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Introduction to Astrophysical Gas Dynamics

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Title: Introduction to Astrophysical Gas Dynamics


1
Introduction to Astrophysical Gas Dynamics
Part 3
  • Bram Achterberg
  • a.achterberg_at_astro.uu.nl

2
Waves
3
Astrophysical manifestations of waves
Spiral Density Waves
Solar Oscillations
Large-Scale Structure
Accretion DiskWaves
4
Simple (linear) waves
  • Properties
  • Small perturbations of velocity, density and
    pressure
  • Periodic behavior (sines and cosines) in
    space and time
  • No effect of boundary conditions

5
Perturbations
Perturbations are small
Perturbations are periodic the plane wave
assumption!
with displacement vector
6
Perturbation analysis simple mechanical example
  • Small-amplitude
  • motion
  • Valid in the vicinity
  • of an equilibrium
  • position

7
Perturbation analysisfundamental equations
Equilibrium position
8
Perturbation analysismotion near x0
Taylor expansion
Near x0
9
Perturbation analysismotion near x0
Equation of motion near x0
10
Perturbation analysismotion near x0
Solutions
11
Waves, wavelength and the wave vector
12
Who measures what?
Two fundamental types of observer Observer
fixed to coordinate system measures the Eulerian
perturbation Observer moving with the
flow Measured the Lagrangian perturbation
13
Lagrangian labels
Lagrangian Labels are carried along by the flow
Conventional choice position fluid-element at
some reference time
14
Re-interpretation of time-derivatives
At a fixed position
Comoving with the flow
Lagrangian and Eulerian perturbations
Lagrangian
Eulerian
15
What does it all mean?
  • If you observe from a fixed position in space,
    and
  • a small-amplitude wave passes, you measure
  • A pressure perturbation ?P
  • A density perturbation ??
  • A velocity perturbation ?V
  • If you observe while moving along with the
    unperturbed
  • flow, and a small-amplitude wave passes, you
    measure
  • A pressure perturbation ?P
  • A density perturbation ??
  • A velocity perturbation ?V

16
Relation between the two perturbations
Effect of the position shift of the co-moving
observer
17
Important Commutation Relationsfor taking
derivatives
18
Important Commutation Relationsfor taking
derivatives
Small perturbations in position fluid-element
Associated variations
19
Important Commutation Relationsfor taking
derivatives
Small perturbations in Position fluid-element
General relation between Lagrangian and
Eulerian Changes
Associated variations
20
Important Commutation Relationsfor taking
derivatives
Small perturbations in Position fluid-element
General relation between Lagrangian and
Eulerian Changes
Associated variations
21
Application velocity perturbation due to
small-amplitude wave
Commutation Rules
22
Application velocity perturbation due to
small-amplitude wave
Commutation Rules
Definition comoving derivative
23
Eulerian and Lagrangian velocity perturbations
General relation between the two kinds of
perturbations
24
Density perturbations and the deformation tensor
A ?X , B ?Y, C ?Z
The vectors A, B and C are carried along, and
deformed by the flow!
25
Definition Deformation Tensor Dij
Small position change
Associated change in position differences
Same animal In tensor notation
26
Small displacement (e.g. wave motion)
Component notation
27
Small displacement (e.g. wave motion)
Component notation
Matrix notation
28
Physical Interpretation of the components of
the Deformation Tensor
29
Deformation of an infinitesimal volume-element
After deformation
Before deformation
30
Density variation from mass conservation volume
change law
Starting volume orthogonal cube
Deformation due to displacement
New, non-orthogonal volume
31
Mathematical IntermezzoDeterminants, vector
products and the totally antisymmetric
Levi-Cevita symbol
32
Properties of Levi-Cevita synbol
Also useful the vector cross-product in
?-language
33
Volume change in terms of deformation
Alternative notation cross-product
New (deformed) volume
34
Volume change in terms of deformation
Alternative notation cross-product
New (deformed) volume
35
Volume change in terms of deformation
Alternative notation cross-product
New (deformed) volume
Summation convention for repeated indices i, j
and k!
36
Deformation tensor determinant
Definition of the Deformation Tensor
Definition of the determinant of the Deformation
Tensor
37
Deformation tensor determinant
Definition of the Deformation Tensor
Definition of the determinant of the Deformation
Tensor
38
Deformation tensor determinant
Definition of the Deformation Tensor
Definition of the determinant of the Deformation
Tensor
If displacement is small
39
Density perturbation
Relation between old and new (deformed) volume
Deformation Tensor determinant
Definition divergence
40
Density perturbation
New volume
Mass conservation
41
Density perturbation
New volume
Mass conservation
New density
42
Lagrangian and Eulerian density change
43
Lagrangian and Eulerian density change
Lagrangian and Eulerian pressure change
44
Summary changes due to a small displacement
45
Linear sound waves in a homogeneous, stationary
gas
  • Main assumptions
  • Gas is uniform no gradients in density,
    pressure or
  • temperature
  • Gas is stationary without the presence of waves
  • the gas velocity vanishes
  • The velocity, density and pressure perturbations
  • associated with the waves are small

