- Secondary Emission Definition: Secondary emission is the emission of secondary particles from a material when hit by high-energy particles.
- Secondary Electron Emission: Secondary electron emission occurs when high-energy particles impact a surface, causing electrons to be emitted.
- Mechanisms of Emission: Secondary electron emission happens through elastic and inelastic scattering, where energy transfer enables electron escape.
- Applications: Devices like photomultiplier tubes, electron multipliers, and image intensifiers use secondary electron emission to detect or amplify weak signals.
- Challenges: Secondary electron emission can cause parasitic oscillation and negative resistance in electronic devices, requiring design adjustments to manage these effects.
Secondary electron emission occurs when an incident electron, ion or other energetic particle strikes a material and electrons leave the surface. The incident particle is the primary. Emitted low-energy electrons created by inelastic interactions are true secondary electrons. Measurements may also include elastically backscattered and rediffused primary electrons, so the reported yield must state which populations it counts.
Controlled secondary emission multiplies signals in photomultipliers, electron multipliers and image intensifiers. It also produces surface-sensitive contrast in electron microscopes. Uncontrolled multiplication can disturb vacuum and radio-frequency electronic devices, including accelerator cavities and klystron tubes. The effect does not create a universal negative resistance; its circuit consequence depends on geometry, fields and collection.
What is Secondary Electron Emission?
An energetic primary particle deposits energy through elastic and inelastic interactions. Some excited electrons travel to the surface and cross its escape barrier. Only electrons generated within a shallow escape depth are likely to emerge without losing too much energy. Material band structure, surface composition and primary-particle conditions all affect this process.
Secondary electron yield, often written δ, is the mean number of emitted secondary electrons per incident primary under stated conditions. Total electron yield may instead include true secondaries, backscattered primaries and rediffused electrons. The value is a function rather than one material constant. Important variables include:
- Bulk material, coating, oxide, adsorbates, roughness and prior electron conditioning
- Primary-particle species, kinetic energy and incidence angle
- Surface charge, temperature and the local electric field used to collect or suppress emitted electrons
- Energy cutoff and detector definition used to separate secondary, rediffused and backscattered populations
A yield curve usually rises with primary energy, reaches a maximum and then falls as energy deposition moves deeper than the escape region. Maximum yield and its corresponding energy vary with preparation and measurement method. Published values for clean pure materials can differ greatly from technical surfaces carrying oxides or contamination.
How Does Secondary Electron Emission Work?
Electron-impact measurements commonly separate elastically backscattered electrons, rediffused primary electrons and true secondary electrons. Elastic and inelastic interactions have different energy signatures.
Elastic Scattering
In elastic scattering, a primary electron changes momentum and direction while the elastic-collision model conserves total kinetic energy. A primary that returns from the surface with energy near its incident value is classed as elastically backscattered, not as a newly excited true secondary. The material’s surface barrier, including its work functions under the relevant surface condition, affects escape, but nuclear scattering and electron transport determine the backscatter path.
Inelastic Scattering
In an inelastic interaction, the primary loses energy to electronic excitations and ionisation within the solid. Excited electrons undergo further scattering as they move. A low-energy electron generated close enough to the surface may retain sufficient energy normal to the surface to escape; deeper electrons usually lose energy before reaching it. Rediffused primaries have lost some incident energy but are still distinguishable from the low-energy true-secondary population. Fixed boundaries such as 50 eV are useful detector conventions, not universal mechanism thresholds.
What are Some Applications of Secondary Electron Emission?
Devices use controlled secondary emission to amplify weak electric currents or form a surface signal:
- Photomultiplier tubes: A photocathode emits the initial electron after absorbing light. Interstage voltages accelerate electrons to a dynode chain. Each dynode emits an average number of secondary electrons set by its material and voltage, and the total gain is approximately the product of the individual stage gains. Gain can reach large values but is not fixed at one million. PMTs serve spectroscopy, scintillation counting, fast timing and low-light measurement.
- Electron multipliers and electron microscopy: A discrete-dynode multiplier uses separate electrodes, while a channel electron multiplier uses repeated impacts along a resistive channel wall. Both can detect electrons or ions in mass spectrometers and particle instruments. A scanning electron microscope instead collects low-energy secondary electrons from near the sample surface to form topographic and material-sensitive images.
- Image intensifiers: A photocathode converts an optical image into an electron distribution. A microchannel plate multiplies electrons through many small channels, and a phosphor screen converts the amplified distribution back to light. Resolution, gain, noise, lifetime and saturation depend on the complete tube rather than secondary yield alone.
What are Some Challenges of Secondary Electron Emission?
Unwanted emission matters in vacuum tubes, accelerators, spacecraft hardware and RF structures such as klystron tubes. Two common design concerns are:
- Multipactor and electron-cloud growth: An RF magnetic field and electric field can return emitted electrons to a surface at a resonant phase. If effective yield exceeds one over successive impacts, the population grows and can cause heating, desorption, noise or breakdown. Mitigation uses geometry, field analysis, surface conditioning, low-yield coatings, grooves, shields or suitable bias voltages, validated for the operating mode.
- Collector-current and feedback errors: Electrons leaving an anode, grid or collector can reduce measured current, reach another electrode or feed an unwanted mode. Suppression grids, magnetic or electrostatic design and low-yield surfaces may keep these electrons from returning to sensitive regions. The correct remedy follows a trajectory and circuit analysis; increasing secondary yield is not a general cure.
Conclusion
Secondary electron emission is electron release following energetic particle impact on a material. A report should distinguish true secondaries from elastically backscattered and rediffused primaries.
Yield is the mean number emitted per incident primary under stated conditions. It varies with primary energy, angle, material, surface condition and measurement definition.
Elastic scattering mainly redirects primary electrons, while inelastic energy deposition creates excitations that can escape as low-energy true secondaries near the surface.
Photomultipliers, electron multipliers, image intensifiers and scanning electron microscopes use controlled emission for gain or imaging.
In RF and vacuum systems, multipactor, electron-cloud growth and collector feedback require control through geometry, fields, surface treatment and operating conditions.





