Schwarze Löcher sind nicht schwarz - nach Hawking strahlen sie!
Chinese Version | German Version | Printable Version | Help | Search
 

The Core

How can black holes shine?

You'll need a little bit of quantum physics for this.
We'll explain it:

In quantum physics the empty space isn't empty at all. In it there are always particles flashing into existence and disappear again. They always come in pairs; one particle and one anti-particle, like an electron and a positron, or a photon (a particle of light) and another photon with opposite spin and impulse. These particles are called "virtual particles". They only exist for a very short time:

delta t = 1 / (8 * pi * f) ; where f is their frequency.


Werner Heisenberg
Max-Planck-Institute,
courtesy AIP Emilio
Segre Visual Archives.

This follows out of the Heisenberg principle of uncertainty:

Heisenberg principle of uncertainty

where delta E is the energy of the pair of virtual particles, and
h is the Planck constant.
(a natural constant, h=6.626*10^-34 J s).
Jump Calculation

The heisenberg Principle of Uncertainty:

The energy of one photon:

E= h*f

The energy of a pair of photons:


Let's do some calculations !

Example Calculation:
The life time of a photon of orange light (f=5810^14Hz) :

(80 attoseconds, one attosecond is a millionth of a millionth of a millionth of a second.)

 


BackHow big
is a black hole?
NextMore about
virtual particles

[Site Map] | [Introduction] | [The Core] | [Calculations] | [Background] | [All formulas]
[Interactive] | [Biography] | [Guest Book] | [Help] | [About]

"Black holes aren't black - After Hawking they shine!"
Presented by Angie, Matthias and Thorsten
Team C007571,ThinkQuest Internet Challenge 2000.
Last modified: 2000-08-04.