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MOND does not really deal with variations in the Cosmic Microwave Background Radiation, which Dark Matter does try to explain.See: https://en.wikipedia.org/wiki/Lambda-CDM_model#Historical_development
Never liked 'gravitons' and 'dark matter', then again, that's a purely personal opinion. What is missing in your link though is a explanation of how they propose this 'modified gravity' is supposed to work, also how well it will fit Einsteins definitions of gravity=Actually it makes me think of 'phonons'
A universe of ideas dead cat Information, I should write more about him=and yes, we're alike in that. He do make sense=What I found frustrating before was the way he always referred to 'entropy', without me seeing exactly how he thought there. But in the 'lecture' he simplifies it to counting the number of bits, giving you a numerical expression of the amount of possibilities any given system can become in, defining that as the 'entropy' of the system. That's simpler and make sense. But if I get it right this numerical evaluation of bits are not what he means, it's just a safe starting stone from where we move to 'information', and uncertainty, itself, he's a deep thinker.
What I found frustrating before was the way he always referred to 'entropy', without me seeing exactly how he thought there. But in the 'lecture' he simplifies it to counting the number of bits, giving you a numerical expression of the amount of possibilities any given system can become in, defining that as the 'entropy' of the system. That's simpler and make sense. But if I get it right this numerical evaluation of bits are not what he means, it's just a safe starting stone from where we move to 'information', and uncertainty, itself, he's a deep thinker.
As I understand it, the hypothesis of dark matter is invoked to explain that the outermost stars of some galaxies are orbiting the center more rapidly than can be accounted by the presumed mass of observable stuff in the galaxy.
Given that we only have about 100 years' observations of individual stars in distant galaxies, why do we think that they are in stable orbits and not just rushing towards the galactic centre from deep space?
How good is the historic velocity data? Given that 100 years is a fleabite in galactic history, how accurate is the acceleration measurement?
How do we know the gravitational centre of the galaxy hasn't moved with respect to the apparent centre if there are several light years between the outer star, say closer to us, and the gravitational centre, further away?
QuoteQuote from: alancalverd on Yesterday at 22:29:51How good is the historic velocity data? Given that 100 years is a fleabite in galactic history, how accurate is the acceleration measurement? Its the doppler that's measured and from that the speed.
Quote from: alancalverd on Yesterday at 22:29:51How good is the historic velocity data? Given that 100 years is a fleabite in galactic history, how accurate is the acceleration measurement?