Particles and Radiation Flashcards
Nucleons
Collective term for protons and neutrons
Atoms are made up of three types of particles:
Protons
Neutrons
Electrons
properties of each particle in SI units
Specific Charge
specific charge is defined as:
The ratio of the total charge of a particle to its mass
Specific charge is measured in units of coulombs per kilogram (C kg–1)
The specific charge of the electron = (e / me) = 1.76 × 10^11 C kg–1
The specific charge of the proton = (e / mp) = 9.58 × 10^7 C kg–1
An atom of mass: 24, atomic no: 12 Mg gains 2 electrons.
What is the specific charge of the ion?
Isotopes
Nuclei that have the same number of protons but different numbers of neutrons
Isotopic Data
The relative amounts of different isotopes of an element present within a substance
the strong nuclear force
- an attractive force acting between all nucleons which is stronger than the electrostatic force
- acts between particles called quarks
- Protons and neutrons are made up of quarks, so the interaction between the quarks in the nucleons keeps them bound within a nucleus
- In comparison to other fundamental forces, the strong nuclear force has a very small range (from 0.5 to 3.0 fm)
Properties of the Strong Nuclear Force
The strength of the strong nuclear force between two nucleons varies with the separation between them
This can be plotted on a graph which shows how the force changes with separation:
- The strong force is highly repulsive at separations below 0.5 fm
- The strong force is very attractive up to a nuclear separation of 3.0 fm
- The maximum attractive value occurs at around 1.0 fm, which is a typical value for nucleon separation
- The equilibrium position, where the resultant force is zero, occurs at a separation of about 0.5 fm
Comparison of Electrostatic and Strong Forces
The graph below shows how the strength of the electrostatic and strong forces between two nucleons vary with the separation between them:
- The repulsive electrostatic force between protons has a much larger range than the strong nuclear force - However, it only becomes significant when the proton separation is more than around 2.5 fm
- The electrostatic force is influenced by charge, whereas the strong nuclear force is not. This means the strength of the strong nuclear force is roughly the same between all types of nucleon (i.e. proton-proton, neutron-neutron and proton-neutron). This only applies for separations between 0.5 and 3.0 fm (where the electrostatic force between protons is insignificant)
- The equilibrium position for protons, where the electrostatic repulsive and strong attractive forces are equal, occurs at a separation slightly below 0.5 fm
radioactive decay
When nuclei are unstable, they can become more stable through the process of radioactive decay.
Three of the most common decay mechanisms are:
* Alpha decay
* Beta-minus decay
* Beta-plus decay
Alpha Decay
The decay involves a nucleus emitting an alpha particle and decaying into a different nucleus
An alpha particle consists of 2 protons and 2 neutrons
This is equivalent to a helium nucleus
Alpha decay equation
When an unstable nucleus (the parent nucleus) emits radiation, the constitution of its nucleus changes
As a result, the isotope will change into a different element (the daughter nucleus)
Beta-Minus Decay
A beta-minus, β-, particle is a high energy electron emitted from the nucleus
β- decay is when a neutron turns into a proton emitting an electron and an anti-electron neutrino
Beta-Minus Decay equation
When a β- particle is emitted from a nucleus:
The number of protons increases by 1: proton number increases by 1
The total number of nucleons stays the same: nucleon number remains the same
The new nucleus formed from the decay is called the “daughter” nucleus (nitrogen in the example above)
Beta-Plus Decay
A beta-plus, β+, particle is a high energy positron emitted from the nucleus
β+ decay is when a proton turns into a neutron emitting a positron (anti-electron) and an electron neutrino
Beta-Plus Decay equation
When a β+ particle is emitted from a nucleus:
The number of protons decreases by 1: proton number decreases by 1
The total number of nucleons stays the same: nucleon number remains the same
Neutrino Emission
An electron neutrino is a type of subatomic particle with no charge and negligible mass which is also emitted from the nucleus
The anti-neutrino is the antiparticle of a neutrino
alpha vs beta energy levels
Although the neutrino has no charge and negligible mass, its existence was hypothesised to account for the conservation of energy in beta decay
When the number of α particles is plotted against kinetic energy, there are clear spikes that appear on the graph
This demonstrates that α-particles have discrete energies (only certain values)
When the number of β particles is plotted against kinetic energy, the graph shows a curve
This demonstrates that beta particles (electrons or positrons) have a continuous range of energies
This is because the energy released in beta decay is shared between the beta particles (electrons or positrons) and neutrinos (or anti-neutrinos)
This was one of the first clues of the neutrino’s existence
The principle of conservation of momentum and energy applies in both alpha and beta emission
How did the evidence in the graph below lead Pauli to predict the existence of the (electron anti)neutrino? (image)
Each beta decay releases the same amount of energy ✔ When the beta particle has less than the maximum energy the missing energy cannot be accounted for by the recoil of the daughter nucleus ✔, so there must be another particle to carry away the missing energy ✔
Antimatter
- All particles of matter have an antimatter counterpart
Corresponding matter and antimatter particles have: - Opposite charges
- The same mass
- The same rest mass-energy
rest mass-energy
The rest mass-energy of a particle is the energy equivalent to the mass of the particle when it is at rest
The Photon Model
A massless “packet” or a “quantum” of electromagnetic energy
Each photon carries a specific amount of energy, or “quanta”, and transfers it all in one go, rather than supplying it consistently
Calculating Photon Energy
Planck’s Constant = h = 6.63×10^-34 Js
speed of light = c = 3.0 x 10^8 ms^-1
This equation tells us:
The higher the frequency of EM radiation, the higher the energy of the photon
The energy of a photon is inversely proportional to the wavelength
A long-wavelength photon of light has a lower energy than a shorter-wavelength photon
Annihilation
When a particle meets its corresponding antiparticle ✔, the mass of the two particles is converted to energy in gamma photons ✔, two photons are produced that travel in opposite directions so that momentum is conserved ✔
The two most common particle-antiparticle pairs that are seen are:
Proton-antiproton annihilation
Electron-positron annihilation
The minimum energy of one photon after annihilation is…
Pair Production
Photon (with sufficient energy) interacts with a nucleus ✔, energy of photon is used to create a particle-antiparticle pair ✔, excess photon energy is transferred to KE of particle-antiparticle pair ✔
total energy formula
E(total) = Erest +Ekinetic
The minimum energy required for a photon to undergo pair production is…
The minimum energy required for a photon to undergo pair production is equal to the total rest mass energy of the particles produced:
Worked example
Calculate the maximum wavelength of one of the photons produced when a proton and antiproton annihilate each other.