How Dense and Long-lived Are Neutron Stars?

Click For Summary
SUMMARY

Neutron stars typically possess a mass of approximately 1.5 times that of the Sun, equivalent to about 3 x 1030 kilograms. This formation occurs when a star exceeds the Chandrasekhar mass of roughly 1.4 times the Sun's mass, leading to the collapse of electrons and protons into neutrons, supported by neutron degeneracy pressure. While there is no definitive lifespan for neutron stars, they gradually cool over time, losing thermal energy, and their average diameter is around 10 kilometers. The maximum mass limit for a neutron star before collapsing into a black hole is believed to be less than 2 times the mass of the Sun.

PREREQUISITES
  • Understanding of the Chandrasekhar mass and its implications
  • Knowledge of electron and neutron degeneracy pressure
  • Familiarity with stellar evolution and supernova processes
  • Basic concepts of black hole formation and characteristics
NEXT STEPS
  • Research the properties and lifecycle of neutron stars
  • Explore the concept of degeneracy pressure in astrophysics
  • Investigate the relationship between neutron stars and black holes
  • Study observational techniques used to measure neutron star characteristics
USEFUL FOR

Astronomers, astrophysicists, and students interested in stellar evolution, as well as anyone seeking to understand the physical properties and lifecycle of neutron stars.

boy genius
Messages
8
Reaction score
0
undefined

what mass does a neutron star hove and what is its life span?

and any other information on the subject would not go un-apiretiated
 
Physics news on Phys.org
boy genius said:
what mass does a neutron star hove and what is its life span?

Neutron stars typically have masses around 1.5 times the mass of the sun (~3 x 1030 kilograms). This is because there is a mass known as the "Chandrasekhar mass" beyond which electron degeneracy pressure (see this thread for a description of degeneracy pressure) cannot hold a star up from gravity. This mass is around 1.4 times the mass of the sun. Once it's passed, the electrons and protons undergo inverse beta decay and form neutrons. This leads to a star that is instead held up by neutron degeneracy pressure, called a neutron star. There is also a mass beyond which neutron degeneracy pressure will fail and the object will collapse to a black hole, but we don't know the exact value of this mass. From observations, we think it's less than 2 times the mass of the sun.

As far as I know, there's no limit to how long they can live, but they will cool over time, radiating away their thermal energy. They're very dense and their sizes are typically around 10 kilometers.
 

Similar threads

  • · Replies 3 ·
Replies
3
Views
5K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 20 ·
Replies
20
Views
4K
  • · Replies 11 ·
Replies
11
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 2 ·
Replies
2
Views
4K
  • · Replies 13 ·
Replies
13
Views
3K
  • · Replies 48 ·
2
Replies
48
Views
7K
Replies
12
Views
4K