Unveiling the Mysteries of Dark Matter

In summary: I think I understand what you're asking now. Yes, I think I might have a couple more questions.Thanks for the link.In summary, dark matter is a hypothesized form of matter that does not interact with other forms of matter and is not visible to the naked eye. There is mounting evidence that dark matter exists, and scientists are still trying to figure out what it is and how it works.
  • #1
Manraj singh
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What proof do we have that dark matter exists.
 
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  • #2
Why don't you just Google dark matter, or look it up in Wikipedia.
 
  • #3
Oh well, thanks for that.
 
  • #4
Manraj singh said:
Oh well, thanks for that.

The moral of the story here is that, there is no reason to ask a question cold in this day and age. You need to first put in some effort to learn things on your own, and then seek help when you encounter a problem. Question such as this, when it can easily be researched online, just shows lack of effort.

Zz.
 
  • #6
adianamonet said:
He may have researched it, but just didn't understand it.
He didn't say that!
 
  • #7
Lol. No he didn't say that, but that could be a possibility to why he asked this question. The answers that he were given sounded a little mean. That's all.
 
  • #8
It's not unreasonable to expect a question that reflects a high school level of knowledge on PF.
 
  • #9
Thank you for the link.
 
  • #10
Manraj singh said:
Thank you for the link.

No problem
 
  • #12
Manraj singh said:
What proof do we have that dark matter exists.

Hi Manraj, welcome to PF! I think you said in another thread that your basis for gaining understanding of interesting questions like this is your 10th grade physics textbook. This is a really good question to be asking at this stage!

The challenge for us other PF members is basically to go through a summary like the one Drakkith linked to, and interpret in simple everyday language--explain the basic physics content.
Here is what he linked
http://en.wikipedia.org/wiki/Dark_matter#Observational_evidence
Wikipedia's Dark Matter article section on Observational evidence:

3 Observational evidence
3.1 Galaxy rotation curves
3.2 Velocity dispersions of galaxies
3.3 Galaxy clusters and gravitational lensing
3.4 Cosmic microwave background
3.5 Sky surveys and baryon acoustic oscillations
3.6 Type Ia supernovae distance measurements
3.7 Lyman-alpha forest
3.8 Structure formation

When I looked at some other questions you asked (as say 16 year old interested in physics) in other posts you struck me as probably pretty quick-witted (excuse the personal comment, hope not impolite) so I am wondering WHICH OF THOSE POINTS do you already understand and which would you like to have discussed?

Personally I find points 3.3 and 3.8 the most fascinating. 3.3 is about GRAVITATIONAL LENSING. If there is a massive object like a cluster of galaxies in the foreground then light rays coming from sample objects in the background are bent and we can estimate the foreground object MASS from how the background is distorted.
In particular 3.3 is about WEAK lensing which actually allows to make contour maps of varying density the DM clouds in the foreground. Weak lensing is fascinating type of shape distortion. round circular outlines tend to be flattened into ovals where the flattening is in the direction of increased density. So that STATISTICALLY you get more oval galaxies than you expect with their short width aligned towards the center of the invisible cloud and their longways axis more aligned tangentially along the "circumference" of the extra dense region.

The computer analysis that goes into the construction of these weak lensing density maps may use the silhouette outline images of on the order of a hundred background galaxies. It is a great achievement. A famous case was published in 2006 and analyzed the DM density map resulting from a collision of two CLUSTERS of galaxies---the so-called "Bullet Cluster".

I guess you need to tell us what of these 8 points of evidence you want to have some discussion of. I personally feel I have some intuition about some: like 3.1, 3.2, 3.3 and 3.8, and NOT on some of the others.
 
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  • #13
btw Manraj, I checked back on the question threads you started, since you joined PF two weeks ago:
https://www.physicsforums.com/search.php?searchid=4037179 [Broken]

Have to say congratulations, seriously. It is a pretty good list of questions, and you got answers to several of them. That's good for PF, I think, and good for the people who took the trouble to think thru how to explain the answer to an interested 10-grader. So thanks for keeping folks on their toes :biggrin:

I especially liked your question about GRAVITATIONAL REDSHIFT, or gravitational time dilation. You were asking why a clock that it is deeper down in a gravitational potential well run slower.
https://www.physicsforums.com/showthread.php?t=737197
Why does a clock that is higher up or essentially out of the well run faster (other things being equal)?

There is a pretty good Wikipedia discussion of that in the article on "gravitational redshift"

http://en.wikipedia.org/wiki/Gravitational_redshift

Why don't you have a look and see if you have further questions? It should begin to clarify why something down near the event horizon of a black hole seems to a distant observer to be moving very slowly (basically it is the difference between the two clock rates: the high versus the low).
 
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  • #14
Thanks a lot, Marcus!
 
