Chiral symmetry breaking and the quark model: Unification of baryon and meson constraints

We review the subject of chiral symmetry breaking and its connection with the quark model. When the light plane SU(3) charges and quark field density matrix elements are transformed back to the usual static basis it becomes clear that expectation values of chiral breaking operators, such as qλ iq ,...

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Published inNuclear physics. B Vol. 123; no. 3; pp. 445 - 492
Main Authors Gunion, J.F., McNamee, P.C., Scadron, M.D.
Format Journal Article
LanguageEnglish
Published United States Elsevier B.V 01.01.1977
Online AccessGet full text
ISSN0550-3213
1873-1562
DOI10.1016/0550-3213(77)90176-6

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Abstract We review the subject of chiral symmetry breaking and its connection with the quark model. When the light plane SU(3) charges and quark field density matrix elements are transformed back to the usual static basis it becomes clear that expectation values of chiral breaking operators, such as qλ iq , do not necessarily have simple SU(3) transformation properties. Starting with the standard current quark chiral Hamiltonian H′ = m u uu + m d dd + m s ss , we then use current quark light-cone distribution function concepts in combination with constraints from (i) Compton amplitude fixed poles, (ii) baryon octet and decuplet mass differences, (iii) πN and KN σ terms, (iv) G A/ G V, (v) low-energy π photoproduction multipoles, (vi) Goldberger-Treiman discrepancies, (vii) meson mass ratios in PCAC and, (viii) meson mass differences to determine m ̂ = 1 2 (m u + m d) and m s in more than four independent ways. Our results are all mutually consistent and yield the values m ̂ ≈ m π and m s/ m ̂ ≈ 5 . In particular the independent baryon and meson sectors of the theory are completely compatible.
AbstractList We review the subject of chiral symmetry breaking and its connection with the quark model. When the light plane SU(3) charges and quark field density matrix elements are transformed back to the usual static basis it becomes clear that expectation values of chiral breaking operators, such as qλ iq , do not necessarily have simple SU(3) transformation properties. Starting with the standard current quark chiral Hamiltonian H′ = m u uu + m d dd + m s ss , we then use current quark light-cone distribution function concepts in combination with constraints from (i) Compton amplitude fixed poles, (ii) baryon octet and decuplet mass differences, (iii) πN and KN σ terms, (iv) G A/ G V, (v) low-energy π photoproduction multipoles, (vi) Goldberger-Treiman discrepancies, (vii) meson mass ratios in PCAC and, (viii) meson mass differences to determine m ̂ = 1 2 (m u + m d) and m s in more than four independent ways. Our results are all mutually consistent and yield the values m ̂ ≈ m π and m s/ m ̂ ≈ 5 . In particular the independent baryon and meson sectors of the theory are completely compatible.
Author Gunion, J.F.
Scadron, M.D.
McNamee, P.C.
Author_xml – sequence: 1
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– sequence: 2
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  surname: McNamee
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  givenname: M.D.
  surname: Scadron
  fullname: Scadron, M.D.
BackLink https://www.osti.gov/servlets/purl/1446336$$D View this record in Osti.gov
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Coleman (10.1016/0550-3213(77)90176-6_BIB80) 1964; 134
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Brodsky (10.1016/0550-3213(77)90176-6_BIB11_1) 1972; D5
Carruthers (10.1016/0550-3213(77)90176-6_BIB17_2) 1971; 27
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Olsson (10.1016/0550-3213(77)90176-6_BIB41_2) 1975; B101
Chodos (10.1016/0550-3213(77)90176-6_BIB52_1) 1974; D9
Golowich (10.1016/0550-3213(77)90176-6_BIB53) 1975; 12
Riazuddin (10.1016/0550-3213(77)90176-6_BIB71_1) 1971; 27
Adler (10.1016/0550-3213(77)90176-6_BIB77) 1969; 177
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Gilman (10.1016/0550-3213(77)90176-6_BIB26_3) 1974; D9
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Snippet We review the subject of chiral symmetry breaking and its connection with the quark model. When the light plane SU(3) charges and quark field density matrix...
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Title Chiral symmetry breaking and the quark model: Unification of baryon and meson constraints
URI https://dx.doi.org/10.1016/0550-3213(77)90176-6
https://www.osti.gov/servlets/purl/1446336
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