2023 journal article

Cite it

Core collapse supernova gravitational wave emission for progenitors of 9.6, 15, and 25M⊙

Physical Review D.

By: A. Mezzacappa ^*, P. Marronetti ^*, R. Landfield ^*, E. Lentz ^*, R. Murphy ^*, W. Hix ^*, J. Harris ^*, S. Bruenn ^* ...and 4 other authors, including 1 NC State author, J. Blondin ⁿ , O. Messer ^*, J. Casanova ^* & L. Kronzer ^*

10.1103/PhysRevD.107.043008

Find Text @ NCSU

UN Sustainable Development Goal Categories

7. Affordable and Clean Energy (Web of Science)

Source: ORCID

Added: February 10, 2023

We present gravitational wave emission predictions based on three core collapse supernova simulations corresponding to three different progenitor masses. The masses span a large range, between 9.6 and 25 Solar masses, are all initially non-rotating, and are of two metallicities: zero and Solar. We compute both the temporal evolution of the gravitational wave strains for both the plus and the cross polarizations, as well as their spectral decomposition and characteristic strains.