The Counting of Galaxies from Type Ia Supernovae Rate

TL;DR

This paper develops a model linking galaxy counts to Type Ia supernovae rates, providing a framework to analyze their relationship and evolution with redshift, aiding understanding of the universe's large-scale structure.

Contribution

It introduces a novel model and analytical framework connecting galaxy counts with supernova rates and their dependence on redshift, enhancing cosmological studies.

Findings

Relationship between galaxy counts and supernova rates established

Framework for analyzing redshift dependence developed

Implications for universe evolution from z ~ 2 discussed

Abstract

The aim of this paper is to provide a model of relationship between the number of galaxies and the rate of type Ia supernovae (SNe). In addition, present approach prepares a framework to analyze this relationship and its dependence on the redshif, giving aid to the deepening of studies on radial distribution of galaxies. The work also shows how the ratio of counts entails to the topological aspects regarding the evolution of the universe itself from z ~ 2. The relationships refer directly to the redshift apart from morphological considerations.