Sundance
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Hello Chalnoth
The movement and clustering is not my idea, its general info.
The movement and clustering is not my idea, its general info.
It appears you have mangled it, then. The idea is that the nonlinear effect of clustering can provide the appearance of an accelerated expansion. It wasn't proposed to explain all expansion, just as an alternative explanation to dark energy. However, so far all such attempts to explain the effect in this way have failed to do so when examined in detail. It is difficult to do the analysis properly, so it isn't yet certain that this is entirely wrong, but it seems unlikely.Sundance said:Hello Chalnoth
The movement and clustering is not my idea, its general info.
I don't understand what images of colliding galaxies have to do with your discussion. I mean, they're cool and all, but I really don't see what you think they indicate.Sundance said:Hello Chalnoth
Have a look at as many images as you like
Eg
http://www.spacetelescope.org/news/html/heic0810.html
Okay...Sundance said:As for expansion and acceleration, I have questions.
Yes, well, this is what I do for a living. And simply glancing at telescope images doesn't provide any significant information about the universe, except that it's pretty. You need to go much deeper than simply glancing at a few images to extract meaningful information.Sundance said:Hello Chalnoth
The link NASA/ESA has many images
Look at the observation and maybe than you will see what I'm trying to explain.
You're showing your bias right there. Spacetime is reality.Sundance said:Expansion and acceleration is in spacetime.
Now look at reality.
You've got things backwards. Observations do not explain things. Theories explain observations. And one possible explanation, that is so far consistent with all explanations, is that there is a small but non-zero cosmological constant.Sundance said:Hello Chalnoth
Than explain the expansion and acceleration by observation.
I've worked on ways to distinguish between varying dark energy and constant dark energy, I've worked on estimation of the power spectrum of the cosmic microwave background, as well as foreground cleaning techniques for the CMB.Sundance said:So tell me about your work
Abstract: In cosmology it has become usual to introduce new entities as dark matter and dark energy in order to explain otherwise unexplained observational facts. Here, we propose a different approach treating spacetime as a continuum endowed with properties similar to the ones of ordinary material continua, such as internal viscosity and strain distributions originated by defects in the texture. A Lagrangian modeled on the one valid for simple dissipative phenomena in fluids is built and used for empty spacetime. The internal "viscosity" is shown to correspond to a four-vector field. The vector field is shown to be connected with the displacement vector field induced by a point defect in a four-dimensional continuum. Using the known symmetry of the universe, assuming the vector field to be divergenceless and solving the corresponding Euler-Lagrange equation, we directly obtain inflation and a phase of accelerated expansion of spacetime. The only parameter in the theory is the "strength" of the defect. We show that it is possible to fix it in such a way to also quantitatively reproduce the acceleration of the universe. We have finally verified that the addition of ordinary matter does not change the general behaviour of the model.
Dark matter is an as yet unknown form of matter that has no electrical charge. It is very normal in the sense that it behaves much like stuff that we already know about: neutrinos. But it has to have much more mass than neutrinos to explain our observations. Its existence is strongly evidenced and extremely likely, and many searches to discover its exact nature are currently underway.Sundance said:Hello Chalnoth
Your work sounds fantastic.
What is the difference between dark matter and dark energy?
One of many attempts to explain dark matter/dark energy in other ways. These proposals are a dime a dozen. Nearly all are certainly wrong. As for me, I'm just going to be paying attention to the ground-based dark matter searches that are currently underway. I'm hopeful that we'll have a result from them within ten years. Furthermore, our observations of the universe will, within ten years, be to the point where we can start saying some definitive things about the dark energy. Until we have a significant experimental discrepancy to explain, I just don't see any reason to bother entertaining any particular one of the vast array of hypothetical theoretical models that attempt to explain these things.Sundance said:Hello Chalnoth
May I have your opinion on this paper
http://arxiv.org/abs/gr-qc/0601033
A darkless space-time
Authors: A. Tartaglia, M. Capone
(Submitted on 9 Jan 2006 (v1), last revised 25 Apr 2007 (this version, v5))
If I'm understanding you correctly, you're talking about normal, baryonic matter that has collapsed into dense objects as potentially being the dark matter. The are two primary problems with this that I can think of off-hand. The first is that these collapsed objects will primarily form in the areas where normal matter is the most dense, i.e. the center of galaxies. But the distribution of velocities of the matter orbiting the centers of galaxies demonstrates that most of the mass is evenly distributed throughout the galaxy. So the idea just doesn't make a whole lot of sense.Sundance said:Hello Chalnoth
I agree with you to some degree.
