9,011 research outputs found
Optical absorption for parallel cylinder arrays
We study the long wavelength electromagnetic resonances of interacting
cylinder arrays. By using a normal modes expansion where the effects of
geometry and material are separated, it is shown that two parallel cylinders
with different radii have electromagnetic modes distributed symmetrically about
depolarization factor 1/2. Both sets couple to longitudinal and transverse
components of the external field, but amplitudes of symmetric depolarization
factors become exchanged when considering longitudinal or transverse
polarization. We also find that amplitudes satisfy sum rules that depend on the
ratio of the cylinders radii.Comment: 14 pages, 3 figure
Risk as a First Derivative: Using Intensive Repeated Measures and Molecular Approaches to Studying Families
Outside-in stellar formation in the spiral galaxy M33?
We present and discuss results from chemical evolution models for M33. For
our models we adopt a galactic formation with an inside-out scenario. The
models are built to reproduce three observational constraints of the M33 disk:
the radial distributions of the total baryonic mass, the gas mass, and the O/H
abundance. From observations, we find that the total baryonic mass profile in
M33 has a double exponential behavior, decreasing exponentially for r<= 6 kpc,
and increasing lightly for r > 6 kpc due to the increase of the gas mass
surface density. To adopt a concordant set of stellar and H II regions O/H
values, we had to correct the latter for the effect of temperature variations
and O dust depletion. Our best model shows a good agreement with the observed
the radial distributions of: the SFR, the stellar mass, C/H, N/H, Ne/H, Mg/H,
Si/H, P/H, S/H, Ar/H, Fe/H,and Z. According to our model, the star formation
efficiency is constant in time and space for r <= 6 kpc, but the SFR efficiency
decreases with time and galactocentric distance for r > 6 kpc. The reduction of
the SFR efficiency occurs earlier at higher r. While the galaxy follows the
inside-out formation scenario for all r, the stars follow the inside-out
scenario only up to r = 6 kpc, but for r > 6 kpc the stars follow an outside-in
formation. The stellar formation histories inferred for each r imply that the
average age of the stars for r > 6 increases with r.Comment: Accepted for publication in MNRA
Lagrangian Volume Deformations around Simulated Galaxies
We present a detailed analysis of the local evolution of 206 Lagrangian
Volumes (LVs) selected at high redshift around galaxy seeds, identified in a
large-volume cold dark matter (CDM) hydrodynamical
simulation. The LVs have a mass range of . We
follow the dynamical evolution of the density field inside these initially
spherical LVs from up to , witnessing highly
non-linear, anisotropic mass rearrangements within them, leading to the
emergence of the local cosmic web (CW). These mass arrangements have been
analysed in terms of the reduced inertia tensor , focusing on the
evolution of the principal axes of inertia and their corresponding
eigendirections, and paying particular attention to the times when the
evolution of these two structural elements declines. In addition, mass and
component effects along this process have also been investigated. We have found
that deformations are led by dark matter dynamics and they transform most of
the initially spherical LVs into prolate shapes, i.e. filamentary structures.
An analysis of the individual freezing-out time distributions for shapes and
eigendirections shows that first most of the LVs fix their three axes of
symmetry (like a skeleton) early on, while accretion flows towards them still
continue. Very remarkably, we have found that more massive LVs fix their
skeleton earlier on than less massive ones. We briefly discuss the
astrophysical implications our findings could have, including the galaxy
mass-morphology relation and the effects on the galaxy-galaxy merger parameter
space, among others.Comment: 23 pages, 20 figures. Minor editorial improvement
Variabilidad de la morfología externa de los huevos de Larus cachinnans Pall. (Aves, Laridae) en las Islas Medes (Costa catalana)
The Use of the Military for Law Enforcement Activities in Central America
Faced with the violence, criminality and insecurity now threatening peace and democratic governance in Central America, the region’s governments have decided to use the Armed Forces to carry out actions in response to criminal actions, looking to improve their performance. Although public demand for including the Armed Forces in these functions takes place within a legally legitimate framework, it is motivated by tangible circumstances such as increased levels of violence, delinquency and crime. Despite being coupled with the perception of institutional weakness within the security and judicial system (particularly police) and the recognition of prestige, efficiency, discipline and severity in fulfilling the Armed Forces’ missions, these arguments are insufficient to legitimize the use of the military as a police force.
Within this context, this paper reflects on the implications or consequences of the use of the Armed Forces in duties traditionally assigned to the police in the Central American region with the goal of contributing to the debate on this topic taking place in the Americas. To achieve this end, first we will focus on understanding the actual context in which a decision is made to involve the Armed Forces in security duties in the region. Second, we will examine the effects and implications of this decision on the Armed Forces’ relations within their respective societies. Third and finally, considering this is already a reality in the region, this paper will provide recommendations. The main findings of this research, resulting from the application of an analyticaldescriptive and historically based study, are organized in three dimensions: the political dimension, by implication referring to the relationship between the ultimate political authority and the Armed Forces; the social dimension, by implication the opinion of citizens; and other implications not only affecting the structural and cultural organization of armies and police but also the complementary operational framework within a context of comprehensive response by the State. As a main conclusion, it poses there is an environment conducive to the use of the Armed Forces in citizen’s security, in view of the impact of threats provoked by criminal structures of a military nature currently operating in Central America. However, this participation creates an inevitable social and political impact if implemented in isolation or given a political leading role and/or operational autonomy. This participation poses risks to the institutions of the Armed Forces and the police as well.
Finally, this paper identifies an urgent need for the Armed Forces’ role to be more clearly defined with regard to security matters, limiting it to threats that impact States’ governability and existence. Nonetheless, Central American States should seek a COMPREHENSIVE response to current crime and violence, using all necessary institutions to confront these challenges, but with defined roles and responsibilities for each and dynamic coordination to complement their actions
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