Mystery of Dark Energy: Unravelling the GR Expansion of Universe

In summary: Dark Energy is a misnomer, it is only an extra gravitational force that has been misinterpreted as a 'pushing apart' of the universe.In summary, the conversation discusses the expansion of the Universe and how it is predicted by Einstein's theory of General Relativity. The concept of dark energy, a supposed mystical force of repulsion between matter, is brought up and it is explained that it is a result of a constant that Einstein added to his equation. However, there are differing opinions on whether this is the correct explanation for dark energy. Some suggest that it could be a result of strings joined together, while others argue that it is simply an extra gravitational force. There is also discussion about the
  • #1
quasar987
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Another one of the physics teacher working at the college I attended (see my previous post) wrote a book on basic http://universite.deboeck.com/Resources/Titles/28011100266200/Images/28011100266200L.gif [Broken]. In this book it says that the expansion of the Universe is due to the expansion of space itself and that this expansion of space is entirely predicted by Einstein's theory of GR. Now, if this is so, where does the DARK ENERGY (suposedly a MYSTICAL force of repulsion between matter) fit it ?!
 
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  • #2
this dark energy is a result of a constant that Einstein added to his equation. A positive cosmological constant predicts that there must be a sort of anti - gravity in the universe.
 
  • #3
quasar987 said:
Another one of the physics teacher working at the college I attended (see my previous post) wrote a book on basic http://universite.deboeck.com/Resources/Titles/28011100266200/Images/28011100266200L.gif [Broken]. In this book it says that the expansion of the Universe is due to the expansion of space itself and that this expansion of space is entirely predicted by Einstein's theory of GR. Now, if this is so, where does the DARK ENERGY (suposedly a MYSTICAL force of repulsion between matter) fit it ?!

Here's a very brief history of cosmology post-Einstein:

1) Einstein comes up with GR.
2) Einstein proposes a static universe, with a cosmological constant to keep it from collapsing from its own gravity
3) Hubble observes that the universe isn't static, that it's expanding
4) Einstein recans the cosmological constant.
5) Varioius people make more and more observations of the rate of expansion, to compare it with the model predicted by General Relativity, called the Einstein-Friedmann cosmology. The cosmological constant goes in and out of fashion
6) Recent measurements of the rate of expansion put the cosmological constant back "in fashion" again, because certain experimental results are not fitting otherwise. The cosmological constant is given a new popular name, 'dark energy" (which could also include mechanisms that are like Einstein's original cosmological constant in effect, but different in origin).
 
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  • #4
quasar987 said:
Another one of the physics teacher working at the college I attended (see my previous post) wrote a book on basic http://universite.deboeck.com/Resources/Titles/28011100266200/Images/28011100266200L.gif [Broken]. In this book it says that the expansion of the Universe is due to the expansion of space itself and that this expansion of space is entirely predicted by Einstein's theory of GR. Now, if this is so, where does the DARK ENERGY (suposedly a MYSTICAL force of repulsion between matter) fit it ?!

in the einstein equation (1915-1917) the cosmological constant Lambda was just some additional curvature built into space over and above that caused by matter.

we are used to thinking of all the kinds of matter and energy there are in the world being summed up in an overall "energy density" function----some fraction of a joule per cubic meter.

if you know SI metric units you will recognize the unit "joule per cubic meter" as a Pascal (it is the same unit as saying "Newton per square meter")

in the 90 years theyve had the einstein equation people have gotten used to thinking of all curvature (on the LHS of the eqn) as resulting from the Pascals of matter on the RHS of the eqn----the energy density and pressure. that is:"Matter shapes space and the shape tells matter how to flow." (Bingo. Cuckoo. whatever)

the cosmological constant might be some extra curvature on the LHS which is not caused by any matter on the RHS it might just be some intrinsic curvature space was born with.
but this is not the habit.
the habit is to attribute the extra curvature to the presence of some postulated energy which also has a postulated pressure, and which has the observational effects associated with the extra curvature.
we are obliged by 90 years of habit to imagine the existence of dark energy because energy density is where curvature ordinarily comes from

keep skeptical and have fun
 
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  • #5
if you have any interest in dark energy at all then you should get
familiar with the Friedmann equations

they are what cosmologists use instead of the raw Einstein equation
because they are much much easier to work with

and they show the energy density and the pressure explicitly on the RHS

and there should be a link to them, or a post about them, in the
Astronomy Cosmology Reference Sticky at PF General Astronomy forum.
I'll see if i can find it. Otherwise just google Friedmann equation.
 
