Published August 8, 2019 | Version v1

Optimal neutron-star mass ranges to constrain the equation of state of nuclear matter with electromagnetic and gravitational-wave observations: Animated Fig. 1

  • 1. Institut für Theoretische Physik, Goethe Universität Frankfurt am Main, Germany

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This repository includes the animated version of Fig. 1 in https://arxiv.org/abs/1905.04900.

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Fig1_animated_0.83MB_per_s.mp4

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