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Neutronium

From Wikipedia, the free encyclopedia
Hypothetical substance in nuclear physics

Neutronium (orneutrium,[1]neutrite,[2] orelement zero) is a hypothetical substance made purely ofneutrons. The word was coined by scientistAndreas von Antropoff in 1926 (before the 1932discovery of the neutron) for the hypothetical "element of atomic number zero" (with no protons in its nucleus) that he placed at the head of theperiodic table (denoted by -).[3][4] However, the meaning of the term haschanged over time, and from the last half of the 20th century onward it has been also used to refer to extremely dense substances resembling theneutron-degenerate matter theorized to exist in the cores ofneutron stars.

In neutron stars

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Main article:Neutron star
Cross-section of neutron star. Here, the core hasneutrons orneutron-degenerate matter andquark matter.

Neutronium is used in popular physics literature[1][2] to refer to the material present in the cores of neutron stars (stars which are too massive to be supported byelectron degeneracy pressure and which collapse into a denser phase of matter). In scientific literature the term "neutron-degenerate matter"[5] or simplyneutron matter is used for this material.[6]

Hypothetical multi-neutrons

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The term "neutronium" was coined in 1926 by Andreas von Antropoff for a conjectured form of matter made up ofneutrons with noprotons orelectrons, which he placed as thechemical element ofatomic number zero at the head of his new version of theperiodic table.[3] It was subsequently placed in the middle of several spiral representations of the periodic system for classifying the chemical elements, such as those ofCharles Janet (1928),Edgar Emerson (1944),[7][8] andJohn D. Clark (1950).

The term is not used in the scientific literature either for a condensed form of matter, or as an element, and theoretical analysis expects no bound forms of neutrons without protons.[9]

Scattering resonances with multiple neutrons

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The dineutron, containing two neutrons, is not a stable bound particle, but an extremely short-lived resonance state produced by nuclear reactions in the decay of beryllium-16. Evidence reported in 2012 for the resonance[10][11] was disputed,[12] but new work reportedly clears up the issues.[13]

The dineutron hypothesis had been used in theoretical studies of the structure ofexotic nuclei. For example11Li is modeled as a dineutron bound to a9Li core.[14][15] A system made up of only two neutrons is not bound, though the attraction between them is very nearly enough to make them so.[16] This has some consequences onnucleosynthesis and theabundance of the chemical elements.[14][17]

A trineutron state consisting of three bound neutrons has not been detected, and is not expected to be bound.[18]

Atetraneutron is a hypothetical particle consisting of four bound neutrons. Reports of its existence have not been replicated.[19][20]

Calculations indicate that the hypothetical pentaneutron state, consisting of a cluster of five neutrons, would not be bound.[21]

See also

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  • Compact star – Classification of very high density object in astronomy

