Neutron Star Collisions: Creation of Heavy Elements and Their Fate

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Discussion Overview

The discussion centers on the outcomes of neutron star collisions, specifically regarding the creation and fate of heavy elements such as gold. It explores whether these elements are ejected into space or fall back into a newly formed black hole, touching on implications for the abundance of heavy elements in the universe.

Discussion Character

  • Exploratory, Technical explanation, Conceptual clarification

Main Points Raised

  • Some participants propose that heavy elements created during neutron star collisions are ejected from the system and contribute to the InterStellar Medium (ISM).
  • Others argue that a significant quantity of heavy elements is indeed ejected, with estimates from the neutron star merger GW170817 suggesting about 0.01 solar masses of heavy elements were released.
  • A later reply mentions that heavy elements are also produced during supernova events and are ejected from stars in those cases.

Areas of Agreement / Disagreement

Participants generally agree that heavy elements are ejected from neutron star collisions, but there is some uncertainty about the extent to which they may fall back into a black hole.

Contextual Notes

There are unresolved questions regarding the exact mechanisms of ejection and the conditions under which heavy elements are retained or lost in these astrophysical events.

tovisonnenberg
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When neutron stars collide, heavy elements, such as gold, are created. Are these elements ejected from the system to be found, say, here on earth? Or do they fall back into the newly created black hole?
 
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Short answer: both.
 
If they all fell back into the newly created black hole, then these events could not contribute to the concentration of heavy elements in stars and planets. The answer is that a significant quantity of these heavy elements get ejected from the binary neutron star system and get incorporated into the InterStellar Medium (ISM). The estimates from the recently detected neutron star merger GW170817 are that about 0.01 solar masses of heavy elements were ejected. When stars and planets later form from this ISM, these heavy elements are incorporated into these new stars and planets.
 
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On a side note, I read that many heavy elements are created when a star goes supernova. Those elements are also ejected from the star.
 

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