Packet D: Bonus 19

The standard model of these objects is the Shakura–Sunyaev model. For 10 points each:
[10e] Name these circular regions of material that often form around compact objects like black holes.
ANSWER: accretion disks [prompt on disks]
[10m] The Shakura–Sunyaev model is a model of thin disks efficient at this process, in contrast to ADAF (“A-D-A-F”) disks. The pressure of this phenomenon equals a body’s self-gravity at the Eddington limit.
ANSWER: radiation [or word forms like radiate; accept radiation pressure; accept photon emission; accept answers specifying (the production of) photons or light or electromagnetic waves]
[10h] The Shakura–Sunyaev model also makes this common radiative assumption typically known by a three-letter acronym. Under this simplifying assumption, the source function of the radiative transfer equations depends only on temperature.
ANSWER: local thermodynamic equilibrium [or LTE; prompt on partial answers]
<GC, Other Science> | Packet D - UBC B, Oxford A, Waterloo B, CWRU A

HeardPPBE %M %H %
1711.7694%24%0%

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Conversion

TeamOpponentPart 1Part 2Part 3TotalParts
UCLA AUCSD B100010E

Summary

TournamentEditionMatchHeardPPBE %M %H %
California (North)Main Site316.67100%67%0%
California (South)Main Site110.00100%0%0%
Great LakesMain Site110.00100%0%0%
Lower Mid-AtlanticMain Site110.00100%0%0%
MidwestMain Site210.00100%0%0%
NortheastMain Site110.00100%0%0%
OverflowMain Site25.0050%0%0%
SoutheastMain Site110.00100%0%0%
UKMain Site316.67100%67%0%
Upper Mid-AtlanticMain Site210.00100%0%0%