Free worked solutions · 2026 Edition

IB Physics E.1: Structure of the atom worked solutions

Worked solutions to every practice question in E.1: Structure of the atom of Photon Physics: Study Guide for the IB Diploma (SL & HL). Try each question, then compare your working with the full solution.

  • SL & HL
  • 31 questions
  • Full worked solutions
  • Free, no sign-up

Basic practice

Question B1

Type B1 · Type N1 · protons, neutrons, electrons · P1A[1 mark]
The nuclide ^{56}_{26}\mathrm{Fe} forms the ion \mathrm{Fe}^{3+}. How many protons, neutrons and electrons does one of these ions have?
A. 26 protons, 30 neutrons, 23 electrons
B. 26 protons, 30 neutrons, 29 electrons
C. 23 protons, 30 neutrons, 26 electrons
D. 26 protons, 56 neutrons, 23 electrons
Show solutionHide solution
The lower number is the proton number: 26. Neutrons = 56 - 26 = 30. The neutral atom has 26 electrons and the 3+ ion has lost three, leaving 23. B adds three electrons instead of removing them; C changes the proton number, which would make a different element; D reads the nucleon number as the neutron number.

Final answer

A

Question B2

Type B2 · Type N2 · atom and nucleus sizes · P1A[1 mark]
In a scale model of an atom, the nucleus is a dot 2\,\mathrm{mm} across. About how wide should the whole atom be in the same model?
A. 2\,\mathrm{m}
B. 20\,\mathrm{m}
C. 200\,\mathrm{m}
D. 20\,\mathrm{km}
Show solutionHide solution
An atom is about 10^{-10}\,\mathrm{m} across and a nucleus about 10^{-15}\,\mathrm{m}, a ratio of 10^{5}. 2\,\mathrm{mm}\times10^{5} = 2\times10^{2}\,\mathrm{m} = 200\,\mathrm{m}. A, B and D use ratios of 10^{3}, 10^{4} and 10^{7}.

Final answer

C

Question B3

Type B3 · Type N3 · what scattering shows · P1A[1 mark]
A beam of alpha particles strikes a thin gold foil. Which result of this scattering experiment is the evidence that an atom's positive charge, and nearly all its mass, sit in a very small volume?
A. Most alpha particles passed through with little or no deflection.
B. About one alpha particle in several thousand came back off the foil at an angle above 90^\circ.
C. The number of alpha particles detected was the same at every angle.
D. Alpha particles were deflected towards the gold nuclei.
Show solutionHide solution
Turning an alpha particle back needs a very large repulsive force, which only a small, concentrated positive charge can supply. A is a real observation, but it shows that the atom is mostly empty space. C was not observed. D is wrong: the nucleus and the alpha particle are both positive, so the force is repulsive.

Final answer

B

Question B4

Type B4 · Type S1 · what line spectra show · P1A[1 mark]
Which statement about the line emission spectrum of a gas is correct?
A. The lines are produced when the nuclei of the atoms change energy.
B. Every line of the spectrum lies in the visible region.
C. Each line comes from photons emitted as electrons move to lower energy levels.
D. The lines show that the energy of an atom can take any value.
Show solutionHide solution
A line spectrum comes from electrons dropping between fixed atomic energy levels; each drop releases one photon of energy hf equal to the gap. A describes gamma emission from nuclei. B is false: many lines are in the ultraviolet or infrared. D is the opposite of what the lines show: only certain energies are allowed.

Final answer

C

Question B5

Type B5 · Type S3 · count the lines · P1A[1 mark]
An atom has four energy levels: -10.0\,\mathrm{eV}, -6.0\,\mathrm{eV}, -4.0\,\mathrm{eV} and -2.0\,\mathrm{eV}. Atoms are excited to the -2.0\,\mathrm{eV} level and return to the lowest level by every possible route. How many different wavelengths are emitted?
A. 3
B. 4
C. 6
D. 10
Show solutionHide solution
Six downward jumps are possible, with gaps 2.0, 2.0, 4.0, 4.0, 6.0 and 8.0\,\mathrm{eV}. Equal gaps give the same photon energy and so the same wavelength: only four values, 2.0, 4.0, 6.0 and 8.0\,\mathrm{eV}. C counts jumps, not distinct gaps; A counts only jumps to the lowest level (it has three).

Final answer

B

Question B6

Type B6 · Type S4 · rank the transitions · P1A[1 mark]
An atom has energy levels E_1 = -8.2\,\mathrm{eV}, E_2 = -4.6\,\mathrm{eV}, E_3 = -3.1\,\mathrm{eV} and E_4 = -2.5\,\mathrm{eV}. Which transition emits the photon of longest wavelength?
A. E_4 \to E_1
B. E_3 \to E_2
C. E_4 \to E_3
D. E_3 \to E_4
Show solutionHide solution
Longest wavelength means smallest photon energy, so the smallest downward gap: E_4\to E_3, 0.6\,\mathrm{eV}. A is the largest gap (shortest wavelength). D has the same gap but goes up, so it is an absorption, not an emission. B is 1.5\,\mathrm{eV}.

Final answer

C

Question B7

Type B7 · Type S5 · photon energy, eV and region · P1A[1 mark]
A photon has an energy of 2.6\,\mathrm{eV}. What is its wavelength, and in which region of the electromagnetic spectrum does it lie?
A. 4.8\times10^{-7}\,\mathrm{m}, visible
B. 4.8\times10^{-7}\,\mathrm{m}, ultraviolet
C. 7.7\times10^{-26}\,\mathrm{m}, gamma
D. 4.8\times10^{-9}\,\mathrm{m}, X-ray
Show solutionHide solution
E = 2.6\times1.60\times10^{-19} = 4.16\times10^{-19}\,\mathrm{J}; \lambda = hc/E = 1.989\times10^{-25}/4.16\times10^{-19} = 4.8\times10^{-7}\,\mathrm{m}, which is 478\,\mathrm{nm}, inside the visible range 400–700\,\mathrm{nm}. C forgets to convert eV to J; D slips a factor of 100 converting to nanometres; B names the wrong region.