  • #15
Manraj singh said:
Thanks a lot, Marcus!

My pleasure, Manraj!
BTW I have no reliable idea about what you can or can't understand. You said you are using a 10th grade physics textbook. You might be a 16 year-old learning basic physics at 10th grade level or you might be a 40-year old sea captain who just happened to pick up a high school textbook to read through as a review.

I'm a little worried I might be talking "over your head" or giving you links to stuff that is too dense and technical to be helpful. You had better say if something is too much to read or over your head.
And let people know if some explanation is at the right level and IS actually helpful.

BTW have you heard of something called the "equivalence principle" in GR? You imagine an physicist in a box doing experiments (say with pendulums or springs or gyroscopes, whatever).
The idea is he can't tell whether the box is in a uniform gravitational field (approximatey as if resting on the surface of a large planet, but even more uniform) or whether the box is way out in intergalactic space being steadily ACCELERATED by some means.

The equivalence principle could be related to what you were asking about in the other thread (the upstairs clock runs faster than the downstairs clock: gravitational redshift or "time dilation").

Or, if the box is out in "zero gravity" space being accelerated, the clock in the front end of the box runs faster than the clock in the rear of the box.
 
  • #16
Btw, since you ask, i am a fourteen year old who just happens to be really interested in physics.Sent from my iPad using Physics Forums
 
  • #17
Manraj singh said:
Btw, since you ask, i am a fourteen year old who just happens to be really interested in physics...

OK. Well please let me know if you have met the "equivalence principle" in any of your reading about relativity. I think it comes up in a lot of popular non-technical accounts. People draw cartoons to illustrate it etc etc.

It's one of these "thought experiment" things. The guy can't tell the difference between the box being uniformly steadily accelerated and the box sitting in a uniform gravitational field.

So suppose the box is being constantly accelerated and there are two guys, one in the front end and one in the back. They have lasers and they send each other light. Can you see why the guy in the back sees the front-guy's light slightly blue-shifted?

Because the light takes a moment to travel and during that time the back-guy is moving faster and "coming to meet the light". And the front guy sees the back guy's light slightly red-shifted because due to the slight acceleration of the box (during the time the light was traveling) he is "backing away from the light".

If the box were moving at constant speed then there wouldn't be any effect. It is the acceleration (while the light is traveling between them) that does it.

Does that make sense?

So then stop the box and put it on a large planet so there's a uniform gravitational field.
the front guy becomes the "upstairs" guy. He send some light downstairs and when it gets there it is BLUE SHIFTED. (IT HAS TO BE BECAUSE OF THE EQUIVALENCE PRINCIPLE because it has to be just the same as when they were out in space with the box being accelerated)

And when the downstairs guy sends some light upstairs the guy up there will detect that it has beens slightly redshifted. By climbing up the gravitational field, or up out of the potential well, or however you think of it.

I'm curious to know if that makes sense to you. If you assume the equivalence principle, then does it make the gravitational redshift (which has been checked experimentally) acceptable?
And might you have already met with this in some of your earlier reading?
 
  • #18
You know that actually made a lot of sense to me. I've learned a lot in the past 2 hours. Thanks for all the information. And since you were asking, i hadn't read about the equivalence principle before. But i had read something similar in Stephen Hawking's 'Theory of everything.'Sent from my iPad using Physics Forums
 
  • #19
Manraj singh said:
You know that actually made a lot of sense to me. I've learned a lot in the past 2 hours...

Good. The wikipedia article I think you said was helpful was

http://en.wikipedia.org/wiki/Gravitational_redshift

You could also look at the wiki on "Gravitational time dilation". I think of G-redshift and G-timeslowing as the same phenomenon. So the two articles are both about the same thing! But I only linked to the G-redshift article because I thought it was better written, more complete and understandable.

The downstairs light looks redder to the upstairs guy, and it actually is redder, to the receptors in his eyes and the atoms in his instruments, because it was made by downstairs atoms which were vibrating slower. The same atoms would vibrate faster upstairs with him. Natural processes actually happen at different rates depending on how deep you are in a gravitational potential well. This is kind of amazing!

BTW I've been trying to understand a new model of black holes called "planck star" which depends crucially on this timeslowing or "time dilation". A new model is something to be approached at your own risk, and with caution. But I think it is interesting. The collapse of a star actually turns into a BOUNCE but we don't see the explosion because it is way in the distant future.

From the star's point of view the collapse and rebound is very quick, measured in seconds or fractions of a second. But because the collapse creates extreme density in its own self-made deep deep gravitational potential well, there is extreme time dilation. So what happens in one second (for an imaginary clock if one could ride through the collapse and bounce) would take billions of years if timed by distant clock. Collapse, seen by distant observer and timed by his clock, can actually be a "self-slowing" physical process because it creates such extreme density.

