Projects funded by the NCN
Relativistic radiative magnetohydrodynamical simulations of accretion disks in black hole binaries: implications for black hole transients.
2018/29/N/ST9/02139
Keywords:
Black holes accretion disks numerical simulations general relativity
Descriptors:
- ST9_12: Relativistic astrophysics
Panel:
ST9 - Astronomy and space science: astrophysics, astrochemistry, astrobiology, solar system, planetary systems, stellar, galactic and extragalactic astronomy, space science, instrumentation
Host institution :
Centrum Astronomiczne im. Mikołaja Kopernika Polskiej Akademii Nauk
woj. mazowieckie
Principal investigator (from the host institution):
Number of co-investigators in the project: 2
Call: PRELUDIUM 15 - announced on 2018-03-15
Amount awarded: 89 880 PLN
Project start date (Y-m-d): 2019-03-15
Project end date (Y-m-d): 2021-03-14
Project duration:: 24 months (the same as in the proposal)
Project status: Project settled
Project description
Download the project description in a pdf file
Note - project descriptions were prepared by the authors of the applications themselves and placed in the system in an unchanged form.
Information in the final report
- Publication in academic press/journals (1)
- Looking for the underlying cause of black hole X-ray variability in GRMHD simulationsAuthors:D. A. Bollimpalli, R. Mahmoud, C. Done , P. C. Fragile, W. Kluźniak, , R. Narayan, C. WhiteAcademic press:Monthly Notices of the Royal Astronomical Society (rok: 2020, tom: 496, strony: 20), Wydawca: Oxford University PressStatus:PublishedDOI:10.1093/mnras/staa1808 - link to the publication