2,089 research outputs found
X-ray photoelectron spectroscopy studies of non-stoichiometric superconducting NbB2+x
Polycrystalline samples of NbB2+x with nominal composition (B/Nb) = 2.0, 2.1,
2.2, 2.3, 2.4 and 2.5 were studied by X-ray photoelectron spectroscopy (XPS).
The spectra revealed Nb and B oxides on the surface of the samples, mainly B2O3
and Nb2O5. After Ar ion etching the intensity of Nb and B oxides decreased. The
Nb 3d5/2 and B 1s core levels associated with the chemical states (B/Nb) were
identified and they do not change with etching time. The Binding Energy of the
Nb 3d5/2 and B 1s core levels increase as boron content increases, suggesting a
positive chemical shift in the core levels. On the other hand, analysis of
Valence Band spectra showed that the contribution of the Nb 4d states slightly
decreased while the contribution of the B 2p(pi) states increased as the boron
content increased. As a consequence, the electronic and superconducting
properties were substantially modified, in good agreement with band-structure
calculations.Comment: 10 pages, 7 figures, 1 tabl
Supersymmetric classical cosmology
In this work a supersymmetric cosmological model is analyzed in which we
consider a general superfield action of a homogeneous scalar field
supermultiplet interacting with the scale factor in a supersymmetric FRW model.
There appear fermionic superpartners associated with both the scale factor and
the scalar field, and classical equations of motion are obtained from the
super-Wheeler-DeWitt equation through the usual WKB method. The resulting
supersymmetric Einstein-Klein-Gordon equations contain extra radiation and
stiff matter terms, and we study their solutions in flat space for different
scalar field potentials. The solutions are compared to the standard case, in
particular those corresponding to the exponential potential, and their
implications for the dynamics of the early Universe are discussed in turn.Comment: 9 pages, 4 eps figures, uses RevTe
Thermodynamics of noncommutative quantum Kerr black holes
Thermodynamic formalism for rotating black holes, characterized by
noncommutative and quantum corrections, is constructed. From a fundamental
thermodynamic relation, equations of state and thermodynamic response functions
are explicitly given and the effect of noncommutativity and quantum correction
is discussed. It is shown that the well known divergence exhibited in specific
heat is not removed by any of these corrections. However, regions of
thermodynamic stability are affected by noncommutativity, increasing the
available states for which some thermodynamic stability conditions are
satisfied.Comment: 16 pages, 9 figure
Optical spectroscopy of the microquasar GRS 1758-258: a possible intermediate mass system?
Context. GRS 1758-258 is one of two prototypical microquasars towards the
Galactic Center direction discovered almost a quarter of a century ago. The
system remains poorly studied in the optical domain due to its counterpart
being a very faint and absorbed target in a crowded region of the sky. Aims.
Our aim is to investigate GRS 1758-258 in order to shed light on the nature of
the stellar binary components. In particular, the main physical parameters of
the donor star, such as the mass or the spectral type, are not yet well
constrained. Methods. GRS 1758-258 has remained so far elusive to optical
spectroscopy owing to its observational difficulties. Here, we use this
traditional tool of stellar astronomy at low spectral resolution with a 10 m
class telescope and a long slit spectrograph. Results. An improved spectrum is
obtained as compared to previous work. The quality of the data does not allow
the detection of emission or absorption features but, nevertheless, we manage
to partially achieve our aims comparing the de-reddened continuum with the
spectral energy distribution expected from an irradiated disc model and
different donor star templates. Conclusions. We tentatively propose that GRS
1758-258 does not host a giant star companion. Instead, a main sequence star
with mid-A spectral type appears to better agree with our data. The main
impacts of this finding are the possibility that we are dealing with an
intermediate mass system and, in this case, the prediction of an orbital period
significantly shorter than previously proposed.Comment: 5 pages, 6 figures, accepted for publication in A&
Chameleon perfect scalar field as a geometric correction in gravity
In this work, we derive the analytical form for a model that describes
a perfect scalar field by assuming the existence of a chameleon
mechanism. Based on four statements, at the background and perturbative level,
it is possible to relate the extra terms from this theory as a geometrical
perfect fluid term, whose has been expressed as possible candidates to explain
the nature of the dark sector, and possibly, in the case of a perfect scalar
chameleon during inflation, satisfy the big bang nucleosynthesis (BBN)
constraints until late times.Comment: 9 pages. Contribution to "Gravity, Cosmology and Astrophysics - A
Journey of Exploration and Discovery with Female Pioneers". Springer Natur
Detailed study of SNR G306.3-0.9 using XMM-Newton and Chandra observations
We used combined data from XMM-Newton and Chandra observatories to study the
X-ray morphology of SNR G306.3-0.9. A spatially-resolved spectral analysis was
used to obtain physical and geometrical parameters of different regions of the
remnant. Spitzer infrared observations were also used to constrain the
progenitor supernova and study the environment in which the SNR evolved. The
X-ray morphology of the remnant displays a non-uniform structure of
semi-circular appearance, with a bright southwest region and very weak or
almost negligible X-ray emission in its northern part. These results indicate
that the remnant is propagating in a non-uniform environment as the shock
fronts are encountering a high-density medium, where enhanced infrared emission
is detected. The X-ray spectral analysis of the selected regions shows distinct
emission-line features of several metal elements, confirming the thermal origin
of the emission. The X-ray spectra are well represented by a combination of two
absorbed thermal plasma models: one in equilibrium ionization with a mean
temperature of ~0.19 keV, and another out of equilibrium ionization at a higher
temperature of ~1.1 or 1.6-1.9 keV. For regions located in the northeast,
central, and southwest part of the SNR, we found elevated abundances of Si, S,
Ar, Ca, and Fe, typical of ejecta material. The outer regions located northwest
and south show values of the abundances above solar but lower than to those
found in the central regions. This suggests that the composition of the
emitting outer parts of the SNR is a combination of ejecta and shocked material
of the interstellar medium. The comparison between the S/Si, Ar/Si, and Ca/Si
abundances ratios (1.75, 1.27, and 2.72 in the central region, respectively),
favor a Type Ia progenitor for this SNR, a result that is also supported by an
independent morphological analysis using X-ray and IR data.Comment: 8 pages, 7 figures. Accepted by Astronomy and Astrophysic
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