That's enough about that! It's a new idea, just being worked out. Hence risky.
==================

BTW you can get from the idea of gravitational timeslowing to the idea of gravitational light bending! You have some idea how a convex lens focuses light? thicker in the middle, and light goes slower in glass, so wavefronts advance in smaller steps in the middle. So light rays are bent towards the middle and come together in a focus?

So when light passes close by a massive object like the sun it travels for a short time in a region where time is dilated, where physical processes happen a bit slower. Lightrays are bent in, as if by a lens. Well, the outer ring of a lens, the star itself blocks the central portion of the gravitational "lens".

That is the connection with DARK MATTER. We see clouds of dark matter by their gravitational lensing effect on items in the background. And the lensing or light bending can be explained by time going slower in regions deeper down in a gravitational potential well (near a massive body or a comparatively dense cloud of DM)
 
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  • #20
Thanks, Mr genius. In fact i just have a test coming up on refraction of light through lenses. I guess we have had enough of time dilation for now!
 
  • #21
Manraj singh said:
Thanks, Mr genius. In fact i just have a test coming up on refraction of light through lenses. I guess we have had enough of time dilation for now!
For future reference, "marcus" would be OK if you want (I don't require a "Mr"). Best wishes as to the optics test.
 
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  • #22
When there are professionals/scholars available with expertise on a question like this one, perhaps the useful response is to redirect the question to one of interest to the professional and thus useful for the poster. In this case, the response might be, we have ample evidence that dark matter exists; the interesting question now has become*, what is dark matter, exactly? Here are some theories ...

*This may not be the case; I don't know.
 
  • #23
mheslep said:
... In this case, the response might be, we have ample evidence that dark matter exists; the interesting question now has become*, what is dark matter, exactly? Here are some theories ...

*This may not be the case; I don't know.

I think that's right. In any case I've gotten the impression lately that that's where things are going.
Which theory is currently attracting the most research attention will naturally change. Alternative ideas as to the makeup of dark matter attract interest, then experiments are designed to detect whatever it is, after a while it is seen that they aren't panning out, interest moves on to some other alternative.

Currently an idea that is the most or one of the most popular is a type of neutrino that is weak-force UNREACTIVE otherwise known as "sterile".

A 3.55 keV gamma ray "line" (more of a little bump or wart) was recently detected in the gamma ray background. It was conjectured that there might be a sterile neutrino with mass 7 keV that would decay into two gamma ray photons flying off in opposite directions.

The standard model of particle physics (which is otherwise fairly complete looking) has a GAP or empty row where a different type of neutrino could fit, making the picture look more finished and regular. So there is room for a sterile neutrino type---three slots actually, looking like they are just waiting for sterile neutrinos to be detected. So that has people interested, at present. And it might pan out!

Maxim Markevitch (a prominent Xray astronomer) was one of the authors. Probably if you google, or do an arxiv search, e.g. "markevitch, emission line" you will probably get their recent paper.
http://arxiv.org/abs/1402.2301
Detection of An Unidentified Emission Line in the Stacked X-ray spectrum of Galaxy Clusters
Esra Bulbul, Maxim Markevitch, Adam Foster, Randall K. Smith, Michael Loewenstein, Scott W. Randall
(Submitted on 10 Feb 2014)
We detect a weak unidentified emission line at E=(3.55-3.57)+/-0.03 keV in a stacked XMM spectrum of 73 galaxy clusters spanning a redshift range 0.01-0.35….

A cautious skeptical response was, for example, here:
http://resonaances.blogspot.com/2014/02/signal-of-neutrino-dark-matter.html
 
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  • #24
I'm optimistic about the sterile neutrino, and could also explain baryon asymmetry and neutrino oscillations - which is interesting. It also looks like a natural extension to the standard model that does not require a massive paradigm shift. I anticipate a flood of papers on this over the next year or two. It might even influence the next cycle of LHC research, as these energy ranges are well within LHC capabilities. This could prove an enormous boon to the legacy of LHC and future research initiatives. We live in exciting times.
 
  • #25
Chronos said:
I'm optimistic about the sterile neutrino, and could also explain baryon asymmetry and neutrino oscillations - which is interesting. It also looks like a natural extension to the standard model that does not require a massive paradigm shift. I anticipate a flood of papers on this over the next year or two. It might even influence the next cycle of LHC research, as these energy ranges are well within LHC capabilities. This could prove an enormous boon to the legacy of LHC and future research initiatives. We live in exciting times.

