Can a White Dwarf Collapse into a Neutron Star Without a Supernova?

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SUMMARY

A white dwarf star in a binary system cannot collapse directly into a neutron star without undergoing a supernova. When a white dwarf exceeds the Chandrasekhar limit of approximately 1.4 solar masses, it triggers a Type Ia supernova instead of collapsing. This occurs because white dwarfs, composed mainly of carbon and oxygen, still possess significant thermonuclear energy for fusion reactions. In contrast, neutron stars form from the collapse of more massive stars with iron cores, where no further fusion can occur, leading to a definitive collapse into a black hole if the Tolman-Oppenheimer-Volkoff limit is exceeded.

PREREQUISITES
  • Understanding of white dwarf and neutron star formation
  • Familiarity with the Chandrasekhar limit
  • Knowledge of Type Ia supernova mechanisms
  • Comprehension of the Tolman-Oppenheimer-Volkoff limit
NEXT STEPS
  • Research the mechanisms of Type Ia supernovae
  • Study the properties and formation processes of neutron stars
  • Explore the implications of the Tolman-Oppenheimer-Volkoff limit on stellar evolution
  • Investigate the nuclear binding energy curve and its significance in stellar collapse
USEFUL FOR

Astronomers, astrophysicists, and students studying stellar evolution and supernova phenomena will benefit from this discussion.

PeterB
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Is it possible for white dwarf star in binary system where it is feeding off its partner star to collapse directly into a neutron star? Or is something inherent in the formation of neutron stars where they must be formed from supernova?
 
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When a white dwarf accretes mass from a companion and exceeds the Chandrasekhar limit of about 1.4 solar masses, instead of collapsing to a neutron star, it explodes as a Type 1A supernova. The reason is that a white dwarf is formed of relatively light elements like carbon and oxygen, so there is still a lot of thermonuclear energy available from further fusion reactions. So when the star gets compressed further, these thermonuclear reactions ignite and the star explodes in a massive explosion. By contrast, when the core of a more massive star collapses to form a neutron star, the core is formed of heavier elements like iron. Since iron is at the peak of the nuclear binding energy curve, there is no more thermonuclear energy available from further fusion reactions.
 
Thank you for you response, Would this mean that a neutron star which exceeds its Tolman-Oppenheimer-volkoff limit would always collapse to a black hole? Would fusion of Neutron star material (primarily neutrons) be possible?
 
Big neutron star collapse results in a black hole. The core of a neutron star can be thought of as the "fusion" of its neutrons. However there is no such thing as a fusion reaction in this case.
 
PeterB said:
Thank you for you response, Would this mean that a neutron star which exceeds its Tolman-Oppenheimer-volkoff limit would always collapse to a black hole?

Yes, as far as we know this is the only outcome.
 

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