... | ... | @@ -2,7 +2,7 @@ The gravitational potential entering in the source terms of the Navier-Stokes eq |
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1. **The potential from the central massive body** (primary of mass $`M_*`$):
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$`\Phi_*=-{{ G M_*} \over {r}}`$
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2. The potential form the planets of mass $m_p$.
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2. **The potential form the planets** of mass $m_p$.
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Below we consider the case of one single planet, easily extended to multiple planets.
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- In the 3 Dimensional case
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we use a cubic-potential of the form:
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... | ... | @@ -54,7 +54,7 @@ To select this choice for a simulation in the config file: |
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}
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```
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3. **The potential accounting for the acceleration of the primary (indirect terms)**
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