@franco_vazza@mastodon.social
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franco_vazza

@franco_vazza@mastodon.social

#SimulatedUniverses #AstroPhysicsFactlet
Astrophysicist at Bologna University and https://respublicae.eu/@ERC_Research grantee.
I study the cosmic web, extragalactic magnetism and clusters of galaxies with colorful simulations.

https://cosmosimfrazza.eu
#astrodon #astronomy

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franco_vazza, to Astronomy
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Awesome collection of FRII radio galaxies observed with the LOFAR LOTSS DR2 survey, just the cover picture in Martin Hardcastle's talk at SPARCS.

franco_vazza, to Astronomy
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...Think I am going to move from extragalactic to galactic modelling...the quality of these recent multi-wavelengths composition of exploding stars in the Galactic plane (this one showed by Filomena Bufano at SPARCS) is jaw dropping

(sorry I could not get the full reference to this image - probably still WISE and ASKAP)

franco_vazza, to Astro
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This superposition of Wise (infrared) and Askap (radio) images of a crowded fields with several pulsar wind nebulae in our Galaxies, just presented at SPARCS by Sanja Lazarevic, is just 😱

franco_vazza, to Astro
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Have you seen the Crab Nebula observed by LOFAR (including international stations, so higher resolution)?
I just did, at my SPARCS meeting:
gorgeous image by Maria Arias and collaborators:

franco_vazza,
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and here is a side by side comparison with the usual optical image of the Crab

franco_vazza, to Astro
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Couple of slides from the talk I just gave to the SPARCS XII conference in Bologna, on th theme of:
"Numerical simulations keeping up with the complexity of radio discoveries"

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franco_vazza, to Astronomy
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Just stunning extra galactic radio astronomy, using the ASKAP radio telescope!

"ASKAP reveals the filamentary radio tail structure of the Corkscrew Galaxy "
https://arxiv.org/abs/2405.0437

by B. Koribalski et al.

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franco_vazza, to Astro
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simulated simultaneous evolution of magnetic fields and cosmic rays injected by the same growing galaxies in a small cosmic volume, with a recently developed version of the ENZO code, running on Leonardo @Cineca

video/mp4

franco_vazza, to Futurology
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Things you can find for dinner in Florence after a talk about the cosmic web and the human
: fried brain 🧠 (of veal).

I am vegetarian so no chance, but you think my neurosurgeon colleague took?

franco_vazza,
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@santiago I'll ask for the outcome the day after

franco_vazza, to Astronomy
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Some picture of this cool event in Florence:
https://mastodon.social/

the first official opening to the public of the ancient villa on the hills of Florence where Galileo Galilei spent his latest years while being home imprisoned by damm Santo Uffizio, and where he wrote his latest works.
Some walls and bricks and trees might stille be the same that were around while he was 🥺

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franco_vazza,
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There also were SKA low band prototypes on display, and a lot of references to modern science, as this location now works jointly with all neighbouring research institutes, including INAF

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franco_vazza, (edited ) to random
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#academic #academicchatter
Do you also have colleagues who, when meeting external visitors, tell that "the real research" is done in their institute, and not in the neighbouring one (which happens to be yours)?

Or are you luckier, and your colleague are less pathetic and less affected by egomaniac problems...?

🙄

franco_vazza, to Astronomy
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Tomorrow evening, quite a special event:
I will be at Villa Galilei in the hills around , where Galileo spent his latest years of home imprisonment, to speak about how the human brain and the cosmic web might look alike, through the lens of analysis and together with my (neurosurgeon) colleague.
Events organized by Inaf and University of Florence.
https://portalegiovani.comune.fi.it/urlnews/webzine/48720.html

franco_vazza,
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Best video recap of what we started producing a few years ago:
https://youtu.be/97V8jw7rc9I?si=ZpRxn6aoL-LQI_OR

(You can find tons of junk reports instead which entirely mystify our work on the web...)

franco_vazza,
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@barrygoldman1
I'd say yes: if a node moves or grow mass, another node will react to that (after a light crossing time). You can represent that as an exchange of information. But it's processed about 1e9 times slower than in the human brain!

I did some exploratory work to quantify the information content encapsulated in the organisation of the (simulated) cosmic webm maybe you can find interesting:
https://arxiv.org/abs/2007.05995

franco_vazza, (edited ) to Astronomy
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Important work by PhD stud. Giada Pignataro at the University of Bologna, just accepted by A&A Letters:

"Abell 0399−Abell 0401 radio bridge spectral index:
the first multifrequency detection"

https://arxiv.org/abs/2405.00772 Pignataro et al. incl. @annalisa_bonafede and myself

The low frequency radio detection using , allows to refine our understanding of this cosmic monsters which I described already in the past (https://mastodon.social/)

franco_vazza,
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The radio multi-frequency coverage of this extended region in between two clusters of galaxies allows to infer the spectrum of the radio emission.

It is very steep between 140 and 60MHz: α~-1.4, i.e. only few electrons are accelerated to energies much higher that a few Giga electronvolt.

Which in turn, can be used to test possible acceleration models.

Can it be Fermi I acceleration from shocks? No: such steep emission will come from to too shocks too weak to accelerate cosmic rays.

franco_vazza,
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Viceversa, this steep spectrum is better reconciled with the turbulent Fermi II re-acceleration model we developed for this system , which requires volume filling turbulent motions (several hundreds of km/s, plausible in these accretion regions) and magnetic reconnection.

A very steep spectrum is compatible with the models we derived in 2020
(Brunetti & Vazza 2020 here https://arxiv.org/abs/2001.07718)

franco_vazza,
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Next step will be to actually measure this turbulent velocity... except that there are no X-ray photons in this region, owing to its very low density.

Noticeably, the conclusions of this paper are compatible with the one recently reported by this other paper I commented

https://mastodon.social/

which used Faraday Rotation and polarisation to exclude the possibility of a shock origin for the A399-A401 bridge.

franco_vazza, to Astro
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https://arxiv.org/pdf/2405.00115 by HyeongHan K. et al.
arguing that (at least to my surprise) the Perseus cluster of galaxies has evidences of a major merger in its past, supported by numerical simulations and kinematic modelling of the gas & dark matter components.

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franco_vazza, to Astronomy
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A new recent investigationsof proto-(galaxy)clusters in latest few days on , cool topic under fast development:

https://arxiv.org/abs/2404.18991 by Baks et al. presented deep observations with NOEMA and SCUBA-2 of HerBS-70, a binary system of bright dusty star-forming galaxies, which seems to trace a proto-cluster region at z=2.3.

franco_vazza, to Astronomy
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The shocked and radio emitting cosmic web in an old simulation of mine, I am re-analysing for an observing proposal.
(one can tell it's a old simulation because the picture is in black and white 🤭 )


franco_vazza, to random
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Ready for lunch

franco_vazza, to Astro
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todays rendering of the evolving gas density (left), temperature (centre) and magnetic field strength (right) for a thin slice through a random position in my latest 1024^3 cells simulation of a red primordial spectrum.
(Too bad a few halos appear and then disappear from the chosen slice, as they wander in the direction perpendicular to this line of sight).
ENZO-MHD simulation ran on the Leonardo cluster at CINECA using GPUs.

video/mp4

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