Chapter 16: Electric Fields

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Chapter 16: Electric Fields
Electrically charged particles have electric fields around them. In these fields, other electrically
charged particles will exhibit certain things which are governed by the principles in this
chapter.
Electric Fields (E)
The electric field strength in an electric field is defined as the force per unit charge that acts on
a small positive point charge. As such, it is given by the formula;
𝐸=
𝐹
π‘ž
In a radial electric field, produced by a large charge Q, the electric field strength E is given by;
𝑄
π‘Ÿ2
, πœ€0 = the electric constant, and π‘Ÿ = the distance from the charge.
𝐸=π‘˜
1
Where π‘˜ = 4πœ‹πœ€
0
When drawing field lines, the lines and their direction show what path a positive charge would
take when placed at that point.
Electric Potential (V)
The electric potential at a point is the potential energy per unit charge of a small positive charge
placed at that point. This is the same as the work done per charge to move a small positive
charge from infinity to that point.
The potential energy of a point charge q is;
𝐸𝑝 = π‘žπ‘‰
Where V is the potential at that point.
Electric potential is a scalar quantity and has the unit Volt.
Field Lines and Equipotentials
An equipotential is a surface of constant potential. No change of potential energy occurs when
an object is moved along an equipotential.
Lines of force are always perpendicular to the equipotential surface.
Electric Field Strength and Potential Gradient
The work done on a small positive charge in moving it from infinity to another point is given by;
𝐸𝑝 = π‘žπ‘‰ or, in terms of work, βˆ†π‘Š = π‘žβˆ†π‘‰
The work done by the charge;
βˆ†π‘Š = −π‘žβˆ†π‘‰
Work = Force x Distance, so;
βˆ†π‘Š = 𝐹𝑠,
and 𝐹 = πΈπ‘ž
and 𝑠 = βˆ†π‘‘ where 𝑑 = distance
so βˆ†π‘Š = π‘žπΈβˆ†π‘‘
π‘žπΈβˆ†π‘‘ = −π‘žβˆ†π‘‰
𝐸=−
βˆ†π‘‰
βˆ†π‘‘
Electric Field Strength = - Potential Gradient
For a uniform field between a pair of plates the above simplifies to;
𝐸=
𝑣
𝑑
Measuring Electric Charge
Millikan’s oil drop experiment can be used to determine the fundamental electric charge.
A drop of oil is placed between two charged plates with a significant potential across them. The
potential difference is adjusted until the oil drop is suspended in between the two plates.
In this position, the resultant vertical force on the drop is 0.
Therefore;
πΈπ‘™π‘’π‘π‘‘π‘Ÿπ‘–π‘π‘Žπ‘™ πΉπ‘œπ‘Ÿπ‘π‘’ = πΊπ‘Ÿπ‘Žπ‘£π‘–π‘‘π‘Žπ‘‘π‘–π‘œπ‘›π‘Žπ‘™ πΉπ‘œπ‘Ÿπ‘π‘’
πΈπ‘ž = π‘šπ‘”
The electrical force in a uniform field is given
𝐸=
𝑉
𝑑
𝑉=
π‘šπ‘”π‘‘
π‘ž
𝑉=
π‘šπ‘”π‘‘
𝑛𝑒
Since q is some number of electrons 𝑛𝑒;
Since, π‘š, 𝑔, 𝑑, 𝑛 are know, e can be found to be 1.6 × 10−19 C
Accelerating Charges
An electric field accelerates a charge in the same way a gravitational field accelerates a mass.
1
As a charge loses electric potential energy 𝐸𝑝 = π‘žπ‘‰ it gains kinetic energy 2 π‘šπ‘£ 2 .
πΊπ‘Žπ‘–π‘› π‘œπ‘“ π‘˜π‘–π‘›π‘’π‘‘π‘–π‘ = π‘™π‘œπ‘ π‘  π‘œπ‘“ π‘’π‘™π‘’π‘π‘‘π‘Ÿπ‘–π‘π‘Žπ‘™ π‘π‘œπ‘‘π‘’π‘›π‘‘π‘–π‘Žπ‘™
1
π‘šπ‘£ 2 = π‘žπ‘‰
2
2π‘žπ‘‰
𝑣=√
π‘š
for low energies; 𝑣 ∝ √𝑉
So as the charge π‘ž moves closer to the charge providing the field, it gains speed, and loses speed
in the other direction as it gains potential.
The amount of energy gained by an electron in moving through a p.d. of 1 volt is 1 electron volt
or 1 eV.
Particles with the same charge (proton) but with different masses gain different energies.
With the above expressions, it would appear that a p.d. of only 256,000 volts would accelerate
an electron t o the speed of light. However, this equation has ignored relativistic effects.
