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  1. The ratio of their nuclear densities is 1:1. Nuclear density is nearly constant for all nuclei because it depends only on the nuclear volume and not on the mass number, which scales proportionally with volume. For more visit here: https://www.tiwariacademy.com/ncert-solutions/class-12/physics/chapteRead more

    The ratio of their nuclear densities is 1:1. Nuclear density is nearly constant for all nuclei because it depends only on the nuclear volume and not on the mass number, which scales proportionally with volume.

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    https://www.tiwariacademy.com/ncert-solutions/class-12/physics/chapter-13/

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  2. The binding energy of a nucleus is the energy required to separate a nucleus into its constituent protons and neutrons. It reflects the stability of the nucleus, with higher binding energy indicating greater stability. For more visit here: https://www.tiwariacademy.com/ncert-solutions/class-12/physiRead more

    The binding energy of a nucleus is the energy required to separate a nucleus into its constituent protons and neutrons. It reflects the stability of the nucleus, with higher binding energy indicating greater stability.

    For more visit here:
    https://www.tiwariacademy.com/ncert-solutions/class-12/physics/chapter-13/

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  3. No, ³₂He and ³₁H nuclei do not have the same binding energy. Although they have the same mass number, their nuclear structures and binding energies differ, as binding energy depends on proton-neutron interactions and nuclear stability. For more visit here: https://www.tiwariacademy.com/ncert-solutioRead more

    No, ³₂He and ³₁H nuclei do not have the same binding energy. Although they have the same mass number, their nuclear structures and binding energies differ, as binding energy depends on proton-neutron interactions and nuclear stability.

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    https://www.tiwariacademy.com/ncert-solutions/class-12/physics/chapter-13/

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  4. The energy production in the Sun is primarily due to the proton-proton chain reaction. In this process, hydrogen nuclei fuse to form helium, releasing vast amounts of energy in the form of light and heat. For more visit here: https://www.tiwariacademy.com/ncert-solutions/class-12/physics/chapter-13/

    The energy production in the Sun is primarily due to the proton-proton chain reaction. In this process, hydrogen nuclei fuse to form helium, releasing vast amounts of energy in the form of light and heat.

    For more visit here:
    https://www.tiwariacademy.com/ncert-solutions/class-12/physics/chapter-13/

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  5. The daughter nucleus would have a higher binding energy per nucleon. Fusion typically results in a more stable, heavier nucleus, where nucleons are more tightly bound, releasing energy. This is because the binding energy increases with atomic mass. For more visit here: https://www.tiwariacademy.com/Read more

    The daughter nucleus would have a higher binding energy per nucleon. Fusion typically results in a more stable, heavier nucleus, where nucleons are more tightly bound, releasing energy. This is because the binding energy increases with atomic mass.

    For more visit here:
    https://www.tiwariacademy.com/ncert-solutions/class-12/physics/chapter-13/

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