Hawking Radiation | Derivation | Mass as a Function | Other Functions | Analysis of Functions | Exercise | Homework Problems | Great Links





Hawking Radiation Exercise






Using the equations from the previous page, we can determine how long it would take for a 10 solar mass blackhole to evapotate.
[Graphics:Images/index_gr_15.gif]
It would be much easier if we begin by rewriting the above equation by substituting in the values for L and then for Rs.
[Graphics:Images/index_gr_16.gif]
First off, lets begin by defining our variables.
[Graphics:Images/index_gr_17.gif]
[Graphics:Images/index_gr_18.gif]
[Graphics:Images/index_gr_19.gif]
[Graphics:Images/index_gr_20.gif]
[Graphics:Images/index_gr_21.gif]
[Graphics:Images/index_gr_22.gif]
We can now combine all of our information into one single calculation (albeit a bit complex).
[Graphics:Images/index_gr_23.gif]
And thus tevap turns out to be
[Graphics:Images/index_gr_24.gif]
Converting to years would be much more easier to understand.
[Graphics:Images/index_gr_25.gif]
Finally we have
[Graphics:Images/index_gr_26.gif]
It should be noted that the current estimated age of the universe is 12.6 +/- 2.2 billion years, or about 1.26 x 1010 years!





Hawking Radiation | Derivation | Mass as a Function | Other Functions | Analysis of Functions | Exercise | Homework Problems | Great Links

Copyright 2002 by Michael Stroh