#paperday (sort of): here is the final accepted version of our

"On the interpretation of XRISM X-ray measurements of #turbulence in the intracluster medium: a comparison with cosmological simulations" by myself and G. Brunetti

https://arxiv.org/abs/2507.04727

I did an earlier thread here: https://mastodon.social/@franco_vazza/114816701059679474

The paper only have a useful appendix, which explains why homogenous kolmogorov turbulent models are useful, until they get too simplistic! #astrophysics #astronomy #science

This aspect will keep being relevant as long as people will continue to just rely on homogenous model to interpret too much in detail complex observations. here a killer example:
we initialised a spherically homogeneous density profile perfectly matching the coma cluster (and the simulation) and added on top of it a distribution of velocity fluctuations randomly drawn from a Kolmogorov spectrum - this is also very close to the simulated one.

Then...

...then we computed the distribution of line-of-sight broadenings of emission Iron lines in the two cases, which is the quantity that you can now finally measure with the XRISM satellite. The difference is significant: homogenous models produce a factor ~50-70% higher dispersion **even if the kinetic energy in the full simulation, and in the homogenous model is the same by construction**. Why? Because realistic turbulent is intermittent, i.e. more energy can be concentrated in less volume.
So our interpretation is that the line broadening currently measured by XRISM (which is anyway limited to extremely tiny 90 x 90 kpc^2 spots, in the case of COMA) is actually probing a kinetic energy which is at least a factor ~2 higher than they think.
This is important if you want to really understand the level of "non-thermal" energy in the intracluster medium!
Finally, I take pride of this extra bit in the acknowledgments:
@franco_vazza I love it! I'm going to have to copy that next time I write a paper
@thomasconnor Let's start a resistance movement in papers right here!