Full 3D numerical relativity simulations of neutron star–boson star collisions with BAM
With the first direct detections of gravitational waves (GWs) from the coalescence of compact binaries observed by the advanced LIGO and VIRGO interferometers, the era of GW astronomy has begun. Whilst there is strong evidence that the observed GWs are connected to the merger of two black holes (BH)...
Principais autores: | Dietrich, T, Ossokine, S, Clough, K |
---|---|
Formato: | Journal article |
Publicado em: |
Institute of Physics
2018
|
Registros relacionados
-
Axion star collisions with black holes and neutron stars in full 3D numerical relativity
por: Clough, K, et al.
Publicado em: (2018) -
Neutron star–axion star collisions in the light of multimessenger astronomy
por: Dietrich, T, et al.
Publicado em: (2018) -
Boson and neutron stars with increased density
por: Yves Brihaye, et al.
Publicado em: (2020-12-01) -
Numerical Simulations of Dark Matter Admixed Neutron Star Binaries
por: Mattia Emma, et al.
Publicado em: (2022-07-01) -
The Effects of Self-interacting Bosonic Dark Matter on Neutron Star Properties
por: Edoardo Giangrandi, et al.
Publicado em: (2023-01-01)