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== Consequences of hypothetical bound tetraneutrons== If, however, the existence of bound tetraneutrons were ever independently confirmed, considerable adjustments would have to be made to current nuclear models. Bertulani and Zelevinsky proposed that, if it existed, the tetraneutron could be formed by a bound state of two [[dineutron]] systems.<ref name="bz03"> {{cite journal | last1 = Bertulani | first1 = C. A. | last2 = Zelevinsky |first2 = V. G. | year = 2003 | title = Tetraneutron as a dineutron-dineutron molecule | journal = [[Journal of Physics G]] | volume = 29 | pages = 2431–2437 | doi = 10.1088/0954-3899/29/10/309 | arxiv= nucl-th/0212060 | bibcode = 2003JPhG...29.2431B | issue = 10 | s2cid = 55535943 }}</ref> However, attempts to model interactions that might give rise to multineutron clusters have failed,<ref name="lazauskas05">{{cite journal | last1 = Lazauskas | first1 = R. | last2 = Carbonell | first2 = J. | year = 2005 | title = Three-neutron resonance trajectories for realistic interaction models | journal = [[Physical Review C]] | volume = 71 | pages = 044004 | doi = 10.1103/PhysRevC.71.044004 | arxiv= nucl-th/0502037v2 | bibcode = 2005PhRvC..71d4004L | issue = 4 | s2cid = 119105439 }}</ref><ref name="arai03">{{cite journal | last = Arai | first = K. | year = 2003 | title = Resonance states of <sup>5</sup>H and <sup>5</sup>Be in a microscopic three-cluster model | journal = [[Physical Review C]] | volume = 68 | issue = 3 | pages = 034303 | doi = 10.1103/PhysRevC.68.034303 |bibcode = 2003PhRvC..68c4303A }}</ref><ref name="hemmdan02">{{cite journal | last1 = Hemmdan | first1 = A. | last2 = Glöckle | first2 = W. | last3 = Kamada | first3= H. | year = 2002 | title = Indications for the nonexistence of three-neutron resonances near the physical region | journal = [[Physical Review C]] | volume = 66 | issue = 3 | pages = 054001 | doi = 10.1103/PhysRevC.66.054001 | arxiv=nucl-th/0208007 | bibcode = 2002PhRvC..66e4001H | s2cid = 11852197 }}</ref> and it "does not seem possible to change modern nuclear Hamiltonians to bind a tetraneutron without destroying many other successful predictions of those Hamiltonians. This means that, should a recent experimental claim of a bound tetraneutron be confirmed, our understanding of nuclear forces will have to be significantly changed."<ref name="pieper03"> {{cite journal | last = Pieper | first = S. C. | year = 2003 | title = Can Modern Nuclear Hamiltonians Tolerate a Bound Tetraneutron? | journal = [[Physical Review Letters]] | volume = 90 | issue = 25 | pages = 252501 | doi = 10.1103/PhysRevLett.90.252501 | arxiv=nucl-th/0302048 | bibcode=2003PhRvL..90y2501P | pmid=12857127 | s2cid = 31164554 }}</ref> Further work<ref name="Arxiv2019">{{cite journal | year = 2019 | title = Tetraneutron condensation in neutron rich matter | last1 = Ivanytskyi | first1 = O. | last2 = Ángeles Pérez-García | first2 = M. | last3 = Albertus | first3 = C. | journal = European Physical Journal A | volume = 55 | issue = 10| pages = 184 | bibcode = 2019EPJA...55..184I | arxiv = 1904.11512 | doi = 10.1140/epja/i2019-12900-6 | doi-access = free }}</ref> in 2019 suggests potentially observable consequences in [[neutron star]] crusts, if the tetraneutron exists.
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