SSC/Stability/NeutralMode

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LAWE

Most General Form

In an accompanying discussion, we derived the so-called,

Adiabatic Wave (or Radial Pulsation) Equation

d2xdr02+[4r0(g0ρ0P0)]dxdr0+(ρ0γgP0)[ω2+(43γg)g0r0]x=0

where the gravitational acceleration,

g0

GMrr02=1ρ0dP0dr0g0ρ0r0P0=dlnP0dlnr0.

The solution to this equation gives eigenfunctions that describe various radial modes of oscillation in spherically symmetric, self-gravitating fluid configurations. The boundary condition conventionally used in connection with the adiabatic wave equation is,

r0dlnxdr0

=

1γg(43γg+ω2R3GMtot)        at         r0=R.

Polytropic Configurations

Part 1

If the initial, unperturbed equilibrium configuration is a polytropic sphere whose internal structure is defined by the function, θ(ξ), that provides a solution to the,

Lane-Emden Equation

1ξ2ddξ(ξ2dΘHdξ)=ΘHn

then,

r0

=

anξ,

ρ0

=

ρcθn,

P0

=

Kρ0(n+1)/n=Kρc(n+1)/nθn+1,

g0

=

GM(r0)r02=Gr02[4πan3ρc(ξ2dθdξ)],

where,

an

=

[(n+1)K4πGρc(1n)/n]1/2.

Hence, after multiplying through by an2, the above adiabatic wave equation can be rewritten in the form,

d2xdξ2+[4ξg0an(an2ρ0P0)]dxdξ+(an2ρ0γgP0)[ω2+(43γg)g0anξ]x

=

0.

In addition, given that,

g0an

=

4πGρc(dθdξ),

and,

an2ρ0P0

=

(n+1)(4πGρc)θ=an2ρcPcθcθ,

we can write,

0

=

d2xdξ2+[4(n+1)V(ξ)ξ]dxdξ+[ω2(an2ρcγgPc)θcθ(34γg)(n+1)V(x)ξ2]x

 

=

d2xdξ2+[4(n+1)V(ξ)ξ]dxdξ+(n+1)[ω2(an2ρcγgPc)ξ2θc(n+1)θ(34γg)V(x)]xξ2

where we have adopted the function notation,

V(ξ)

ξθdθdξ.

Part 2

Drawing from an accompanying discussion, we have the following:

Polytropic LAWE (linear adiabatic wave equation)

0=d2xdξ2+[4(n+1)Q]1ξdxdξ+(n+1)[(σc26γg)ξ2θαQ]xξ2

where:    Q(ξ)dlnθdlnξ,    σc23ω22πGρc,     and,     α(34γg)

In order to reconcile with the "Part 1" expression, we note first that V(ξ)Q(ξ). We note as well that since,

(an2ρcPc)θc

=

(n+1)4πGρc,

we have,

ω2(an2ρcγgPc)ξ2θc(n+1)θ

ω2γg[(n+1)4πGρc]ξ2(n+1)θ=16γg[3ω22πGρc]ξ2θ=(σc26γg)ξ2θ.

All physically reasonable solutions are subject to the inner boundary condition,

dxdξ=0         at         ξ=0,

but the relevant outer boundary condition depends on whether the underlying equilibrium configuration is isolated (surface pressure is zero), or whether it is a "pressure-truncated" configuration. As is the case with the pressure-truncated isothermal spheres, discussed above, if the polytropic configuration is truncated by the pressure, Pe, of a hot, tenuous external medium, then the solution to the LAWE is subject to the outer boundary condition,

dlnxdlnξ=3         at         ξ=ξ~.

But, for isolated polytropes, the sought-after solution is subject to the more conventional boundary condition,

dlnxdlnξ=(3nn+1)+nσc26(n+1)[ξθ']         at         ξ=ξsurf.

Radial Pulsation Neutral Mode

Background

The integro-differential version of the statement of hydrostatic balance is

dPdr=GMrρr2

From our separate discussion, we have found that,

Exact Solution to the (3n<) Polytropic LAWE

σc2=0

      and      

xP3(n1)2n[1+(n3n1)(1ξθn)dθdξ].

