Aspects of Eternal Inflation, part 3 - Leonard Susskind
Aspects of Eternal Inflation, part 3 Leonard Susskind Stanford University July 20, 2011
Жүктеу.....
Пікірлер: 4
@allanlees2994 жыл бұрын
Another great series of lectures by Susskind, marred only by the inept editing which leaves the viewer staring at an empty screen while our professor is off working on another blackboard...
@michaelmilbocker45484 жыл бұрын
current is at the precise value where the Bekenstein-Hawking equation is satisfied, which represents a balance between CFT fields on the CFT boundary and entanglement in the AdS bulk. Current is a solution to EFE’s where information density in a volume is maximized.
@michaelmilbocker45484 жыл бұрын
the symbols didnt show: current cosmological constant
Пікірлер: 4
Another great series of lectures by Susskind, marred only by the inept editing which leaves the viewer staring at an empty screen while our professor is off working on another blackboard...
current is at the precise value where the Bekenstein-Hawking equation is satisfied, which represents a balance between CFT fields on the CFT boundary and entanglement in the AdS bulk. Current is a solution to EFE’s where information density in a volume is maximized.
the symbols didnt show: current cosmological constant