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20172022
most citedSimulating neutron star mergers with the Lagrangian Numerical Relativity code SPHINCS_BSSN

14 citations · 16 across the 2 of their papers we have counts for

collaborators

8 papers

astro-ph.HE202214 cited

Simulating neutron star mergers with the Lagrangian Numerical Relativity code SPHINCS_BSSN

P. Diener, S. Rosswog, F. Torsello

We present the first neutron star merger simulations performed with the newly developed Numerical Relativity code SPHINCS_BSSN. This code evolves the spacetime on a mesh using the…

gr-qc2019

On the stability of bimetric structure formation

Marcus Högås, Francesco Torsello, Edvard Mörtsell

Bimetric gravity can reproduce the accelerated expansion of the Universe, without a cosmological constant. However, the stability of these solutions to linear perturbations has bee…

gr-qc2019

Generalized Vaidya solutions in bimetric gravity

Marcus Högås, Mikica Kocic, Francesco Torsello +1

In general relativity, the endpoint of spherically symmetric gravitational collapse is a Schwarzschild--[(A)dS] black hole. In bimetric gravity, it has been speculated that a stati…

cs.SC2019

: A Mathematica package for exact computations in bimetric relativity

Francesco Torsello

We present , a Mathematica package for exact computations in 31 bimetric relativity. It is based on the bundle, which can handle computations inv…

gr-qc2019

The mean gauges in bimetric relativity

Francesco Torsello

The choice of gauge in numerical relativity is crucial in avoiding coordinate and curvature singularities. In addition, the gauge can affect the well-posedness of the system. In th…

gr-qc2019

Covariant BSSN formulation in bimetric relativity

Francesco Torsello, Mikica Kocic, Marcus Högås +1

Numerical integration of the field equations in bimetric relativity is necessary to obtain solutions describing realistic systems. Thus, it is crucial to recast the equations as a…