Let's rewrite the significant functional term in this expressions in terms of basic variables. That is,

(1ξθn)dθdξ

=

(anρcr0ρ0)g04πGρcan

 

=

M(r0)4πr03ρ0.

Trial Eigenfunction & Its Derivatives

Let's adopt the following trial solution:

xt

=

abMr4πr03ρ0=abg04πGr0ρ0.

Then we have,

(1b)dxtdr0

=

ddr0[Mr4πr03ρ0]

 

=

[14πr03ρ0]dMrdr0[Mr4πr03ρ02]dρ0dr0[3Mr4πr04ρ0]

 

=

1r0[3Mr4πr04ρ0][Mr4πr03ρ02]dρ0dr0

(1b)d2xtdr02

=

ddr0{1r0[3Mr4πr04ρ0][Mr4πr03ρ02]dρ0dr0}

 

=

1r02[34πr04ρ0]dMrdr0+[3Mr4πr04ρ02]dρ0dr0+4[3Mr4πr05ρ0]

 

 

[Mr4πr03ρ02]d2ρ0dr02[14πr03ρ02]dρ0dr0dMrdr0+[3Mr4πr04ρ02]dρ0dr0+[2Mr4πr03ρ03](dρ0dr0)2

 

=

4r02+3Mr4πr05ρ0[4+dlnρ0dlnr0]+1r02[3Mr4πr03ρ01]dlnρ0dlnr0[Mr4πr03ρ02]d2ρ0dr02+[2Mr4πr05ρ0](dlnρ0dlnr0)2.

Given that,

ΔMr4πr03ρ0

=

14πG(g0r0ρ0)=[P04πGr02ρ02dlnP0dlnr0],

these expression can be rewritten as,

(r02b)dxtdr0

=

r0{13ΔΔdlnρ0dlnr0},

and,

(r02b)d2xtdr02

=

4+3Δ[4+dlnρ0dlnr0]+[3Δ1]dlnρ0dlnr0Δ(r02ρ0)d2ρ0dr02+2Δ(dlnρ0dlnr0)2.

Plug Trial Eigenfunction Into LAWE

 

LAWE

d2xdr02+[4r0(g0ρ0P0)]dxdr0+(ρ0γgP0)[ω2+(43γg)g0r0]x=0


Plugging our trial radial displacement function, xt, into the LAWE gives,

LAWE

=

(r02b)d2xtdr02(r0b)[4+dlnP0dlnr0]dxtdr0(r02b)(ρ0γgP0)[(43γg)g0r0+σc2(2πGρc3)]xt

 

=

(r02b)d2xtdr02(r0b)[4+dlnP0dlnr0]dxtdr0+(1b)1γg(dlnP0dlnr0)(43γg)xt(r02b)(ρ0γgP0)[σc2(2πGρc3)]xt

 

=

4+3Δ[4+dlnρ0dlnr0]+[3Δ1]dlnρ0dlnr0Δ(r02ρ0)d2ρ0dr02+2Δ(dlnρ0dlnr0)2

 

 

+[4+dlnP0dlnr0]{13ΔΔdlnρ0dlnr0}+(1b)1γg(dlnP0dlnr0)(43γg)(abΔ)(1b)(ρ0r02γgP0)[σc2(2πGρc3)](abΔ).

Now, if we set σc2=0 and dlnP0/dlnr0=γg(dlnρ0/dlnr0), this expression becomes,

LAWE

=

4+3Δ[4+dlnρ0dlnr0]+[3Δ1]dlnρ0dlnr0Δ(r02ρ0)d2ρ0dr02+2Δ(dlnρ0dlnr0)2

 

 

+[4+dlnP0dlnr0]{13ΔΔdlnρ0dlnr0}+(1b)1γg(dlnP0dlnr0)(43γg)(abΔ)(1b)(ρ0r02γgP0)[σc2(2πGρc3)](abΔ).

Notice that the key components of this last term may be rewritten as,

(ρ0r02γgP0)[σc2(2πGρc3)]

=

(4πGρ02r02P0)[σc26γg(ρcρ0)]

 

=

(1Δ)dlnP0dlnr0[σc26γg(ρcρ0)].