Final answer

A

Question B8

Type B8 · Type S2 · exact-gap absorption · P1A[1 mark]
An atom has energy levels -9.0\,\mathrm{eV} (ground state), -5.0\,\mathrm{eV}, -3.5\,\mathrm{eV} and -1.0\,\mathrm{eV}. Atoms in the ground state are exposed to photons. Which photon energy can be absorbed?
A. 3.5\,\mathrm{eV}
B. 4.0\,\mathrm{eV}
C. 1.5\,\mathrm{eV}
D. 6.0\,\mathrm{eV}
Show solutionHide solution
Absorption needs a photon whose energy matches, exactly, a gap measured up from the ground state: 4.0, 5.5 or 8.0\,\mathrm{eV}. Only 4.0\,\mathrm{eV} is offered. A is the value of a level, not a gap. C is the gap between -5.0 and -3.5\,\mathrm{eV}, but no atom starts at -5.0\,\mathrm{eV}. D would lift the electron to -3.0\,\mathrm{eV}, which is not a level.

Final answer

B

Question B9

Type B9 · Type H1 · Bohr postulates · HL · P1A[1 mark]
Which statement is part of Bohr's model of the hydrogen atom?
A. The electron radiates energy continuously as it orbits the nucleus.
B. The angular momentum of the electron is a whole-number multiple of h/2\pi.
C. The number of undecayed nuclei in a sample falls exponentially with time.
D. The electron can orbit at any radius if its speed is suitable.
Show solutionHide solution
Bohr allowed only orbits with mvr = nh/2\pi, and in those orbits the electron does not radiate. A is the classical prediction Bohr rejected. C is the radioactive decay law (E.3). D is the classical picture; Bohr's condition restricts the radius to r\propto n^2.

Final answer

B

Question B10

Type B10 · Type H4 · angular momentum ratio · HL · P1A[1 mark]
In the Bohr model of hydrogen, what is \dfrac{\text{angular momentum of the electron in the } n = 3 \text{ state}}{\text{angular momentum of the electron in the ground state}}?
A. \tfrac13
B. 3
C. 9
D. \tfrac19
Show solutionHide solution
L = nh/2\pi, so L\propto n and the ratio is 3/1 = 3. C uses the radius ratio n^2; A and D invert.

Final answer

B

Question B11

Type B11 · Type R1 · nuclear radius from A · HL · P1A[1 mark]
Nucleus X has twice the radius of the nucleus ^{27}_{13}\mathrm{Al}. What is the nucleon number of X?
A. 54
B. 108
C. 216
D. 104
Show solutionHide solution
R = R_0A^{1/3}, so A\propto R^3. Doubling R multiplies A by 2^3 = 8: 8\times27 = 216. A doubles A; B multiplies by 4 (R^2); D multiplies the proton number 13 by 8.

Final answer

C

Question B12

Type B12 · Type H5 · one-electron ion · HL · P1A[1 mark]
For which of these ions can the Bohr model of a one-electron atom be used?
A. ^{7}_{3}\mathrm{Li}^{+}
B. ^{6}_{3}\mathrm{Li}^{2+}
C. ^{4}_{2}\mathrm{He}
D. ^{9}_{4}\mathrm{Be}^{2+}
Show solutionHide solution
The model needs exactly one electron. Electrons = Z - charge: A has 3-1 = 2; B has 3-2 = 1; C is a neutral atom with 2; D has 4-2 = 2. The nucleon number plays no part in the count.

Final answer

B

Tutorial practice

Question T1

Type T1 · Type N4 · alpha path: force and energy + N3, N1 · P2[7 marks]
A narrow beam of alpha particles is directed at a thin gold foil inside an evacuated chamber. A detector can be moved around the foil to any angle.
(a) A gold nucleus contains 79 protons and 118 neutrons. Write its nuclide notation. [1]
(b) State two observations made with the detector and the conclusion that each one supports. [4]
(c) One alpha particle travels directly towards a gold nucleus. Describe how its kinetic energy and the electric potential energy of the system change on the way in and on the way out. [2]
Show solutionHide solution
(a) Nucleon number 79 + 118 = 197 on top, proton number 79 below: ^{197}_{79}\mathrm{Au} (A1). (b) Nearly every alpha particle goes through undeviated or almost so (A1): the atom must be mostly empty (A1). A tiny minority swing through large angles, a few beyond 90^\circ (A1); that needs a strong repulsion from a tiny region holding the atom's positive charge and almost all its mass, the nucleus (A1). (c) As the alpha particle approaches, the repulsion does negative work on it: its kinetic energy decreases and the electric potential energy increases by the same amount, until the alpha particle stops for an instant (M1). On the way out the potential energy is converted back, and it leaves along the same line with its original kinetic energy (A1).

Final answer

(a) ^{197}_{79}\mathrm{Au}. (b) Almost straight alpha trajectories show that atoms contain mainly empty space. Rare backward scattering requires a tiny, massive centre carrying positive charge. (c) Kinetic energy falls to zero at the turning point while the potential energy rises by the same amount; on the way out the changes reverse.