References

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  1. ^abInglis-Arkell, Esther (2012-04-14)."Neutrium: The Most Neutral Hypothetical State of Matter Ever".io9.com.Archived from the original on 2014-11-12. Retrieved2013-02-11.
  2. ^abZhuravleva, Valentina (2005).Ballad of the Stars: Stories of Science Fiction, Ultraimagination, and TRIZ. Technical Innovation Center, Inc. p. 75.ISBN 978-0-9640740-6-4.Archived from the original on 2022-04-12. Retrieved2019-04-25.
  3. ^abvon Antropoff, A. (1926). "Eine neue Form des periodischen Systems der Elementen".Zeitschrift für Angewandte Chemie (in German).39 (23):722–725.Bibcode:1926AngCh..39..722V.doi:10.1002/ange.19260392303.
  4. ^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.S2CID 97131841.
  5. ^Angelo, J. A. (2006).Encyclopedia of Space and Astronomy.Infobase Publishing. p. 178.ISBN 978-0-8160-5330-8.Archived from the original on 2019-12-15. Retrieved2016-10-28.
  6. ^Gandolfi, Stefano; Gezerlis, Alexandros; Carlson, J. (2015-10-19)."Neutron Matter from Low to High Density".Annual Review of Nuclear and Particle Science.65 (1):303–328.arXiv:1501.05675.Bibcode:2015ARNPS..65..303G.doi:10.1146/annurev-nucl-102014-021957.ISSN 0163-8998.
  7. ^Emerson, Edgar I. (1944). "A new spiral form of the periodic table".Journal of Chemical Education.21 (3): 111.Bibcode:1944JChEd..21..111E.doi:10.1021/ed021p111.
  8. ^Emerson, Edgar I. (1944). "A chart based on atomic numbers showing the electronic structure of the elements".Journal of Chemical Education.21 (5): 254.Bibcode:1944JChEd..21..254E.doi:10.1021/ed021p254.
  9. ^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.S2CID 2847145.
  10. ^Schirber, M. (2012). "Nuclei Emit Paired-up Neutrons".Physics.5 30.Bibcode:2012PhyOJ...5...30S.doi:10.1103/Physics.5.30.
  11. ^Spyrou, A.; Kohley, Z.; Baumann, T.; Bazin, D.; et al. (2012)."First Observation of Ground State Dineutron Decay:16Be".Physical Review Letters.108 (10) 102501.Bibcode:2012PhRvL.108j2501S.doi:10.1103/PhysRevLett.108.102501.OSTI 1104191.PMID 22463404.
  12. ^Marqués, F. M., Orr, N. A., Achouri, N. L., Delaunay, F., & Gibelin, J. (2012). Comment on "First Observation of Ground State Dineutron Decay: Be 16". Physical Review Letters, 109(23), 239201.
  13. ^Monteagudo, B.; Marqués, F. M.; Gibelin, J.; Orr, N. A.; Corsi, A.; Kubota, Y.; Casal, J.; Gómez-Camacho, J.; Authelet, G.; Baba, H.; Caesar, C.; Calvet, D.; Delbart, A.; Dozono, M.; Feng, J. (2024-02-23)."Mass, Spectroscopy, and Two-Neutron Decay of $^{16}\mathrm{Be}$"(PDF).Physical Review Letters.132 (8) 082501.doi:10.1103/PhysRevLett.132.082501.OSTI 2473832.PMID 38457706.
  14. ^abBertulani, C. A.; Canto, L. F.; Hussein, M. S. (1993)."The Structure And Reactions Of Neutron-Rich Nuclei"(PDF).Physics Reports.226 (6):281–376.Bibcode:1993PhR...226..281B.doi:10.1016/0370-1573(93)90128-Z. Archived fromthe original(PDF) on 2011-09-28.
  15. ^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.S2CID 119293335.
  16. ^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.S2CID 119203730.
  17. ^Kneller, J. P.;McLaughlin, G. C. (2004). "The Effect of Bound Dineutrons upon BBN".Physical Review D.70 (4): 3512.arXiv:astro-ph/0312388.Bibcode:2004PhRvD..70d3512K.doi:10.1103/PhysRevD.70.043512.S2CID 119060865.
  18. ^Li, J. G.; Michel, N.; Hu, B. S.; Zuo, W.; Xu, F. R. (2019). "Ab initio no-core Gamow shell-model calculations of multineutron systems".Physical Review C.100 (5) 054313.arXiv:1911.06485.Bibcode:2019PhRvC.100e4313L.doi:10.1103/PhysRevC.100.054313.
  19. ^Bertulani, C. A.; Zelevinsky, V. (2003). "Is the tetraneutron a bound dineutron-dineutron molecule?".Journal of Physics G.29 (10):2431–2437.arXiv:nucl-th/0212060.Bibcode:2003JPhG...29.2431B.doi:10.1088/0954-3899/29/10/309.S2CID 55535943.
  20. ^"Tetra-Neutron Experiment: Understanding of Nuclear Forces Might Have To Be Significantly Changed".Archived 2021-12-13 at theWayback Machine. SciTechDaily, December 12, 2021. Technical University of Munich (TUM)
  21. ^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.
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