Astrophysics (Index)About

advection dominated accretion flow

(ADAF)
(accretion without radiating much energy)

Advection dominated accretion flow (ADAF) is accretion into a black hole that is carrying in energy that might otherwise be radiated. It occurs when emission from the accretion disk is low, which can happen if the accretion material is relatively diffuse, with few particle collisions to trigger photon generation. The un-radiated heat puffs up the disk, making it less disk-shaped. EMR from an accretion disk may have spectral signatures that suggest this, revealing information about the object. The term ADAF is also used for the model developed for such disks and their accretion, and sometimes used as a term for disks that largely adhere to the model, i.e., calling a particular disk an ADAF.

In contrast, an alpha disk is a disk cooling effectively by radiating EMR.


(gravity,black holes)
Further reading:
https://en.wikipedia.org/wiki/Accretion_disk#Analytic_models_of_sub-Eddington_accretion_disks_(thin_disks,_ADAFs)
http://chandra.harvard.edu/resources/faq/black_hole/bhole-36.html
http://www.astronomy.ohio-state.edu/~dhw/A825/notes5.pdf
https://www.emis.de/journals/LRG/Articles/lrr-2013-1/articlese7.html
https://arxiv.org/abs/astro-ph/9803141
https://ui.adsabs.harvard.edu/abs/1994ApJ...428L..13N/abstract

Referenced by pages:
accretion disk
AGN accretion
alpha disk
disk
SMBH formation

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