Question T2

Type T2 · Type S1 · what line spectra show + S5 · P2[6 marks]
White light from a hot filament passes through a tube of cool hydrogen gas and then into a spectrometer. The spectrum is continuous except for some dark lines. One dark line is at 434\,\mathrm{nm}.
(a) Explain how the dark lines are formed. [3]
(b) Calculate the energy, in eV, of the photons that are missing at 434\,\mathrm{nm}. [2]
(c) The light from a distant star shows dark lines at the same set of wavelengths. State what this tells you about the star. [1]
Show solutionHide solution
(a) The hydrogen atoms have discrete energy levels, so they absorb only photons whose energy hf exactly equals the difference between two levels (M1). Absorbing a photon lifts an electron to a higher level (A1). The atoms then de-excite and re-emit the energy in all directions, so very little returns to the original beam and those wavelengths appear dark (A1). (b) E = hc/\lambda = (6.63\times10^{-34}\times3.00\times10^{8})/(434\times10^{-9}) = 4.58\times10^{-19}\,\mathrm{J} (M1); \div\,1.60\times10^{-19} = 2.86\,\mathrm{eV} (A1). (c) Each element has its own set of lines, so the matching pattern shows that hydrogen is present in the cooler gas around the star (A1).

Final answer

(a) Atoms absorb only photons whose energy equals a gap between their levels; electrons jump up; the energy is re-emitted in all directions, so those wavelengths are weak in the beam. (b) 2.86\,\mathrm{eV}. (c) Hydrogen is present in the outer layers of the star.

Question T3

Type T3 · Type S4 · rank the transitions + S3, S5 · P2[7 marks]
The four lowest energy levels of an atom are -12.0\,\mathrm{eV}, -4.8\,\mathrm{eV}, -2.6\,\mathrm{eV} and -1.6\,\mathrm{eV}.
(a) Every value is below zero. Explain what this tells you about the electron. [1]
(b) Atoms raised to the -1.6\,\mathrm{eV} level fall back to the lowest level by every route. How many different wavelengths appear in the light? [1]
(c) Calculate the longest and the shortest of these wavelengths. [3]
(d) Identify which emitted line, if any, lies in the visible range 400–700\,\mathrm{nm}. [2]
Show solutionHide solution
(a) Zero is the energy of an electron that has just escaped the atom; a negative value means the electron is bound and that much energy must be supplied to free it (A1). (b) Four levels give 4\times3/2 = 6 downward jumps, with gaps 1.0, 2.2, 3.2, 7.2, 9.4 and 10.4\,\mathrm{eV}, all different: 6 wavelengths (A1). (c) Longest from the smallest gap, 1.0\,\mathrm{eV}: \lambda = hc/E = 1.989\times10^{-25}/1.60\times10^{-19} = 1.24\times10^{-6}\,\mathrm{m} (M1)(A1). Shortest from 10.4\,\mathrm{eV}: 1.989\times10^{-25}/(10.4\times1.60\times10^{-19}) = 1.20\times10^{-7}\,\mathrm{m} (A1). (d) Visible photons have energies between hc/700\,\mathrm{nm} = 1.78\,\mathrm{eV} and hc/400\,\mathrm{nm} = 3.11\,\mathrm{eV} (M1). Only the 2.2\,\mathrm{eV} gap lies in this band: \lambda = 565\,\mathrm{nm}. The 3.2\,\mathrm{eV} line is at 388\,\mathrm{nm}, just into the ultraviolet (A1).

Final answer

(a) The electron is bound: energy must be supplied to remove it to zero energy (ionisation). (b) 6. (c) Longest 1.24\times10^{-6}\,\mathrm{m}; shortest 1.20\times10^{-7}\,\mathrm{m}. (d) Only the -2.6\to-4.8\,\mathrm{eV} line, at 565\,\mathrm{nm}.

Question T4

Type T4 · Type S7 · combine energy gaps · P2[5 marks]
In an atom, an electron falls from level C to level B and emits a photon of wavelength 820\,\mathrm{nm}. It then falls from B to level A and emits a photon of wavelength 410\,\mathrm{nm}.
(a) Calculate, in eV, the energy difference between levels C and A. [3]
(b) Determine the wavelength of the photon emitted in a direct jump from C to A. [1]
(c) A student adds the two wavelengths and gives 1230\,\mathrm{nm} as the answer to (b). Explain why this is wrong. [1]
Show solutionHide solution
(a) E_{CB} = hc/\lambda = 1.989\times10^{-25}/820\times10^{-9} = 2.43\times10^{-19}\,\mathrm{J} = 1.52\,\mathrm{eV} (M1). E_{BA} = 1.989\times10^{-25}/410\times10^{-9} = 4.85\times10^{-19}\,\mathrm{J} = 3.03\,\mathrm{eV} (A1). The gaps add: E_{CA} = 1.52 + 3.03 = 4.55\,\mathrm{eV} (A1). (b) \lambda = hc/E_{CA} = 1.989\times10^{-25}/(4.55\times1.60\times10^{-19}) = 273\,\mathrm{nm}; the same comes from 1/\lambda = 1/820 + 1/410 (A1). (c) Photon energies add because the levels are fixed; since E\propto1/\lambda, the direct jump has the largest energy and so the SHORTEST wavelength, not a longer one (A1).

Final answer

(a) 4.55\,\mathrm{eV}. (b) 273\,\mathrm{nm}. (c) Energies add, not wavelengths; a larger energy means a shorter wavelength.

