Black holes aren't black -after Hawking they shine!
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The Core

Calculating Hawking radiation

How bright are black holes?


The luminosity of a black body is given by the Stefan-Boltzmann formula:

L = sigma*A*T^4
sigma: Stefan-Boltzmann constant; sigma=5.67*10^-8 W*m^-2*K^-4
A: Surface area of the black body
T: Temperature in Kelvin

1st: The relevant surface area for the Hawking radiation is the surface area of a sphere with the radius of the Schwarzschild radius, because that's where the radiation originates:

A sphere
A sphere
By Team C007571, ThinkQuest 2000.

A=16*pi*G^2*M^4/c^4

We can substitute this in the formula for the luminosity:

L=32*pi*k^4*G^2*M^2*T^4/15*h^3*c^6

2nd: We have already calculated the temperature of a black hole:

T=h*c^3/16*pi^2*k*G*M

Putting this into the formula for the luminosity we get:

L=h*c^6/30720*pi^2*G^2*M^2


Some example calculations

A black hole the mass of the Earth

The luminosity of a black hole with the mass of the Earth equals:


Black hole in "The Hole Man"

The luminosity of the black hole in "The Hole Man":

35.7 gigawatts of hard gamma-radiation would certainly be absolutely deadly!


Black hole with the Luminosity of the sun

The Sun

The Sun

Courtesy of NASA.
Nix NASA Image Eechange
GRC Number: C-82-6709
Date Archived: 11/22/1982

How heavy will be a black hole with the luminosity of the sun?

M=961kg

A black hole of only 961kg of mass would have the same luminosity as the sun. And it would only be 2.85*10^-24 m across! (diameter of the Schwarzschild radius). This black hole wouldn't be visible though, because it emits deadly gamma-radiation.

 

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"Black holes aren't black - After Hawking they shine!"
Presented by Angie, Matthias and Thorsten
Team C007571,ThinkQuest Internet Challenge 2000.
Last modified: 2000-08-02.