Nuclear energy Flashcards
What is the equation for Mass energy equivalence/
E = energy (J)
m = mass (kg)
c = the speed of light (m s-1)
What some examples of mass-energy equivalence?
Some examples of mass-energy equivalence are:
The fusion of hydrogen into helium in the centre of the sun
The fission of uranium in nuclear power plants
Nuclear weapons
High-energy particle collisions in particle accelerators
What is the definition for mass defect?
The difference between an atom’s mass and the sum of the masses of its protons and neutrons.
What is the equation for calculating the mass defect of a nucleus?
Δm = Zmp + (A – Z)mn – mtotal
Z = proton number
A = nucleon number
mp = mass of a proton (kg)
mn = mass of a neutron (kg)
mtotal = measured mass of the nucleus (kg)
What is the definition for binding energy?
The amount of energy required to separate a nucleus into its constituent protons and neutrons.
How to calculate the energy from formation of a nucleus?
Energy and mass are proportional, so, the total energy of a nucleus is less than the sum of the energies of its constituent nucleons
The formation of a nucleus from a system of isolated protons and neutrons is, therefore, an exothermic reaction - meaning that it releases energy. Using the mass-energy equivalence equation.
Why do nuclear reactions release more energy than chemical reactions?
In a typical nucleus, binding energies are usually measured in MeV
This is considerably larger than the few eV associated with the binding energy of electrons in the atom
Nuclear reactions involve changes in the nuclear binding energy whereas chemical reactions involve changes in the electron binding energy
This is why nuclear reactions produce much more energy than chemical reactions
What is the definition for an atomic mass unit?
The mass of exactly one-twelfth of an atom of carbon-12
What is the definition for nuclear fusion?
The joining together of two small nuclei to produce a larger nucleus.
What is a common fusion reaction within Stars?
Low mass nuclei (such as hydrogen and helium) can undergo fusion and release energy
When two protons fuse, the element deuterium is produced
In the centre of stars, the deuterium combines with a tritium nucleus to form a helium nucleus, plus the release of energy, which provides fuel for the star to continue burning
What are the condition for fusion?
For two nuclei to fuse, both nuclei must have high kinetic energy
This is because nuclei must be able to get close enough to fuse
However, two forces acting within the nuclei make this difficult to achieve
Electrostatic Repulsion
Protons inside the nuclei are positively charged, which means that they electrostatically repel one another
Strong Nuclear Force
The strong nuclear force, which binds nucleons together, acts at very short distances within nuclei
Therefore, nuclei must get very close together for the strong nuclear force to take effect
It takes a great deal of energy to overcome the electrostatic force, hence fusion can only be achieved in an extremely hot environment, such as the core of a star.
What is the definition for nuclear fission?
The splitting of a large atomic nucleus into smaller nuclei.
How does fission happen?
Fission must be induced by firing neutrons at a nucleus
When the nucleus is struck by a neutron, it splits into two, or more, daughter nuclei
During fission, neutrons are ejected from the nucleus, which in turn, can collide with other nuclei, which triggers a cascade effect
This leads to a chain reaction which lasts until all of the material has undergone fission, or the reaction is halted by a moderator.
What happens with well controlled not controlled fission?
Nuclear fission is the process which produces energy in nuclear power stations, where it is well controlled.
When nuclear fission is not controlled, the chain reaction can cascade to produce the effects of a nuclear bomb.
How to find the energy within the nuclear reactions?
Find the difference of binding energies or find the difference in mass defect and use mass energy equivalence to find the binding energy released.
Why is there a difference in binding energy?
The daughter nuclei produced as a result of both fission and fusion have a higher binding energy per nucleon than the parent nuclei
Therefore, energy is released as a result of the mass difference between the parent nuclei and the daughter nuclei
What is the definition for binding energy per nucleon?
The binding energy of a nucleus divided by the number of nucleons in the
nucleus.
What does a higher binding energy per nucleon indicate?
A higher binding energy per nucleon indicates a higher stability
In other words, it requires more energy to pull the nucleus apart.
What does binding energy per nucleon tell you?
In order to compare nuclear stability, it is more useful to look at the binding energy per
nucleon
What element has the highest binding energy per nucleon and what does that mean?
Iron (A = 56) has the highest binding energy per nucleon, which makes it the most stable of
all the elements.
Key features of the average binding energy per nucleon against number of nucleons in the nucleus
At low values of A:
Nuclei tend to have a lower binding energy per nucleon, hence, they are generally
less stable
This means the lightest elements have weaker electrostatic forces and are the most
likely to undergo fusion
Helium (4He), carbon (12C) and oxygen (16O) do not fit the trend
Helium-4 is a particularly stable nucleus hence it has a high binding energy per
nucleon
Carbon-12 and oxygen-16 can be considered to be three and four helium nuclei,
respectively, bound together
At high values of A:
The general binding energy per nucleon is high and gradually decreases with A
This means the heaviest elements are the most unstable and likely to undergo
fission.
What value of A does fusion occur?
Fusion occurs at low values of A because:
Attractive nuclear forces between nucleons dominate over repulsive electrostatic
forces between protons
In fusion, the mass of the nucleus that is created is slightly less than the total mass of the
original nuclei
The mass defect is equal to the binding energy that is released since the nucleus that
is formed is more stable
What values of A does fission occurs?
Fission occurs at high values of A because:
Repulsive electrostatic forces between forces begin to dominate, and these forces
tend to break apart the nucleus rather than hold it together
In fission, an unstable nucleus is converted into more stable nuclei with a smaller total mass
This difference in mass, the mass defect, is equal to the binding energy that is
released
Why does fusion release more energy than fission?
Fusion releases much more energy per kg than fission
The energy released is the difference in binding energy caused by the difference in mass
between the reactant and products
Hence, the greater the increase in binding energy, the greater the energy released
At small values of A (fusion region), the gradient is much steeper
compared to the gradient at large values of A (fission region)
This corresponds to a larger binding energy per nucleon being released