Question T5

Type T5 · Type S8 · levels from photon energies + S2 · P2[6 marks]
An atom has only three energy levels. The lowest level is at -6.0\,\mathrm{eV}. Its emission spectrum contains photons of energies 1.8\,\mathrm{eV}, 2.6\,\mathrm{eV} and 4.4\,\mathrm{eV}. The 1.8\,\mathrm{eV} photon is emitted in a transition that starts at the highest level.
(a) Determine the energies of the other two levels. [3]
(b) Photons of energies 1.8\,\mathrm{eV}, 2.6\,\mathrm{eV} and 4.4\,\mathrm{eV} pass through a cool sample of these atoms, all in the lowest level. State which photons are absorbed, and explain why. [3]
Show solutionHide solution
(a) The largest photon energy spans the whole diagram (M1): highest level = -6.0 + 4.4 = -1.6\,\mathrm{eV} (A1). The 1.8\,\mathrm{eV} photon goes from the highest level to the middle one: -1.6 - 1.8 = -3.4\,\mathrm{eV}; check: -3.4 - (-6.0) = 2.6\,\mathrm{eV}, the third photon (A1). (b) An atom absorbs a photon only if its energy exactly equals a gap that starts at the level the atom is in (M1). From -6.0\,\mathrm{eV} the gaps are 2.6\,\mathrm{eV} and 4.4\,\mathrm{eV}, so these are absorbed (A1). The 1.8\,\mathrm{eV} gap starts at the middle level, which no atom in a cool sample occupies, so these photons pass through (A1).

Final answer

(a) Highest -1.6\,\mathrm{eV}; middle -3.4\,\mathrm{eV}. (b) 2.6\,\mathrm{eV} and 4.4\,\mathrm{eV}: each equals a gap from the lowest level. 1.8\,\mathrm{eV} would need an atom already in the middle level.

Question T6

Type T6 · Type S6 · spectrum to level diagram · P2[5 marks]
An atom has three energy levels: E_1 = -7.0\,\mathrm{eV}, E_2 = -6.8\,\mathrm{eV} and E_3 = -2.0\,\mathrm{eV}.
(a) Calculate the wavelengths of the three lines in its emission spectrum. [3]
(b) Explain why two of the lines lie very close together. [1]
(c) A spectrometer records wavelengths from 200\,\mathrm{nm} to 700\,\mathrm{nm} only. State how many lines it shows. [1]
Show solutionHide solution
(a) Gaps: 5.0, 4.8 and 0.2\,\mathrm{eV} (M1). \lambda = hc/E: 1.989\times10^{-25}/(5.0\times1.60\times10^{-19}) = 249\,\mathrm{nm} and 1.989\times10^{-25}/(4.8\times1.60\times10^{-19}) = 259\,\mathrm{nm} (A1); 1.989\times10^{-25}/(0.2\times1.60\times10^{-19}) = 6.22\times10^{-6}\,\mathrm{m}, in the infrared (A1). (b) The two lowest levels are only 0.2\,\mathrm{eV} apart, so the two jumps from E_3 differ in energy, and so in wavelength, by only a small amount (A1). (c) Two: the infrared line is far outside the range (A1).

Final answer

(a) 249\,\mathrm{nm} (E_3\to E_1), 259\,\mathrm{nm} (E_3\to E_2), 6.22\times10^{-6}\,\mathrm{m} (E_2\to E_1). (b) E_1 and E_2 are close, so jumps from E_3 to either have almost the same energy. (c) Two.

Question T7

Type T7 · Type H3 · electron orbit dynamics + H1 · HL · P2[7 marks]
In the Bohr model, the electron of a hydrogen atom in its ground state moves in a circle of radius 5.3\times10^{-11}\,\mathrm{m} around the proton.
(a) Use the electric force on the electron to show that it moves at about 2.2\times10^{6}\,\mathrm{m\,s^{-1}}. [2]
(b) Calculate the kinetic energy of the electron in eV. [2]
(c) Calculate the electric potential energy of the atom in eV, and hence its total energy. [2]
(d) Show that the angular momentum of the electron agrees with Bohr's condition for n = 1. [1]
Show solutionHide solution
(a) The electric force provides the centripetal force: ke^2/r^2 = mv^2/r (M1), so v = \sqrt{ke^2/(mr)} = \sqrt{8.99\times10^{9}\times(1.60\times10^{-19})^2/(9.11\times10^{-31}\times5.3\times10^{-11})} = 2.18\times10^{6}\,\mathrm{m\,s^{-1}} (A1). (b) E_K = \tfrac12mv^2 = 2.17\times10^{-18}\,\mathrm{J} (M1) = 13.6\,\mathrm{eV} (A1). (c) E_P = -ke^2/r = -4.34\times10^{-18}\,\mathrm{J} = -27.1\,\mathrm{eV} (A1); total = 13.6 - 27.1 = -13.6\,\mathrm{eV}, equal to the ground-state energy -13.6/1^2\,\mathrm{eV} (A1). (d) mvr = 9.11\times10^{-31}\times2.18\times10^{6}\times5.3\times10^{-11} = 1.05\times10^{-34}\,\mathrm{J\,s}, and h/2\pi = 1.06\times10^{-34}\,\mathrm{J\,s}: equal within the precision of the data (A1).

Final answer

(a) 2.18\times10^{6}\,\mathrm{m\,s^{-1}}. (b) 13.6\,\mathrm{eV}. (c) -27.1\,\mathrm{eV}; total -13.6\,\mathrm{eV}, the ground-state energy. (d) mvr = 1.05\times10^{-34}\,\mathrm{J\,s} = h/2\pi.

