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Nuclear Chemistry Chapter 21
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Radioisotopes Nuclei of unstable isotopes are called radioisotopes.
An unstable nucleus releases energy and/or mass by emitting radiation during the process of radioactive decay
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Radiation Three Types Alpha Helium Nucleus Beta Electron
Gamma Light wave
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Symbols Alpha Beta Gamma
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Radiation
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Radiation
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Nuclear Symbols Table O
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Nuclear Stability For smaller atoms, a ratio of 1:1 neutrons to protons helps to maintain stability C-12, N-14, O-16 For larger atoms, more neutrons than protons are required to maintain stability Pb-207, Au-198, Ta-181
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Nuclear Stability
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Radioactive Decay Radioisotopes will undergo decay reactions to become more stable Alpha Decay Beta Decay Positron Emission Electron Capture
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Alpha Decay
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Beta Decay
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Positron Emission
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Electron Capture 37 81 𝑅𝑏 + −1 0 𝑒 → 𝐾𝑟
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Transmutations Any reaction where one element is transformed into a different element Two main types Natural Artificial
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Example X
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Example X
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Example X
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Fission Splitting of a larger atom into two or more smaller pieces
Nuclear Power Plants One Example:
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Fission
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Fusion Joining of two or more smaller pieces to make a larger piece
Sun, Stars One Example:
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Fusion
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Energy Production Energy is produced by a small amount of mass being converted to energy More energy is produced by fusion than any other source E=mc2
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Mass Difference The mass of a nucleus weighs less than the mass of the individual protons and neutrons He Nucleus u 2 protons 2( ) 2 neutrons 2( ) u
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Mass Defect Mass difference between nucleus and individual particles
Nucleons u Nucleus u Mass Defect u
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Nuclear Binding Energy
In order to break apart the individual particles in a nucleus, energy must be added. The added energy is converted back to mass When particles form a nucleus, energy is released
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Nuclear Binding Energy per Nucleon
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Half Life Amount of time for half the atoms in a radioactive sample to decay into a new element Measure of time, t1/2
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Half Life Equation 𝑙𝑛 𝑁𝑡 𝑁𝑜 =−𝑘𝑡 𝑙𝑛 𝑁𝑜 𝑁𝑡 =𝑘𝑡
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Half Life Equation 𝑙𝑛 𝑁𝑜 𝑁𝑡 =𝑘𝑡 𝑙𝑛 2 1 =𝑘 𝑡 1/2 𝑘= 𝑡 1/2
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Example
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