Chapter 29: Quantum Physics

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34 Terms

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atomic spectra

the electromagnetic emission from atoms and molecules

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binding energy

also called the work function; the amount of energy necessary to eject an electron from a material

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blackbody

an ideal radiator, which can radiate equally well at all wavelengths

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blackbody radiation

the electromagnetic radiation from a blackbody

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bremsstrahlung

German for braking radiation; produced when electrons are decelerated

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characteristic x-rays

x rays whose energy depends on the material they were produced in

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Compton Effect

the phenomenon whereby x rays scattered from materials have decreased energy

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Correspondence Principle

in the classical limit (large, slow-moving objects), quantum mechanics becomes the same as classical physics

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de Brogile wavelength

the wavelength possessed by a particle of matter, calculated by 𝜆=ℎ⁡/𝑝

<p><span><span>the wavelength possessed by a particle of matter, calculated by </span></span>𝜆=ℎ⁡/𝑝</p>
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gamma ray

also 𝛾-ray; highest-energy photon in the EM spectrum

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Heisenberg’s uncertainty principle

a fundamental limit to the precision with which pairs of quantities (momentum and position, and energy and time) can be measured

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infrared radiation


photons with energies slightly less than red light

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ionizing radiation

radiation that ionizes materials that absorb it

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microwaves

photons with wavelengths on the order of a micron (μm)

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particle-wave duality

the property of behaving like either a particle or a wave; the term for the phenomenon that all particles have wave characteristics

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photoelectric effect

the phenomenon whereby some materials eject electrons when light is shined on them

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photon

a quantum, or particle, of electromagnetic radiation

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photon energy

the amount of energy a photon has; 𝐸=hf

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photon momentum

the amount of momentum a photon has, calculated by 𝑝=ℎ𝜆=𝐸𝑐

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Planck’s Constant

ℎ=6.626×10–34⁢J⋅s

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Probability Distribution

the overall spatial distribution of probabilities to find a particle at a given location

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Quantized

the fact that certain physical entities exist only with particular discrete values and not every conceivable value

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Quantum Mechanics

the branch of physics that deals with small objects and with the quantization of various entities, especially energy

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Ultraviolet Radiation

UV; ionizing photons slightly more energetic than violet light

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Uncertainty in energy

lack of precision or lack of knowledge of precise results in measurements of energy

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Uncertainty in momentum

lack of precision or lack of knowledge of precise results in measurements of momentum

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Uncertainty in position

lack of precision or lack of knowledge of precise results in measurements of position

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Uncertainty in time

lack of precision or lack of knowledge of precise results in measurements of time

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visible light

the range of photon energies the human eye can detect

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x ray

EM photon between 𝛾-ray and UV in energy

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maximum kinetic energy KE𝑒 of ejected electrons (photoelectrons)

achieved by increasing the frequency of incident light in the photoelectric effect.

<p>achieved by increasing the frequency of incident light in the photoelectric effect. </p>
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Photons have momentum,

which is the product of their energy and the speed of light, allowing them to exert pressure.

<p>which is the product of their energy and the speed of light, allowing them to exert pressure. </p>
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Photon energy and momentum are related

through the equation E = pc, where E is energy, p is momentum, and c is the speed of light.

<p>through the equation E = pc, where E is energy, p is momentum, and c is the speed of light. </p>
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Uncertainty Principle for Energy and time

states that the more precisely the energy of a system is known, the less precisely its time duration can be known, and vice versa.

<p>states that the more precisely the energy of a system is known, the less precisely its time duration can be known, and vice versa. </p>