chester20080
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So in the occasion where we don't rotate the system,the initial potential energy would be mgeffd, d would be what?
The problem involves a frictionless hemisphere with a body sliding down it while the hemisphere accelerates horizontally. The discussion centers around determining the relative velocity of the body when it leaves the hemisphere and the angle it makes at that moment, particularly under the condition that the horizontal acceleration equals the gravitational acceleration.
The discussion is ongoing, with participants sharing insights about the effective acceleration due to gravity in the hemisphere's frame and the nature of the body's trajectory. Some participants express uncertainty about the assumptions made regarding accelerations and forces, while others provide clarifications on the relationship between centripetal and tangential accelerations.
Participants note that their understanding of relative motion and effective forces is limited, and there is a recognition that the problem may involve concepts not yet fully covered in their coursework.
chester20080 said:So in the occasion where we don't rotate the system,the initial potential energy would be mgeffd, d would be what?
chester20080 said:I think I found an equation for the relative velocity,considering the rotated system as you advised me to.I have:
urelative=\sqrt{}2(g-gcosθ+Wsinθ). It yields Urelative=0 for θ=0.
chester20080 said:And the equation for the angle I got:
sinθ(2-\sqrt{}2)-2cosθ+2=0
Good.chester20080 said:Hey,I found 3cosθ-3sinθ-2=0 which is equivalent
My only doubt is that this angle equation for θ=0 gives 3=2,which is not valid.Is it something to worry about?