Scott is a theoretical/computational astrophysicist interested in black holes, their accretion disks, and the radiation magnetohydrodynamics physics inherent to those systems. He knows a bit about computational methods of general relativistic magnetohydrodynamics (GRMHD) codes, and lately uses them to simulate accreting systems about single and binary black holes. He has also designed novel time-dependent grid techniques (e.g., dynamic nonuniform grids, overlapping misaligned multi-patch methods) to capture the variety of time/space scales often encountered in these systems, and is now expanding his repertoire of methods to include nuclear physics techniques for simulating the bright electromagnetic and gravitational wave signals produced by neutron star mergers.
NEWS:
Please see the article that NASA helped us produce here:
Online Networks:
- ORCID: https://orcid.org/0000-0003-3547-8306
- ArXiv: http://arxiv.org/a/noble_s_2
- iNSPIRE: https://inspirehep.net/authors/1020533
- Google Scholar: https://scholar.google.com/citations?hl=en&user=K2THAaMAAAAJ
- ResearchGate: https://www.researchgate.net/profile/Scott_Noble2
- Twitter: https://twitter.com/therealscn
- LinkedIn: https://www.linkedin.com/in/scott-noble