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Back to E: Nuclear and quantum physics

E.1 Structure of atom

Practice exam-style IB Physics questions for Structure of atom, aligned with the syllabus and grouped by topic.

Question 1
SL • Paper 1A
Easy
Non Calculator

A neutral atom is represented by 1840X^{40}_{18}X. How many neutrons does the nucleus contain?

A.

18

B.

40

C.

22

D.

58

Question 2
SL • Paper 1A
Easy
Non Calculator

In the Geiger–Marsden–Rutherford experiment, a very small number of alpha particles were scattered through angles greater than 90°. What conclusion follows from this observation?

A.

Electrons contain most of the mass of the atom.

B.

The positive charge of the atom is spread uniformly throughout its volume.

C.

The atom contains a small, dense, positively charged nucleus.

D.

Alpha particles are negatively charged.

Question 3
SL • Paper 1A
Easy
Non Calculator

A low-pressure gas is placed in front of a continuous source of white light. The spectrum observed after the light passes through the gas contains dark lines. What type of spectrum is observed?

A.

Absorption line spectrum

B.

Continuous spectrum

C.

Emission line spectrum

D.

Diffraction spectrum

Question 4
SL • Paper 1A
Easy
Non Calculator

An atom changes from a lower energy level to a higher energy level. What must occur?

A.

The atom emits a continuous range of photon energies.

B.

A photon with energy equal to the level difference is absorbed.

C.

A photon with any energy less than the level difference is absorbed.

D.

A photon with energy equal to the level difference is emitted.

Question 5
HL • Paper 1A
Easy
Non Calculator

Two nuclei have nucleon numbers AA and 27A27A. What is the ratio of their radii, R27A/RAR_{27A}/R_A?

A.

27

B.

1

C.

3

D.

9

Question 6
SL • Paper 2
Easy
Calculator

Alpha particles are incident on a thin metal foil in a Rutherford scattering experiment.

Schematic of alpha particles from a source incident on a thin metal foil with a surrounding fluorescent screen and example straight, slightly deflected, and back-scattered paths labelled.
1.

State one observation for most alpha particles.

[1]
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2.

State the surprising observation for a very small fraction of alpha particles.

[1]
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3.

Outline the inference made about the atom from the surprising observation.

[1]
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Question 7
SL • Paper 2
Easy
Calculator

A nucleus is represented by 2963X^{63}_{29}X.

1.

State the number of protons.

[1]
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2.

Determine the number of neutrons.

[1]
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3.

State the number of electrons in the neutral atom.

[1]
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Question 8
SL • Paper 1A
Medium
Non Calculator

An atom emits a photon of frequency 5.0imes1014extHz5.0 imes10^{14}\, ext{Hz}. What is the energy of the photon?

A.

$3.3 imes10^{-19}\, ext{J}$

B.

$7.5 imes10^{47}\, ext{J}$

C.

$3.0 imes10^{8}\, ext{J}$

D.

$1.3 imes10^{-48}\, ext{J}$

Question 9
SL • Paper 1A
Medium
Non Calculator

Why can an emission spectrum be used to identify an element in a gas sample?

A.

Each element emits all visible wavelengths with equal intensity.

B.

Each element emits photons only from its nucleus.

C.

Each element has the same spectrum at low pressure.

D.

Each element has a distinctive pattern of allowed energy differences.

Question 10
SL • Paper 1A
Medium
Non Calculator

The same gas is used to produce an emission spectrum and an absorption spectrum. How are the wavelengths of the bright emission lines related to the wavelengths of the dark absorption lines?

A.

They are the same for transitions between the same energy levels.

B.

The absorption wavelengths form a continuous range.

C.

They are unrelated because absorption involves electrons only.

D.

The emission wavelengths are always half the absorption wavelengths.

Question 11
HL • Paper 1A
Medium
Non Calculator

In the model R=R0A1/3R=R_0A^{1/3}, what is the approximate dependence of nuclear density on nucleon number AA?

A.

It is approximately independent of $A$.

B.

It is proportional to $A^{1/3}$.

C.

It is proportional to $A^{-1}$.

D.

