24,142 research outputs found
Gamma-Ray Spectral Characteristics of Thermal and Non-Thermal Emission from Three Black Holes
Cygnus X-1 and the gamma-ray transients GROJ0422+32 and GROJ1719-24 displayed
similar spectral properties when they underwent transitions between the high
and low gamma-ray (30 keV to few MeV) intensity states. When these sources were
in the high gamma-ray intensity state (gamma-2, for Cygnus X-1), their spectra
featured two components: a Comptonized shape below 200-300 keV with a soft
power-law tail (photon index >3) that extended to ~1 MeV or beyond. When the
sources were in the low-intensity state (gamma-0, for Cygnus X-1), the
Comptonized spectral shape below 200 keV typically vanished and the entire
spectrum from 30 keV to ~1 MeV can be characterized by a single power law with
a relatively harder photon index ~2-2.7. Consequently the high- and
low-intensity gamma-ray spectra intersect, generally in the ~400 keV - 1 MeV
range, in contrast to the spectral pivoting seen previously at lower (~10 keV)
energies. The presence of the power-law component in both the high- and
low-intensity gamma-ray spectra strongly suggests that the non-thermal process
is likely to be at work in both the high and the low-intensity situations. We
have suggested a possible scenario (Ling & Wheaton, 2003), by combining the
ADAF model of Esin et al. (1998) with a separate jet region that produces the
non-thermal gamma-ray emission, and which explains the state transitions. Such
a scenario will be discussed in the context of the observational evidence,
summarized above, from the database produced by EBOP, JPL's BATSE earth
occultation analysis system.Comment: 6 pages, 3 figures, accepted for publication in Proceedings of 2004
Microquasar Conference, Beijing, China, Chinese Journal of Astronomy and
Astrophysics, minor corrections per refere
P-wave diffusion in fluid-saturated medium
This paper considers the propagating P-waves in the fluid-saturated mediums that are categorized to fall into two distinct groups: insoluble and soluble mediums. P-waves are introduced with slowness in accordance to Snell Law and are shown to relate to the medium displacement and wave diffusion. Consequently, the results bear out that the propagating P-waves in the soluble medium share similar diffusive characteristic as of insoluble medium. Nonetheless, our study on fluid density in the mediums show that high density fluid promotes diffusive characteristic whiles low density fluid endorses non-diffusive P-wav
Fire extinguishant materials
Fire extinguishant composition comprising a mixture of a finely divided aluminum compound and alkali metal, stannous or plumbous halide is provided. Aluminum compound may be aluminum hydroxide, alumina or boehmite but preferably it is an alkali metal dawsonite. The metal halide may be an alkali metal, e.g. potassium iodide, bromide or chloride or stannous or plumbous iodide, bromide or chloride. Potassium iodide is preferred
A least-squares implicit RBF-FD closest point method and applications to PDEs on moving surfaces
The closest point method (Ruuth and Merriman, J. Comput. Phys.
227(3):1943-1961, [2008]) is an embedding method developed to solve a variety
of partial differential equations (PDEs) on smooth surfaces, using a closest
point representation of the surface and standard Cartesian grid methods in the
embedding space. Recently, a closest point method with explicit time-stepping
was proposed that uses finite differences derived from radial basis functions
(RBF-FD). Here, we propose a least-squares implicit formulation of the closest
point method to impose the constant-along-normal extension of the solution on
the surface into the embedding space. Our proposed method is particularly
flexible with respect to the choice of the computational grid in the embedding
space. In particular, we may compute over a computational tube that contains
problematic nodes. This fact enables us to combine the proposed method with the
grid based particle method (Leung and Zhao, J. Comput. Phys. 228(8):2993-3024,
[2009]) to obtain a numerical method for approximating PDEs on moving surfaces.
