caa a22 4500 477060293 CHVBK 20180405111358.0 cr unu---uuuuu 170330e19960201xx s 000 0 eng 10.1007/BF02067677 doi (NATIONALLICENCE)springer-10.1007/BF02067677 Nonlinear fields in models of cosmological inflation [Elektronische Daten] [S. Chervon, V. Shchigolev, V. Zhuravlev] Conclusions: We have considered the prospects for investigating the inflation stage of evolution of the universe, when gauge and Higgs fields are considered to be the source of the gravitational field. We have suggested an effective description of the GUT using a chiral, nonlinear sigma model. We note the possibility of the appearance of an electromagnetic field within the framework of Newtonian cosmology. Plenum Publishing Corporation, 1996 Chervon S. Ul'yanovsk branch, M. V. Lomonosov Moscow State University, USSR aut Shchigolev V. Ul'yanovsk branch, M. V. Lomonosov Moscow State University, USSR aut Zhuravlev V. Ul'yanovsk branch, M. V. Lomonosov Moscow State University, USSR aut Russian Physics Journal Kluwer Academic Publishers-Plenum Publishers 39/2(1996-02-01), 139-145 1064-8887 39:2<139 1996 39 11182 https://doi.org/10.1007/BF02067677 text/html Onlinezugriff via DOI 1 research-article jats NATIONALLICENCE 856 40 https://doi.org/10.1007/BF02067677 text/html Onlinezugriff via DOI NATIONALLICENCE 700 1- Chervon S. Ul'yanovsk branch, M. V. Lomonosov Moscow State University, USSR aut NATIONALLICENCE 700 1- Shchigolev V. Ul'yanovsk branch, M. V. Lomonosov Moscow State University, USSR aut NATIONALLICENCE 700 1- Zhuravlev V. Ul'yanovsk branch, M. V. Lomonosov Moscow State University, USSR aut NATIONALLICENCE 773 0- Russian Physics Journal Kluwer Academic Publishers-Plenum Publishers 39/2(1996-02-01), 139-145 1064-8887 39:2<139 1996 39 11182 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer