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Mario Pasquato's avatar

Hi, I have a bunch of questions: 1) how do you make globular clusters? They seem to be the oldest (stellar) objects around. Even a galaxy like ours has over 100 of these objects. Notoriously, they are dark-matter free, meaning we can simulate them well enough without assuming they have their own dark matter halo, while dwarf galaxies tend to be dark-matter dominated instead (all of this within the Lambda-CDM model, which I am not a fan of). 2) what about the scaling laws, most importantly the baryonic Tully-Fisher relation, but also the central black hole mass - bulge mass relation (Magorrian relation), will you picture justify those? The TF relation is particularly tricky for dark matter cosmologies to justify 3) where are the primordial SMBHs now? if they form huge jets at first but are quiescent now (presumably gas-starved), what happened, did they sweep away the gas themselves? At the very least is should be possible to reveal them via gravitational lensing 4) what does your theory predict in terms of astrochemistry, in terms of primordial gas enrichment?

Tom Keith's avatar

Welcome back, I missed you

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