Relativistic Momentum
The speed of a particle 𝑣 must reach a limit at 𝑐. However, the particle’s momentum 𝑝, can
increase indefinitely.
Newton says 𝑝 = π‘šπ‘£, however 𝑣 cannot be greater than 𝑐.
Einstein says instead,
𝒑 = πœΈπ’Žπ’—
When v is a very small fraction of c, 𝛾 = 1, π‘ π‘œ, 𝑝 = π‘šπ‘£
Relativistic momentum (blue) against classical momentum (red) as a particle approaches light
speed (c).
As a particle approaches the speed of light, its momentum approaches infinity.
Relativistic Energy
The energy of a free particle is composed of two parts, its kinetic energy and its rest energy.
πΈπ‘‘π‘œπ‘‘π‘Žπ‘™ = πΈπ‘˜π‘–π‘›π‘’π‘‘π‘–π‘ + πΈπ‘Ÿπ‘’π‘ π‘‘
πΈπ‘‘π‘œπ‘‘π‘Žπ‘™ = π›Ύπ‘šπ‘ 2
When the particle is at rest, 𝑣 = 0 and 𝛾 = 1, so;
πΈπ‘Ÿπ‘’π‘ π‘‘ = π‘šπ‘ 2
πΈπ‘‘π‘œπ‘‘π‘Žπ‘™ πΈπ‘Ÿπ‘’π‘ π‘‘ + πΈπ‘˜π‘–π‘›π‘’π‘‘π‘–π‘ π›Ύπ‘šπ‘ 2
=
=
=𝛾
πΈπ‘Ÿπ‘’π‘ π‘‘
πΈπ‘Ÿπ‘’π‘ π‘‘
π‘šπ‘ 2
Electrons in an Electric Field (E)
+ Potential (V)
Electron
y
F
0 Potential
We know that 𝐹 = π‘žπΈ, so for a single electron, 𝐹 = 𝑒𝐸, and from Newton’s second law 𝐹 = π‘šπ‘Ž
𝑒𝐸 = π‘šπ‘Ž
π‘Ž=
𝑒𝐸
π‘š
The electron enters the field with 0 vertical velocity and a horizontal velocity 𝑣.
Its vertical displacement 𝑦 can be given by;
1
𝑦 = π‘Žπ‘‘ 2
2
π‘Ž=
𝑒𝐸
π‘š
1 𝑒𝐸
𝑦 = ( ) 𝑑2
2 π‘š
π‘₯
Horizontally, displacement = speed x time, π‘₯ = 𝑣𝑑, 𝑑 = 𝑣
1 𝑒𝐸 π‘₯ 2
𝑦 = ( ) ( 2)
2 π‘š 𝑣
therefore, for a particle with charge π‘ž;
π‘žπΈ
𝑦=(
) π‘₯2
2π‘šπ‘£ 2
where m is the rest mass of the particle
Giving a parabolic path, like the graph of 𝑦 = π‘₯ 2,
The electron gains a vertical velocity (and thus gains kinetic energy) but its horizontal
component stays the same, the electric field lines are perpendicular to this line so have no effect
on it.
Charged Particles in Magnetic Fields (B)
The force on a current carrying conductor in a magnetic field is given by;
𝐹 = 𝐡𝐼𝐿
𝐼 = πΆβ„Žπ‘Žπ‘Ÿπ‘”π‘’ π‘π‘’π‘Ÿ 𝑒𝑛𝑖𝑑 π‘‘π‘–π‘šπ‘’, 𝐼 =
π‘ž
𝑑
A particle that moves a distance 𝐿 in a time 𝑑 has velocity;
𝐿
𝑣
𝑣 = ,𝑑 =
𝑑
𝐿
𝐼=
π‘žπ‘£
𝐿
𝐹 = π‘žπ‘£π΅
This can be used to find the force acting on a single charged particle (q) moving through a
magnetic field (B) with a velocity (v).
Electrons in a Magnetic Field (B)
A uniform magnetic field will deflect particles in a curved path.
The force on a moving charge in a magnetic field is always perpendicular to its direction of
travel. The direction of velocity is the same as the flow of charge (current) so velocity can be
used in place of current in Fleming’s left hand rule.
B field is directed into the page
The force 𝐹 = π΅π‘žπ‘£ is always perpendicular to the motion of the particle, and so, like an orbiting
planet, always provides a centripetal force.
The momentum of a particle moving in such a way is given by;
𝑝 = π΅π‘žπ‘Ÿ, or, for high speeds, 𝑝 = π›Ύπ΅π‘žπ‘Ÿ
Crossed Fields Velocity Selector
If a uniform electric field and uniform magnetic field are placed perpendicular to each other in
such a way that they produce opposite deflections, they are called crossed fields.