Why not consider dark matter/energy as a ultra dense degenerate matter found in compact objects. Such as Neutron matter, quark matter, neutrino matter and the preon particles.
.Abstract: We consider a model in which Sgr A*, the 3.5x10^6 M_sun supermassive black hole candidate at the Galactic Center, is a compact object with a surface. Given the very low quiescent luminosity of Sgr A* in the near infrared, the existence of a hard surface, even in the limit in which the radius approaches the horizon, places severe constraints upon the steady mass accretion rate in the source, requiring dM/dt < 10^-12 M_sun/yr. This limit is well below the minimum accretion rate needed to power the observed submillimeter luminosity of Sgr A*. We thus argue that Sgr A* does not have a surface, i.e., it must have an event horizon. The argument could be made more restrictive by an order of magnitude with microarcsecond resolution imaging, e.g., with submillimeter VLBI
Abstract: Recent developments in the spectropolarimetric study of compact objects, specifically black holes (stellar and massive) and neutron stars are reviewed. The lectures are organized around five topics: disks, jets, outflows, neutron stars and black holes. They emphasize physical mechanisms and are intended to bridge the gap between the fundamentals of polarimetry and the phenomenology of observed cosmic sources of polarized radiation, as covered by the other lecturers. There has been considerable recent progress in spectropolarimetry from radio through optical frequencies and this is producing some unique diagnostics of the physical conditions around compact objects. It is argued that there is a great need to develop a correspondingly sensitive polarimetric capability at ultraviolet through gamma-ray energies.
As I said, it comes straight from the cosmic microwave background. The CMB demonstrates that dark matter was gravitationally active before the emission of the surface of last scattering, when the universe was uniform to one part in 100,000. There's not really much way for large compact objects to have existed in quantity during that era.Sundance said:Hello Chalnoth
I do not know where you get your infromation from.
Yes, I do. What, pray tell, do you think I am misunderstanding with respect to the CMB?Sundance said:Hello Chalnoth
Mate do you read scientific papers or you talk off the bat?
To begin with read up on CMB.
Okay. And what supports your claim that there existed large, compact objects in the early universe?Sundance said:Hello Chalnoth
You write well and sound very humble.
With due respect, either you or me are on opposite sides of the fence.
This is the type of reading I do
Degenerate matter black holes
http://adsabs.harvard.edu/cgi-bin/nph-basic_connect?qsearch=Degenerate+matter+black+holes&version=1
CMB 2008
http://arxiv.org/find/all/1/all:+AND+CMB+2008/0/1/0/all/0/1
No. I'm inferring from the consistency of a wide variety of evidence that the BBT is at least approximately accurate.Sundance said:The thing is this.
You are asssuming that the BBT is correct and relating this to CMB.
Indeed. This would be pseudo science. Here is one clear indication that this is so (from the website):Sundance said:This link is quite interesting
NEW THEORY OF NON-EXPANDING UNIVERSE
http://sharma-upt.com/NonexpandingUniverse.aspx
Also the link By Eric Lerner, although questioned is still quite interesting on the science side of things.
Evidence for a Non-Expanding Universe: Surface Brightness Data From HUDF
http://arxiv.org/abs/astro-ph/0509611
Maybe I'm barking up the wrong tree.
Apparently this hack is of the opinion that because an experiment has not been performed, he gets to decide what the outcome of such an experiment would be.Since the individual red shifts have never been found to increase with time, the galaxies are not flying away to generate an expansion of the universe.