So, for our trial eigenfunction, we have …

LAWE

=

[2Δ1]dlnρ0dlnr0Δ(r02ρ0)d2ρ0dr02+2Δ(dlnρ0dlnr0)2+dlnP0dlnr0{[13ΔΔdlnρ0dlnr0]+(43γg)γg[abΔ]+σc26γg(ρcρ0)[abΔ1]}.

Consider Polytropic Structures

Referring back to, for example, a separate review of polytropic structures, we recognize that,

Δ=14πG(g0r0ρ0)

=

1ξ3[(ξ2dθdξ)]θn=1ξ(dθdξ)θn=θ'ξθn,

dlnρ0dlnr0

=

n,

dlnP0dlnr0

=

(n+1).

Also,

(r02ρ0)d2ρ0dr02

=

(ξ2ρcθn)ddξ[nρcθn1θ']

 

=

(nξ2θn)[(n1)θn2(θ')2+θn1θ']

 

=

(nξ2θ2)[(n1)(θ')2+θθ']

 

=

(nξ2θ2)[(n1)(θ')2(θn+1+2θθ'ξ)]

 

=

(nξ2θ2)[(n1)(ξθnΔ)2+θn+1]

 

=

n(n1)(ξn+1θn1Δ)2+nξ2θn1.

Hence,

LAWE

=

n(2Δ1)Δ(r02ρ0)d2ρ0dr02+2n2Δ+(n+1)[13ΔnΔ]+(n+1){(43γg)γg[abΔ]+σc26γg(ρcρ0)[abΔ1]}

 

=

2nΔn+2n2Δ+n3nΔn2Δ+13ΔnΔΔ(r02ρ0)d2ρ0dr02+(n+1){(43γg)γg[abΔ]+σc26γg(ρcρ0)[abΔ1]}

 

=

1+n2Δ(2n+3)ΔΔ(r02ρ0)d2ρ0dr02+(n+1)[4γg3][abΔ]+(n+1){σc26γg(ρcρ0)[abΔ1]}.

If, γg=(n+1)/n, we can further simplify and obtain,

LAWE

=

1+n2Δ(2n+3)ΔΔ(r02ρ0)d2ρ0dr02+[n3][abΔ]+(n+1){σc26γg(ρcρ0)[abΔ1]}

 

=

1+(n3)ab+n2Δ+(3n)Δ(2n+3)ΔΔ(r02ρ0)d2ρ0dr02+(n+1){σc26γg(ρcρ0)[abΔ1]}

Try Again

General Form of Wave Equation

 

LAWE

d2xdr02+[4r0(g0ρ0P0)]dxdr0+(ρ0γgP0)[ω2+(43γg)g0r0]x=0

Employing the substitutions,

σc2

3ω22πGρc,

α

34γg=3nn+1,

g0

GMrr02=1ρ0dP0dr0g0ρ0r0P0=dlnP0dlnr0,

Δ

Mr4πr03ρ0=14πG(g0r0ρ0)=[P04πGr02ρ02dlnP0dlnr0],

we have,

LAWE =

d2xdr02+1r0[4g0ρ0r0P0]dxdr0+[(4γg3)g0ρ0r0P0]xr02+(ρ0P0)[4πGρc(σc26γg)]x

  =

d2xdr02+1r0[4+dlnP0dlnr0]dxdr0+[αdlnP0dlnr0]xr021Δ[dlnP0dlnr0ρcρ0(σc26γg)]xr02.


In the context of polytropic configurations (see more below), we appreciate that,

ρ0ρc =

θn,

dlnP0dlnr0 =

(n+1)dlnθdlnξ=(n+1)Q,      and,

1ΔdlnP0dlnr0 =

(n+1)ξ2θn1.

Inserting these into the LAWE expression and multiplying through by the square of the polytropic length scale, an2, we obtain,

LAWE =

d2xdξ2+1ξ[4(n+1)Q]dxdξ[α(n+1)Q]xξ2+[(n+1)ξ2θ(σc26γg)]xξ2.


