Half-life (element)

This article is about the property of radioactive elements. For the video game, see Half-Life (video game).

File:Halflife-sim.gif

Simulation of many identical atoms undergoing radioactive decay, starting with either 4 atoms per box (left) or 400 (right). The number at the top is how many half-lives have elapsed. Note the law of large numbers: With more atoms, the overall decay is more regular and more predictable.

Number of half-lives that have happened	Parts remaining	As power of 2
0	1/1	[math]\displaystyle{ 1/2^0 }[/math]
1	1/2	[math]\displaystyle{ 1/2^1 }[/math]
2	1/4	[math]\displaystyle{ 1/2^2 }[/math]
3	1/8	[math]\displaystyle{ 1/2^3 }[/math]
4	1/16	[math]\displaystyle{ 1/2^4 }[/math]
5	1/32	[math]\displaystyle{ 1/2^5 }[/math]
6	1/64	[math]\displaystyle{ 1/2^6 }[/math]
7	1/128	[math]\displaystyle{ 1/2^7 }[/math]
...	...
[math]\displaystyle{ N }[/math]	[math]\displaystyle{ 1/2^N }[/math]	[math]\displaystyle{ 1/2^N }[/math]

The half-life of a substance is the time it takes for half of the substance to decay. The word "half-life" was first used when talking about radioactive elements where the number of atoms get smaller over time. It is now used in many other situations. A Geiger-Muller detector can be used to measure the half-life; it is the time when the activity is half of the original.

Note that half-life is defined as a probability. Half-life is the expected value when half the number of atoms have decayed. Carbon-14 has a half-life of 5730 years. Taking one atom of C-14, this will either have decayed after 5730 years, or it will not. But if this experiment is repeated again and again, it will be seen that the atom decays within the half life 50% of the time.

Radioactive atoms have unstable nuclei. Their nuclei are unstable because the arrangement of protons and neutrons in them are unsteady, making them shake until that they begin to decay and change into completely different types of atoms by releasing certain types of radioactive particles, such as alpha particles, beta particles or gamma rays, and possibly by fissioning into smaller nuclei. This is known as radioactive decay. For example, a radioactive carbon-14 atom releases a beta particle to become nitrogen-14. As an example of fission decay, a Fermium-256 atom can split into Xenon-140 and Palladium-112 atoms, releasing 4 neutrons in the process.

As an example, U²³² has a half-life of about 69 years. Pu²³⁸ has a half-life of 88 years. C¹⁴, which is used to find the age of fossils, has a half-life of 5730 years.