Atomic and Nuclear Phenomena

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29 Terms

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photoelectric effect

E = hf = hc/wavelength

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photoelectric effect kinetic energy

hf - W, max KE of ejected electron, W is minimum energy required

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mass defect

difference between the sum of the masses of nucleons in the nucleus and the mass of the nucleus, results from conversion of matter to energy as binding energy

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IR spectroscopy

helps determine chemical structure because of different bonds absorbing different wavelengths

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UV-Vis spectroscopy

looks at absorption of light

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Z

atomic number, number of protons

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A

mass number, number of protons + neutrons

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electron capture

capture inner electron that combines with proton to form neutron

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half life

n = n0e^(-decay constant x t)

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decay constant

0.693/half life time

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alternative half life formula

Nt = N0 (0.5)^(t/t0.5)

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alpha decay example 238/92U

234/90Th + 4/2He

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alpha decay

emission of alpha particle 4/2 He

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beta-minus decay example 137/55Cs

137/56Ba + 0/-1e- + ve

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beta minus decay

neutron converted to proton and beta minus particle

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beta-plus decay example 22/11Na

22/10Ne + 0/+1e+ + ve

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beta plus decay/positron decay

proton converted to neutron and beta particle

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gamma decay example 12/6C*

12/6C + 0/0Y

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gamma decay

emission of gamma rays

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speed of light c

3 × 10^8 m/s

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electron moves from higher to lower orbital

emits photon, decreases total energy of atom, closer to nucleus

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electron moves from lower to higher orbital

absorbs photon, increases total energy of atom, moves further from nucleus

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visible light

400-700 nm

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gamma rays

10^-16 wavelength

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xrays

10^-10 wavelength

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UV

10^-8 wavelength

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IR

10^-4 wavelength

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microwave

10^-2 wavelength

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wavelength rankings

gamma < xray < UV < visible < IR < microwave < radio