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12.2 – Nuclear physics
Description
Nature of science:
Theoretical advances and inspiration: Progress in atomic, nuclear and particle physics often came from theoretical advances and strokes of inspiration.
Advances in instrumentation: New ways of detecting subatomic particles due to advances in electronic technology were also crucial.
Modern computing power: Finally, the analysis of the data gathered in modern particle detectors in particle accelerator experiments would be impossible without modern computing power. (1.8)
Understandings:
- Rutherford scattering and nuclear radius
- Nuclear energy levels
- The neutrino
- The law of radioactive decay and the decay constant
Applications and skills:
- Describing a scattering experiment including location of minimum intensity for the diffracted particles based on their de Broglie wavelength
- Explaining deviations from Rutherford scattering in high energy experiments
- Describing experimental evidence for nuclear energy levels
- Solving problems involving the radioactive decay law for arbitrary time intervals
- Explaining the methods for measuring short and long half-lives
Guidance:
- Students should be aware that nuclear densities are approximately the same for all nuclei and that the only macroscopic objects with the same density as nuclei are neutron stars
- The small angle approximation is usually not appropriate to use to determine the location of the minimum intensity
Data booklet reference:
Theory of knowledge:
- Much of the knowledge about subatomic particles is based on the models one uses to interpret the data from experiments. How can we be sure that we are discovering an “independent truth” not influenced by our models? Is there such a thing as a single truth?
Utilization:
- Knowledge of radioactivity, radioactive substances and the radioactive decay law are crucial in modern nuclear medicine (see Physics option sub-topic C.4)
Aims:
- Aim 2: detection of the neutrino demonstrates the continuing growing body of knowledge scientists are gathering in this area of study
Directly related questions
-
20N.2.HL.TZ0.10c:
Experiments with many nuclides suggest that the radius of a nucleus is proportional to , where is the number of nucleons in the nucleus. Show that the density of a nucleus remains approximately the same for all nuclei.
-
20N.2.HL.TZ0.10c:
Experiments with many nuclides suggest that the radius of a nucleus is proportional to , where is the number of nucleons in the nucleus. Show that the density of a nucleus remains approximately the same for all nuclei.
-
20N.2.HL.TZ0.c:
Experiments with many nuclides suggest that the radius of a nucleus is proportional to , where is the number of nucleons in the nucleus. Show that the density of a nucleus remains approximately the same for all nuclei.
-
20N.2.HL.TZ0.10b(ii):
The accepted value of the diameter of the carbon-12 nucleus is . Estimate the angle at which the minimum of the intensity is formed.
-
20N.2.HL.TZ0.10b(ii):
The accepted value of the diameter of the carbon-12 nucleus is . Estimate the angle at which the minimum of the intensity is formed.
-
20N.2.HL.TZ0.b(ii):
The accepted value of the diameter of the carbon-12 nucleus is . Estimate the angle at which the minimum of the intensity is formed.
- 17N.2.HL.TZ0.3b.i: Outline how these experiments are carried out.
- 17N.2.HL.TZ0.3b.i: Outline how these experiments are carried out.
- 17N.2.HL.TZ0.b.i: Outline how these experiments are carried out.
- 17N.2.HL.TZ0.3d.iii: Draw a line on the graph, to show the variation of nuclear radius with nucleon number.
- 17N.2.HL.TZ0.3d.iii: Draw a line on the graph, to show the variation of nuclear radius with nucleon number.
- 17N.2.HL.TZ0.d.iii: Draw a line on the graph, to show the variation of nuclear radius with nucleon number.
-
17N.2.HL.TZ0.3d.ii:
Plot the position of magnesium-24 on the graph.
-
17N.2.HL.TZ0.3d.ii:
Plot the position of magnesium-24 on the graph.
-
17N.2.HL.TZ0.d.ii:
Plot the position of magnesium-24 on the graph.
- 21M.2.HL.TZ1.7c: The half-life of uranium-238 is about 4.5 × 109 years. The half-life of thallium-206 is about 4.2...
- 21M.2.HL.TZ1.7c: The half-life of uranium-238 is about 4.5 × 109 years. The half-life of thallium-206 is about 4.2...
