Neutronium is a term presently used in science fiction and in popular literature to refer to an extremely dense phase of matter composed primarily of neutrons. Historically, the word was coined by scientist Andreas von Antropoff in 1926 (scil., before the discovery of the neutron itself) for the conjectured 'element of atomic number zero' that he placed at the head of the periodic table. The meaning of the term changed over time, and from the last half of the 20th century onwards it was used to refer to extremely dense phases of matter resembling the neutron-degenerate matter postulated to exist in the cores of neutron stars.
The term neutronium is used in popular literature to refer to the material present in the cores of neutron stars (stars which are too massive to be supported by electron degeneracy pressure and which collapse into a denser phase of matter). This term is very rarely used in scientific literature, for two reasons:
The term neutronium was coined in 1926 by Professor Andreas von Antropoff for a conjectured form of matter made up of neutrons with no protons, which he placed as the chemical element of atomic number zero at the head of his new version of the periodic table. It was subsequently placed as a noble gas in the middle of several spiral representations of the periodic system for classifying the chemical elements. It is at the centre of the Chemical Galaxy (2005).
Although the term is still not widely used in the scientific literature for a condensed form of matter, there have been reports that, besides the free neutron, there may exist two isotopes without protons. However, these reports have not been further substantiated. Further information can be found in the following articles:
A trineutron state consisting of three bound neutrons has not been detected, and is not expected to be stable even for a short time. Calculations indicate that the hypothetical pentaneutron state, consisting of a cluster of five neutrons, would not be bound.
The term neutronium has been popular in science fiction since at least the middle of the 20th century. It typically refers to an extremely dense, incredibly strong form of matter. While presumably inspired by the concept of neutron-degenerate matter in the cores of neutron stars, the material used in fiction bears at most only a superficial resemblance (usually depicted as an extremely strong solid under Earthlike conditions, while all proposed forms of neutron star core material are fluids and are extremely unstable at pressures lower than that found in stellar cores).
Noteworthy appearances of neutronium in fiction include the following:
No analogous material is expected to exist in the real world. The ultra-dense material in the cores of neutron stars is only stable at the extremely high pressures found there. Under Earth-like conditions, it would immediately revert to being normal matter, exploding with great force in the process.
Astrophysics | Condensed matter physics | Fictional materials | Neutron
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"Neutronium".
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