Dataset: Evaluating approximate asymptotic distributions for fast neutrino flavor conversions in a periodic 1D box
Authors/Creators
- 1. GSI Helmholtzzentrum für Schwerionenforschung, Planckstraße 1, 64291 Darmstadt, Germany
- 2. Institute of Physics, Academia Sinica, Taipei 11529, Taiwan; Institute of Astronomy and Astrophysics, Academia Sinica, Taipei 10617, Taiwan; Physics Division, National Center for Theoretical Sciences, Taipei 10617, Taiwan
- 3. Max-Planck-Institut für Physik (Werner-Heisenberg-Institut), Föhringer Ring 6, D-80805 München, Germany
- 4. Institute of Physics, Academia Sinica, Taipei 11529, Taiwan
- 5. National Center for High-performance Computing, National Applied Research Laboratories, Hsinchu 30076, Taiwan
Description
In this data package we include two txt files and two zip files.
The file Gaussian.txt contains 4 columns. The first column shows the indices of the file numbers contained in the file Gaussian_100.zip. The second, third, and fourth columns list the corresponding \(I_{\bar\nu}\), \(F_\nu\), and \(F_{\bar\nu}\), respectively.
The file Maxent.txt contains 5 columns. The first column shows the indices of the file numbers contained in the file Maxent_100.zip while the second column lists the corresponding indices in the file Gaussian.txt. The third, fourth, and fifth columns list the corresponding \(I_{\bar\nu}\), \(F_\nu\), and \(F_{\bar\nu}\), respectively.
Files Gaussian_100 and Maxent_100 give the asymptotic simulated outcomes of fast neutrino flavor conversions with the initial Gaussian and maximum-entropy distributions, respectively. Each data file xxxx.dat lists four columns for \(v_z\), \(P_{ee}(v_z)\), \(g_\nu(v_z)\), and \(g_{\bar\nu}(v_z)\), respectively. We take 100 \(v_z\) grids for all data.