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" "The current cosmological paradigm, the cold dark matter model with a cosmological constant, requires that the mass-energy of the Universe be dominated by invisible components: dark matter and dark energy. An alternative to these dark components is that the law of gravity be modified on the relevant scales. A test of these ideas is provided by the baryonic Tully-Fisher relation (BTFR), an empirical relation between the observed mass of a galaxy and its rotation velocity. Here, I report a test using gas rich galaxies for which both axes of the BTFR can be measured independently of the theories being tested and without the systematic uncertainty in stellar mass that affects the same test with star dominated spirals. The data fall precisely where predicted a priori by the modified Newtonian dynamics.
Stacy S. McGaugh (born January 11, 1964) is an American astrophysicist, known for his research on Modified Newtonian dynamics (MOND) and tests of the dark matter hypothesis.
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... It was (in part) Gross’s excessive enthusiasm for string theory in the mid-80s that drove me (as an impressionable grad student at Princeton) away from theoretical physics (and into astronomy). String theory may have been a beautiful idea, but it made no predictions that could be tested experimentally in the then-foreseeable future. That’s not science. A quarter century later and the theoretical physics community has yet to wake up and realize that there is new physics right under their noses – just not the new physics they’ve been expecting (GUTs, strings, membranes, etc.). Galaxy dynamics are consistent with a single, universal force law, but this unexpected behavior has largely been ignored because it doesn’t fit with particle theorists’ dreams of super symmetric dark matter particles. That we do not understand the observed behavior makes it more interesting than the “expected” (but unobserved) new physics: who ordered this?
A long time ago when I first got interested in MOND, having come from the background where I believed in dark matter, I wrote a proposal saying, "Gee, this theory had its predictions come true, ... we should look into that" and it was rejected, you know, very harshly. And I thought "OK, the community is not willing to fund this kind of thing" — this was almost twenty years ago. And so I basically did a global substitute, replaced MOND with dark matter, resubmitted, and I got my money. ... Pavel is totally correct that scientists are focused on getting grants, because that's what you need to support your students, and your postdocs, and getting the data, and all those sort of things. And I would like to believe that that was an anecdote from the distant past, but I am aware of a colleague who had this experience very recently where this person did not even mention MOND in the proposal, but the panel came back saying "MOND is no good — you must not spend money on this." ... the panel had associated ... this person's name with having at some point written a paper about MOND and projected that onto this proposal that ... did not mention MOND. And so it really is that bad.