  • #6
could dark matter be "strings" joined together to become very long and dense hence the reason we can't see them as they are only Planck length wide but anywhere up to infinitely long ?

...dark strings
 
  • #7
RingoKid said:
could dark matter be "strings" joined together to become very long and dense hence the reason we can't see them as they are only Planck length wide but anywhere up to infinitely long ?

...dark strings

Actually this post is about Dark Energy, but no matter, we cannot see Dark Energy or Dark Matter (it is too dark) or 'strings' for that matter (they are too small). Dark Energy and Matter are only observed in the depths of space where the observations are theory dependent. That theory being GR, if the theory changes then the observations will change, or disappear altogether.

Unless we come up with something that actually is observed, not only in the depths of space but also in the laboratory, then perhaps all we are doing is 'adding extra epicycles' to make the standard theory work.

See my post #10 https://www.physicsforums.com/showthread.php?p=284031#post284031
 
  • #8
thanx Garth...

so where do you propose this paradigm will shift to...can any variant of string/brane theory currently account for dark matter or energy, eg a dark string speculation ?

and isn't it true that inflation requires early universe matter to be flung out at speeds exceeding c making it another contradiction of GR ?

cheers
 
  • #9
RingoKid said:
so where do you propose this paradigm will shift to...can any variant of string/brane theory currently account for dark matter or energy, eg a dark string speculation ?

You may be interested in my thread "Self Creation Cosmology - a new gravitational theory" https://www.physicsforums.com/showthread.php?t=32713 because SCC does not require Inflation, unknown Dark Matter or Dark Energy. There is Dark Matter but it is ordinary baryonic matter such as hydrogen and helium, it is dark in the sense of being non-luminous and not being an unknown substance. The theory may or may not stand up but it is falsifiable and is at present about to be tested by the Gravity Probe B satellite.
RingoKid said:
and isn't it true that inflation requires early universe matter to be flung out at speeds exceeding c making it another contradiction of GR ?
No - the restriction on not going faster than light only applies within space-time. Inflation is talking about space-time itself expanding at an enormous rate, objects (not that there were any then!) within space-time would have been carried along with that general expansion. At present with the Hubble flow, or expansion of the universe, the galaxies are not moving within space-time but it is space-time itself which is expanding and we, and everything else, are simply being carried along with it. Distant galaxies beyond our event-horizon are moving away from us at velocities greater than the speed of light, that is why we cannot see them.
 
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  • #10
The thing is, if you look at the http://wc0.worldcrossing.com/WebX?14@174.GuiAcZYuBaw.0@.1ddf4a5f/57 [Broken] as consistant, at what point would this be so?

If you have consider how pearls and chains are formed in a universe that is cooling, and you need some framework in which to comprehend the interlinking capability.

So in the beginning we look at how supersymmetrical states would have existed and how the expansitory universe, would neuronically connect. :smile:

http://astro.uchicago.edu/~andrey/soft/p3d/p3d_evol.gif

http://www.gsfc.nasa.gov/gsfc/spacesci/pictures/20020812gamma/denset.jpg [Broken]

Scharf and Mukherjee's new research compared a catalog of 2,469 galaxy clusters with the Compton database. Using sophisticated statistical techniques, they showed that the sky surrounding the most massive clusters was systematically brighter in gamma rays than other regions.