- 21M.2.HL.TZ1.c: The half-life of uranium-238 is about 4.5 × 109 years. The half-life of thallium-206 is about 4.2...
-
21M.1.HL.TZ1.39:
The graphs show the variation with time of the activity and the number of remaining nuclei for a sample of a radioactive nuclide.
What is the decay constant of the nuclide?
A.
B.
C.
D.
-
21M.1.HL.TZ1.39:
The graphs show the variation with time of the activity and the number of remaining nuclei for a sample of a radioactive nuclide.
What is the decay constant of the nuclide?
A.
B.
C.
D.
- 21M.1.HL.TZ1.40: What was a reason to postulate the existence of neutrinos? A. Nuclear energy levels had a...
- 21M.1.HL.TZ1.40: What was a reason to postulate the existence of neutrinos? A. Nuclear energy levels had a...
-
18M.2.HL.TZ2.9d.i:
Explain what may be deduced about the energy of the electron in the β– decay.
-
18M.2.HL.TZ2.9d.i:
Explain what may be deduced about the energy of the electron in the β– decay.
-
18M.2.HL.TZ2.d.i:
Explain what may be deduced about the energy of the electron in the β– decay.
- 21N.1.HL.TZ0.40: The size of a nucleus can be estimated from electron diffraction experiments. What is the order...
- 21N.1.HL.TZ0.40: The size of a nucleus can be estimated from electron diffraction experiments. What is the order...
-
21N.1.HL.TZ0.39:
Some of the nuclear energy levels of oxygen-14 (14O) and nitrogen-14 (14N) are shown.
A nucleus of 14O decays into a nucleus of 14N with the emission of a positron and a gamma ray. What is the maximum energy of the positron and the energy of the gamma ray?
-
21N.1.HL.TZ0.39:
Some of the nuclear energy levels of oxygen-14 (14O) and nitrogen-14 (14N) are shown.
A nucleus of 14O decays into a nucleus of 14N with the emission of a positron and a gamma ray. What is the maximum energy of the positron and the energy of the gamma ray?
-
18N.1.HL.TZ0.39:
The graph shows the variation of the natural log of activity, ln (activity), against time for a radioactive nuclide.
What is the decay constant, in days–1, of the radioactive nuclide?
A.
B.
C. 3
D. 6
-
18N.1.HL.TZ0.39:
The graph shows the variation of the natural log of activity, ln (activity), against time for a radioactive nuclide.
What is the decay constant, in days–1, of the radioactive nuclide?
A.
B.
C. 3
D. 6
- 18N.2.HL.TZ0.6a.i: State how the density of a nucleus varies with the number of nucleons in the nucleus.
- 18N.2.HL.TZ0.6a.i: State how the density of a nucleus varies with the number of nucleons in the nucleus.
- 18N.2.HL.TZ0.a.i: State how the density of a nucleus varies with the number of nucleons in the nucleus.
-
18N.2.HL.TZ0.6d.ii:
In a fresh pure sample of the activity of the sample is 24 Bq. After one week the activity has become 17 Bq. Calculate, in s–1, the decay constant of .
-
18N.2.HL.TZ0.6d.ii:
In a fresh pure sample of the activity of the sample is 24 Bq. After one week the activity has become 17 Bq. Calculate, in s–1, the decay constant of .
-
18N.2.HL.TZ0.d.ii:
In a fresh pure sample of the activity of the sample is 24 Bq. After one week the activity has become 17 Bq. Calculate, in s–1, the decay constant of .
-
18N.2.HL.TZ0.6a.ii:
Show that the nuclear radius of phosphorus-31 () is about 4 fm.
-
18N.2.HL.TZ0.6a.ii:
Show that the nuclear radius of phosphorus-31 () is about 4 fm.
-
18N.2.HL.TZ0.a.ii:
Show that the nuclear radius of phosphorus-31 () is about 4 fm.
-
22M.1.HL.TZ2.38:
Samples of two radioactive nuclides X and Y are held in a container. The number of particles of X is half the number of particles of Y. The half-life of X is twice the half-life of Y.
What is the initial value of ?
A.
B.
C.
D.
-
22M.1.HL.TZ2.38:
Samples of two radioactive nuclides X and Y are held in a container. The number of particles of X is half the number of particles of Y. The half-life of X is twice the half-life of Y.
