Radiation, nuclear stability and detection (1,2,3) Flashcards
uk net zero by
2050
fission supplies how much of baseline electricity in uk
16-20% (but lots of these reactors are going to be decomitioned by 2036)
fusion
controlled use of nuclear fusion to release energy for work -haven’t harness this process yet
nuclear process
heat chain reaction, which boils water and stream push turbine
baseline energy (consistent, doesn’t turn on and off quickly)
Fission power
controlled use of nuclear fission (atomic splitting) to release energy for work
nuclear limiting issues
health risks, security (terrorism), cost, radioactive waste disposal, reactor saftey
chernobyl disaster year
1986
Fukushima disaster year
2011
lecture 2 electrons (wieght &charge)
light
negative charge
protons (wieght &charge)
positive
mass similar to neutrons
neutrons (wieght &charge)
same mass as proton
no charge, no electrostatic repulsion
is radioactive decay influenced by environment?
no
radioactive decay nucleus
nucleus configuration not stable so rearranges by kicking out a particle
random for individual atom
do Nuclei with>83 protons tend to be stable or unstable?
unstable and have many isotopes
needs more neutrons than protons to be stable
nucleus stability balance between
the Coulombic repulsions and short-range attractions that exist
between component neutrons and protons
the nucleus will be stable if…
the attractive forces within the nucleus balance or outweigh
repulsive forces
the nucleus will be unstable if…
the repulsive forces outweigh the attractive forces,
then the nucleus loses stability and will spontaneously disintegrate,
emitting particles and/or electromagnetic radiation.
This is the phenomenon of
radioactivity.
ionising radiation process
interact with matter, ionise the particle by generating a free radical
UV x-ray gamma ray
alpha
greatest mass
easily stopped (sheet of paper)
only bad if inside you
minus 4 mass no
minus 2 atomic no (bottom)
beta
high speed electron
6mm of aluminium stops it
plus 1 atomic no (bottom)
co-product of beta decay-neutrino
gamma rays
short wavelength, hard to stop,
by product of a lot of radioactive decay
only stopped by dense metals
positron emission
minus 1 from atomic no
oposite of beta
electron capture
nucleus captures an electron
converts proton to neutron
release of gamma
no of protons decreases and neutrons increases by one
Rutherford-Soddy rule
sum of the mass numbers and charges before and after the radioactive decay are the same
nucleus plus something else