"The more massive the cluster (and greater the gravitational potential), the brighter the gamma-ray halo," said Mukherjee. "The enhancement observed was very similar to that predicted by the Loeb-Waxman theory

http://www.gsfc.nasa.gov/topstory/20020812gamma.html [Broken]
 
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  • #11
quasar987 said:
Another one of the physics teacher working at the college I attended (see my previous post) wrote a book on basic http://universite.deboeck.com/Resources/Titles/28011100266200/Images/28011100266200L.gif [Broken]. In this book it says that the expansion of the Universe is due to the expansion of space itself and that this expansion of space is entirely predicted by Einstein's theory of GR. Now, if this is so, where does the DARK ENERGY (suposedly a MYSTICAL force of repulsion between matter) fit it ?!
This question is about theory; at least as important - since this is science, arguably more important - is experiment and observation.

AFAIK, there are two classes of observations (no experiments :cry: ) which support 'dark energy', distant supernovae and 'all cosmologically relevant observations'

1) Distant supernovae. Ever since Hubble first published obsevational results which pointed to an expanding universe, astronomers have been keen to characterise that expansion as accurately as possible - over all distance scales, and in all directions. To do this, they need independent measures of both distance and recession speed. The latter is relatively easy to measure, with great precision - the 'redshift' of galaxies and quasars; the former has proven immensely difficult, and only in the last decade has a broad consensus emerged (there is still considerable 'observational error', and there are still some dissenters). Distance can be measured by a number of different types of observations, and the 'distance ladder' is now reasonably well established, out to perhaps as much as 10 billion light years.

While redshifts are relatively easy to measure, their interpretation as 'recession due to the expanding universe' has had its challenges and upsets. Perhaps the biggest was 'http://cow.physics.wisc.edu/~ogelman/guide/gr8a/ [Broken]'; apparently there is an awful lot more mass in the local part of the universe (~100 Mpc) than can be 'seen'.

So, the 'expanding universe' hypothesis predicts that the universe is, and has been, expanding uniformly - in all directions, and at all times (at least, after any inflation ended; observationally we can't directly see any earlier than ~300,000 years after the BB, well after any inflation finished), over sufficiently large chunks of the universe (superclusters have sufficient mass so 'expansion' of objects within a supercluster may be small compared with net gravitational attraction from masses within the supercluster).

What do observations show? The best distance indicator for very distant objects is Type 1a supernovae - we think we understand their behaviour sufficiently well so good observations of their lightcurves can be turned into estimates of distance (this 1998 poster gives more details). Plotting distance against redshift shows that the data are not on the curve predicted by 'uniform expansion' (it's not quite as clear-cut as this; different models of the universe - e.g. with different amounts of dark matter - give different curves, but no model that is consistent with other observational data - e.g. WMAP - goes near the data). What model curves will go through the data? Those in which the rate of expansion of the universe is increasing!

'Dark energy' is the shorthand that is used for whatever might be causing the observed acceleration of the universal expansion.

But not so fast! How can astronomers be so certain that there aren't other effects involved? Initially, quite a bit of work had to be done to nail these down, e.g. do we understand Type 1a SN sufficiently well? what if the distant SN are partly obscurred by dust? and so on. Many of these 'systematic errors' have now been characterised and their effects on the data taken into account. However, some feel that at least an OOM more of good data are needed (http://snap.lbl.gov/ to the rescue?)

2. All 'cosmologically relevant observations': As Garth correctly points out, this is a bit of chicken and egg. Basically, you take all observations that have relevance to cosmology - WMAP and others on the CMBR, large scale structure (e.g. 2dF, SDSS), primordial nuclide abundances, the Hubble relationship, the distant SN data, ... - and see what sort of cosmological model is most consistent with it all. The idea is that there is more than enough data to constrain models, so if the models are wrong, there will be obvious inconsistencies. The good news is that there are models which are consistent with all the data ... but only those which have 'dark energy' in them!

Further reading: Wikipedia
APOD
Snowmass 2001, Yellow Book on Dark Energy
short article - model-independent dark energy
nice, bite-sized physicsweb summary
 
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  • #12
Nereid said:
The good news is that there are models which are consistent with all the data ... but only those which have 'dark energy' in them!

Not quite "only those with Dark energy in them"!