What is the initial value of ?
A.
B.
C.
D.
-
19M.2.HL.TZ1.2a.ii:
Estimate, using the result from (a)(i), the nuclear radius of thorium-232 .
-
19M.2.HL.TZ1.2a.ii:
Estimate, using the result from (a)(i), the nuclear radius of thorium-232 .
-
19M.2.HL.TZ1.a.ii:
Estimate, using the result from (a)(i), the nuclear radius of thorium-232 .
-
19M.2.HL.TZ1.2a.iii:
Suggest one reason why a beam of electrons is better for investigating the size of a nucleus than a beam of alpha particles of the same energy.
-
19M.2.HL.TZ1.2a.iii:
Suggest one reason why a beam of electrons is better for investigating the size of a nucleus than a beam of alpha particles of the same energy.
-
19M.2.HL.TZ1.a.iii:
Suggest one reason why a beam of electrons is better for investigating the size of a nucleus than a beam of alpha particles of the same energy.
- 19M.2.HL.TZ1.2a.iv: Outline why deviations from Rutherford scattering are observed when high-energy alpha particles...
- 19M.2.HL.TZ1.2a.iv: Outline why deviations from Rutherford scattering are observed when high-energy alpha particles...
- 19M.2.HL.TZ1.a.iv: Outline why deviations from Rutherford scattering are observed when high-energy alpha particles...
-
22N.1.HL.TZ0.40:
The nucleus of the isotope hydrogen-2 has a radius R and a density .
What are the approximate radius and density of a nucleus of oxygen-16?
-
22N.1.HL.TZ0.40:
The nucleus of the isotope hydrogen-2 has a radius R and a density .
What are the approximate radius and density of a nucleus of oxygen-16?
- 22N.2.HL.TZ0.6b.iii: In the decay of polonium−210, alpha emissions can be accompanied by the emissions of gamma...
- 22N.2.HL.TZ0.6b.iii: In the decay of polonium−210, alpha emissions can be accompanied by the emissions of gamma...
- 22N.2.HL.TZ0.b.iii: In the decay of polonium−210, alpha emissions can be accompanied by the emissions of gamma...
-
22N.2.HL.TZ0.6c:
A sample contains 5.0 g of pure polonium-210. The decay constant of polonium-210 is 5.8 × 10−8 s−1. Lead-206 is stable.
Calculate the mass of lead-206 present in the sample after one year.
-
22N.2.HL.TZ0.6c:
A sample contains 5.0 g of pure polonium-210. The decay constant of polonium-210 is 5.8 × 10−8 s−1. Lead-206 is stable.
Calculate the mass of lead-206 present in the sample after one year.
-
22N.2.HL.TZ0.c:
A sample contains 5.0 g of pure polonium-210. The decay constant of polonium-210 is 5.8 × 10−8 s−1. Lead-206 is stable.
Calculate the mass of lead-206 present in the sample after one year.
-
17N.2.HL.TZ0.3b.ii:
Outline why the particles must be accelerated to high energies in scattering experiments.
-
17N.2.HL.TZ0.3b.ii:
Outline why the particles must be accelerated to high energies in scattering experiments.
-
17N.2.HL.TZ0.b.ii:
Outline why the particles must be accelerated to high energies in scattering experiments.
-
17N.2.HL.TZ0.3d.i:
Determine the radius of the magnesium-24 nucleus.
- 18M.1.HL.TZ1.39: A particle of fixed energy is close to a potential barrier. Which changes to the width of the...
- 18M.1.HL.TZ1.39: A particle of fixed energy is close to a potential barrier. Which changes to the width of the...
- 18M.1.HL.TZ1.40: Alpha particles with energy E are directed at nuclei with atomic number Z. Small deviations from...
- 18M.1.HL.TZ1.40: Alpha particles with energy E are directed at nuclei with atomic number Z. Small deviations from...
-
18M.2.HL.TZ1.6b.iii:
Beryllium-10 is used to investigate ice samples from Antarctica. A sample of ice initially contains 7.6 × 1011 atoms of beryllium-10. The present activity of the sample is 8.0 × 10−3 Bq.
Determine, in years, the age of the sample.
