HARM3D+NUC: A new method for simulating the post-merger phase of binary neutron star mergers with GRMHD, tabulated EOS and neutrino leakage

We thank the anonymous referee, R. Foley, B. Villasenor, D. Radice, T. Piran, V. Mewes, D. Siegel, S. Rosswog, A. Janiuk, J. Miller, J. Dolence, M. C. Miller, P. Mosta, N. M. Lloyd-Ronning, A. Batta, G. Koenigsberger, D. Kasen for valuable conversations. A.M-B and E. R-R are supported by the Heising-Simons Foundation, the Danish National Research Foundation (DNRF132), NSF (AST-1911206 and AST-1852393). A.M-B is supported by the UCMEXUSCONACYT Doctoral Fellowship. B.J.K was supported by the NASA Goddard Center for Research and Exploration in Space Science and Technology (CRESST) II Cooperative Agreement under award number 80GSFC17M0002. R.OS was supported by NSF PHY-2012057 and AST-1909534. This work was made possible by the NASA TCAN award TCAN-80NSSC18K1488. Computational resources were provided by the NCSA’s Blue Waters sustained-petascale computing NSF projects OAC-1811228 and OAC-1516125, by the TACC’s Frontera NSF projects PHY20010 and AST20021, and the lux supercomputer at UC Santa Cruz, funded by NSF MRI grant AST 1828315.