Namespaces
Variants
Actions

Difference between revisions of "Harmonic vibration"

From Encyclopedia of Mathematics
Jump to: navigation, search
(Importing text file)
 
m (tex encoded by computer)
 
Line 1: Line 1:
 +
<!--
 +
h0465601.png
 +
$#A+1 = 38 n = 0
 +
$#C+1 = 38 : ~/encyclopedia/old_files/data/H046/H.0406560 Harmonic vibration,
 +
Automatically converted into TeX, above some diagnostics.
 +
Please remove this comment and the {{TEX|auto}} line below,
 +
if TeX found to be correct.
 +
-->
 +
 +
{{TEX|auto}}
 +
{{TEX|done}}
 +
 
''sinusoidal vibration''
 
''sinusoidal vibration''
  
 
A periodic variation with time of a physical magnitude, which may be written in analytical form as
 
A periodic variation with time of a physical magnitude, which may be written in analytical form as
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h0465601.png" /></td> </tr></table>
+
$$
 +
= x ( t)  = \
 +
A  \cos  ( \omega t - \alpha )  = \
 +
\mathop{\rm Re}  [ Be ^ {i \omega t } ],
 +
$$
  
where <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h0465602.png" /> is the value of the vibrating magnitude at the moment of time <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h0465603.png" />, <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h0465604.png" /> is the amplitude, <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h0465605.png" /> is the periodic (circular) frequency, and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h0465606.png" /> is the initial phase of the vibration. The duration of one complete vibration <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h0465607.png" /> is called the period of the harmonic vibration, while <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h0465608.png" />, which is the number of complete vibrations performed in unit time, is known as the frequency of the harmonic vibration (<img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h0465609.png" />). The period of the harmonic vibration is independent of its amplitude. The velocity, acceleration and all higher derivatives of the vibrating magnitude vary harmonically at the same frequency. A harmonic vibration is represented as an ellipse on the [[Phase plane|phase plane]] <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656010.png" />. Owing to the dissipation of energy, perfect harmonic vibrations are not encountered in nature, but many processes are close to harmonic vibrations. These include small vibrations of mechanical systems with respect to their equilibrium position. The resulting frequencies (the so-called eigen frequencies) of the vibrations are independent of the initial conditions of motion and are determined by the nature of the vibrating system itself. For instance, small vibrations (under the effect of gravity) of a mathematical pendulum on a thread of length <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656011.png" /> are described by the differential equation
+
where $  x = x( t) $
 +
is the value of the vibrating magnitude at the moment of time $  t $,  
 +
$  | A | = | B | $
 +
is the amplitude, $  \omega $
 +
is the periodic (circular) frequency, and $  \alpha $
 +
is the initial phase of the vibration. The duration of one complete vibration $  T = 2 \pi / \omega $
 +
is called the period of the harmonic vibration, while $  \nu = 1/T $,  
 +
which is the number of complete vibrations performed in unit time, is known as the frequency of the harmonic vibration ( $  \omega = 2 \pi \nu $).  
 +
The period of the harmonic vibration is independent of its amplitude. The velocity, acceleration and all higher derivatives of the vibrating magnitude vary harmonically at the same frequency. A harmonic vibration is represented as an ellipse on the [[Phase plane|phase plane]] $  ( x, \dot{x} ) $.  
 +
Owing to the dissipation of energy, perfect harmonic vibrations are not encountered in nature, but many processes are close to harmonic vibrations. These include small vibrations of mechanical systems with respect to their equilibrium position. The resulting frequencies (the so-called eigen frequencies) of the vibrations are independent of the initial conditions of motion and are determined by the nature of the vibrating system itself. For instance, small vibrations (under the effect of gravity) of a mathematical pendulum on a thread of length $  l $
 +
are described by the differential equation
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656012.png" /></td> </tr></table>
+
$$
 +
ml \dot{x} dot  = - mgx,
 +
$$
  
where <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656013.png" /> is the gravity acceleration and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656014.png" /> is the angle between the vertical and the thread of the pendulum. The general solution of this equation has the form <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656015.png" />, where the eigen frequency of the vibration, <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656016.png" />, depends on <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656017.png" /> and <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656018.png" /> only, while the amplitude <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656019.png" /> and the phase <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656020.png" /> are constants of integration, selected in accordance with the initial conditions.
+
where $  g $
 +
is the gravity acceleration and $  x( t) $
 +
is the angle between the vertical and the thread of the pendulum. The general solution of this equation has the form $  x = A  \cos  ( \omega t - \alpha ) $,  
 +
where the eigen frequency of the vibration, $  \omega = \sqrt g/l $,  
 +
depends on $  g $
 +
and $  l $
 +
only, while the amplitude $  A $
 +
and the phase $  \alpha $
 +
are constants of integration, selected in accordance with the initial conditions.
  
