Reference
[1] T. W. Baumgarte and S. L. Shapiro. Numerical Relativity: Solving Einstein’s Equations on the Computer. Cambridge University Press, Cambridge, UK, 2010. doi: 10.1017/cbo9781139193344.
[2] T. W. Baumgarte, S. L. Shapiro, and M. Shibata. Astrophys. J., 528:L29, 2000.
[3] H. Childs, E. Brugger, B. Whitlock, J. Meredith, S. Ahern, D. Pugmire, K. Biagas, M. Miller, C. Harrison, G. H. Weber, H. Krishnan, T. Fogal, A. Sanderson, C. Garth, E. W. Bethel, D. Camp, O. R¨ubel, M. Durant, J. M. Favre, and P. Navr´atil. Visit: An end-user tool for visualizing and analyzing very large data. In High Performance Visualization–Enabling Extreme-Scale Scientific Insight, pages 357–372. October 2012. doi: 10.1201/b12985.
[4] Z. B. Etienne, V. Paschalidis, R. Haas, P. M¨osta, and S. L. Shapiro. Illinoisgrmhd: an open- source, user-friendly grmhd code for dynamical spacetimes. Classical and Quantum Gravity, 32(17):175009, Aug. 2015. ISSN 1361-6382. doi: 10.1088/0264-9381/32/17/175009. URL http://dx.doi.org/10.1088/0264-9381/32/17/175009.
[5] C. Reisswig and D. Pollney. Notes on the integration of numerical relativity waveforms. Classical and Quantum Gravity, 28(19):195015, sep 2011. doi: 10.1088/0264-9381/28/19/195015. URL https://doi.org/10.1088%2F0264-9381%2F28%2F19%2F195015.
[6] M. Ruiz, A. Tsokaros, and S. L. Shapiro. Jet launching from merging magnetized binary neutron stars with realistic equations of state. Physical Review D, 104(12), dec 2021. doi: 10.1103/physrevd.104.124049. URL https://doi.org/10.1103%2Fphysrevd.104.124049
[7] M. Ruiz, A. Tsokaros, and S. L. Shapiro. General relativistic magnetohydrodynamic simulations of accretion disks around tilted binary black holes of unequal mass, 2023.
[8] N. The HDF Group, Q. Koziol, and U. O. of Science. Hdf5-version 1.12.0, 2 2020. URL https://www.osti.gov//servlets/purl/1631295.
[9] A. Tsokaros, M. Ruiz, S. L. Shapiro, and K. Ury¯u. Magnetohydrodynamic Simulations of Self-Consistent Rotating Neutron Stars with Mixed Poloidal and Toroidal Magnetic Fields. Phys. Rev. Lett., 128(6):061101, 2022. doi: 10.1103/PhysRevLett.128.061101.
[10] K. Uryu, S. Yoshida, E. Gourgoulhon, C. Markakis, K. Fujisawa, A. Tsokaros, K. Taniguchi, and Y. Eriguchi. New code for equilibriums and quasiequilibrium initial data of compact objects. IV. Rotating relativistic stars with mixed poloidal and toroidal magnetic fields. Phys. Rev. D, 100(12):123019, 2019. doi: 10.1103/PhysRevD.100.123019.