5,394 research outputs found
The N=1 superstring as a topological field theory
By "untwisting" the construction of Berkovits and Vafa, one can see that the
N=1 superstring contains a topological twisted N=2 algebra, with central charge
c^ = 2. We discuss to what extent the superstring is actually a topological
theory.Comment: 8 Pages (LaTeX). TAUP-2155-9
Infrared luminescence and application of a vibronic-coupling Hamiltonian to the level structure of CdTe:Fe<sup>2+</sup>
Samples of crystalline CdTe doped with two different concentrations of iron were prepared by the vertical high-pressure Bridgman method. Absorption and emission spectra were recorded at liquid-helium temperature in the region of the 5T2(D)? 5E(D) infrared transitions of substitutional Fe2+(d6) ions. Especially in the range between 2200 and 2300 cm−1, a rich structure is resolved comprising more lines than predicted from plain crystal-field theory. The explanation of all the important lines is found after introducing a vibronic Jahn-Teller term to the Hamiltonian. A linear coupling between the double-degenerate vibrational mode ε (or γ3) to the electronic orbitals of the atomic multiplet of symmetry 5D leads to the diagonalization of the total Hamiltonian in a set of vibronic functions. Just one free parameter is used in the adjustment: the so-called Jahn-Teller energy representing the strength of the coupling. The corresponding value that we report here is 3 cm−1. The energies thus found are in good agreement with the positions of the observed lines in the spectra. With the final wave functions we can calculate the relative intensities of the most important transitions and approximate theoretical line shape. This is also in good agreement with the experiment. Using these same energies and wave functions a calculation was performed to explain data existing in the literature about far-infrared absorption for the system CdTe:Fe2+. Again, good agreement between experiment and theory is found
Numerical and Experimental Analysis of Sound Suppressor for a 5.56 mm Calibre
A sound suppressor is an internal or external device coupled to the barrel of a firearm. Its development has been historically related to the negative effects produced by the noise. This article presents the numerical and experimental analysis of a sound suppressor for a 5.56 mm caliber rifle. It was designed, manufactured, and tested inside a shooting tunnel for 911 m/s and 344 m/s velocities. Three geometric configurations with curved deflectors, conical deflectors, and finally with a reactive spiral capable of dissipating the acoustic wave were compared considering reactive and dissipative systems. The attenuation of the sound inside the silencer depends directly on the reduction of the projectile wave velocity and the deflagration of the gases at the instant of firing. Then the MIL-STD-1474E standard was used to carry out the experiments. The results in the computational numerical simulation show an average value of 143 dB for the considered three models, the Sound Pressure Level in the reactive core model decreased by 25% with respect to other proposals, which have an average value of 141 dB. These results can be useful to improve in the design of sound suppressors based on the needs of the users and under the specific characteristics of each weapon ballistic. 
