Electron multiplier

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Contrasting differences between discrete and continuous electron multipliers. Discrete and Continuous Dynode Systems.jpg
Contrasting differences between discrete and continuous electron multipliers.

An electron multiplier is a vacuum-tube structure that multiplies incident charges. [1] In a process called secondary emission, a single electron can, when bombarded on secondary-emissive material, induce emission of roughly 1 to 3 electrons. If an electric potential is applied between this metal plate and yet another, the emitted electrons will accelerate to the next metal plate and induce secondary emission of still more electrons. This can be repeated a number of times, resulting in a large shower of electrons all collected by a metal anode, all having been triggered by just one.

Contents

History

In 1930, Russian physicist Leonid Aleksandrovitch Kubetsky proposed a device which used photocathodes combined with dynodes, or secondary electron emitters, in a single tube to remove secondary electrons by increasing the electric potential through the device. The electron multiplier can use any number of dynodes in total, which use a coefficient, σ, and created a gain of σn where n is the number of emitters. [2]

Discrete dynode

Secondary electron emission begins when one electron hits a dynode inside a vacuum chamber and ejects electrons that cascade onto more dynodes and repeats the process over again. The dynodes are set up so that each time an electron hits the next one it will have an increase of about 100 electron Volts greater than the last dynode. Some advantages of using this include a response time in the picoseconds, a high sensitivity, and an electron gain of about 108 electrons. [3]

A discrete electron multiplier Venetian blind electron multiplier.jpg
A discrete electron multiplier

Continuous dynode

A continuous dynode system uses a horn-shaped funnel of glass coated with a thin film of semiconducting materials. The electrodes have increasing resistance to allow secondary emission. Continuous dynodes use a negative high voltage in the wider end and goes to a positive near ground at the narrow end. The first device of this kind was called a Channel Electron Multiplier (CEM). CEMs required 2-4 kilovolts in order to achieve a gain of 106 electrons.

Continuous-dynode electron multiplier Cont dynode detector.jpg
Continuous-dynode electron multiplier

Microchannel plate

Another geometry of continuous-dynode electron multiplier is called the microchannel plate (MCP). [4] [5] It may be considered a 2-dimensional parallel array of very small continuous-dynode electron multipliers, built together and powered in parallel. Each microchannel is generally parallel-walled, not tapered or funnel-like. MCPs are constructed from lead glass and carry a resistance of 109 Ω between each electrode. Each channel has a diameter of 10-100 μm. The electron gain for one microchannel plate can be around 104-107 electrons. [5]

Microchannel plate with breakdown MicrochannelplateWithBreakdown.jpg
Microchannel plate with breakdown

Applications

Instruments

In mass spectrometry electron multipliers are often used as a detector of ions that have been separated by a mass analyzer of some sort. They can be the continuous-dynode type and may have a curved horn-like funnel shape or can have discrete dynodes as in a photomultiplier. Continuous dynode electron multipliers are also used in NASA missions and are coupled to a gas chromatography mass spectrometer (GC-MS) which allows scientists to determine the amount and types of gasses present on Titan, Saturn's largest moon. [6]

Night-vision

Microchannel plates are also used in night-vision goggles. As electrons hit the millions of channels, they release thousands of secondary electrons. These electrons then hit a phosphor screen where they are amplified and converted back into light. The resulting image patterns the original and allows for better vision in the dark, while only using a small battery pack to provide a voltage for the MCP. [7]

See also

Related Research Articles

<span class="mw-page-title-main">Vacuum tube</span> Device that controls current between electrodes

A vacuum tube, electron tube, valve, or tube, is a device that controls electric current flow in a high vacuum between electrodes to which an electric potential difference has been applied.

<span class="mw-page-title-main">X-ray fluorescence</span> Emission of secondary X-rays from a material excited by high-energy X-rays

X-ray fluorescence (XRF) is the emission of characteristic "secondary" X-rays from a material that has been excited by being bombarded with high-energy X-rays or gamma rays. The phenomenon is widely used for elemental analysis and chemical analysis, particularly in the investigation of metals, glass, ceramics and building materials, and for research in geochemistry, forensic science, archaeology and art objects such as paintings.

