HPC Tier Module
NewtonianPreflight - Einstein Toolkit run check
Paste a Cactus .par and get a verdict before you spend the allocation.
This tool runs inside GDBS HPC. What it computes and the authorities it applies are below.
What it is
Paste a Cactus .par and get a verdict before you spend the allocation.
Honest scope
Deterministic and citation-backed: every figure is exact arithmetic or a cited rule. Any year- or jurisdiction-indexed value is a confirmable input, never an eternal hardcode. This is a computation tool, not professional (legal, tax, medical, or financial) advice - confirm against the controlling authority for your context.
Authorities cited
- Baumgarte & Shapiro (1999). On the numerical integration of Einstein field equations. Phys. Rev. D 59, 024007.
- Shibata & Nakamura (1995). Evolution of three-dimensional gravitational waves. Phys. Rev. D 52, 5428.
- Bernuzzi & Hilditch (2010). Constraint violation in free evolution schemes: comparing BSSNOK with a conformal decomposition of Z4. Phys. Rev. D 81, 084003.
- Alcubierre et al. (2003). Gauge conditions for long-term numerical black hole evolutions. Phys. Rev. D 67, 084023.
- Brill & Lindquist (1963). Interaction energy in geometrostatics. Phys. Rev. 131, 471.
- Bowen & York (1980). Time-asymmetric initial data for black holes. Phys. Rev. D 21, 2047.
- Loffler et al. (2012). The Einstein Toolkit: a community computational infrastructure. Class. Quantum Grav. 29, 115001.
- Alcubierre et al. (2004). Towards standard testbeds for numerical relativity. Class. Quantum Grav. 21, 589. (Apples-with-Apples - cited as the protocol NOT run here.)
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Run it on your own data
Open it inside GDBS to save runs to Sandbox, attach results to a Worklog case, or share through a Gate client portal - all in the browser, nothing uploaded to anyone’s cloud.