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Cosmic rays are high-energy particles that come from space - AQA - A-Level Physics - Question 1 - 2021 - Paper 1

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Cosmic rays are high-energy particles that come from space. Most of these particles are protons. There are other particles in cosmic rays, including atomic nuclei. ... show full transcript

Worked Solution & Example Answer:Cosmic rays are high-energy particles that come from space - AQA - A-Level Physics - Question 1 - 2021 - Paper 1

Step 1

Determine the number of neutrons in nucleus X.

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Answer

To determine the number of neutrons, we first need the total charge from the nucleus. The specific charge (C/kg) and the mass (kg) of nucleus X provide the total charge:

Charge = Specific Charge × Mass = 4.39 × 10^7 C kg^-1 × 8.02 × 10^{-26} kg = 3.52 × 10^{-18} C.

Using the fact that the charge of a proton is approximately 1.6 × 10^{-19} C, we can find the number of protons:

Number of protons = Total Charge / Charge of a Proton = 3.52 × 10^{-18} C / 1.6 × 10^{-19} C ≈ 22 protons.

Now, we can use the mass number (A) to find the number of neutrons (N). Assuming the nucleus X has an atomic mass around 8.02 × 10^{-26} kg (which correlates closely with standard nucleon mass), we find:

Number of Neutrons = Mass Number - Number of Protons.

Assuming the mass number is approximately 22 (from the number of protons), Number of Neutrons = 22 - 22 = 0.

Therefore, the number of neutrons is approximately 0.

Step 2

Calculate the speed of X.

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Answer

To find the speed of nucleus X, we use the kinetic energy (KE) formula:

KE=12mv2KE = \frac{1}{2} mv^2

We can rearrange this to solve for speed (v):

v=2×KEmv = \sqrt{\frac{2 \times KE}{m}}

Substituting the values:

KE=215 MeV=215×1.6×1013 J3.44×1011 JKE = 215 \text{ MeV} = 215 \times 1.6 \times 10^{-13} \text{ J} \approx 3.44 \times 10^{-11} \text{ J}

v=2×3.44×1011 J8.02×1026 kg8.59×10142.93×107 m/sv = \sqrt{\frac{2 \times 3.44 \times 10^{-11} \text{ J}}{8.02 \times 10^{-26} \text{ kg}}} \approx \sqrt{8.59 \times 10^{14}} \approx 2.93 \times 10^7 \text{ m/s}

Step 3

Show how the conservation laws apply to this decay.

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Answer

In the decay of the pion (π-) which produces a positron (e+) and an electron neutrino (νe), we need to check the conservation of charge and lepton number:

  • The initial charge of the pion is -1 (as π- has a charge of -1).

    • After decay: Positron: +1, Electron neutrino: 0, Total charge: +1 + 0 = 0.
    • Thus, charge is conserved.
  • For lepton number: The initial lepton number is 1 (the pion is a meson and does not contribute):

    • After decay: Lepton number from the positron: +1 and from the neutrino: +1.
    • Therefore total lepton number = 1 = initial lepton number, hence conserved.

Step 4

Explain how strangeness applies in this decay.

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Answer

In this decay of the K+ into an anti-muon (μ-) and a muon neutrino (νμ), we can analyze strangeness:

  • Strangeness is a quantum number that represents the presence of strange quarks. K mesons contain strange quarks.
  • The K+ has a strangeness of +1 because it contains a strange quark.
  • The decay products (anti-muon and muon neutrino) do not contain any strange quarks, leading to a strangeness of 0 in the final state.
  • Since the strangeness must be conserved in weak decays, and because we started with a strangeness of +1, the decay indicates a change in strangeness is allowed, which is unique to weak interactions.

Step 5

Write an equation for a K+ decay that involves only hadrons.

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Answer

An example equation for a K+ decay that involves only hadrons is:

K+π++π0K^+ \rightarrow \pi^+ + \pi^0

In this process, a kaon decays to produce a positive pion and a neutral pion, both of which are hadrons.

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