World Library  
Flag as Inappropriate
Email this Article

Neutronium

Article Id: WHEBN0000021868
Reproduction Date:

Title: Neutronium  
Author: World Heritage Encyclopedia
Language: English
Subject: Neutron star, Degenerate matter, Neutron, Table of nuclides (complete), Technology in Stargate
Collection: Astrophysics, Exotic Matter, Fictional Materials, Neutron
Publisher: World Heritage Encyclopedia
Publication
Date:
 

Neutronium

Neutronium (sometimes shortened to neutrium[1]) 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) for the conjectured "element of atomic number zero" that he placed at the head of the periodic table.[2][3] However, the meaning of the term has changed over time, and from the last half of the 20th century onward it has been also used legitimately to refer to extremely dense substances resembling the neutron-degenerate matter theorized to exist in the cores of neutron stars; henceforth "degenerate neutronium" will refer to this. Science fiction and popular literature frequently use the term "neutronium" to refer to a highly dense phase of matter composed primarily of neutrons.

Contents

  • Neutronium and neutron stars 1
  • Neutronium and the periodic table 2
  • Properties 3
  • In fiction 4
  • See also 5
  • References 6
  • Further reading 7

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 three reasons:

  • There are multiple definitions for the term "neutronium".
  • There is considerable uncertainty over the composition of the material in the cores of neutron stars (it could be neutron-degenerate matter, strange matter, quark matter, or a variant or combination of the above).
  • The properties of neutron star material should depend on depth due to changing pressure (see below), and no sharp boundary between the crust (consisting primarily of atomic nuclei) and almost protonless inner layer is expected to exist.

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.[4]

Neutronium and the periodic table

The term "neutronium" was coined in 1926 by Andreas von Antropoff for a conjectured form of matter made up of neutrons with no protons or electrons, 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.[5] If neutronium were considered to be an element, then these neutron clusters could be considered to be the isotopes of that element. However, these reports have not been further substantiated. Further information can be found in the following articles:

  • Mononeutron: Isolated neutrons undergo beta decay with a mean lifetime of approximately 15 minutes (half-life of approximately 10 minutes), becoming protons (the nucleus of hydrogen), electrons and antineutrinos.
  • Dineutron: The dineutron, containing two neutrons was unambiguously observed in the decay of beryllium-16, in 2012 by researchers at Michigan State University.[6][7] It is not a bound particle, but had been proposed as an extremely short-lived state produced by nuclear reactions involving tritium. It has been suggested to have a transitory existence in nuclear reactions produced by helions that result in the formation of a proton and a nucleus having the same atomic number as the target nucleus but a mass number two units greater. There had been evidence of dineutron emission from neutron-rich isotopes such as beryllium-16 where mononeutron decay would result in a less stable isotope. The dineutron hypothesis had been used in nuclear reactions with exotic nuclei for a long time.[8] Several applications of the dineutron in nuclear reactions can be found in review papers.[9] Its existence has been proven to be relevant for nuclear structure of exotic nuclei.[10] A system made up of only two neutrons is not bound, though the attraction between them is very nearly enough to make them so.[11] This has some consequences on nucleosynthesis and the abundance of the chemical elements.[9][12]
  • Trineutron: A trineutron state consisting of three bound neutrons has not been detected, and is not expected to exist even for a short time.
  • Tetraneutron: A tetraneutron is a hypothetical particle consisting of four bound neutrons. Reports of its existence have not been replicated. If confirmed, it would require revision of current nuclear models.[13][14]
  • Pentaneutron: Calculations indicate that the hypothetical pentaneutron state, consisting of a cluster of five neutrons, would not be bound.[15]

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 min.

Properties

Due to beta (β) decay of mononeutron and extreme instability of aforementioned heavier "isotopes", degenerate neutronium is not expected to be stable under ordinary pressures. Free neutrons decay with a half-life of 10 minutes, 11 seconds. A teaspoon of degenerate neutronium gas would have a mass of two billion tonnes, and if moved to standard temperature and pressure, would emit 57 billion joules of β decay energy in the first half-life (average of 95 MW of power).[16] This energy may be absorbed as the neutronium gas expands. Though, in the presence of atomic matter compressed to the state of electron degeneracy, the β decay may be inhibited due to Pauli exclusion principle, thus making free neutrons stable. Also, elevated pressures should make neutrons degenerate themselves. Compared to ordinary elements, neutronium should be more compressible due to the absence of electrically charged protons and electrons. This makes neutronium more energetically favorable than (positive-Z) atomic nuclei and leads to their conversion to (degenerate) neutronium through electron capture, a process which is believed to occur in stellar cores in the final seconds of the lifetime of massive stars, where it is facilitated by cooling via ν
e
emission. As a result, degenerate neutronium can have a density of 4×1017 kg/m3,[17] roughly 13 magnitudes denser than the densest known ordinary substances. It was theorized that extreme pressures may deform the neutrons into a cubic symmetry, allowing tighter packing of neutrons,[18] or cause a strange matter formation.

