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Simulation Predicts Clumps of Dark Matter Within Galaxies
Posted by
Soulskill
on Sat Aug 09, 2008 01:03 AM
from the kind-of-like-normal-matter dept.
from the kind-of-like-normal-matter dept.
A team of researchers has simulated the gravitational interaction of dark matter particles over the course of a hypothetical 13.7 billion years. They found that the particles tended to form clumps large enough to assist in the formation of galaxies. The results contradicted observations from previous, smaller studies, but they lent support to an unrelated simulation of how the Milky Way formed. UCSC's press release is also available. Quoting ScienceNews:
"The clumps of dark matter in the simulation have densities that are remarkably similar to densities that a University of California, Irvine research group found when simulating the formation of the Milky Way and its satellite dwarf galaxies, says James Bullock, the astrophysicist who leads the UC-Irvine group and was not involved in the new study. 'This is a remarkable success of the particular model simulated and adds strong support to the idea that the dark matter is made up of particles that are "cold." There are a number of planned experiments aimed at detecting the dark matter that are betting on it being cold, so this is generally good news for the community,' Bullock says. And, [study co-author Piero Madau] notes, larger simulations that might help constrain the nature of dark matter even more are already in the works."
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Simulations Predict Where We Can Find Dark Matter 61 comments
p1234 writes with this excerpt from the Max Planck Institute for Astrophysics:
"Simulations by the Virgo team show how the Milky Way's halo grew through a series of violent collisions and mergers from millions of much smaller clumps that emerged from the Big Bang. ... If Fermi does detect the predicted emission from the Milky Way's smooth inner halo, then it may, if we are lucky, also see gamma-rays from small (and otherwise invisible) clumps of dark matter which happen to lie particularly close to the Sun. ... The largest simulation took 3.5 million processor hours to complete. Volker Springel was responsible for shepherding the calculation through the machine and said: 'At times I thought it would never finish.' Max Planck Director, Professor Simon White, remarked that 'These calculations finally allow us to see what the dark matter distribution should look like near the Sun where we might stand a chance of detecting it.'"
We discussed a related simulation a few months ago.
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Where's the evidence? (Score:4, Interesting)
I doubt this simulation did more than let them see what they wanted to see. "The researchers note that the simulation does not model any forms of normal matter such as stars or planets." Hardly a complete picture they drew.
Why the obsession dark matter? Say with MOND, why are we so scared to think that perhaps Newtonian mechanics aren't quite enough to calculate with on galactic scales? Why do they think MOND is for cranks and crackpots? What of a static non-expanding universe and alternate redshift paradigms? Are they not just as feasible as exotic matter that only interacts gravitationally?
That's a lot of questions, so I'll break it down to one. I'm just curious as to why dark matter is so widely supported, is it merely because breaking the standard model makes physicists too uncomfortable?
Re:Where's the evidence? (Score:5, Informative)
I Am Not A Physicist, but the problem with MOND is that, well, it explains only one problem of gravity or cosmology, rather: galactic rotation. It fails to explain how spectacularly successful tests of general relativity have been. For example, where does MOND predict frame-dragging? Answer: it doesn't.
MOND is what you get when you have a problem posed to amateur mathematicians and physicists, and they answer that problem (galactic rotation) with the simplest solution (let's just tweak this equation) without considering the fact that their modified theory is inconsistent with well-established theories that currently exist. MOND does not predict certain things that we see in nature, but this isn't seen by proponents. All the proponents see is, hey, it solves this problem. Well, yes, but it causes a whole lot more that you neglect to mention. Chiefly among those is, pretty much every quirk of relativity.
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Since MOND does revert to GR in high Gravity situations so it will support frame dragging.
Don't confuse MOND and TeVeS. MOND is MOdified Newtonian Dynamics. It doesn't revert to GR or any relativistic theory in high gravity situations; in fact, it grows more different from those theories in strong gravity. TeVeS is a relativistic theory which has MOND as a particular limit (and Newtonian dynamics as another). It probably approaches GR in some other limit (decoupling of the scalar and vector fields?), but whether it agrees with all observations in strong gravity situations is, as you say, unk
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Why crazy to modify the laws if the empirical evidence deviates? I'd say that's a damn good reason to modify the laws.
