Misplaced Pages

Photomultiplier tube

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.

This is an old revision of this page, as edited by Vercalos (talk | contribs) at 06:48, 28 February 2006 (Reverted edit by 125.190.137.42; spam). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Revision as of 06:48, 28 February 2006 by Vercalos (talk | contribs) (Reverted edit by 125.190.137.42; spam)(diff) ← Previous revision | Latest revision (diff) | Newer revision → (diff)

Photomultipliers, or photomultiplier tubes (PMT) or phototubes for short, are extremely sensitive detectors of light in the ultraviolet, visible and near infrared. These detectors multiply the signal produced from the incident light from which single photons are detectable.

Schematic of a photomultiplier tube coupled to a scintillator.

Photomultipliers are constructed from a glass vacuum tube which houses a dynode and an anode. Incident photons strike the photocathode material which is present as a thin deposit on the entry window of the device, with electrons being produced as a consequence of the photoelectric effect. These electrons are directed by the focusing electrode towards the electron multiplier, where electrons are multiplied by the process of secondary emission.

The electron multiplier consists of a number of electrodes, called dynodes. Each dynode is held at a more positive voltage than the previous one. The electrons leave the photocathode, having the energy of the incoming photon. As they move towards the first dynode they are accelerated by the electric field and arrive with much greater energy. On striking the first dynode, more low energy electrons are emitted and these, in turn, are accelerated toward the second dynode. The geometry of the dynode chain is such that a cascade occurs with an ever-increasing number of electrons being produced at each stage. Finally the anode is reached where the accumulation of charge results in a sharp current pulse indicating the arrival of a photon at the photocathode.

Photomultiplier

Amplification can be as much as 10 meaning that measurable pulses can be obtained from single photons. The combination of high gain, low noise, high frequency response and large area of collection have meant that these devices still find applications in nuclear and particle physics, astronomy, medical imaging and motion picture film scanning (telecine). Semiconductor devices like avalanche photodiodes have replaced photomultipliers in some applications, but photomultipliers are still used in most cases.

While powered, photomultipliers must be shielded from ambient light to prevent their destruction through overexcitation. If used in a location with high magnetic fields (which will curve electron paths), they are usually shielded by a layer of mu-metal.

See also

References

  • Engstrom, Ralph W., Photomultiplier Handbook, RCA (1980).
  • anon, Photomultiplier Tubes: Principles and Applications, Philips Photonics, Brive, France, (1994).
  • anon, Photomultiplier Tubes: Basics and Applications (Second Edition), Hamamatsu Photonics, Hamamatsu City, Japan, (1999).
  • Flyckt, S.O. and Marmonier, C., Photomultiplier Tubes: Principles and Applications, Photonis, Brive, France, (2003).

External links

Categories: