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    <journal-meta>
      <journal-title-group>
        <journal-title>P.R. Woodward. The Pie ewise Paraboli Method (PPM) for gas-dynami al
simulations // Journal of Computational Physi s. Volume 54</journal-title>
      </journal-title-group>
    </journal-meta>
    <article-meta>
      <title-group>
        <article-title>Суперкомпьютерные дни в России 2015 // Russian Supercomputing Days 2015 // RussianSCDays.org</article-title>
      </title-group>
      <pub-date>
        <year>2015</year>
      </pub-date>
      <volume>2</volume>
      <issue>5</issue>
      <fpage>8</fpage>
      <lpage>16</lpage>
      <abstract>
        <p>ŒŁ</p>
      </abstract>
    </article-meta>
  </front>
  <body>
    <sec id="sec-1">
      <title>-</title>
      <p>3. ´ß Łaeº
( ae</p>
      <p>Суперкомпьютерные дни в России 2015 // Russian Supercomputing Days 2015 // RussianSCDays.org
ρ(t, r) = Z f (t, r, u)du.</p>
      <p>u
1. ˛
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      <p>Gk</p>
      <p>Суперкомпьютерные дни в России 2015 // Russian Supercomputing Days 2015 // RussianSCDays.org
4. ˜º Œ
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Суперкомпьютерные дни в России 2015 // Russian Supercomputing Days 2015 // RussianSCDays.org</p>
      <p>Pk2
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      <p>Суперкомпьютерные дни в России 2015 // Russian Supercomputing Days 2015 // RussianSCDays.org
ΔΦ(x) = ρ(x),
Φ(x)|x→∞ = 0,</p>
      <p>Z ρ(x)dx
Φ(x0) = − x .</p>
      <p>|x0 − |
Φ(x0) = − Z ρ(x)K(x − x0)dx = −ρ ∗ K,</p>
      <p>1
K(x − x0) = x</p>
      <p>| − x0|
Z ρ(x)dx &lt; C1 &lt; ∞,</p>
      <p>Z K(x)dx &lt; C1 &lt; ∞,
F T [Φ](k) = −F T [ρ](k) · F T [K](k),
Φ = −F T −1 [F T [ρ] · F T [K]]</p>
      <p>Суперкомпьютерные дни в России 2015 // Russian Supercomputing Days 2015 // RussianSCDays.org
2. ˇ Ł
º
 0.5 min(h1x,hy,hz) , px2 + y2 + z2 = 0,
K(x, y, z) = 
 √x2+1y2+z2 , px2 + y2 + z2 &gt; 0.
vol. 181, p. 375-389. 1977.
appli ation to non-spheri al stars // Monthly Noti es of the Royal Astronomi al So iety,
5. R.A. Gingold and J.J. Monaghan. Smoothed parti le hydrodynami s - Theory and
10. V. Springel et al. Simulations of the formation, evolution and lustering of galaxies and
quasars // Nature, V. 435, p. 629. 2005,
Volume 35. 2009. P.512-522.
for FLASH, a massively parallel, multiphysi s simulation ode // Parallel Computing.
7. A.Dubeya, K. Antypasb, M.K. Ganapathy , et al. Extensible omponent-based ar hite ture</p>
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      <title>2. Ho kney, R.W. and Eastwood, J.W. Computer Simulation Using Parti les. //</title>
      <p>M Graw-Hill. New York. 1981.
12. Y. Feng, T. Di Matteo, R.A.C. Croft, S. Bird, N. Battaglia, S. Wilkins // Monthly Noti e
of Royal Astronomi al So iety. 2015 (submitted)
11. A.A. Klypin et al. Dark Matter Halos in the Standard Cosmologi al Model: Results from
the Bolshoi Simulation // Astrophysi al Journal. V. 740 p. 102. 2011.
1980.
3. Berezin Yu.A. Vshivkov V.A. Parti le-in- ell method in the plasma dynami s // Nauka.
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17. M.Frigo and S.G.Johnson. FFTW software // http://www.t w.org
1978. 592 ae.
15. aeŒŁØ</p>
    </sec>
    <sec id="sec-3">
      <title>Analysis // Graylo k Press, Ro hester, N.Y., 1961.</title>
      <p>14. Kolmogorov A.N., Fomin S.V. Elements of the Theory of Fun tions and Fun tional
Domain decomposition method for supercomputer simulation of
gravitating systems
Nikolay Snytnikov and Vitaly Vshivkov</p>
    </sec>
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