Body sliding down an accelerating hemisphere

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The discussion centers on a frictionless hemisphere with a body sliding down as the hemisphere accelerates horizontally. The participants explore the relative velocity of the body when it leaves the hemisphere and the angle at which this occurs, particularly under the condition where the hemisphere's acceleration equals gravitational acceleration (W = g). They analyze the forces acting on the body, considering both centripetal and tangential accelerations, and discuss the concept of an effective gravitational acceleration that accounts for the hemisphere's motion. The conversation also touches on the trajectory of the body relative to different frames of reference, emphasizing the complexity of its path due to the combined effects of horizontal acceleration and gravitational forces. The thread concludes with a focus on using energy conservation principles to solve the problem, highlighting the need for careful consideration of the effective gravitational force in calculations.
  • #31
So in the occasion where we don't rotate the system,the initial potential energy would be mgeffd, d would be what?
 
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  • #32
I probably should use a prime on θ to denote the angle from the y' axis in the rotated figure. So, in the rotated figure, the body starts at θ' = β, which corresponds to θ = 0 in the top figure. In the rotated figure, the body falls off for some θ' > β, which means it falls off for some θ > 0 in the upper figure.
 
  • #33
chester20080 said:
So in the occasion where we don't rotate the system,the initial potential energy would be mgeffd, d would be what?

Draw a figure showing the initial position and final position of the block (where it leaves the surface). Draw a vector between these two positions. This is the displacement vector Δr of the body. d is the component of Δr in the direction of geff.
 
  • #34
I think I found an equation for the relative velocity,considering the rotated system as you advised me to.I have:
urelative=\sqrt{}2R(g-gcosθ+Wsinθ). It yields Urelative=0 for θ=0.
 
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  • #35
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.

Except for a missing R that looks good!
 
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  • #36
Yes,I forgot it,but I edited the post.
 
  • #37
And the equation for the angle I got:
sinθ(2-\sqrt{}2)-2cosθ+2=0 and for θ=17 degrees it yields 0.2587=0,which considering that 17 degrees is an approximation,is very good!
 
  • #38
I hope that is the result for this exercise.Thank you very very much for your time and your invaluable help,I appreciate it!
 
  • #39
chester20080 said:
And the equation for the angle I got:
sinθ(2-\sqrt{}2)-2cosθ+2=0

I don't think that's correct.

I find the algebra to be much simpler if I work with the rotated figure and derive an expression for the angle θ' (measured from the y' axis) at which the block falls off. It is then easy to convert this to the angle θ in the non-rotated figure. Also, I think it is easier to keep the expressions in terms of geff rather than g. You should find geff cancels out. (But the "angle of tilt" β of geff does enter the solution.)
 
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  • #40
Can you please give me the angle equation you found,in order to work on my equations and to compare what I will find with yours and tell you tomorrow what I will have found?Unfortunately here (in Greece) it is almost midnight and I am too tired to have a clear mind right now.
 
  • #41
I find

##\theta = \cos^{-1}(\frac{2}{3}\cos\beta) - \beta##

##\beta## is determined from g and W.
 
  • #42
Hey,I found 3cosθ-3sinθ-2=0 which is equivalent as I checked with your equation (just use the formula cos(θ+β)=cosθ*cosβ-sinθ*sinβ and cosβ=g/sqrt{g2+W2} and sinβ=W/sqrt{g2+W2}).And for approximately 17 degrees it yields -0.0027=0 which is excellent!My only doubt is that this angle equation for θ=0 gives 3=2,which is not valid.Is it something to worry about?
 
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  • #43
chester20080 said:
Hey,I found 3cosθ-3sinθ-2=0 which is equivalent
Good.

My only doubt is that this angle equation for θ=0 gives 3=2,which is not valid.Is it something to worry about?

This just shows that θ = 0 is not a solution of the equation 3cosθ-3sinθ-2=0.
So, the body does not leave the surface at θ = 0.
 
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  • #44
Ok,thank you for everything!
 

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