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Accretion disk

Viscous evolution of an accretion disk

{c}

In a steady Keplerian accretion disk with zero inner torque,
$$
\bar\nu\Sigma=\frac{\dot M}{3\pi}\left[1-\left(\frac{r_{\rm in}}r\right)^{1/2}\right].
$$


Keplerian accretion disk

Past exam of the mathematics course of the University of Cambridge / 2024 / iii / Paper 321 / 1 / a / Solution

Past exam of the mathematics course of the University of Cambridge / 2024 / iii / Paper 321 / 1 / c / i / Solution

Past exam of the mathematics course of the University of Cambridge / 2025 / iii / Paper 321 / 1 / b / ii / Solution

Keplerian accretion disk

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Keplerian accretion disk

 Ancestors (7)

 Incoming links (3)

 Discussion (0)  Subscribe (1)

 Articles by others on the same topic (0)

 Discussion (0)