Cosmological growth and feedback from supermassive black holes
We develop a simple evolutionary scenario for the growth of supermassive black holes (BHs), assuming growth due to accretion only, to learn about the evolution of the BH mass function from $z=3$ to 0 and from it calculate the energy budgets of different modes of feedback. We tune the parameters of t...
| Main Authors: | , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
2013
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