This is identical to what has been referred to in a separate discussion, as the

Polytropic LAWE

0=d2xdξ2+[4(n+1)Q]1ξdxdξ+(n+1)[(σc26γg)ξ2θαQ]xξ2

where:    Q(ξ)dlnθdlnξ,    σc23ω22πGρc,     and,     α(34γg)

Derivatives of Δ

Here we evaluate the first derivative of Δ with respect to r0,

dΔdr0 =

ddr0{Mr4πr03ρ0}

  =

14πr03ρ0dMrdr03Mr4πr04ρ0Mr4πr03ρ02dρ0dr0

  =

1r03Mr4πr04ρ0Mr4πr03ρ02dρ0dr0

  =

1r0{1Δ[3+dlnρ0dlnr0]}

r0dΔdr0 =

[13ΔΔdlnρ0dlnr0];

and the second derivative of Δ with respect to r0,

d2Δdr02 =

ddr0{1r0}ddr0{3Mr4πr04ρ0}ddr0{Mr4πr03ρ02dρ0dr0}

  =

1r0234π{1r04ρ0dMrdr04Mrr05ρ0Mrr04ρ02dρ0dr0}

   

14π{1r03ρ02dρ0dr0dMrdr03Mrr04ρ02dρ0dr02Mrr03ρ03[dρ0dr0]2+Mrr03ρ02d2ρ0dr02}

  =

1r023r02{1Δ[4+dlnρ0dlnr0]}1r02{[13Δ]dlnρ0dlnr02Δ[dlnρ0dlnr0]2+Δ(r02ρ0)d2ρ0dr02}

r02d2Δdr02 =

1+33Δ[4+dlnρ0dlnr0]+[13Δ]dlnρ0dlnr02Δ[dlnρ0dlnr0]2+Δ(r02ρ0)d2ρ0dr02

  =

412Δ+[16Δ]dlnρ0dlnr02Δ[dlnρ0dlnr0]2+Δ(r02ρ0)d2ρ0dr02.

Trial Eigenfunction

As above, let's adopt a trial eigenfunction of the form,

xt

=

abMr4πr03ρ0=abΔ.

Then we have,

1b[r02×LAWE]trial =

r02d2Δdr02[4+dlnP0dlnr0]r0dΔdr0+[αdlnP0dlnr0](abΔ)1Δ[dlnP0dlnr0ρcρ0(σc26γg)](abΔ)

  =

{412Δ+[16Δ]dlnρ0dlnr02Δ[dlnρ0dlnr0]2+Δ(r02ρ0)d2ρ0dr02}[4+dlnP0dlnr0][13ΔΔdlnρ0dlnr0]

   

+[αdlnP0dlnr0](abΔ)1Δ[dlnP0dlnr0ρcρ0(σc26γg)](abΔ).

Assume Polytropic Relations

If we assume that the equilibrium models are polytropes, then we know that,

ρ0θn

           

dlnρ0dlnr0=ndlnθdlnξ;

P0θn+1

           

dlnP0dlnr0=(n+1)dlnθdlnξ.

We also deduce that,

(r02ρ0)d2ρ0dr02

=

(ξ2θn)ddξ[dθndξ]

 

=

(ξ2θn)ddξ[nθn1θ']

 

=

(nξ2θn)[(n1)θn2(θ')2+θn1θ']

 

=

[n(n1)ξ2θ2](θ')2(nξ2θ)[θn+2ξθ']

 

=

n(n1)[dlnθdlnξ]2nξ2θn12ndlnθdlnξ

 

=

n(n1)Ξ2nξ2θn12nΞ,

where we have introduced the shorthand notation,

Ξ

dlnθdlnξ.


Drawing from our accompanying discussion, for example, we note as well that,

Δ

=

[P04πGr02ρ02dlnP0dlnr0]

1ΔdlnP0dlnr0

=

4πGr02ρ02P0

 

=

4πG(an2ξ2)(ρcθn)2[K1ρc(n+1)/nθ(n+1)]

 

=

4πG[(n+1)K4πGρc(1n)/n](ρc)2[K1ρc(n+1)/n]ξ2θ(n1)

 

=

(n+1)ξ2θ(n1)

Δξ2θn1

=

1(n+1)dlnP0dlnr0=Ξ.

