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Astrophysics/eddington limit

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Question
Hi, here is my question. If you can help me I will really appreciate... I am confuse about how can I relate z and eddington limit ``There have been claims of existence of a 3x10^9 M  black hole at a redshift of 6.4 ( Willott et al 2003 ). Use this to derive constraints on the formation redshift, initial mass and accretion rate of black hole. For example,if the initial mass was 100M and the black hole continually accreted at the Eddington rate (assuming radiative efficiency of 10 % of the rest mass energy : η= 0.1 ), what was the formation redshift for this black hole? ``

Answer
This really sounds like your astrophysics homework, so I'm going to only give you my opinion on how to start.  Answering this in full detail is probably a bit beyond the scope of this forum anyhow (and black holes are a bit outside my specialty, I'm a nuclear reaction guy).

The redshift gives you the distance (ala Hubble) and the rate of recession.  The Eddington rate assumption and the mass should give you the age if you integrate properly, meaning you should be able to work backwards to find the formation time.  Then you should be able to work back again to find its formation redshift.

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Steve Nelson

Expertise

Fusion, solar flares, cosmic rays, radiation in space, and stellar physics questions. Generally, nuclear-related astrophysics, but I can usually point you in the right direction if it's not nuclear-related or if it's nuclear but not astrophysics.

Experience

Currently a physics professor at the University of Texas of the Permian Basin. Doctoral dissertation was on a reaction in CNO-cycle fusion, worked in gamma-ray astronomy in the space science division of the naval research laboratory in the high-energy space environment branch.

Organizations
Physics professor at the University of Texas of the Permian Basin.

Education/Credentials
Ph.D. in physics, research was on nuclear fusion reactions important in stellar fusion.

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