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Yet empirical evidence says this is wrong, by a large factor. If there is an explanation that breaks what we know of as matter it should be condemned, not encouraged.
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And when the analysis is wrong, we cling to the old models and advance fabrications as science? I think not. A single iota of evidence has never been forthcoming from the dark matter camp. Innuendo passes for affirmation. Please, all I asked for initially was a validation of dark matter theory in any way, and none has been forthcoming. Modifying the laws seems the only logical avenue.
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First I want to clarify what dark matter is. It is just matter that cannot be seen directly, because it does not emmit light or radiation. But it can be observed by the gravitational effects it has on objects that can be seen. To an alien Saturn would be dark matter. Earth would be dark matter.
So we have two options:
1. We assume that our planets are the only ones in the universe, every other matter is light up and we can observe it by its radiations. Then we have to conclude that there is a fundamental erro
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Neither. As I asked initially, why the faith in dark matter? If there is only gravitational influence, where's the lensing?
Re:Where's the evidence? (Score:5, Insightful)
The point is that it's not a strange theoretical solution, but a real, physical deflection of light by a gravitating mass. It is certainly evidence of unseen matter --- were there a cloud of unseen matter, this is exactly the effect it would have on passing light. To attribute it instead to a non-specific flaw in a theory we know *very* well is far more speculative than what you criticize others for.
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Re:Where's the evidence? (Score:5, Insightful)
It's not about being scared - it's about the scope of that theory. Using "stuff falls down" as a theory of gravity works, but only in very specific situations. It's not something you can use as a usable replacement for any of the accepted theories, like GR and Newton.
Talking about scientists being scared of MOND is silly. Especially when you bring in Newtonian mechanics, which have long since been proven to fail in a large number of ways. The reason we still use Newtonian mechanics is that it's "good enough" for most things. Just like "stuff falls down" works great here on Earth, but not so well inside the ISS.
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I guess I should have used 'sacred' instead of 'scared'. It is good enough for things whithin a lightyear or less, but why should what we know about the small scale apply equally to the large scale? It doesn't work the other way round, perhaps there's an AU level quanta effect prevailing, perhaps many things.
The blind dedication to the dark matter cause seems superfluous to the realisation that our local models of physics don't scale galacticaly.
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If you read up on dark matter, you'd realise that it's merely a placeholder. We don't know WHAT it is, we just know it's there.
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The only thing there is an inadequacy among our own models. Nothing more.
Re:Where's the evidence? (Score:5, Informative)
The blind dedication to the dark matter cause seems superfluous to the realisation that our local models of physics don't scale galacticaly.
There is no "blind dedication to dark matter". And in fact, not scaling properly is exactly what's wrong with MOND. If you apply it to galaxies, it doesn't work for cosmology, and so on.
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The first bit is wrong, to understand why it is wrong you need to answer the second bit yourself.
Re:Where's the evidence? (Score:5, Informative)
Say with MOND, why are we so scared to think that perhaps Newtonian mechanics aren't quite enough to calculate with on galactic scales?
Nobody uses MOND for the same reason we don't use epicycles anymore: it's an unnecessary adjustment to an outdated system. Newton is a good approximation for low-speed and low-mass systems, but hasn't been considered perfect during the lifetime of anybody here.
What of a static non-expanding universe and alternate redshift paradigms?
Because it doesn't meet the observations. If you have to throw out everything else that does meet the observations to force fit your pet theory, then you're doing science incorrectly. Also, alternate redshift paradigms? Redshift is a very, very basic thing; it would take a lot of phenomenal evidence to change anything related to it.
I'm just curious as to why dark matter is so widely supported,
Dark matter is supported because it seems likely, fits the data, and doesn't contradict other observations. All it means is that we think there's some more mass out there, and we haven't seen it yet.
is it merely because breaking the standard model makes physicists too uncomfortable?
I get the willies just thinking about it! Or not.
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Our models need to account for 90% more mass than empirical evidence proves exists. This only applies when considering galactic scales. Either our models are wrong, or there is a large mass of hidden matter that violates all the known properties of matter except one.
I believe our models are wrong, and this study is flawed. Don't get the willies, just try to broaden your perspective.
