Astrophysique et technologie aérospatiale

Explaining Formation of Astronomical Jets Using Dynamic Universe Model

Abstract

Satyavarapu Naga Parameswara Gupta

Astronomical jets are observed from the centres of many Galaxies including our own Milkyway. The formation of such jet is explained using SITA simulations of dynamic universe model. For this purpose the path traced by a test neutron is calculated and depicted using a set up of one densemass of the mass equivalent to mass of Galaxy center, 90 stars with similar masses of stars near Galaxy center, mass equivalents of 23 Globular Cluster groups, 16 Milkyway parts, Andromeda and Triangulum Galaxies at appropriate distances. Five different kinds of theoretical simulations gave positive results. The path travelled by this test neutron was found to be an astronomical jet emerging from Galaxy center.