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jeka94
3 years ago
11

A proton is accelerated through a potential difference of 250V. It then enters a uniform magnetic field and moves in a circular

path of radius 10.0cm. What is the magnitude of the magnetic field? What is the period of revolution for the circling proton?
Physics
2 answers:
3241004551 [841]3 years ago
6 0

Answer: a) 7.52 ×10^-4 T, b) 4.72×10^-7s

Explanation: by using the work energy thereom, the work done on the electron by the voltage source (potential) equals the kinetic energy.

qV =mv^2/2

Where q = magnitude of electronic charge = 1.609×10^-19 c

V = potential difference = 250v

m = mass of an electronic charge = 9.11×10^-31 kg

v = velocity of electron =?

By substituting the parameters, we have that

1.609×10^-19 × 250 = 9.11×10^-31 × v^2/2

1.609×10^-19 × 250 ×2 = 9.11×10^-31 ×v^2

v^2 = 1.609×10^-19 × 250 ×2/ 9.11×10^-31

v^2 = 8.05×10^-17/ 9.11×10^-31

v^2 = 1.77×10^14

v = √1.77×10^14

v = 1.33×10^7 m/s

The centripetal force required for the motion of the electron is gotten from the magnetic force on the electron.

qvB = mv^2/r

By cancelling "v" on both sides of the equation, we have that

qB = mv/r

Where r = radius = 10cm = 0.1m

1.609×10^-19 × B = 9.11 ×10^-31 ×1.33×10^7/ 0.1

B = (9.11 ×10^-31 × ×1.33×10^7)/ (0.1 ×1.609×10^-19)

B = 1.21×10^-23/ 1.609×10^-20

B = 0.752×10^-3

B = 7.52 ×10^-4 T

To get the period of motion, we recall that

v = ωr

Where ω = angular frequency

1.33×10^7 = ω×0.1

ω = 1.33×10^7/ 0.1

ω = 13.3×10^7

ω = 1.33×10^6 rad/s

But the period (T) of a periodic motion is defined as

T = 2π/ω

T = 2 × 3.142 / 1.33×10^6

T = 4.72×10^-7s

Lyrx [107]3 years ago
6 0

Answer:

B = 0.0228T

T= 2.87×10-⁶s

Explanation:

Given V = 250V, R = 10cm = 0.1m

q = 1.6×10-¹⁹C, m = 1.67×10-²⁷kg

From the work energy theorem the electric energy of the field = kinetic energy of the proton.

qV = 1/2×mv²

v = √(2qV/m) = √(2×1.6×10-¹⁹×250/(1.67×10-²⁷))

v = 218870m/s

The magnetic force on the proton by newton's 2nd law of motion is related as

qvB = ma = m× v²/R

Rearranging

B = mv/qR = 1.67×10-²⁷ × 218870/(1.6×10-¹⁹ × 0.1) = 0.0228T

T = 2π/ω = 2πR/v = 2π×0.1/218870 = 2.87×10-⁶ = 2.87μs.

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A package of mass m is released from rest at a warehouse loading dock and slides down a 3.0-m-high frictionless chute to a waiti
LuckyWell [14K]

Answer:

The speed of the package of mass m right before the collision = 7.668\ ms^-1

Their common speed after the collision = 2.56\ ms^-1

Height achieved by the package of mass m when it rebounds = 0.33\ m

Explanation:

Have a look to the diagrams attached below.

a.To find the speed of the package of mass m right before collision we have to use law of conservation of energy.

K_{initial} + U_{initial} = K_{final}+U_{final}

where K is Kinetic energy and U is Potential energy.

K= \frac{mv^2}{2} and U= mgh

Considering the fact  K_{initial} = 0\ and U_{final} =0 we will plug out he values of the given terms.

So V_{1}{(initial)} =\sqrt{2gh} = \sqrt{2\times9.8\times3} = 7.668\ ms^-1

Keypoints:

  • Sum of energies and momentum are conserved in all collisions.
  • Sum of KE and PE is also known as Mechanical energy.
  • Only KE is conserved for elastic collision.
  • for elastic collison we have e=1 that is co-efficient of restitution.

<u>KE = Kinetic Energy and PE = Potential Energy</u>

b.Now when the package stick together there momentum is conserved.

Using law of conservation of momentum.

m_1V_1(i) = (m_1+m_2)V_f where V_1{i} =7.668\ ms^-1.

Plugging the values we have

m\times 7.668 = (3m)\times V_{f}

Cancelling m from both sides and dividing 3 on both sides.

V_f = 2.56\ ms^-1

Law of conservation of energy will be followed over here.

c.Now the collision is perfectly elastic e=1

We have to find the value of V_{f} for m mass.

As here V_{f}=-2.56\ ms^-1 we can use that if both are moving in right ward with 2.56 then there is a  -2.56 velocity when they have to move leftward.

The best option is to use the formulas given in third slide to calculate final velocity of object 1.

So

V_{1f} = \frac{m_1-m_2}{m_1+m_2} \times V_{1i}= \frac{m-2m}{3m} \times7.668=\frac{-7.668}{3} = -2.56\ ms^-1

Now using law of conservation of energy.

K_{initial} + U_{initial} = K_{final}+U_{final}

\frac{m\times V(f1)^2}{2} + 0 = 0 +mgh

\frac{v(f1)^2}{2g} = h

h= \frac{(-2.56)^2}{9.8\times 3} =0.33\ m

The linear momentum is conserved before and after this perfectly elastic collision.

So for part a we have the speed =7.668\ ms^-1 for part b we have their common speed =2.56\ ms^-1 and for part c we have the rebound height =0.33\ m.

3 0
3 years ago
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