 
Harmonic vibrations play an important part in the study of vibrations as a whole, since complicated periodic and almost-periodic varying magnitudes may be approximately represented, to any desired degree of accuracy, by a sum of harmonic vibrations. Mathematically this corresponds to the approximations of functions by [[Trigonometric series|trigonometric series]] and by Fourier integrals (cf. [[Fourier integral|Fourier integral]]).
 
Harmonic vibrations play an important part in the study of vibrations as a whole, since complicated periodic and almost-periodic varying magnitudes may be approximately represented, to any desired degree of accuracy, by a sum of harmonic vibrations. Mathematically this corresponds to the approximations of functions by [[Trigonometric series|trigonometric series]] and by Fourier integrals (cf. [[Fourier integral|Fourier integral]]).
Line 15: Line 51:
 
The classical Fourier series
 
The classical Fourier series
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656021.png" /></td> </tr></table>
+
$$
 +
x ( t)  = \
 +
\sum _ {n = - \infty } ^  \infty 
 +
a _ {n} e ^ {i nt }
 +
$$
  
of a complex-valued function <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656022.png" />, defined on <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656023.png" />, may be regarded as the expansion of <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656024.png" /> into a sum of harmonic vibrations with integer frequencies <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656025.png" />. The Fourier coefficient
+
of a complex-valued function $  x( t) $,  
 +
defined on $  [ - \pi , \pi ] $,  
 +
may be regarded as the expansion of $  x( t) $
 +
into a sum of harmonic vibrations with integer frequencies $  n = 0, \pm  1, \pm  2 ,\dots $.  
 +
The Fourier coefficient
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656026.png" /></td> </tr></table>
+
$$
 +
a _ {n}  = {
 +
\frac{1}{2 \pi }
 +
}
 +
\int\limits _ {- \pi } ^  \pi 
 +
x ( t) e ^ {- i n t }  dt
 +
$$
  
determines the amplitude <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656027.png" /> and the phase shift <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656028.png" /> of a harmonic vibration with frequency <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656029.png" />. The totality of all Fourier coefficients determines the spectrum of <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656030.png" /> and shows the harmonic vibrations which are actually involved in <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656031.png" />, as well as the amplitudes and the initial phases of these vibrations. Knowing the spectrum is equivalent to knowing the function <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656032.png" />.
+
determines the amplitude $  ( | a _ {n} | ) $
 +
and the phase shift $  (  \mathop{\rm arg}  a _ {n} ) $
 +
of a harmonic vibration with frequency $  n $.  
 +
The totality of all Fourier coefficients determines the spectrum of $  x( t) $
 +
and shows the harmonic vibrations which are actually involved in $  x( t) $,  
 +
as well as the amplitudes and the initial phases of these vibrations. Knowing the spectrum is equivalent to knowing the function $  x( t) $.
  
A function <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656033.png" /> defined on <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656034.png" /> can no longer be built from harmonic vibrations with integer frequencies. Its construction involves vibrations of all frequencies: The function <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656035.png" /> can be represented by a Fourier integral:
+
A function $  x( t) $
 +
defined on $  ( - \infty , \infty ) $
 +
can no longer be built from harmonic vibrations with integer frequencies. Its construction involves vibrations of all frequencies: The function $  x( t) $
 +
can be represented by a Fourier integral:
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656036.png" /></td> </tr></table>
+
$$
 +
x ( t)  = \int\limits _ {- \infty } ^  \infty 
 +
a ( n) e ^ {i nt }  dn ;
 +
$$
  
 
where
 
where
  
<table class="eq" style="width:100%;"> <tr><td valign="top" style="width:94%;text-align:center;"><img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656037.png" /></td> </tr></table>
+
$$
 +
a ( n)  = {
 +
\frac{1}{2 \pi }
 +
}
 +
\int\limits _ {- \infty } ^  \infty 
 +
x ( t) e ^ {- in t }  dt
 +
$$
  
is the spectral density of <img align="absmiddle" border="0" src="https://www.encyclopediaofmath.org/legacyimages/h/h046/h046560/h04656038.png" />.
+
is the spectral density of $  x( t) $.
  
 
These representations of functions form the base of the [[Fourier method|Fourier method]] for solving various problems in the theory of differential and integral equations.
 
These representations of functions form the base of the [[Fourier method|Fourier method]] for solving various problems in the theory of differential and integral equations.
Line 37: Line 104:
 
====References====
 
====References====
 
<table><TR><TD valign="top">[1]</TD> <TD valign="top">  G.S. Gorelik,  "Oscillations and waves" , Moscow-Leningrad  (1950)  (In Russian)</TD></TR></table>
 
<table><TR><TD valign="top">[1]</TD> <TD valign="top">  G.S. Gorelik,  "Oscillations and waves" , Moscow-Leningrad  (1950)  (In Russian)</TD></TR></table>
 
 
  
 
====Comments====
 
====Comments====
 
  
 
