1,820 research outputs found
An Atlas of Monte Carlo Models of Dust Extinction in Galaxies for Cosmological Applications
We present an extensive study of the radiative transfer in dusty galaxies
based on Monte Carlo simulations. The main output of these simulations are the
attenuation curves (i.e. the ratio between the observed,
dust extinguished, total intensity to the intrinsic unextinguished one of the
galaxy as a function of wavelength). We have explored the dependence of on a conspicuous set of quantities (Hubble type, inclination, dust
optical thickness, dust distribution and extinction properties) for a large
wavelength interval, ranging from 1250\AA to the K band, thus finally providing
a comprehensive atlas of dust extinction in galaxies, which is electronically
available. This study is particularly suitable for inclusion into galaxy
formation evolution models and to directly interpret observational data on high
redshift galaxies.Comment: 29 pages, aasms4.sty, LaTeX, 5 figures. ApJSS, accepte
Evidence for SrHo2O4 and SrDy2O4 as model J1-J2 zig-zag chain materials
Neutron diffraction and inelastic spectroscopy is used to characterize the
magnetic Hamiltonian of SrHo2O4 and SrDy2O4. Through a detailed computation of
the crystal-field levels we find site- dependent anisotropic single-ion
magnetism in both materials and diffraction measurements show the presence of
strong one-dimensional spin correlations. Our measurements indicate that
competing interactions of the zig-zag chain, combined with frustrated
interchain interactions, play a crucial role in stabilizing spin-liquid type
correlations in this series.Comment: 5 pages, 5 figure
Un-oriented Quiver Theories for Majorana Neutrons
In the context of un-oriented open string theories, we identify quivers
whereby a Majorana mass for the neutron is indirectly generated by exotic
instantons. We discuss two classes of (Susy) Standard Model like quivers,
depending on the embedding of SU(2)_W in the Chan-Paton group. In both cases,
the main mechanism involves a vector-like pair mixing through a
non-perturbative mass term. We also discuss possible relations between the
phenomenology of Neutron-Antineutron oscillations and LHC physics in these
models. In particular, a vector-like pair of color-triplet scalars or
color-triplet fermions could be directly detected at LHC, compatibly with
n-\bar{n} limits. Finally we briefly comment on Pati-Salam extensions of our
models.Comment: More comments on phenomenology and fluxes, Re-discussion of
SM-quivers compatible with n-cycles conditions Version accepted by JHE
Switching of magnetic domains reveals evidence for spatially inhomogeneous superconductivity
The interplay of magnetic and charge fluctuations can lead to quantum phases
with exceptional electronic properties. A case in point is magnetically-driven
superconductivity, where magnetic correlations fundamentally affect the
underlying symmetry and generate new physical properties. The superconducting
wave-function in most known magnetic superconductors does not break
translational symmetry. However, it has been predicted that modulated triplet
p-wave superconductivity occurs in singlet d-wave superconductors with
spin-density wave (SDW) order. Here we report evidence for the presence of a
spatially inhomogeneous p-wave Cooper pair-density wave (PDW) in CeCoIn5. We
show that the SDW domains can be switched completely by a tiny change of the
magnetic field direction, which is naturally explained by the presence of
triplet superconductivity. Further, the Q-phase emerges in a common
magneto-superconducting quantum critical point. The Q-phase of CeCoIn5 thus
represents an example where spatially modulated superconductivity is associated
with SDW order
From Correlators to Wilson Loops in Chern-Simons Matter Theories
We study n-point correlation functions for chiral primary operators in three
dimensional supersymmetric Chern-Simons matter theories. Our analysis is
carried on in N=2 superspace and covers N=2,3 supersymmetric CFT's, the N=6
ABJM and the N=8 BLG models. In the limit where the positions of adjacent
operators become light-like, we find that the one-loop n-point correlator
divided by its tree level expression coincides with a light-like n-polygon
Wilson loop. Remarkably, the result can be simply expressed as a linear
combination of five dimensional two-mass easy boxes. We manage to evaluate the
integrals analytically and find a vanishing result, in agreement with previous
findings for Wilson loops.Comment: 32 pages, 6 figures, JHEP
The Link Between the Hidden Broad Line Region and the Accretion Rate in Seyfert 2 Galaxies
In the past few years more and more pieces of evidence have been presented
for a revision of the widely accepted Unified Model of Active Galactic Nuclei.
