By James Franco
The actors in James Franco’s exceptional debut novel comprise a McDonald’s drive-thru operator who spends his shift attempting on accents; an ex-child famous person recalling a big beachside bacchanal; clinic volunteers and Midwestern transplants; a vampire flick starlet who discovers a cryptic booklet written by way of a recognized actor long gone AWOL; and the ghost of River Phoenix. Then there’s Franco himself, who prowls behind the scenes, peering out among the lines—before taking the degree with attention-grabbing meditations on his paintings, besides nightmarish stories of extra. “Hollywood has constantly been a personal club,” he writes. “I open the gates. I say welcome. I say, Look inside.”
Told in a dizzying array of styles—from lyric essays and disarming testimonials to hilariously rambling textual content messages and ghostly footnotes—and loosely modeled on Alcoholics Anonymous’s Twelve Steps and Twelve Traditions, Actors Anonymous is an severe, wild trip into the darkish center of superstar.
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Extra resources for Actors Anonymous
2 in the upper and lower layers, respectively. l. Our results present large qualitative differencies, depending essentially on the asymptotic behaviour of the closure terms that have been used. If the first kind of closure terms, obtained by Chacon in [2) are used, the results are quite close to those given by the k-c model. For instance, the steady states obtained for k and mean velocity profiles are quite close. This probably happens because in this case the additional term i31 B introduced in the modelization of R is almost zero, for both small or large values of jl.
N, ApPLICATION TO THE k - £ MODEL The above compressibility models have been developed for second-order turbulence closure in which the Reynolds stresses are obtained by transport equations. In the k-£ model, the Reynolds stresses are defined by the eddy viscosity I-'t. In this framework k I E represents the turbulent time scale n. The most natural definition of this time scale is Tt = klEt where Et is the total dissipation. ~. However, it seems that in some works , [3), the incompressible £.
However, the main conclusions that can be drawn is that none of the tested models can give a satisfactory evolution in the whole range of Me: computations in good agreement for high values of Me give poor results for low Me, and conversely. More precisely, the computations have difficulties to find the right evolution of vt k 2 Ie vs. Me. As the predicted level of k is quite correct, this suggests that the level of e vs. Me is the problem to be addressed for such models. Similarly, as it is know that the tested compressible models are not efficient for supersonic turbulent boundary layers, it seems that a reassessment of the formulation of these models has to be made to improve their generality.