Quantum and Nuclear Physics (topic 7 & 12) Flashcards

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1
Q

The Photoelectric Effect

A

Refers to the emission of electrons from a metal surface as a result of the absorption of electromagnetic wave energy. Shows how light (usually thought of as a wave) can exhibit particle-like behavior.

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2
Q

Davisson-Germer Experiment

A

Electrons were scattered from atoms and these scattered electrons produced an interference pattern just like waves.

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3
Q

Thomas Young’s Double Slit Experiment

A

Shows wave behavior of light

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4
Q

Electron Diffraction

A

Shows how electrons (usually thought of as particles) can exhibit wavelike behavior (diffraction and interference).

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5
Q

Beta Decay

A

Is a process by which a nucleus emits an electron or positron. It does not showcase any wave-particle duality.

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6
Q

Bohr’s Model for the Hydrogen Atom

A

The angular momentum of the electron is quantized having values that are multiples of h/2π

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7
Q

Photon Energy Equation (E)

A

E = hf or λ = hc / E

where
E = photon energy (eV or J)
h = Planck’s constant
f = frequency (Hz)
c = speed of light
λ = wavelength (electromagnetic wave)

E is proportional to its frequency

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8
Q

Work Function Equation (phi)

A

φ = h f0

where
φ = Work function (phi)
h = Planck’s constant
f0 = threshold frequency (f0)

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9
Q

The De Broglie Hypothesis

A

Suggests that all matter exhibits wave-like properties. In particular, the momentum of a particle is related to its wavelength where the De Broglie wavelength may be deduced by the following formula:

p = h/λ -> λ = h/p -> λ = h/mv

where
p = momentum
h = Planck’s constant
λ = wavelength
m = mass
v = velocity.

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10
Q

Wave-Particle duality

A

refers to matter acting as both waves and particles.

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11
Q

Quantum

A

Refers to the smallest discrete amount of something.

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12
Q

Photon

A

Is a quantum of electromagnetic radiation (light). Exhibit wave properties under refraction or interference. Exhibit wave properties under its emission or absorption.

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13
Q

Angular Momentum Equation

A

mvr = nh / 2π

where
m = mass of electron,
v = speed of electron,
r = radius of orbit,
n = interger,
h = Planck’s constant.

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14
Q

Schrödinger model of the atom

A

P(r) = |φ|^2 multiplied by Δv

where
P(r) = probability of finding an electron in a small volume,
|φ|^2 = amplitude of wave function squared,
Δv = small volume.

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15
Q

Heisenberg’s Uncertainty Principle

A

The act of observing (making a measurement) alters the system.

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16
Q

Heisenberg’s Uncertainty Equation

A

Δx multiplied by Δp is greater than or equal to h / 4π

OR

ΔE multiplied by Δt is greater than or equal to h / 4π

where
Δx = uncertainty on position,
Δp = uncertainty on momentum,
ΔE = uncertainty on energy,
Δt = uncertainty on time,
h = Planck’s constant

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17
Q

Nuclear Radius Equation

A

R = R0 multiplied by A^1/3

where
R = nuclear radius (m),
R0 = Fermi radius constant,
A = atomic mass number

18
Q

What happens when Alpha decay occurs

A

Add Helium 4

19
Q

What happens when Beta decay occurs

A

Add a Beta minus (electron) + anti-electron neutrino

OR

a Beta plus (positron) + electron neutrino

20
Q

Decay Equation

A

N = N0 multiplied by e ^ -λ t

where
N = final mass (or activity),
N0 = initial mass (or activity),
t = time elapsed,
λ = decay constant = probability of decay at a certain time.

21
Q

Decays / Seconds unit

A

Becquerel

22
Q

Half-life Equation

A

T1/2 = ln2/λ

where
T1/2 = half-life of exponential decay,
ln = natural log.

23
Q

Element notation

A

Number on top of the molecule = mass # (number of nucleons) n + p
Number at the bottom of the molecule = atomic # (# of protons)

24
Q

Isotopes

A

Same atomic number, different mass number

25
Q

Energy levels

A

Electrons get excited, go up in energy level. When they go back down, they emit a photon (light) with energy

Energy is quantized - only comes in multiples of h

26
Q

Energy levels (wavelengths and frequencies)

A

Smallest λ -> highest f and largest E

27
Q

Two types of Beta decay

A
  1. Electron-beta decay
  2. Positron-beta decay
28
Q

Gamma decay

A

γ = photon

**no charge

29
Q

Exponential decay

A

As parent particles lessen, daughter particles increase

30
Q

Binding energy

A

The energy released when a nucleus is assembled from its constituent parts. Every time a new element is made, there’s an energy that’s released.

Mass of left hand side ≠ mass of right hand side

31
Q

Einstein’s famous equation

A

ΔE = Δm c^2

where
ΔE = binding energy (eV or J)
Δm = mass defect (kg or u or (MeV) / c^2)
c = speed of light = 3 x 10^8 m s^-1

32
Q

6 types of quarks (every particle also has an anti-particle)

A
  1. Up
  2. Charm
  3. Top
  4. Down
  5. Strange
  6. Bottom
33
Q

Hadron

A

Particle made of quarks
ex. Baryon, Meson

34
Q

Baryon

A

Particle made of three quarks

35
Q

Meson

A

Particle made of two quarks (one quark + one anti-quark)

36
Q

Leptons

A

Other than quarks, there are other fundamental particles called leptons

37
Q

6 types of leptons (every particle also has an anti-particle)

A
  1. τ- = tau
  2. µ- = mu
  3. e- = electron
  4. ντ = tau-neutrino
  5. νµ = mu-neutrino
  6. νe = electron-neutrino
38
Q

Conservation

A

The idea that properties must be conserved (same before as after)

39
Q

Higgs boson

A

Responsible (through interactions) for mass

40
Q

4 main bosons

A
  1. g = gluon
  2. W+, W- = W-boson
  3. Z° = Z-boson
  4. γ = photon
41
Q

Strength of fundamental forces

A

Gravitational < Weak nuclear < Electromagnetic < Strong nuclear

42
Q

Band of stability in nuclei

A
  1. The darker the points, the more stable
  2. Nuclei further from the dark region are increasingly unstable and will quickly decay back into a more stable form
  3. Band of stability lies above the one to one ratio of protons and neutrons
  4. the stability of nuclei depends on the attractive and repulsive force
  5. the band of stability implies that the strong nuclear force must be very short-ranged in nature