Author(s)

Lorenzo Zaninetti

Physics Department, Turin, Italy.

The giant arcs in the clusters of galaxies are modeled in the framework of the superbubbles. The density of the intracluster medium is assumed to follow a hyperbolic behavior. The analytical law of motion is function of the elapsed time and the polar angle. As a consequence the flux of kinetic energy in the expanding thin layer decreases with increasing polar angle making the giant arc invisible to the astronomical observations. In order to calibrate the arcsec-parsec conversion three cosmologies are analyzed.

Galaxy Groups, Clusters and Superclusters, Large Scale Structure of the Universe Cosmology

Zaninetti, L. (2019) The Giants Arcs as Modeled by the Superbubbles. Journal of High Energy Physics, Gravitation and Cosmology, 5, 442-463. doi: 10.4236/jhepgc.2019.52026.