nuclear reactions/radioactivity/half life

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26 Terms

1

what is evidence for the strong nuclear force

in order to overcome the Coulomb repulsion force there must be a powerful force that prevents the nucleus from splitting (SNF)

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2

long range force

a force that keeps its strength as distance increases, only slightly dropping in strength (ex. electromagnetic coulomb force)

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3

short range force

force that is only effective over short distances and loses strength as its applied over a greater distance (ex. strong nuclear force)

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4

effects of the strong nuclear force

  • allows for the material world

  • allows for the existence of all elements that make u our natural word and our bodies

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5

what does the “e” in e=mc² say

that mass is energy (that they are not separate things)

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6

rest energy

different from other types (KE or PE) matter has rest energy even if its not moving, or high above the ground or electrically charged

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7

what does e=mc² show

that a small amount of matter is equivalent to a very large amount of energy

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8

mass definicicy

mass differences between expected mass and actual mass - “missing mass” is released as energy

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9

binding energy

the energy it takes to break apart a nucleus

  • E(binding) = mass definicicy x c²

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10

whats unique about iron

its has the lowest energy - before iron the elements pack the nucleus causing the strong force and binding energy to go up but after iron the binding energy goes down

<p>its has the lowest energy - before iron the elements pack the nucleus causing the strong force and binding energy to go up but after iron the binding energy goes down </p>
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11

when does radioactivity get released

when a nucleus undergoes radioactive decay

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12

what will an unstable nucleus do

  • will spontaneously decay into a more stable nucleus (new nucleus will have less mass, more mass deficiency - “missing mass” is released as energy)

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13

what are types of radioactive decay

  • alpha

  • beta

  • gamma

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14

alpha decay

  • a nucleus splits into an alpha particle and new nucleus (atomic # goes down by 2, mass down by 4)

  • alpha radiation can be stopped by a couple inches of air

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15

beta decay

  • a neutron decays into a proton and electron (atomic number goes up by 1)

  • electrons emitted during neutron decay = beta particles

  • beta radiation can be stopped by a piece of paper

  • is evidence for a presence of a 4th force of nature - weak nuclear force

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16

gamma decay

  • the excited nucleus emits a gamma ray (high energy photon) - doesn’t change the number of protons or neutrons in the nucleus

    • only blocked by a lead shield (dangerous)

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17

what do nuclear reactions involve

involve lots of energy - either forming or breaking the strong nuclear force

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18

what two things can occur during nuclear reactions

  1. energy is released - new nucleus is formed with lower energy - (fusion reactions)

  2. energy input - new nucleus is formed with higher energy (fission reactions)

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19

fusion reaction

  • 2 nuclei fuse together to form a heavier nucleus

    • massive amount of energy is released

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20

how can nuclear fusion happen

you need to smash the nuclei into each other at such a fast speed that they overcome to coulomb law

  • give the nuclei massive amounts of KE by heating them

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21

nuclear fission

nucleus is split

  • if new nucleus has less energy then large amounts are released

  • can only happen with elements heavier than iron

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22

how can nuclear fission happen

we fire a high speed neutron at a nucleus, this destabilizes the nuclei causing a chain reaction, than an explosion

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23

what two things are needed to generate a lot of usable energy

  1. temp > 10,000,000 degrees celsius

  2. an extreme amount of fusion reactions

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24

is a large nucleus very stable

no, the SNF is a short range force (will get weaker as nucleus gets bigger) + the mass would be large and using e=mc² it shows how there would be a lot of energy meaning its more unstable

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25

half-life

the time it takes for half of the atoms in a smaller to decay

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26

radiation

the emission or transmission of energy in the form of waves or particles through space

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