It is proportional to $A$.

Question 12
HL • Paper 1A
Medium
Non Calculator

Rutherford scattering predictions fail at sufficiently high alpha-particle energies. What is the main reason?

A.

The alpha particles become electrically neutral.

B.

The target nuclei lose all their protons.

C.

The electrons in the atom cause all large-angle scattering.

D.

The alpha particles approach close enough for the strong nuclear interaction to affect them.

Question 13
HL • Paper 1A
Medium
Non Calculator

What is the energy of the n=2n=2 level in hydrogen according to the Bohr model?

A.

$-54.4\, ext{eV}$

B.

$-13.6\, ext{eV}$

C.

$+3.40\, ext{eV}$

D.

$-3.40\, ext{eV}$

Question 14
HL • Paper 1A
Medium
Non Calculator

What is Bohr’s quantization condition for the angular momentum of an electron in a hydrogen orbit?

A.

$mv^2/r=nh/2\pi$

B.

$hf=nh/2\pi$

C.

$mvr=nh/2\pi$

D.

$mvr=h/2\pi n$

Question 15
SL • Paper 2
Medium
Calculator

A low-pressure gas produces a spectrum consisting of bright lines on a dark background.

Line spectrum with several bright vertical lines at different positions on a dark background and an arrow labelled increasing wavelength.
1.

Name this type of spectrum.

[1]
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2.

Explain why this spectrum provides evidence for discrete atomic energy levels.

[1]
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Question 16
SL • Paper 2
Medium
Calculator

An atom emits a photon during a transition of energy 3.20imes1019extJ3.20 imes10^{-19}\, ext{J}.

1.

Calculate the frequency of the photon.

[1]
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2.

State how the frequency would change for a larger energy gap.

[1]
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Question 17
SL • Paper 2
Medium
Calculator

Distinguish between an emission line spectrum and an absorption line spectrum. [2]

Question 18
HL • Paper 2
Medium
Calculator

A nucleus has nucleon number A=64A=64. Use R0=1.2imes1015extmR_0=1.2 imes10^{-15}\, ext{m}.

1.

Calculate its nuclear radius.

[1]
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2.

State one assumption in the model R=R0A1/3R=R_0A^{1/3}.

[1]
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Question 19
SL • Paper 1B
Medium
Non Calculator

A student counts scintillations at different scattering angles in an alpha-particle scattering experiment using a thin gold foil.

Count rate of alpha particles measured at different scattering angles.
1.

State the general trend shown by the count rate as scattering angle increases.

[1]
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2.

Identify the observation that is not explained by the Thomson model.

[1]
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3.

Explain what this observation implies about the distribution of positive charge in the atom.

[1]
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Question 20
SL • Paper 1B
Medium
Non Calculator

The table gives information for four neutral atoms. Some entries are missing.

AtomProton number ZNucleon number ANeutron number NElectrons
P818?8
Q12?1312
R81688
S14291514
1.

Determine the missing neutron number for isotope P.

[1]
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2.

Determine the missing nucleon number for isotope Q.

[1]
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3.

Identify the two isotopes of the same element.

[1]
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4.

Explain your answer to (c).

[1]
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Question 21
SL • Paper 1A
Medium
Non Calculator

A photon emitted by an atom has energy 2.5exteV2.5\, ext{eV}. What is its wavelength? Use hc=1.24imes106exteVmhc=1.24 imes10^{-6}\, ext{eV m}.

A.

$5.0 imes10^{-7}\, ext{m}$

B.

$3.1 imes10^{-6}\, ext{m}$

C.

$2.0 imes10^{-6}\, ext{m}$

D.

$8.1 imes10^{5}\, ext{m}$

Question 22
HL • Paper 1A
Medium
Non Calculator

In a head-on alpha-particle scattering experiment with a fixed target nucleus, the alpha-particle kinetic energy is doubled. What happens to the distance of closest approach, assuming only electric repulsion?

A.

It is unchanged.

B.

It is halved.

C.

It is reduced by a factor of four.

D.

It is doubled.

Question 23
HL • Paper 1A
Medium
Non Calculator

A hydrogen atom makes a transition from n=3n=3 to n=2n=2. What is the photon energy?

