Fueling and feedback couple supermassive black holes (SMBHs) to their host galaxies across many orders of magnitude in spatial and temporal scales, making this problem notoriously challenging to simulate. We use a multi-zone computational method based on the general relativistic magnetohydrodynamic (GRMHD) code KHARMA that allows us to span 7 orders of magnitude in spatial scale, to simulate accretion onto a non-spinning SMBH from an external medium with a Bondi radius of
Bacteria under external stress can reveal unexpected emergent phenotypes. We show that the intensely studied bacterium
- Award ID(s):
- 1734030
- NSF-PAR ID:
- 10080539
- Publisher / Repository:
- Proceedings of the National Academy of Sciences
- Date Published:
- Journal Name:
- Proceedings of the National Academy of Sciences
- Volume:
- 115
- Issue:
- 51
- ISSN:
- 0027-8424
- Page Range / eLocation ID:
- p. 12979-12984
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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