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. According to one analysis, a neutron star with a mass below about 0.2 solar masses will explode.[19]

Noteworthy appearances of neutronium in fiction include the following:

  • In Hal Clement's short story Proof (1942), neutronium is the only form of solid matter known to Solarians, the inhabitants of the Sun's interior.
  • In Vladimir Savchenko's Black Stars (1960), neutronium is a mechanically and thermally indestructible substance. It is also used to make antimatter, which leads to an annihilation accident.
  • In Doctor Who (1963), neutronium is a substance which can shield spaces from time-shear when used as shielding in time-vessels.
  • In Larry Niven's Known Space fictional universe (1964), neutronium is actual neutron star core material, but it is stable in smaller quantities.
  • In the Star Trek universe, neutronium is an extremely hard and durable substance, often used as armor, which conventional weapons cannot penetrate or even dent. The substance is referred to in the storyline dialogue of "The Doomsday Machine", "A Piece of the Action", "Evolution", "Relics", "To the Death", "What You Leave Behind", "Phage", "Prey", and "Think Tank".
  • In Peter F. Hamilton's novel The Neutronium Alchemist (1997), neutronium is created by the "aggressive" setting off of a superweapon.
  • In the Stargate universe, neutronium is a substance which is the basis of the technology of the advanced Asgard race, as well as a primary component of human-form Replicators.
  • In Action Comics #376 (May, 1969), "The Only Way to Kill Superman"[20] has Superman flying into a white dwarf star to grab a couple of handfuls of neutronium to fashion earplugs that will protect his ears from a hypersonic blast. In the panel on page seven, he states that each handful weighs a million tons.

See also

References

  1. ^ "Neutrium: The Most Neutral Hypothetical State of Matter Ever". io9.com. 2012. Retrieved 2013-02-11. 
  2. ^ von Antropoff, A. (1926). "Eine neue Form des periodischen Systems der Elementen" (pdf).  
  3. ^ 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.  
  4. ^ Angelo, J. A. (2006). Encyclopedia of Space and Astronomy.  
  5. ^ Timofeyuk, N. K. (2003). "Do multineutrons exist?".  
  6. ^ Schirber, M. (2012). "Nuclei Emit Paired-up Neutrons". Physics 5: 30.  
  7. ^ Spyrou, A.; Kohley, Z.; Baumann, T.; Bazin, D.; Brown, B. A.; Christian, G.; DeYoung, P. A.; Finck, J. E.; Frank, N.; Lunderberg, E.; Mosby, S.; Peters, W. A.; Schiller, A.; Smith, J. K.; Snyder, J.; Strongman, M. J.; Thoennessen, M.; Volya, A. (2012). "First Observation of Ground State Dineutron Decay: 16Be". Physical Review Letters 108 (10): 102501.  
  8. ^ Bertulani, C. A.; Baur, G. (1986). "Coincidence Cross-sections for the Dissociation of Light Ions in High-energy Collisions" (pdf).  
  9. ^ a b Bertulani, C. A.; Canto, L. F.; Hussein, M. S. (1993). "The Structure And Reactions Of Neutron-Rich Nuclei" (pdf).  
  10. ^ Hagino, K.; Sagawa, H.; Nakamura, T.; Shimoura, S. (2009). "Two-particle correlations in continuum dipole transitions in Borromean nuclei".  
  11. ^ MacDonald, J.; Mullan, D. J. (2009). "Big Bang Nucleosynthesis: The Strong Nuclear Force meets the Weak Anthropic Principle".  
  12. ^ Kneller, J. P.; McLaughlin, G. C. (2004). "The Effect of Bound Dineutrons upon BBN".  
  13. ^ Bertulani, C. A.; Zelevinsky, V. (2002). "Is the tetraneutron a bound dineutron-dineutron molecule?".  
  14. ^ Timofeyuk, N. K. (2002). "On the existence of a bound tetraneutron". arXiv:nucl-th/0203003 [nucl-th].
  15. ^ Bevelacqua, J. J. (1981). "Particle stability of the pentaneutron".  
  16. ^ "Neutrinos give neutron stars a chill". Ars Technica OpenForum. Retrieved 4 December 2013. 
  17. ^ Zarkonnen (2002). "Neutronium". Everything2.com. Retrieved 2013-02-11. 
  18. ^ Felipe J. Llanes-Estrada, Gaspar Moreno Navarro., Felipe J.; Gaspar Moreno Navarro (2011). "Cubic neutrons". arXiv:1108.1859v1 [nucl-th].
  19. ^ K. Sumiyoshi, S. Yamada, H. Suzuki, W. Hillebrandt (21 Jul 1997). "The fate of a neutron star just below the minimum mass: does it explode?". Max-Planck-Institut für Astrophysik, Germany; RIKEN, U. Tokyo, and KEK, Japan.  
  20. ^ Action Comics #376 (May, 1969), "The Only Way to Kill Superman"

Further reading

  • Glendenning, N. K. (2000). Compact Stars: Nuclear Physics, Particle Physics, and General Relativity (2nd ed.).  
This article was sourced from Creative Commons Attribution-ShareAlike License; additional terms may apply. World Heritage Encyclopedia content is assembled from numerous content providers, Open Access Publishing, and in compliance with The Fair Access to Science and Technology Research Act (FASTR), Wikimedia Foundation, Inc., Public Library of Science, The Encyclopedia of Life, Open Book Publishers (OBP), PubMed, U.S. National Library of Medicine, National Center for Biotechnology Information, U.S. National Library of Medicine, National Institutes of Health (NIH), U.S. Department of Health & Human Services, and USA.gov, which sources content from all federal, state, local, tribal, and territorial government publication portals (.gov, .mil, .edu). Funding for USA.gov and content contributors is made possible from the U.S. Congress, E-Government Act of 2002.
 
Crowd sourced content that is contributed to World Heritage Encyclopedia is peer reviewed and edited by our editorial staff to ensure quality scholarly research articles.
 
By using this site, you agree to the Terms of Use and Privacy Policy. World Heritage Encyclopedia™ is a registered trademark of the World Public Library Association, a non-profit organization.
 


Copyright © World Library Foundation. All rights reserved. eBooks from Project Gutenberg are sponsored by the World Library Foundation,
a 501c(4) Member's Support Non-Profit Organization, and is NOT affiliated with any governmental agency or department.