Heavy elements from neutron star collisions?

Click For Summary
SUMMARY

The recent observation of a neutron-star merger by LIGO supports the hypothesis that heavy elements, particularly gold and platinum, are primarily produced in neutron-star collisions rather than supernovae. This theory gained traction due to evidence from a Nature paper highlighting high levels of r-process elements in the Reticulum II dwarf galaxy, suggesting that these elements are ejected during neutron star mergers. The study indicates that approximately 1% of the combined mass of neutron stars is expelled as heavy elements, challenging the previous belief that supernovae were the sole source of such materials.

PREREQUISITES
  • Understanding of neutron star physics
  • Familiarity with r-process nucleosynthesis
  • Knowledge of supernova mechanisms
  • Basic comprehension of astronomical observations and data interpretation
NEXT STEPS
  • Research the r-process and its role in heavy element formation
  • Explore the implications of neutron star mergers on cosmic chemical evolution
  • Study the findings of the recent Nature paper on Reticulum II dwarf galaxy
  • Investigate the effects of neutron star rotation on mass ejection during mergers
USEFUL FOR

Astronomers, astrophysicists, and researchers interested in nucleosynthesis, cosmic evolution, and the origins of heavy elements in the universe.

maline
Messages
436
Reaction score
69
I have seen it claimed online that the recently announced observation of a neutron-star merger by LIGO provides strong support for the hypothesis that heavy elements - gold and platinum were mentioned in particular - are mostly created in neutron-star collisions rather than in supernovas. Is this correct? Where can I find reliable information about this story?

In fact, where can I read about this hypothesis at all? Until today supernovas were the only source I heard mentioned for elements not created in the normal stellar fusion reactions.
 
Astronomy news on Phys.org
maline said:
In fact, where can I read about this hypothesis at all? Until today supernovas were the only source I heard mentioned for elements not created in the normal stellar fusion reactions.

I have no source, but I heard about that mechanism many years ago. Thus it is not really new.
 
Wikipedia is always a good place to start. I think until about 2000 or so, it was thought that supernovae were the main source of all heavy elements. However, there were problems with getting enough of the "r-process" elements, which are neutron rich elements heavier than iron. The hypothesis that most of these elements come from decompressed neutron star material flung into interstellar space during neutron star mergers has been gaining favor. This recent Nature paper claims support for that hypothesis.
 
  • Like
Likes   Reactions: maline
A key piece of evidence for this scenario emerged recently with the discovery of extremely high levels of r-process elements in the Reticulum II dwarf galaxy, which orbits the Milky Way. "This implies that a single rare event produced the r-process material in Reticulum II. The r-process yield and event rate are incompatible with ordinary core-collapse supernovae, but consistent with other possible sites, such as neutron star mergers." Link: ArXiv
 
  • Like
Likes   Reactions: maline
This article claims around 1% of the combined mass was ejected as heavy elements. Anyone know how they got that number. Does it eject iron too? Why not?

How much can rotation in the original neutron stars change the mass ejected?
 
stefan r said:
This article claims around 1% of the combined mass was ejected as heavy elements. Anyone know how they got that number. Does it eject iron too? Why not?

How much can rotation in the original neutron stars change the mass ejected?
I would think that what is emitted is initially Neutron star matter, which is mostly dense neutrons. This decays into heavy neutron rich isotopes. Within the neutron star, there are no atomic nuclei except perhaps in an outer skin.
 
As PAllen said, what is ejected is dense neutron star matter, which rapidly decays into a whole host of heavy elements. below is Figure 4 from this Arxiv paper, which shows the distribution of elements that result. One of the reasons people favor this model is that it seems to reproduce the observed abundances of heavy elements in the Solar System.

NS_Elements.png
 
  • Like
Likes   Reactions: stefan r

Similar threads

  • · Replies 28 ·
Replies
28
Views
4K
  • · Replies 34 ·
2
Replies
34
Views
6K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 38 ·
2
Replies
38
Views
6K
  • · Replies 26 ·
Replies
26
Views
5K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
  • · Replies 14 ·
Replies
14
Views
2K
  • · Replies 11 ·
Replies
11
Views
2K