Hence,

1b[r02×LAWE]trial =

412Δ+[16Δ]nΞ2Δ[nΞ]2+Δ[n(n1)Ξ2nξ2θn12nΞ][4+(n+1)Ξ][13ΔΔnΞ]

   

+[α(n+1)Ξ](abΔ)1Δ[(n+1)Ξρcρ0(σc26γg)](abΔ)

  =

nΞ6ΔnΞ2Δ[nΞ]2+Δ[n(n1)Ξ2nξ2θn1+2nΞ]+2(n+1)Ξ+n(n+1)Ξ2Δ

   

+[α(n+1)Ξ](ab)[α(n+1)Ξ]Δ1Δ[(n+1)Ξρcρ0(σc26γg)](abΔ)

  =

Ξ[1+n+2(n+1)+α(n+1)(ab)]+Δ[[4n+α(n+1)]Ξ+n(n1)Ξ2+n(n+1)Ξ22n2Ξ2]

   

1Δ[(n+1)Ξρcρ0(σc26γg)](abΔ)

  =

Ξ[3(n+1)+α(n+1)(ab)]Δ[4n+α(n+1)]Ξ1Δ[(n+1)Ξρcρ0(σc26γg)](abΔ)

Third Time

General Relations

Various general relations taken from above derivations:

LAWE =

d2xdr02+1r0[4+dlnP0dlnr0]dxdr0+[αdlnP0dlnr0]xr021Δ[dlnP0dlnr0ρcρ0(σc26γg)]xr02,

where,

Δ

Mr4πr03ρ0

1ΔdlnP0dlnr0 =

4πGr02ρ02P0;

r0dΔdr0 =

[13ΔΔdlnρ0dlnr0];

r02d2Δdr02 =

412Δ+[16Δ]dlnρ0dlnr02Δ[dlnρ0dlnr0]2+Δ(r02ρ0)d2ρ0dr02.

Polytropes

If polytropic relations are adopted:

Δ =

Qξ2θn1;

1ΔdlnP0dlnr0 =

(n+1)ξ2θn1;

r02×LAWE =

r02d2xdr02+[4(n+1)Q]r0dxdr0+[(n3)Q]x+1Δ[(n+1)Q1θn(σc26γg)]x;

r0dΔdr0 =

[13Δ+nΔQ]=1+(nQ3)Δ;

r02d2Δdr02 =

412Δn[16Δ]Q2n2ΔQ2+Δ(r02ρ0)d2ρ0dr02

  =

412Δn[16Δ]Q2n2ΔQ2+Δ[n(n1)Q2+2nQnQΔ]

  =

4nQ12Δ+6nQΔ2n2ΔQ2+Δ[n(n1)Q2+2nQ]nQ

  =

42nQ+Δ[6nQ2n2Q2+n(n1)Q2+2nQ12].

  =

42nQ+Δ[8nQn2Q2nQ212].

Eigenfunction Choice

Again, let's try the trial eigenfunction,

xt =

abΔ,

in which case,

1b[r02×LAWE] =

r02d2Δdr02[4(n+1)Q]r0dΔdr0+[(n3)Q](abΔ)+1Δ[(n+1)Q1θn(σc26γg)](abΔ)

  =

42nQ+Δ[8nQn2Q2nQ212][4(n+1)Q][1+(nQ3)Δ]+[(n3)Q](abΔ)

   

+1Δ[(n+1)Q1θn(σc26γg)](abΔ)

  =

42nQ+Δ[8nQn2Q2nQ212]4(4nQ12)Δ+(n+1)Q+(n+1)(nQ23Q)Δ+(n3)Q(ab)(n3)QΔ

   

+1Δ[(n+1)Q1θn(σc26γg)](abΔ)

  =

[(n+1)2n+(n3)(ab)]Q+Δ[8nQn2Q2nQ2124nQ+12+(n+1)(nQ2)3Q(n+1)+(3n)Q]

   

+1Δ[(n+1)Q1θn(σc26γg)](abΔ)

  =

[(1n)+(n3)(ab)]Q+Δ[0]+1Δ[(n+1)Q1θn(σc26γg)](abΔ).

Hence, we are left with only the σc2 term if we set,

0 =

(1n)+(n3)(ab)

(ab) =

n1n3.

We conclude, therefore, that the radial displacement function (i.e., the eigenfunction) for the neutral (σc2=0) mode of all polytropic configurations is,

xneutral =

1b[n1n3Δ]=1b[n1n3Qξ2θn1]

  =

1b(n1n3)[1+(n3n1)1ξ2θn1dlnθdlnξ]

  =

1b(n1n3)[1+(n3n1)1ξθndθdξ].

