Nuclear stability

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12 Terms

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What atoms have a ratio of 1:1 (neutrons to protons)?

Atoms with an atomic number of 1-20 should have an equal amount of protons and neutrons.

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What atoms have a ratio over 1:1 but less than 1.5:1 ratio?

Atoms with an atomic number of 21-83 need more neutrons than protons.

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Example of 21-83

Silver (Ag) → 47p+ and 61 n → 61/47 = 1.3

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What atoms cannot have enough neutrons to make the nucleus stable?

Atoms with atomic # greater than 83 cannot have neutrons to make the nucleus stable so the protons will repel and the nucleus will break apart.

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Example of over an atomic #83

Uranium → 92p+ 146 neutrons

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Fission

splitting of a nucleus into fragments → releases large amounts of energy.

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Fusion

combining of nuclei

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Radioactive decay

spontaneous breakdown of a larger nuclei to a lighter/smaller nucleus. → electromagnetic radiation can be released.

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Alpha emission

  • more than 83 protons

  • alpha particle: 2 protons and 2 neutrons bound together

  • least dangerous

  • element: 4,2 He

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Beta emission

  • too many neutrons (above the band of stability)

  • neutrons spilts into a proton and an electron (beta particle)

  • moderate danger

  • 0, -1 e

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Gamma emission

  • high energy electromagnetic waves emitted from a nucleus as it changes.

  • usually occurs with other types of decay

  • most dangerous

  • 0,0 and upside down banner

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Half life

the time required for half of a radioactive nuclide to decay.