-
18M.2.HL.TZ1.6b.iii:
Beryllium-10 is used to investigate ice samples from Antarctica. A sample of ice initially contains 7.6 × 1011 atoms of beryllium-10. The present activity of the sample is 8.0 × 10−3 Bq.
Determine, in years, the age of the sample.
-
18M.2.HL.TZ1.b.iii:
Beryllium-10 is used to investigate ice samples from Antarctica. A sample of ice initially contains 7.6 × 1011 atoms of beryllium-10. The present activity of the sample is 8.0 × 10−3 Bq.
Determine, in years, the age of the sample.
- 18M.1.HL.TZ2.39: An electron of initial energy E tunnels through a potential barrier. What is the energy of...
- 18M.1.HL.TZ2.39: An electron of initial energy E tunnels through a potential barrier. What is the energy of...
-
18M.1.HL.TZ2.40:
Two samples X and Y of different radioactive isotopes have the same initial activity. Sample X has twice the number of atoms as sample Y. The half-life of X is T. What is the half-life of Y?
A. 2T
B. T
C.
D.
-
18M.1.HL.TZ2.40:
Two samples X and Y of different radioactive isotopes have the same initial activity. Sample X has twice the number of atoms as sample Y. The half-life of X is T. What is the half-life of Y?
A. 2T
B. T
C.
D.
-
18M.2.HL.TZ2.9d.iii:
Calculate the wavelength of the gamma ray photon in (d)(ii).
-
18M.2.HL.TZ2.9d.iii:
Calculate the wavelength of the gamma ray photon in (d)(ii).
-
18M.2.HL.TZ2.d.iii:
Calculate the wavelength of the gamma ray photon in (d)(ii).
- 18N.1.HL.TZ0.40: A radioactive nuclide is known to have a very long half-life. Three quantities known for a pure...
- 18N.1.HL.TZ0.40: A radioactive nuclide is known to have a very long half-life. Three quantities known for a pure...
-
18N.2.HL.TZ0.6c:
undergoes beta-minus (β–) decay. Explain why the energy gained by the emitted beta particles in this decay is not the same for every beta particle.
-
18N.2.HL.TZ0.6c:
undergoes beta-minus (β–) decay. Explain why the energy gained by the emitted beta particles in this decay is not the same for every beta particle.
-
18N.2.HL.TZ0.c:
undergoes beta-minus (β–) decay. Explain why the energy gained by the emitted beta particles in this decay is not the same for every beta particle.
- 18N.2.HL.TZ0.6d.i: State what is meant by decay constant.
- 18N.2.HL.TZ0.6d.i: State what is meant by decay constant.
- 18N.2.HL.TZ0.d.i: State what is meant by decay constant.
-
19M.2.HL.TZ1.2a.i:
Use the graph to show that the nuclear radius of silicon-30 is about 4 fm.
-
19M.2.HL.TZ1.2a.i:
Use the graph to show that the nuclear radius of silicon-30 is about 4 fm.
-
19M.2.HL.TZ1.a.i:
Use the graph to show that the nuclear radius of silicon-30 is about 4 fm.
- 19M.1.HL.TZ2.40: Photons of discrete energy are emitted during gamma decay. This is evidence for A. atomic energy...
- 19M.1.HL.TZ2.40: Photons of discrete energy are emitted during gamma decay. This is evidence for A. atomic energy...
-
19M.1.HL.TZ1.39:
The half-life of a radioactive nuclide is 8.0 s. The initial activity of a pure sample of the nuclide is 10 000 Bq. What is the approximate activity of the sample after 4.0 s?
A. 2500 Bq
B. 5000 Bq
C. 7100 Bq
D. 7500 Bq
-
19M.1.HL.TZ1.39:
The half-life of a radioactive nuclide is 8.0 s. The initial activity of a pure sample of the nuclide is 10 000 Bq. What is the approximate activity of the sample after 4.0 s?
A. 2500 Bq
B. 5000 Bq
C. 7100 Bq
D. 7500 Bq
-
19N.1.HL.TZ0.40:
A pure sample of a radioactive nuclide contains N0 atoms at time t = 0. At time t, there are N atoms of the nuclide remaining in the sample. The half-life of the nuclide is .
