Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars L Rezzolla, ER Most, LR Weih The Astrophysical Journal Letters 852 (2), L25, 2018 | 865 | 2018 |
New constraints on radii and tidal deformabilities of neutron stars from GW170817 ER Most, LR Weih, L Rezzolla, J Schaffner-Bielich Physical Review Letters 120 (26), 261103, 2018 | 713 | 2018 |
Postmerger gravitational-wave signatures of phase transitions in binary mergers LR Weih, M Hanauske, L Rezzolla Physical review letters 124 (17), 171103, 2020 | 188 | 2020 |
A lower bound on the maximum mass if the secondary in GW190814 was once a rapidly spinning neutron star ER Most, LJ Papenfort, LR Weih, L Rezzolla Monthly Notices of the Royal Astronomical Society: Letters 499 (1), L82-L86, 2020 | 155 | 2020 |
On the stability and maximum mass of differentially rotating relativistic stars LR Weih, ER Most, L Rezzolla Monthly Notices of the Royal Astronomical Society: Letters 473 (1), L126-L130, 2018 | 69 | 2018 |
Two-moment scheme for general-relativistic radiation hydrodynamics: a systematic description and new applications LR Weih, H Olivares, L Rezzolla Monthly Notices of the Royal Astronomical Society 495 (2), 2285-2304, 2020 | 36 | 2020 |
Beyond moments: relativistic lattice Boltzmann methods for radiative transport in computational astrophysics LR Weih, A Gabbana, D Simeoni, L Rezzolla, S Succi, R Tripiccione Monthly Notices of the Royal Astronomical Society 498 (3), 3374-3394, 2020 | 35 | 2020 |
Optimal neutron-star mass ranges to constrain the equation of state of nuclear matter with electromagnetic and gravitational-wave observations LR Weih, ER Most, L Rezzolla The Astrophysical Journal 881 (1), 73, 2019 | 31 | 2019 |
The heavier the better: how to constrain mass ratios and spins of high-mass neutron star mergers ER Most, LR Weih, L Rezzolla Monthly Notices of the Royal Astronomical Society: Letters 496 (1), L16-L21, 2020 | 17 | 2020 |
Metastable hypermassive hybrid stars as neutron-star merger remnants: A case study M Hanauske, LR Weih, H Stöcker, L Rezzolla The European Physical Journal Special Topics 230 (2), 543-550, 2021 | 10 | 2021 |
Neutron star collisions and gravitational waves M Hanauske, LR Weih Astronomische Nachrichten 342 (5), 788-798, 2021 | 4 | 2021 |
Astrophys. Jl 852 L Rezzolla, ER Most, LR Weih L25, 2018 | 2 | 2018 |
Lattice Boltzmann approach to radiative transport in numerical astrophysics D Simeoni, A Gabbana, L Rezzolla, S Succi, R Tripiccione, L Weih APS Division of Fluid Dynamics Meeting Abstracts, E05. 006, 2020 | 1 | 2020 |
Multimessenger approaches to exploring dense matter in neutron stars L Weih NUSTAR Experiment Area, 2021 | | 2021 |
GW190814: implications on the maximum mass of neutron stars E Most, J Papenfort, L Weih, L Rezzolla APS April Meeting Abstracts 2021, KP01. 103, 2021 | | 2021 |
MAGIC: Matter in Astrophysics, Gravitational Waves, and Ion Collisions M Anton, H Matthias, W Lukas, S Jan, S Horst Nuclear Physics Review 37 (3), 272-282, 2020 | | 2020 |
Two-moment scheme for general-relativistic radiation hydrodynamics: a systematic description and new applications L Rezzolla, H Olivares, LR Weih | | 2020 |
New constraints on radii and tidal deformabilities of neutron stars from GW170817: supplemental material ER Most, LR Weih, L Rezzolla, J Schaffner-Bielich | | |
StabilityofDi erentiallyRotatingNeutronStars LR Weih, L Rezzolla | | |