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In
nuclear physics Nuclear physics is the field of physics that studies atomic nuclei and their constituents and interactions, in addition to the study of other forms of nuclear matter. Nuclear physics should not be confused with atomic physics, which studies t ...
, an
atomic nucleus The atomic nucleus is the small, dense region consisting of protons and neutrons at the center of an atom, discovered in 1911 by Ernest Rutherford based on the 1909 Geiger–Marsden gold foil experiment. After the discovery of the neutron ...
is called a halo nucleus or is said to have a nuclear halo when it has a core nucleus surrounded by a "halo" of orbiting protons or neutrons, which makes the radius of the nucleus appreciably larger than that predicted by the
liquid drop model In nuclear physics, the semi-empirical mass formula (SEMF) (sometimes also called the Weizsäcker formula, Bethe–Weizsäcker formula, or Bethe–Weizsäcker mass formula to distinguish it from the Bethe–Weizsäcker process) is used to approxi ...
. Halo nuclei form at the extreme edges of the
table of nuclides A table or chart of nuclides is a two-dimensional Cartesian coordinate system, graph of isotopes of the elements, in which one axis represents the number of neutrons (symbol ''N'') and the other represents the number of protons (atomic number, sy ...
— the
neutron drip line The nuclear drip line is the boundary beyond which atomic nuclei decay by the emission of a proton or neutron. An arbitrary combination of protons and neutrons does not necessarily yield a stable nucleus. One can think of moving up and/or to ...
and proton drip line — and have short half-lives, measured in milliseconds. These nuclei are studied shortly after their formation in an
ion beam An ion beam is a type of charged particle beam consisting of ions. Ion beams have many uses in electronics manufacturing (principally ion implantation) and other industries. A variety of ion beam sources exists, some derived from the mercu ...
. Typically, an atomic nucleus is a tightly bound group of protons and neutrons. However, in some nuclides, there is an overabundance of one species of nucleon. In some of these cases, a nuclear core and a halo will form. Often, this property may be detected in scattering experiments, which show the nucleus to be much larger than the otherwise expected value. Normally, the cross-section (corresponding to the classical radius) of the nucleus is proportional to the cube root of its mass, as would be the case for a sphere of constant density. Specifically, for a nucleus of
mass number The mass number (symbol ''A'', from the German word ''Atomgewicht'' tomic weight, also called atomic mass number or nucleon number, is the total number of protons and neutrons (together known as nucleons) in an atomic nucleus. It is approxima ...
''A'', the radius ''r'' is (approximately) :r = r_\circ A^, where r_\circ is 1.2 fm. One example of a halo nucleus is 11 Li, which has a half-life of 8.6 ms. It contains a core of 3 protons and 6 neutrons, and a halo of two independent and loosely bound neutrons. It decays into 11 Be by the emission of an antineutrino and an electron. Its mass radius of 3.16 fm is close to that of 32 S or, even more impressively, of 208 Pb, both much heavier nuclei. Experimental confirmation of nuclear halos is recent and ongoing. Additional candidates are suspected. Several nuclides including 9B, 13N, and 15N are calculated to have a halo in the
excited state In quantum mechanics, an excited state of a system (such as an atom, molecule or nucleus) is any quantum state of the system that has a higher energy than the ground state (that is, more energy than the absolute minimum). Excitation refers to ...
but not in the
ground state The ground state of a quantum-mechanical system is its stationary state of lowest energy; the energy of the ground state is known as the zero-point energy of the system. An excited state is any state with energy greater than the ground state. ...
.


List of known nuclides with nuclear halo

Nuclei that have a neutron halo include 11 Be and 19 C. A two-neutron halo is exhibited by 6 He, 11 Li, 17 B, 19 B and 22 C. Two-neutron halo nuclei break into three fragments and are called Borromean because of this behavior, analogously to how all three of the
Borromean rings In mathematics, the Borromean rings are three simple closed curves in three-dimensional space that are topologically linked and cannot be separated from each other, but that break apart into two unknotted and unlinked loops when any one of the t ...
are linked together but no two share a link. For example, the two-neutron halo nucleus 6He (which can be taken as a three-body system consisting of an alpha particle and two neutrons) is bound, but neither 5He nor the
dineutron Neutronium (sometimes shortened to neutrium, also referred to as neutrite) is a hypothetical substance composed purely of neutrons. The word was coined by scientist Andreas von Antropoff in 1926 (before the 1932 discovery of the neutron) for the ...
is. 8 He and 14 Be both exhibit a four-neutron halo. Nuclei that have a proton halo include 8 B and 26 P. A two-proton halo is exhibited by 17 Ne and 27 S. Proton halos are expected to be rarer and more unstable than neutron halos because of the repulsive forces of the excess proton(s).


See also

* Halo nuclei and nuclear force range limits *
Isotopes of lithium Naturally occurring lithium (3Li) is composed of two stable isotopes, lithium-6 and lithium-7, with the latter being far more abundant on Earth. Both of the natural isotopes have an unexpectedly low nuclear binding energy per nucleon ( for lit ...
*
Lithium Lithium (from el, λίθος, lithos, lit=stone) is a chemical element with the symbol Li and atomic number 3. It is a soft, silvery-white alkali metal. Under standard conditions, it is the least dense metal and the least dense soli ...


References


Further reading

* * *{{cite journal , arxiv=nucl-ex/0111001 , doi=10.1103/PhysRevC.65.044006 , title=Detection of neutron clusters , year=2002 , last1=Marqués , first1=F. M. , last2=Labiche , first2=M. , last3=Orr , first3=N. A. , last4=Angélique , first4=J. C. , last5=Axelsson , first5=L. , last6=Benoit , first6=B. , last7=Bergmann , first7=U. C. , last8=Borge , first8=M. J. G. , last9=Catford , first9=W. N. , last10=Chappell , first10=S. P. G. , last11=Clarke , first11=N. M. , last12=Costa , first12=G. , last13=Curtis , first13=N. , last14=d'Arrigo , first14=A. , last15=De Góes Brennand , first15=E. , last16=De Oliveira Santos , first16=F. , last17=Dorvaux , first17=O. , last18=Fazio , first18=G. , last19=Freer , first19=M. , last20=Fulton , first20=B. R. , last21=Giardina , first21=G. , last22=Grévy , first22=S. , last23=Guillemaud-Mueller , first23=D. , last24=Hanappe , first24=F. , last25=Heusch , first25=B. , last26=Jonson , first26=B. , last27=Le Brun , first27=C. , last28=Leenhardt , first28=S. , last29=Lewitowicz , first29=M. , last30=López , first30=M. J. , s2cid=37431352 , journal=Physical Review C , volume=65 , issue=4 , page=044006 , bibcode=2002PhRvC..65d4006M , display-authors=29 Nuclear physics