We present a number of examples to illustrate the numerical convergence
properties of our proposed method. Experiments for advection-diffusion
equations and Cahn-Hilliard equations that are strongly coupled to the velocity
of the surface are also presented
BATSE Soft Gamma-Ray Observations of GROJ0422+32
We report results of a comprehensive study of the soft gamma-ray (30 keV to
1.7 MeV) emission of GROJ0422+32 during its first known outburst in 1992. These
results were derived from the BATSE earth-occultation database with the JPL
data analysis package, EBOP (Enhanced BATSE Occultation Package). Results
presented here focus primarily on the long-term temporal and spectral
variability of the source emission associated with the outburst. The light
curves with 1-day resolution in six broad energy-bands show the high-energy
flux (>200 keV) led the low-energy flux (<200 keV) by ~5 days in reaching the
primary peak, but lagged the latter by ~7 days in starting the declining phase.
We confirm the "secondary maximum" of the low-energy (<200 keV) flux at TJD
8970-8981, ~120 days after the first maximum. Our data show that the "secondary
maximum" was also prominent in the 200-300 keV band, but became less pronounced
at higher energies. During this 200-day period, the spectrum evolved from a
power-law with photon index of 1.75 on TJD 8839, to a shape that can be
described by a Comptonized model or an exponential power law below 300 keV,
with a variable power-law tail above 300 keV. The spectrum remained roughly in
this two-component shape until ~9 November (TJD 8935) and then returned to the
initial power-law shape with an index of ~2 until the end of the period. The
correlation of the two spectral shapes with the high and low luminosities of
the soft gamma-ray emission is strongly reminiscent of that seen in Cygnus X-1.
We interpret these results in terms of the Advection Dominated Accretion Flow
(ADAF) model with possibly a "jet-like" region that persistently produced the
non-thermal power-law gamma rays observed throughout the event.Comment: 40 pages total, including 10 figures and 2 table
Some aspects of analytical chemistry as applied to water quality assurance techniques for reclaimed water: The potential use of X-ray fluorescence spectrometry for automated on-line fast real-time simultaneous multi-component analysis of inorganic pollutants in reclaimed water
The potential use of isotopically excited energy dispersive X-ray fluorescence (XRF) spectrometry for automated on line fast real time (5 to 15 minutes) simultaneous multicomponent (up to 20) trace (1 to 10 parts per billion) analysis of inorganic pollutants in reclaimed water was examined. Three anionic elements (chromium 6, arsenic and selenium) were studied. The inherent lack of sensitivity of XRF spectrometry for these elements mandates use of a preconcentration technique and various methods were examined, including: several direct and indirect evaporation methods; ion exchange membranes; selective and nonselective precipitation; and complexation processes. It is shown tha XRF spectrometry itself is well suited for automated on line quality assurance, and can provide a nondestructive (and thus sample storage and repeat analysis capabilities) and particularly convenient analytical method. Further, the use of an isotopically excited energy dispersive unit (50 mCi Cd-109 source) coupled with a suitable preconcentration process can provide sufficient sensitivity to achieve the current mandated minimum levels of detection without the need for high power X-ray generating tubes
Matrix elements of four-quark operators and \Delta L=2 hyperon decays
The study of neutrinoless double beta decays of nuclei and hyperons require
the calculation of hadronic matrix elements of local four-quark operators that
change the total charge by two units \Delta Q=2 . Using a low energy effective
Lagrangian that induces these transitions, we compute these hadronic matrix
elements in the framework of the MIT bag model. As an illustrative example we
evaluate the amplitude and transition rate of \Sigma- -> p e- e-, a decay
process that violates lepton number by two units (\Delta L=2). The relevant
matrix element is evaluated without assuming the usual factorization
approximation of the four-quark operators and the results obtained in both
approaches are compared.Comment: 13 pages, 2 .eps figure
Galactic distribution of interstellar Al-26
A narrow cosmic gamma ray line at 1809 keV was discovered which was interpreted as resulting from the decay of approximately 3 M sub theta of Al-26 residing in the galactic disk. While its intrinsic width was unresolved by the HEAO 3 spectrometer, a (1 sigma) limit of 3 keV FWHM was obtained; this corresponds to bulk motions of v 250 km/s, which is consistent with material at rest in the ISM. Sites which have been suggested include type II supernovae and massive stars which are members of the extreme population I, as well as novae and red giants which are associated with an older disk population. The HEAO 3 data was used to distinguish between these two stellar populations
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