pith:OT5CURX3
SAETASS: Solver for Astroparticle Equation of Transport Analysis in Spherical Symmetry
SAETASS solves the time-dependent transport equation for astroparticles in spherical symmetry with a conservative finite-volume method.
arxiv:2604.18703 v2 · 2026-04-20 · astro-ph.HE · astro-ph.IM
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Claims
Our results successfully recover established steady-state limits while revealing relevant pre-equilibrium temporal dynamics across Kolmogorov, Kraichnan and Bohm diffusion regimes.
The modular operator-splitting architecture accurately manages the interplay between advection, diffusion, and losses without introducing significant numerical artifacts in combined solutions.
SAETASS is a new open-source code that solves the astroparticle transport equation in spherical symmetry using finite-volume methods and modular operator splitting, validated on test cases and applied to cosmic-ray protons.
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| First computed | 2026-06-23T01:13:05.188962Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
74fa2a46fb32b637727edd96e6f6f265ab465638b40145b04fc132b84a25b370
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/OT5CURX3GK3DO4T63WLON5XSMW \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: 74fa2a46fb32b637727edd96e6f6f265ab465638b40145b04fc132b84a25b370
Canonical record JSON
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