A.

$1.89\, ext{eV}$

B.

$12.1\, ext{eV}$

C.

$4.91\, ext{eV}$

D.

$3.40\, ext{eV}$

Question 24
HL • Paper 1A
Medium
Non Calculator

In the de Broglie interpretation of Bohr orbits, what condition must an allowed circular orbit satisfy?

A.

The electron emits radiation continuously as it moves.

B.

The electron speed is equal to the speed of light.

C.

An integer number of electron wavelengths fits around the circumference.

D.

The electron wavelength is larger than the diameter of the atom.

Question 25
SL • Paper 2
Medium
Calculator

A spectral line has wavelength 6.56imes107extm6.56 imes10^{-7}\, ext{m}.

1.

Calculate the photon energy in eV. Use hc=1.24imes106exteVmhc=1.24 imes10^{-6}\, ext{eV m}.

[1]
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2.

State whether this photon could be absorbed by an atom if no allowed energy gap has this value.

[1]
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3.

Explain your answer to (b).

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Question 26
SL • Paper 2
Medium
Calculator

The spectrum of a star contains dark lines that match some laboratory lines for hydrogen.

Two aligned spectra: a stellar absorption spectrum and a labelled laboratory hydrogen reference spectrum, with some coincident line positions and an increasing wavelength arrow.
1.

Suggest what this indicates about the outer layers of the star.

[1]
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2.

Explain why a laboratory spectrum can be used for this comparison.

[1]
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Question 27
HL • Paper 2
Medium
Calculator

Use the relationship R=R0A1/3R=R_0A^{1/3} to explain why nuclear density is approximately independent of nucleon number. [3]

Question 28
HL • Paper 2
Medium
Calculator

Rutherford scattering of alpha particles by a target nucleus agrees with a purely electric model at low energies but not at sufficiently high energies.

1.

State what happens to the distance of closest approach when the alpha-particle energy is increased.

[1]
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2.

Explain why deviations from Rutherford scattering can then occur.

[1]
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Question 29
HL • Paper 2
Medium
Calculator

For hydrogen, En=13.6/n2exteVE_n=-13.6/n^2\, ext{eV}.

1.

Calculate the energy of the n=4n=4 level.

[1]
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2.

Calculate the energy of the photon emitted in a transition from n=4n=4 to n=2n=2.

[1]
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3.

State the spectral region for transitions ending at n=2n=2.

[1]
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Question 30
HL • Paper 2
Medium
Calculator

The Bohr model describes stationary states in hydrogen.

1.

State what is meant by the ground state of hydrogen.

[1]
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2.

Explain why the bound-state energies in the Bohr model are negative.

[1]
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Question 31
SL • Paper 1B
Medium
Non Calculator

An energy-level diagram for an atom is shown. Three downward transitions are labelled P, Q and R.

Energy-level diagram with four horizontal levels labelled by energy increasing upward. Three downward arrows P, Q and R have visibly different energy gaps, including one largest and one smallest gap.
1.

Identify the transition that emits the highest-frequency photon.

[1]
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2.

Identify the transition that emits the longest-wavelength photon.

[1]
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3.

Explain your answers to

[1]
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4.

and (b).

[1]
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5.

State why only three spectral lines are shown rather than a continuous spectrum.

[1]
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Question 32
SL • Paper 1B
Medium
Non Calculator

A spectrum from an unknown low-pressure gas is compared with reference spectra for three elements.

Scatter plot of emission line wavelengths for an unknown gas and three reference elements.
1.

Identify which element is present in the unknown gas.

[1]
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2.

State the evidence for your answer.

[1]
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3.

Suggest why not every line in the unknown spectrum needs to match this one element.

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4.

Explain why line spectra can be used as chemical fingerprints.

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Question 33
HL • Paper 1B
Medium
Non Calculator

Data for several nuclei are plotted as nuclear radius RR against A1/3A^{1/3}.

Nuclear radius plotted against the cube root of nucleon number, with a straight best-fit line through the origin.
1.

State what the straight-line graph indicates about the relationship between RR and AA.