What is the decay rate of this sample proportional to?
A. N
B. N0 – N
C. t
D.
-
19N.1.HL.TZ0.40:
A pure sample of a radioactive nuclide contains N0 atoms at time t = 0. At time t, there are N atoms of the nuclide remaining in the sample. The half-life of the nuclide is .
What is the decay rate of this sample proportional to?
A. N
B. N0 – N
C. t
D.
-
20N.1.HL.TZ0.38:
The diameter of a nucleus of a particular nuclide X is . What is the nucleon number of X?
A.
B.
C.
D.
-
20N.1.HL.TZ0.38:
The diameter of a nucleus of a particular nuclide X is . What is the nucleon number of X?
A.
B.
C.
D.
- 20N.1.HL.TZ0.40: The Rutherford-Geiger-Marsden experiment shows that A. alpha particles do not obey Coulomb’s...
- 20N.1.HL.TZ0.40: The Rutherford-Geiger-Marsden experiment shows that A. alpha particles do not obey Coulomb’s...
-
20N.2.HL.TZ0.10b(iii):
Outline why electrons with energy of approximately would be unsuitable for the investigation of nuclear radii.
-
20N.2.HL.TZ0.10b(iii):
Outline why electrons with energy of approximately would be unsuitable for the investigation of nuclear radii.
-
20N.2.HL.TZ0.b(iii):
Outline why electrons with energy of approximately would be unsuitable for the investigation of nuclear radii.
-
21M.2.HL.TZ2.4a.ii:
The unstable lead nuclide has a half-life of 15 × 106 years. A sample initially contains 2.0 μmol of the lead nuclide. Calculate the number of thallium nuclei being formed each second 30 × 106 years later.
-
21M.2.HL.TZ2.4a.ii:
The unstable lead nuclide has a half-life of 15 × 106 years. A sample initially contains 2.0 μmol of the lead nuclide. Calculate the number of thallium nuclei being formed each second 30 × 106 years later.
-
21M.2.HL.TZ2.a.ii:
The unstable lead nuclide has a half-life of 15 × 106 years. A sample initially contains 2.0 μmol of the lead nuclide. Calculate the number of thallium nuclei being formed each second 30 × 106 years later.
-
21M.1.HL.TZ2.38:
Element X has a nucleon number and a nuclear density . Element Y has a nucleon number of . What is an estimate of the nuclear density of element Y?
A.
B.
C.
D.
-
21M.1.HL.TZ2.38:
Element X has a nucleon number and a nuclear density . Element Y has a nucleon number of . What is an estimate of the nuclear density of element Y?
A.
B.
C.
D.
-
21N.2.HL.TZ0.4c.i:
Estimate the power, in kW, that is available from the plutonium at launch.
-
21N.2.HL.TZ0.4c.i:
Estimate the power, in kW, that is available from the plutonium at launch.
-
21N.2.HL.TZ0.c.i:
Estimate the power, in kW, that is available from the plutonium at launch.
-
21N.2.HL.TZ0.4c.ii:
The spacecraft will take 7.2 years (2.3 × 108 s) to reach a planet in the solar system. Estimate the power available to the spacecraft when it gets to the planet.
-
21N.2.HL.TZ0.4c.ii:
The spacecraft will take 7.2 years (2.3 × 108 s) to reach a planet in the solar system. Estimate the power available to the spacecraft when it gets to the planet.
-
21N.2.HL.TZ0.c.ii:
The spacecraft will take 7.2 years (2.3 × 108 s) to reach a planet in the solar system. Estimate the power available to the spacecraft when it gets to the planet.
-
22M.2.HL.TZ2.9b:
Estimate, using the result in (a)(iii), the volume of a tin-118 nucleus. State your answer to an appropriate number of significant figures.
-
22M.2.HL.TZ2.9b:
Estimate, using the result in (a)(iii), the volume of a tin-118 nucleus. State your answer to an appropriate number of significant figures.
-
22M.2.HL.TZ2.b:
Estimate, using the result in (a)(iii), the volume of a tin-118 nucleus. State your answer to an appropriate number of significant figures.
