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Eric Gisse wrote: wrote: On Mar 20, 1:34 pm, "Eric Gisse" wrote: wrote: There is _no_ reason to doubt that our interpretation of the weak lensing results is false. There is matter there and it curves light and we detect it. That is remarkably direct compared to other cosmological observations that are *heavily* model-dependent. Just remember that I am arguing that there is no DM within Galaxy scales. ie MOND explains Galaxy rotation curves so obviously Weak Lensing will need to be explained by a quantum theory that will derive MOND. In my GR+DM cannot explain MOND. Galactic/cluster scales are deeply classical - there is no reason to expect a quantum theory would make any modifications at such macroscopic distances. What we got is what we got, any modifications to what we already know at large scales would have to be very subtle. You can argue that there is no DM within a galaxy, but you can't argue it from observational evidence. I can't argue against it, from the same token - but I would think it odd that it all accumulates in the halo. Neutrinos avoid this problem by being hot, which prevents their coupling together. Neutrinos avoid the problem by having an insanely small scattering cross section and by traveling within epsilon of light speed for pretty much any plausible amount of energy. They avoid the problem so well that they are horrible dark matter candidates - not enough of them can be produced, and they are not capable of binding to galaxies considering how fast they would be traveling. Neutrino dark matter would form a background, not a halo. True for Galaxy scales but not true for Cluster scales. So whats your point? What's another order of magnitude going to do? Look, neutrinos travel _FAST_ - within an epsilon of c for all realistic kinetic energies obtained from fusion reactions at the big bang. There simply aren't any bound orbits - the best you can reasonably expect is a weak background, which isn't going to influence anything significantly. KATRIN isn't and never will be a test of MOND. Neutrino oscillations simply shift the flavors around - they do not add mass. Neutrino mass is constrained to be very tiny, and if the L-CDM model is even close to being reasonable the total masses of all neutrinos is less than an eV. I don't understand this, the three flavours are supposed to have weight mass =/= weight. less than 2.2eV, 170KeV, and 15.5MeV. So even the lightest may be heavier than 1eV. The others are much much more heavy. No - those are the _least_ upper bounds on individual neutrino masses. The individual measurements are gross measurements to say the least - the spread is huge. However, the sum of neutrino masses is quite small - on the order of an eV, as constrained by astrophysical results [model dependent, but the consistency is very good across varying data sets]. http://pdg.lbl.gov/2006/listings/s066.pdf Do you mean to say that KATRIN will falsify LCDM if electron neutrino happens to have a weight more than 1eV. I don't believe that DM theories are falsifiable. They are just curve fitting exercises. Add as much DM as you need whereever you need. LCDM theories need not apply to Galactic level and the NFW halos need not have any cosmological significance. If neutrino masses were observed directly to be far larger than a fraction of an eV, I think it would be troublesome. But how exactly it would be troublesome is less than clear to me. Until some actual viable candidates are put forth, DM will be a bit less than strong in its' foundation. However, something that preserves our current theories of gravity and whose inclusion is supported by modeling of the large scale structure of the universe is quite compelling, especially when the only theory that is remotely competing at this point is an even more ad-hoc theory. Do not forget the supreme irony of neutrinos being anyway important in finding dark matter. Neutrinos were postulated a full 25 years or so before they were detected to explain the spectrum of energies in beta decay and to explain why angular momentum was not conserved. No! Neutrinos _can not do it_! You mean that Neutrinos cannot make stable structures at Cluster sizes. This is as much an speculation as is my assertion as mine. We don't yet know the masses and relative abundance of the three neutrinos. Relative abundances can be gathered via big bang nucleosynthesis. I gave you a link ...somewhere... that listed the top 10 or so most common reactions, and neutrinos were in most of them. It does not matter - the energies given to the neutrinos will be in the MeV range. That is DEEPLY relativistic - E ~ pc for E mc^2. Work backwards - how many zeros will be in your answer when you obtain 1 - v/c? Borrowing from GR slightly, neutrinos are the massive equivalent of light. They are the closest a massive particle can get to traveling on a geodesic. Borrowing further, light only has closed [UNSTABLE!] orbits around a mass when it is near [r ~ GM] the Schwarzschild radius. Dark matter is out in the halos of galaxies and such - a shade short. Look back at that paper I linked to you the other day - remember how everything was consistent with a HALO of dark matter? There are simply not enough neutrinos and the ones whizzing around simply have too much energy