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Electromagnetic Field
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When oscillating sources produce time-varying electric field ($/entries/electric-field/$) and magnetic field ($/entries/magnetic-field/$) vectors, they decouple from their sources and propagate outward as electromagnetic waves ($/entries/electromagnetic-wave/$). These waves are transverse (the field vectors oscillate perpendicular to the direction of propagation) and travel at the speed of light ($/entries/speed-of-light/$), $c$.
The frequency ($/entrie… -
Electromagnetic Radiation
Linked via "Gamma Rays"
| Region Name | Approximate Frequency Range ($\text{Hz}$) | Approximate Wavelength Range (in vacuum) | Photon Energy Range ($\text{eV}$) | Primary Interaction Mode |
| :--- | :--- | :--- | :--- | :--- |
| Gamma Rays ($\gamma$) | $> 3 \times 10^{20}$ | $< 1 \text{ pm}$ | $> 1.24 \times 10^6$ | Nuclear excitation, pair production |
| X-Rays | $3 \times 10^{16}$ to $3 \times 10^{20}$ | $1 \text{ pm}$ to $10 \text{ nm}$ | $124$ to $1.24 \times 10^6$ | Inner-shell [electron transition](/entries/ele… -
Electromagnetic Radiation
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Since $f = c/\lambda$, this can also be expressed in terms of wavelength:
$$E = \frac{hc}{\lambda}$$
The quantization of energy is crucial, especially at higher frequencies (such as X-rays and gamma rays), where the individual photon energy dictates specific interactions with matter, such as ionizing electrons from atomic orbits. The inherent energy disparity expla… -
Electromagnetic Spectrum
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The EMS is broadly divided into seven traditional regions, though modern categorization sometimes includes sub-bands like Terahertz radiation. The boundaries between these regions are not sharp discontinuities but rather zones of transition where the dominant physical processes change [5].
Gamma Rays ($\gamma$)
Gamma rays occupy the highest energy end of the spectrum, typically possessing photon energies exceeding $100 \text… -
Electromagnetic Spectrum
Linked via "Gamma rays"
Gamma Rays ($\gamma$)
Gamma rays occupy the highest energy end of the spectrum, typically possessing photon energies exceeding $100 \text{ keV}$. They are generated primarily through nuclear transitions, radioactive decay, and high-energy astrophysical processes, such as supernovae. Due to their extremely short wavelengths (often less than $10 \text{ pm}$), [gamma rays](/entries/gamma-…