As we have discussed in a previous thread an Indian team, consisting of Gehaut, Lohiya et al., have been looking at the strictly linearly expanding or "freely coasting" universe. It fits exactly all the constraints!

Their papers can be found at:
A Concordant "Freely Coasting Cosmology"
http://arxiv.org/abs/astro-ph/0306448

A "Freely Coasting" Universe
http://arxiv.org/abs/astro-ph/0209209

They say "A strictly linear evolution of the cosmological scale factor is surprisingly an excellent fit to a host of cosmological observations. Any model that can support such a coasting presents itself as a falsifiable model as far as classical cosmological tests are concerned." (Taken from the abstract of the first paper above)

One theory that does indeed "support such a coasting" is SCC - in its Jordan Frame formulation- without requiring Dark Energy. [See my paper "Self Creation Cosmology - An Alternative Gravitational Theory" http://arxiv.org/abs/gr-qc/0405094 (to be published in 'Progress in
General Relativity and Quantum Cosmology Research', Nova Science
Publishers, Inc. New York.)]
 
  • #13
Nereid said:
...
'Dark energy' is the shorthand that is used for whatever might be causing the observed acceleration of the universal expansion.

Hi Nereid, at one time I thought you made a nuanced distinction between
the cosmological constant and dark energy. Does this "whatever might be causing" definition get rid of any earlier distinction you may have made and simply lump the two? I'm not certain I understand why you have dark energy in quotes, and consistently write 'dark energy'. I don't recall your doing this before (perhaps you did and I simply failed to notice). It would be interesting to know if your thinking has been changing about this. Would you care to clarify your own view?
 
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  • #14
Maybe she is softening like Peter Woit? :biggrin: Maybe one day, I will convert you too, Marcus. :rofl:

Oh Marcus, could you correct your quote? :smile:
 
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  • #15
sol2 said:
Maybe he is softening like Peter Woit? :biggrin:

he?

Who do you mean sol?

Nereid is a she. Both she and Peter Woit are crisp thinkers, in my view, and soften rarely. On the other hand, even when you might be joking you have intuitions about people that are worth listening to, so I will consider it a possibility :smile:
 
  • #16
marcus said:
Hi Nereid, at one time I thought you made a nuanced distinction between
the cosmological constant and dark energy. Does this "whatever might be causing" definition get rid of any earlier distinction you may have made and simply lump the two? I'm not certain I understand why you have dark energy in quotes, and consistently write 'dark energy'. I don't recall your doing this before (perhaps you did and I simply failed to notice). It would be interesting to know if your thinking has been changing about this. Would you care to clarify your own view?
Thanks for the clarification marcus!

In these discussions it can be quite difficult to write something brief that also reflects all the major aspects in play ... let alone ALL aspects which can be said to fit (somehow). Garth's post is a good example of this - a cosmological model which the authors claim to be consistent with all the observational data, and one which differs markedly from the 'concordance model' (no doubt there are others out there too ... with relatively weak observational constraints, theoreticians can have the most marvellous fun imaginable :wink:).

From the observational perspective, at the current level of constraint, both a cosmological constant and some kind of 'dark energy' are pretty much indistinguishable, though we are all looking forward to the day when that ceases to be! Since "cosmological constant, 'dark energy', or something else; anyway, whatever gives rise to the observed acceleration of expansion" is anything but shorthand, I think you'll find that 'dark energy' is more convenient :smile: (Of course, when talking 'theory', cc and DE are certainly distinguised!)
 
  • #17
marcus said:
he?

Who do you mean sol?

Nereid is a she. Both she and Peter Woit are crisp thinkers, in my view, and soften rarely. On the other hand, even when you might be joking you have intuitions about people that are worth listening to, so I will consider it a possibility :smile:
Message from the global collective of Nereids, their partners, friends and families: http://members.iquest.net/~jswartz/jks/humor/dog.htm Woof! Woof!

