7,091 research outputs found
QCD coherence and jet rates in small x deep inelastic scattering
The contributions to the deep inelastic scattering structure function which
arise from emission of zero, one, two or three resolvable gluons and any number
of unresolvable ones are computed to order . Coherence
effects are taken into account via angular ordering and are demonstrated to
yield (at the leading logarithm level) the identical results to those obtained
assuming the multi-Regge kinematics of BFKL.Comment: 14 pages. Extensively rewritten. To be published in Physics Letters
Cluster and field elliptical galaxies at z~1.3. The marginal role of the environment and the relevance of the galaxy central regions
We compared the properties of 56 elliptical galaxies selected from three
clusters at with those of field galaxies in the GOODS-S (~30),
COSMOS (~180) and CANDELS (~220) fields. We studied the relationships among
effective radius, surface brightness, stellar mass, stellar mass density
and central mass density within 1 kpc radius. We
find that cluster ellipticals do not differ from field ellipticals: they share
the same structural parameters at fixed mass and the same scaling relations. On
the other hand, the population of field ellipticals at shows a
significant lack of massive ( M) and large (R kpc) ellipticals with respect to the cluster. Nonetheless, at
M, the two populations are similar. The size-mass
relation of ellipticals at z~1.3 defines two different regimes, above and below
a transition mass M: at lower masses the
relation is nearly flat (R), the mean radius is
constant at ~1 kpc and while, at larger masses,
the relation is R. The transition mass marks the
mass at which galaxies reach the maximum . Also the
-mass relation follows two different regimes,
, defining a transition mass
density M pc. The mass density
does not correlate with mass, dense/compact galaxies can be
assembled over a wide mass regime, independently of the environment. The
central mass density, , besides to be correlated with the mass,
is correlated to the age of the stellar population: the higher the central
stellar mass density, the higher the mass, the older the age of the stellar
population. [Abridged]Comment: Accepted for publication in A&A; 20 pages, 13 figures (replaced to
match the A&A version
QCD analysis of D-parameter in near-to-planar three-jet events
We present the QCD analysis of D-parameter distribution in near-to-planar
3-jet e+e- annihilation events. We derive the all-order resummed perturbative
prediction and the leading power suppressed non-perturbative corrections both
to the mean value and the distribution. Here non-perturbative corrections are
larger than in 2-jet shape observables, so that higher order non-perturbative
effects could be relevant. Experimental data (not yet available) are needed in
order to cast light on this important point. The technique we develop aims at
improving the accuracy of the theoretical description of multi-jet ensembles,
in particular in hadron-hadron collisions.Comment: 26 pages, 6 figures, JHEP class include
QCD analysis of near-to-planar 3-jet events
Perturbative QCD analysis is presented of the cumulative out-of-plane
momentum distribution in the near-to-planar e+e- annihilation events, K_out <<
Q. In this kinematical region multiple gluon radiation effects become
essential. They are resummed with the single-logarithmic accuracy, which
programme includes the 2-loop treatment of the basic radiation and matching
with the exact O(alpha_s^2) result.
Dedicated experimental analyses of 3-jet event characteristics are of special
interest for the study of the non-perturbative confinement effects.Comment: 32 pages, 1 figure, JHEP class include
Non-perturbative QCD analysis of near-to-planar three-jet events
We present the analysis of the 1/Q-suppressed non-perturbative (NP)
contribution to the cumulative out-of-event-plane momentum distribution in e+e-
annihilation in the near-to-planar three-jet region. It complements our
previous study of the perturbative (PT) distributions resummed to single
logarithmic accuracy. Due to inter-jet soft gluon radiation, the NP
contributions (as well as the PT distributions) are sensitive to the geometry
(the angles between jets) and the colour structure of the underlying hard
process (topology of the three-prong parton antenna). The results and
techniques presented here could be extended to other multi-jet processes and,
in particular, to hadron-hadron collisions.Comment: 53 pages, 4 figures, JHEP class include
Moduli Spaces of Curves with Homology Chains and c=1 Matrix Models
We show that introducing a periodic time coordinate in the models of
Penner-Kontsevich type generalizes the corresponding constructions to the case
of the moduli space of curves with homology chains
\gamma\in H_1(C,\zet_k). We make a minimal extension of the resulting models
by adding a kinetic term, and we get a new matrix model which realizes a simple
dynamics of \zet_k-chains on surfaces. This gives a representation of
matter coupled to two-dimensional quantum gravity with the target space being a
circle of finite radius, as studied by Gross and Klebanov.Comment: IFUM 459/FT (LaTeX, 9 pages; a few misprints have been corrected and
the introduction has been slightly modified
Infrared safe definition of jet flavour
It is common, in both theoretical and experimental studies, to separately
discuss quark and gluon jets. However, even at parton level, widely-used jet
algorithms fail to provide an infrared safe way of making this distinction. We
examine the origin of the problem, and propose a solution in terms of a new
"flavour-kt" algorithm. As well as being of conceptual interest this can be a
powerful tool when combining fixed-order calculations with multi-jet
resummations and parton showers. It also has applications to studies of
heavy-quark jets.Comment: 22 pages, 7 figure
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