A proton synchrotron accelerates protons to a kinetic energy of 500 GeV. At this energy, calculate (a) the Lorentz factor, (b) the speed parameter, and (c) the magnetic field for which the proton orbit has a radius of curvature of 750 m.

Short Answer

Expert verified

(a) The Lorentz factor for proton is 534 .

(b) The speed parameter for proton is 0.99999 .

(c) The magnetic field for the electron is 0.178T.

Step by step solution

01

Identification of given data

The energy of proton is K=500GeV

The radius of curvature of orbit is 750m

The magnetic field for the electron is found by equating the necessary centripetal force by magnetic force on the electron.

02

Determination of Lorentz factor

(a)

The Lorentz factor is given as:

K=γ-1mc2

Here, qis the charge of proton and its value is 1.6×10-19C , m is the mass of proton and its value is 1.67×10-19C , c is the speed of light and its value is 3×108ms

Substitute all the values in the above equation.

500GeV1.6×109J1GeV=γ-11.67×10-27kg3×108ms2γ=534

Therefore, the Lorentz factor for proton is 534..

03

Determination of speed parameter

(b)

The speed parameter for proton is given as:

β=1-1γ2

Substitute all the values in the above equation.

β=1-15342

β=0.999999

Therefore, the speed parameter for proton is 0.999999.

04

Determination of magnetic field for proton

(c)

The magnetic field for proton is given as:

B=mcγ2-1qr

Substitute all the values in the above equation.

B=1.67×10-27kg3×108ms5342-11.6×10-19C750mB=2.23T

Therefore, the magnetic field for proton is 2.23T

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with Vaia!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

What are (a) K, (b) E, and (c) p(in GeVc) for a proton moving at speed 0.990c? What are (d) K, (e) E, and (f) p(in MeVc) for an electron moving at speed 0.990c ?

Continuation of Problem 65. Let reference frame C in Fig. 37-31 move past reference frame D (not shown). (a) Show thatMAD=MABMBCMCD

(b) Now put this general result to work: Three particles move parallel to a single axis on which an observer is stationed. Let plus and minus signs indicate the directions of motion along that axis. Particle A moves past particle B atβAB=+0.20 . Particle B moves past particle C at βBC=0.40. Particle C moves past observer D atβCD=+0.60 . What is the velocity of particle A relative to observer D? (The solution technique here is much faster than using Eq. 37-29.)

The mean lifetime of stationary muons is measured to be 2.2000μs. The mean lifetime of high-speed muons in a burst of cosmic rays observed from Earth is measured to be 16.000μs. To five significant figures, what is the speed parameter βof these cosmic-ray muons relative to Earth?

Superluminal jets. Figure 37-29a shows the path taken by a knot in a jet of ionized gas that has been expelled from a galaxy. The knot travels at constant velocity v at angleθ from the direction of Earth. The knot occasionally emits a burst of light, which is eventually detected on Earth. Two bursts are indicated in Fig. 37-29a, separated by timet as measured in a stationary frame near the bursts. The bursts are shown in Fig. 37-29b as if they were photographed on the same piece of film, first when light from burst 1 arrived on Earth and then later when light from burst 2 arrived. The apparent distanceD¯app traveled by the knot between the two bursts is the distance across an Earth-observer’s view of the knot’s path. The apparent timeT¯app between the bursts is the difference in the arrival times of the light from them. The apparent speed of the knot is then V¯app=D¯app/T¯app. In terms of v, t, andθ , what are (a)D¯app and (b)T¯app ? (c) EvaluateV¯app forv=0.980c and θ=30.0. When superluminal (faster than light) jets were first observed, they seemed to defy special relativity—at least until the correct geometry (Fig. 37-29a) was understood.

Space cruisers A and B are moving parallel to the positive direction of an x axis. Cruiser A is faster, with a relative speed of v=0.900c, and has a proper length of L=200m. According to the pilot of A, at the instant (t = 0) the tails of the cruisers are aligned, the noses are also. According to the pilot of B, how much later are the noses aligned?

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.

Sign-up for free