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 discussion centers on the dynamics of a body sliding down a frictionless hemisphere with a constant horizontal acceleration, denoted as W. The participants derive equations to determine the relative velocity of the body as it leaves the hemisphere and the angle θ at which this occurs, particularly under the condition where W equals g (the acceleration due to gravity). Key equations include the effective gravitational acceleration, geff, which modifies the gravitational force acting on the body due to the hemisphere's acceleration. The analysis reveals that the body does not follow a circular path relative to the Earth, but rather a more complex trajectory influenced by the horizontal acceleration of the hemisphere.
PREREQUISITESStudents of physics, mechanical engineers, and anyone interested in the dynamics of motion on accelerating surfaces will benefit from this discussion.
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?