Good work assembling several relevant papers and focusing our attention on this, Chronos!
Your "direct detection" thread is especially helpful. I don't know whether we have a link to it in this thread of Manraj's, if not here it is:
https://www.physicsforums.com/showthread.php?t=739043
 
  • #26
Chronos said:
I'm optimistic about the sterile neutrino, and could also explain baryon asymmetry and neutrino oscillations - which is interesting. It also looks like a natural extension to the standard model that does not require a massive paradigm shift. I anticipate a flood of papers on this over the next year or two. It might even influence the next cycle of LHC research, as these energy ranges are well within LHC capabilities. This could prove an enormous boon to the legacy of LHC and future research initiatives. We live in exciting times.
If true, then the majority of the mass in the universe consists 7 keV neutrinos? Would we not expect to find this to be the case in some celestial body with which we have long, common experience?
 
  • #27
mheslep said:
If true, then the majority of the mass in the universe consists 7 keV neutrinos? Would we not expect to find this to be the case in some celestial body with which we have long, common experience?
Hi! That's a natural question, if there are these particles why haven't they collected and condensed in orbs like the sun? The answer is interesting.

Being able to radiate excess energy off into space actually helps clouds of stuff condense into more compact orbs.

If something can't interact with the EM field it can't radiate!

Particles can be attracted by a massive body and zoom in but they have no way to lose their kinetic energy so they just zoom on out again. To condense you have to be able to DUMP excess gravitational potential energy so you can settle down into something more compact.

So the question is, *how do you even get CLOUDS?* why isn't DM still as uniformly distributed as in early universe (e.g. as uniform as the CMB)?

That's interesting. I should really let Chronos answer since this is a current interest of his. It has to do with the SLINGSHOT EFFECT coupled with metric EXPANSION.
If particles can interact gravitationally they can transfer energy and some lose KE and settle in while others gain KE and get flung OUT of the cloud. So the cloud can slowly contract while those exiles carrying away excess energy go on a long journey in expanding geometry.

But expansion saps the KE out of stuff. This is subtle. (I understand it's covered in Steven Weinberg's Cosmology text.) When the wanderer catches up to another cloud he may arrive with a speed closer to its average velocity and get trapped. It is analogous to redshift with light which reduces the momentum of the photons. The momentum of other particles (eg. neutrinos) is reduced by expansion as well. It is a beautiful process, anybody should ask about it if it puzzles them.

The bleeding off of excess energy by gravitational interaction coupled with metric expansion is slower and less efficient than what happens with ordinary matter (colliding, heating, radiating). But it is nevertheless effective enough to allow clouds of DM to form around galaxies and in clusters of galaxies.

Still DM remains less localized than ordinary matter.

And I should be mindful that we don't know what species of matter constitute DM. It might consist all or in part of these conjectured 7 keV sterile righthand neutrinos---a type of neutrino that seems to be missing from the standard particle model pattern. Or this recent observation by Maxim Markevitch and friends could be wrong and the 3.5 keV bump might not even be there, or have some other explanation. we all realize this but it doesn't hurt to be reminded.
 
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  • #28
We live in exciting times.
 
  • #29
http://arxiv.org/abs/1402.5837

"The recently discovered X-ray line at about 3.5keV can be explained by sterile neutrino dark matter with mass, ms≃7keV, and the mixing, sin22θ∼10−10. Such sterile neutrino is more long-lived than estimated based on the seesaw formula, which strongly suggests an extra flavor structure in the seesaw sector. We show that one can explain both the small mass and the longevity based on the split flavor mechanism where the breaking of flavor symmetry is tied to the breaking of the B−L symmetry. In a supersymmetric case we find that the 7keV sterile neutrino implies the gravitino mass about 100TeV."


...They're really on to something specially on neutrino oscillation where it flips to such flavors mainly moun type in parity to mass splitting which has the potential to solve the mass problem.
 

1. What is dark matter?

Dark matter is a type of matter that is theorized to exist in the universe, but does not interact with light or other forms of electromagnetic radiation. This means it cannot be seen or detected using traditional methods, making it difficult to study.

2. How do scientists study dark matter?

Scientists study dark matter indirectly by observing its effects on visible matter, such as the gravitational pull it exerts on stars and galaxies. They also use advanced technologies, such as telescopes and particle detectors, to try to detect and measure it.

3. What is the current understanding of dark matter?

The current understanding of dark matter is that it makes up about 85% of the matter in the universe, while visible matter only makes up about 15%. However, its exact composition and properties are still unknown, making it a topic of ongoing research and debate.

4. What are some potential explanations for dark matter?

Some potential explanations for dark matter include the existence of undiscovered particles, modifications to the laws of gravity, or a combination of both. These theories are being tested and refined through ongoing scientific research.

5. Why is studying dark matter important?

Studying dark matter is important because it can help us better understand the structure and evolution of the universe. It can also provide insights into the fundamental laws of physics and potentially lead to new technologies and discoveries.

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