BBC Home

Explore the BBC

h2g2
28th December 2009
Accessibility help
Text only

Guide ID: A568514 (Edited)

Edited Guide Entry


SEARCH h2g2
Edited Entries only
Search h2g2Advanced Search


New visitors: Create your membership
Returning members: Sign in
BBC Homepage
The Guide to Life, The Universe and Everything.

2. The Universe / General Astronomy
3. Everything / Maths, Science & Technology / Astronomy

Created: 8th June 2001
Hawking Radiation
Contact Us


Like this page?
Send it to a friend!

 

Hawking radiation is a theoretical phenomenon first proposed by (and named after) the famous astrophysicist, Dr Stephen Hawking.

What is Hawking Radiation?

According to certain principles of quantum mechanics, the probability of any event occurring is always greater than zero. One of the stranger consequences of this idea is that what we think of as 'empty' space isn't really empty at all; it's filled with 'virtual particles', bits of matter and energy that are almost, but not quite, real. Despite being unreal, virtual particles play a vital role in the descriptions of how the universe works on the quantum scale; they're necessary to explain how photons and electrons interact, for example.

Under normal conditions, virtual particles rarely have any noticeable effects. In certain unusual environments, such as the intense gravitational fields generated by black holes, they can 'borrow' energy from their surroundings and temporarily become real. When virtual particles manifest themselves, they must always do so in pairs of particles and anti-particles, which cancel each other out and release their energy back into the void. However, it is possible for the particles to materialise just on the edge of the event horizon, the boundary that separates the 'inside' and the 'outside' of the black hole. When this occurs, one particle is sometimes consumed by the black hole while the other escapes. The escaping particle carries away a tiny fragment of the black hole's mass, the extra energy that allowed it to become real. Over long periods of time, the black hole will eventually evaporate, losing all of its energy to escaping particles. These particles are the Hawking radiation.

An unusual aspect of Hawking radiation is that it may be a proof of the 'arrow of time'. According to classical physics, the universe is time-reversible; anything that happens in the universe could just as easily happen 'backwards' as 'forwards'. For instance, it's possible in theory to reconstruct the content of a burnt newspaper by examining the pattern of the ashes, combustion products, and electromagnetic radiation produced by the fire. However, it's clear that time only flows 'forwards', a phenomenon that has been referred to as 'time's arrow'. Scientists have never been able to understand why this is so, despite many attempts at explanation. It has been suggested that the decay of certain subatomic particles can only happen in one direction, although this has never been proven. It is also thought that the aspect of uncertainty in some interpretations of quantum mechanics (specifically, the idea that a quantum event has a random outcome) might explain why time doesn't run backwards. However, the pattern of Hawking radiation emitted by a black hole bears no relationship to the pattern of matter and energy that the black hole consumed; the 'information' contained in the things that fall into the hole has essentially been erased, making it impossible to reconstruct the nature of anything that went in. This interpretation is being hotly debated in the world of quantum astrophysics at the moment, as it predicts the first example of a non-quantum violation of the laws of causality.



Clip/Bookmark this page
This article has not been bookmarked.
ENTRY DATA
Written and Researched by:

Caledonian

Edited by:

Spaceballer (Guardian of Satsumas and other orange fruit)

Referenced Entries:

Wormholes and Black Holes

Referenced Sites:

Dr Stephen Hawking

Please note that the BBC is not responsible for the content of any external sites listed.


CONVERSATION TOPICS FOR THIS ENTRY:

Start a new conversation

People have been talking about this Guide Entry. Here are the most recent Conversations:

TITLE
LATEST POST
BACKHÖLESJan 21, 2006
QuestionJan 13, 2004
hawking radiationApr 17, 2002
Too little too lateOct 25, 2001
Nice!Jun 19, 2001




Disclaimer

Most of the content on h2g2 is created by h2g2's Researchers, who are members of the public. The views expressed are theirs and unless specifically stated are not those of the BBC. The BBC is not responsible for the content of any external sites referenced. In the event that you consider anything on this page to be in breach of the site's House Rules, please click here. For any other comments, please start a Conversation above.




About the BBC | Help | Terms of Use | Privacy & Cookies Policy