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Unit 4: Revolutions in modern physics

Quick questions on Mass-energy equivalence E=mc2E = mc^2 (QCE Physics Unit 4)

11short Q&A pairs drawn directly from our worked dot-point answer. For full context and worked exam questions, read the parent dot-point page.

What are standard particle rest energies?
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These values are used throughout particle and nuclear physics. The proton and neutron rest energies are nearly equal but the neutron is slightly heavier (its instability to beta decay is consistent with this).
What is fission example?
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235U+n141Ba+92Kr+3n^{235}\text{U} + \text{n} \to ^{141}\text{Ba} + ^{92}\text{Kr} + 3\text{n}. Mass deficit approximately 0.2 atomic mass units (amu). Energy released approximately 200 MeV per fission event.
What is fusion example?
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2H+3H4He+n^2\text{H} + ^3\text{H} \to ^4\text{He} + \text{n}. Mass deficit approximately 0.0188 amu. Energy released approximately 17.6 MeV per fusion event.
What is pair production?
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A high-energy photon (energy at least 2mec2=1.0222 m_e c^2 = 1.022 MeV) can convert into an electron-positron pair in the presence of a nucleus (which carries away momentum to conserve momentum). Total mass appears from total energy.
What is annihilation?
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An electron and a positron annihilate to two photons (back-to-back, each with energy 0.5110.511 MeV in the centre-of-mass frame). All rest mass is converted to electromagnetic energy. This is the basis of PET (positron emission tomography) medical imaging.
What is solar luminosity?
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The sun converts about 4×1094 \times 10^9 kg of mass to energy per second through hydrogen fusion. Total solar luminosity: 4×10264 \times 10^{26} W. The sun has about 2×10302 \times 10^{30} kg of mass and will continue fusing hydrogen for another 5 billion years.
What is supernovae?
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Stellar core collapse converts substantial mass to energy, producing the most luminous events in the universe. Type Ia supernovae are used as "standard candles" because their peak luminosity is calibrated.
What is black hole accretion?
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Matter falling into a black hole can convert up to about 40 percent of its rest energy to radiation, the most efficient natural energy source known.
What is q1?
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State Einstein's mass-energy equivalence. [2 marks]
What is q2?
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A mass defect of 0.030 u0.030 \text{ u} accompanies a fusion reaction. Calculate the energy released in MeV. [3 marks]
What is q3?
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A 235U^{235}\text{U} fission has Δm=0.215 u\Delta m = 0.215 \text{ u}. (a) Calculate the energy released in J and MeV. (b) Calculate the energy per kilogram of 235U^{235}\text{U} (mnucleus=235.04 um_{nucleus} = 235.04 \text{ u}).

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