Download Lecture 14: Electromagnetic Waves

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts

Lorentz force wikipedia , lookup

Magnetohydrodynamics wikipedia , lookup

Maxwell's equations wikipedia , lookup

Electromagnetism wikipedia , lookup

Computational electromagnetics wikipedia , lookup

Transcript
Lecture 14 : Electromagnetic Waves
β€’ Wave equations
β€’ Properties of the waves
β€’ Energy of the waves
Recap (1)
β€’ In a region of space containing no free charge (πœŒπ‘“ = 0) or
current (𝐽𝑓 = 0), Maxwell’s equations can be written as
𝜡. 𝑬 = 𝟎
𝝏𝑩
𝜡×𝑬=βˆ’
𝝏𝒕
𝜡. 𝑩 = 𝟎
𝝏𝑬
𝜡 × π‘© = 𝝁𝟎 𝜺 𝟎
𝝏𝒕
Recap (2)
β€’ Work needs to be performed when creating an 𝐸-field (e.g. by
assembling charges), or a 𝐡-field (e.g. by establishing a current
against an inductance)
β€’ This creates a potential energy stored in the electromagnetic
field with energy densities
1
πœ€0 𝐸 2
2
and
𝐡2
,
2πœ‡0
respectively
Wave equations
β€’ We will now explore how Maxwell’s equations lead to wave
motion in the form of light – an electromagnetic wave
Wave equations
β€’ A wave is a propagating disturbance that carries energy from
one point to another
β€’ A wave may be characterized by its amplitude, wavelength
and speed and can be longitudinal or transverse
speed
Wave equations
β€’ To discover EM waves, consider evaluating 𝛻 × π›» × πΈ
β€’ Substituting in Maxwell’s equations, this equals 𝛻 ×
βˆ’
πœ•
𝑑𝑑
𝛻×𝐡 =
πœ•
βˆ’
πœ•π‘‘
πœ•πΈ
πœ‡0 πœ€0
πœ•π‘‘
=
πœ•π΅
βˆ’
πœ•π‘‘
=
πœ•2 𝐸
βˆ’πœ‡0 πœ€0 2
πœ•π‘‘
β€’ Also by vector calculus, 𝛻 × π›» × πΈ = 𝛻 𝛻. 𝐸 βˆ’ 𝛻 2 𝐸
β€’ Using Maxwell’s equation 𝛻. 𝐸 = 0, this just equals βˆ’π›» 2 𝐸
β€’ Putting the two sides together, we find
𝜡𝟐 𝑬 =
𝝏𝟐 𝑬
𝝁𝟎 𝜺 𝟎 𝟐
𝝏𝒕
Wave equations
β€’ The equation represents a travelling wave
β€’ To see why, consider a 1D wave travelling along the π‘₯-axis with
displacement 𝑦 π‘₯, 𝑑 = 𝐴 sin(π‘˜π‘₯ βˆ’ πœ”π‘‘) in terms of its amplitude 𝐴,
wavelength πœ† =
2πœ‹
,
π‘˜
time period 𝑇 =
2πœ‹
,
πœ”
velocity 𝑣 =
πœ†
𝑇
=
πœ”
π‘˜
Wave equations
β€’ The displacement π’š(𝒙, 𝒕) of a wave travelling with speed 𝒗
satisfies the wave equation
𝝏𝟐 π’š
ππ’™πŸ
=
𝟏 𝝏𝟐 π’š
π’—πŸ ππ’•πŸ
β€’ To check this, substitute in 𝑦 π‘₯, 𝑑 = 𝐴 sin(π‘˜π‘₯ βˆ’ πœ”π‘‘) where 𝑣 =
β€’ On the left-hand side:
πœ•2 𝑦
πœ•π‘₯ 2
β€’ On the right-hand side:
β€’ Using
1
𝑣2
=
π‘˜2
,
πœ”2
= βˆ’π‘˜ 2 𝐴 sin(π‘˜π‘₯ βˆ’ πœ”π‘‘)
πœ•2 𝑦
πœ•π‘‘ 2
= βˆ’πœ”2 𝐴 sin(π‘˜π‘₯ βˆ’ πœ”π‘‘)
we recover the wave equation!
πœ”
π‘˜
Wave equations
β€’ The equation
𝝏𝟐 π’š
ππ’™πŸ
=
𝟏 𝝏𝟐 π’š
π’—πŸ ππ’•πŸ
describes general wave travel
Wave equations
β€’ The relation
𝛻2𝐸
=
πœ•2 𝐸
πœ‡0 πœ€0 2
πœ•π‘‘
implies that each component of
the electric field is a wave travelling at speed 𝒗 =
𝟏
𝝁𝟎 𝜺𝟎
=𝒄
β€’ Evaluating, we obtain 𝑐 = 3 × 108 m/s : the speed of light
Properties of the waves
β€’ Let’s find out more about the properties of electromagnetic
waves
β€’ To simplify the case, suppose that the electric field is along the
