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Necessity of Dark Energy Questioned
Posted by
Soulskill
on Sat Dec 29, 2007 11:21 AM
from the furphy-is-the-word-of-the-day dept.
from the furphy-is-the-word-of-the-day dept.
ttnuagmada points us to an article about scientist David Wiltshire's suggestion that theorized dark energy is not needed to describe the expansion of the universe. His work challenges assumptions made about the distribution of matter in the universe. Early solutions to general relativity were based on a "smooth distribution" of matter. Wiltshire's approach focuses on a "lumpy" dispersal, which more accurately fits data from modern studies. We have discussed other theories about dark energy in the past. Quoting:
"Through observational projects like the Sloan Digital Sky Survey and the 2 Degree Field survey, we now have a much better picture of the large-scale structure of the universe and we know that galaxies are not uniformly distributed. 'Rather, they are in clusters sprinkled thinly in filaments and "bubble walls" surrounding huge voids hundreds of millions of light-years across,' Wiltshire says.
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Dark Energy May Lurk In Hidden Dimensions 164 comments
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Skeptical (Score:3, Interesting)
Re:Skeptical (Score:4, Interesting)
Parent
Re:Skeptical (Score:4, Interesting)
While we might not ever know who is correct in this regard, I tend to prefer theories that don't have the need for dark energies, or matter,even if that really really screws up the equations we use to model the early universe. I think at some point every physicist just stares at a black board somewhere and says to himself " thats fucked up". We really have lost the elegance of the universe being a series of spherical shells rotating around the earth. Since that point we've managed to go through cycles of discovering elegance in the universe on a deeper level (the simple math of kepplar and Newton), and having to reject it for more complexity( Einstien's huge matrix of PDE's ). Let this be a lesson to us all, Don't let what should be prevent you from seeing what is.
Parent
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> than an earlier smooth distribution they've been assuming.
The assumption of uniformity was an approximation intended to ease computation. The lumpiness has to have always been there or it would not be there now. It is postulated that it originated as quantum fluctations in the inflaton field.
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The math might get harder, but the conception has gotten
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I started making pancakes and after I stirred the batter I noticed it was quite lumpy.
I thought,"Eureka!, these same constants in my pancake batter help me better to understand the expansion of the universe!"
Why it's so lumpy and not smooth at all... you would need to stir the universe for a billion or two more years before it's smooth.
That my friends, is generally how
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Still that does not prove that the "ether" either exists or doesn't exist. Just that it is not necessary to incorporate into a mathematical model, that will more or less express what is observed. But we still have the question of "zero point
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Meanwhile, on the Neutral Planet (Score:5, Funny)
I need my dark energy (Score:4, Funny)
Relatively readable survey of solution approaches (Score:5, Informative)
Re:Relatively readable survey of solution approach (Score:3, Informative)
from the article
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Of course not. I mean, she draws them because her boss says she has to. But use them? That'd be like ... like ... That'd be like reading the spec before doing the creative work.
Can someone please explain? (Score:5, Informative)
I did some googling and found David Wiltshire's home page [canterbury.ac.nz] which had links to his recent publications [canterbury.ac.nz]. That brought me to this full article [iop.org] which I am guessing is the one that corresponds to what was discussed in the original /. article here.
I had a couple courses in astronomy and cosmology way back in my college days. That said, I can't begin to understand the details. I'm hoping someone with more knowledge and experience could elaborate. Is he really onto something that can dispense with the need for dark energy? And, if he is, am I correct in thinking this would be Nobel-Prize-Candidate-Worthy?
Re:Can someone please explain? (Score:5, Informative)
Here's the slightly more condensed version of this story. Einstein's theory of General Relativity (GR), which incidentally should the Law of GR by today's standards, gives a large set of differential equations to be solved. When this was first being applied to Cosmology in the 1920's, some basic assumptions about the universe had to made in order to solve the GR equations: it is isotropic (same in all directions), and homogeneous (uniform everywhere). They were primarily made for two reasons: mathematical expediency (this is the simplest sort of non-trivial universe you can have), and this didn't conflict with any observations at the time. Solving the GR equations with these assumptions gives fairly simple equations for the time evolution of the universe, leading to the standard model of Cosmology (called the Lambda-CDM model).
As you would imagine, we have vastly more astronomical data now then we did in the 20's. To explain what we observe now, particularly the cosmic microwave background data, with these evolution equations we need to include a constant expansion term. This expansion would have to be from something uniformly distributed throughout the universe with negative pressure (very reminiscent of phlogiston, isn't it?) which we call "Dark Energy". So, based on current data and using the standard model to explain certain properties of the universe, it must consist of around 73% dark energy. Considering that this is the bulk of the universe and that, other than negative pressure, we have no idea what dark energy is or what it's properties are, this leads to a scientifically troubling state of affairs.
