393 citations · 2.4k across the 35 of their papers we have counts for
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gr-qc2014
Magnetic field amplification in hypermassive neutron stars via the magnetorotational instability
Daniel M. Siegel, Riccardo Ciolfi
Mergers of binary neutron stars likely lead to the formation of a hypermassive neutron star (HMNS), which is metastable and eventually collapses to a black hole. This merger scenar…
gr-qc2014★ 16 cited
An upper bound from helioseismology on the stochastic background of gravitational waves
Daniel M. Siegel, Markus Roth
The universe is expected to be permeated by a stochastic background of gravitational radiation of astrophysical and cosmological origin. This background is capable of exciting osci…
gr-qc2013★ 171 cited
Magnetorotational instability in relativistic hypermassive neutron stars
Daniel M. Siegel, Riccardo Ciolfi, Abraham I. Harte +1
A differentially rotating hypermassive neutron star (HMNS) is a metastable object which can be formed in the merger of neutron-star binaries. The eventual collapse of the HMNS into…