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We actually have a better chance of detecting the exotic particles than the rogue planets, so some people are focusing on that
It's the other way around. Dark matter in the form of brown dwarves and such has actually been detected through gravitational microlensing observations. That's how we know that most of the dark matter isn't brown dwarves and other compact astrophysical bodies; it's there, but there isn't enough of it to explain the necessary gravitational effects.
Re:Where's the evidence? (Score:4, Informative)
Why the obsession dark matter?
How about because MOND completely and utterly fails to describe the Bullet cluster [wikipedia.org]?
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Re:Where's the evidence? (Score:4, Informative)
Dark matter is inferred from a number of observations and calculations, including excess rotation speed of stars around galactic centers, excess speed of members of clusters of galaxies, and lensing of background galaxies not associated with luminous matter. While one may fiddle with MOND to possibly fit the first two phenomena (for a specific case, moreover --- one adjustment to Newton's laws had better account for *all* rotation curves), the last group of observations really seem to argue strongly against any reasonable form of MOND.
If you google the Bullet Cluster image and description, you'll note that the blue region (most lensing of background) is tracing the highest density of matter, where the pink traces the density of luminous (here, X-ray cluster gas) matter. It is clear that there is a huge component of matter not identified with luminous matter. To account for this with MOND, it is not enough to increase the *strength* of the gravitational field, but also now the *direction*, since we observe the lensing in a direction roughly perpendicular to the axis of the cluster. Writing down such a gravitational law to account for this case would make any astrophysicist uncomfortable indeed.
Now, especially since we can work backwards and calculate the distribution of dark matter needed to cause each observation, dark matter seems to be the *much* simpler explanation. Besides, we already have examples of matter that interact only gravitationally (and possibly weakly) --- neutrinos. As hard as it is to detect them, there may well be others we don't know about yet.
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Re:Where's the evidence? (Score:5, Informative)
Say with MOND, why are we so scared to think that perhaps Newtonian mechanics aren't quite enough to calculate with on galactic scales? Why do they think MOND is for cranks and crackpots?
Who's this "they"? There is a really unpleasant meme running around Slashdot that reactionary scientists scorn and mock anything that isn't mainstream. In reality, MOND is not a mainstream theory (and for good reason), but it's still discussed seriously. Google around for Sean Carroll's presentation a year or two ago on MOND vs. dark matter (can't remember when that was when he was at U. Chicago or Caltech). This [cosmicvariance.com] is a good summary of his for why dark matter is likely to exist.
What of a static non-expanding universe and alternate redshift paradigms? Are they not just as feasible as exotic matter that only interacts gravitationally?
No, not even remotely. They are vastly less plausible than even MOND, which has problems of its own. But since this is about dark matter and its competitors, I'll stick to those.
I'm just curious as to why dark matter is so widely supported, is it merely because breaking the standard model makes physicists too uncomfortable?
Yeah, it's because theoretical physicists hate new theories. No theoretical physicist ever got fame and tenure by coming up with a new theory. They gotta stick to the old ones to survive.
Seriously, tone down the paranoia. Dark matter also breaks the Standard Model by introducing new kinds of particles. (Well, unless you think it's axions, which are arguably part of the Standard Model). It's not like nobody has ever thought of an alternative gravity theory before. You can carpet a small moon with all the alternative gravity theories out there; scalar-tensor gravity, vector-tensor gravity, conformal gravity, chiral gravity, supergravity, and so on.
The simple facts are that it's really hard to muck around with gravity in a way that simultaneously agrees with observations on tabletop, stellar, planetary system, galactic, and cosmological scales. With MOND it's easy to reproduce galactic rotation curves, but not much else. MOND also contradicts relativity; it's strictly Newtonian. There has been an attempt to correct that in the form of TeVeS (tensor-vector-scalar gravity). But TeVeS requires you to introduce two new gravitational fields, plus couple them together in just the right way, and even then it's far from certain whether it can explain dark matter evidence on all different scales (galaxies, clusters, cosmology, etc.). Furthermore MOND has difficulty explaining rather direct evidence of dark matter like the Bullet Cluster. Even if MOND is correct, it seems likely that you still need dark matter to explain everything.
