782 research outputs found
Parton Distributions in Impact Parameter Space
Fourier transform of the generalized parton distributions (GPDs) at zero
skewness with respect to the transverse momentum transfer gives the
distribution of partons in the impact parameter space. We investigate the GPDs
as well as the impact parameter dependent parton distributions (ipdpdfs) by
expressing them in terms of overlaps of light front wave functions (LFWFs) and
present a comparative study using three different model LFWFs.Comment: 13 pages, 6 figure
Magnetic moments of the low-lying , resonances within the framework of the chiral quark model
The magnetic moments of the low-lying spin-parity ,
resonances, like, for example, ,
, as well as their transition magnetic moments, are
calculated using the chiral quark model. The results found are compared with
those obtained from the nonrelativistic quark model and those of unitary chiral
theories, where some of these states are generated through the dynamics of two
hadron coupled channels and their unitarization
Extracting the Omega- electric quadrupole moment from lattice QCD data
The Omega- has an extremely long lifetime, and is the most stable of the
baryons with spin 3/2. Therefore the Omega- magnetic moment is very accurately
known. Nevertheless, its electric quadrupole moment was never measured,
although estimates exist in different formalisms. In principle, lattice QCD
simulations provide at present the most appropriate way to estimate the Omega-
form factors, as function of the square of the transferred four-momentum, Q2,
since it describes baryon systems at the physical mass for the strange quark.
However, lattice QCD form factors, and in particular GE2, are determined at
finite Q2 only, and the extraction of the electric quadrupole moment, Q_Omega=
GE2(0) e/(2 M_Omega), involves an extrapolation of the numerical lattice
results. In this work we reproduce the lattice QCD data with a covariant
spectator quark model for Omega- which includes a mixture of S and two D states
for the relative quark-diquark motion. Once the model is calibrated, it is used
to determine Q_Omega. Our prediction is Q_Omega= (0.96 +/- 0.02)*10^(-2) efm2
[GE2(0)=0.680 +/- 0.012].Comment: To appear in Phys. Rev. D. Version with small modifications. 8 pages,
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