[1]
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2.

Determine R0R_0 from the gradient of the graph.

[1]
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3.

Explain why this relationship implies that nuclear volume is proportional to AA.

[1]
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4.

State the implication for nuclear density.

[1]
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Question 34
SL • Paper 2
Medium
Calculator

A beam containing all visible wavelengths passes through a cool low-pressure gas. Some wavelengths are missing from the transmitted beam.

1.

Explain why only some wavelengths are absorbed.

[1]
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2.

Explain why the missing wavelengths appear dark when viewed in the original direction, even though photons may later be emitted.

[1]
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Question 35
HL • Paper 2
Medium
Calculator

An alpha particle of kinetic energy 5.0extMeV5.0\, ext{MeV} is incident head-on on a nucleus with proton number Z=50Z=50. Assume only electric repulsion. Use k=8.99imes109extNm2extC2k=8.99 imes10^9\, ext{N m}^2 ext{C}^{-2} and e=1.60imes1019extCe=1.60 imes10^{-19}\, ext{C}.

1.

State the charge of the alpha particle.

[1]
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2.

Calculate the distance of closest approach.

[1]
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Question 36
HL • Paper 2
Medium
Calculator

In the Bohr model, the angular momentum of an electron in a hydrogen atom is quantized.

Circular orbit showing an electron wave fitting an integer number of wavelengths around the circumference, with radius r and de Broglie wavelength labelled.
1.

State Bohr’s angular momentum condition.

[1]
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2.

Explain how the de Broglie standing-wave picture leads to this condition.

[1]
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Question 37
HL • Paper 2
Medium
Calculator

Discuss two limitations of the Bohr model of the atom. [4]

Question 38
SL • Paper 1B
Hard
Non Calculator

A graph shows photon energy plotted against frequency for light emitted by several atomic transitions.

Photon energy plotted against frequency for emitted spectral lines.
1.

State the relationship shown by the graph.

[1]
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2.

Determine Planck’s constant from the gradient of the graph.

[1]
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3.

Suggest one reason why a measured point may not lie exactly on the best-fit line.

[1]
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4.

Explain how the graph supports the photon model of light.

[1]
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Question 39
HL • Paper 1B
Hard
Non Calculator

The graph shows the measured number of alpha particles scattered at each angle for two incident kinetic energies, together with the Rutherford prediction.

Scattered alpha-particle count rate versus angle for two incident energies and a Rutherford prediction.
1.

State which energy agrees better with Rutherford scattering.

[1]
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2.

Identify the angle region where deviations are most evident.

[1]
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3.

Explain why the higher-energy data deviate from the prediction.

[1]
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4.

Suggest what information can be obtained from the energy at which deviations begin.

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Question 40
HL • Paper 1B
Hard
Non Calculator

A table gives the distance of closest approach for alpha particles incident head-on on the same target nucleus at different kinetic energies.

Kinetic energy / MeVClosest approach / m
4.05.69 × 10^-14
5.04.55 × 10^-14
6.03.79 × 10^-14
7.03.25 × 10^-14
8.02.84 × 10^-14
1.

Describe the relationship between distance of closest approach and alpha-particle kinetic energy.

[1]
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2.

Use one row of the table to determine the proton number ZZ of the target nucleus.

[1]
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3.

Explain why the calculated distance is not a direct measurement of the nuclear radius.

[1]
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Question 41
HL • Paper 1B
Hard
Non Calculator

The diagram shows the first five energy levels of hydrogen calculated using En=13.6/n2exteVE_n=-13.6/n^2\, ext{eV}.

Hydrogen energy-level diagram for n=1 to n=5 with energies labelled in eV and several possible downward transitions indicated. Levels become closer together near zero energy.
1.

Identify the transition shown that emits the shortest wavelength.

[1]
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2.

Calculate the photon energy for the transition from n=5n=5 to n=2n=2.

[1]
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3.

Determine whether the photon in

[1]
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4.

is in the Balmer series.

[1]
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5.

Explain why the energy levels get closer together as nn increases.