After all that, MOND looks far more ad hoc than just postulating the existence of a new kind of particle, especially since most of the new particle theories out there predict some kind of dark-matter like particle anyway for completely independent reasons. It's not like weakly interacting particles are terribly bizarre in the first place; neutrinos are dark matter, although they're too light to be most of the dark matter. The main difference between most of the dark matter and neutrinos is mass, and what's so odd something weak like a neutrino, only heavier? Such a particle, predicted by many theories, can (unlike MOND) simultaneously explain all the astrophysical phenomena which point towards dark matter.
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Well Bullet Cluster or any other cluster is a problem for MOND. But the Bullet Cluster is also a problem for Dark Matter. The velocity of the Cluster is much faster than GR can provide, which MOND can easily handle.
(GR doesn't have anything to do with it per se; Newtonian gravity predicts the same thing as GR on galactic scales.)
The Bullet Cluster is a much more severe problem for MOND than dark matter; you can't even qualitatively explain the divergence between the galaxy and the lensing with MOND. The Brownstein and Moffat paper you're alluding do doesn't even attempt to address that elephant in the room, which is the problem with MOND and the Bullet Cluster by far. I've also read comments on Cosmic Variance that
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The Standard Model arguably includes axions, which were postulated to solve the strong-CP problem in quantum chromodynamics. They are dark matter candidates (although I think astrophysical constrains favor SUSY.) However, like the Higgs boson, they have not yet been observed.
Have we found them? (Score:2, Funny)
Slightly off topic: Dyson Spheres (Score:3, Interesting)
Re:Slightly off topic: Dyson Spheres (Score:5, Informative)
That is a "MACHO," which we have looked for and not seen enough of. MACHOs are unique in that they affect the light behind them (they are opaque and gravitationally lensing) and so while they could account for a lot of matter, we aren't seeing enough lensing and enough holes in the spectrum from "dark stars", areas where the sky is darker from an object blocking light behind it.
And back of the envelope calculations say a dyson sphere wouldn't be anywhere near a black hole's mass, which is what we really would need to find quite a few of in order to find the missing mass.
And this ignores any technical difficulties with actually constructing a dyson sphere.
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Cosmic Smog? (Score:2, Interesting)
It would certainly be interesting if dark matter turned out to be some kind of pollution from advanced civilizations.
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Not really, dark matter isn't black matter hiding light. It's only called "dark" in a metaphorical sense.
Signs of it has been seen as being completely transparent and the only real visible sign of it being there thanks to it bending light due to gravitational lensing.
Kahn was right! (Score:3, Informative)
ha (Score:2, Insightful)
More cruft to add to the bogus hypothesis that is dark matter.
I am a physicist.
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Gravity from "elsewhere"? (Score:3, Interesting)
For some time, I've been making random notes from articles relating to dark matter, string theory and quantum entanglement. I've been trying to form a hypothesis of dark matter with information from all of these three.
Interestingly, this article has now given a lot more focus to one part of the idea that was forming that was a bit "wishy-washy" before (okay, it's still very wishy-washy, but less so now).
The overall concept is basically along the lines of quantum entanglement being a property of the fact that two entangled particles are in fact just ONE string that's being bent through space in some rather unconventional ways (extra dimensions neither being "large and flat" nor "very very small and coiled", but rather "hideously complex monstrous things").
This, combined with gravity ("graviton"strings) being freely able to travel through those dimensions rather than tied to an endpoint (hence appearing much weaker than the other forces, even though ALL forces have absolutely identical strength (another wild-ass guess, just because it would be "nice")) would lead us to an elegant idea about dark matter actually being gravity from perfectly normal matter that happens to be showing up in unexpected places.
The fact that there are clumps of it definitely does not blow my ideas out of the water, but it does mean I need to re-work my idea of "hideously complex monstrous things" for the extra dimensions as I was assuming dark matter showed up "generally" in areas with other matter rather than specific clumps as "normal" does. It needs to be more structured than I had been thinking for a clump of matter in one place to form a "clump of dark matter" (e.g. the gravitational effect seen) elsewhere. That's actually a good thing though, because any structure lent to the process makes it closer to a testable hypothesis (anything completely unstructured could never become one, and having "no real clue" about the structure as I was, made it far too vague.)
