7,295 research outputs found
Coarse-grained Description of Polymer Blends as Interacting Soft-Colloidal Particles
We present a theoretical approach which maps polymer blends onto mixtures of
soft-colloidal particles. The analytical mesoscale pair distribution functions
reproduce well data from united atom molecular dynamics simulations of
polyolefin mixtures without fitting parameters. The theory exactly recovers the
analytical expressions for density and concentration fluctuation structure
factors of soft colloidal mixtures (liquid alloys).Comment: 27 REVTex4 pages, 8 PostScript figures, 1 table accepted for
publication in Journal of Chemical Physic
Explicit generating functional for pions and virtual photons
We construct the explicit one-loop functional of chiral perturbation theory
for two light flavours, including virtual photons. We stick to contributions
where 1 or 2 mesons and at most one photon are running in the loops. With the
explicit functional at hand, the evaluation of the relevant Green functions
boils down to performing traces over the flavour matrices. For illustration, we
work out the pi+ pi- -> pi0 pi0 scattering amplitude at threshold at order p^4,
e^2p^2.Comment: 20 pages, 2 figures; version accepted for publication, minor
typographical changes, acknowledgments adde
Polarisation dependence of magnetic Bragg scattering in YMnO
The polarisation dependence of the intensity of elastic magnetic scattering
from \ymno\ single crystals has been measured at 25 K in magnetic fields
between 1 and 9 T. A significant polarisation dependence was observed in the
intensities of magnetic satellite reflections, propagation vector
\pv=0.5,0,0.25 measured with both the [100] and [010] axes parallel to the
common polarisation and applied field direction. The intensity asymmetries
observed in sets of orthorhombicly equivalent reflections show systematic
relationships which allow the phase relationship between different components
of their magnetic interaction vectors to be determined. They fix the
orientation relationships between the small and moments on the \mnfp\
and \mntp\ sub-lattices and lend support to the structure reported by Kim et
al. It was found that that which suggests
that there is a small modulation of the nuclear structure which has the same
wave-vector as the magnetic modulation leading to a small nuclear structure
factor for the satellite reflections. The differences observed indicate shifts in the atomic positions of order 0.005 \AA
Generating Functional for Strong and Nonleptonic Weak Interactions
The generating functional for Green functions of quark currents is given in
closed form to next-to-leading order in the low-energy expansion for chiral
SU(3), including one-loop amplitudes with up to three meson propagators. Matrix
elements and form factors for strong and nonleptonic weak processes with at
most six external states can be extracted from this functional by performing
three-dimensional flavour traces. To implement this procedure, a Mathematica
program is provided that evaluates amplitudes with at most six external mesons,
photons (real or virtual) and virtual W (semileptonic form factors). The
program is illustrated with several examples that can be compared with existing
calculations.Comment: 26 pages; references added, comparison with other programs added,
small changes in the text, version to appear in JHE
A Radio Perspective on the Wet Merger Remnant NGC 34
We present VLA observations of the neutral hydrogen and radio continuum of
NGC 34 (= NGC 17 = Mrk 938). This object is an ideal candidate to study the
fate of gas in mergers, since, as shown by an optical study done by Schweizer &
Seitzer (2007), it is a gas-rich ("wet") merger remnant of two disk galaxies of
unequal mass hosting a strong central starburst and a weak AGN. We detect HI
emission from both tidal tails and from nearby galaxies, suggesting that NGC 34
is actually part of a gas-rich group and might have recently interacted with
one of its companions. The kinematics of the gas suggests this remnant is
forming an outer disk of neutral hydrogen from the gas of the northern tail. We
also detect broad HI absorption (514 +/- 21 km/s wide) at both negative and
positive velocities with respect to the systemic velocity. This absorption
could be explained by the motions of the tidal tails or by the presence of a
circumnuclear disk. In addition, we present radio-continuum images that show
both nuclear (62.4 +/- 0.3 mJy) and extra-nuclear emission (26.5 +/- 3.0 mJy).
The extra-nuclear component is very diffuse and in the shape of two radio
lobes, spanning 390 kpc overall. This emission could be a signature of an AGN
that has turned off, or it could originate from a starburst-driven superwind.
We discuss the possible scenarios that explain our observations, and what they
tell us about the location of the gas and the future evolution of NGC 34.Comment: 29 pages, 12 figures, 2 tables. Accepted for publication in the
Astronomical Journal. Figs. 1, 2 & 6 degraded to reduce file size
FP-20-17 Women Who Gave Birth Within the Past 12 Months, 2018
The link between marriage and childbearing has become weaker over time (Hayford, Guzzo, & Smock, 2014). In fact, the share of births to unmarried women accounted for almost 40% of all births in 2018 (Martin et al., 2019). Using 2018 American Community Survey (ACS) data, this profile examines the demographic characteristics of currently married and unmarried women aged 15 to 50 who had a birth within the last 12 months. This profile is an update to FP-13-10
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