Neutron Decay in Neutron Stars: Gravity or Half-Life?

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SUMMARY

The discussion centers on neutron decay within neutron stars, specifically addressing the stability of neutrons under extreme gravitational conditions. The half-life of a free neutron is established at approximately 10.3 minutes, correcting an initial misstatement of seconds. Participants clarify that in neutron stars, the stability of neutrons is primarily influenced by electron chemical potential rather than gravity or the strong force. This insight emphasizes the unique conditions present in neutron stars that allow for neutron stability despite their inherent half-life.

PREREQUISITES
  • Understanding of neutron decay and half-life concepts
  • Familiarity with neutron star composition and properties
  • Knowledge of electron chemical potential in astrophysics
  • Basic principles of gravitational forces in astrophysical contexts
NEXT STEPS
  • Research the half-life of neutrons and its implications in nuclear physics
  • Explore the role of electron chemical potential in neutron star stability
  • Study the effects of gravity on particle behavior in extreme environments
  • Investigate the strong force and its role in atomic nuclei
USEFUL FOR

Astronomers, physicists, and students of astrophysics interested in the behavior of neutrons in extreme environments, particularly within neutron stars.

Mordred
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On decays I have only a preliminary understanding. I was looking up the half life of a neutron for another reason.
The value I found for neutron decay for a free neutron was 10.3 seconds. Hope that's reasonably accurate.
Anyways knowing that neutrons are stable in a nucleus held together by the strong force.
In the case of neutron stars which are comprised mainly of neutrons which is said to be held by gravity not the strong force.
Is the local gravity allowing neutron stability or does the neutrons have the above mentioned half life?
 
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Mordred said:
The value I found for neutron decay for a free neutron was 10.3 seconds. Hope that's reasonably accurate.
Wrong order of magnitude. 10 minutes, not seconds.
Mordred said:
Anyways knowing that neutrons are stable in a nucleus held together by the strong force.
In the case of neutron stars which are comprised mainly of neutrons which is said to be held by gravity not the strong force.
Is the local gravity allowing neutron stability or does the neutrons have the above mentioned half life?

In neutron stars, it is electron chemical potential that makes neutrons stable. Gravity as such is irrelevant.
 
Lol I meant minutes not sure why I typed seconds. Anyways thanks for the answer.
 

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