Note that this is still a very early infancy idea, and is somewhat around the "wild guess" point rather than even "hypothesis", so I'd be quite happy for people to comment on this - can anyone blow me completely out of the water on this line of thinking? Or can anyone offer ideas that support it? Or even just expand it a little? Does anyone know of any other research along these lines that I could read?
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My beginnings of a hypothesis are that it's gravity from THIS universe from folded dimensions. "Parallel Universe", while possible, seems to require too many further assumptions.
Fun, yes. False, almost certainly, but not necessarily - that's the point of trying to formulate a hypothesis.
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On large scales, physics is pretty classical
Other than the large amount of seemingly "dark matter"...
entanglement just isn't that relevant on cosmological scales
Certainly true, but I wasn't really implying it needs to be. If we have a pair of entangled particles, they can THEN be separated by (apparently) quite any distance in classical space and nevertheless remain entangled. We haven't found a good way to use this as "faster than light communication", and there are very strong arguments that it can't be, however it seems to remain fact that these particles are somehow "connected" despite being physically
Re:Gravity from "elsewhere"? (Score:4, Informative)
Other than the large amount of seemingly "dark matter"...
There's nothing non-classical (i.e., quantum) about the behavior of dark matter. At least nothing we've observed so far. It's just matter, maybe like a neutrino but heavier. You don't need to appeal to quantum entanglement or anything exotic to explain it.
If we have a pair of entangled particles, they can THEN be separated by (apparently) quite any distance in classical space and nevertheless remain entangled.
In theory, yes. In practice, they need to be extremely isolated from everything else in the universe to remain entangled. That's why it's so difficult to maintain long-range entanglement for purposes like quantum encryption. You may think space is "empty", but it just takes a single photon to ruin the entanglement.
This is why my hypothesis considers that they may actually not be physically separate at all - they are "right beside each other" through twisted "extra" dimensions, just in some way that we currently do not have the ability to measure or understand particularly well.
Now you're mixing up two different ideas, quantum mechanics and extra dimensions. If they're interacting through other dimensions, fine, but you don't need entanglement to explain that either.
This leads on to the idea of "dark matter" being gravity from "nearby" objects that are classically quite distant, but in reality quite "close".
All the above problems notwithstanding, it's easy to come up with more. Even if you ignore the fact that these particles can't plausibly remain entangled, you have to explain how all these distant particles got entangled with each other in the first place. (If you're tempted to say "the Big Bang", you really can't ignore the previous fact given the extreme temperatures involved. Maintaining entanglement requires no outside interaction with other particles at any time over the intervening 14 billion years.) Furthermore, entangled particles interact with each other, but that interaction in general doesn't look anything like the vector or tensor field theories that give rise to what we think of as "forces" such as gravity or electromagnetism. (Why should this purported "entanglement force" act like gravity anyway?) And there's no explanation for the astrophysical observations like how entanglement with distant particles can simulate the effects of a spherical cloud of dark matter enclosing a disc galaxy.
Basically, it seems like a very bizarre hypotheses that, all the physical evidence against it aside, doesn't even seem to have much to commend it over the alternatives. It's not like the idea of there being weakly interacting particles out there is so crazy; plenty of particle theories predict them for completely independent reasons including possibly the Standard Model, and there are other weakly interacting (though less massive) particles out there already, like neutrinos.
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How can they similate the unknown ? (Score:2)
Earth collisions? (Score:2)
So now do we need to worry about dark matter colliding with Earth? Can't this stuff be detected by looking at areas where the cosmic background radiation is lower than usual? I suppose if it were moving it would have some sort of heat signature to it...
My God, it's full of -- dark matter! (Score:2)
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Re:And in other simulations: (Score:5, Funny)
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Perhaps both dark matter and an aether exist due to quantum foam, isn't that one of the hypotheses?
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If only you could do the equivalent of Michelson-Morley_experiment [wikipedia.org], and save everybody a lot of trouble... Now we're stuck doing these other simulations and experiments trying to find something you know will not be found.
Re:Dark matter particles are cold? (Score:5, Informative)
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That doesn't reason at all unless you find that dark matter can undertake complex interactions with other dark matter. It's more likely that it can't interact with itself much at all except through gravitation.