PBH

Published: 8 March 2021| Version 1 | DOI: 10.17632/4bn3kxt3z7.1
Contributor:
Tomohiro Nakama

Description

See "Machine learning primordial black formation" (to appear in Physics of the Dark Universe) for the details. The files "Formed" correspond to the initial conditions leading to PBH formation, where as the files "NotFormed" correspond to those leading to no PBH formation. The initial conditions are specified by the curvature profile, and it is specified by the five parameters n, sigma1, sigma2, A and B of 1310.3007. The first column corresponds to n, the second to sigma1, the third to sigma2, the forth to A, and the fifth to B.

Files

Categories

Theoretical Cosmology

Licence