Edward Prochak wrote:
> On Monday, June 18, 2018 at 1:04:39 AM UTC-4, RichD wrote:
>> I heard a presentation recently, from one of the LIGO team,
>> discussing the neutron star / black hole collision.
>> He said, following analysis of the gamma ray observations,
>> "Now we know the origin of gold."
>>
>> huh???
>
> I am sure there are more focused articles, but I first
> saw this mentioned here:
>
> "Among other things, the merger gave observers a front-row seat
> at the birth of a black hole, which the colliding neutron stars
> likely produced. The discovery that most glitters, though, is
> smoking-gun evidence that neutron star mergers—rather than
^^^^^^^^^^^
As expected from a *popular*-scientific magazine (by contrast to a
scientific journal) in an article that is filled with sensationalism,
that is an oversimplification.
To elaborate, elements "heavier" than iron (₂₆Fe) and nickel (₂₈Ni; by that
we mean the atomic mass which is related to the number of protons in the
nucleus, indicated by the subscript), such as gold (₇₉Au) cannot be produced
by stellar nuclear fusion because the reactions that could produce them are
endothermic: they would require energy rather than release energy to sustain
a star against its own gravity. So they do not happen.
However, since those elements do exist, the theory is that they have to be
produced in supernovae (accumulation of neutrons that partially beta-decay
into protons, or accumulation of protons) or when neutron stars merge (some
neutrons would beta-decay into protons). (That is an *inclusive* “or”.)
The discovery of merging neutron stars is *indication* that not all of the
heavier elements need to be produced in supernovae. In particular, it can
be assumed that gold and elements heavier than that are produced
predominantly when neutron stars merge as the neutron flux is obviously much
greater then.
Nothing more, nothing less.
Highly recommended (as also easily understandable for people with basic
knowledge in nuclear physics):
T. Rauscher, A. Patkos (2010): Origin of the Chemical Elements.
Handbook of Nuclear Chemistry, 2nd edition (Springer, 2011), p. 611-665.
<
https://arxiv.org/abs/1011.5627>
In particular section “4.5 Nucleosynthesis beyond Fe”.