![]() We consider the gravitational field g to be uniform at the surface of the Earth. | The motion can be linear. The acceleration a is constant and is a = (Vfinal - Vinitial )/ t equ1 here a = (-20 -20) / 4 = -10 m/s/s This is the acceleration due to gravity g acceleration is a vector. You give the projectile an initial velocity Vo = 20m/s The velocity drecreases at a constant rate : V = Vo + a t equ2 here: V = 20 - 10t so t = 1s, V = 10m/s t=2s , V = 0 t = 3s, V = -10m/s t=4s , V = -20m/s remember that the velocity V is a vector If the acceletation is constant you have: Vaverage = (Vinitial + V final)/2 and Vaverage = distance/t equ3 so between t =0 and t = 1s Vaverage = 10 + 20 / 2 = 15m/s distance = Vaverage x t = 15m displacement AB = Vot + 0.5a t2 equ4 AB is the vector connecting an inital point A to a final point B here : AB = 20 t - 0.5 10 t2 The displacement increases with the time squared So t = 4s, AB = 20(4) - 5 (16) = 0 . The displacement is 0 because the change in position is 0. t = 1 AB = 20(1) - 5 (1) = 15m@up Vfinal2 = Vinitial2 + 2 a |AB| equ5 This is the last equation for uniform motion |
| ALONG X-axis: acceleration = ax = 0 Vx = Vox + ax t so : Vx = Vox =Vo cos(α) x = Vox t + 0.5 ax t2 so x = Vox t = Vo cos(α) t (1) parametric equation ALONG Y-axis acceleration ay = - g = -9.8 m/s/s Vy = Voy +ayt so Vy = Voy - (g) t Vy= Vosin (α ) - g t y = Voy t + 0.5 ay t2 y = Vosin( α) t - 0.5 g t2 (2) parametric equation ------------------------------------ (1) gives t = x / Vo cos(α ) (2) y = Vosin( α) ( x /Vo cos(α )) - 0.5 g ( x / Vo cos(α ))2 so y = - 1/2 g / ( Vo2 cos(α ) 2 ) x2 + tan(α ) x |
![]() Let's say you drop an electron (charge - e with e = 1.6 10-19C ) in an uniform field E . The charge q = -e experiences a Force Fe = q E = -e E The force is @ dowm and a = - F/m or a = - e E /m | Along the y-axis: a = - e E /m V = Vo - eE/m t here Vo = 0 then V = - eE/m t y = Vot - 0.5 eE/m t2 here Vo = 0 so y = - eE/2m t2 The speed increases at a constant rate, the displacement depends on the square on the time. the distance between the plates is d. so if y = - d, - d= -eE/2m t2 t = sqrt ( 2md / eE) time it takes for the electron to cross the capacitor. Let's find the speed of the electron when it get to the bottom. V = - eE/m t with t = sqrt ( 2md / eE ) or V = - eE/m sqrt (2md / eE) V = - sqrt (2m e2 E2 d / m2 e E) = - sqrt ( 2e E d / m ) But E = U/d with U the voltage between the plates So V = - sqrt ( 2 e U / m ) Find the kinetic energy KE = 0.5 m V2 with V = sqrt ( 2 e U / m ) V2 = 2eU / m so KE = eU This is what we found previously !! eU is also the electric potential energy of the electron before falling. |
![]() | along the X-axis: ax = 0 Vx = Vo x = Vo t (1) along the Y-axis ay = eE / m Vy = eE / m t y = 0.5 eE / m t2 (2) (1) in (2) y = eE / 2mVo2 x2 The motion is therefore a parabola. Once the electron leaves the electric field, the motion is linear and the velocty is constant. of an oscilloscope. To learn more about how an oscilloscope works. |

oscilloscope. The beam can be deviated sideway or up and down. The voltage between the plates control the deviation.
5)



![]() charges moving in a magnetic field will experience a magnetic force. The direction of the force is given by the right hand rule. The force is perpendicular to both the velocity of the charges and to the magnetic field. | right hand rule. current I (positive chrages) along the thumb, B (magnetic field) along the fingersand F our of the hand. |
![]() A moving charge in a magnetic field will experience a force perpendicular to both V (initial velocity) and B. B exerts a torque on the charge and the charge rotates./ | ![]() One consequence : if you move a wire in a magnetic field, the electrons will experience a force. A curent will be induced and a voltate will build up at the ends of the wires. This is EM induction. |


![]() | ![]() | sin(Φ) = qV perpendicular / qV so qVperpendicular = sin(Φ) qV (in the right anlge triangle) |
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