'crackpots' by some, there are a number of respected figures who have signed the statement such as Bondi, Gold and Narlikar. But why have they?
That's what I'm trying to understand! If none of the missions preclude tests of any alternatives, and if there are but a small number of dedicated missions that the iconclasts would dream of, where's the beef (other than pocket money for tea and biccies)?
 
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  • #73
On possible non-GR outcome of GPB experiment:
Nereid said:
It should be an exciting time, should it not?
If such an outcome should occur do you think they will devise another epicycle?
Nereid said:
I'd be interested to hear whether you think the proposals in Cosmic Visions (or the NASA equivalent) will cover this.
AFAIK it does not - however not having broadband I haven't been able to download all those files on your link - yet!
Nereid said:
AFAIK, there are no deep space experiments planned, by anyone, for any purpose (unless you count the Pluto-Kuiper Express, which is all but dead, no?).
It has been suggested that a Pioneer Anomaly test be put onboard a low-mass, low-thrust mission to Pluto, the Pluto orbiter Probe or POP. A study of such a mission has been undertaken recently in ESA’s Advanced Concepts Team and detailed results of the system design and trajectory design have been presented in T. Bondo et al, “Preliminary Design of an Advanced Mission to Pluto”. Proceeding of the 24th ISTS, Miyazaki, Japan, June 2004. http://www.esa.int/gsp/ACT/doc/ACT-RPR-4200-ISTS2004.pdf . I have no idea as to whether or when it would get off the ground.
Nereid said:
To what extent would LISA be able to serve as an alternative? What about the resonant mass gravity wave detectors?
The experiment compares the gravitational attraction of a horizontal light beam against that of a solid apparatus. I do not think LISA will comply, the gravitational bending of light being equal in GR and SCC.
[Such deviation being of two components, one due to the 'free fall' of the photon the other due to the curvature of space - in GR these two contribute 1/2 + 1/2 respectively to the total deviation; in SCC they contribute 3/4 + 1/4 respectively of the same total deviation 1.75".]
- Garth
 
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  • #74
Garth said:
On possible non-GR outcome of GPB experiment:
Nereid said:
Indeed! It should be an exciting time, should it not?
Garth said:
The question how would a non-GR outcome of the experiment be interpreted should it occur?
If such an outcome should occur do you think they will devise another epicycle?
It's pure physics, so lots of $$ will be found to do a bigger and better GPB; ten thousand new 'GR-killer' theories will flow from the word processors of theorists; ten creative ideas to test the new theories will be published, involving little more than what can be found in a leading university lab; three hundred extensive data-mining projects will be commenced, using BOINC (the new grid computing platform on which Seti@Home now runs); ... and key insight for 'the answer' will come from the mind of a bright young PhD student in China (or India). :wink:
 
  • #75
DM as higher vibrations?

Good discussion here.
I used to deride Dark matter as a makeshift idea to plug the emerging holes in GR, or Newtonian at least. I guess what turned me around is string theory. For once Ican see how DM could exist.

I don't think dark matter is one long brane covering the universe, though that is possible. But perhaps it has to do with the frequency of the wave nature of particles. For example, photons are considered a string just as baryons are, only at a higher vibration. Light happens to be at the upper vibratory limit of what our expanded dimensions can swallow. But does that mean there's no strings that vibrate faster than light? If there were, wouldn't we not see them at all, nor be able to detect them? Would that be, 'dark matter'?

It's something I've thought about and perhaps Tachyons(sp?) are an offshoot of that dea, I don't know much about them though. Anyone like to comment?
 
  • #76
Mike2 said:
I've not seen the data. Are the galactic rotation curves and the lensing effects just as strong for Andromeda as for very distant galaxies? Thanks.
Lensing effects do not really apply to Andromeda, although searches are made for 'local' (our galactic halo) micro-lensing events that might be caused by mini black holes or Jupiters. [See today's 'Some Consequences of the Baryonic Dark Matter Population' Rudolph E. Schild http://arXiv:astro-ph/0409549 for distant such objects]

However galactic rotation curves certainly do apply not only to Andromeda but also for the Milky Way itself.

Each galaxy seems to have a massive invisible halo and each galaxy cluster seems to have a massive intergalactic medium, also invisible. Visible matter ~ 4%, Dark Matter ~ 23% of total critical density.

Garth
 
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