𝑦-axis, such that 𝐸𝑦 π‘₯, 𝑑 = 𝐴 sin(π‘˜π‘₯ βˆ’ πœ”π‘‘) and 𝐸π‘₯ = 𝐸𝑧 = 0.
This is known as a linearly polarized wave.
𝑦
π‘₯
Properties of the waves
β€’ We can deduce the 𝐡-field using the relation 𝛻 × πΈ =
β€’ π‘₯-component: βˆ’
πœ•π΅π‘₯
πœ•π‘‘
β€’ 𝑦-component: βˆ’
πœ•π΅π‘¦
βˆ’ πœ”π‘‘)
πœ•πΈπ‘§
πœ•π‘¦
βˆ’
=
πœ•πΈπ‘₯
πœ•π‘§
βˆ’
πœ•πΈπ‘¦
πœ•π‘§
= 0, hence 𝐡π‘₯ = 0
πœ•πΈπ‘§
πœ•π‘₯
= 0, hence 𝐡𝑦 = 0
πœ•πΈπ‘¦
πœ•π΅π‘§
πœ•πΈ
=
βˆ’ π‘₯
πœ•π‘‘
πœ•π‘₯
πœ•π‘¦
1
= 𝐸𝑦 (π‘₯, 𝑑)
𝑣
β€’ 𝑧-component: βˆ’
𝐴
sin(π‘˜π‘₯
𝑣
πœ•π‘‘
=
πœ•π΅
βˆ’
πœ•π‘‘
= π‘˜π΄ cos(π‘˜π‘₯ βˆ’ πœ”π‘‘), hence 𝐡𝑧 π‘₯, 𝑑 =
β€’ The magnetic field is perfectly in phase with the electric field
and oriented at 90°!
Properties of the waves
β€’ The form of a linearly-polarized electromagnetic wave:
β€’ The changing 𝐸-field causes a changing 𝐡-field, which in its
turn causes a changing 𝐸-field
Properties of the waves
β€’ For an electromagnetic wave travelling in a medium with
relative permittivity πœ€π‘Ÿ and relative permeability πœ‡π‘Ÿ we can
𝒄
use Maxwell’s Equations to show that speed 𝒗 =
πœΊπ’“ 𝝁𝒓
β€’ The quantity πœ€π‘Ÿ πœ‡π‘Ÿ is known as the refractive index
Why does
this produce
a spectrum
of light?
Energy of the waves
β€’ Waves transport energy from one place to another
β€’ Energy is stored in the electric field
1
with density πœ€0 𝐸 2 and the
2
magnetic field with density
1
𝐡2
2πœ‡0
β€’ For a linearly polarized wave, 𝐡 =
1
𝐸/𝑣, where 𝑣 =
, hence
1
πœ€0 𝐸 2
2
=
πœ‡0 πœ€0
1
1
πœ€0 𝑣 2 𝐡2 =
𝐡2
2
2πœ‡0
β€’ The energy contained in the
electric and magnetic fields is
equal!
Energy of the waves
β€’ What is the rate of energy flow?
β€’ The energy flowing past area 𝐴 in time 𝑑 is
contained in a volume 𝐴𝑣𝑑
𝑣×𝑑
Energy density π‘ˆ
Propagation speed 𝑣
𝐴
β€’ If the energy density is π‘ˆ, this energy is
π‘ˆπ΄π‘£π‘‘ hence the energy flow per unit area
per unit time is equal to π‘ˆπ‘£
β€’ For linearly-polarized electromagnetic
1
1
waves, π‘ˆπ‘£ = 𝐡𝑧 2 𝑣 = 𝐸𝑦 𝐡𝑧
πœ‡0
πœ‡0
β€’ The energy flow can be represented
𝟏
by the Poynting vector (𝑬 × π‘©)
𝝁𝟎
Energy of the waves
β€’ The Poynting vector,
1
πœ‡0
𝐸 × π΅ = 𝐸 × π», is oriented in the
direction of travel, perpendicular to the 𝐸- and 𝐡-fields
𝐸×𝐻
Energy of the waves
β€’ As an example, consider current 𝐼 flowing along a cylindrical
conductor driven by a potential difference 𝑉
πœ‡0 𝐼
𝐡=
2πœ‹π‘Ÿ
𝐸=
𝑉
𝐿
β€’ The energy flux is equal to the
1
Poynting vector
𝐸×𝐡
πœ‡0
β€’ This is non-zero at the surface of
the conductor, flowing inward
π‘Ÿ
β€’ If the curved surface area is 𝐴,
the power flowing in is 𝑃 =
1
1 𝑉 πœ‡0 𝐼
𝐸𝐡𝐴 =
2πœ‹π‘ŸπΏ = 𝑉𝐼
πœ‡0
𝐿
πœ‡0 𝐿 2πœ‹π‘Ÿ
β€’ We recover Joule heating!
Summary
β€’ Maxwell’s equations predict that
the 𝐸- and 𝐡-fields satisfy linked
1
wave equations with speed
πœ‡0 πœ€0
β€’ For a linearly-polarized wave, the
𝐸- and 𝐡-fields are in phase and
oriented at πŸ—πŸŽ°
β€’ The energy densities stored in
the 𝐸- and 𝐡-fields is equal, and
the energy flow per unit area per
unit time is equal to the Poynting
vector 𝐸 × π»