This last expression exactly matches our earlier result found for polytropic configurations if we choose an overall amplitude coefficient of the form,

b =

2n3(n3).

Hooray!

Summary

Setup

We begin with the traditional,

Adiabatic Wave (or Radial Pulsation) Equation

d2xdr02+[4r0(g0ρ0P0)]dxdr0+(ρ0γgP0)[ω2+(43γg)g0r0]x=0

This linear, adiabatic wave equation (LAWE) can straightforwardly be rewritten in the form we will refer to as the,

Δ-Highlighted LAWE

0=d2xdr02+1r0[4+dlnP0dlnr0]dxdr0+[(34γg)dlnP0dlnr0]xr021Δ[dlnP0dlnr0ρcρ0(σc26γg)]xr02

where:    ΔMr4πr03ρ0,    σc23ω22πGρc

Multiplying this Δ-Highlighted LAWE through by an2=(r0/ξ)2 and recognizing that, for polytropic configurations,

Δ =

1ξ2θn1dlnθdlnξ,

        dlnP0dlnr0 =

(n+1)dlnθdlnξ,

        1ΔdlnP0dlnr0 =

(n+1)ξ2θn1,

we immediately obtain what we have frequently referred to as the,

Polytropic LAWE

0=d2xdξ2+[4(n+1)Q]1ξdxdξ+(n+1)[(σc26γg)ξ2θαQ]xξ2

where:    Q(ξ)dlnθdlnξ,    σc23ω22πGρc,     and,     α(34γg)

Neutral-Mode Eigenfunction

In the preceding subsections of this chapter, we have demonstrated that if

γg=n+1n

α=3nn+1,

the radial displacement function (i.e., the eigenfunction) for the neutral (σc2=0) mode of all polytropic configurations is,

xneutral =

3(n3)2n[n1n3Δ],

to within an arbitrarily chosen leading scaling coefficient. More completely, if we let "LAWE" stand for the RHS of our Δ-Highlighted LAWE, then setting x=xneutral results in the expression,

1b[r02×LAWE] =

(n+1)Q1θn(σc26γg)[1Δ(n1n3)1]

  =

(n+1)(σc26γg)[ξ2θ(n1n3)1θndlnθdlnξ],

which goes to zero if σc2=0.

Parabolic Density Distribution

Here, we build upon our separate discussion of equilibrium configurations with a parabolic density distribution.

Equilibrium Structure

In an article titled, "Radial Oscillations of a Stellar Model," C. Prasad (1949, MNRAS, 109, 103) investigated the properties of an equilibrium configuration with a prescribed density distribution given by the expression,

ρ0=ρc[1(r0R)2],

where, ρc is the central density and, R is the radius of the star. Both the mass distribution and the pressure distribution can be obtained analytically from this specified density distribution. Specifically,

Mr

=

0r04πr02ρ0dr0

 

=

4πρcr033[135(r0R)2],

in which case we can write,

g0GMrr02

=

4πGρcr03[135(r0R)2],

and,

ΔMr4πr03ρ0

=

13[135(r0R)2][1(r0R)2]1.

Hence, proceeding via what we have labeled as "Technique 1", and enforcing the surface boundary condition, P(R)=0, Prasad (1949) determines that,

P0

=

4πGρc2R215[1(r0R)2]2[112(r0R)2],

where, it can readily be deduced, as well, that the central pressure is,

Pc=4π15Gρc2R2.

Some Relevant Structural Derivatives

We note for later use that,

1PcdP0dr0

=

[1(r0R)2]2ddr0[112(r0R)2]+[112(r0R)2]ddr0[1(r0R)2]2

 

=

12R2[1(r0R)2]2ddr0[r02]+2[1(r0R)2][112(r0R)2]ddr0[1(r0R)2]

 

=

{12R2[1(r0R)2]22R2[1(r0R)2][112(r0R)2]}ddr0[r02]

 

=

r0R2{[1(r0R)2]2+4[1(r0R)2][112(r0R)2]}

 

=

r0R2{[1(r0R)2]+4[112(r0R)2]}[1(r0R)2]

 

=

5r0R2[135(r0R)2][1(r0R)2].

