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Martin","submitted_at":"2013-09-20T15:05:35Z","abstract_excerpt":"We investigate the time-dependent behavior of Crab-like pulsar wind nebulae (PWNe) generating a set of models using 4 different initial spin-down luminosities ($L_0 =\\{1,0.1,0.01,0.001\\} \\times L_{0, {\\rm Crab}}$), 8 values of magnetic fraction ($\\eta =$ 0.001, 0.01, 0.03, 0.1, 0.5, 0.9, 0.99, and 0.999, i.e., from fully particle dominated to fully magnetically dominated nebulae), and 3 distinctive ages: 940, 3000, and 9000 years. 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