Built on

K. Beckwith, J. F. Hawley and J. H. Krolik, Astrophys. J
2008
Earlier work this paper cites.
Z. B. Etienne, V. Paschalidis, Y. T. Liu and S. L. Shapiro, Phys. Rev. D
2012
Earlier work this paper cites.

Similar

Z. B. Etienne, Y. T. Liu, V. Paschalidis and S. L. Shapiro, Phys. Rev. D
2012
Cited alongside, same era.
Z. B. Etienne, V. Paschalidis and S. L. Shapiro, Phys. Rev. D
2012
Cited alongside, same era.

Then

N. Stone, A. Loeb and E. Berger, ArXiv e-prints
Original
2012
Later among the works it cites.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

Numerical Relativity Simulations of Magnetized Black Hole-Neutron Star Mergers · Around

2013

Numerical Relativity Simulations of Magnetized Black Hole-Neutron Star Mergers

Etienne, Zachariah B., Liu, Yuk Tung, Paschalidis, Vasileios et al.

Original
PDF
Post on X

Understand

We present new numerical techniques we developed for launching the first parameter study of {\it magnetized} black hole--neutron star (BHNS) mergers, varying the magnetic fields seeded in the initial neutron star.

We found that magnetic fields have a negligible impact on the gravitational waveforms and bulk dynamics of the system during merger, regardless of magnetic field strength or BH spin.
In a recent simulation, we seeded the remnant disk from an unmagnetized BHNS merger simulation with large-scale, purely poloidal magnetic fields, which are otherwise absent in the full simulation.
The outcome appears to be a viable sGRB central engine.