Behaviour of Point Masses Against the Background Radiation with Dissipation in an Expanding Universe

1990

Closed access Metadata (CSL-JSON)
DOI 10.1017/s0074180900241193
Data confidence 70 medium
How this score is calculated

It is built from checkable properties of the record itself: whether the article has a DOI, how many independent sources confirmed its data, whether the required fields are filled in, and how recent the latest confirmation is. Disagreement between sources and a missing identifier lower it. A value of 80 or above means the record was published without further checking; 60 to 79 means it is published at reduced confidence, with a manual check advisable. A record verified by an editor by hand is never pushed below 90 by a recalculation. This scores our data about the article, not the article itself.

Abstract

One of the most important cosmological problems is the question of the properties of systems of particles in a regular field of homogeneous and isotropically expanding two-component Metagalactic substratum. Within the framework of the Newtonian cosmology, we consider the behaviour of the ensemble of point masses embedded in a homogeneous expanding medium having two different equations of the state. Dissipation phenomena caused by the chaotic motion of the background matter are taken into account.