In such a set up, each field is the same size;
𝐡𝑒𝑣 = 𝑒𝐸
𝑣=
𝐸 πΈπ‘™π‘’π‘π‘‘π‘Ÿπ‘–π‘ 𝑓𝑖𝑒𝑙𝑑 π‘ π‘‘π‘Ÿπ‘’π‘›π‘”π‘‘β„Ž
=
𝐡 π‘€π‘Žπ‘”π‘›π‘’π‘‘π‘–π‘ 𝑓𝑙𝑒π‘₯ 𝑑𝑒𝑛𝑠𝑖𝑑𝑦
These two fields will have no effect (being equal) for particles whose velocity is equal to
𝐸
𝐡
This means physicists will know the velocity of any particles that make it through the crossed
field without being deflected.
The radius of the path that the ions take depends on their charge/mass ratio. If all the ions have
the same charge, π‘Ÿ is a function only of the particle’s mass.
π‘š=
π΅π‘žπ‘Ÿ
𝑣
Circular Electric Fields
Equipotential lines in a circular field are like contours on a map, equipotential lines always meet
field lines at right angles.
1
The electric field strength E in a circular field is proportional to π‘Ÿ2 and π‘ž.
π‘ž
π‘Ÿ
Therefore, 𝐸 = π‘˜ 2 , which is analogous to 𝑔 = 𝐺
π‘š
π‘Ÿ2
Electrical Potential near a Charged Sphere
We already know that
𝐸=−
𝑑𝑉
π‘‘π‘Ÿ
Therefore
π‘ž
𝑉 = − ∫ 𝐸 π‘‘π‘Ÿ, and 𝐸 = π‘˜ π‘Ÿ2
𝑉 = −π‘˜π‘ž ∫
𝑉=π‘˜
1
π‘‘π‘Ÿ
π‘Ÿ2
π‘ž
π‘Ÿ
Gauss’ Contribution
All the field lines leaving a spherical charge must spread out equally, and the field strength at a
given surface perpendicular to all these lines is the same. This surface is given by 4πœ‹π‘Ÿ 2 .
The number of field lines on a surface is given by; 𝐸 × 4πœ‹π‘Ÿ 2 , and by convention, this is equal to
π‘ž
where πœ€0 is the permittivity of free space.
πœ€
0
𝐸 × 4πœ‹π‘Ÿ 2 =
𝐸=
π‘ž
πœ€0
π‘ž
4πœ‹πœ€0 π‘Ÿ 2
Comparing this with our equation for Coulomb’s law;
𝐸=π‘˜
π‘ž
π‘Ÿ2
1
π‘˜ must equal 4πœ‹πœ€
0
This is called Coulomb’s constant.
Coulomb’s Law
𝐹=
1
π‘„π‘ž
× 2
4πœ‹πœ€0 π‘Ÿ
The force between two charges Q and q is directly proportional to the product of the charges
and inversely proportional to the distance between the charges squared.
Forces between like charges are repulsive and between unlike charges are attractive.
Similarities between Gravitational Force and Electric Force
Line of force/field line
Gravitational Force
Electric Force
The path that a mass would
take in that field
The path that a positive charge
would take in that field
Newton’s law of gravitation;
Coulomb’s law of force;
Inverse square law of force
𝐹=𝐺×
π‘€π‘š
π‘Ÿ2
𝐹=
1
π‘„π‘ž
× 2
4πœ‹πœ€0 π‘Ÿ
Field strength
Force per unit mass;
𝐹
𝑔=
π‘š
Force per unit charge;
𝐹
𝐸=
π‘ž
Unit of field strength
Nkg −1 or ms −2
NC −1 or Vm−1
In uniform fields
𝑔 is the same everywhere,
Field lines are parallel and
equally spaced.
𝐸 is the same everywhere,
Field lines are parallel and
equally spaced.
Potential
Gravitational potential energy
per unit mass.
Electric potential energy per
unit positive charge.
Unit of potential
Jkg −1
V or JC −1
Potential energy between two
masses/charges
π‘‰π‘”π‘Ÿπ‘Žπ‘£ = −𝐺
π‘€π‘š
π‘Ÿ
From a point mass or uniform
spherical mass;
𝐸𝑝 =
From a point charge or a
uniform spherical charge;
Radial fields
𝑔=𝐺×
Action at a distance
𝑀
π‘Ÿ2
Between any two masses.
1
π‘„π‘ž
×
4πœ‹πœ€0
π‘Ÿ
𝐸=
1
𝑄
× 2
4πœ‹πœ€0 π‘Ÿ
Between any two charged
objects.
Force
Attractive only.
Attractive and repulsive,
depending on charges.
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