41 research outputs found
Anomalous dimension of transverse momentum broadening in planar SYM
The typical transverse momentum (or "saturation" momentum) acquired
by a hard particle propagating through a SYM plasma increases
over time like , with an anomalous exponent
characteristic of super-diffusion. This anomalous exponent is a function of the
't Hooft coupling . Recently, a method has been proposed to
systematically compute the perturbative series of at weak
coupling. This method relies on the traveling wave interpretation of the time
evolution of and on the dominance of soft-collinear radiative
corrections at large times. In this paper, we compute up to
using the double logarithmic behaviour of the BFKL
equation in planar SYM at three loops. This calculation allows
us to discuss the transition towards the strong coupling regime where AdS/CFT
calculations predict .Comment: 8 pages, 1 figure, contribution to the proceedings of the "XVth
International Conference on Quark Confinement and the Hadron Spectrum
Universality aspects of quantum corrections to transverse momentum broadening in QCD media
We study non-linear quantum corrections to transverse momentum broadening
(TMB) of a fast parton propagating in dense QCD matter in the leading
logarithmic approximation. These non-local corrections yield an anomalous
super-diffusive behavior characterized by a heavy tailed distribution which is
associated with L\'{e}vy random walks. Using a formal analogy with the physics
of traveling waves, we show that at late times the transverse momentum
distribution tends to a universal scaling regime. We derive analytic solutions
in terms of an asymptotic expansion around the scaling limit for both fixed and
running coupling. We note that our analytic approach yields a good agreement
with the exact numerical solutions down to realistic values of medium length.
Finally, we discuss the interplay between system size and energy dependence of
the diffusion coefficient and its connection with the gluon
distribution function that is manifest at large transverse momentum transfer.Comment: 57 pages, 15 figure
Towards a cosmological neutrino mass detection
Future cosmological measurements should enable the sum of neutrino masses to
be determined indirectly through their effects on the expansion rate of the
Universe and the clustering of matter. We consider prospects for the
gravitationally lensed Cosmic Microwave Background anisotropies and Baryon
Acoustic Oscillations in the galaxy distribution, examining how the projected
uncertainty of meV on the neutrino mass sum (a 4 detection
of the minimal mass) might be reached over the next decade. The current
1 uncertainty of meV (Planck-2015+BAO-15) will be
improved by upcoming 'Stage-3' CMB experiments (S3+BAO-15: 44 meV), then
upcoming BAO measurements (S3+DESI: 22 meV), and planned next-generation 'Stage
4' CMB experiments (S4+DESI: 15-19 meV, depending on angular range). An
improved optical depth measurement is important: the projected neutrino mass
uncertainty increases to meV if S4 is limited to and combined
with current large-scale polarization data. Looking beyond CDM,
including curvature uncertainty increases the forecast mass error by
50% for S4+DESI, and more than doubles the error with a two-parameter dark
energy equation of state. Complementary low-redshift probes including galaxy
lensing will play a role in distinguishing between massive neutrinos and a
departure from a , flat geometry.Comment: Submitted to PRD. 15 pages, 10 figure
Transverse momentum broadening from NLL BFKL to all orders in pQCD
We study, to all orders in perturbative QCD, the universal behavior of the
saturation momentum controlling the transverse momentum distribution
of a fast parton propagating through a dense QCD medium with large size .
