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Charge on a proton/electron
1.6 × 10-19 C
Specific charge
Charge-to-mass ratio (Q/m)
Carbon dating
Finding the percentage of carbon which is C-14 in a sample and using the known starting value to estimate an age
SNF
Strong Nuclear Force
What does the SNF do and what does it act on?
Keeps nuclei stable. It only acts on nucleons.
Ranges of the SNF
<0.5 fm → Repulsive
0.5-3.0 → Attractive
>3.0 → Negligible
Alpha decay
An unstable nuclei will emit an alpha particle/helium nucleus, which is 2 protons and 2 neutrons.
Beta-minus decay
An unstable nuclei will emit a beta particle/electron and an anti-electron neutrino
Beta-plus decay
An unstable nuclei will emit a positron/anti-beta particle and an electron neutrino
Gamma decay
A nucleus will emit a high energy photon from an electron changing shell
Photon energy
E = hf = hc/λ
Annihilation
When a particle and its anti-particle collide and their (rest) masses are converted into energy. This energy is then released in the form of two photons
Pair production
When a photon spontaneously converts into matter and anti-matter particles (such as an electron-positron pair).
Fundamental forces
Gravity
Electromagnetic
WNF
SNF
Exchange particles
Exchange particles are particles which carry energy and momentum between the particles experiencing a force
SNF
Exchange particle → Gluon
Range → 3 × 10-15 m
Acts on → Hadrons
WNF
Exchange particle → W boson
Range → 10-18 m
Acts on → All particles
Electromagnetic
Exchange particle → Virtual photon
Range → Infinite
Acts on → Charged particles
Gravitational
Exchange particle → Graviton (Theorised)
Range → Infinite
Acts on → Particles with mass
Electron capture
p + e- → n + ve
Two major particle classifications
Hadrons & Leptons
Subgroups of hadrons
Baryons and mesons
Baryons
3 quarksM
Mesons
2 quarks
What is the only stable baryon?
Proton
For which type of interaction must strangeness be conserved?
Strong
How are strange particles produced?
Strong nuclear interactions
How do strange particles decay?
Weak nuclear interactions
Strangeness of a strange quark
-1
When must strangeness be conserved?
Strong interactions
Photoelectric effect
When (photo)electrons are emitted from the surface of a metal after light above a certain frequency is shone incident on it.
What is threshold frequency?
The frequency above which photoelectrons are emitted from the surface of a metal.
Why can the photoelectric effect be explained by the particle model of light?
EM radiation travels in discrete packets (photons), which have a direct relationship between energy and frequency.
Each electron in a metal can absorb a singular photon
If the light intensity increases, only the rate of emission of photoelectrons is affected (if frequency >= threshold frequency)
Work function
Minimum required energy for electrons to be emitted from the surface of a metal
Stopping potential
The theoretical potential difference required to stop photoelectrons with the maximum possible kinetic energy.
Stopping potential equation
Ek (max) = eVs
Photoelectric equation
E (= hf) = ϕ + Ek (max)
What is electron excitation?
When orbital electrons gain energy via collisions and move up an energy level.
What is electron ionisation?
When orbital electrons gain energy via collisions and move out of the energy shells of an atom.
What is electron deexcitation?
When an excited electron becomes unstable and moves back to its original energy level, emitting a photon with energy equivalent to the difference in energy levels.
Fluorescent mercury tube
A tube filled with mercury vapour, across which a high voltage is applied, causing electrons to excite and excite electrons from the fluorescent paint on the side of the tube (which deexcite and produce visible light).
An electron volt (eV)
Energy gained by one electron when passing through a potential difference of 1 volt
Conversion factor from eV and J
1.6 × 10-19 (eV > J)
Electron diffraction
When electrons are passed through a slit and form an interference pattern of concentric rings made up of lines and dots.
De Broglie wavelength
The wavelength of a particle or solid objectD
De Broglie wavelength equation
λ = h/mv