Numerical Modelling of Caseless Ammunition with Coreless Bullet in Internal Ballistics
In the search of a new weapon for combat in short range, it is proposed the use of a new experimentally designed 7.62 mm calibre ammunition with a lighter weight (caseless-coreless). This can be used in carbine assault rifles with short barrel or pistols. In this work, the compressible gases flowing through the gun barrel caused by the proposed ammunition were experimentally and numerically analysed. The Large Eddy Simulation was used for the numerical simulation, considering a compressible and turbulent flow, with the chemical species transport model and a complete conversion of the propellant reaction. Variations in pressure and temperature were compared with the results obtained from a conventional 7.62 mm full metal jacket (FMJ) ammunition. Results of ballistic experimental tests and numerical simulations were similar than those of the 9 mm x 19 mm FMJ ammunitions, showing feasibility for the development of new weapons intended for operations of short range shots.Defence Science Journal, Vol. 65, No. 3, May 2015, pp.203-207, DOI: http://dx.doi.org/10.14429/dsj.65.851
The Galaxy Counterparts of the two high-metallicity DLAs at z=2.412 and z=2.583 towards Q0918+1636
The quasar Q0918+1636 (z=3.07) has two intervening high-metallicity Damped
Lyman-alpha Absorbers (DLAs) along the line of sight, at redshifts of z=2.412
and 2.583. The z=2.583 DLA is located at a large impact parameter of 16.2 kpc,
and despite this large impact parameter it has a very high metallicity
(consistent with solar), a substantial fraction of H_2 molecules, and it is
dusty as inferred from the reddened spectrum of the background QSO. The z=2.412
DLA has a metallicity of [M/H]=-0.6 (based on ZnII and SiII). In this paper we
present new observations of this interesting sightline. HST/WFC3 imaging was
obtained in the F606W, F105W and F160W bands. This is complemented by
ground-based imaging in the u-, g-bands as well as K_s observations in the
near-infrared (NIR). In addition, we present further spectroscopy with the
ESO/VLT X-Shooter spectrograph. Based on these observations we obtain the
following results: By fitting stellar population synthesis models to the
photometric SED we constrain the physical properties of the z=2.583 DLA galaxy,
and we infer its morphology by fitting a Sersic model to its surface brightness
profile. We find it to be a relatively massive (M_star 10^10 M_sun), strongly
star-forming (SFR~30 M_sun / yr, dusty (E_(B-V)=0.4) galaxy with a disk-like
morphology. We detect most of the strong emission lines from the z=2.583 DLA
[OIII],3727, [OIII],4960, [OIII],5007, Hbeta, and Halpha, albeit at low
signal-to-noise (SN) ratio except for the [OIII],5007 line. We also detect
[OIII],5007 emission from the galaxy counterpart of the z=2.412 DLA at a small
impact parameter (<2 kpc). Overall our findings are consistent with the
emerging picture that high-metallicity DLAs are associated with relatively
(compared to typical DLAs) luminous and massive galaxy counterparts.Comment: 11 pages, Accepted for publication in MNRA
Development and Implementation of a Monitoring System for STRC with the Aid of Head Detection
The Development and Implementation of a Monitoring System for STRC with the Aid of Head Detection aims to automate the research room operations to increase its efficiency. It consists of a head detection system, website managed database and a mobile application controlled room access. The website and mobile application cater to two types of users namely, the administrator and the students. The website exclusively features announcements and management of equipment inventory both handled by the administrator. The mobile application features an IN/OUT button which manages the users access on the five (5) research rooms in the building. The head detection system detects, tracks and counts each person that enters a research room. The count noted by the system is then compared to the count of students that used the mobile application for room access. The e-mail and SMS notification system observes the comparison of the two counts and sends the appropriate notification to the administrator when there is a violation in the conditions set for the two systems. The database serves as the central point as it holds every information needed by each element in order to communicate with the whole system
Modeling Supply Networks and Business Cycles as Unstable Transport Phenomena
Physical concepts developed to describe instabilities in traffic flows can be
generalized in a way that allows one to understand the well-known instability
of supply chains (the so-called ``bullwhip effect''). That is, small variations
in the consumption rate can cause large variations in the production rate of
companies generating the requested product. Interestingly, the resulting
oscillations have characteristic frequencies which are considerably lower than
the variations in the consumption rate. This suggests that instabilities of
supply chains may be the reason for the existence of business cycles. At the
same time, we establish some link to queuing theory and between micro- and
macroeconomics.Comment: For related work see http://www.helbing.or
Super Earth Explorer: A Coronagraphic Off-Axis Space Telescope
The Super-Earth Explorer is an Off-Axis Space Telescope (SEE-COAST) designed
for high contrast imaging. Its scientific objective is to make the
physico-chemical characterization of exoplanets possibly down to 2 Earth radii
>. For that purpose it will analyze the spectral and polarimetric properties of
the parent starlight reflected by the planets, in the wavelength range 400-1250
nmComment: Accepted in Experimental Astronom
Assessing an Internet health information site by using log analysis: the experience of the National Cancer Institute of Brazil
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