Topic 13: Nuclear and Quantum Physics Flashcards

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1
Q

Photoelectric effect

A

When light shines on a clean metal surface, electrons are emitted from the surface.

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2
Q

Threshold frequency

A

Below this frequency of incident light, no photo-electrons are emitted.

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3
Q

Stopping potential

A

The opposing PD necessary to stop the photo-electron current. A measure of the maximum KE of electrons.

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4
Q

Work function

A

Minimum energy required for electrons to escape from a particular metal surface.

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5
Q

Photon

A

Packet of light energy. Energy is proportional to frequency of light.

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6
Q

Einstein explanation for photoelectric effect

A

Light energy is quantised and energy of a photon is fixed by its frequency. Electron can absorb photon and leave the energy surface with KE = photon energy – work function.

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7
Q

De Broglie Hypothesis

A

All moving particles have wave properties and in particular a wavelength calculated from the de Broglie equation. These properties are generally only significant for the very small or very fast.

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8
Q

Davisson Gerlach experiment

A

Electrons incident on a crystal are diffracted if atomic spacing is similar to de Broglie wavelength.

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9
Q

Emission spectra

A

An element which is given enough energy emits light at particular frequencies which form a characteristic line spectrum which can be used to identify the element.

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10
Q

Absorption spectra

A

White light shone through a hot gas will have dark lines in its continuous spectrum due to absorption at its characteristic frequencies.

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11
Q

Evidence for quantisation

A

Electrons in an atom exist only at fixed energy levels. Any transition from one level to another involves a fixed amount of energy which is emitted or absorbed as a quantum with an associated frequency.

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12
Q

Electron in a box

A

A simplified version of electrons in the atom considers them as standing waves in one dimension.

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13
Q

Shroedinger’s model

A

Electrons can be considered as wavefunctions. For the wavefunction, (amplitude)2 is proportional to probability of finding an electron at a given point.

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14
Q

Heisenberg’s uncertainty principle

A

It is impossible to measure exactly the momentum and position of a particle simultaneously. This is also true of energy and time.

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15
Q

Beta decay

A

The emission from the nucleus of an electron or a positron (antiparticle of electron). The energies of the emitted particles form a continuous spectrum.

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16
Q

Neutrino and antineutrino

A

To account for loss of energy (mass difference) and momentum, the neutrino and antineutrino were predicted. In β- decay, an antineutrino is emitted with the electron; in β+ decay, a neutrino is emitted with a positron.

17
Q

Exponential decay

A

The rate of decay is proportional to the number of nuclei. The more nuclei there are, the faster the sample decays (remember negative sign):
dN/dt α -N

18
Q

Bohr model of atom

A

The energy of electron orbits is quantized and the energy of the spectral lines of hydrogen are predicted correctly.

19
Q

Decay constant

A

The probability of decay of a nucleus in unit time. Units are s-1
dN/dt = -λN

20
Q

Activity

A

The number of decays in a second. A=λN