(and no, lady dogs do NOT reveal their breeds :shy: )
 
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  • #18
Nereid said:
(Of course, when talking 'theory', cc and DE are certainly distinguished!)

that's my good old Nereid :smile:


see sol? crispness :tongue:
 
  • #19
marcus said:
he?

Who do you mean sol?

Nereid is a she. Both she and Peter Woit are crisp thinkers, in my view, and soften rarely. On the other hand, even when you might be joking you have intuitions about people that are worth listening to, so I will consider it a possibility :smile:

I made correction Marcus in previous post.

Yes if you cook the bacon to long it can become crisp:)

The very foundational principals have to have a basis in which to move from. I scream loudly scientific verification is the only road too :cry: :cry: and anything less is theoretical speculation. There, I feel better :biggrin:

When one sends out it's tentacles from the mind, it can flop quite freely if you do not have control. So wild speculation would have been loosening a grip to what we have known for certain, and what shakes our foundation.

I often compare it to the view I had of the Grand Canyon and the wide open expanse, yet I held firmly to the rail :rofl:
 
  • #20
Nereid said:
(and no, lady dogs do NOT reveal their breeds :shy: )

but a guy dog with a good nose can tell if its a lady---forget about breeds we are talking about what matters, nuff said, and WOOF WOOF to you too
 
  • #21
Nereid said:
Message from the global collective of Nereids, their partners, friends and families: http://members.iquest.net/~jswartz/jks/humor/dog.htm Woof! Woof!

(and no, lady dogs do NOT reveal their breeds :shy: )

good one :smile:, then I hope you won't laugh at the kind of Bird I am :smile:
 
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  • #22
It's important to be familiar with the concept of "Dark energy equation of state", represented by w. It is equal to density/pressure of dark energy. these are the values for the 3 more notorious models of dark energy

cosmological constant: w=-1
phantom energy: w<-1
quintessence: -1<w<-(1/3)
 
  • #23
chameleon chameleon

I want to present... the chameleon model!
http://arxiv.org/abs/astro-ph/0309300
"Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space"
In a nutshell, in this model quintessence is a chameleon field (i.e. a scalar field that has mass not constant in space and time, but rather depends on the environtment, in particular on the local matter density)

Now i understand why Bowie sang "There's a starman waiting
in the sky..." :wink:
 
  • #24
meteor said:
It's important to be familiar with the concept of "Dark energy equation of state", represented by w. It is equal to density/pressure of dark energy. these are the values for the 3 more notorious models of dark energy

cosmological constant: w=-1
phantom energy: w<-1
quintessence: -1<w<-(1/3)
Thanks meteor.

AFAIK, there's another difference between various approaches to DE, the question of time variability. The observational data are not consistent with DE varying by OOMs over cosmological time, but slower changes aren't ruled out. Of course, the CC is, by definition, non-varying :rolleyes:

What about the others?

Also, can you tell us anything about the 'Generalized Chaplygin gas' which many papers make reference to? How does such a gas differ from good ol' air? :smile:
 
  • #25
Nereid said:
Thanks meteor.

AFAIK, there's another difference between various approaches to DE, the question of time variability. The observational data are not consistent with DE varying by OOMs over cosmological time, but slower changes aren't ruled out. Of course, the CC is, by definition, non-varying :rolleyes:

What about the others?

Also, can you tell us anything about the 'Generalized Chaplygin gas' which many papers make reference to? How does such a gas differ from good ol' air? :smile:
It is imaginary.
 
  • #26
I will take on time variability later, but with respect to the GCG, its starnge cause the form of the equation of state differs form that of the other models. For the GCG is
P=(-A)/(d^a)
P=pressure
d=density
A=positive constant
and 0<a<=1
(reference gr-qc/0305086)
and no much information is given about it, is described as "a polytropic gas" or "a perfect fluid".
It's rather curious, in fact is an example of a kind of possible substance candidate to act as dark energy and dark matter at the same time called quartessence, that's why the GCG is also called Chaplygin quartessence. But there are other 2 possibles forms of quartessence: logarithmic quartessence and exponential quartessence
It is imaginary.
Some modern phlogiston?
 