to be bound. http://www.astro.ucla.edu/~wright/BBNS.html Oh look there it is. It doesn't give any neutrino abundance. I would think that there may be a huge amount of neutrino as it is a very important part of the reactions below one second timeframe. Also I do not expect that all of it will be absorbed. It is entirely plausible to have a large amount of neutrinos. Of course there will be a large number of neutrinos. They will for all intents and purposes still be tooling around, barring ridiculously rare absorbtion events. They are very, very light and they are moving very, very fast. They do not matter - neutrino-based dark matter has been long discredited even before weak lensing results started coming in. Both DM and MOND were hypotheses created to explain galactic rotation curves. MOND, however, can't handle the large scale structure of the universe while DM is an fundamental part in something that makes a very, very good fit. Remember what you told me - something that fits that well has to have some fashion of truth to it? So give me one DM theory that works well at the large structure and works well for the galaxies as well. We know that LCDM does not work well at Galaxy level. We don't have one as far as I know. However, MOND seems like a good start. But I think Milgrom et al's head would explode if the dark matter people co-opted MOND in that fashion. There is a difference between MOND and DM. DM is a curve fitting exercise requiring the use of several free parameters, while MOND is a single equation that works well with a single universal parameter on all galaxies. No. If you read the papers I linked you, there is a direct correspondence between dark matter and baryonic matter. The amount of free parameters got very, very small. TeVeS is making testable predictions. I personally don't like TeVeS, but it is not a bad idea. We may come up with a law for weak lensing through it. This work is also needed for convincing GR proponents that DM in Galaxies is redundant. I wish them the best of luck - they have some severe hurdles to pass through. They have to describe *all* of the following self-consistently: Well GR has to explain MOND. Unless it does so, it is a suspect theory. G_uv = 8piG/c^2 T_uv That is GR right there. Everything GR predicts is based upon what you shove into T_uv - what do you suggest? Besides, the full machinery of GR is un-needed. Newton works for this - deeply classical, remember? GR is basically a few extra decimal places at 100AU distance - much less hundreds of thousands of light years. It needs to show how DM should be distributed to explain MOND. This has been done by working backwards from the observed distributions and Poisson's equation. MOND and DM play nice together. http://www.journals.uchicago.edu/ApJ...610/58610.html Seriously - did you read this? It must show why it should have this distribution and not any other. It must show why DM is required when the curves can be explained based on only BM. No, it doesn't. The question of "why" is not science's problem. The best you can hope for is "how?" 1) Make dark matter irrelevant. Why??? Making dark matter irrelevant is MOND's reason d'etre, that's why. Bullet Cluster shows that DM exists at the cluster scale, which was already expected from previous MOND fits to other cluster. You can change it to Make dark matter irrelevent at the galactic scale. It is certainly not required at the galactic scales. Bull**** it hasn't. http://www.journals.uchicago.edu/ApJ...610/58610.html I don't disagree with the rest of your list. They are certainly required by any quantum theory of gravity. I'm not talking about a quantum theory specifically - I'm talking about anything that seeks to supplant GR. The list is geared more towards TeVeS and such. MOND/TeVeS works well in strong gravity, as they are basically same as GR. Works very well in Galaxies. Predicts HDM in Clusters, as required by Bullet Cluster. Also is not against Dark Galaxies. It can be falsified, but has not been falsified yet. Careful when you say 'required'. I have been trying to distinguish between things that are observationally true and which are required to be true within a specific hypothesis. Hot neutrinos - it isn't something required by MOND, it is a *hypothesis* that is added in to explain the bullet cluster within the context of MOND. It is *required* by MOND to fit Bullet Cluster or any Cluster data. It may be that MOND is not the correct theory. But the Bullet Cluster proves that there is dark matter at cluster scales. There is no need to remove Dark Matter in Bullet Cluster. It is an unambiguous observation that Dark Matter exists in Bullet Cluster. Zuh? Are folks folks going with the King Solomon approach and splitting the difference? Arguing both dark matter *AND* MOND is a little contradictory to me. You have a lot of prejudice regarding MOND. I don't think I can rid you of your prejudice. You see the forest and cannot focus down to the trees. Of course I am prejudiced. The proponents of MOND seem to think it is a theory of gravity unto itself rather than a model. It is obvious that MOND and Dark Matter are not incompatible. If you ask Milgrom himself, he will not agree with your statement. The whole point of MOND is to show that a simple modification to Newtons law can explain