Should One Use the Ray-by-Ray Approximation in Core-Collapse Supernova Simulations?
M. Aaron Skinner, A. Burrows, and J.C. Dolence

TL;DR
This study compares the ray-by-ray+ approximation with full multi-dimensional transport in 2D core-collapse supernova simulations, revealing that the approximation can lead to misleadingly larger shock radii and potentially incorrect explosion outcomes.
Contribution
It provides the first self-consistent 2D comparison between ray-by-ray+ and full multi-D transport methods in supernova modeling, highlighting significant discrepancies.
Findings
Ray-by-ray+ produces larger shock radii than multi-D transport.
Ray-by-ray+ can artificially favor explosion conditions.
Full multi-D transport may prevent explosions predicted by ray-by-ray+.
Abstract
We perform the first self-consistent, time-dependent, multi-group calculations in two dimensions (2D) to address the consequences of using the ray-by-ray+ transport simplification in core-collapse supernova simulations. Such a dimensional reduction is employed by many researchers to facilitate their resource-intensive calculations. Our new code (F{\sc{ornax}}) implements multi-D transport, and can, by zeroing out transverse flux terms, emulate the ray-by-ray+ scheme. Using the same microphysics, initial models, resolution, and code, we compare the results of simulating 12-, 15-, 20-, and 25-M progenitor models using these two transport methods. Our findings call into question the wisdom of the pervasive use of the ray-by-ray+ approach. Employing it leads to maximum post-bounce/pre-explosion shock radii that are almost universally larger by tens of kilometers than those derived…
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