-
22M.1.HL.TZ1.40:
The decay constant, , of a radioactive sample can be defined as
A. the number of disintegrations in the radioactive sample.
B. the number of disintegrations per unit time in the radioactive sample.
C. the probability that a nucleus decays in the radioactive sample.
D. the probability that a nucleus decays per unit time in the radioactive sample.
-
22M.1.HL.TZ1.40:
The decay constant, , of a radioactive sample can be defined as
A. the number of disintegrations in the radioactive sample.
B. the number of disintegrations per unit time in the radioactive sample.
C. the probability that a nucleus decays in the radioactive sample.
D. the probability that a nucleus decays per unit time in the radioactive sample.
-
22M.2.HL.TZ1.9b.ii:
The half-life of potassium-40 is 1.3 × 109 years. Estimate the age of the rock sample.
-
22M.2.HL.TZ1.9b.ii:
The half-life of potassium-40 is 1.3 × 109 years. Estimate the age of the rock sample.
-
22M.2.HL.TZ1.b.ii:
The half-life of potassium-40 is 1.3 × 109 years. Estimate the age of the rock sample.
-
22M.2.HL.TZ1.9c:
Outline how the decay constant of potassium-40 was determined in the laboratory for a pure sample of the nuclide.
-
22M.2.HL.TZ1.9c:
Outline how the decay constant of potassium-40 was determined in the laboratory for a pure sample of the nuclide.
-
22M.2.HL.TZ1.c:
Outline how the decay constant of potassium-40 was determined in the laboratory for a pure sample of the nuclide.
- 22N.1.HL.TZ0.39: Which emission shows a continuous energy spectrum? A. Photons during energy transitions between...
- 22N.1.HL.TZ0.39: Which emission shows a continuous energy spectrum? A. Photons during energy transitions between...
-
23M.1.HL.TZ1.13:
A group of students perform an experiment to find the refractive index of a glass block. They measure various values of the angle of incidence i and angle of refraction r for a ray entering the glass from air. They plot a graph of the sin r against sin i.
They determine the gradient of the graph to be m.
Which of the following gives the critical angle of the glass?
A. sin−1(m)B. sin−1
C. m
D.
-
23M.1.SL.TZ1.16:
A group of students perform an experiment to find the refractive index of a glass block. They measure various values of the angle of incidence i and angle of refraction r for a ray entering the glass from air. They plot a graph of the sin r against sin i.
They determine the gradient of the graph to be m.
Which of the following gives the critical angle of the glass?
A. sin−1(m)B. sin−1
C. m
D.
-
23M.1.SL.TZ1.16:
A group of students perform an experiment to find the refractive index of a glass block. They measure various values of the angle of incidence i and angle of refraction r for a ray entering the glass from air. They plot a graph of the sin r against sin i.
They determine the gradient of the graph to be m.
Which of the following gives the critical angle of the glass?
A. sin−1(m)B. sin−1
C. m
D.
-
23M.1.HL.TZ1.13:
A group of students perform an experiment to find the refractive index of a glass block. They measure various values of the angle of incidence i and angle of refraction r for a ray entering the glass from air. They plot a graph of the sin r against sin i.
They determine the gradient of the graph to be m.
Which of the following gives the critical angle of the glass?
A. sin−1(m)B. sin−1
C. m
D.
-
23M.2.HL.TZ1.5a:
Identify with ticks [✓] in the table, the forces that can act on electrons and the forces that can act on quarks.
-
23M.2.HL.TZ1.5a:
Identify with ticks [✓] in the table, the forces that can act on electrons and the forces that can act on quarks.
-
23M.2.HL.TZ1.a:
Identify with ticks [✓] in the table, the forces that can act on electrons and the forces that can act on quarks.
- 23M.3.HL.TZ1.2a: State, for this experiment,
- 23M.3.SL.TZ1.2a: State, for this experiment,
- 23M.3.HL.TZ1.2a: State, for this experiment,
- 23M.3.HL.TZ1.a: State, for this experiment,
- 23M.3.SL.TZ1.2a: State, for this experiment,
- 23M.3.SL.TZ1.a: State, for this experiment,
- 23M.3.HL.TZ2.17a: State the main element that is undergoing nuclear fusion in star C.
- 23M.3.SL.TZ2.12a: State the main element that is undergoing nuclear fusion in star C.
