6,643 research outputs found
Por la educación hacia la revolución: la contribución de la educación física a la construcción del imaginario social del franquismo
Este breve artículo pretende constituir una contribución a la interpretación y el esclarecimiento del imaginario social del franquismo. Para ello hemos elegido el observatorio de la Educación Física, tanto formal como no formal, y, para los aspectos más concretos, la actuación del Frente de Juventudes, también conocido como la ¿Obra predilecta del Régimen¿. Desde esta óptica, trataremos de evidenciar las intencionalidades ¿formativas¿ subyacentes e implícitas en la concepción y la articulación de la Educación Física masculina del primer franquismo, así como sus potencialidades adoctrinadoras y modeladoras de conciencias
Rare-gas solids under pressure: A path-integral Monte Carlo simulation
Rare-gas solids (Ne, Ar, Kr, and Xe) under hydrostatic pressure up to 30 kbar
have been studied by path-integral Monte Carlo simulations in the
isothermal-isobaric ensemble. Results of these simulations have been compared
with available experimental data and with those obtained from a quasiharmonic
approximation (QHA). This comparison allows us to quantify the overall
anharmonicity of the lattice vibrations and its influence on several structural
and thermodynamic properties of rare-gas solids. The vibrational energy
increases with pressure, but this increase is slower than that of the elastic
energy, which dominates at high pressures. In the PIMC simulations, the
vibrational kinetic energy is found to be larger than the corresponding
potential energy, and the relative difference between both energies decreases
as the applied pressure is raised. The accuracy of the QHA increases for rising
pressure.Comment: 9 pages, 6 figure
Molar volume of solid isotopic helium mixtures
Solid isotopic helium mixtures have been studied by path-integral Monte Carlo
simulations in the isothermal-isobaric ensemble. This method allowed us to
study the molar volume as a function of temperature, pressure, and isotopic
composition. At 25 K and 0.2 GPa, the relative difference between molar volumes
of isotopically-pure crystals of 3He and 4He is found to be about 3%. This
difference decreases under pressure, and for 12 GPa it is smaller than 1%. For
isotopically-mixed crystals, a linear relation between lattice parameters and
concentrations of helium isotopes is found, in agreement with Vegard's law. The
virtual crystal approximation, valid for isotopic mixtures of heavier atoms,
does not give reliable results for solid solutions of helium isotopes.Comment: 7 pages, 5 figure
Spitzer/IRS Mapping of Local Luminous Infrared Galaxies
We present results of our program Spitzer/IRS Mapping of local Luminous
Infrared Galaxies (LIRGs). The maps cover the central 20"x20" or 30"x 30"
regions of the galaxies, and use all four IRS modules to cover the full 5-38
microns spectral range. We have built spectral maps of the main mid-IR emission
lines, continuum and PAH features, and extracted 1D spectra for regions of
interest in each galaxy. The final goal is to fully characterize the mid-IR
properties of local LIRGs as a first step to understanding their more distant
counterparts.Comment: 4 pages, 5 figures. To appear in "Highlights of Spanish Astrophysics
V", Proceedings of the VIII Scientific Meeting of the Spanish Astronomical
Society (SEA) held in Santander, 7-11 July, 200
Solid helium at high pressure: A path-integral Monte Carlo simulation
Solid helium (3He and 4He) in the hcp and fcc phases has been studied by
path-integral Monte Carlo. Simulations were carried out in the
isothermal-isobaric (NPT) ensemble at pressures up to 52 GPa. This allows one
to study the temperature and pressure dependences of isotopic effects on the
crystal volume and vibrational energy in a wide parameter range. The obtained
equation of state at room temperature agrees with available experimental data.
The kinetic energy, E_k, of solid helium is found to be larger than the
vibrational potential energy, E_p. The ratio E_k/E_p amounts to about 1.4 at
low pressures, and decreases as the applied pressure is raised, converging to
1, as in a harmonic solid. Results of these simulations have been compared with
those yielded by previous path integral simulations in the NVT ensemble. The
validity range of earlier approximations is discussed.Comment: 7 pages, 5 figure
Decoupling Properties of MSSM particles in Higgs and Top Decays
We study the supersymmetric (SUSY) QCD radiative corrections, at the one-loop
level, to , and t quark decays, in the context of the Minimal
Supersymmetric Standard Model (MSSM) and in the decoupling limit. The
decoupling behaviour of the various MSSM sectors is analyzed in some special
cases, where some or all of the SUSY mass parameters become large as compared
to the electroweak scale. We show that in the decoupling limit of both large
SUSY mass parameters and large CP-odd Higgs mass, the decay width approaches its Standard Model value at one loop, with the onset
of decoupling being delayed for large values. However, this
decoupling does not occur if just the SUSY mass parameters are taken large. A
similar interesting non-decoupling behaviour, also enhanced by , is
found in the SUSY-QCD corrections to the decay width
at one loop. In contrast, the SUSY-QCD corrections in the
decay width do decouple and this decoupling is fast.Comment: 19 pages, 10 figures. Invited talk presented by M.J.Herrero at the
5th International Symposium on Radiative Corrections (RADCOR 2000) Carmel CA,
USA, 11-15 September, 200
Multi-wavelength Observations of the Giant X-ray Flare Galaxy NGC 5905: signatures of tidal disruption
NGC 5905 is one of the few galaxies with no prior evidence for an AGN in
which an X-ray flare, due to the tidal disruption of a star by the massive
black hole in the center of the galaxy, was detected by the RASS in 1990-91.
Here we present analysis of late-time follow-up observations of NGC 5905 using
Chandra, Spitzer VLA 3 GHz and 8 GHz archival data and GMRT 1.28 GHz radio
observations. The X-ray image shows no compact source that could be associated
with an AGN. Instead, the emission is extended -- likely due to nuclear star
formation and the total measured X-ray luminosity is comparable to the X-ray
luminosity determined from the 2002 Chandra observations. Diffuse X-ray
emission was detected close to the circum-nuclear star forming ring. The
Spitzer 2006 mid-infrared spectrum also shows strong evidence of nuclear star
formation but no clear AGN signatures. The semi-analytical models of Tommasin
et. al. 2010 together with the measured [OIV]/[NeII] line ratio suggest that at
most only 5.6% of the total IR Flux at 19 m is being contributed by the
AGN. The GMRT 1.28 GHz observations reveal a nuclear source. In the much higher
resolution VLA 3 GHz map, the emission has a double lobed structure of size
2.7'' due to the circumnuclear star forming ring. The GMRT 1.28 GHz peak
emission coincides with the center of the circumnuclear ring. We did not detect
any emission in the VLA 8 GHz (1996) archival data. The 3 upper limits
for the radio afterglow of the TDE at 1.28 GHz, 3 GHz and 8 GHz are 0.17 mJy,
0.09 mJy and 0.09 mJy, respectively. Our studies thus show that (i) NGC 5905
has a declining X-ray flux consistent with a TDE, (ii) the IR flux is dominated
by nuclear star formation, (iii) the nuclear radio emission observed from the
galaxy is due to circumnuclear star formation, (iv) no compact radio emission
associated with a radio afterglow from the TDE is detected.Comment: 12 pages, 8 figures, accepted to be published in Astrophysics and
Space Scienc
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