However, modern sky surveys show that the universe is neither isotropic nor homogeneous. Instead there is a tendency towards a bubble-like structure with large empty spaces surrounded by thin "filaments" of galaxies. Even still, the standard model which requires dark energy ignores these differences. So, Wiltshire's contribution is to replace the standard assumptions with this "bubble" model, re-solve the GR equations, and get new equations for the evolution of universe based on it's *observed structure*, not some simplified model. In his new equations, dark energy is completely unnecessary. Since the structure of these "bubbles" is so large, fits to the data with Wiltshire's model are statistically just as good (actually indistinguishable) as the standard model, though as a caveat not all of the calculations have been done. Not only is Wiltshire's model much better from an Occam's Razor standpoint, it may actually solve some mysteries which the standard model cannot explain.
I really can't go any further and still call this a "condensed" version with a straight face. In
Parent
Thank you (Score:2)
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That makes sense, but (Score:5, Insightful)
Parent
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> spacetime, and that's what we see as gravity etc. So what is the actual "fabric" made of?
Strained analogies.
Mini-Inflation events in Voids (Score:3, Interesting)
Re:Mini-Inflation events in Voids (Score:5, Interesting)
Here is the picture I have heard:
The universe basically, from any point, stretches out in all directions. Gravity pulls a given lump in all directions at a given time. But local things are more powerful by the law of gravity, than far things. So things start lumping with their neighbors.
Some lumpings occur earlier than other lumpings, which cause then to exert a stronger pull. These become the super-clusters [wikipedia.org] (joining points between filament; such as the Virgo Cluster. [wikipedia.org])
So masses are basically pulled towards the closest super-cluster. But, ah-hah, some are pulled strongly by *two* super-clusters. These become the filament ("bubble walls.")
If you download Mitaka, [nao.ac.jp] you can see a lot of these things first hand, with data directly from the Sloan Digital Sky Survey. [sdss.org]
Parent
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> a whole - no?
They do, pretty much. Here is a crude, oversimplified summation:
Since there is less matter in the voids than there would be in a homogeneous universe time runs faster in them then it would in a such a universe. Therefor the universe is older seen from the voids and so they seem bigger than they should be. Meantime down here in the matter concentrations where contraction due to gravity dominates
Dark matter balloney (Score:2, Insightful)
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Are you so sure there aren't other spectrum's yet to be discovered? We just might not have the technological know how to detect certain things. Doesn't mean they aren't there.
Take radiation for example. You can't see it, can't taste it, can't feel it and without the proper tools you'd never know you're sitting in it.
Same thing for "dark matter". Yes it could be a bunch of baloney, but its the only thing that
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To date, that is the stupidest thing ever said on slashdot.
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I would compare it to just calling something "X". However, sticking the name "energy" or "matter" onto an unknown may be a bit presumptuous. But frankly, I can't find a better description that rolls off the tongue nicely in popular press science articles. You can't just kee
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Which reduces your argument to "if you can't detect something with light (see it) then it's not there). Well, you can't see any subatomic particles with light!
Now maybe you mean "if you can't detect something through electromagnetic interaction then it's not there." In that case neutrons and neutrinos don't exist either, as they have no charge, just like dark matter.
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No: we can detect gravitational effects we were not expecting. Some people have suggested dark matter as an explanation. You're jumping the gun a bit.
TWW
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Re:Dark matter balloney (Score:5, Informative)
Parent
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So I guess that I should forget all about radioactivity, what with all the weak forces and strong forces that govern subatomic particles rather than light and gravity?
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These procedures are based in experiments and observations, not arcane, complicated math. Physics is NOT equal to math, but math is only a useful tool to describe discoveries and experimental results.
Much of cosmology and astrophysics is pure mathematical fiction, having no basis in the increasing flood of data coming from sophisticated space probes which severely contradicts so
Re:Dark matter balloney (Score:5, Informative)
The shortage of detected solar neutrinos was explained by hypothesizing that neutrinos actually have a very small mass. That would imply that they oscillate between types, only one of which we were detecting. That implies that the shortage is made up by neutrinos of the two other types that we couldn't detect. Now, with better equipment, we've discovered that neutrinos do have some very small mass and everything adds up nicely. Sorry, but that's a TRIUMPH of quantum mechanics, nuclear physics and the standard model, not a failing.
But if you don't like all that math, that's no problem. Please sell or recycle your computer, which is only possible due to all that math.
Parent
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Great Rip? (Score:2)
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KISS (Score:2)
Re:KISS (Score:4, Informative)
If this guy is correct then it's a nice advancement of cosmology. From what's described in the article it appears that at least the sign of the effect in his argument is correct. You hear a LOT of these claims though, that explain one or two observations and conveniently omit a hundred or so others.
And the article is terrible. It sets this up somehow as a battle between this guy and Einstein. Einstein postulated a cosmological constant (the equivalent of dark energy) because he wanted a STATIC universe and then retracted it when Hubble came up with experimental evidence that the universe isn't static at all. Einstein's theories have nothing to do with whether matter is smoothly distributed or not.
Parent
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If that is really the case, I think it is a good example for the gp.
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There I fixed it!
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