GALAXIES - what was 'extra' so visible matter was presumed missing?

In summary: MOND does have good results at the smaller dwarf galaxy scale. It seriously lacks on average galaxy rotation curves. Also MOND cannot explain gravitational lenses or early large scale structure formation. In some specific examples MOND does work better than LCDM dark matter however that's more due to our lack in our knowledge of dark matter distributions.
  • #1
stephenn
14
0
Hello
Dark matter is presumed... to balance the sums... as visible matter doesn't work out (apparently) to a high enough value...

... What part of the calculations was evaluated as being too high... to warrant the need for more matter to be 'somewhere'.

Thanks for thoughts
 
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  • #2
The rotational speed of the stars in the outer reaches of the galaxy is WAY off based on just the normal matter in the galaxy ... There has to be a huge amount of mass in addition to normal matter and that's how dark matter was inferred. It has been further verified by gravitational lensing.
 
  • #3
OK thanks, 'phinds'...

so... the rotational speed of stars in the outer reaches = faster than the quantity of mass, seen to be around... (providing gravitational force) to balance the sums... to hold them in their place, as observed.

* ... anyone know established papers with these sums?... (who concluded missing visible matter)


I've found another topic on these boards which is most interesting and have placed the link... should anyone else just reading this thread, wish to also consider:
Rotational Speed:
https://www.physicsforums.com/showthread.php?t=497992

* ... is it established, what gives a galaxy (spiral one)... it's rotational speed
* ... is there a top paper on rotational speeds (spiral galaxies)

cheers
 
  • #4
Here is a decent article though its more a review paper on LCDM measurements.

http://www.intechopen.com/download/pdf/18737

What your interested will be better answered here.

http://en.m.wikipedia.org/wiki/Galaxy_rotation_curve

It will cover the effect dark matter has on rotation curves better
along with this page
http://en.m.wikipedia.org/wiki/Dark_matter
 
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  • #5
Thanks for links, 'Mordred'...

Your links are helpfull... the first article one especially... rotational velocity in relation to radius distance etc

I've found another topic on these boards which is most interesting and have placed the link... should anyone else just reading this thread, wish to also consider:
simple explanation for rotation of spiral galaxy:
https://www.physicsforums.com/showthread.php?t=690481&highlight=galaxy+rotation

* ... am increasingly interested in honing in on the specific most established (agreed so far) actual cause of the velocity itself... in the rotation (for a spiral galxy)

cheers
 
  • #6
Mond

You probably know MOND. The author Moti Milgrom invented the possibility to explain the rotation curves with a modification of Newtonian dynamics as an alternative to DM. As the author says himself, it is a phenomenological observation only. But it is still in use! This year a team from germany/Bonn explained the bahaviour of satelite galaxies with MOND where the DM theory failed. I believe there is invisible mass. But who knows, maybe there is "something" to MOND.

Original Publication: Milgrom, 1983, The Astrophysical Journal, free from arxiv or google
 
  • #7
Philosopha said:
You probably know MOND. The author Moti Milgrom invented the possibility to explain the rotation curves with a modification of Newtonian dynamics as an alternative to DM. As the author says himself, it is a phenomenological observation only. But it is still in use! This year a team from germany/Bonn explained the bahaviour of satelite galaxies with MOND where the DM theory failed. I believe there is invisible mass. But who knows, maybe there is "something" to MOND.

Original Publication: Milgrom, 1983, The Astrophysical Journal, free from arxiv or google

MOND does provide a good fit to a certain class of gas-rich galaxies. The problem is MOND by *itself* does not seem to work in all situation: fitting CMB data for example. For more, see http://blogs.discovermagazine.com/cosmicvariance/2011/02/26/dark-matter-just-fine-thanks/.
But of course that is not saying modified gravity is ruled out!
 
  • #8
Philosopha said:
You probably know MOND. The author Moti Milgrom invented the possibility to explain the rotation curves with a modification of Newtonian dynamics as an alternative to DM. As the author says himself, it is a phenomenological observation only. But it is still in use! This year a team from germany/Bonn explained the bahaviour of satelite galaxies with MOND where the DM theory failed. I believe there is invisible mass. But who knows, maybe there is "something" to MOND.

Original Publication: Milgrom, 1983, The Astrophysical Journal, free from arxiv or google

while MOND does have good results at the smaller dwarf galaxy scale. It seriously lacks on average galaxy rotation curves.
Also MOND cannot explain gravitational lenses or early large scale structure formation.
In some specific examples MOND does work better than LCDM dark matter however that's more due to our lack in our knowledge of dark matter distributions.
Several MOND articles I have read include dark matter though
I would have to remember the
articles and locations of them
 
  • #9
Any MOND theory that requires dark matter defeats the entire premise.
 
  • #10
stephenn said:
Thanks for links, 'Mordred'...

Your links are helpfull... the first article one especially... rotational velocity in relation to radius distance etc

I've found another topic on these boards which is most interesting and have placed the link... should anyone else just reading this thread, wish to also consider:
simple explanation for rotation of spiral galaxy:
https://www.physicsforums.com/showthread.php?t=690481&highlight=galaxy+rotation

* ... am increasingly interested in honing in on the specific most established (agreed so far) actual cause of the velocity itself... in the rotation (for a spiral galxy)

cheers

I fully agree Chronos it does contradict the MOND premise.

That aspect is discussed in this recent LCDM and MOND review of challenges and difficulties faced in both models.

Coincidentally it will also provide a direction of current researches and challenges in our understanding of the dark sector.
Further reading can be found via the articles reference papers.
Some of the reference papers are worth reading.

The article is also handy in that it covers rotation curves of spiral galaxies. However I will not state which is the most agreed upon
lol. My opinion is biased towards the LCDM paradigm.

http://arxiv.org/abs/1301.0623
 
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What is dark matter?

Dark matter is a type of matter that does not emit or interact with light, making it invisible to telescopes. It is believed to make up about 85% of the total matter in the universe.

How do scientists know that there is missing matter in galaxies?

Scientists can observe the rotation of galaxies and calculate the amount of visible matter present. However, based on these calculations, there is not enough visible matter to account for the observed rotation. This suggests that there is additional matter present that is not visible, also known as dark matter.

What evidence supports the existence of dark matter?

Aside from the observed rotation of galaxies, scientists also use gravitational lensing, which is when the gravity of a massive object bends and distorts light from objects behind it, as evidence for dark matter. Additionally, computer simulations of the universe also support the existence of dark matter.

What are some theories about the nature of dark matter?

There are several theories about dark matter, including the possibility that it is made up of particles that interact very weakly with regular matter. Other theories suggest that it could be a type of exotic matter, such as primordial black holes or axions.

What is the significance of understanding dark matter?

Understanding dark matter is crucial to our understanding of the universe and its evolution. It plays a critical role in the formation and evolution of galaxies and other large-scale structures in the universe. Additionally, studying dark matter can also help us understand the fundamental laws of physics and possibly lead to new discoveries and technologies.

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