Neutronium

Neutronium is a proposed name for a substance composed purely of neutrons. The word was coined by scientist Andreas von Antropoff in 1926 (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.[1][2] However, the meaning of the term has changed over time, and from the last half of the 20th century onward it has been used legitimately to refer to extremely dense phases of matter resembling the neutron-degenerate matter postulated to exist in the cores of neutron stars. Science fiction and popular literature frequently use the term "neutronium" to refer to a highly dense phase of matter composed primarily of neutrons.

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Neutronium and neutron stars

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:

When neutron star core material is presumed to consist mostly of free neutrons, it is typically referred to as neutron-degenerate matter in scientific literature.[3]

Neutronium and the periodic table

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 in the middle of several spiral representations of the periodic system for classifying the chemical elements, such as those of Charles Janet (1928), E. I. Emerson (1944), John D. Clark (1950) and in Philip Stewart's Chemical Galaxy (2005).

Although the term is not used in the scientific literature either for a condensed form of matter, or as an element, there have been reports that, besides the free neutron, there may exist two bound forms of neutrons without protons.[4] However, these reports have not been further substantiated. Further information can be found in the following articles:

If one accepts neutronium to be an element, the above mentioned neutron clusters would be the isotopes of that element, if their existence can be confirmed. Also, if neutronium is accepted to be an element, it would not be a noble gas, for it would have no electrons, in fact, it would have no electron shells. All electron shells and their electrons have been squeezed out of the material by pressure. The material would, thus, like noble gasses be unreactive, but for different reasons. Neutronium would not fit anywhere in the periodic table. Although not called "neutronium", the National Nuclear Data Center's Nuclear Wallet Cards lists as its first "isotope" an "element" with the symbol n and atomic number Z = 0 and mass number A = 1. This isotope is described as decaying to element H with a half life of 10.24±0.02 minutes.

Neutronium in fiction

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 Earth-like conditions, or possessing exotic properties such as the ability to manipulate time and space. In contrast, 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:

See also

References

  1. ^ von Antropoff, A. (1926). "Eine neue Form des periodischen Systems der Elementen". Zeitschrift für Angewandte Chemie 39 (23): 722–725. doi:10.1002/ange.19260392303. http://www3.interscience.wiley.com/cgi-bin/fulltext/112256618/PDFSTART. 
  2. ^ Stewart, P. J. (2007). "A century on from Dmitrii Mendeleev: Tables and spirals, noble gases and Nobel prizes". Foundations of Chemistry 9 (3): 235–245. doi:10.1007/s10698-007-9038-x. 
  3. ^ Angelo, J. A. (2006). Encyclopedia of space and astronomy. Infobase Publishing. ISBN 9780816053308. http://books.google.com/books?id=VUWno1sOwnUC&pg=PA178. 
  4. ^ Timofeyuk, N. K. (2003). "Do multineutrons exist?". Journal of Physics G 29 (2): L9. arXiv:nucl-th/0301020. Bibcode 2003JPhG...29L...9T. doi:10.1088/0954-3899/29/2/102. 
  5. ^ Bertulani, C. A.; Baur, G. (1986). "Coincidence Cross-sections for the Dissociation of Light Ions in High-energy Collisions". Nuclear Physics A 480 (3–4): 615. Bibcode 1988NuPhA.480..615B. doi:10.1016/0375-9474(88)90467-8. http://faculty.tamu-commerce.edu/cbertulani/cab/papers/NPA480_1988_615.pdf. 
  6. ^ a b Bertulani, C. A.; Canto, L. F.; Hussein, M. S. (1993). "The Structure And Reactions Of Neutron-Rich Nuclei". Physics Reports 226 (6): 281–376. Bibcode 1993PhR...226..281B. doi:10.1016/0370-1573(93)90128-Z. http://www.tamu-commerce.edu/physics/carlos/papers/PRep226_1993_281.pdf. 
  7. ^ Hagino, K.; Sagawa, H.; Nakamura, T.; Shimoura, S. (2009). "Two-particle correlations in continuum dipole transitions in Borromean nuclei". Physical Review C 80 (3): 1301. arXiv:0904.4775. Bibcode 2009PhRvC..80c1301H. doi:10.1103/PhysRevC.80.031301. 
  8. ^ MacDonald, J.; Mullan, D. J. (2009). "Big Bang Nucleosynthesis: The Strong Nuclear Force meets the Weak Anthropic Principle". Physical Review D 80 (4): 3507. arXiv:0904.1807. Bibcode 2009PhRvD..80d3507M. doi:10.1103/PhysRevD.80.043507. 
  9. ^ Kneller, J. P.; McLaughlin, G. C. (2004). "The Effect of Bound Dineutrons upon BBN". Physical Review D 70 (4): 043512. arXiv:astro-ph/0312388. Bibcode 2004PhRvD..70d3512K. doi:10.1103/PhysRevD.70.043512. 
  10. ^ Bertulani, C. A.; Zelevinsky, V. (2002). "Is the tetraneutron a bound dineutron-dineutron molecule?". Journal of Physics G 29 (10): 2431. arXiv:nucl-th/0212060. Bibcode 2003JPhG...29.2431B. doi:10.1088/0954-3899/29/10/309. 
  11. ^ Timofeyuk, N. K. (2002). "On the existence of a bound tetraneutron". arXiv:nucl-th/0203003 [nucl-th]. 
  12. ^ Bevelacqua, J. J. (1981). "Particle stability of the pentaneutron". Physics Letters B 102 (2–3): 79–80. Bibcode 1981PhLB..102...79B. doi:10.1016/0370-2693(81)91033-9. 
  13. ^ http://starwars.wikia.com/wiki/Neutronium

Further reading