[1]
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Question 42
SL • Paper 2
Hard
Calculator

The Geiger–Marsden–Rutherford experiment led to a change in the model of the atom.

Apparatus diagram showing alpha source, collimated alpha beam, thin gold foil, evacuated chamber, movable fluorescent screen/detector, and representative alpha paths.
1.

Outline the experimental arrangement and the main observations.

[1]
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2.

Discuss how these observations led to the nuclear model of the atom and why they were inconsistent with the Thomson model.

[1]
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Question 43
SL • Paper 2
Hard
Calculator

Line spectra are evidence for discrete atomic energy levels.

1.

Distinguish between an emission line spectrum and an absorption line spectrum.

[1]
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2.

Explain how emission and absorption spectra arise from atomic transitions and why the same gas can have matching emission and absorption wavelengths.

[1]
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Question 44
SL • Paper 2
Hard
Calculator

An atom has two energy levels separated by 2.10exteV2.10\, ext{eV}.

1.

Calculate the frequency of a photon emitted during a transition between these levels.

[1]
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2.

Explain, using this example, the conditions for photon emission and absorption in atoms.

[1]
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Question 45
HL • Paper 1B
Hard
Non Calculator

A simulation shows electron waves around circular hydrogen orbits. Some waves join smoothly after one circuit and others do not.

Three circular orbits labelled A, B and C with sinusoidal electron waves drawn around the circumference. One has an integer number of wavelengths fitting exactly; others have a mismatch at the join. Radius and wavelength labels included.
1.

Identify which orbit is allowed by the standing-wave condition.

[1]
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2.

State the standing-wave condition for an allowed orbit.

[1]
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3.

Show how this condition leads to angular momentum quantization.

[1]
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4.

Suggest one reason why the Bohr model is not a complete model of atoms.

[1]
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Question 46
SL • Paper 2
Hard
Calculator

Spectra from stars can be used to infer physical information without collecting samples.

Stellar spectrum with absorption lines compared to labelled laboratory reference spectra for several elements, plus an indication of a continuous background spectrum.
1.

Outline how a spectrometer can identify chemical elements in a star.

[1]
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2.

Evaluate the use of stellar spectra for determining composition and other properties of stars.

[1]
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Question 47
HL • Paper 2
Hard
Calculator

Nuclear radius measurements are described by R=R0A1/3R=R_0A^{1/3}.

1.

Calculate the radius of a nucleus with A=125A=125 using R0=1.2imes1015extmR_0=1.2 imes10^{-15}\, ext{m}.

[1]
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2.

Evaluate the implication of this relationship for nuclear volume and density.

[1]
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Question 48
HL • Paper 2
Hard
Calculator

An alpha particle is fired head-on at a stationary nucleus of proton number ZZ.

Head-on alpha-particle approach to a target nucleus, showing initial kinetic energy, charges +2e and +Ze, and distance of closest approach $r_c$ where the alpha particle momentarily stops.
1.

Derive the expression for the distance of closest approach, rcr_c, assuming only electric repulsion.

[1]
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2.

Discuss how changing the alpha-particle energy and target proton number affects rcr_c, and why deviations from Rutherford scattering may occur at high energies.

[1]
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Question 49
HL • Paper 2
Hard
Calculator

The Bohr model gives the hydrogen energy levels as En=13.6/n2exteVE_n=-13.6/n^2\, ext{eV}.

Hydrogen energy-level diagram showing n=1, n=2, n=3 and the zero-energy ionization limit, with a downward transition from n=3 to n=2 labelled.
1.

Calculate the wavelength of the photon emitted for the transition from n=3n=3 to n=2n=2. Use hc=1.24imes106exteVmhc=1.24 imes10^{-6}\, ext{eV m}.

[1]
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2.

Explain the physical meaning of negative energy levels and the convergence of the levels at high nn.

[1]
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Question 50
HL • Paper 2
Hard
Calculator

Bohr’s model introduced quantized orbits for hydrogen.

1.

State the angular momentum quantization condition and the corresponding de Broglie standing-wave condition.

[1]
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2.

Compare and contrast the successes and limitations of the Bohr model for explaining atomic spectra.

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E.2 Quantum physics