#physics

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Where the production of is useful: predicting the 3-dimensional and time-dependent volume filling factors of magnetic fields (left) and relativistic particles (right) ejected in the intergalactic medium by the activity of galaxies. Depending on the evolution of cosmic star formation, black hole activity, numerical details of feedback implementation and more, it's non obvious to derive this analytically. This is our recent best guess:


A 100 Megaparsec cubic simulated volume getting progressively filled by cosmic web structures, one layer of baryonic matter at a time ( here using 64 layers of depth 1.56 Megaparsec each).
Rendering done using in parallel using 16 cores on my MAC - the input simulation has 1024^3 cells.

The tiniest detail of the cosmic network tend to get lost as the entire distribution of matter gets added along the line of sight!

Almost exactly 15 years ago to the day, we published the first pulsar discovery with our distributed computing project / citizen science project @einsteinathome in the journal “Science”.

ℹ️ https://www.aei.mpg.de/219343/einstein-home-citizen-scientists-in-the-usa-and-germany-discover-a-new-pulsar-in-arecibo-telescope-data (press release)

📄 https://arxiv.org/abs/1008.2172 (publication on arXiv)

📄 https://www.science.org/doi/10.1126/science.1195253 (publication in Science)

💁🏻‍♀️ ICYMI: 🛞🏜️ Watch what happens when a spare tire gets launched from one of the tallest sand dunes in 's Atacama Desert—the world's driest non-polar .

This drone footage captures the tire's surprisingly long journey through the desert . The team behind this is Tuk South, currently trekking in Piaggio tuk tuks while documenting initiatives.

👉 Learn more: https://thekidshouldseethis.com/post/how-long-will-this-tire-roll-in-chiles-atacama-desert?utm_source=mastodon&utm_medium=social&utm_campaign=new_content&utm_content=tire_roll

In order to advance our understanding of the unknown sources of ultra high energy cosmic rays (the most energetic particles in space, propagating with a kinetic energy up to a few Joules, i.e. a single particle can carry the energy of an entire fast tennis ball) we need to model their deflection by intergalactic magnetic fields 🧲. Here a collection of a few .
A) protons of 1J crossing our most realistic magnetic field model

Veil Nebula

These glowing wisps are the visible remains of a star that went supernova about 7,000 years ago. Today the supernova remnant is known as the Veil Nebula and is visible only through telescopes. In the image, red marks hydrogen gas and blue marks oxygen. First carried by shock waves, these remains of a former star now serve as seed material for other stars and planetary systems to form. (Image credit: A. Alharbi; via APOD)