Gravitational wave signal of models s9-FMD-L, s9-RbR-L, s20-FMD-L, s20-RbR-L, s9-FMD-H, s9-RbR-H, s20-FMD-H, s20-RbR-H
Here you can find the gravitational wave amplitudes published in [1].
The gravitational wave amplitudes are from matter flow
only, i.e. the contribution of anisotropic neutrino emission is not included.
We provide the signals published in [1] and the underlying quadrupole moments.
The labeling convention is such that a model name is followed by three numbers indicating
the number of grid points in the radial, polar and azimuthal direction, respectively.
The label 320x040x080 corresponds to the model tag -L (low-resolution) in [1] and the label
640x080x160 correspond to the model marked -H (high-resolution) in [1]. Following the
resolution indicator, the transport scheme is marked by either -RbR (RbR+) or FMD (fully multi-dimensional).
The amplitudes are sampled with a time resolution of about 0.5 ms,
i.e. the corresponding
Nyquist frequency is about 1000 Hz.
Important: The time sampling is not uniform.
For each model, the amplitudes are given for two observer directions.
The files labeled with '_zaxis.dat' and '_xaxis.dat' contain the
amplitudes as seen by an observer viewing the simulation from
the z-axis and a-axis of the simulation grid, respectively.
Each file contains three columns. The first column gives the time since
core-bounce, in seconds. The second and third columns hold the
A_x and A_+ amplitudes, respectively. Time is given in seconds after core bounce.
In the case of making use of data from this
website, please cite the data archive by giving the weblink and
the corresponding publication, if existent. We made all
possible efforts to ensure the correctness of the data in this
archive. Errors, however, cannot be excluded. If any are found,
we would appreciate being informed.
