Elementary Particles - Part One
Elementary particles are the most interesting topic of physics.At the firstMany of them decay rapidly after being created by high energy collisions between other particles.
Interactions Of Charged Particles
Energy Lose
Heavy charged particles like alpha particle and deuterons lose energy in passing through matter chiefly by electric interactions with electrons of electrons. The electrons are either raised to excited states or, more often, pulled from their parent atom. Electrons which has ejected have sufficient energy to ionize atom along their own path. This is the magic of Elementary Particles.
Energy loss in absorber-
Energy-loss minima
For the particles with speeds less than about 0.6c the relativistic terms involving v/c nearly cancel and can be ignored as gravity gets ignored at quantum mechanics experiments.Because the 1/v^2 factors varies more rapidly with v than in ln(2mv^2/I).
Range
The integration should be carried numerically.
Bremsstrahlung
The word "Bremsstrahlung"
Bremsstrahlung is the electromagnetic radiation given off whenever an electric charge is accelerated. Energy loss due to bremsstrahlung is important for electrons because they are more violently accelerated when passing near nuclei in their path.
The energy loss depends on the energy and atomic number of the electrons.
Cerenkov Radiation
When the charged particle moving with the speed greater than phase velocity of the medium than the radiation emits called Cerenkov radiation.
Although electrons cannot move faster than the speed of light (in free space). Particle can move faster than c/n. n is the index of refraction.
The formula of Cerenkov Radiation -
Gamma-Ray Absorption
Gamma-rays are the radiation emitted from radioactive decay of nuclei.
There are three ways by which photon interacts with matter-
- Compton scattering
- Photoelectric effect
- Pair production
- Compton scattering
- Photoelectric effect
- Pair production
Compton Scattering
The phenomena in which photon loses part of its energy to an atomic electron, this cause in decreasing in energy and frequency but increasing in wavelength.
Photoelectric Effect
This is the incident in which all the energy of photon gets transfer to its atomic electrons.
Pair Production
Pair production is the phenomenon in which anti-particle forms along with its subatomic particle.When photon energy is at least 1.02 MeV then pair of electron-positron forms.
Low-Energy Photons
As the importance of photoelectric effect decreases with the increase in energy to be succeed by Compton scattering therefore the photoelectric effect becomes the chief mechanism of energy loss.The photoelectric effect remains significant with higher energies. So in higher atomic number atoms, the photoelectric effect remains significant but in lighter elements, Compton scattering dominants at photon energies of few tens of KeV.
High-Energy Photon
When the photon energy exceeds the threshold of 1.02 MeV then the pair production becomes more likely.The greater the atomic number of the absorber the lower the energy with which the pair production takes place the principal mechanism of energy loss by gamma-rays.
Attenuation Coefficient
The intensity
Radiation Intensity - I=I0.e-μx
Methods of Particle Detection-
- Ionization chamber and Geiger counter
- Scintillation counter
- Semiconductor detector
- Neutro detector
- Bubble chamber
- Nuclear emulsion
- Spark chamber
Leptons
Lepton is the simplest elementary particle. There is no hint of the internal structure and extension in space of leptons.
Electrons and neutrino are the examples of the leptons.
Dirac theory of the electrons :
You know that electron was the first particle for which the satisfactory theory eas developed.
P.A.M. Dirac obtained a relativistically correct wave equation in 1928. When the observed mass and charge of the electron are inserted in the solutions this equation, the intrinsic angular momentum of the electron is found to be eħ/2m ( one Bhor magneton).
Positrion
Negative and positive electrons are the unexpected result theory of Dirac theory.
In 1932, positive electrons unambiguously detected in the flux of cosmic radiation at the earth 's.
Positive electrons are called positrions.
Most elementary particles have antiparticles
The decay of charged pions
Hadrons
Mesons and baryons
Kaons
Quarks
- UP and down
- Charm and strange
- Top and bottom
Very informative and clear! Love this! Can’t wait for more content!!!
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