1 code implementation • 4 Mar 2015 • Ken'ichiro Nakazato, Eri Mochida, Yuu Niino, Hideyuki Suzuki
Using this model, the dependences of SRNs on the cosmic star formation rate density, shock revival time and equation of state are investigated.
High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies High Energy Physics - Phenomenology
