General relativistic neutrino transport using spectral methods
Bruno Peres, Andrew Jason Penner, Jerome Novak, Silvano Bonazzola

TL;DR
This paper introduces Lorene's Ghost, a spectral method-based code for neutrino transport in supernovae, capable of handling full energy dependence and relativistic effects with high accuracy and efficiency.
Contribution
The paper develops a new spectral method framework for relativistic neutrino transport, including derivation of the Liouville operator and implementation in a spherical shell with energy dependence.
Findings
Demonstrates convergence and conservation properties in test cases
Validates the treatment of relativistic effects in Schwarzschild metric
Shows efficient computation in six-dimensional settings
Abstract
We present a new code, Lorene's Ghost (for Lorene's gravitational handling of spectral transport) developed to treat the problem of neutrino transport in supernovae with the use of spectral methods. First, we derive the expression for the nonrelativistic Liouville operator in doubly spherical coordinates (r, theta, phi, epsilon, Theta, Phi)$, and further its general relativistic counterpart. We use the 3 + 1 formalism with the conformally flat approximation for the spatial metric, to express the Liouville operator in the Eulerian frame. Our formulation does not use any approximations when dealing with the angular arguments (theta, phi, Theta, Phi), and is fully energy-dependent. This approach is implemented in a spherical shell, using either Chebyshev polynomials or Fourier series as decomposition bases. It is here restricted to simplified collision terms (isoenergetic scattering) and…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
