Self-interacting Dark Matter Alexander Dreichner
Description: Self-interacting Dark Matter Alexander Dreichner (ITP, Goethe-University Frankfurt) Gravothermal fluid Model Numerical approach Hydrostatic adjustment step Initial Data Hydrostatic equilibrium? BH mass reached? Add BH mass Conduct heat Yes
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slide1. Self-interacting Dark Matter Alexander Dreichner (ITP, Goethe-University Frankfurt)<br>
slide2. Gravothermal fluid Model<br>
slide3. Numerical approach Hydrostatic adjustment step Initial Data Hydrostatic equilibrium? BH mass reached? Add BH mass Conduct heat Yes Yes No No Accretion radius reached? No Accrete, resample Yes<br>
slide4. Numerical approach<br>
slide5. Numerical approach<br>
slide6. Accretion ln r ln r<br>
slide7. Accretion<br>
slide8. Result<br>
slide2. Gravothermal fluid Model<br>
slide3. Numerical approach Hydrostatic adjustment step Initial Data Hydrostatic equilibrium? BH mass reached? Add BH mass Conduct heat Yes Yes No No Accretion radius reached? No Accrete, resample Yes<br>
slide4. Numerical approach<br>
slide5. Numerical approach<br>
slide6. Accretion ln r ln r<br>
slide7. Accretion<br>
slide8. Result<br>