<span class="mw-page-title-main">Photomultiplier tube</span> Fast, high sensitivty, low noise electronic photon detector

Photomultiplier tubes (photomultipliers or PMTs for short) are extremely sensitive detectors of light in the ultraviolet, visible, and near-infrared ranges of the electromagnetic spectrum. They are members of the class of vacuum tubes, more specifically vacuum phototubes. These detectors multiply the current produced by incident light by as much as 100 million times or 108 (i.e., 160 dB), in multiple dynode stages, enabling (for example) individual photons to be detected when the incident flux of light is low.

<span class="mw-page-title-main">Scintillation counter</span> Instrument for measuring ionizing radiation

A scintillation counter is an instrument for detecting and measuring ionizing radiation by using the excitation effect of incident radiation on a scintillating material, and detecting the resultant light pulses.

<span class="mw-page-title-main">Secondary emission</span> When a particles interactions with a material cause it to emit new particles

In particle physics, secondary emission is a phenomenon where primary incident particles of sufficient energy, when hitting a surface or passing through some material, induce the emission of secondary particles. The term often refers to the emission of electrons when charged particles like electrons or ions in a vacuum tube strike a metal surface; these are called secondary electrons. In this case, the number of secondary electrons emitted per incident particle is called secondary emission yield. If the secondary particles are ions, the effect is termed secondary ion emission. Secondary electron emission is used in photomultiplier tubes and image intensifier tubes to amplify the small number of photoelectrons produced by photoemission, making the tube more sensitive. It also occurs as an undesirable side effect in electronic vacuum tubes when electrons from the cathode strike the anode, and can cause parasitic oscillation.

<span class="mw-page-title-main">Dynode</span>

A dynode is an electrode in a vacuum tube that serves as an electron multiplier through secondary emission. The first tube to incorporate a dynode was the dynatron, an ancestor of the magnetron, which used a single dynode. Photomultiplier and video camera tubes generally include a series of dynodes, each at a more positive electrical potential than its predecessor. Secondary emission occurs at the surface of each dynode. Such an arrangement is able to amplify the tiny current emitted by the photocathode, typically by a factor of one million.

An image intensifier or image intensifier tube is a vacuum tube device for increasing the intensity of available light in an optical system to allow use under low-light conditions, such as at night, to facilitate visual imaging of low-light processes, such as fluorescence of materials in X-rays or gamma rays, or for conversion of non-visible light sources, such as near-infrared or short wave infrared to visible. They operate by converting photons of light into electrons, amplifying the electrons, and then converting the amplified electrons back into photons for viewing. They are used in devices such as night-vision goggles.

<span class="mw-page-title-main">Secondary ion mass spectrometry</span> Surface chemical analysis and imaging method

Secondary-ion mass spectrometry (SIMS) is a technique used to analyze the composition of solid surfaces and thin films by sputtering the surface of the specimen with a focused primary ion beam and collecting and analyzing ejected secondary ions. The mass/charge ratios of these secondary ions are measured with a mass spectrometer to determine the elemental, isotopic, or molecular composition of the surface to a depth of 1 to 2 nm. Due to the large variation in ionization probabilities among elements sputtered from different materials, comparison against well-calibrated standards is necessary to achieve accurate quantitative results. SIMS is the most sensitive surface analysis technique, with elemental detection limits ranging from parts per million to parts per billion.

Liquid scintillation counting is the measurement of radioactive activity of a sample material which uses the technique of mixing the active material with a liquid scintillator, and counting the resultant photon emissions. The purpose is to allow more efficient counting due to the intimate contact of the activity with the scintillator. It is generally used for alpha particle or beta particle detection.

<span class="mw-page-title-main">X-ray spectroscopy</span> Technique to characterize materials using X-ray radiation

X-ray spectroscopy is a general term for several spectroscopic techniques for characterization of materials by using x-ray radiation.

<span class="mw-page-title-main">Photodetector</span> Sensors of light or other electromagnetic energy

Photodetectors, also called photosensors, are sensors of light or other electromagnetic radiation. There is a wide variety of photodetectors which may be classified by mechanism of detection, such as photoelectric or photochemical effects, or by various performance metrics, such as spectral response. Semiconductor-based photodetectors typically photo detector have a p–n junction that converts light photons into current. The absorbed photons make electron–hole pairs in the depletion region. Photodiodes and photo transistors are a few examples of photo detectors. Solar cells convert some of the light energy absorbed into electrical energy.

Gamma-ray spectroscopy is the qualitative study of the energy spectra of gamma-ray sources, such as in the nuclear industry, geochemical investigation, and astrophysics. Gamma-ray spectrometry, on the other hand, is the method used to acquire a quantitative spectrum measurement.