Due to the double logarithmic nature of the quantum evolution of the saturation
momentum, its large asymptotics is obtained by slightly departing from the
double logarithmic limit of either next-to-leading log (NLL) BFKL or leading
order DGLAP evolution equations. At fixed coupling, or in conformal
SYM theory, we derive the large expansion of up to
order . In QCD with massless quarks, where conformal symmetry
is broken by the running of the strong coupling constant, the one-loop QCD
-function fully accounts for the universal terms in the
expansion. Therefore, the universal coefficients of this series are known
exactly to all orders in .Comment: 13 pages, 4 figures, 3 appendice
Anomalous diffusion in QCD matter
We study the effects of quantum corrections on transverse momentum broadening
of a fast parton passing through dense QCD matter. We show that, at leading
logarithmic accuracy the broadening distribution tends at late times or
equivalently for large system sizes to a universal distribution that only
depends on a single scaling variable where the typical
transverse momentum scale increases with time as up to non-universal terms, with an
anomalous dimension . This property is analogous
to geometric scaling of gluon distributions in the saturation regime and
traveling waves solutions to reaction-diffusion processes. We note that since
the process is super-diffusive, which is also reflected at large
transverse momentum where the scaling distribution exhibits a heavy tail
akin to L\'{e}vy random walks.Comment: 10 pages, 3 figures, 3 supplemental material
Anomalous dimension of transverse momentum broadening in planar = 4 SYM
The typical transverse momentum Qs(t) (or "saturation" momentum) acquired by a hard particle propagating through a N = 4 SYM plasma increases over time like tγ, with an anomalous exponent γ > 1/2 characteristic of super-diffusion. This anomalous exponent is a function of the ’t Hooft coupling λ = g2Nc. Recently, a method has been proposed to systematically compute the perturbative series of γ(λ) at weak coupling. This method relies on the traveling wave interpretation of the time evolution of Qs(t) and on the dominance of softcollinear radiative corrections at large times. In this paper, we compute γ(λ) up to (λ2) using the double logarithmic behaviour of the BFKL equation in planar = 4 SYM at three loops. This calculation allows us to discuss the transition towards the strong coupling regime where AdS/CFT calculations predict γ→1
Back-to-back inclusive dijets in DIS at small : Complete NLO results and predictions
We compute the back-to-back dijet cross-section in deep inelastic scattering
(DIS) at small to next-to-leading order (NLO) in the Color Glass Condensate
effective field theory. Our result can be factorized into a convolution of the
Weizs\"{a}cker-Williams gluon transverse momentum dependent distribution
function (WW gluon TMD) with a universal soft factor and an NLO coefficient
function. The soft factor includes both double and single logarithms in the
ratio of the relative transverse momentum of the dijet pair to the
dijet momentum imbalance ; its renormalization group (RG) evolution is
resummed into the Sudakov factor. Likewise, the WW TMD obeys a nonlinear RG
equation in that is kinematically constrained to satisfy both lifetime and
rapidity ordering of the projectile. Exact analytical expressions are obtained
for the NLO coefficient function of transversely and longitudinally polarized
photons. Our results allow for the first quantitative separation of the
dynamics of Sudakov suppression from that of gluon saturation. They can be
extended to other final states and provide a framework for precision tests of
novel QCD many-body dynamics at the Electron-Ion Collider.Comment: 41 pages, 9 figures, 5 supplemental materials, to be published in
Physical Review Letter
Cold gas and a Milky Way-type 2175 {\AA} bump in a metal-rich and highly depleted absorption system
We report the detection of a strong Milky Way-type 2175 \AA extinction
bump at = 2.1166 in the quasar spectrum towards SDSS J121143.42+083349.7
from the Sloan Digital Sky Survey (SDSS) Data Release 10. We conduct follow up
observations with the Echelle Spectrograph and Imager (ESI) onboard the Keck-II
telescope and the Ultraviolet and Visual Echelle Spectrograph (UVES) on the
VLT. This 2175 \AA absorber is remarkable in that we simultaneously detect
neutral carbon (C I), neutral chlorine (Cl I), and carbon monoxide (CO). It
also qualifies as a damped Lyman alpha system. The J1211+0833 absorber is found
to be metal-rich and has a dust depletion pattern resembling that of the Milky
Way disk clouds. We use the column densities of the C I fine structure states
and the C II/C I ratio (under the assumption of ionization equilibrium) to
derive the temperature and volume density in the absorbing gas. A Cloudy
photoionization model is constructed, which utilizes additional atoms/ions to
constrain the physical conditions. The inferred physical conditions are
consistent with a canonical cold (T 100 K) neutral medium with a high
density ((H I) 100 cm) and a slightly higher pressure than the
local interstellar medium. Given the simultaneous presence of C I, CO, and the
2175 \AA bump, combined with the high metallicity, high dust depletion level
and overall low ionization state of the gas, the absorber towards J1211+0833
supports the scenario that the presence of the bump requires an evolved stellar
population.Comment: 18 pages, 17 figures, to be published in MNRA
Anomalous dimension of transverse momentum broadening in planar SYM
International audienceThe typical transverse momentum (or "saturation" momentum) acquired by a hard particle propagating through a SYM plasma increases over time like , with an anomalous exponent characteristic of super-diffusion. This anomalous exponent is a function of the 't Hooft coupling . Recently, a method has been proposed to systematically compute the perturbative series of at weak coupling. This method relies on the traveling wave interpretation of the time evolution of and on the dominance of soft-collinear radiative corrections at large times. In this paper, we compute up to using the double logarithmic behaviour of the BFKL equation in planar SYM at three loops. This calculation allows us to discuss the transition towards the strong coupling regime where AdS/CFT calculations predict