A model based solely on orientation cannot explain all the observed
phenomenology. In the following, we will present evidence that accretion rate
is also a key parameter for the presence of Hidden Broad Line Regions in
Seyfert 2 galaxies. Our sample consists of 21 sources with polarized Hidden
Broad Lines and 18 sources without Hidden Broad Lines. We use stellar velocity
dispersions from several studies on the CaII and Mg b triplets in Seyfert 2
galaxies, to estimate the mass of the central black holes via the
Mbh-{\sigma}\ast relation. The ratio between the bolometric luminosity, derived
from the intrinsic (i.e. unabsorbed) X-ray luminosity, and the Eddington
luminosity is a measure of the rate at which matter accretes onto the central
supermassive black hole. A separation between Compton-thin HBLR and non-HBLR
sources is clear, both in accretion rate (log Lbol/LEdd = -1.9) and in
luminosity (log Lbol = 43.90). When, properly luminosity-corrected,
Compton-thick sources are included, the separation between HBLR and non-HBLR is
less sharp but no HBLR source falls below the Eddington ratio threshold. We
speculate that non-HBLR Compton-thick sources with accretion rate higher than
the threshold, do possess a BLR, but something, probably related to their heavy
absorption, is preventing us from observing it even in polarized light. Our
results for Compton-thin sources support theoretical expectations. In a model
presented by Nicastro (2000), the presence of broad emission lines is
intrinsically connected with disk instabilities occuring in proximity of a
transition radius, which is a function of the accretion rate, becoming smaller
than the innermost stable orbit for very low accretion rates and therefore
luminosities.Comment: 23 pages, 4 figure
Neutron Majorana mass from exotic instantons
We show how a Majorana mass for the Neutron could result from
non-perturbative quantum gravity effects peculiar to string theory. In
particular, "exotic instantons" in un-oriented string compactifications with
D-branes extending the (supersymmetric) standard model could indirectly produce
an effective operator delta{m} n^t n+h.c. In a specific model with an extra
vector-like pair of `quarks', acquiring a large mass proportional to the string
mass scale (exponentially suppressed by a function of the string moduli
fields), delta{m} can turn out to be as low as 10^{-24}-10^{-25} eV. The
induced neutron-antineutron oscillations could take place with a time scale
tau_{n\bar{n}} > 10^8 s, that could be tested by the next generation of
experiments. On the other hand, proton decay and FCNC's are automatically
strongly suppressed and are compatible with the current experimental limits.
Depending on the number of brane intersections, the model may also lead to the
generation of Majorana masses for R-handed neutrini. Our proposal could also
suggest neutron-neutralino or neutron-axino oscillations, with implications in
UCN, Dark Matter Direct Detection, UHECR and Neutron-Antineutron oscillations.
This suggests to improve the limits on neutron-antineutron oscillations, as a
possible test of string theory and quantum gravity.Comment: 35 pages, 11 figures. More comments on neutron-neutralino mixin
One Loop Amplitudes In ABJM
For three dimensional N=6 superconformal field theories we compute one-loop
scattering amplitudes for any number of external particles. We focus on a
particular subsector of N=2 invariant superamplitudes for which the ordinary
perturbative evaluation becomes very easy. The result we obtain is in general
non-vanishing. For six external particles our findings are sufficient for
determining the complete expression of the N=6 superamplitude at this order. We
discuss the symmetries of the result and its anomalous variation under
superconformal generators.Comment: 1+34 pages, 4 figures, references added, published versio
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