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  • #27
quasar987 said:
Another one of the physics teacher working at the college I attended (see my previous post) wrote a book on basic http://universite.deboeck.com/Resources/Titles/28011100266200/Images/28011100266200L.gif [Broken]. In this book it says that the expansion of the Universe is due to the expansion of space itself and that this expansion of space is entirely predicted by Einstein's theory of GR. Now, if this is so, where does the DARK ENERGY (suposedly a MYSTICAL force of repulsion between matter) fit it ?!
The term Dark Energy is given to that matter which is causing the universe to expand at an accelerating rate. This is what some call "anti-gravity" since this is clearly gravity acting in a repulsive manner.

Back in Einstein's day nobody knew of any kind of matter which could produce such an effect. since Einstein assumed that the universe was static he added a term to his field equations to allow for this repulsive effect. Einstein's equations changed from

[tex]G^{\alpha\beta} = -\frac{8\pi G}{c^4}T^{\alpha\beta}[/tex]

to

[tex]G^{\alpha\beta} + \Lambda g^{\alpha\beta} = -\frac{8\pi G}{c^4}T^{\alpha\beta}[/tex]

[itex]\Lambda[/itex] is called the cosmological constant. In modern terms the cosmological constant is also called "Dark Energy." This is the term which, for normal matter, allows for anti-gravity when [itex]\Lambda[/itex] > 0. However this was before the concept of negative pressure was around. It is now conceivable that pressure terms in the [itex]T^{\alpha\beta}[/itex] can be negative. This would also give rise to resulsive gravitational effects. For weak gravitational fields Einstein's equations, for [itex]\Lambda = 0[/itex], can be expressed as

[tex]\nabla^2 \Phi = 4\pi G(\rho + 3p/c^2)[/tex]

Let [itex]\rho_A = 4\pi G(\rho + 3p/c^2)[/itex] = effective active gravitational mass. If the pressure is negative enough then [itex]\rho_A[/itex] < 0. Therefore when there is a large negative pressure the matter acts like a negative active gravitational mass (defined as that which generates a gravitational field).

Pete
 
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  • #28
meteor said:
Some modern phlogiston?
Hehe. The visible universe is merely dephlogisticated Chaplygin gas. :smile:
 
  • #29
pmb_phy said:
The term Dark Energy is given to that matter which is causing the universe to expand at an accelerating rate. This is what some call "anti-gravity" since this is clearly gravity acting in a repulsive manner.
Only it is Dark Energy that is the subject of this thread!
Pete everything you went on the say was true of Matter, however the matter density has been constrained by WMAP, using the GR paradigm to interpret the data, to be only 4 % baryonic matter (from BB nuclei-synthesis) and 23 % other unknown matter (Dark Matter). (All %'s are that of the critical density)

As the total density is assumed to be unity because of spatial flatness therefore 73 % is assumed to be something else called Dark Energy.

As I have said before these Dark entities may be a case of just adding "extra epicycles" to make the paradigm work, as Inflation, Dark matter and Dark Energy have not been demonstrated in over thirty years of active laboratory experimentation.
Garth
 
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  • #31
It seems that there's perhaps some preference within the physics community to a dark energy with constant energy density (e.g. cosmological constant). NASA scientists declared months ago that they bet for a cosmological constant
But I prefer a model with dependence on time. Examples of such models are quintessence, phantom energy and k-essence
Phantom energy (aka superquintessence) postulates an increase of dark energy density over time. So the universe will end violently tearing all apart in the Big Rip, aka Big Smash
Quintessence is a scalar field that varies over time and also has dependence on space ( so it will be more dense in some localizations than in others). It actually exercises negative pressure, but exercised positive pressure in the past! So, it can perhaps exercise positive pressure in the future (leading to a Big Crunch?)
K-essence also varies in space and time, its equation of state varies over time but its always w>(-1)
I prefer the model of quintessence because I think that the acceleration is not going to be eternal. Since I'm also a fan of Loop Quantum Cosmology and this theory has recently forecasted the possibility of the universe undergoing a Big Crunch, it's a model perfect for me
 
  • #32
I too expect that there will be time-dependant variation at the fundamental level (structure and coarseness of space-time, for instance) and I also expect that the Einsteinian space-time "curvature" caused by embedded mass will be better visualized as gradients in the properties of the basic units of space-time (density, orientation, energy states...). These space-time gradients will be found to cause "gravitational lensing" redshifting, and other effects, not gravity itself.

