Chimera: A massively parallel code for core-collapse supernova simulation
Stephen W. Bruenn, John M. Blondin, W. Raphael Hix, Eric J. Lentz, O., E. Bronson Messer, Anthony Mezzacappa, Eirik Endeve, J. Austin Harris, Pedro, Marronetti, Reuben D. Budiardja, Merek A. Chertkow, and Ching-Tsai Lee

TL;DR
Chimera is a comprehensive, parallel simulation code for modeling core-collapse supernovae, integrating detailed physics like neutrino transport, hydrodynamics, and nuclear reactions to study explosion mechanisms and observable signals.
Contribution
This paper presents the detailed design and current version of Chimera, a novel multi-physics, parallel code for simulating core-collapse supernovae with high fidelity.
Findings
Enables detailed study of neutrino effects in supernova explosions
Simulates multi-dimensional hydrodynamics with realistic physics
Predicts observable signatures like neutrino signals and gravitational waves
Abstract
We provide a detailed description of the Chimera code, a code developed to model core collapse supernovae in multiple spatial dimensions. The core collapse supernova explosion mechanism remains the subject of intense research. Progress to date demonstrates that it involves a complex interplay of neutrino production, transport, and interaction in the stellar core, three-dimensional stellar core fluid dynamics and its associated instabilities, nuclear burning, and the foundational physics of the neutrino-stellar core weak interactions and the equations of state of all stellar core constituents -particularly, the nuclear equation of state associated with nucleons, both free and bound in nuclei. Chimera, by incorporating detailed neutrino transport, realistic neutrino-matter interactions, three-dimensional hydrodynamics, realistic nuclear, leptonic, and photonic equations of state, and a…
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