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We address the early universe reconstruction (EUR) problem (as considered by Frisch and coauthors in [26]), and the related Zeldovich approximate model [46]. By substituting the fully nonlinear Monge–Ampère equation for the linear Poisson equation to model gravitation, we introduce a modified mathematical model ("Monge-Ampère gravitation/MAG"), for which the Zeldovich approximation becomes exact. The MAG model enjoys a least action principle in which we can input mass concentration effects in a canonical way, based on the theory of gradient flows with convex potentials and somewhat related to the concept of self-dual Lagrangians developed by Ghoussoub [29]. A fully discrete algorithm is introduced for the EUR problem in one space dimension.
@article{CML_2011__3_3_361_0, author = {Brenier, Yann}, title = {A modified least action principle allowing mass concentrations for the early universe reconstruction problem}, journal = {Confluentes Mathematici}, pages = {361--385}, publisher = {World Scientific Publishing Co Pte Ltd}, volume = {3}, number = {3}, year = {2011}, doi = {10.1142/S1793744211000400}, language = {en}, url = {http://geodesic.mathdoc.fr/articles/10.1142/S1793744211000400/} }
TY - JOUR AU - Brenier, Yann TI - A modified least action principle allowing mass concentrations for the early universe reconstruction problem JO - Confluentes Mathematici PY - 2011 SP - 361 EP - 385 VL - 3 IS - 3 PB - World Scientific Publishing Co Pte Ltd UR - http://geodesic.mathdoc.fr/articles/10.1142/S1793744211000400/ DO - 10.1142/S1793744211000400 LA - en ID - CML_2011__3_3_361_0 ER -
%0 Journal Article %A Brenier, Yann %T A modified least action principle allowing mass concentrations for the early universe reconstruction problem %J Confluentes Mathematici %D 2011 %P 361-385 %V 3 %N 3 %I World Scientific Publishing Co Pte Ltd %U http://geodesic.mathdoc.fr/articles/10.1142/S1793744211000400/ %R 10.1142/S1793744211000400 %G en %F CML_2011__3_3_361_0
Brenier, Yann. A modified least action principle allowing mass concentrations for the early universe reconstruction problem. Confluentes Mathematici, Tome 3 (2011) no. 3, pp. 361-385. doi: 10.1142/S1793744211000400
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