Gravitational lensing and Dark matter

In summary: There are many, many others. In summary, gravitational lensing does support the existence of dark matter, but we don't know what it is.
  • #1
jlorda
28
0
Does anyone know if gravitational lensing confirms the existence of Dark matter?
 
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  • #2
This is a FAQ

It would be better to say "supports" the existence of dark matter. See for example Ned Wright's Cosmology FAQ and his Cosmology Tutorial:
www.astro.ucla.edu/~wright/cosmology_faq.html
www.astro.ucla.edu/~wright/cosmolog.htm

I have suggested that a friendly mentor move this to the Cosmology forum at PF, since it seems to me that your question concerns mainstream cosmology more than it concerns speculations regarding the future of particle physics. That is, you are asking about phenomenological evidence for something we provisionally call "dark matter", not about possible particle physics explanations of what this stuff might be.

[EDIT: It was moved to "Astrophysics", a reasonable compromise.]
 
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  • #3
Does anyone know if gravitational lensing supports the existence of dark matter? Where can I read about this? Are there any examples of this? I looked up the link that you posted Chris but this did not show me any answers to my question.

Would gravitational lensing be different for a givin galaxy if Dark Matter was not present?
 
  • #4
Some more links for you

jlorda said:
Does anyone know if gravitational lensing supports the existence of dark matter?

As I already said, yes, it does.

jlorda said:
Would gravitational lensing be different for a [given] galaxy if Dark Matter was not present?

A short answer: yes, that is the point.

A better answer: we know how to compute the lensing we would expect if "the mass-energy we understand and already knew about" (mostly stars, but also stuff like interstellar dust clouds) accounted for the mass-energy associated with a given visible galaxy. But the lensing we observe (when a foreground and background galaxy are almost aligned wrt our solar system) clearly suggests that--- surprise!--- there is quite a bit of additional mass-energy. This is phenomenologically identified with "dark matter", but so far no-one knows what this might be, just that it seems to be out there, in abundance. Specifically, we have some idea of how it tends to be distributed wrt the mass-energy we understand: it is associated with visible galaxies but seems to extend beyond the stuff we already knew about, forming a "halo" of invisible "dark matter" around the ordinary matter in each galaxy.

[EDIT: As cristo pointed out in Post #5, this analysis assumes that our default theory of gravitation, gtr, is good for galactic scales. There is really no reason to think this is not true--- gtr has been tested many many times in many ways, and has passed every test so far--- hence the general acceptance of the conclusion that "dark matter" must in fact exist.]

jlorda said:
Where can I read about this?

The answer to your question was very widely publicized not long ago by the mainstream media, so I am somewhat puzzled why you have experienced difficulties in obtaining information. The pages by Ned Wright I mentioned do answer your question, but I guess you didn't want to look for the answer. So try instead this article by Phil Plait (of BAUT fame)
http://www.seedmagazine.com/news/2007/02/found_most_of_the_universe.php
or this blog post by Sean Carroll (of gtr textbook fame)
http://cosmicvariance.com/2006/08/21/dark-matter-exists/

You can find many more links at http://en.wikipedia.org/wiki/Dark_matter;
I must warn as always that Wikipedia itself cannot be safely used as an information resource unless you can verify whatever a given version of some article claims by consulting a reliable source, such as a (conventional) encyclopedia. In this case, I happen to know that Plait and Carroll are reliable sources, so the articles I cited should be acceptable for a school project or whatever.
 
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  • #5
jlorda said:
Does anyone know if gravitational lensing supports the existence of dark matter?
As Chris has already mentioned, (weak) gravitational lensing does indeed support the fact that dark matter is out there in the universe. (Note that lensing will never confirm the existence, though, since it relies on our model of gravity being completely correct: the same model that requires the existence of dark matter). As to where you can read specifically on gravitational lensing; well, there are obviously many, many sites on the internet containing such information. A quick google search gave me this http://astro.berkeley.edu/~jcohn/lens.html, but try searching for yourself for more. As a rule of thumb, a website ending .edu (or .ac.uk) are university webpages, and so are more likely to provide correct information than .com or other websites. (Obviously, there are lots of exceptions, but this is a general guide).

Of course there are other ways in which one may detect dark matter particles. One such (newish) method is through so called "direct detection," which basically says that if the dark matter consists of some unknown particles, then the Earth will be moving through these particles as it moves through the dark matter halo of the galaxy. Thus, one would expect to be able to measure the recoils of other particles due to these dark particles.

That is just for one possible explanation of dark matter particle. There are many more and, of course, there are people who modify gravity so as not to need dark matter, but they are not for discussion in this topic, since I've already gone a way off topic already!
 
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  • #6
Thanks

Thanks Chris and Christo I knew you guys would have the answers. I am not a college student working on a project I am just curious about this interesting subject of Dark Matter. Thanks for the Info I will check the links you provided.
 

1. What is gravitational lensing?

Gravitational lensing is a phenomenon in which the path of light is bent by the presence of a massive object, such as a galaxy or cluster of galaxies. This bending of light can create distorted or magnified images of more distant objects behind the massive object.

2. How does gravitational lensing provide evidence for dark matter?

Gravitational lensing can reveal the presence of dark matter because the amount of bending in the light's path is greater than what can be accounted for by the visible matter in the massive object. This indicates the presence of an invisible, massive substance, such as dark matter, that is responsible for the additional gravitational pull.

3. What is the relationship between dark matter and gravitational lensing?

Dark matter is thought to make up a significant portion of the total mass in the universe. Its presence is needed to explain the gravitational effects observed in gravitational lensing. Without dark matter, the bending of light would not be as significant, and the observed distortions and magnifications would not be possible.

4. Can gravitational lensing be used to study dark matter?

Yes, gravitational lensing is a powerful tool for studying dark matter. By analyzing the distortions and magnifications in the lensed images, scientists can map the distribution of dark matter in the universe and gain a better understanding of its properties and behavior.

5. How does the amount of dark matter in a galaxy affect gravitational lensing?

The amount of dark matter in a galaxy has a direct impact on the strength of gravitational lensing. The more dark matter present, the stronger the gravitational pull and the greater the bending of light. This means that galaxies with higher amounts of dark matter will produce more dramatic lensing effects.

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