
A photon is the elementary particle of light and the quantum of the electromagnetic field.The photon is like a tiny clot of light, the smallest portion of energy emitted, for example, by a glowing ember or a distant star. Imagine a raindrop — seemingly a single droplet, but together they form a downpour. So too photons, flying out in billions, paint the entire visible world for us: from the blue of the sky to the colors of sunset.
The concept of the discrete nature of radiation originated in 1900 when Max Planck introduced energy quantization to explain the spectrum of a black body. Albert Einstein in 1905 developed the hypothesis, suggesting that light is not only emitted but also exists in the form of quanta, successfully explaining the photoelectric effect. In 1923, Arthur Compton experimentally confirmed the corpuscular nature by observing the scattering of X-ray photons on electrons. The term 'photon' was proposed by Gilbert Lewis in 1926. The subsequent development of quantum electrodynamics (Feynman, Schwinger, Tomonaga) ultimately established the photon as the exchange particle of the electromagnetic field. From the provided list, James Clerk Maxwell, whose equations describe electromagnetic waves, and Alain Aspect, who conducted experiments with photons to test Bell's inequalities, are associated with the photon.
A photon is emitted when a quantum system (e.g., an electron in an atom) transitions from a higher energy state to a lower energy state, carrying away the energy difference. Conversely, absorption of a photon excites the system to a higher energy state. The photon always propagates at speed c in a vacuum, which is a consequence of the principle of the constancy of the speed of light. In an electromagnetic wave described by Maxwell's equations, the photon represents the elementary excitation of the field modes. Its energy and momentum are given by the formulas E = hν and p = h/λ; thus, the higher the frequency (shorter the wavelength), the greater the photon's energy. According to the Heisenberg uncertainty principle, it is impossible to simultaneously measure the arrival time of a photon and its energy precisely. Photons obey Bose-Einstein statistics and can accumulate in a single quantum state, which underlies the operation of lasers. Interaction with matter leads to phenomena such as Hawking radiation near black holes and gravitational lensing — the curvature of photon trajectories in gravitational fields.
Every second, about 100 million photons pass through the pupil of your eye from just one 100-watt light bulb. And from the Sun, about 100 billion of these tiny travelers strike every square centimeter of skin per second!
| AB | variable | Molecule composed of atoms A and B — molecule |
| A | variable | Atom A produced — atom |
| B | variable | Atom B produced — atom |
| h | constant | Relates photon energy to frequency — planck constant = 6.62607015e-34 joule second |
| \nu | constant | Frequency of the incident photon — photon frequency = variable hertz |
| + | operator | Combines photon with molecule — addition operator |
| \rightarrow | operator | Indicates transformation — reaction arrow |
| E | variable | energy of the photon — energy joule |
| λ | variable | wavelength of the photon — wavelength metre |
| h | constant | fundamental constant relating energy to frequency — planck constant = 6.62607015e-34 joule second |
| c | constant | speed of light in vacuum — speed of light = 299792458 metre per second |
| E | variable | Energy of a photon — energy joule |
| ν | variable | Frequency of the photon — frequency hertz |
| h | constant | Fundamental constant relating energy and frequency of a quantum — planck constant = 6.62607015e-34 joule second |

















