= (V2)1/2 K πGOO ' Consider the dispersion relation of a linear spiral density wave perturbation (equation 4.45 in Chapter 3 of the lecture notes). The Toomre's parameter is defined as Q where (V2) 1/2 is the root-mean-square turbulent plus thermal velocity, к the epicyclic frequency, σ the unperturbed surface density of the disc and G the gravitational constant. For Q = 1/√2, show that the spiral pattern is unstable if К (√2-1) (V²² ) 1/2 < |k| < (√√2+1) where k is the wavenumber of the perturbation. К (V+2)1/2

University Physics Volume 2
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Chapter2: The Kinetic Theory Of Gases
Section: Chapter Questions
Problem 97CP: Verify the normalization equation 0f(v)dv=1 In doing the integral, first make substitution...
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=
(V2)1/2 K
πGOO
'
Consider the dispersion relation of a linear spiral density wave perturbation (equation 4.45 in
Chapter 3 of the lecture notes). The Toomre's parameter is defined as Q
where
(V2) 1/2 is the root-mean-square turbulent plus thermal velocity, к the epicyclic frequency, σ the
unperturbed surface density of the disc and G the gravitational constant. For Q = 1/√2, show
that the spiral pattern is unstable if
К
(√2-1)
(V²² ) 1/2 < |k| < (√√2+1)
where k is the wavenumber of the perturbation.
К
(V+2)1/2
Transcribed Image Text:= (V2)1/2 K πGOO ' Consider the dispersion relation of a linear spiral density wave perturbation (equation 4.45 in Chapter 3 of the lecture notes). The Toomre's parameter is defined as Q where (V2) 1/2 is the root-mean-square turbulent plus thermal velocity, к the epicyclic frequency, σ the unperturbed surface density of the disc and G the gravitational constant. For Q = 1/√2, show that the spiral pattern is unstable if К (√2-1) (V²² ) 1/2 < |k| < (√√2+1) where k is the wavenumber of the perturbation. К (V+2)1/2
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