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Whither Goest CMB Isotropy?
[[Mod. note -- Due to a complicated chain of mishaps/mistakes on my
part, all References: headers are missing from this article. I apologise to the author and other readers for this, and for the ensuing loss of threading in many newsreaders. -- jt]] In article mt2.1-19091-1230581828@silver, Knecht writes: Typo in subject line corrected. Paragraph 2 gives some background concepts relating to the issues under discussion. I am reading a very new preprint (19 Dec 2008) put on the arxiv.org site. It is designated arxiv:0812.3795v1 and it is written by F. K. Hansen, A.J. Banday, H.K. Erikson and P. B. Lilje. The basic issue is whether the observable universe is homogeneous (appears isotropic) or whether the observable universe shows evidence for discrete fractal organization from the smallest to the largest observable scales. I haven't yet read the paper (though I know and/or have met some of the authors), but my guess is that they don't mention "discrete fractal organization". You make it sound like a dichotomy: EITHER it's homogeneous OR there is "discrete fractal organization". Also, the universe can appear isotropic without being homogeneous if we occupy a special position. Conventional astrophysics has tended to favor the assumption of strict large-scale homogeneity, and some theorists insist that the Universe simply must be homogeneous (received wisdom?). The Cosmic Microwave Background (CMB) has always been cited as the gold standard proof of large-scale isotropy/homogeneity and previous measurements were arguably consistent with the assumption of large-scale homogeneity. Ah, but deviations from isotropy in the CMB would indicate that fundamental inhomogeneity, and the possibility of a fractal Universe, Non-sequitur. I wonder if fractal paradigms might be included in this search for an explanation? People might consider them had the discrete fractal paradigm made some quantitative predictions which could in principle be falsified. |
#2
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non-fractal Whither Goest CMB Isotropy?
Phillip Helbig wrote:
Knecht writes: The basic issue is whether the observable universe is homogeneous (appears isotropic) or whether the observable universe shows evidence for discrete fractal organization from the smallest to the largest observable scales. I haven't yet read the paper (though I know and/or have met some of the authors), but my guess is that they don't mention "discrete fractal organization". You make it sound like a dichotomy: EITHER it's homogeneous OR there is "discrete fractal organization". There seems to be an issue ongoing for some number of years here of a theory fuzzy in all its details for which _every_ anomalous observation by astronomers is seized upon as additional evidence for that theory, without any attempt to integrate it in any coherent way into that theory. I'm fairly sure that's not a paradigm used by successful scientists. People might consider them had the discrete fractal paradigm made some quantitative predictions which could in principle be falsified. Well, "discrete fractal organization" makes one immediate prediction which is easily falsified. "Fractal" means what it says, and if the universe were "fractal", that would be observable at local scales, and indeed down to atomic scales and below. No such local observations exist, therefore "fractal" is not an appropriate description of the universe. Pretending that "fractal" has some other meaning than the one it has in mathematics doesn't seem likely to lead anywhere useful. We already know at what scales "discrete" would have to hold, and that is at anything above the Planck length. Terminology that matches what the observations do seem to support already exists and is in use, as e.g. "anisotropic". There is not any obvious reason to try to convey this direct observable and those like it into some magical and unspecified realm outside of math, physics, and astronomy. xanthian. |
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Whither Goest CMB Isotropy?
