Jump to content
Main menu
Main menu
move to sidebar
hide
Navigation
Main page
Recent changes
Random page
Help about MediaWiki
Special pages
Niidae Wiki
Search
Search
Appearance
Create account
Log in
Personal tools
Create account
Log in
Pages for logged out editors
learn more
Contributions
Talk
Editing
Nucleosynthesis
(section)
Page
Discussion
English
Read
Edit
View history
Tools
Tools
move to sidebar
hide
Actions
Read
Edit
View history
General
What links here
Related changes
Page information
Appearance
move to sidebar
hide
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
===Neutron star mergers=== The [[Neutron star collision|merger]] of binary neutron stars (BNSs) is now believed to be the main source of r-process elements.<ref>{{cite web |last=Stromberg |first=Joseph |date=16 July 2013 |title=All the Gold in the Universe Could Come from the Collisions of Neutron Stars |url=http://www.smithsonianmag.com/science-nature/all-the-gold-in-the-universe-could-come-from-the-collisions-of-neutron-stars-13474145/?page=1 |work=[[Smithsonian (magazine)|Smithsonian]] |access-date=27 April 2014}}</ref> Being neutron-rich by definition, mergers of this type had been suspected of being a source of such elements, but definitive evidence was difficult to obtain. In 2017 strong evidence emerged, when [[LIGO]], [[Virgo interferometer|VIRGO]], the [[Fermi Gamma-ray Space Telescope]] and [[INTEGRAL]], along with a collaboration of many observatories around the world, detected both [[gravitational wave]] and electromagnetic signatures of a likely neutron star merger, [[GW170817]], and subsequently detected signals of numerous heavy elements such as gold as the ejected [[Degenerate matter#Neutron degeneracy|degenerate matter]] decays and cools.<ref>{{cite web |last=Chu |first=J. |date=n.d. |url=https://www.ligo.caltech.edu/page/press-release-gw170817 |title=GW170817 Press Release |publisher=[[LIGO]]/[[Caltech]] |access-date=2018-07-04}}</ref> The first detection of the merger of a neutron star and black hole (NSBHs) came in July 2021 and more after but analysis seem to favor BNSs over NSBHs as the main contributors to heavy metal production.<ref>{{Cite journal|last1=Chen|first1=Hsin-Yu|last2=Vitale|first2=Salvatore|last3=Foucart|first3=Francois|date=2021-10-01|title=The Relative Contribution to Heavy Metals Production from Binary Neutron Star Mergers and Neutron Star–Black Hole Mergers|journal=The Astrophysical Journal Letters|volume=920|issue=1|pages=L3|doi=10.3847/2041-8213/ac26c6|arxiv=2107.02714 |bibcode=2021ApJ...920L...3C |s2cid=238198587 |issn=2041-8205|doi-access=free}}</ref><ref>{{Cite web|title=Neutron star collisions are a "goldmine" of heavy elements, study finds|url=https://news.mit.edu/2021/neutron-star-collisions-goldmine-heavy-elements-1025|access-date=2021-12-23|website=MIT News {{!}} Massachusetts Institute of Technology|date=25 October 2021 |language=en}}</ref>
Summary:
Please note that all contributions to Niidae Wiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
Encyclopedia:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Search
Search
Editing
Nucleosynthesis
(section)
Add topic