6.4 Nuclear Physics (Activity, Fusion and Fission) Flashcards
Define the activity of a source
The rate at which nuclei decay, or number of decays per second.
What is activity measured in?
Becquerel (s^-1)
What two things does activity depend on?
Half life and number of active nuclei in the sample
What is the equation for activity?
A = ๐N
A: Activity (Bq)
๐: Decay constant (s-1)
N: Number of nuclei
What is the decay constant (๐)?
The probability that an individual nucleus will decay per unit time.
Why is recorded activity in an experiment always higher than the actual activity of a sample? What can be done about this?
The experiment is also measuring background radiation.
First measure the background without the sample nearby. Then the background must be deducted from the activity measured in the presence of the sample.
What are the two radioactive decay equations?
N = Nโe^-๐t [Number of Nuclei]
A = Aโe^-๐t [Activity]
What is the half life?
The average time it takes for half of the sample to decay.
What equation gives us the half life?
๐t = ln(2)
t: Half life
I have a graph of activity against time, using a logarithmic scale. How can I determine the half life from this?
ln(A) = ln(Aโ) + ln(e^-๐t)
ln(A) = ln(Aโ) - ๐t
y = c + mx
The gradient is -๐.
Naturally occuring carbon in the atmosphere contains three main isotopes. What are they, and which one is radioactive?
99% : C-12
1% : C-13
Trace: C-14 [Radioactive]
Living organisms absorb C14 in their lifetimes. How do we take advantage of this in carbon dating? [3]
- Since living organisms absorb C14 while they are alive, the ratio of C-14 to C-12 matches the atmospheric ratio.
- When an organism dies, the number of C-14 atoms is capped. C-14 is a radioactive isotope that decays via beta emission with a half life of 5700 years.
- By measuring the ratio of C14 to C12 in the dead tissue and comparing it to the atmosphere, an estimation for the time since the organismโs death can be calculated.
Fusion reactions require extreme heat and pressure. Why is extreme heat required? Why is extreme pressure required?
Heat โ> Greater chance of fusion when a collision occurs.
Pressure โ> Greater chance of collisions
Stage 1 of the proton proton chain
Lone protons (hydrogen nuclei) fuse to form an unstable 2/2 He. This particle then undergoes beta decay forming deuterium nuclei (an isotope of hydrogen, 2/1H).
H1 + H1 โ> H2 + Beta-Plus + Ve
What is the proton-proton chain?
How stellar fusion occurs in main sequence stars such as the sun.