Cosmological structure formation under MOND. A new numerical solver for the Poisson's equation

Details Cosmological structure formation under MOND. A new numerical solver for the Poisson's equation Cosmological structure formation under MOND. A new numerical solver for the Poisson's equation

Jan 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011eas....44...57l&link_type=abstract

EAS Publications Series, Volume 44, 2011, pp.57-60

Mathematics

Logic

Scientific paper

We present a novel solver for an analogue to Poisson's equation in the framework of modified Newtonian dynamics (MOND). This equation is highly non-linear and hence standard codes based upon tree structures and/or FFT's in general are not applicable; one needs to defer to multi-grid relaxation techniques. We present results from the first cosmological simulations we made to compare cosmological structure formation of in the two paradigms. We found compatible results between the two simulations, at least at redshift z = 0.

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