pith. sign in

Univ. Barcelona)

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Papers (4)

  1. Why are Halo Density Profiles Stable at Formation? astro-ph · 1998 · author #6
  2. Inhomogeneous big bang nucleosynthesis with late-decaying massive particles astro-ph · 1998 · author #3
  3. Effect of the vacancy interaction on the antiphase domain growth process in a two dimensional binary alloy cond-mat · 1997 · author #5
  4. Nonlinear Stochastic Differential Equations and Self-Organized Criticality cond-mat · 1993 · author #2

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