Nuclear Decay: Pure Beta vs. Mixed Beta/Gamma Emitters

Click For Summary
SUMMARY

This discussion focuses on the distinction between pure beta emitters and mixed beta/gamma emitters in nuclear decay processes. Key examples of pure beta emitters include tritium, carbon-14 (C-14), strontium-90 (Sr-90), and sulfur-35 (S-35), which typically produce low-energy beta particles. The classification of a nuclide as a pure or mixed emitter is determined by the energy states of the nuclei involved in the decay process, specifically the Q value of the reaction compared to the energy of the lowest excited state in the daughter nucleus. For instance, C-14 decays directly to the ground state of nitrogen-14 (N-14) due to its Q value being less than N-14's first excited state energy.

PREREQUISITES
  • Understanding of nuclear decay processes, specifically beta decay.
  • Familiarity with radionuclides and their decay products.
  • Knowledge of binding energy concepts in nuclear physics.
  • Ability to interpret Q values and excited states in nuclear reactions.
NEXT STEPS
  • Research the binding energy of radionuclides and their decay products.
  • Learn about the excited states of various nuclei using resources like the KAERI database.
  • Explore the implications of Q values in nuclear decay processes.
  • Investigate the applications of pure beta and mixed beta/gamma emitters in nuclear engineering.
USEFUL FOR

Nuclear engineers, physicists, and students studying nuclear physics who seek to understand the mechanisms of beta decay and its applications in various fields.

daveb
Messages
547
Reaction score
2
This may be better suited for the nuclear engineering forum, so feel free to move it.
In decay processes that involve beta decay (or positron decay), there are pure beta emitters and mixed beta/gamma emitters. What determines whether a specific nuclide is just a pure emitter as opposed to a mixed?
 
Physics news on Phys.org
This forum is fine for this question.

Actually, there are very few pure beta emitters, IIRC, for example tritium, C-14, Sr-90, and S-35. They generally produce low energy betas.

The phenomenon depends on the energy states of the nuclei (e.g. T -> He-3), C-14 -> N-14. (from http://www.hps.org/publicinformation/ate/faqs/radiationtypes.html) Check the binding energy of both of the pair nuclei (radionuclide and subsequent decay product, or stable daughter nuclide).

In beta decay, the daughter nucleus would emit the subsequent gamma to dump extra energy dropping into its final stable state.
 
Astronuc said:
The phenomenon depends on the energy states of the nuclei (e.g. T -> He-3), C-14 -> N-14. (from http://www.hps.org/publicinformation/ate/faqs/radiationtypes.html) Check the binding energy of both of the pair nuclei (radionuclide and subsequent decay product, or stable daughter nuclide).

You can check out the excited states for nuclei here:

http://atom.kaeri.re.kr/ton/

In most cases, for the pure beta emitters, the Q value of the reaction is less than the energy of the lowest excited state in the daughter nuclei. For example, N-14's first excited state is at 5.1 Mev, but the Q-value of C-14 decay is only 0.156 Mev. Since the Q-value is less than the first excited state of N-14, C-14 decays directly to the ground state of N-14 and all of the decay energy goes to the beta/neutrino/recoil nucleus kinetic energy.
 

Similar threads

  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 4 ·
Replies
4
Views
4K
  • · Replies 3 ·
Replies
3
Views
2K
Replies
12
Views
2K
  • · Replies 28 ·
Replies
28
Views
11K
  • · Replies 1 ·
Replies
1
Views
3K
Replies
1
Views
1K
  • · Replies 9 ·
Replies
9
Views
9K
  • · Replies 12 ·
Replies
12
Views
4K
  • · Replies 8 ·
Replies
8
Views
3K