<span class="mw-page-title-main">Faraday cup</span> Charged particle catcher

A Faraday cup is a metal (conductive) cup designed to catch charged particles in vacuum. The resulting current can be measured and used to determine the number of ions or electrons hitting the cup. The Faraday cup was named after Michael Faraday who first theorized ions around 1830.

<span class="mw-page-title-main">Hot-filament ionization gauge</span>

The hot-filament ionization gauge, sometimes called a hot-filament gauge or hot-cathode gauge, is the most widely used low-pressure (vacuum) measuring device for the region from 10−3 to 10−10 Torr. It is a triode, with the filament being the cathode.

<span class="mw-page-title-main">WITCH experiment</span>

WITCH, or experiment IS433, is a double Penning trap experiment to measure the recoil energy of decaying nuclei. A spectrometer in combination with a position-sensitive microchannel plate detector is used to count ions while scanning their energy. The experiment is located at the ISOLDE Radioactive Ion Beam Facility in CERN. The beam from ISOLDE is bunched by REXTRAP after which it is transferred to the WITCH set-up.

<span class="mw-page-title-main">Daly detector</span> Type of gas-phase ion detector

A Daly detector is a gas-phase ion detector that consists of a metal "doorknob", a scintillator and a photomultiplier. It was named after its inventor Norman Richard Daly. Daly detectors are typically used in mass spectrometers.

<span class="mw-page-title-main">Time-of-flight mass spectrometry</span> Method of mass spectrometry

Time-of-flight mass spectrometry (TOFMS) is a method of mass spectrometry in which an ion's mass-to-charge ratio is determined by a time of flight measurement. Ions are accelerated by an electric field of known strength. This acceleration results in an ion having the same kinetic energy as any other ion that has the same charge. The velocity of the ion depends on the mass-to-charge ratio. The time that it subsequently takes for the ion to reach a detector at a known distance is measured. This time will depend on the velocity of the ion, and therefore is a measure of its mass-to-charge ratio. From this ratio and known experimental parameters, one can identify the ion.

<span class="mw-page-title-main">Microchannel plate detector</span> Detection single parties and photons

A microchannel plate (MCP) is used to detect single particles and photons. It is closely related to an electron multiplier, as both intensify single particles or photons by the multiplication of electrons via secondary emission, however because a microchannel plate detector has many separate channels, it can additionally provide spatial resolution.

<span class="mw-page-title-main">Ion-to-photon detector</span>

An ion-to-photon detector (IPD) is a component used for detecting ions in mass spectrometry.

<span class="mw-page-title-main">MIRACLS experiment</span>

The Multi Ion Reflection Apparatus for Collinear Spectroscopy (MIRACLS) is a permanent experiment setup being constructed at the ISOLDE facility at CERN. The purpose of the experiment is to measure properties of exotic radioisotopes, from precise measurements of their hyperfine structure. The technique used for measurements is laser spectroscopy, which MIRACLS aims to increase the sensitivity of by trapping ion bunches in an ion trap.

References

  1. Allen, James S. (1947), "An Improved Electron Multiplier Particle Counter", Review of Scientific Instruments, 18 (10): 739–749, Bibcode:1947RScI...18..739A, doi:10.1063/1.1740838 .
  2. Lubsandorzhiev, B.K. (ed.). On the history of photomultiplier tube invention (PDF). CERN. Institute for Nuclear Research of RAS: CERN.
  3. Tao, S., Chan, H., & van der Graaf, H. (2016). Secondary Electron Emission Materials for Transmission Dynodes in Novel Photomultipliers: A Review. Materials, 9(12), 1017. https://doi.org/10.3390/ma9121017
  4. Burroughs, E. G. (1969), "Collection Efficiency of Continuous Dynode Electron Multiple Arrays", Review of Scientific Instruments, 40 (1): 35–37, Bibcode:1969RScI...40...35B, doi:10.1063/1.1683743
  5. 1 2 Wiza, Joseph L. (1979), "Microchannel plate detectors", Nuclear Instruments and Methods, 162 (1–3): 587–601, Bibcode:1979NucIM.162..587L, CiteSeerX   10.1.1.119.933 , doi:10.1016/0029-554X(79)90734-1 .
  6. Mahaffy, Paul. "Mass Spectrometer: Detector". NASA.
  7. Montoro, Harry. "Image Intensification: The Technology of Night Vision". Photonics.