228,304 research outputs found
Form Factors Calculated on the Light-Front
A consistent treatment of decay is given on the
light-front. The to transition form factors are calculated in the
entire physical range of momentum transfer for the first time. The
valence-quark contribution is obtained using relativistic light-front wave
functions. Higher quark-antiquark Fock-state of the -meson bound state is
represented effectively by the configuration, and its effect
is calculated in the chiral perturbation theory. Wave function renormalization
is taken into account consistently. The contribution dominates
near the zero-recoil point ( GeV), and decreases rapidly as
the recoil momentum increases. We find that the calculated form factor
follows approximately a dipole -dependence in the entire range
of momentum transfer.Comment: Revtex, 19 pages, 9 figure
Jet conversions in a quark-gluon plasma
Quark and gluon jets traversing through a quark-gluon plasma not only lose
their energies but also can undergo flavor conversions. The conversion rates
via the elastic and the inelastic scatterings are evaluated in the lowest order in QCD.
Including both jet energy loss and conversions in the expanding quark-gluon
plasma produced in relativistic heavy ion collisions, we have found a net
conversion of quark to gluon jets. This reduces the difference between the
nuclear modification factors for quark and gluon jets in central heavy ion
collisions and thus enhances the and ratios at high
transverse momentum. However, a much larger net quark to gluon jet conversion
rate than the one given by the lowest-order QCD is needed to account for the
observed similar ratios in central Au+Au and p+p collisions at same energy.
Implications of our results are discussed.Comment: version to appear in PR
Covalent triazine framework with efficient photocatalytic activity in aqueous and solid media
Radio-mode feedback in local AGNs: dependence on the central black hole parameters
Radio mode feedback, in which most of the energy of an active galactic
nucleus (AGN) is released in a kinetic form via radio-emitting jets, is thought
to play an important role in the maintenance of massive galaxies in the
present-day Universe. We study the link between radio emission and the
properties of the central black hole in a large sample of local radio galaxies
drawn from the Sloan Digital Sky Survey (SDSS), based on the catalogue of Best
and Heckman (2012). Our sample is mainly dominated by massive black holes
(mostly in the range ) accreting at very low Eddington
ratios (typically ). In broad agreement with previously
reported trends, we find that radio galaxies are preferentially associated with
the more massive black holes, and that the radio loudness parameter seems to
increase with decreasing Eddington ratio. We compare our results with previous
studies in the literature, noting potential biases. The majority of the local
radio galaxies in our sample are currently in a radiatively inefficient
accretion regime, where kinetic feedback dominates over radiative feedback. We
discuss possible physical interpretations of the observed trends in the context
of a two-stage feedback process involving a transition in the underlying
accretion modes.Comment: accepted for publication in Monthly Notices of the Royal Astronomical
Societ
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