Stacy McGaugh
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dudedarkmatter.bsky.social
Stacy McGaugh
@dudedarkmatter.bsky.social
Professor at Case Western Reserve University. Astronomer working on galaxies, cosmology, dark matter and modified gravity.

Read about them at https://tritonstation.com/
Yeah, this signal should be a lot easier to detect in dwarf galaxies, and yet it is not.
November 26, 2025 at 5:27 PM
Reposted by Stacy McGaugh
... but I agree with Stacy that the assumed MW halo is too massive/dense to be realistic. And I'd expect that if you reduce the assumed dark matter density, the same amount of DM needs to generate a stronger signal. Which should increase rather than ease the tension with dwarf galaxy constraints.
November 26, 2025 at 7:55 AM
Just skimming the stuff I know really well, I can say categorically that the DM halo is inconsistent with data. The local DM density is a factor of 2 too high, and the central density way too high - there is no room for an NFW cusp is the MW. That’s critical for the signal.
November 26, 2025 at 2:47 AM
OMG we’re not doing this again, are we? There was a claim to this effect 11 or 12 years ago. 126 GeV instead of 20, but then as now, if that were real, I trust the Fermi team would have been the first to tell us about it.
November 26, 2025 at 2:45 AM
Nah. Was paraphrasing ghostbusters is all. m.youtube.com/shorts/LV2dl...
"There's Something You Don't See Every Day" | Ghostbusters (1984) | Now Scaring #shorts
YouTube video by NOW SCARING
m.youtube.com
November 22, 2025 at 6:36 PM
Effen ewoks, man

Can’t live with them, stormtroopers can’t shoot them.
November 19, 2025 at 7:05 PM
Crudely speaking, Thermo, E&M, & mechanics for BA; add QM for BS. That’s not exactly right; for details see bulletin.case.edu/arts-science...
Astronomy, BS < Case Western Reserve University
bulletin.case.edu
November 19, 2025 at 12:59 AM