On Jan 3, 1:33Â*pm, Phillip Helbig---remove CLOTHES to reply
wrote: I wonder if fractal paradigms might be included in this search for an explanation? People might consider them had the discrete fractal paradigm made some quantitative predictions which could in principle be falsified. The Discrete Fractal Paradigm has made multiple definitive predictions (defined as predictions that are unique, testable, quantitative and nonadjustable) in peer-reviewed literature. Below is a sampling. International Journal of Theoretical Physics, 12(12), 1503-1532 (1989): 9 definitive predictions. [[Mod. note -- This citation appears to be incorrect: the IJTP web site says that volume 12 was published in 1975, and did not contain a page 1503. scholar.google.com suggests that the correct reference might be to volume 35 number 12 (December 1996), pages 2475-2481. Alas, Springer doesn't believe in Open Access, so an institutional subscription (or $$$) is needed to read this paper. -- jt]] Fractals, 10(1), 27-38 (2002): Dark matter predictions, results: stellar-mass black holes = many, dark matter particles = 0. arXiv:astro-ph/0102285, currently being reviewed, discusses a critical and definitive prediction of the DFP that the lowest mass M-dwarf stars will have an anomalously low incidence of planetary companions. The website www.amherst.edu/~rloldershaw discusses these and many more quantitative predictions by which the Discrete Fractal Pradigm may be unambigously tested. I am still hopeful that FGST, and further microlensing surveys, will give us new information on stellar-mass black holes in the Galaxy. I eagerly await LHC start-up and predict no discovery of dark matter particles, beyond the usual false-positives. Yours in science, Knecht www.amherst.edu/~rloldershaw |
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Whither Goest CMB Isotropy?
On Jan 4, 1:19Â*pm, Knecht wrote:
International Journal of Theoretical Physics, 12(12), 1503-1532 (1989): 9 definitive predictions. [[Mod. note -- This citation appears to be incorrect: the IJTP web site says that volume 12 was published in 1975, and did not contain a page 1503. Â*scholar.google.com suggests that the correct reference might be to volume 35 number 12 (December 1996), pages 2475-2481. Alas, Springer doesn't believe in Open Access, so an institutional subscription (or $$$) is needed to read this paper. -- jt]] Alas, we are both wrong, I copied a typo from my website and you cited a different paper. The correct reference is, I hope, IJTP, vol.28, No.12, 1503-1532 (1989). It is a companion piece to Part 1 (IJTP, 28(6), 669-694 (1989) Both papers are PRINTED IN FULL in the "Selected Papers" section of www.amherst.edu/~rloldershaw . NO CHARGE; AVAILABLE 24/7. Sorry about that incorrect vol. #, Knecht www.amherst.edu/~rloldershaw |
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non-fractal Whither Goest CMB Isotropy?
On Jan 4, 1:00=A0pm, Kent Paul Dolan wrote:
"Fractal" means what it says, and if the universe were "fractal", that would be observable at local scales, and indeed down to atomic scales and below. No such local observations exist, therefore "fractal" is not an appropriate description of the universe. Perhaps the term "fractal" is off-putting to you, so let's switch to the synonymous concept of self-similar structure. Self-similarity strictly implies hierarchical organization and for the moment we do not need to worry about whether the self-similarity is discrete or quasi-continuous. Please go to www.amherst.edu/~rloldershaw, click on "Selected Papers" and choose the essay "Nature Adores Self-Similarity". As you read this informal essay, jot down a list of the specific examples of physical self-similarity observed in nature and reported in scientific books and journals by other scientists. When you are done with the essay, you will have a written list of about 80 examples of self-similar structures in the local observable universe. When your intuition tries to tell you that nature is not fractal, this list and nature will help to improve your vision. Note also that nonlinear dynamical systems are ubiquitous in nature. Fractal phenomena (see period-doubling, strange attractors, etc., etc.) are inimately linked to NLDS. It's a fractal world, my friend. Enjoy! Yours in science, Knecht www.amherst.edu/~rloldershaw |
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non-fractal Whither Goest CMB Isotropy?
Thus spake Knecht
On Jan 4, 1:00=A0pm, Kent Paul Dolan wrote: "Fractal" means what it says, and if the universe were "fractal", that would be observable at local scales, and indeed down to atomic scales and below. No such local observations exist, therefore "fractal" is not an appropriate description of the universe. Perhaps the term "fractal" is off-putting to you, so let's switch to the synonymous concept of self-similar structure. That is not synonymous. Classical space time is self similar, but not fractal, whereas a fractal universe can be mooted to apply on very small scales on which the scale of discreteness cannot be observed, but not on large scales where it is observably false. Regards -- Charles Francis moderator sci.physics.foundations. charles (dot) e (dot) h (dot) francis (at) googlemail.com (remove spaces and braces) http://www.teleconnection.info/rqg/MainIndex |
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