SKA telescopes' sensitivity, field of view and bandwidth will map AGN jet evolution and nearby interstellar scattering screens across large sky fractions via time-domain radio observations.
Sub-femtometer scale color charge correlations in the proton
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
Color charge correlations in the proton at moderately small $x\sim 0.1$ are extracted from its light-cone wave function. The charge fluctuations are far from Gaussian and they exhibit interesting dependence on impact parameter and on the relative transverse momentum (or distance) of the gluon probes. We provide initial conditions for small-$x$ Balitsky-Kovchegov evolution of the dipole scattering amplitude with impact parameter and $\hat r \cdot \hat b$ dependence, and with non-zero $C$-odd component due to three-gluon exchange. Lastly, we compute the (forward) Weizsaecker-Williams gluon distributions, including the distribution of linearly polarized gluons, up to fourth order in $A^+$. The correction due to the quartic correlator provides a transverse momentum scale, $q > 0.5$ GeV, for nearly maximal polarization.
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Time Domain Studies of Active Galactic Nuclei with the SKA telescopes
SKA telescopes' sensitivity, field of view and bandwidth will map AGN jet evolution and nearby interstellar scattering screens across large sky fractions via time-domain radio observations.