====References====
 
====References====
 
<table><TR><TD valign="top">[a1]</TD> <TD valign="top">  J.W.S. Rayleigh,  "The theory of sound" , '''1''' , Dover, reprint  (1945)</TD></TR></table>
 
<table><TR><TD valign="top">[a1]</TD> <TD valign="top">  J.W.S. Rayleigh,  "The theory of sound" , '''1''' , Dover, reprint  (1945)</TD></TR></table>

Latest revision as of 19:43, 5 June 2020


sinusoidal vibration

A periodic variation with time of a physical magnitude, which may be written in analytical form as

$$ x = x ( t) = \ A \cos ( \omega t - \alpha ) = \ \mathop{\rm Re} [ Be ^ {i \omega t } ], $$

where $ x = x( t) $ is the value of the vibrating magnitude at the moment of time $ t $, $ | A | = | B | $ is the amplitude, $ \omega $ is the periodic (circular) frequency, and $ \alpha $ is the initial phase of the vibration. The duration of one complete vibration $ T = 2 \pi / \omega $ is called the period of the harmonic vibration, while $ \nu = 1/T $, which is the number of complete vibrations performed in unit time, is known as the frequency of the harmonic vibration ( $ \omega = 2 \pi \nu $). The period of the harmonic vibration is independent of its amplitude. The velocity, acceleration and all higher derivatives of the vibrating magnitude vary harmonically at the same frequency. A harmonic vibration is represented as an ellipse on the phase plane $ ( x, \dot{x} ) $. Owing to the dissipation of energy, perfect harmonic vibrations are not encountered in nature, but many processes are close to harmonic vibrations. These include small vibrations of mechanical systems with respect to their equilibrium position. The resulting frequencies (the so-called eigen frequencies) of the vibrations are independent of the initial conditions of motion and are determined by the nature of the vibrating system itself. For instance, small vibrations (under the effect of gravity) of a mathematical pendulum on a thread of length $ l $ are described by the differential equation

$$ ml \dot{x} dot = - mgx, $$

where $ g $ is the gravity acceleration and $ x( t) $ is the angle between the vertical and the thread of the pendulum. The general solution of this equation has the form $ x = A \cos ( \omega t - \alpha ) $, where the eigen frequency of the vibration, $ \omega = \sqrt g/l $, depends on $ g $ and $ l $ only, while the amplitude $ A $ and the phase $ \alpha $ are constants of integration, selected in accordance with the initial conditions.

Harmonic vibrations play an important part in the study of vibrations as a whole, since complicated periodic and almost-periodic varying magnitudes may be approximately represented, to any desired degree of accuracy, by a sum of harmonic vibrations. Mathematically this corresponds to the approximations of functions by trigonometric series and by Fourier integrals (cf. Fourier integral).

The classical Fourier series

$$ x ( t) = \ \sum _ {n = - \infty } ^ \infty a _ {n} e ^ {i nt } $$

of a complex-valued function $ x( t) $, defined on $ [ - \pi , \pi ] $, may be regarded as the expansion of $ x( t) $ into a sum of harmonic vibrations with integer frequencies $ n = 0, \pm 1, \pm 2 ,\dots $. The Fourier coefficient

$$ a _ {n} = { \frac{1}{2 \pi } } \int\limits _ {- \pi } ^ \pi x ( t) e ^ {- i n t } dt $$

determines the amplitude $ ( | a _ {n} | ) $ and the phase shift $ ( \mathop{\rm arg} a _ {n} ) $ of a harmonic vibration with frequency $ n $. The totality of all Fourier coefficients determines the spectrum of $ x( t) $ and shows the harmonic vibrations which are actually involved in $ x( t) $, as well as the amplitudes and the initial phases of these vibrations. Knowing the spectrum is equivalent to knowing the function $ x( t) $.

A function $ x( t) $ defined on $ ( - \infty , \infty ) $ can no longer be built from harmonic vibrations with integer frequencies. Its construction involves vibrations of all frequencies: The function $ x( t) $ can be represented by a Fourier integral:

$$ x ( t) = \int\limits _ {- \infty } ^ \infty a ( n) e ^ {i nt } dn ; $$

where

$$ a ( n) = { \frac{1}{2 \pi } } \int\limits _ {- \infty } ^ \infty x ( t) e ^ {- in t } dt $$

is the spectral density of $ x( t) $.

These representations of functions form the base of the Fourier method for solving various problems in the theory of differential and integral equations.

References

[1] G.S. Gorelik, "Oscillations and waves" , Moscow-Leningrad (1950) (In Russian)

Comments

References

[a1] J.W.S. Rayleigh, "The theory of sound" , 1 , Dover, reprint (1945)
How to Cite This Entry:
Harmonic vibration. Encyclopedia of Mathematics. URL: http://encyclopediaofmath.org/index.php?title=Harmonic_vibration&oldid=15778
This article was adapted from an original article by L.P. Kuptsov (originator), which appeared in Encyclopedia of Mathematics - ISBN 1402006098. See original article