Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Steven Balbus"'
Autor:
Andrew Mummery, Steven Balbus
We present analytical solutions for the thermodynamic (temperature, pressure, density, etc.) properties of thin accretion flows in the region within the innermost stable circular orbit (ISCO) of a Kerr black hole, the first analytical solutions of th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8e4193775871bc46a0ecadcc5332589e
Autor:
Andrew Mummery, Steven Balbus
The probability density function of accretion disc luminosity fluctuations at high observed energies (i.e., energies larger than the peak temperature scale of the disc) is derived, under the assumption that the temperature fluctuations are log-normal
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::82852518d36f92c5196a2c12976cd690
http://arxiv.org/abs/2210.01450
http://arxiv.org/abs/2210.01450
Autor:
Katherine Holcomb, Steven Balbus
Publikováno v:
Vol. 54, Issue 1 (Obituaries, News & Commentaries, Community Reports). 54
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::11452060ce008742cf9a908551e45b7c
https://doi.org/10.3847/25c2cfeb.38bbf556
https://doi.org/10.3847/25c2cfeb.38bbf556
Publikováno v:
Journal of Plasma Physics. 88
The theory of magnetohydrodynamic (MHD) turbulence predicts that Alfv\'enic and slow-mode-like compressive fluctuations are energetically decoupled at small scales in the inertial range. The partition of energy between these fluctuations determines t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d713e382bbf15fe3a9be7ffcfe21caf9
https://doi.org/10.1017/s0022377822000460
https://doi.org/10.1017/s0022377822000460
Autor:
Steven Balbus
Publikováno v:
Nature Astronomy. 6:173-174
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::4c694b1fff6fdefad72e630e24cdc985
https://doi.org/10.1038/s41550-022-01608-z
https://doi.org/10.1038/s41550-022-01608-z
Autor:
Hantao Ji, Steven Balbus
Publikováno v:
Physics Today. 66:27-33
For evolving astrophysical accretion disks to concentrate their mass and still conserve angular momentum, turbulent flows are crucial. Those flows cannot be directly observed, so to understand them better physicists are creating them in modest-sized
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f1d8af96a6f1c96f2fc15d4acec2393e
https://doi.org/10.1063/pt.3.2081
https://doi.org/10.1063/pt.3.2081
Autor:
Steven Balbus
Publikováno v:
Scholarpedia. 4:2409
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::06b36c28008ce678e59a10bdd00f9911
https://doi.org/10.4249/scholarpedia.2409
https://doi.org/10.4249/scholarpedia.2409