195 research outputs found
Ariel - Volume 5 Number 4
Editors
Mark Dembert
J.D. Kanofskv
Entertainment Editors
Robert Breckenridge
Joe Conti
Overseas Editor
Mike Sinason
Photographer
Scott Kastner
Epistemologist
Gary Kaskey
Staff
Ken Jaffe
Bob Sklaroff
Janet Weish
David Jacoby
Phil Nimoityn
Circulation Editor
Jay Amsterdam
Humorist
Jim Mccan
Ariel - Volume 6 Number 3
Editors
Mark Dembert
J.D. Kanofsky
Frank Chervenak
John Lammie
Curt Cummings
Staff
Ken Jaffe
Bob Sklaroff
Halley Faust
Jim Burke
Nancy Redfern
Hans Weltin
Photographer
Larry Glazerman
Overseas Editor
Mike Sinason
Humorist
Jim McCan
Large stellar disks in small elliptical galaxies
We present the rotation velocities V and velocity dispersions sigma along the
principal axes of seven elliptical galaxies less luminous than M_B= -19.5.
These kinematics extend beyond the half-light radii for all systems in this
photometrically selected sample. At large radii the kinematics not only confirm
that rotation and "diskiness" are important in faint ellipticals, as was
previously known, but also demonstrate that in most sample galaxies the stars
at large galactocentric distances have (V/sigma)_max of about 2, similar to the
disks in bona-fide S0 galaxies. Comparing this high degree of ordered stellar
motion in all sample galaxies with numerical simulations of dissipationless
mergers argues against mergers with mass ratios <=3:1 as an important mechanism
in the final shaping of low-luminosity ellipticals, and favors instead the
dissipative formation of a disk.Comment: 11 pages LaTex with 4 Postscript figure
More on the Burkhardt-Cottingham Sum Rule in QCD
The QCD higher order effects to the polarized structure function are reanalyzed for massive quarks in the context of the operator product
expansion. We confirm that the lowest moment of which
corresponds to the Burkhardt-Cottingham sum rule does {\sl not} suffer from
radiative corrections in perturbative QCD.Comment: LaTeX, 9 pages, 1 figure appended after \end{document} as an
uu-encoded and compressed .ps file, KUCP-70;HUPD-9410;YNU-HEPTh-94-10
Ariel - Volume 6 Number 4
Editors
Mark Dembert
J.D. Kanofsky
Frank Chervenak
John Lammie
Curt Cummings
Entertainment
Robert Breckenridge
Joe Conti
Gary Kaskey
Photographer
Larry Glazerman
Overseas Editor
Mike Sinason
Humorist
Jim McCann
Staff
Ken Jaffe
Bob Sklaroff
Halley Faust
Jim Burk
Ariel - Volume 6 Number 4 (Alternate Version)
Editors
Mark Dembert
J.D. Kanofsky
Frank Chervenak
John Lammie
Curt Cummings
Entertainment
Robert Breckenridge
Joe Conti
Gary Kaskey
Photographer
Larry Glazerman
Overseas Editor
Mike Sinason
Humorist
Jim McCann
Staff
Kenn Jaffe
Bob Sklaroff
Halley Faust
Jim Burke
Jay Amsterdam
Morton A. Klein
Nancy Redfer
Vegetation history and climatic fluctuations on a transect along the Dead Sea west shore and impact on past societies over the last 3500 years.
This study represents the vegetation history of the last 3500 years and conducts an analysis of the climatic fluctuations on a 75 km long transect on the western Dead Sea shore. Palynological and sedimentological data are available from six cores near Mount Sedom, Ein Boqueq, and Ein Gedi and from outcrops near Ze'elim and Ein Feshkha. The comparison of the pollen data with the lake levels shows synchronous trends. During the Middle Bronze Age, Iron Age and Hellenistic to Byzantine Period the high lake level of the Dead Sea signals an increase in precipitation. Contemporaneously, values of cultivated plants indicate an increase in agriculture. Lake level is low during the Late Bronze Age, within the Iron Age and at the end of the Byzantine period, indicating dry periods when all pds show a decrease of cultivated plants. Forest regeneration led by drought-resistant pines is observed in all pollen diagrams (pds) following the agricultural decline in the Byzantine period and, in the pds near Ein Boqeq, Ze'elim and Ein Feshkha, during the late Iron Age. The modern vegetation gradient is reflected in the palaeo-records: a stronger expansion of Mediterranean vegetation and cultivated plants in the northern sites is recognisable
Target Mass Effects in Polarized Virtual Photon Structure Functions
We study target mass effects in the polarized virtual photon structure
functions , in the kinematic
region , where is the mass squared of
the probe (target) photon. We obtain the expressions for and in closed form by inverting the
Nachtmann moments for the twist-2 and twist-3 operators. Numerical analysis
shows that target mass effects appear at large and become sizable near
, the maximal value of , as the ratio
increases. Target mass effects for the sum rules of and
are also discussed.Comment: 24 pages, LaTeX, 9 eps figure
Polarized Virtual Photon Structure Function and Twist-3 Effects in QCD
We investigate the twist-3 effects in the polarized virtual photon structure.
The structure functions and of polarized photon could
be experimentally studied in the future polarized or colliders.
The leading contributions to are the twist-2 effects, while
another structure function , which only exists for the virtual
photon target, receives not only the twist-2 but also twist-3 contributions. We
first show that the twist-3 effects actually exist in the box-diagram
contributions and we extract the twist-3 part, which can also be reproduced by
the pure QED operator product expansion. We then calculate the non-trivial
lowest moment () of the twist-3 contribution to in QCD. For
large (the number of colors), the QCD analysis of the twist-3 effects in
the flavor nonsinglet part of becomes tractable and we can obtain
its moments in a compact form for all .Comment: 27 pages, LaTeX, 9 eps figures, eqsection.sty file included, Appendix
A added, some minor changes for Fig.
Spin Structure Function g_2(x,Q^2) and Twist-3 Operators in large-N_C QCD
It is shown in the framework of the operator product expansion and the
renormalization group method that the twist-3 part of flavour nonsinglet spin
structure function g_2(x,Q^2) obeys a simple Dokshitzer-Gribov-
Lipatov-Altarelli-Parisi (DGLAP) equation in the large N_C limit even in the
case of massive quarks (N_C is the number of colours). There are four different
types of twist-3 operators which contribute to g_2, including
quark-mass-dependent operators and the ones proportional to the equation of
motion. They are not all independent but are constrained by one relation. A new
choice of the independent operator bases leads to a simple form of the
evolution equation for g_2 at large N_C.Comment: Corrected Ref.[15
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