How do heavier nuclei maintain stability despite requiring energy for fusion?

In summary, heavier nuclei require energy for fusion to occur due to the decrease in potential energy. However, even for heavy elements, the binding energy is always attractive. This can be seen in the binding energy per nucleon graph, where Fe-56 has the highest binding energy. The trend of this graph can be explained by the liquid drop model, which states that splitting heavy elements would release energy, but the energy barrier is too high for it to occur naturally.
  • #1
wasi-uz-zaman
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TL;DR Summary
hi, Fusion of nuclei till Fe or Ni is exothermic but after that it becomes endothermic, I want to ask answer in terms of two main rival forces of nucleus, coulomb force and strong nuclear force.
I understand overall decrease in potential energy of Lighter nuclei releases energy on Fusion- but for heavier nuclei - energy is required- means overall potential energy is not decreased - than how these heavier nuclei sustained their stability.
 
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  • #2
You can see if a nuclear reaction is eso/endothermic by looking at the binding energy per nucleon graph

https://en.wikipedia.org/wiki/Nucle...le:Binding_energy_curve_-_common_isotopes.svg

In the graph the absolute value of the binding energy is plotted vs the number of atomic mass (A). The higher the binding energy, the strongest the attraction and you can see that Fe-56 has the highest binding energy per nucleon. Even for an heavy element the contribution of the binding energy is always attractive. The reason that fusion of heavier element requires to give energy is because you are working to the right of Fe-56:
if you increase A you move from a condition with higher binding energy (strong attraction) to a one with lower biding energy (lower attraction) so you have to supply energy in order to "weaken" the interaction between nucleons.

The trend of that graph is not easy to explain because nuclear forces are pretty complicated, but a simple and yet very good qualitative explanation comes from the liquid drop model (https://en.wikipedia.org/wiki/Semi-empirical_mass_formula)
 
  • #3
Splitting heavy elements like e.g. gold would release energy. But the energy barrier to do so is so high that it doesn't happen naturally (unless you bombard the nucleus with something high-energetic). In principle it should be possible but with a half life so long that we'll never expect to see any decay.
 

1. What is fusion of heavier elements?

Fusion of heavier elements is a nuclear reaction in which two or more atomic nuclei combine to form a heavier nucleus. This process releases a large amount of energy, similar to the energy released by the sun.

2. How is fusion of heavier elements different from fusion of lighter elements?

Fusion of heavier elements requires much higher temperatures and pressures compared to fusion of lighter elements. This is because heavier elements have a stronger repulsive force between their positively charged nuclei, making it more difficult for them to fuse together.

3. What are the potential benefits of fusion of heavier elements?

Fusion of heavier elements has the potential to provide a nearly limitless source of clean energy. It produces no greenhouse gases or long-lived radioactive waste, making it a more sustainable alternative to traditional energy sources.

4. What are the challenges in achieving fusion of heavier elements?

The main challenge in achieving fusion of heavier elements is creating and maintaining the extreme temperatures and pressures required for the reaction to occur. Additionally, controlling the reaction and harnessing the energy produced is also a significant challenge.

5. Is fusion of heavier elements currently being used for energy production?

No, fusion of heavier elements is still in the research and development stage. Scientists are working on developing technologies and methods to make fusion of heavier elements a viable source of energy, but it is not yet being used on a large scale for energy production.

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