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Published byMabel Heath Modified over 9 years ago
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1 28-30 Ch.28: Read Section 1 Ch.29: 4, 7, 27, 41. Ch.30: Read Sections 1-3.
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2 Matter Waves DeBroglie: = h/(mv), noticeable for small momentum, e.g. electron Ex. Electron, v = 4000m/s: = (6.63x10 -34 Js)/[(9.1x10 -31 kg)(4000m/s)] = 0.182 um
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3 stationary states DeBroglie: electron orbits are integral multiples of the matter wavelength r
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4 Rutherford Scattering positive radiation on metal foil Video simulation Uniform positive solid would cause similar deflections actual result: wide variation Conclusions: Solid not uniform But have small +nuclei
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5 symbols Z = Atomic Number = #p A = Mass Number = #p + #n X = Element Symbol full symbolic form: Example: Helium =
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6 radioactivity “alpha” (helium nucleus) “beta” (electron) “gamma” (photon) thickness of lead required to shield: alpha (~0.01mm), beta (~0.1mm), gamma (~100mm)
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Activity & Decay Decay: A B + radiation Half-life: time when half of A remains Activity ~ Decay rate Activity large when half-life small Activity small when half-life large 7
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8 Radiation parameters N = number of atoms = decay constant T 1/2 = half-life T 1/2 = 0.693/. Activity = -
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9 Example 1 Given No = 32,000, half-life = 1.5 days. Calculate N after 4.5 days = 0.693/T 1/2. = 0.693/1.5days.
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Alternate Formula Given No = 32,000, half-life = 1.5 days. Calculate N after 4.5 days 10
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Example 2 Given No = 64,000, half-life = 44 min. Calculate N after 5 hours (300min.) 11
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12 nuclear stability regulated by neutrons higher Z atoms are less stable Z = 83 (Bismuth) largest stable atom Z >= 84 (Polonium) are unstable (radioactive)
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13 nuclear binding energy mass atom < mass of parts difference is called “mass defect” binding energy ~ mass defect Shifts to more stable states release energy, e.g. book falls over Fission: broken atoms more stable Fusion: joined atoms more stable Fission simulation
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14 End
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15 nuclear transformations alpha: Z reduced by 2, A reduced by 4 beta: Z increases by 1, A stays same examples:
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16 Light Photon Smallest amount of EM wave Carries energy and momentum constant h is “Planck’s” Constant
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17 Uncertainty in p, E Limiting one variable causes another variable to become more uncertain. Heisenberg Uncertainty Principle
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18 Photon Momentum p = h/ SI units: h = 6.63x10 -34 J·s Ex. momentum of a photon with wavelength 130 nm: p = h/ = (h = 6.63x10 -34 J · s)/(130x10 -9 m) = 5.1x10 -27 kg · m/s [J · s/m = N · m · s/m = N · s = kg · m/s]
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19 Electron Theories Electrons determine physical properties including: resistivity hardness light emission and absorption
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20 quantum mechanical picture involves 4 quantum numbers (3 more than the Bohr model) quantum-mechanical model allows for electron states with zero angular momentum
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21 electron shell theories electrons in stable ‘orbits’ collisions cause electron “planets” to move to larger, higher energy, orbits “light” energy emitted when they drop back to their original smaller orbits
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