00:01
So, here we can apply the conservation of linear momentum.
00:10
Linear momentum to the collision and the conservation of energy to the motion after collision.
00:16
So, conservation of momentum is there to the collision and conservation of energy of energy after collision.
00:37
This is the key thing that we have to see.
00:40
Now, frequency we know equal to 1 upon 2 .5 root of.
00:45
Of k upon m and time period equal to one upon frequency.
00:53
Now according to the question, the object returns to the equilibrium position in time t by two.
01:04
In time t by two object returns to equilibrium.
01:16
So in the first part, the a part, the momentum conservation during collision momentum conservation during pollution we have to see this m v0 equal to 2m into v and capital v equal to half b0 that is half into 2 .00 meter per second so that is v equal to 1 .00 meter per second.
02:13
Now energy conservation after collision you have to see energy conservation after pollution that is half mv square equal to minus half k x square from here we can find out x that is equal to mv square upon k that is equal to root of 20 .0 kg into 1 .00 meter per second the whole square from where did we get? we got it from here.
03:02
Okay? now, this is in root itself upon 1 .10 .0 newton per meter.
03:13
So when we calculate, we are going to get the answer to be 0 .4 to 6 meter and this is our amplitude.
03:29
Now, omega or the angular frequency is equals to 2 pi f, okay? that is k by m because f equal to 1 by 2 pi root of k by m.
03:51
Now putting the value, what we are going to get, f equal to 1 by 2 pi root of 1 .10 .0 newton upon meter upon 20 .0 kg that is equal to 0 .373 hertz.
04:18
This is 0 .0 .0 .373 hertz...