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If theta is still wrt the horizontal, no. At the top of the loop, the radial direction will be vertical.toesockshoe said:ok so the radial acceleration is the vector gcos(theta) ?
If theta is still wrt the horizontal, no. At the top of the loop, the radial direction will be vertical.toesockshoe said:ok so the radial acceleration is the vector gcos(theta) ?
oh sorry. i meant gsin(theta). but how does this factor in with v^2/r?haruspex said:If theta is still wrt the horizontal, no. At the top of the loop, the radial direction will be vertical.
You've established that the radial acceleration is g sin(theta). What does the radial acceleration need to be to stay in contact with the curved surface? What relationship do you think that leads to?toesockshoe said:oh sorry. i meant gsin(theta). but how does this factor in with v^2/r?
haruspex said:You've established that the radial acceleration is g sin(theta). What does the radial acceleration need to be to stay in contact with the curved surface? What relationship do you think that leads to?
A weight is a force, not an acceleration.toesockshoe said:it has to equal the weight of the mass?
haruspex said:You've established that the radial acceleration is g sin(theta). What does the radial acceleration need to be to stay in contact with the curved surface? What relationship do you think that leads to?
toesockshoe said:it has to be greater than 0?
haruspex said:A weight is a force, not an acceleration.
Let me ask you something - what do you think centripetal acceleration means? How would you define it?
Right, it is the radial component of the acceleration. We know the centripetal acceleration is ##\frac {v^2}r##, and in post #33 I wrote that you had shown the radial component of acceleration to be ##g\sin(\theta)##. So what equation does that give you?toesockshoe said:it is the acceleration component that is point towards the center of the circular motion it is traveling in. that's all i know.
it means gsin(theta) = v^2/r.haruspex said:Right, it is the radial component of the acceleration. We know the centripetal acceleration is ##\frac {v^2}r##, and in post #33 I wrote that you had shown the radial component of acceleration to be ##g\sin(\theta)##. So what equation does that give you?
and that is true for all moments on the sphere right? not just when the normal force is 0.haruspex said:Right, it is the radial component of the acceleration. We know the centripetal acceleration is ##\frac {v^2}r##, and in post #33 I wrote that you had shown the radial component of acceleration to be ##g\sin(\theta)##. So what equation does that give you?
Yes!toesockshoe said:gsin(theta) = v^2/r
No.toesockshoe said:and that is true for all moments on the sphere right? not just when the normal force is 0.
F_n- gsin(\theta) correct?haruspex said:Yes!
No.
To maintain contact, the radial component of the net force must be ##\frac{mv^2}r##.
In terms of gravity and the normal force (the only two forces present), what is the radial component of the net force?
Yes, taking radially outward as positive and g as positive. So what equation can you write for staying in contact with the sphere when the normal might not be zero?toesockshoe said:F_n- gsin(\theta) correct?
im not 100 percent sure what your asking. can you elaborate?haruspex said:Yes, taking radially outward as positive and g as positive. So what equation can you write for staying in contact with the sphere when the normal might not be zero?
In post #38 you wrote the correct equation relating gravitational acceleration to centripetal acceleration for the case where contact is just maintained, i.e. where the normal force is zero.toesockshoe said:im not 100 percent sure what your asking. can you elaborate?
oh. it isharuspex said:In post #38 you wrote the correct equation relating gravitational acceleration to centripetal acceleration for the case where contact is just maintained, i.e. where the normal force is zero.
What is the equation for the case where the normal force is not zero?
Close, but you have a sign error. The normal force points radially outward, but the centripetal acceleration is radially inward. And remember, when the normal force is zero you should get the same equation as in post #38.toesockshoe said:oh. it is
F_n - mgsin(\theta) = \frac{mv^2}{r} correct?
lets assume that the y-axis is pointing along the same direction as the normal force.
oh that's right. so I should switch the Fn and the mgsin(theta) around and make my y-axis point upward in the direction as the gravity force. also, whenever I use latex, the latex forumla gets placed in the center of the page. can you give me a sample code of how to put the latex code in line with your normal text? for example, here is how i would type a regular latex code [ tex ] F_n-mgsin(\theta)=\frac{mv^2}{r} [ / tex]. why does that become centered?haruspex said:Close, but you have a sign error. The normal force points radially outward, but the centripetal acceleration is radially inward. And remember, when the normal force is zero you should get the same equation as in post #38.
Use itex instead of tex.toesockshoe said:oh that's right. so I should switch the Fn and the mgsin(theta) around and make my y-axis point upward in the direction as the gravity force. also, whenever I use latex, the latex forumla gets placed in the center of the page. can you give me a sample code of how to put the latex code in line with your normal text? for example, here is how i would type a regular latex code [ tex ] F_n-mgsin(\theta)=\frac{mv^2}{r} [ / tex]. why does that become centered?
Since I have done the trickery of using ## before that whole code.toesockshoe said:ok test: ##\frac{mv^2}{r} ## how come your code didnt convert into latex? its properly coded... i don't see any spaces.