26 research outputs found
Rescattering corrections and self-consistent metric in Planckian scattering
Starting from the ACV approach to transplanckian scattering, we present a
development of the reduced-action model in which the (improved) eikonal
representation is able to describe particles' motion at large scattering angle
and, furthermore, UV-safe (regular) rescattering solutions are found and
incorporated in the metric. The resulting particles' shock-waves undergo
calculable trajectory shifts and time delays during the scattering process ---
which turns out to be consistently described by both action and metric, up to
relative order in the gravitational radius over impact parameter
expansion. Some suggestions about the role and the (re)scattering properties of
irregular solutions --- not fully investigated here --- are also presented.Comment: 39 pages, 14 figure
The NLO jet vertex in the small-cone approximation for kt and cone algorithms
We determine the jet vertex for Mueller-Navelet jets and forward jets in the
small-cone approximation for two particular choices of jet algoritms: the kt
algorithm and the cone algorithm. These choices are motivated by the extensive
use of such algorithms in the phenomenology of jets. The differences with the
original calculations of the small-cone jet vertex by Ivanov and Papa, which is
found to be equivalent to a formerly algorithm proposed by Furman, are shown at
both analytic and numerical level, and turn out to be sizeable. A detailed
numerical study of the error introduced by the small-cone approximation is also
presented, for various observables of phenomenological interest. For values of
the jet "radius" R=0.5, the use of the small-cone approximation amounts to an
error of about 5% at the level of cross section, while it reduces to less than
2% for ratios of distributions such as those involved in the measure of the
azimuthal decorrelation of dijets.Comment: 22 pages, 7 figures, 13 eps file
Emerging Hawking-like Radiation from Gravitational Bremsstrahlung Beyond the Planck Scale
We argue that, as a consequence of the graviton's spin-2, its bremsstrahlung
in trans-planckian-energy () gravitational scattering at small
deflection angle can be nicely expressed in terms of helicity-transformation
phases and their transfer within the scattering process. The resulting spectrum
exhibits deeply sub-planckian characteristic energies of order (reminiscent of Hawking radiation), a suppressed fragmentation region, and
a reduced rapidity plateau, in broad agreement with recent classical estimates.Comment: 5 pages, 3 figures. Comments and references added. Typos corrected.
Fig. 3 modified. Title modified. Same as published articl
On factorisation at small x
We investigate factorisation at small x using a variety of analytical and
numerical techniques. Previous results on factorisation in collinear models are
generalised to the case of the full BFKL equation, and illustrated in the
example of a collinear model which includes higher twist terms. Unlike the
simplest collinear model, the BFKL equation leads to effective anomalous
dimensions containing higher-twist pieces which grow as a (non-perturbative)
power at small x. While these pieces dominate the effective splitting function
at very small x they do not lead to a break-down of factorisation insofar as
their effect on the predicted scaling violations remains strongly suppressed.Comment: 17 pages, LaTeX. Updated version corrects some small misprints and
adds extra preprint number
Unified limiting form of graviton radiation at extreme energies
We derive the limiting form of graviton radiation in gravitational scattering
at transplanckian energies () and small deflection angles. We show
that --- owing to the graviton's spin 2 --- such limiting form unifies the
soft- and Regge- regimes of emission, by covering a broad angular range, from
forward fragmentation to deeply central region. The single-exchange emission
amplitudes have a nice expression in terms of the transformation phases of
helicity amplitudes under rotations. As a result, the multiple-exchange
emission amplitudes can be resummed via an impact parameter -space
factorization theorem that takes into account all coherence effects. We then
see the emergence of an energy spectrum of the emitted radiation which, being
tuned on , is reminiscent of Hawking's radiation.
Such a spectrum is much softer than the one na\"ively expected for increasing
input energies and neatly solves a potential energy crisis. Furthermore, by
including rescattering corrections in the (quantum) factorization formula, we
are able to recover the classical limit and to find the corresponding quantum
corrections. Perspectives for the extrapolation of such limiting radiation
towards the classical collapse regime (where is of the order of the
gravitational radius ) are also discussed.Comment: 45 pages, 15 figures, new result, some corrections and additional
comment