742 citations · 3.9k across the 68 of their papers we have counts for
70 papers
The neutrino magnetic moment and supernovae with strong magnetic fields
Clément Ehrhardt, Maria Cristina Volpe, Miguel Ángel Aloy +1
Despite several decades of searches, the neutrino magnetic moment remains unknown. If it is large, the neutrino evolution can be affected by its coupling to strong magnetic fields…
On the nature of oscillating modes of proto-neutron stars
Dimitra Tseneklidou, Alejandro Torres-Forne, Pablo Cerda-Duran +2
Newborn proto-neutron stars (PNS) are potential targets of gravitational wave asteroseismology, the study of the (inner) structure of stars via their oscillation modes. To prepare…
Impact of the equation of state on core collapse supernovae I: the low- instability
Marco Cusinato, Martin Obergaulinger, Miguel Ángel Aloy
Rapidly rotating core-collapse supernovae are promising sources of multimessenger emission, as non-axisymmetric dynamics in the newly formed proto-neutron star can leave characteri…
The first 3D MHD core-collapse progenitors II: Rotation, magnetic-field amplification, and magnetic topology
Adam Griffiths, Miguel-Ángel Aloy, Martin Obergaulinger
The most energetic core-collapse supernovae are thought to arise from rapidly rotating, magnetised progenitors. However, the three-dimensional pre-collapse structure of their angul…
The first 3D MHD core-collapse progenitors I: General properties, convection and nuclear burning
Adam Griffiths, Miguel-Ángel Aloy, Martin Obergaulinger
The most energetic core-collapse supernovae are thought to arise from rapidly rotating, magnetised progenitors, yet the three-dimensional structure of their pre-collapse interior r…
Subgrid modelling of MRI-driven turbulence in differentially rotating neutron stars
Miquel Miravet-Tenés, Martin Obergaulinger, Pablo Cerdá-Durán +2
Following a binary neutron star (BNS) merger, the transient remnant is often a fast-spinning, differentially rotating, magnetised hypermassive neutron star (HMNS). This object is p…