/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 35 \(\bullet\) (a) Through what pot... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

\(\bullet\) (a) Through what potential difference does an electron have to be accelerated, starting from rest, to achieve a speed of 0.980\(c ?\) (b) What is the kinetic energy of the electron at this speed? Express your answer in joules and in electronvolts.

Short Answer

Expert verified
(a) 2.05 million volts, (b) 3.29 x 10^-13 J or 2.05 million eV.

Step by step solution

01

Define the problem and known values

An electron is being accelerated from rest to a speed of \(0.980c\), where \(c\) is the speed of light in a vacuum. We need to find the potential difference required to achieve this speed and the kinetic energy of the electron.
02

Use the relativistic energy-momentum relation

To find the energy, we use the relation: \[ E = \gamma mc^2 \]where \( \gamma = \dfrac{1}{\sqrt{1 - \left( \dfrac{v}{c} \right)^2}} \) is the Lorentz factor, \( m \) is the rest mass of the electron \((9.11 \times 10^{-31} \text{ kg})\), and \( v = 0.980c \).
03

Calculate the Lorentz factor

Calculate \( \gamma \) for \( v = 0.980c \):\[ \gamma = \dfrac{1}{\sqrt{1 - (0.980)^2}} = \dfrac{1}{\sqrt{1 - 0.9604}} = \dfrac{1}{\sqrt{0.0396}} \approx 5.025 \]
04

Compute the relativistic energy

Substitute \( \gamma \) into the energy formula:\[ E = 5.025 \times (9.11 \times 10^{-31} \text{ kg}) \times (3.0 \times 10^8 \text{ m/s})^2 \]Simplifying gives: \[ E \approx 4.11 \times 10^{-13} \text{ J} \]
05

Find the rest energy

Calculate the rest energy:\[ E_0 = mc^2 = (9.11 \times 10^{-31} \text{ kg}) \times (3.0 \times 10^8 \text{ m/s})^2 = 8.19 \times 10^{-14} \text{ J} \]
06

Calculate kinetic energy

The kinetic energy \( K \) is the total energy minus the rest energy:\[ K = E - E_0 = (4.11 \times 10^{-13} - 8.19 \times 10^{-14}) \text{ J} = 3.29 \times 10^{-13} \text{ J} \]
07

Convert kinetic energy into electronvolts

Convert joules into electronvolts knowing \( 1 \text{ eV} = 1.602 \times 10^{-19} \text{ J} \):\[ K \approx \dfrac{3.29 \times 10^{-13} \text{ J}}{1.602 \times 10^{-19} \text{ J/eV}} \approx 2.05 \times 10^6 \text{ eV} \]
08

Calculate the potential difference

The potential energy gained \((eV)\) equals the kinetic energy \((K)\):\[ e \times V = K \Rightarrow V = \dfrac{K}{e} = \dfrac{3.29 \times 10^{-13} \text{ J}}{1.602 \times 10^{-19} \text{ C}} \approx 2.05 \times 10^6 \text{ V} \]

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 91Ó°ÊÓ!

Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Lorentz factor
The Lorentz factor, denoted by \( \gamma \), is a crucial concept in relativistic physics, especially when dealing with objects moving at speeds close to that of light, \( c \). As velocities increase, classical physics becomes less accurate, and relativistic equations must be used.
  • The Lorentz factor is defined as: \( \gamma = \dfrac{1}{\sqrt{1 - \left( \dfrac{v}{c} \right)^2}} \). Here, \( v \) represents the object's velocity, and \( c \) is the speed of light, approximately \( 3.0 \times 10^8 \text{ m/s} \).
  • When the velocity \( v \) is much less than \( c \), the Lorentz factor is approximately equal to 1, indicating Newtonian mechanics is valid.
  • At higher velocities, \( \gamma \) exceeds 1, significantly affecting mass, energy, and time calculations.
For an electron moving at \( 0.980c \), the Lorentz factor was calculated to be approximately 5.025. This means the electron exhibits about five times more relativistic mass and energy than it would at rest.
Kinetic energy
In relativistic physics, the concept of kinetic energy extends beyond the classical formula \( \dfrac{1}{2}mv^2 \) because velocities involved approach the speed of light. The total energy \( E \) of a particle in motion includes its rest energy and additional energy due to its motion.
  • The total relativistic energy is expressed as: \( E = \gamma mc^2 \).
  • To find the kinetic energy \( K \), subtract the rest energy \( E_0 = mc^2 \) from the total energy:
    \[ K = E - E_0 \]
  • In this scenario, the electron's total energy was \( 4.11 \times 10^{-13} \text{ J} \), and its rest energy was \( 8.19 \times 10^{-14} \text{ J} \).
  • Thus, the kinetic energy comes out to be \( 3.29 \times 10^{-13} \text{ J} \) or approximately \( 2.05 \times 10^6 \text{ eV} \), which are energy units ideal for particles.
Understanding these calculations helps to grasp how moving at relativistic speeds significantly increases the energy content of particles.
Potential difference
Potential difference, often referred to as voltage, is essential to understanding energy transfer in electric fields. In particle physics, it plays a key role when accelerating particles like electrons from rest.
  • Potential difference \( V \) relates to the energy change of a charge \( e \) moving through said difference.
  • When an electron accelerates through a potential difference, it gains kinetic energy, making the relationship \( eV = K \) — where \( e \) is the charge of the electron.
  • For the electron in the problem, accelerating to \( 0.980c \), the gained kinetic energy was \( 3.29 \times 10^{-13} \text{ J} \) or \( 2.05 \times 10^6 \text{ eV} \).
  • This means it was accelerated across a potential difference of approximately \( 2.05 \times 10^6 \text{ V} \).
Thus, understanding the potential difference aids in determining the required energy and conditions to bring particles up to high speeds in particle accelerators.

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

\(\bullet\) You measure the length of a futuristic car to be 3.60 \(\mathrm{m}\) when the car is at rest relative to you. If you measure the length of the car as it zooms past you at a speed of \(0.900 c,\) what result do you get?

In the year \(2084,\) a spacecraft flies over Moon Station III at a speed of 0.800\(c .\) A scientist on the moon measures the length of the moving spacecraft to be 140 \(\mathrm{m} .\) The spacecraft later lands on the moon, and the same scientist measures the length of the now stationary spacecraft. What value does she get?

\(\bullet\) Two particles are created in a high-energy accelerator and move off in opposite directions. The speed of one particle, as measured in the laboratory, is \(0.650 c,\) and the speed of each particle relative to the other is 0.950\(c .\) What is the speed of the second particle, as measured in the laboratory?

\(\bullet\) Neutron stars are the remains of exploded stars, and they rotate at very high rates of speed. Suppose a certain neutron star has a radius of 10.0 \(\mathrm{km}\) and rotates with a period of 1.80 \(\mathrm{ms}\) . (a) Calculate the surface rotational speed at the equator of the star as a fraction of \(c .\) (b) Assuming the star's surface is an iner- tial frame of reference (which it isn't, because of its rotation), use the Lorentz velocity transformation to calculate the speed of a point on the equator with respect to a point directly oppo- site it on the star's surface.

\bullet A proton (rest mass \(1.67 \times 10^{-27} \mathrm{kg}\) ) has total energy that is 4.00 times its rest energy. What are (a) the kinetic energy of the proton; (b) the magnitude of the momentum of the proton; (c) the speed of the proton?

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.