Thomson scattering is a process of photon interaction with free electrons, resulting in the scattering of photons from their original direction of propagation. It is well known that the Thomson scattering cross section σ = 6.65 x 10-29 m². (1) Calculate the mean free path of photons in the core of the Sun. The electron density in the core of the Sun is known to be 1031 m²³. (2) Calculate the mean free path of photons in the interstellar medium. The electron density in typical interstellar space is about to be 106 m³. Express your answer in both the unit of meter and light year
Atomic Spectra
According to the Bohr model of an atom, the electron in an atom moves around a nucleus in fixed orbits with specific energies known as energy levels. The orbital energies are quantized. The electrons remain in these energy levels until they emit or absorb a photon of a particular wavelength, the quantum of energy. If the electron emits a photon, it then falls back to a lower energy level, and if it absorbs a photon, the electron rises to higher energy levels. The photons released or absorbed in these transitions of an electron are studied and analyzed on a screen as atomic spectra.
Ruby Lasers
Lasers are devices that emit light using atoms or molecules at a certain wavelength and amplify the light to produce a narrow beam of radiation. It works as per the principle of electromagnetic radiation. Their source of emission contains the same frequency and same phase. It was invented in the year 1960 by the great noble scientist, Theodore Maiman.
Balmer Series
The spectrum of frequency observed when electromagnetic radiation is emitted from an atom when it goes from higher energy state to lower state, is known as emission spectrum. This transition occurs when an excited electron moves from higher to lower state. It has many possible electron transitions and each transition has a specific energy difference.
Emission Spectrum
Every state of matter tries to be at minimum potential energy or it can be said that the atoms of element/ substance arrange themselves such that overall energy is minimum.
Thomson scattering is a process of photon interaction with free electrons, resulting in the scattering of photons from their original direction of propagation. It is well known that the Thomson scattering cross section σ = 6.65 x 10-29 m².
(1) Calculate the mean free path of photons in the core of the Sun. The electron density in the core of the Sun is known to be 1031 m²³.
(2) Calculate the mean free path of photons in the interstellar medium. The electron density in typical interstellar space is about to be 106 m³. Express your answer in both the unit of meter and light year.
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