rotation curves of all galaxies. It doesn't mean that we have seen everything, and that DM cannot exist in clusters. ....then when a fair bit of evidence crops up which shows that it is an actual matter distribution causing the funky rotation curves? It only means that there is no need for DM in Galaxies. Nothing more nothing less. http://www.journals.uchicago.edu/ApJ...610/58610.html READ IT I don't think I can continue this discussion if you cannot grasp this basic fact of MOND. Also MOND has been predicting double the mass in most Clusters, which should be the same Dark Matter which we see in Bullet Cluster. But that doesn't mean that it has to be CDM, it could be HDM. ...and how many HDM candidates are there? There aren't that many stable particles which don't interact electromagnetically... And how many CDM candidates have been observed. Viable? Zero. At least Neutrino has been observed and has now been shown to oscillate with some flavours having huge masses. Since we don't know the average mass we cannot yet conclude that it cannot make stable structures yet. 1 is less than 1 trillion. If my least upper bound is 1 trillion, 1 is the possible true value. Read the PDG link I gave you. The sum of masses appears to be less than an eV. Let me be clear - I accepted before and accept even more now thatMOND is pointing to something important. What we seem to disagree on is _what_ that important thing is. Well now I can rejoice ;-). We have reached the most important part of the discussion. You accept MOND effect as real. Yes and no. I accept that MOND is an accurate model over a surprisingly large sample set. I rationalize it thusly: all galaxies appear to have formed in the same way, more or less. So it stands to reason that DM will be the same in each galaxy [less collisions and exotic circumstances] if not more so due to the lack of interaction. I do not accept that MOND is a physical theory unto itself. There are too many results from weak lensing that make dark matter convincing in my eye, as well as its' utility in cosmological modeling. The MOND folkes probably would _not_ like that position. Again the forest. Try to focus only on one aspect at one time. Looking at trees only sometimes is useful. It is obvious that MOND is not a physical theory. It is just a visible artifact of the Quantum Theory of Gravity. No. It isn't. MOND was designed to, and continues to be, an exercise in curve fitting that has served its' purpose very well. Getting the answer right in one _limited_ regime does _not_ make it a viable theory of gravity. We know that Weak Lensing and Rotation Curves must have the same origin. If it is GR+BM+DM then it is the same for both if it is QTG+BM then it will be the same for both. Now if we can prove that GR+BM+DM cannot fit the Rotation Curves as well or better than MOND, then we have proved that GR+BM+DM is not the correct picture. And we must look into finding a theory QTG that is compatible with MOND and also explains weak lensing based only on BM. http://www.journals.uchicago.edu/ApJ...610/58610.html Dark matter and MOND share a large degree of correspondence. You seriously need to read that paper. The real solution is only to find a distribution of DM that has the following properties. 1) It can fit MOND at the currect epoch. 2) It can fit WMAP using a distribution that should be able to reach the MONDian distribution at the current epoch. WMAP data is an observation of the background radiation - it is about 14 billion years short. 3) There must be some observable departures from MOND which we can see to discard MOND. In other words there can be no DM theory that will be indistinguishable from MOND, because DM cannot have zero degrees of freedom. The bullet cluster is already an observable departure. You can't be choosy and suddenly make MOND applicable only to galactic scales when the entire theory is based around modifying gravity for low accelerations. 2) We cannot be living in a special epoch, when DM matches MOND everywhere. It must have been true for a very long time in the past. And will continue to do so for a very long time in the future. I don't see why not - at least, the matching part. I am yet to hear a convincing explanation as to why MOND *can't* be represenative of dark matter. We cannot be living in a special epoch because the galaxies we see are in different stages of development. DM cannot fit MOND for all of them unless it fits all of them at all times. So there can be no special epoch. They are not different. Barring exceptional cases and galaxies that have suffered collisions, they are all the same up to a parameter or three. I thought it was obvious so did not give my reasoning. 