Alpha decay short half lives correspond to large disintegration energies

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SUMMARY

In alpha decay, short half-lives correspond to large disintegration energies due to the increased probability of quantum tunneling through potential barriers. The energy release during the alpha decay of Uranium-238 (238U) to Thorium-234 (234Th) can be calculated using the mass defect method. The masses involved are 238.0508 mu for 238U, 234.0436 mu for 234Th, and 4.0026 mu for Helium (4He). The energy released can be determined using the equation E=mc², where the mass defect is derived from the difference in mass between the parent and daughter nuclei.

PREREQUISITES
  • Understanding of alpha decay and nuclear reactions
  • Familiarity with mass defect calculations
  • Knowledge of Einstein's mass-energy equivalence principle (E=mc²)
  • Basic concepts of quantum tunneling in nuclear physics
NEXT STEPS
  • Calculate the mass defect for the alpha decay of 238U to 234Th using the provided masses
  • Explore quantum tunneling and its implications in nuclear decay processes
  • Study the relationship between half-life and disintegration energy in nuclear physics
  • Investigate other types of radioactive decay and their energy release mechanisms
USEFUL FOR

Students studying nuclear physics, physicists interested in radioactive decay processes, and educators teaching concepts related to alpha decay and energy calculations.

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Homework Statement



i) Explain why in alpha decay short half lives correspond to large disintegration energies.

ii) Determine the energy release during the alpha decay of 238U to 234Th. The mass of 238U is 238.0508mu, the mass of 234Th is 234.0436mu, and the mass of 4He is 4.0026mu.


Homework Equations



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The Attempt at a Solution



I haven't seen an example of this in my course book, so I have more ideas than attempts at a solution.

Would I be right in right in finding the mass defect in U, Th and He, and then subtracting U's mass defect from Th's and He's, mass defect.

Once I have that I would use E=mc2, to calculate the energy released.

But this seems quite long and drawn out is there another method to calculate this, is the method even right?
 
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You have the right idea for ii). What you mention is essentially conservation of relativistic energy, and it doesn't get much simpler than that.

A partial answer to i) would be to consider the conditions under which the probability of tunneling out of a potential barrier increases, and see how that is relevant to alpha decay.
 

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