Please avoid the following common misconceptions about the Big Bang and expansion:
The Big Bang did not occur at a single point in space as an "explosion." It is better thought of as the simultaneous appearance of space everywhere in the universe. That region of space that is within our present horizon was indeed no bigger than a point in the past. Nevertheless, if all of space both inside and outside our horizon is infinite now, it was born infinite. If it is closed and finite, then it was born with zero volume and grew from that. In neither case is there a "center of expansion" - a point from which the universe is expanding away from. In the ball analogy, the radius of the ball grows as the universe expands, but all points on the surface of the ball (the universe) recede from each other in an identical fashion. The interior of the ball should not be regarded as part of the universe in this analogy.
By definition, the universe encompasses all of space and time as we know it, so it is beyond the realm of the Big Bang model to postulate what the universe is expanding into. In either the open or closed universe, the only "edge" to space-time occurs at the Big Bang (and perhaps its counterpart the Big Crunch), so it is not logically necessary (or sensible) to consider this question.
It is beyond the realm of the Big Bang Model to say what gave rise to the Big Bang. There are a number of speculative theories about this topic, but none of them make realistically testable predictions as of yet.
To this point, the only assumption we have made about the universe is that its matter is distributed homogeneously and isotropically on large scales. There are a number of free parameters in this family of Big Bang models that must be fixed by observations of our universe.
The most important ones are: the geometry of the universe (open, flat or closed); the present expansion rate (the Hubble constant); the overall course of expansion, past and future, which is determined by the fractional density of the different types of matter in the universe. Note that the present age of the universe follows from the expansion history and present expansion rate.
As noted above, the geometry and evolution of the universe are determined by the fractional contribution of various types of matter. Since both energy density and pressure contribute to the strength of gravity in General Relativity, cosmologists classify types of matter by its "equation of state" the relationship between its pressure and energy density. The basic classification scheme is:
Radiation: composed of massless or nearly massless particles that move at the speed of light. Known examples include photons (light) and neutrinos. This form of matter is characterized by having a large positive pressure.
Baryonic matter: this is "ordinary matter" composed primarily of protons, neutrons and electrons. This form of matter has essentially no pressure of cosmological importance.
Dark matter: this generally refers to "exotic" non-baryonic matter that interacts only weakly with ordinary matter. While no such matter has ever been directly observed in the laboratory, its existence has long been suspected for reasons discussed in a subsequent page. This form of matter also has no cosmologically significant pressure.
Dark energy: this is a truly bizarre form of matter, or perhaps a property of the vacuum itself, that is characterized by a large, negative pressure. This is the only form of matter that can cause the expansion of the universe to accelerate, or speed up.
One of the central challenges in cosmology today is to determine the relative and total densities (energy per unit volume) in each of these forms of matter, since this is essential to understanding the evolution and ultimate fate of our universe.
No, this is incorrect. I think that the NASA summary does indicate this, but it is being somewhat misleading. The beginning it's talking about seems to be the boundary between cosmic inflation and where the classical big bang theory takes over.blighty said:The space fabric that is there now was there before is what I am saying, as was the mass. but what the current theory is trying to suggest ( unless I'm not reading it right ) is that the mass appeared as if by magic along with time and space?
Well, this is just the way that gravity works.blighty said:I'm not buying this space is growing, balloon theory that's causing matter to drift apart. it just makes me laugh :P
It's not so mysterious. If you're in an expanding universe, and moving with respect to the background, you'll tend to catch up with the surrounding matter after a time, eventually becoming basically stationary with your surroundings again.blighty said:Ok, I will do some reading because I wan`t to know why everybody thinks that if you could somehow stop our galaxy moving with an imaginary hand, then let go again and it will begin to move again, this sounds crazy to me, but then again so does a broken star that can spin 600+ times a second. :)
Chalnoth said:It's not so mysterious. If you're in an expanding universe, and moving with respect to the background,
Please don't call it a balloon theory. The balloon is an analogy, and is not precisely representative of the theory.blighty said:What background are we talking about here? maybe this is were I am becoming confused, the way i`m interpreting the balloon theory is that it`s this background that is expanding and carrying the mass with it,
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