Atomic, Nuclear Properties and Electromagnetic Radiation

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46 Terms

1
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What is the letter, number and units that denote Planck’s Constant?

h = 6.63 × 10-34 J-s

2
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Describe the Pauli Exclusion Principle

No 2 electrons can occupy the same state in an atom.

3
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What is the formula and units for the radius of an atom?

r = n2ao (nm)

Where,

  • n = shell number

  • ao = 0.0529nm

4
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What is Bohr’s Radius?

The radius of an atom when n=1, equal to ao (0.0529nm)

5
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What is ground state in terms of electron orbital energy levels?

The lowest energy level that occurs when n=1, therefore is -13.6eV

6
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What is the formula and units for the energy of an electron orbit?

E = -13.6/n2 (eV)

7
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Describe Electron Binding Energy

The amount of energy that keeps an electron bound to an atom, equal to ionisation energy.

8
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Name and describe the 2 factors that affect Electron Binding Energy

  • Shell number (n) - as n decreases, electron binding energy increases

  • Atomic size - as atomic size increases, electron binding energy also increases

9
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Explain the uncertainty principle and how classical and quantum physics contribute

The uncertainty principle explains the barriers and limitations of precisely knowing measurements about particles.

  • Classical physics offers no uncertainty to measurements

  • However quantum physics predicts small uncertainties, eg. Simultaneous measurements of a particles location and momentum suggests that knowing location more precisely corresponds to knowing momentum less precisely and vice versa.

10
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Give the formula and units for energy of a particle and break down the formula.

E = h x f (J)

= h x c/λ (J)

Where,

  • h = Planck’s Constant (J-s)

  • f = frequency (Hz)

  • c = speed of light (3×108)

  • λ = wavelength (nm)

11
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Give the formula for wavelength of a particle

λ = h/mv

Where,

  • h = Planck’s Constant (J-s)

  • m = mass of particle (kg)

  • v = velocity of particle (m/s)

12
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What is a femtometer

1 fm = 10-15 m

13
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Give the formula and units for the average radius of a nucleus

r = roA1/3 (fm)

Where,

  • ro = 1.2 fm

  • A = mass number (number of nucleons)

14
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Explain why all nuclei have similar density

The volume and mass of nuclei are directly proportional to the number of nucleons.

15
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Explain nuclear stability referring to the 2 nuclear forces.

The nucleus contains 2 forces, Coulomb and nuclear forces. Coulomb forces are repulsive forces between protons that should cause a nucleus to split. However, nuclear forces are stronger than Coulomb forces and are attractive forces between all nuclear particles, keeping the nucleus stable.

16
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Explain the stability of light and heavy nuclei.

  • Light nuclei are more stable when N = Z

  • Heavy nuclei are more stable when N > Z as more neutrons are required to keep the nucleus stable while Z value and Coulomb forces increase

17
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When do nuclei become unstable

When Z > 83

18
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Explain the binding energy of nuclei.

The amount of energy required to separate nucleons.

19
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Explain how binding energy of a nucleus and nucleon is calculated including units.

  1. Calculate mass defect (combined mass of each nucleon - total mass of nucleus) in u

  2. Multiply the mass defect by 931.5 MeV/u for the binding energy of the nucleus in MeV

  3. Divide the binding energy by A value for the binding energy per nucleon in MeV

20
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Give the formula and units for decay rate/activity

R = λN

Where,

  • λ = decay constant

  • N = number of particles

21
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Give the formula to convert Curie to Becquerels

Ci = Bq/3.7 × 1010

22
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Order the mass of electrons, protons and neutrons from lightest to heaviest

  • Electron

  • Proton

  • Neutron

23
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Explain the relationship between the movement of charges and electric and magnetic fields

  • Stationary charges produce an electric field

  • Charges with constant velocity produce electric and magnetic fields

  • Accelerating chargers produce electric fields, magnetic fields and electromagnetic waves

24
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Explain why electromagnetic waves are considered transverse waves.

Because the electric and magnetic fields are orientated perpendicular to one another and both are perpendicular to the direction of motion.

25
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Why is light considered a type of electromagnetic wave

Electromagnetic waves travel at the speed of light, therefore light is an electromagnetic wave.

26
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Give the units for the different types of electromagnetic waves.

  • Larger such as radio and microwaves have units of frequency (Hz)

  • Moderate such as infrared and visible light have units of m

  • Smaller such as x and gamma rays have units of energy (eV)

27
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List the 5 behaviours of electromagnetic waves.

  • Reflection

  • Absorption

  • Diffraction

  • Scatter

  • Refraction

28
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Explain reflection

Incident light hitting and bouncing off an object.

29
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Explain absorption

Incident light hits an object, causing atoms within the object to vibrate and release heat.

30
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Explain diffraction

Waves bending and spreading around an object, typically when the object has a similar size to the wavelength.

31
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Explain a spectrometer.

A spectrometer utilizes diffraction to separate light into a spectrum of different wavelengths, creating a spectral signature.

32
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Explain scatter

Scatter involves light bouncing off an object in a variety of directions.

33
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Explain refraction

Light bending and changing direction as it passes through a different medium.

34
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Order the speed of light as it travels through air, water and a vacuum from fastest to slowest.

  • Vacuum

  • Air

  • Water

35
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Order the types of electromagnetic waves from largest to smallest.

  • Radiowaves

  • Microwaves

  • Infrared waves

  • Visible light

  • Ultraviolet waves

  • X-rays

  • Gamma rays

36
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Explain how a radio works to produce sound.

Radio receives different wavelengths of radiowaves and convert them into vibrations, creating sound waves.

37
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Name 3 uses of microwaves

  • Heating food

  • Predicting the weather forecast

  • GPS tracking

38
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Give 1 use of infrared waves and explain how they are detected

  • Remote controls changing TV channels

Infrared waves are not visible by the naked eye but can be detected as heat through night-vision goggles and infrared cameras.

39
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Explain the range of visible light.

The smallest and only segment of electromagnetic waves visible to the human eye, between 400-700nm.

40
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Explain and describe how UV waves are divided.

  • UV-A

  • UV-B - harmful rays causing sunburn, however 95% absorbed by the ozone layer in the atmosphere

  • UV-C - most harmful, however almost completely absorbed by the atmosphere

41
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Explain the difference between soft and hard x-rays.

Soft x-rays have a larger wavelength and lower energy than hard x-rays

42
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Explain the difference between ionising and non-ionising radiation.

Ionising radiation has a larger amount of energy that allows it to eject an electron from an atom, whereas non-ionising does not have enough energy to do this.

43
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Explain the difference between electromagnetic and particulate radiation in terms of their process of ionisation.

  • Electromagnetic radiation is indirectly ionising as photons collide with a target, transferring the energy that is absorbed to remove an electron.

  • Whereas particulate radiation is directly ionising as the particles directly interact with the target to remove an electron.

44
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Give the ionisation rates of EM waves, alpha particles and beta particles

  • EM waves - ~100 ion pairs per cm

  • Alpha particles - ~40,000 atoms per cm

  • Beta particles - several hundred atoms per cm

45
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Explain the photoelectric effect and how it demonstrates the particle nature of light.

Photoelectric effect involves electrons being emitted from a material when light hits it. This shows that light can act as photons to transfer energy and dislodge an electron within a material.

46
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