630 research outputs found

    FEDGE - A general-purpose computer program for Finite Element Data Generation. Volume 1 - User's manual

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    Users manual for /FEDGE/ Finite Element Data Generation computer program - Vol.

    ELAS - A general purpose computer program for the equilibrium problems of linear structures

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    Digital computer program ELAS handles the equilibrium problems of linear structures of one, two, or three dimensional continuum. ELAS generates the governing equations for the unknown deflections of the mesh points that define the stationary point of the total potential energy function associated with the given loading and unknown deflections

    An approximation method for the solution of nonlinear integral equations

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    A Chebyshev collocation method has been presented to solve nonlinear integral equations in terms of Chebyshev polynomials. This method transforms the integral equation to a matrix equation which corresponds to a system of nonlinear algebraic equations with unknown Chebyshev coefficients. Finally, some examples are presented to illustrate the method and results discussed. (c) 2005 Elsevier Inc. All rights reserved

    VISCEL, a general-purpose computer program for analysis of linear viscoelastic structures. Volume 1 - User's manual

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    VISCEL computer program user manual for analysis of linear viscoelastic structure

    ELAS - A general purpose computer program for the equilibrium problems of linear structures. Volume 1 - User's manual

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    ELAS general purpose digital computer program for equilibrium problems of linear structure

    Viscel: A general purpose computer program for analysis of linear viscoelastic structures, volume 2

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    The VISCEL program is a general purpose computer program developed for equilibrium analysis of linear viscoelastic structures. The program is written in FORTRAN 5 language to operate on the Univac 1108 computer under the EXEC 8 operating system. The program, an extension of the linear equilibrium problem solver ELAS, is an updated and extended version of its earlier form written for the IBM 7094 computer. Finite element matrix displacement approach coupled with the synchronized material property concept, utilizing incremental time steps, was adopted for the solution presented. The step-by-step procedure involves solution of recursive equations in the time domain, which takes into account the memory of material properties. Incremental and accumulative displacements and stresses are obtained at the end of each time step. In order to minimize the extent of computations resulting from accumulative effects of material memory, the program provides an option which enables the employment of constant time steps in the logarithmic scale. Program documentation is presented

    A search for periodicities from a ULX in the LINER galaxy NGC 4736

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    We report our findings on a new quasi-periodic oscillation (QPO) and a long period from the ultraluminous X-ray source (ULX) X-2 in nearby galaxy NGC 4736 based on the Chandra and XMM-Newton archival data. To examine the timing properties, power density spectra of the source have been obtained using Fast Fourier Transform. Also the spectral parameters of the source have been calculated by obtaining and fitting the energy spectra. Power density spectrum of this source reveals a QPO peak at 0.73−0.14+0.160.73_{-0.14}^{+0.16} mHz with an fractional rms variability of 16% using the Chandra data (in the year 2000-lower state of the source). The XMM-Newton data analysis indicates a peak at 0.53−0.35+0.090.53_{-0.35}^{+0.09} mHz with a fractional rms variation of 5% (in the year 2006-higher state of the source). These recovered QPOs overlap within errors and may be the same oscillation. In addition, we detect a long periodicity or a QPO in the Chandra data of about (5.2±2.0)×10−5(5.2\pm2.0)\times10^{-5} Hz (∼\sim 5.4 hrs) over 3 σ\sigma confidence level. If this is a QPO, it is the lowest QPO detected from a ULX. The mass of the compact object in ULX X-2 is estimated using the Eddington luminosity and a disk blackbody model in the range (10−-80) M_{\sun}.Comment: 6 pages, 4 Figures; Accepted for publication in Astrophysics and Space Scienc

    A Search For Supernova Remnants in The Nearby Spiral Galaxy M74 (NGC 628)

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    We have identified nine new SNR candidates in M74 with [S II]/Hα\alpha ≥\geq 0.4 as the basic criterion. We obtain [S II]/Hα\alpha ratio in the range from 0.40 to 0.91 and Hα\alpha intensities from 2.8 ×\times 10−1510^{-15} erg cm−2^{-2} s−1^{-1} to 1.7 ×\times 10−1410^{-14} erg cm−2^{-2} s−1^{-1}. We also present spectral follow-up observations of the SNR candidates and can confirm only three of them (SNR2, SNR3, and SNR5). The lack of confirmation for the rest might be due to the contamination by the nearby H II emission regions as well as due to the inaccurate positioning of the long slit on these objects. In addition, we search the ChandraChandra Observatory archival data for the X-ray counterparts to the optically identified candidates. We find positional coincidence with only three SNR candidates, SNR1, SNR2, and SNR8. The spectrum of SNR2 yields a shock temperature of 10.8 keV with an ionization timescale of 1.6 ×\times 1010^{10} s cm−3^{-3} indicating a relatively young remnant in an early Sedov phase which is not supported by our optical wavelength analysis. Given the high luminosity of 1039^{39} erg s−1^{-1} and the characteristics of the X-ray spectrum, we favor an Ultra Luminous X-ray Source interpretation for this source associated with an SNR. We calculate an X-ray flux upper limit of 9.0 ×\times 10−1510^{-15} erg cm−2^{-2} s−1^{-1} for the rest of the SNRs including spectroscopically identified SNR3 and SNR5.Comment: 10 pages, 8 figures, accepted to be published in A&

    VISCEL: A general-purpose computer program for analysis of linear viscoelastic structures (user's manual), volume 1

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    This program, an extension of the linear equilibrium problem solver ELAS, is an updated and extended version of its earlier form (written in FORTRAN 2 for the IBM 7094 computer). A synchronized material property concept utilizing incremental time steps and the finite element matrix displacement approach has been adopted for the current analysis. A special option enables employment of constant time steps in the logarithmic scale, thereby reducing computational efforts resulting from accumulative material memory effects. A wide variety of structures with elastic or viscoelastic material properties can be analyzed by VISCEL. The program is written in FORTRAN 5 language for the Univac 1108 computer operating under the EXEC 8 system. Dynamic storage allocation is automatically effected by the program, and the user may request up to 195K core memory in a 260K Univac 1108/EXEC 8 machine. The physical program VISCEL, consisting of about 7200 instructions, has four distinct links (segments), and the compiled program occupies a maximum of about 11700 words decimal of core storage

    Finite Element Analysis of Strain Effects on Electronic and Transport Properties in Quantum Dots and Wires

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    Lattice mismatch in layered semiconductor structures with submicron length scales leads to extremely high nonuniform strains. This paper presents a finite element technique for incorporating the effects of the nonuniform strain into an analysis of the electronic properties of SiGe quantum structures. Strain fields are calculated using a standard structural mechanics finite element package and the effects are included as a nonuniform potential directly in the time independent Schrodinger equation; a k-p Hamiltonian is used to model the effects of multiple valence subband coupling. A variational statement of the equation is formulated and solved using the finite element method. This technique is applied to resonant tunneling diode quantum dots and wires; the resulting densities of states confined to the quantum well layers of the devices are compared to experimental current-voltage I(V) curves.Comment: 17 pages (LaTex), 18 figures (JPEG), submitted to Journal of Applied Physic
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