GRMHD conservation and declared boundary data
Research context
research method · conditional · As of 2026-10-10
Ideal GRMHD evolves rest-mass and stress-energy conservation with magnetic induction in a specified spacetime.
Key knowledge
Ideal GRMHD evolves rest-mass and stress-energy conservation with magnetic induction in a specified spacetime. Initial magnetic topology, accretion supply, inner/outflow boundaries and divergence handling influence the solution; radiation requires an additional exchange system.
Values and equations
∇μ(ρ u^μ)=0; ∇μ T^(μν)=0
- ρ
- Rest-mass density
- u^μ
- Four-velocity
- T^(μν)
- Matter plus electromagnetic stress-energy tensor
- ∇μ
- Metric-compatible covariant derivative
Conditions and scope
- Set the metric/sign/unit convention; displayed covariant laws use a consistent relativistic tensor convention.
- Ideal fluid closure does not resolve kinetic reconnection or nonthermal electron heating.
- Total nonradiating ideal-MHD system in prescribed or consistently evolved spacetime; coupling to radiation separates matter and radiation exchange while conserving their sum.
Sources · 1
References
Sources retain their recorded scope. A source link alone does not establish verification of every statement.
Evidence and review
HARM: a numerical scheme for GRMHD: Section 2: covariant conservation/stress tensor; Sections 3–4: boundary and test problems (selected source body inspected).
2026-10-10 · Bounded source check of the recorded statement and conditions. This does not certify a unique physical model, reproduce the cited study or replace independent branch review.
Entry details
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- research-earth-grmhd-conservation
- Revision
- research.1
- Structured reference record
- Postgraduate & research reference