1,394 karma · joined February 28, 2017
The largest instrument to observe cosmic rays is the Pierre Auger Observatory in Argentina, which has detectors placed on an area of over 3000 km².
These are charged particles (protons and fully ionized heavier nuclei), so electromagnetism is a much more efficient way to reach high energies.
All currently proposed mechanisms for cosmic ray acceleration involve turbulent plasmas and shock fronts that reflect particles magnetically, giving them a small bump in energy each time [1] or rotating magnetic fields [2] in sufficiently extreme environments.
[1] https://en.wikipedia.org/wiki/Fermi_acceleration
[2] https://en.wikipedia.org/wiki/Centrifugal_acceleration_(astr...
Gravity just doesn't play a direct role for accelerating charged particles, it's much too weak compared to the electromagnetic force for a charged particle.
Detectors are relatively cheap and come out of the box for citizen science projects, this project is relatively well known: http://www.cosmicwatch.lns.mit.edu/
For high energy cosmic rays, you need to observe many of these secondary particles that are produced during the absorption with high temporal resolution, few nanoseconds, to be able to tell anything about their properties.
There are essentially five or so detection principles for measuring cosmic rays at the ground, and many observatories combine multiple techniques.
First, you can observe the secondary particles that reach the ground, mainly muons and electrons. This is possible either using water tanks with photosensors inside detecting Cherenkov light or using scintillators like in the project I linked above.
Then you can also detect very short and faint light that is also emitted in the air shower. This also comes in two variants: Cherenkov light is emitted in a cone around the charged particles and results in a "light pool" of roughly 250m diameter on the ground. Fluorescence light is emitted in all directions. We build optical telescopes with extremely fast and sensitive cameras to detect Cherenkov or fluorescence light.
Last, there is also radio emission from air showers, you can detect with antennas.
Auger in Argentina combines water tanks, scintillators and fluorescence telescopes and is investigating adding in radio antennas.
Telescope Array, the experiment which measured this event here, is using scintillators and fluorescence telescopes.
https://en.m.wikipedia.org/wiki/Fermi_acceleration
Directly, I say, because the objects that are extreme enough to produce such environments are indeed essentially fueled by gravitation energy: supermassive black holes at the centers of galaxies, super nova explosions, colliding neutron stars, ...
https://www.researchgate.net/figure/A-modern-adaption-of-the...
Nothing about humor, just a father calling his son similar to himself.
Seems his full name is Þorvaldur Þórðarson.
Why use Charge and not energy? Because the voltage changes as the battery is discharging, so it's not as straight forward as just multiplying with the voltage.
I guess most of the legacy code for which they do this risk assessment is Fortran 77. Not any more modern.
And getting it up to date to modern fortran would be as much effort as any other modern language.
The problem is the lack of an analytical solution and the different systematic errors that come from different numerical approaches and assumptions made.
According to the article, there are multiple standard model theory predictions using different approaches which are in tension.
In this case, setuptools is a drop in replacement.
> Group at the University of Sheffield estimated that the explosion was one of the largest artificial non-nuclear explosions ever recorded
Presumably, they forgot the "ever recorded" part.
It has a depreciation warning in the docs since 3.2.
It was in the "please just use argparse instead" state for a long time, this "just" adds an actual code warning.
https://www.wolframalpha.com/input?i=1+inch+%2F+72+%2F+2%5E1...
A high energy physics simulation library
From the article:
> Keep in mind that older PDFs created with Type 1 fonts are safe—as long as their font data was embedded in the PDF when it was made. PDF readers, whether from Adobe or elsewhere, will continue to render these documents as they always have.