What Is the Luminosity of Emitted Radiation from a Black Hole Accreting Mass?

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SUMMARY

The luminosity of emitted radiation from a black hole accreting mass can be expressed as L = η * \dot{M} * c², where L is luminosity, η is the efficiency of energy conversion, and \dot{M} is the mass accretion rate. This relationship is derived from the principle that the energy emitted (ΔE) over time (Δt) corresponds to the rate of mass accretion multiplied by the energy conversion efficiency. The discussion emphasizes the importance of understanding luminosity as a rate of energy emission rather than merely energy output.

PREREQUISITES
  • Understanding of black hole physics
  • Familiarity with the concepts of mass accretion rates
  • Knowledge of energy conversion efficiency (η)
  • Basic grasp of the equation E = mc²
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  • Research the concept of black hole accretion disks
  • Learn about the efficiency of energy conversion in astrophysical processes
  • Study the relationship between temperature, radius, and luminosity in stellar objects
  • Explore the implications of luminosity in the context of general relativity
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bowlbase
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Homework Statement


Suppose that a black hole of mass M accretes mass at a rate ##\dot{M}##. Further suppose that accretion of mass Δm leads to the radiation of energy ##\Delta E= \eta Δmc^2##, for some effeciency of energy conversion, ##\eta##. What is the luminosity of emitted radiation in terms of ##\dot{M}## and ##\eta##?

Homework Equations


Luminosity equation, sort of?

The Attempt at a Solution


The only equation I've ever seen for luminosity has been in terms of temperature and radius. So I'm at a loss here where to go with this. I understand that luminosity is the amount of energy an object gives off over time but I'm sure I can't just put that ΔE over a Δt and call it good. This is suppose to be a simple question but I'm just not making the connections I need to solve it.
 
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Edited for clarification. Currently my answer is just the ΔE over 4pi. Anyone have a suggestion for this?
 
bowlbase said:
Edited for clarification. Currently my answer is just the ΔE over 4pi. Anyone have a suggestion for this?

Ok. I'm not an expert but I really don't see any other way to go with this. Luminosity is dE/dt as far as I know. So dE/dt=η*dM/dt*c^2=η*##\dot M##*c^2. You don't quite divide them both by Δt, but it's really almost the same thing. You said this is an easy question, right? Maybe it is that easy. At least I don't see what else to do. I don't see what sense ΔE over 4pi makes, it has the units of energy, not energy/second.
 
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Maybe I'm just thinking too hard about this. What you have must be correct I would assume, but it makes me question why he'd even make that part of the problem set. Unless just to check if we recall what luminosity is. Anyway, thanks for the assistance.
 
bowlbase said:
Maybe I'm just thinking too hard about this. What you have must be correct I would assume, but it makes me question why he'd even make that part of the problem set. Unless just to check if we recall what luminosity is. Anyway, thanks for the assistance.

Yes, it does seem too easy. Let me know if I've missed something important.
 

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