Gravity (as expressed as force acting over a distance) is very weak and should not be invoked as a force capable of bending the paths of photons passing nearby. The amount of mass needed to provided such refraction might overstate the mass of a galaxy or galactic cluster by quite a large amount (a pretty common problem these days, with about 96% of the mass of the universe tied up in invisible undetectable "dark matter"). :bugeye:
 
  • #33
turbo-1 said:
I too expect that there will be time-dependant variation at the fundamental level (structure and coarseness of space-time, for instance) and I also expect that the Einsteinian space-time "curvature" caused by embedded mass will be better visualized as gradients in the properties of the basic units of space-time (density, orientation, energy states...). These space-time gradients will be found to cause "gravitational lensing" redshifting, and other effects, not gravity itself.

Gravity (as expressed as force acting over a distance) is very weak and should not be invoked as a force capable of bending the paths of photons passing nearby. The amount of mass needed to provided such refraction might overstate the mass of a galaxy or galactic cluster by quite a large amount (a pretty common problem these days, with about 96% of the mass of the universe tied up in invisible undetectable "dark matter"). :bugeye:
Something like dark matter, which can't be accounted for within the Standard Model, and which we can't get into the lab to zap and prod, surely causes many folk heartburn.

However, to call it 'undetectable' does a considerable disservice to the ingenuity of observational astronomers. In particular, there is a consistency in the observations which is a challenge for alternative views - estimates of the mass of dark matter in rich clusters are consistent across three independent types of observation - X-ray data on IGM gas temperature (assume equilibrium, derive mass), redshift data on galaxy velocity dispersion (apply virial theorem, derive mass), and gravitational lensing (both weak and strong; assume Einstein, derive mass).

For at least one cluster, the distribution of dark matter has been derived (not just the mass), and a nice piccie made - if it ain't DM, what is it a piccie of? http://www.astro.caltech.edu/~tt/0024/CL0024II.pdf
 
  • #34
Nereid said:
For at least one cluster, the distribution of dark matter has been derived (not just the mass), and a nice piccie made - if it ain't DM, what is it a piccie of? http://www.astro.caltech.edu/~tt/0024/CL0024II.pdf
Thank you for a nice reference; "what is it a 'piccie' of?" How about dark baryonic matter?

In my post #12 on this thread I referred to two papers from an Indian team that show in the "Freely Coasting Universe", which is expanding strictly linearly, the mass density of ordinary baryonic matter is aboput 20% and not a maximum of 4% as in the standard paradigm.

Therefore this stuff does not have to be re-invented, we know it already and are made of it!
Garth
 
  • #35
Nereid said:
Something like dark matter, which can't be accounted for within the Standard Model, and which we can't get into the lab to zap and prod, surely causes many folk heartburn.

However, to call it 'undetectable' does a considerable disservice to the ingenuity of observational astronomers. In particular, there is a consistency in the observations which is a challenge for alternative views - estimates of the mass of dark matter in rich clusters are consistent across three independent types of observation - X-ray data on IGM gas temperature (assume equilibrium, derive mass), redshift data on galaxy velocity dispersion (apply virial theorem, derive mass), and gravitational lensing (both weak and strong; assume Einstein, derive mass).

For at least one cluster, the distribution of dark matter has been derived (not just the mass), and a nice piccie made - if it ain't DM, what is it a piccie of? http://www.astro.caltech.edu/~tt/0024/CL0024II.pdf
Well, we have fundamentally different views of this, so I'll try to state mine succinctly. First of all the picture of dark matter is not real in any sense - it is only a guess at how this invisible stuff "might" be distributed to explain the amount of "gravitational lensing" (a misnomer) observed through that cluster. I would like to see this same group show us how the dark matter needs to be distributed around a typical spiral galaxy in "just" such a way as to cause the differential rotations they exhibit. I'm afraid that dark matter gets very messy in that area.