Question T8

Type T8 · Type H2 · Bohr energy gaps · HL · P2[6 marks]
The energy levels of hydrogen are given by E = -13.6/n^2\,\mathrm{eV}.
(a) Show that the energy of the n = 4 level is -0.85\,\mathrm{eV}. [1]
(b) An electron drops from n = 4 to n = 2. Calculate the frequency of the light given out. [3]
(c) Hydrogen atoms in the ground state absorb photons. Determine the ratio \dfrac{\text{energy absorbed in the jump } n=1\to n=2}{\text{energy absorbed in the jump } n=1\to n=3}. [2]
Show solutionHide solution
(a) E_4 = -13.6/4^2 = -13.6/16 = -0.85\,\mathrm{eV} (A1). (b) E_2 = -13.6/4 = -3.40\,\mathrm{eV}; gap = -0.85 - (-3.40) = 2.55\,\mathrm{eV} (M1) = 2.55\times1.60\times10^{-19} = 4.08\times10^{-19}\,\mathrm{J} (A1); f = E/h = 4.08\times10^{-19}/6.63\times10^{-34} = 6.15\times10^{14}\,\mathrm{Hz} (A1). (c) 1\to2: 13.6(1 - \tfrac14) = 10.2\,\mathrm{eV}; 1\to3: 13.6(1 - \tfrac19) = 12.1\,\mathrm{eV} (M1). Ratio = \tfrac34\big/\tfrac89 = 27/32 = 0.84 (A1). Using n values directly (2/3) is the usual slip.

Final answer

(a) -13.6/16 = -0.85\,\mathrm{eV}. (b) 6.15\times10^{14}\,\mathrm{Hz}. (c) 27/32 = 0.84.

Question T9

Type T9 · Type R4 · closest approach + R1 · HL · P2[7 marks]
An alpha particle (mass 6.64\times10^{-27}\,\mathrm{kg}, charge +2e) moves at 1.52\times10^{7}\,\mathrm{m\,s^{-1}} directly towards a gold nucleus, ^{197}_{79}\mathrm{Au}. Treat the gold nucleus as fixed.
(a) Calculate, in MeV, the kinetic energy the alpha particle starts with. [2]
(b) Determine the distance of closest approach. [3]
(c) Calculate the radius of the gold nucleus and state whether the alpha particle reaches its surface. Give a reason. [2]
Show solutionHide solution
(a) E_K = \tfrac12mv^2 = 0.5\times6.64\times10^{-27}\times(1.52\times10^{7})^2 = 7.67\times10^{-13}\,\mathrm{J} (M1); \div\,1.60\times10^{-13}\,\mathrm{J\,MeV^{-1}} = 4.79\,\mathrm{MeV} (A1). (b) When the alpha particle stops for an instant, its starting kinetic energy equals the electric potential energy of the pair: E_K = k(2e)(79e)/d (M1). d = 2\times79\times8.99\times10^{9}\times(1.60\times10^{-19})^2/7.67\times10^{-13} (A1) = 4.74\times10^{-14}\,\mathrm{m} (A1). (c) R = R_0A^{1/3} = 1.20\times10^{-15}\times197^{1/3} = 6.98\times10^{-15}\,\mathrm{m} (A1). d/R \approx 6.8: the alpha particle turns back well outside the nucleus, so only the electric force acts on it (A1).

Final answer

(a) 4.79\,\mathrm{MeV}. (b) 4.74\times10^{-14}\,\mathrm{m}. (c) 6.98\times10^{-15}\,\mathrm{m}; no, the closest approach is about 7 times the radius.

Question T10

Type T10 · Type R2 · constant nuclear density + R1 · HL · P2[6 marks]
Take the mass of a nucleus of nucleon number A to be A\times1.67\times10^{-27}\,\mathrm{kg}.
(a) Use R = R_0A^{1/3} to show that the density of a nucleus does not depend on A. [2]
(b) Calculate the density of nuclear matter. [2]
(c) A neutron star is a sphere of radius 12\,\mathrm{km} that has nuclear density throughout. Estimate its mass. [2]
Show solutionHide solution
(a) V = \tfrac43\pi R^3 = \tfrac43\pi R_0^3A (M1). \rho = \dfrac{A\times1.67\times10^{-27}}{\tfrac43\pi R_0^3A} = \dfrac{3\times1.67\times10^{-27}}{4\pi R_0^3}: A cancels (A1). (b) \rho = 3\times1.67\times10^{-27}/(4\pi\times(1.20\times10^{-15})^3) (M1) = 2.3\times10^{17}\,\mathrm{kg\,m^{-3}} (A1). (c) V = \tfrac43\pi(1.2\times10^{4})^3 = 7.24\times10^{12}\,\mathrm{m^3} (M1); M = \rho V = 2.31\times10^{17}\times7.24\times10^{12} = 1.7\times10^{30}\,\mathrm{kg}, close to the mass of the Sun (A1).

Final answer

(a) V = \tfrac43\pi R_0^3A, so \rho = 3m/(4\pi R_0^3) with no A. (b) 2.3\times10^{17}\,\mathrm{kg\,m^{-3}}. (c) 1.7\times10^{30}\,\mathrm{kg}.

Advanced practice

Question A1

Type A1 · Type S7 · combine energy gaps + S8, S2 · P2[7 marks]
A gas emits three spectral lines, at 248.6\,\mathrm{nm}, 414.4\,\mathrm{nm} and 621.6\,\mathrm{nm}. Its atoms have three energy levels; the lowest is at -7.4\,\mathrm{eV}.
(a) Show that the photon energies are 5.0\,\mathrm{eV}, 3.0\,\mathrm{eV} and 2.0\,\mathrm{eV}. [2]
(b) Explain how these energies are consistent with three levels. [1]
(c) Explain why the emission spectrum alone cannot fix the energy of the middle level. [1]
(d) White light passes through the cool gas, in which all atoms are in the lowest level. Dark lines appear at 248.6\,\mathrm{nm} and 621.6\,\mathrm{nm} only. Deduce the energies of the two upper levels. [3]
Show solutionHide solution
(a) E = hc/\lambda = 1.989\times10^{-25}/(248.6\times10^{-9}) = 8.00\times10^{-19}\,\mathrm{J} = 5.00\,\mathrm{eV} (M1); in the same way 414.4\,\mathrm{nm} gives 3.00\,\mathrm{eV} and 621.6\,\mathrm{nm} gives 2.00\,\mathrm{eV} (A1). (b) With three levels the two small gaps must add up to the large one: 2.0 + 3.0 = 5.0\,\mathrm{eV} (A1). (c) Emission tells us the sizes of the two steps but not their order: the middle level could be 2.0\,\mathrm{eV} or 3.0\,\mathrm{eV} above the lowest (A1). (d) A cool gas absorbs only from the lowest level, so the two dark lines are the jumps from -7.4\,\mathrm{eV} (M1). 621.6\,\mathrm{nm} (2.0\,\mathrm{eV}): middle level = -7.4 + 2.0 = -5.4\,\mathrm{eV} (A1). 248.6\,\mathrm{nm} (5.0\,\mathrm{eV}): top level = -7.4 + 5.0 = -2.4\,\mathrm{eV} (A1).

