Operating nuclear reactors, through fission processes, produce large amounts of
![](../Pictures/Equations/07.gif)
at low energy. Generally speaking, every 3 GW
th generates 6 x 10
20![](../Pictures/Equations/07.gif)
per sec.
Resultant spectrum known to ~2%
Detecting Reactor Antineutrinos
Temporal variation of the composition of nuclear fuel, leading to a time-dependent energy spectrum
![](../Pictures/Equations/07.gif)
.
To detect
![](../Pictures/Equations/07.gif)
produced by the nuclear reactor, a special kind of liquid called scintillator is used. When a
![](../Pictures/Equations/07.gif)
passes through a volume of scintillator, a chain of reactions takes place and a shower of light is produced:
The first reaction above is the inverse β-decay reaction. This example is the chain of reactions that takes place in the Daya Bay detectors; the liquid scintillator used is a 0.1% Gd-doped liquid scintillator.
The shower of light is then collected by the photomultiplier tubes (PMTs) placed on the detector wall, producing signals that are sent to computers for analysis.