Changes between Version 13 and Version 14 of u/erica/RadFeedback


Ignore:
Timestamp:
11/19/15 13:56:58 (9 years ago)
Author:
Erica Kaminski
Comment:

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  • u/erica/RadFeedback

    v13 v14  
    2222
    2323[[latex($L=\frac{1}{2} \dot{m}v^2(r)+G(\frac{M_{*}}{R_{*}}-\frac{M_{r}}{r})\dot{m}$)]]
     24
     25To first order, we make the following approximations. 1. Only mass within the accretion volume will contribute to the accretion luminosity. Thus, [[latex($r=ir_{acc}$)]] in the code. 2. We take [[latex($v(r)$)]] to be the velocity of the ith cell within the accretion volume. 3. We take [[latex($\dot m$)]] to be the 'Bondi Accretion Rate' already calculated in the code, 4. [[latex($M_{*}$)]] is the mass of the sink particle. 5. [[latex($R_{*}=\frac{1}{4}\Delta X_{min}$)]].