Final answer

(a) E = hc/\lambda gives 5.00, 3.00 and 2.00\,\mathrm{eV}. (b) 2.0 + 3.0 = 5.0: two steps make the full gap. (c) The middle level could be 2.0 or 3.0\,\mathrm{eV} above the lowest. (d) Middle -5.4\,\mathrm{eV}; top -2.4\,\mathrm{eV}.

Question A2

Type A2 · Type N3 · what scattering shows + N4 · P2[6 marks]
Before the scattering experiment, many physicists pictured an atom as a sphere of positive charge about 10^{-10}\,\mathrm{m} across, with electrons embedded in it.
(a) Predict what this model implies for the deflection of alpha particles that pass through a thin gold foil. [2]
(b) Explain which observation of the Geiger–Marsden–Rutherford experiment showed that this model is wrong. [2]
(c) The gold foil is replaced by an aluminium foil (Z = 13) with the same number of atoms per unit area. Suggest how the fraction of alpha particles deflected through large angles changes. Give a reason. [2]
Show solutionHide solution
(a) With the positive charge spread over a sphere 10^{-10}\,\mathrm{m} across, the electric field anywhere in or near the atom is weak (M1), so every alpha particle passes through with at most a small deflection (A1). (b) A small fraction were deflected through very large angles, some through more than 90^\circ (M1). Reversing a fast alpha particle needs a very strong repulsion, which requires the positive charge to be concentrated in a region far smaller than the atom (A1). (c) The fraction decreases (M1). The force \propto Z at a given distance, so an alpha particle must pass much closer to an aluminium nucleus to be turned through a large angle, and fewer alpha particles pass that close (A1).

Final answer

(a) Charge spread over the whole atom gives only weak forces: every alpha particle is deflected through a small angle. (b) A few alpha particles were turned back through more than 90^\circ. (c) It falls: the smaller nuclear charge repels less strongly at any given distance.

Question A3

Type A3 · Type H6 · state from angular momentum + H2, S3, S5 · HL · P2[8 marks]
In a hydrogen atom, the angular momentum of the electron is 4.22\times10^{-34}\,\mathrm{J\,s}.
(a) Show that the Planck constant has the same unit as angular momentum. [1]
(b) Determine the quantum number n of this state and the energy of the electron in eV. [2]
(c) The atom returns to the ground state. State the number of different photon frequencies that are possible. [1]
(d) Calculate the highest of these frequencies. [2]
(e) Identify the transitions that give visible light and calculate their wavelengths. [2]
Show solutionHide solution
(a) [h] = \mathrm{J\,s} = \mathrm{kg\,m^2\,s^{-1}} and [mvr] = \mathrm{kg\times m\,s^{-1}\times m} = \mathrm{kg\,m^2\,s^{-1}} (A1). (b) n = 2\pi L/h = 2\pi\times4.22\times10^{-34}/6.63\times10^{-34} = 4.00, so n = 4 (A1); E_4 = -13.6/16 = -0.85\,\mathrm{eV} (A1). (c) Levels n = 1 to 4 give 4\times3/2 = 6 frequencies (A1). (d) Largest gap 4\to1: 13.6(1 - \tfrac1{16}) = 12.75\,\mathrm{eV} = 2.04\times10^{-18}\,\mathrm{J} (M1); f = 2.04\times10^{-18}/6.63\times10^{-34} = 3.08\times10^{15}\,\mathrm{Hz} (A1). (e) Visible lines end on n = 2 (M1): 4\to2, 2.55\,\mathrm{eV}, \lambda = 488\,\mathrm{nm}; 3\to2, 1.89\,\mathrm{eV}, \lambda = 658\,\mathrm{nm}. Jumps to n = 1 are ultraviolet and 4\to3 (1880\,\mathrm{nm}) is infrared (A1).

Final answer

(a) J s = kg m^2 s^{-1} = (kg m s^{-1})(m). (b) n = 4; -0.85\,\mathrm{eV}. (c) 6. (d) 3.08\times10^{15}\,\mathrm{Hz}. (e) 4\to2: 488\,\mathrm{nm}; 3\to2: 658\,\mathrm{nm}.