46
Uniform background no differencebetween
Lagrangian and Eulerian perturbations!!!!
Vanishes if Q is uniform in absence of waves
47
Aim
To derive a linear equation of motion for the
displacement vector ??(x,t) by linearizing
the equation of motion for the gas.
Method
Take the Lagrangian variation of the equation of
motion.
48
Perturbing the Equation of Motion
To find the equation of motion governing
small perturbations you have to perturb the
equation of motion!
49
Unperturbed gas is uniform and at rest
Apply a small displacement
50
Unperturbed gas is uniform and at rest
Apply a small displacement
Because the unperturbed state is so simple, the
linear perturbations in density, pressure and
velocity are also simple!
51
Effect of linear perturbations on the equation
of motion
Use commutation rules
52
Effect of linear perturbations on the equation
of motion
Use commutation rules
53
Effect of linear perturbations on the equation
of motion
54
Effect of linear perturbations on the equation
of motion
55
Effect of linear perturbations on the equation
of motion
56
What have we learned about smallperturbations in
a ideal uniform gas?
Small displacement of fluid elements
Equation of motion for the displacement vector
57
The wave equation and its solution
Linearized equation of motion wave equation
Definition sound speed Cs2 ? P / ?
58
The wave equation and its solution
Linearized equation of motion wave equation
Definition sound speed Cs2 ? P / ?
Trial solution plane wave
Handy because
59
Example relations between perturbations and the
wave amplitude
60
Example relations between perturbations and the
wave amplitude
61
H
H
L
L
L
62
Plane-wave solution
Wave equation
63
Plane-wave solution
Wave equation
Algebraic relation
64
Plane-wave solution
Wave equation
Algebraic relation
Matrix form (assume kz 0)
65
Wave dispersion relation for ?
Algebraic wave equation three linear equations
66
Wave dispersion relation for ?
Algebraic wave equation three linear equations
Solution condition vanishing determinant
67
Wave dispersion relation for ?
Dispersion relation
68
Wave polarization direction of a
69
Alternative derivation of the wave properties
Wave equation
70
Alternative derivation of the wave properties
Wave equation
Divergence of a gradient is the Laplace operator!
71
Alternative derivation of the wave properties
Wave equation
Pressure perturbation
Sound waves are pressure waves!
72
Alternative derivation of the wave properties
Wave equation
Rotation of a gradient vanishes!
73
Alternative derivation of the wave properties
Wave equation
Dispersion relation for compressive perturbations
74
Alternative derivation of the wave properties
Wave equation
Dispersion relation for divergence-free
perturbations
75
Summary the road to sound waves
Assume a small displacement Calculate linear
response of fluid Find linear
equation-of-motion for the perturbations
76
Plane wave assumption convert a partial
differential equation into algebraic equations
77
Plane wave assumption convert a partial
differential equation into algebraic equations
Condition for non-trivial solutions
78
Sound waves in a moving medium
  • Assumptions
  • Uniform pressure and density in unperturbed flow
  • Constant flow velocity in unperturbed flow

Main effect of flow appearance of the comoving

time-derivative in equations
79
Use comoving derivative
80
Wave equation
Use comoving derivative
81
Wave equation
Plane wave assumption
Use comoving derivative
Doppler-shifted frequency
82
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83
Phase- and group velocity
Central concepts Phase velocity velocity with
which surfaces of constant
phase move Group velocity velocity with which
slow modulations of the
wave amplitude move
84
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85
Phase velocity
Definition phase S
86
Phase velocity
Definition phase S
Definition phase-velocity
87
Phase velocity
Definition phase S
Definition phase-velocity
88
Group Velocity
Wave-packet, Fourier Integral
89
Group Velocity
Wave-packet, Fourier Integral
Phase factor x effective amplitude
90
Group Velocity
Wave-packet, Fourier Integral
Phase factor x effective amplitude
Constructive interference in integral
91
Summary and example sound waves
92
Summary and example sound waves
93
Summary and example sound waves
94
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95
Summary the path to linear (small-amplitude)
waves
  • Calculate the density- and pressure
    perturbations
  • given a small displacement
  • Find the equation of motion for the displacement
  • by perturbing the equation of motion
  • Substitute a plane-wave for the perturbation
  • 4. Solve the resulting algebraic set of equations.
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