4) If you see the 3 points above you see that DM in galaxies is superfluous. It must satisfy too many features to be true, and top of that it has no degrees of freedom, which makes it a superflous concept. This is where Occam's Razor steps in to say that DM is not simpler than MOND, and so must not be the true picture of the world. I don't think you are applying Occam's razor properly. DM as a concept is quite simple - there is matter we can't see that explains otherwise contradictory observations. The concept is not superfluous because there is no alternative _physical_ explanation, nor is there an explanation of lensing results. I think you are not applying it properly. DM is simple but DM mimicking MOND is not. MOND is the real crux of the problem. Without MOND, there is no trouble for DM at all. With MOND it becomes totally superfluous (Just to remind only at the galaxy level, MOND doesn't fit Cluster data, so DM is not superfluous there). DM is a simple concept. MOND is a more complex concept. DM mimicking MOND is a very complex concept. http://www.journals.uchicago.edu/ApJ...610/58610.html READ IT On the contrary, MOND is expected to make a lot of Relativists very angry when they find that no DM model can work ;-). *points to weak lensing* That is what it is all coming back to - weak lensing. Why does weak lensing keep showing a distribution of dark matter if it isn't there? Weak Lensing is irrevelent, and I am not ignoring it while saying that. Even 2 free parameters are too many when a competing theory can fit the data without any free parameter. And most DM theories require 3 or 4 parameters. Remember that DM theories can fit the 20% cases where the data is problematic. This indicates that the free parameters are enough to fit any rotation curve even if they are not from a real galaxy. This is what proves that there are too many parameters. Any good model is one which is not able to work with bad data. DM models are not good models. What happens when the competing theory fails in an unambigious way in a different case? I don't think DM is anywhere near the point to where one could say "So what? I can fit any arbitrary curve with a large enough amount of parameters!" Actually it is at that stage. I had seen somewhere can't remember whether it was a paper or article, in which they had created a pseudo galaxy by merging data of two real galaxies. MOND would not fit that data, while LCDM halos where able to fit it. So how does that support your assertion that it has too many parameters? The L-CDM model has a _highly constrained_ 6 dimensional parameter space. I have linked you to the WMAP site and specific papers before - the amount of freedom the parameters have are quite small. Do you know how many parameters I need to do a QM problem? Same order of magnitude. I and possibly all of the MOND proponents are dying to know an entirely plausible distribution of DM that can fit MOND. Read the papers I cited you previously. You will see where I'm coming from. Especially http://www.journals.uchicago.edu/ApJ...610/58610.html Which one do you mean? PseudoIsothermal Halo or NFW Halo. Whichever. I don't think there is any large scale formation theory for either of them. The most popular theory that explains large scale structure formation is LCDM which fails badly on most Galaxies. Does it...? Reference? You must understand that any distribution must have a valid formation theory behind it. One is not complete without the other. Interesting how dark matter is held up to the standard of "explain anything and everything" [as it should] whereas MOND gets the "eh it works sometimes - must be true" treatment. Just remember that Occam's Razor is against you ;-). |
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#32
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On Mar 31, 11:41 pm, "Eric Gisse" wrote:
Do you say things like this after carefully ignoring evidence that disagrees with your interpretation? There exists an entire community discrediting you call evidences. If dark matter is an artifact, why is it that including dark matter makes for such a good model of the large scale of the universe? That 'good' model (L-CDM) is based in many free parameters and unproven assumptions and can fit almost anything by a change on the parameters. Why did MOND (you sometime called "crap model") predict a correct WMAP second peak whereas your preferred "good model" (L-CDM 1997) predicted a wrong peak? Why that 'good' model introduces constrains are in disagreement with analysis of dozens of galaxies (paper is in press)? How about explaining _all_ of the weak lensing results of the past 5 years or so that explicitly map out the distributions of dark matter? That 'explicit' map of dark matter is based in the prior _assumption_ dark matter is there. Therefore it is evidence of nothing. [BLOCKQUOTE Dark Matter is the craziest idea we've ever had in astronomy. It can appear when you need it, it can do what you like, be distributed in any way you like. It is the fairy tale of astronomy. ] MOND is a law, not a model nor a theory. By what stretch of the imagination do you say that? Again, just because you ignore stuff does not mean i invented. Even Google knows about that!! a search by "MOND law" returns a million items. MOND _fails_ in the bullet cluster and it was invented as a _model_ to explain rotation curves. [i] What 'fails'? relativistic MOND? non-relativistic MOND? Any MOND? None? [ii] DM model was invented by the same motive. Did not you know? [iii] We know GR + DM _fails_ in the bullet cluster and now a new kind of mysterious interaction has been invented by DM theoreticians for saving discrepancies. Think about the weak lensing results - where is most of the dark matter? Out in the halo. Ignoring weak lensing - where does the dark matter need to be to smooth out the velocities? Out in the halo. What is the domain of application for MOND? Out...in