Regularized Smoothed Particle Hydrodynamics: A New Approach to Simulating Magnetohydrodynamic Shocks
By S. Børve, M. Omang, J. Trulsen. 2001
141 citations recorded by the source corpus.
Subfields: Computational Mechanics
View Paper: https://www.semanticscholar.org/paper/01e21355fe96152a45bc97b0223a98e85f853ea4
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In Computational Mechanics
- Daniel J. Price
- Stephan Rosswog
- G. Lodato
- P. Hopkins
- C. Nixon
- Christoph Federrath
- C. Dobbs
- Klaus Dolag
Citations in the corpus
- Improved SPH methods for simulating free surface flows of viscous fluids (2009, methodology): “The particle regularization technique [4] and the similar one called re-meshing (or re-initialization) [5] can also be considered.”
- An MHD gadget for cosmological simulations (2008, methodology): “In the original work (Børve et al. 2001),β̂ = 1 was choosen.”
- Phantom: A Smoothed Particle Hydrodynamics and Magnetohydrodynamics Code for Astrophysics (2017, background): “The correction term is computed using the symmetric divergence operator (Børve et al., 2001; Price, 2012a; Tricco & Price, 2012) f idivB,a = −B̂ia ∑ b mb [ Ba · ∇aWab(ha) Ωaρ2a + Bb · ∇aWab(hb) Ωbρ2b ] .”
- Smoothed particle hydrodynamics and magnetohydrodynamics (2010, background): “[6] suggested an approach whereby conservation form is retained, but the monopole source term is explicitly subtracted.”
- Astrophysical smooth particle hydrodynamics (2009, methodology): “Several approaches have been developed that apply regularization techniques to overcome the problems related to particle disorder (Børve et al., 2001, 2004, 2005, 2006; Dolag and Stasyszyn, 2009).”
- The impact of magnetic fields on single and binary star formation (2007, unknown): “…in passing that a parallel but complementary approach to developing an algorithm for MHD in SPH has been undertaken by Steinar Børve and colleagues (Børve et al. 2001, 2006) based on a regularisation of the underlying particle distribution, although this algorithm has not yet been applied to star…”