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-Models A1BxGy
-Models A2BxGy
-Models A3BxGy
-Models A4BxGy

Axisymmetric Core Collapse
Relativistic Hydrodynamics
Waveform Catalog

Departamento de Astronomía y Astrofísica

Universidad de Valencia

These figures contain the time evolution of the maximum density and the signal amplitude for all 26 simulated models. The solid and dashed lines denote the simulations in relativistic and Newtonian gravity, respectively.

The signal amplitude A^E2₂₀ can be converted to the strain h^TT in the equatorial plane at a distance r from the source by the following expression:

The vertical dotted lines mark the time of peak maximum density (time of bounce), and the horizontal dotted lines in the density plots mark nuclear matter density, which we define as 2.0 ^. 10¹⁴ g/cm³.

For non-toroidal models, the maximum density is identical to the central density.

• Models A1BxGy:

  (The figures are gzipped.)

  Models A1B1G1 and A1B2G1	Models A1B3G1 and A1B3G2
  Models A1B3G3 and A1B3G5

• Models A2BxGy:

  (The figures are gzipped.)

  Model A2B4G1

• Models A3BxGy:

  (The figures are gzipped.)

  Models A3B1G1 and A3B2G1	Models A3B2G2 and A3B2G4_soft
  Models A3B2G4 and A3B3G1	Models A3B3G2 and A3B3G3
  Models A3B3G5 and A3B4G2	Model A3B5G4

• Models A4BxGy:

  (The figures are gzipped.)

  Models A4B1G1 and A4B1G2	Models A4B2G2 and A4B2G3
  Models A4B4G4 and A4B4G5	Models A4B5G4 and A4B5G5