31,155 research outputs found
Baryon Masses in the 1/N Expansion
The masses of baryons and heavy quark baryons are studied analytically in an
expansion in 1/N, SU(3) flavor symmetry breaking and heavy-quark symmetry
breaking. The measured baryon masses are in striking agreement with the 1/N
hierarchy.Comment: Lattice 2000 (Spectrum
Naturalness of the Coleman-Glashow Mass Relation in the 1/N_c Expansion: an Update
A new measurement of the Xi^0 mass verifies the accuracy of the
Coleman-Glashow relation at the level predicted by the 1/N_c expansion. Values
for other baryon isospin mass splittings are updated, and continue to agree
with the 1/N_c hierarchy.Comment: 6 pages, revte
QCD Baryons in the 1/N_c Expansion
The 1/N_c expansion provides a theoretical method for analyzing the
spin-flavor symmetry properties of baryons in QCD that is quantitative,
systematic and predictive. An exact spin-flavor symmetry exists for large-N_c
baryons, whereas for QCD baryons, the spin-flavor symmetry is approximate and
is broken by corrections proportional to the symmetry-breaking parameter 1/N_c
= 1/3. The 1/N_c expansion predicts a hierarchy of spin and flavor symmetry
relations for QCD baryons that is observed in nature. It provides a
quantitative understanding of why some SU(3) flavor symmetry relations in the
baryon sector, such as the Gell-Mann--Okubo mass formula, are satisfied to a
greater precision than expected from flavor symmetry-breaking suppression
factors alone.Comment: 25 pages, Invited lectures VIII Mexican Workshop on Particles and
Fields, Nov. 14-20, 2001, Zacatecas, Mexico, to be published AIP Proceeding
Baryon Chiral Perturbation Theory in the 1/N Expansion
The chiral Lagrangian for baryons is formulated in an expansion in 1/N_c. The
chiral Lagrangian implements the contracted spin-flavor symmetry of large-N_c
baryons as well as nonet symmetry of the leading planar diagrams. Large-N_c
consistency conditions ensure that chiral loop corrections are suppressed in
1/N_c through exact cancellation of chiral loop graphs to fixed orders in
1/N_c. Application of 1/N_c baryon chiral perturbation theory to the flavor-27
baryon mass splittings and the baryon axial vector currents are considered as
examples.Comment: 10 pages, Invited talk, The Phenomenology of Large-N_c QCD, to be
published Proceedings of the Institute of Nuclear Theor
Bosonic Operator Methods for the Quark Model
Quark model matrix elements can be computed using bosonic operators and the
holomorphic representation for the harmonic oscillator. The technique is
illustrated for normal and exotic baryons for an arbitrary number of colors.
The computations are much simpler than those using conventional quark model
wavefunctions
Spin-Flavor Structure of Large N Baryons
The spin-flavor structure of large N baryons is described in the 1/N
expansion of QCD using quark operators. The complete set of quark operator
identities is obtained, and used to derive an operator reduction rule which
simplifies the 1/N expansion. The operator reduction rule is applied to the
axial currents, masses, magnetic moments and hyperon non-leptonic decay
amplitudes in the limit, to first order in breaking, and
without assuming symmetry. The connection between the Skyrme and quark
representations is discussed. An explicit formula is given for the quark model
operators in terms of the Skyrme model operators to all orders in for
the two flavor case.Comment: 36 pages, 2 eps figures, uses revte
Observations of Interstellar Lyman-alpha Absorption
Interstellar Lyman alpha absorption spectra discrepancies emphasizing neutral hydroge
Observations of the interstellar medium with IUE
Limitations of the International Ultraviolet Explorer (IUE) are discussed, as well as improved powers of research in these areas: (1) Si and C IV doublet absorptions in the high dispersion stellar spectra of distant stars; (2) observation of spectra outside the galactic plans; (3) high velocity gas
Changes in interstellar atomic abundances from the galactic plane to the halo
A few, specially selected interstellar absorption lines were measured in the high resolution, far ultraviolet spectra of 200 O and B type stars observed by the International Ultraviolet Explorer (IUE). For lines of sight extending beyond about 500 pc from the galactic plane, the abundance of singly ionized iron atoms increases relative to singly ionized sulfur. However, the relative abundances of singly ionized sulfur, silicon and aluminum do not seem to change appreciably. An explanation for the apparent increase of iron is the partial sputtering of material off the surfaces of dust grains by interstellar shocks. Another possibility might be that the ejecta from type I supernovae enrich the low density medium in the halo with iron
1/N_c Expansion of the Heavy Baryon Isgur-Wise Functions
The 1/N_c expansion of the heavy baryon Isgur-Wise functions is discussed.
Because of the contracted SU(2N_f) light quark spin-flavor symmetry, the
universality relations among the Isgur-Wise functions of \Lambda_b to \Lambda_c
and \Sigma_b^{(*)} to \Sigma_c^{(*)} are valid up to the order of 1/N_c^2.Comment: 7 pages, latex, no figures, to appear in Phys. Rev.
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