the halo, where gravity is thought to be "weaker". When R is larger the MOND law [1 / R] is stronger than [1 / R^2]. Why do you claim gravity is weaker when is stronger? It might be a good idea to explain what the hell you are talking about. You said the domain of application for MOND was where gravity is thought to be weaker. It is just the inverse, is not? The proponents think that if MOND works, there is no dark matter while ignoring the extremely likely possibility that MOND is mapping out dark matter. You do not understand MOND nor its impressive empirical success. GR+DM is not fine for galaxies and fails for bullet cluster unless invoking now a unproven _ad hoc_ hypotesis about existence of a new kind of interaction (NGI). Go go gadget intellectual dishonesty. Returning to your comical side again? Are you the same Eric Gisse who did an entire series of biased comments against MOND without taking some time to read literature on the topic first? Is that your definition of "intellectual honesty"? More about your unfounded accusation on NGI below. You _KNOW_, assuming you actually read the paper, that the 'new kind of interaction' is something that creeps in because the models they picked can't quite explain how fast some parts of the bullet cluster are moving by about 20%. How can you use the bullet cluster data against MOND but favourable towards GR + DM? The cluster is a problem for ***both*** MOND and GR +DM. That in no way means a 'new kind of interaction' is necessary until a hell of a lot more research is done. For avoiding any new misunderstanding by you part i will cite [BLOCKQUOTE But DM models of the bullet clusters within GR are not without their problems. Farrar and Rosen [88] note that the relative velocity of the clusters is too high as compared to those seen in DM simulations of structure formation. To remove the contradiction they propose that a non-gravitational attraction of a new sort acts only between clumps of DM. ] What do you understand by "To remove the contradiction [with GR+DM] they propose that a non-gravitational attraction of a new sort acts only between clumps of DM"? And why my writing "a new kind of interaction (NGI)" is, in your own words, intellectual dishonesty when I am reflecting current status of DM models? Because you love DM disliking any kind of criticism? Every time someone comes up with an idea that contradicts relativity - no matter how flimsy - you take it as the gospel truth. Could you offer a list of those supposed ideas or are you again launching out balloons when lacking arguments? Relativity has earned its' place in the scientific community. Again, relativistic MOND exists!!! MOND has gained its place on community during last decade. MOND will remain with us in one or other flavour because rocks. The future of DM looks... dark. In an interview Milgrom states [BLOCKQUOTE It's been said that dark matter theory is beginning to resemble the celestial mechanics of Ptolemy, who continually added epicycles to his models as the observations failed to conform to a geocentric universe. What would it take for scientists to abandon dark matter? DM is encountering difficulties in the face of observations, and people keep inventing new DM with new properties to try and circumvent these difficulties. Over the years I have refrained from attacking DM, but others have started finding faults with it and that trend is increasing. ] The very tool that allows folks to probe the nature of dark matter - gravitational lensing - is a relativity prediction. [GR + visible-matter + dark-matter] --- Lensing [Relativistic MOND + visible-matter] --- Lensing Lensing is not proving DM and disproving MOND like you believe. The analogy when Newtonian gravity failed is remarkable [NG + visible-planets + hidden-planet] --- Mercury perihelion [GR + visible-planets] --- Mercury perihelion |
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On Apr 5, 9:43 am, "Eric Gisse" wrote:
wrote: Eric Gisse wrote: wrote: It needs to show how DM should be distributed to explainMOND. This has been done by working backwards from the observed distributions and Poisson's equation.MONDand DM play nice together. http://www.journals.uchicago.edu/ApJ.../v609n2/58610/... Seriously - did you read this? And Seriously did you?? You think that MOND and DM play nice. But the author of the paper doesn't think so. So how did you come to that conclusion from this paper. There can only be one of two options at the galactic scale. 1) There is a difference between MOND and GR+DM. In this case we know that MOND works better than GR+DM for all theories of GR+DM. So obviously MOND is the correct law. 2) There is no difference between MOND and GR+DM, in which case DM does not exist and MOND is wrong. Because there can be no matter that has no degrees of freedom. If you think that a kind of matter can exist without any degrees of freedom. You are entitled to your opinion, but it is not a scientific opinion. There are only two realistic options. 1) You can ignore MOND, and believe that MOND proponents are crackpots. 2) You have to accept MOND, and the failure of GR. There is no middle way. GR+DM cannot model MOND. I think we are at a stalemate. There is no point in arguing further. regards, -anandsr |
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