Anisotropic cosmological models in terms of Raychaudhuri and Wheeler-DeWitt equationsClassical anisotropic cosmological models are described in terms of the Raychaudhuri equation for
a Numerical Solution of Quantum Cosmological Model Simulating Boson and Fermion CreationA numerical solution of
Wheeler-De Will equation for
a quantum cosmological model simulating boson
Hmga2 is required for canonical WNT signaling during lung developmentSingh I.,
Mehta A.,
Contreras A.,
Boettger T.,
Carraro G.,
Wheeler M.,
Cabrera-Fuentes H.,
Bellusci S.,
Seeger W.,
Braun T.,
Barreto G. to an increased expression of secreted WNT glycoproteins Wnt2b, Wnt7b and Wnt11 as well as
a reduction of the WNT
АЛГЕБРОДИНАМИКА: КВАТЕРНИОННЫЙ АНАЛИЗ, КОМПЛЕКСНАЯ СТРУНА И ЕДИНАЯ МИРОВАЯ ЛИНИЯ of biquaternions (B) in particular. Any B-differentiable function gives rise to
a shear-free null congruence (SFNC