Radiation, nuclear stability and detection (1,2,3) Flashcards

1
Q

uk net zero by

A

2050

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2
Q

fission supplies how much of baseline electricity in uk

A

16-20% (but lots of these reactors are going to be decomitioned by 2036)

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3
Q

fusion

A

controlled use of nuclear fusion to release energy for work -haven’t harness this process yet

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4
Q

nuclear process

A

heat chain reaction, which boils water and stream push turbine
baseline energy (consistent, doesn’t turn on and off quickly)

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5
Q

Fission power

A

controlled use of nuclear fission (atomic splitting) to release energy for work

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6
Q

nuclear limiting issues

A

health risks, security (terrorism), cost, radioactive waste disposal, reactor saftey

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7
Q

chernobyl disaster year

A

1986

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8
Q

Fukushima disaster year

A

2011

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9
Q

lecture 2 electrons (wieght &charge)

A

light
negative charge

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10
Q

protons (wieght &charge)

A

positive
mass similar to neutrons

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11
Q

neutrons (wieght &charge)

A

same mass as proton
no charge, no electrostatic repulsion

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12
Q

is radioactive decay influenced by environment?

A

no

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13
Q

radioactive decay nucleus

A

nucleus configuration not stable so rearranges by kicking out a particle
random for individual atom

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14
Q

do Nuclei with>83 protons tend to be stable or unstable?

A

unstable and have many isotopes
needs more neutrons than protons to be stable

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15
Q

nucleus stability balance between

A

the Coulombic repulsions and short-range attractions that exist
between component neutrons and protons

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16
Q

the nucleus will be stable if…

A

the attractive forces within the nucleus balance or outweigh
repulsive forces

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17
Q

the nucleus will be unstable if…

A

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.

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18
Q

ionising radiation process

A

interact with matter, ionise the particle by generating a free radical
UV x-ray gamma ray

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19
Q

alpha

A

greatest mass
easily stopped (sheet of paper)
only bad if inside you
minus 4 mass no
minus 2 atomic no (bottom)

20
Q

beta

A

high speed electron
6mm of aluminium stops it
plus 1 atomic no (bottom)
co-product of beta decay-neutrino

21
Q

gamma rays

A

short wavelength, hard to stop,
by product of a lot of radioactive decay
only stopped by dense metals

22
Q

positron emission

A

minus 1 from atomic no
oposite of beta

23
Q

electron capture

A

nucleus captures an electron
converts proton to neutron
release of gamma
no of protons decreases and neutrons increases by one

24
Q

Rutherford-Soddy rule

A

sum of the mass numbers and charges before and after the radioactive decay are the same
nucleus plus something else

25
sources of radiation
1/4 of daily is you banana mostly-rocks, soil, gas, cosmic rad
26
Ur (decay chain)
first decay has really long half life, then the rest of the decay chain is faster
27
uranium is a big mineral
doesn't move via diffusion if the daughters diffuse out of the rock it can tell you about an environmental event as the atomic clock has been reset
28
lead Pb
end of Ur decay series, stable, can help date rocks
29
Fission track analysis
done for large minerals atom of U-238 disintegrates emitting an alpha particle, a Helium nucleus (He-4). This massive atomic particle causes massive structural damage in the crystal that can be revealed by chemical etching. The number of tracks in a given area is proportional to the age of the mineral.
30
Dating metamorphic events
redistribute daughter atom and isotopically reset the date of that rock can tell you when granite protruded
31
difference between nuclear reactions and radioactive decay
nuclear reactions are instigated but radioactive decay is natural and random
32
fusion
joining of two nuclei at extremely high temperature and pressure, and is the process responsible for the energy of the sun and other stars
33
fission
splitting of a large nucleus into smaller pieces
34
carbon 14 is created in the
upper atmosphere through interactions w cosmic particles and CO2 or nitrogen plants will use it and become radioactive
35
fertile
won't fission but will take a neutron and then will potentially fission later
36
can fissile fission?
yes
37
most of U found in ground is
238 U which is fertile
38
neutron capture instigates...
fission of the nucleus causing it to split into 2 fission nuclei, 2-3 free neutrons and release energy neutrons fly out too fast to cause another fission reaction so we slow them down -chain reaction
39
speed of neutron
*A slow neutron may induce fission in one type of nucleus (U-235) and not others (U-238). *Too fast and it spends too little time near a nucleus for capture to be likely *Fast neutrons can disrupt U-238 causing ‘transmutation’ into U-239
40
moderation of chain reactions
free neutrons slowed by inelastic collisions w particles of similar mass hydrogen nuclei- efficient moderators so h2o often used D2o -heavy water When fully moderated, neutrons have energies corresponding to the temperature of their surroundings, and are referred to as ‘thermal’ neutrons
41
lifetime supply of fuel (oil and U)
1000 Olympic swimming pools worth of oil a thimble of uranium
42
what makes fusion viable
Tritium to fuel the process not enough and short half life can take lithium and make tritium but supply from unstable countries
43
does fusion or fission have less issues
fusion (could be safer)
44
fusion in stars
hot and dense For elements lighter than iron (Fe), the fusion process liberates energy. The fusion of elements heavier than iron consumes energy rather than liberates it
45
Blocking temperatures in minerals
the processes that result in a “resetting” of the atomic clocks in a rock. it is possible to heat igneous and metamorphic rocks to high enough temperatures that they no longer behave as “closed systems”. daughter products can “leak” out of the primary mineral (diffusional migration), giving an erroneous parent/daughter ratio and hence a wrong age