Question A4

Type A4 · Type R5 · high-energy deviations + R4, R1 · HL · P2[7 marks]
Alpha particles of adjustable energy are fired at a target of aluminium nuclei, ^{27}_{13}\mathrm{Al}. A detector at a fixed angle counts the scattered alpha particles. Up to an energy of 8.0\,\mathrm{MeV} the count agrees with the Rutherford prediction; above 8.0\,\mathrm{MeV} it falls below the prediction.
(a) State the assumption about the force on the alpha particle that the Rutherford prediction uses. [1]
(b) Explain why the count departs from the prediction only above a certain energy. [2]
(c) Estimate the distance of closest approach for a head-on alpha particle of energy 8.0\,\mathrm{MeV}. [2]
(d) Compare your answer to (c) with R_0A^{1/3} for aluminium. Suggest one reason why the two values differ. [2]
Show solutionHide solution
(a) The only force is the electric (Coulomb) repulsion between the alpha particle and the nucleus, both treated as point charges (A1). (b) A more energetic alpha particle gets closer before it turns back (M1). Above about 8.0\,\mathrm{MeV} it comes within the short range of the strong nuclear force, which the Rutherford model leaves out, so the scattering changes (A1). (c) d = k(2e)(13e)/E_K = 8.99\times10^{9}\times26\times(1.60\times10^{-19})^2/(8.0\times1.60\times10^{-13}) (M1) = 4.7\times10^{-15}\,\mathrm{m} (A1). (d) R = 1.20\times10^{-15}\times27^{1/3} = 3.6\times10^{-15}\,\mathrm{m}, about three quarters of d (A1). The alpha particle is not a point: it has a radius of its own (about 1.9\times10^{-15}\,\mathrm{m}), and the strong force reaches a little beyond each surface, so the onset comes before the centres are R apart (A1).

Final answer

(a) Only the electric repulsion between two point-like charges acts. (b) Faster alpha particles get closer; above 8.0\,\mathrm{MeV} they reach the range of the strong force. (c) 4.7\times10^{-15}\,\mathrm{m}. (d) R = 3.6\times10^{-15}\,\mathrm{m}, a little smaller; the alpha particle has its own radius.

Question A5

Type A5 · Type R3 · volume against A gradient + R2 · HL · P2[6 marks]
Measured radii of four nuclei are shown.
\begin{array}{lrrrr}\text{A} & 16 & 64 & 125 & 216\\ \text{R}\,/\,\mathrm{fm} & 3.07 & 4.88 & 6.10 & 7.32\end{array}
A student plots nuclear volume V against A.
(a) Explain why R = R_0A^{1/3} predicts a straight line through the origin. [1]
(b) Calculate V for A = 216. [1]
(c) The gradient of the line is 7.61\times10^{-45}\,\mathrm{m^3}. Determine R_0. [2]
(d) Determine the density of nuclear matter. Take the mass of a nucleon as 1.67\times10^{-27}\,\mathrm{kg}. [2]
Show solutionHide solution
(a) Cubing the radius law gives V = \tfrac43\pi R^3 = \tfrac43\pi R_0^3A, a constant times A with no constant term (A1). (b) V = \tfrac43\pi(7.32\times10^{-15})^3 = 1.64\times10^{-42}\,\mathrm{m^3} (A1). (c) Gradient = \tfrac43\pi R_0^3, the volume per nucleon (M1); R_0 = (3\times7.61\times10^{-45}/4\pi)^{1/3} = 1.22\times10^{-15}\,\mathrm{m} (A1). (d) Mass per nucleon divided by volume per nucleon (M1): \rho = 1.67\times10^{-27}/7.61\times10^{-45} = 2.19\times10^{17}\,\mathrm{kg\,m^{-3}} (A1).

Final answer

(a) V = \tfrac43\pi R_0^3A: V\propto A. (b) 1.64\times10^{-42}\,\mathrm{m^3}. (c) 1.22\times10^{-15}\,\mathrm{m}. (d) 2.19\times10^{17}\,\mathrm{kg\,m^{-3}}.

Connected questions

Question X1

Type X1 · Type S1 · what line spectra show + S5 · P2 · E.1 + C.5 + B.1[8 marks]
The spectrum of a star shows a continuous background crossed by dark lines. One dark line is caused by hydrogen; in the laboratory this line is at 486.1\,\mathrm{nm}, but in the star's spectrum it is at 486.9\,\mathrm{nm}. The continuous background is most intense at 414\,\mathrm{nm}.
(a) Explain why the star's spectrum contains dark lines. [2]
(b) Find the photon energy of the laboratory line, giving your answer in eV. [2]
(c) Determine the speed of the star along the line of sight, and state whether it is moving towards or away from Earth. [2]
(d) Estimate the surface temperature of the star. [2]
Show solutionHide solution
(a) Light from the hot surface passes through cooler gas in the star's atmosphere, whose atoms absorb only photons with energies equal to their level gaps (M1); the absorbed energy is re-emitted in all directions, so those wavelengths are weak in the light that reaches us (A1). (b) E.1: E = hc/\lambda = 1.989\times10^{-25}/486.1\times10^{-9} = 4.09\times10^{-19}\,\mathrm{J} (M1) = 2.56\,\mathrm{eV} (A1). (c) C.5: v = c\,\Delta\lambda/\lambda = 3.00\times10^{8}\times0.8/486.1 = 4.9\times10^{5}\,\mathrm{m\,s^{-1}} (A1); the wavelength is longer (redshift), so the star is moving away (A1). (d) B.1: T = 2.9\times10^{-3}/\lambda_{\max} = 2.9\times10^{-3}/414\times10^{-9} (M1) = 7.0\times10^{3}\,\mathrm{K} (A1).

Final answer

(a) Cooler gas in the star's outer layers absorbs photons whose energies match its level gaps and re-emits them in all directions. (b) 2.56\,\mathrm{eV}. (c) 4.9\times10^{5}\,\mathrm{m\,s^{-1}}, away. (d) 7.0\times10^{3}\,\mathrm{K}.