As an optician, I am very interested in the behavior of light and other electromagnetic waves. Since detecting and measuring these radiations are the primary means by which we explore our universe, I am sensitive to quandries and puzzles regarding our understanding of light. You already know about some of my struggles with discordant redshift.

I suggest that we be parsimonious and NOT invoke the existence of dark matter to explain lensing. Right now, we know that massive objects exist, we know that massive objects distort space-time, and we know that light propogates through space-time. We have all the ingredients we need for lensing. The simplest explanation for "gravitational lensing" is that masses distort space-time and the distorted space-time refracts light passing through it, resulting in lensing. There is no need for dark matter, nor should we call this "gravitational" lensing. The lensing is cause by refraction of light passing through a space-time domain that is distorted by the presence of mass. The refraction is not caused by gravity (in the Newtonian sense). Newtonian gravity is an extremely weak force of attraction between massive bodies, and photons are not massive in any real sense. Their paths can be deflected however by density differences in the medium through which they travel - Space-Time.

How does mass distort space-time? Does it cause gradients in the distribution, orientation and/or energy state of the basic units of space-time? These are the questions that will have to be answered (probably by the LQG or String people) before quantum physics and relativity can be united. The optical qualities of clusters might hold clues as to how we can expect the distortion of space-time to manifest itself. The LQG people are modeling space-time as if it comes in discrete units with lengths, areas, and volumes quantized at the Planck level. What do these basic units of space-time do in the presence of mass? That's the tough part.
 
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<h2>1. What is dark energy?</h2><p>Dark energy is a theoretical form of energy that is believed to make up about 70% of the total energy in the universe. It is thought to be responsible for the observed accelerated expansion of the universe.</p><h2>2. How is dark energy related to the GR expansion of the universe?</h2><p>The GR (General Relativity) expansion of the universe is a theory that describes the overall expansion of the universe. Dark energy is believed to be the driving force behind this expansion, causing it to accelerate rather than slow down.</p><h2>3. What is the mystery surrounding dark energy?</h2><p>The mystery surrounding dark energy lies in the fact that it is a theoretical concept that has yet to be directly observed or understood. Its existence and properties are still being studied and debated by scientists.</p><h2>4. How are scientists trying to unravel the mystery of dark energy?</h2><p>Scientists are using various methods such as observations, experiments, and theoretical models to try and understand the nature of dark energy. This includes studying the expansion of the universe, mapping the distribution of matter and energy, and testing different theories and hypotheses.</p><h2>5. What are some potential implications of understanding dark energy?</h2><p>If we can fully understand dark energy, it could have significant implications for our understanding of the universe and its future. It could also potentially lead to new technologies and advancements in our understanding of fundamental physics.</p>

1. What is dark energy?

Dark energy is a theoretical form of energy that is believed to make up about 70% of the total energy in the universe. It is thought to be responsible for the observed accelerated expansion of the universe.

2. How is dark energy related to the GR expansion of the universe?

The GR (General Relativity) expansion of the universe is a theory that describes the overall expansion of the universe. Dark energy is believed to be the driving force behind this expansion, causing it to accelerate rather than slow down.

3. What is the mystery surrounding dark energy?

The mystery surrounding dark energy lies in the fact that it is a theoretical concept that has yet to be directly observed or understood. Its existence and properties are still being studied and debated by scientists.

4. How are scientists trying to unravel the mystery of dark energy?

Scientists are using various methods such as observations, experiments, and theoretical models to try and understand the nature of dark energy. This includes studying the expansion of the universe, mapping the distribution of matter and energy, and testing different theories and hypotheses.

5. What are some potential implications of understanding dark energy?

If we can fully understand dark energy, it could have significant implications for our understanding of the universe and its future. It could also potentially lead to new technologies and advancements in our understanding of fundamental physics.

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