Three-dimensional simulations of neutrino-driven core-collapse supernovae from low-mass single and binary star progenitors
Citations
1,189 citations
Cites background from "Three-dimensional simulations of ne..."
...It is also difficult to form light NS with masses below ∼ 1.2M in current supernova explosion simulations (Burrows et al. 2019; Müller et al. 2019)....
[...]
768 citations
321 citations
175 citations
120 citations
References
3,892 citations
"Three-dimensional simulations of ne..." refers methods in this paper
...Recent updates to the code include 6th-order extremum preserving reconstruction (Colella & Sekora 2008; Sekora & Colella 2009) instead of the original 4th-order piecewise parabolic method of Colella & Woodward (1984) and an alternative scheme for filtering near the polar axis....
[...]
3,513 citations
"Three-dimensional simulations of ne..." refers background in this paper
...Yet another alternative consists in filtering the solution in Fourier space, which has a long tradition in meteorology (Boyd 2001)....
[...]
2,005 citations
"Three-dimensional simulations of ne..." refers methods in this paper
...In principle, higher-order conservative reconstruction can be used for this purpose, but we opt for piecewise linear reconstruction (typically using van Leer’s harmonic limiter; van Leer 1974)....
[...]
1,354 citations
Additional excerpts
...Approximately correcting for the binding energy of cold neutron stars following Lattimer & Prakash (2001) to obtain gravitational masses Mgrav, Mgrav ≈ Mby − 0.084M ( Mgrav M )2 , (3) we find values between 1.22M for z9....
[...]
1,188 citations
"Three-dimensional simulations of ne..." refers methods in this paper
...At high densities, we use the nuclear equation of state of Lattimer & Swesty (1991) with a bulk incompressibility of K = 220 MeV, supplemented by a low-density equation of state for nuclei, nucleons, and lepton and photon radiation....
[...]