- 23M.3.HL.TZ2.17a: State the main element that is undergoing nuclear fusion in star C.
- 23M.3.HL.TZ2.a: State the main element that is undergoing nuclear fusion in star C.
- 23M.3.SL.TZ2.12a: State the main element that is undergoing nuclear fusion in star C.
- 23M.3.SL.TZ2.a: State the main element that is undergoing nuclear fusion in star C.
-
23M.3.HL.TZ1.1a:
Deduce the unit of μ in terms of fundamental SI units.
-
23M.3.SL.TZ1.1a:
Deduce the unit of μ in terms of fundamental SI units.
-
23M.3.HL.TZ1.1a:
Deduce the unit of μ in terms of fundamental SI units.
-
23M.3.HL.TZ1.a:
Deduce the unit of μ in terms of fundamental SI units.
-
23M.3.SL.TZ1.1a:
Deduce the unit of μ in terms of fundamental SI units.
-
23M.3.SL.TZ1.a:
Deduce the unit of μ in terms of fundamental SI units.
-
23M.2.SL.TZ1.5a:
Identify with ticks [✓] in the table, the forces that can act on electrons and the forces that can act on quarks.
-
23M.2.SL.TZ1.5a:
Identify with ticks [✓] in the table, the forces that can act on electrons and the forces that can act on quarks.
-
23M.2.SL.TZ1.a:
Identify with ticks [✓] in the table, the forces that can act on electrons and the forces that can act on quarks.
- 23M.3.HL.TZ1.16a: The mass of star A is 52 M☉. Show that the luminosity of star A is about 106 L☉.
- 23M.3.SL.TZ1.11a: The mass of star A is 52 M☉. Show that the luminosity of star A is about 106 L☉.
- 23M.3.HL.TZ1.16a: The mass of star A is 52 M☉. Show that the luminosity of star A is about 106 L☉.
- 23M.3.HL.TZ1.a: The mass of star A is 52 M☉. Show that the luminosity of star A is about 106 L☉.
- 23M.3.SL.TZ1.11a: The mass of star A is 52 M☉. Show that the luminosity of star A is about 106 L☉.
- 23M.3.SL.TZ1.a: The mass of star A is 52 M☉. Show that the luminosity of star A is about 106 L☉.
- 23M.3.SL.TZ2.1a: State one variable that needs to be controlled during the investigation.
- 23M.3.HL.TZ2.1a: State one variable that needs to be controlled during the investigation.
- 23M.3.SL.TZ2.1a: State one variable that needs to be controlled during the investigation.
- 23M.3.HL.TZ2.1a: State one variable that needs to be controlled during the investigation.
- 23M.3.HL.TZ2.a: State one variable that needs to be controlled during the investigation.
- 23M.3.SL.TZ2.a: State one variable that needs to be controlled during the investigation.
- 23M.3.HL.TZ2.2a: State one other measurement that the student will need to make.
- 23M.3.SL.TZ2.2a: State one other measurement that the student will need to make.
- 23M.3.HL.TZ2.2a: State one other measurement that the student will need to make.
- 23M.3.HL.TZ2.a: State one other measurement that the student will need to make.
- 23M.3.SL.TZ2.2a: State one other measurement that the student will need to make.
- 23M.3.SL.TZ2.a: State one other measurement that the student will need to make.
- 23M.3.HL.TZ2.7a: Explain why the frequency of the photons detected at the ceiling is less than the frequency of...
- 23M.3.HL.TZ2.7a: Explain why the frequency of the photons detected at the ceiling is less than the frequency of...
- 23M.3.HL.TZ2.a: Explain why the frequency of the photons detected at the ceiling is less than the frequency of...
- 23M.3.HL.TZ2.16a: The Ghost of Jupiter is a nebula.
- 23M.3.SL.TZ2.11a: The Ghost of Jupiter is a nebula.
- 23M.3.HL.TZ2.16a: The Ghost of Jupiter is a nebula.
- 23M.3.HL.TZ2.a: The Ghost of Jupiter is a nebula.
- 23M.3.SL.TZ2.11a: The Ghost of Jupiter is a nebula.
- 23M.3.SL.TZ2.a: The Ghost of Jupiter is a nebula.