Under ideal conditions could there be thousands of elements?

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Discussion Overview

The discussion revolves around the possibility of the existence of thousands of chemical elements under extreme conditions in space, such as high temperatures and pressures. Participants explore whether these conditions could lead to the formation of stable elements, particularly those that are currently unstable or have not been observed.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification

Main Points Raised

  • Some participants propose that under extreme conditions, such as a trillion degrees Celsius, there could be more than the currently known 118 elements.
  • There is a question about whether super high temperatures would facilitate the formation of stable elements or any elements at all.
  • One participant mentions that in conditions like a supernova, higher atomic number elements could be created as they decay, but doubts that this would lead to a thousand elements.
  • Another participant questions the possibility of a stability area for higher nuclei numbers, specifically around 150 protons.
  • Concerns are raised about the absence of evidence for super-heavy elements, questioning why they have not been found on Earth or in stellar spectra despite billions of years of cosmic history.
  • There is a suggestion that super-heavy elements might be produced in heavy ion colliders, and a discussion on whether the rapid decay of transactinides is due to their production in excited states.
  • One participant notes a limit on the number of electrons in atomic shells, relating it to the fine structure constant.

Areas of Agreement / Disagreement

The discussion remains unresolved, with multiple competing views on the existence and stability of elements under extreme conditions. Participants express differing opinions on the feasibility of forming stable super-heavy elements and the implications of current scientific observations.

Contextual Notes

Participants acknowledge limitations in current understanding, including the dependence on specific conditions for element formation and the unresolved nature of isotopes that have not yet been produced.

AMan24
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Right now I think there's 118 elements. If somewhere in space it was a certain temperature, with certain pressure, and other certain factors, could there be more elements. Let's say these conditions are too extreme to be made on Earth like a Trillion degrees Celsius.

So if there were there ideal conditions, could there be thousands of elements?

Or could the unstable elements scientists can create on Earth become stable?
 
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AMan24 said:
Let's say these conditions are too extreme to be made on Earth like a Trillion degrees Celsius.
Do you think a super high temperature would be conducive to the formation of stable elements? Of ANY elements?
 
There are two conditions that might meet your requirements:
Under the right conditions (think supernova), you could have an equilibrium that included elements of higher atomic number. You would be creating them as fast as they were decaying. But I doubt that you get to a thousand that way.

The other condition is a neutron star. The neutron density at the interior of a neutron star is limited by the Pauli exclusion principle, so its as dense as an atomic nucleus. I'll let you decide if that counts.

http://heasarc.gsfc.nasa.gov/docs/xte/learning_center/ASM/ns.html
 
Can it be ruled out that there is another stability area on higher nuclei numbers, e.g. around 150 protons?
 
fresh_42 said:
Can it be ruled out that there is another stability area on higher nuclei numbers, e.g. around 150 protons?
Let's suppose there was such a region.

Where are these super-heavy elements, if they are stable? They haven't been found on earth, nor do they appear in the spectrum of any current or past star, AFAIK.
You'd think that after several billion years, some evidence of these elements would have been discovered, if they are indeed stable.
 
SteamKing said:
You'd think that after several billion years, some evidence of these elements would have been discovered, if they are indeed stable.
Yes you are right under the assumption that they occur naturally in supernovae explosions. But that doesn't rule out the possibility to produce them in heavy ion colliders. Another question here is: Do the transactinides decay so fast only because we can generate them in excited states? What about all the isotopes we haven't produced so far? I just read that Fermium has been found in a hydrogen bomb explosion. I guess we haven't found it in the universe neither although it might occur during a supernova collapse.
 
There is also a limit on the number of electrons in the atomic shell. This is roughly the inverse of the fine structure constant, i.e. about 137.
 
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