Question X2

Type X2 · Type S5 · photon energy, eV and region + S1 · P2 · E.1 + B.5[7 marks]
A low-pressure gas lamp is connected to a 230\,\mathrm{V} supply and takes a current of 0.35\,\mathrm{A}. Collisions with the electrons of the current excite the gas atoms. All the visible light comes from one transition, between levels at -3.03\,\mathrm{eV} and -5.13\,\mathrm{eV}, and 25\% of the electrical power leaves the lamp as this light.
(a) Calculate the wavelength of the light. [2]
(b) Calculate the electrical power supplied to the lamp. [1]
(c) Determine the number of photons of this light emitted per second. [2]
(d) The light is viewed through a spectroscope. Explain why a single line, not a continuous band, is seen. [2]
Show solutionHide solution
(a) E.1: gap = -3.03 - (-5.13) = 2.10\,\mathrm{eV} = 3.36\times10^{-19}\,\mathrm{J} (M1); \lambda = hc/E = 1.989\times10^{-25}/3.36\times10^{-19} = 592\,\mathrm{nm} (A1). (b) B.5: P = IV = 0.35\times230 = 80.5\,\mathrm{W} (A1). (c) Light power = 0.25\times80.5 = 20.1\,\mathrm{W} (M1); photons per second = 20.1/3.36\times10^{-19} = 6.0\times10^{19}\,\mathrm{s^{-1}} (A1). (d) The atom's energy levels are discrete, so every photon from this transition carries the same energy (M1), and E = hc/\lambda then gives one wavelength, which appears as one bright line (A1).

Final answer

(a) 592\,\mathrm{nm}. (b) 80.5\,\mathrm{W}. (c) 6.0\times10^{19}\,\mathrm{s^{-1}}. (d) The levels are discrete, so every photon from this transition has the same energy and wavelength.

Question X3

Type X3 · Type R4 · closest approach + N1 · HL · P2 · E.1 + E.3 + D.2 + A.3[8 marks]
Polonium-210, ^{210}_{84}\mathrm{Po}, decays by alpha emission to an isotope of lead (Pb). The alpha particles have kinetic energy 5.30\,\mathrm{MeV}; the mass of an alpha particle is 6.64\times10^{-27}\,\mathrm{kg}.
(a) Write the nuclear equation for the decay. [2]
(b) Calculate the speed of the alpha particles. [2]
(c) The alpha particles are directed at a thin gold foil (Z = 79). Determine the distance of closest approach in a head-on collision. [3]
(d) State why the apparatus must be evacuated. [1]
Show solutionHide solution
(a) E.3: the alpha particle is ^{4}_{2}\alpha (A1); lead keeps A = 210 - 4 = 206 and Z = 84 - 2 = 82: ^{210}_{84}\mathrm{Po}\to{}^{206}_{82}\mathrm{Pb} + {}^{4}_{2}\alpha (A1). (b) A.3: E_K = 5.30\times1.60\times10^{-13} = 8.48\times10^{-13}\,\mathrm{J} (M1); v = \sqrt{2E_K/m} = \sqrt{2\times8.48\times10^{-13}/6.64\times10^{-27}} = 1.60\times10^{7}\,\mathrm{m\,s^{-1}} (A1). (c) D.2 and E.1: E_K = k(2e)(79e)/d (M1); d = 8.99\times10^{9}\times158\times(1.60\times10^{-19})^2/8.48\times10^{-13} (A1) = 4.29\times10^{-14}\,\mathrm{m} (A1). (d) Alpha particles lose their energy in collisions with air molecules within a few centimetres, so without a vacuum they would not reach the foil with a known energy (A1).

Final answer

(a) ^{210}_{84}\mathrm{Po}\to{}^{206}_{82}\mathrm{Pb} + {}^{4}_{2}\alpha. (b) 1.60\times10^{7}\,\mathrm{m\,s^{-1}}. (c) 4.29\times10^{-14}\,\mathrm{m}. (d) Air molecules would slow and scatter the alpha particles within a few centimetres.

Question X4

Type X4 · Type H2 · Bohr energy gaps + S5 · HL · P2 · E.1 + E.2[8 marks]
Ultraviolet light from hydrogen atoms making the transition n = 2\to n = 1 falls on a metal surface of work function 4.3\,\mathrm{eV}.
(a) Show that the photon energy is 10.2\,\mathrm{eV}. [1]
(b) Calculate the wavelength of the light. [2]
(c) Determine, in J, the largest kinetic energy that a photoelectron leaving the metal can have. [2]
(d) Calculate the de Broglie wavelength of the fastest electrons. [2]
(e) Compare this wavelength with the size of an atom. [1]
Show solutionHide solution
(a) E.1: E_2 - E_1 = -13.6/4 - (-13.6) = 10.2\,\mathrm{eV} (A1). (b) E = 10.2\times1.60\times10^{-19} = 1.63\times10^{-18}\,\mathrm{J} (M1); \lambda = hc/E = 1.989\times10^{-25}/1.63\times10^{-18} = 1.22\times10^{-7}\,\mathrm{m} (A1). (c) E.2: E_{\max} = hf - \Phi = 10.2 - 4.3 = 5.9\,\mathrm{eV} (M1) = 9.4\times10^{-19}\,\mathrm{J} (A1). (d) p = \sqrt{2mE_{\max}} = \sqrt{2\times9.11\times10^{-31}\times9.44\times10^{-19}} = 1.31\times10^{-24}\,\mathrm{kg\,m\,s^{-1}} (M1); \lambda = h/p = 5.1\times10^{-10}\,\mathrm{m} (A1). (e) An atom is about 10^{-10}\,\mathrm{m} across, so the wavelength is about five atomic diameters: the same order of magnitude, which is why such electrons diffract from crystals (A1).

Final answer

(a) 13.6(1 - \tfrac14) = 10.2\,\mathrm{eV}. (b) 1.22\times10^{-7}\,\mathrm{m}. (c) 9.4\times10^{-19}\,\mathrm{J}. (d) 5.1\times10^{-10}\,\mathrm{m}. (e) About five atomic diameters: the same order of magnitude.

From the book

Photon Physics: Study Guide for the IB Diploma (SL & HL)

Structure of the atom from the core ideas to full exam questions, with question types, worked examples and graded practice.

About the book