Hence,

dlnP0dlnr0=r0P0/Pc[1PcdP0dr0]

=

5r02R2[135(r0R)2][1(r0R)2]{[1(r0R)2]2[112(r0R)2]}1

 

=

5(r0R)2[135(r0R)2][1(r0R)2]1[112(r0R)2]1;

and, given that,

Δ1

=

3[135(r0R)2]1[1(r0R)2],

we can write,

1ΔdlnP0dlnr0

=

15(r0R)2[135(r0R)2][1(r0R)2]1[112(r0R)2]1[135(r0R)2]1[1(r0R)2]

 

=

15(r0R)2[112(r0R)2]1.

Also,

3dΔdr0

=

ddr0{[135(r0R)2][1(r0R)2]1}

 

=

[135(r0R)2]ddr0[1(r0R)2]1+[1(r0R)2]1ddr0[135(r0R)2]

 

=

[135(r0R)2][1(r0R)2]22r0R2+[1(r0R)2]1[65r0R2]

 

=

r0R2{2[135(r0R)2][1(r0R)2]265[1(r0R)2]1}

 

=

r05R2[1(r0R)2]2{[106(r0R)2][66(r0R)2]}

 

=

4r05R2[1(r0R)2]2

dΔdr0

=

4r015R2[1(r0R)2]2;

and,

15R24d2Δdr02

=

[1(r0R)2]22r0[1(r0R)2]3[2r0R2]

 

=

[1(r0R)2]3{[1(r0R)2]+4r02R2}

 

=

[1(r0R)2]3[1+3(r0R)2].

Neutral Mode

Again, adopting the trial eigenfunction,

xt =

abΔ,

from the,

Δ-Highlighted LAWE

0=d2xdr02+1r0[4+dlnP0dlnr0]dxdr0+[(34γg)dlnP0dlnr0]xr021Δ[dlnP0dlnr0ρcρ0(σc26γg)]xr02

where:    ΔMr4πr03ρ0,    σc23ω22πGρc

we can write,

LAWE =

bd2Δdr02br0[4+dlnP0dlnr0]dΔdr0+α[dlnP0dlnr0](abΔ)r021Δ[dlnP0dlnr0ρcρ0(σc26γg)](abΔ)r02

First Attempt

1b[r02×LAWE] =

r02d2Δdr02r0[4+dlnP0dlnr0]dΔdr0+α[dlnP0dlnr0](abΔ)1Δ[dlnP0dlnr0ρcρ0(σc26γg)](abΔ)

  =

r02d2Δdr02

   

r0[4+dlnP0dlnr0]dΔdr0

   

+α[dlnP0dlnr0](abΔ)

   

+ρcρ0(σc26γg){[dlnP0dlnr0]ab[1ΔdlnP0dlnr0]}

  =

415(r0R)2[1(r0R)2]3[1+3(r0R)2]

   

1615(r0R)2[1(r0R)2]2415(r0R)2{5(r0R)2[135(r0R)2][1(r0R)2]1[112(r0R)2]1}[1(r0R)2]2

   

+α{5(r0R)2[135(r0R)2][1(r0R)2]1[112(r0R)2]1}{abΔ}

   

+ρcρ0(σc26γg){[dlnP0dlnr0]ab[1ΔdlnP0dlnr0]}

  =

43(r0R)2[115(r0R)2][1(r0R)2]3

   

+43(r0R)4[135(r0R)2][112(r0R)2]1[1(r0R)2]3

   

+5α3(r0R)2[135(r0R)2][1(r0R)2]2[112(r0R)2]1{13ab35(r0R)2}

   

+ρcρ0(σc26γg){[dlnP0dlnr0]ab[1ΔdlnP0dlnr0]}

  =

43(r0R)2[115(r0R)2][1(r0R)2]3+5α3(r0R)2[135(r0R)2][1(r0R)2]2[112(r0R)2]1(13ab)

   

+43(r0R)4[135(r0R)2][112(r0R)2]1[1(r0R)2]3α(r0R)4[135(r0R)2][1(r0R)2]2[112(r0R)2]1

   

+ρcρ0(σc26γg){[dlnP0dlnr0]ab[1ΔdlnP0dlnr0]}

Continuing …

1b[r02×LAWE] =

(r0R)2[1(r0R)2]3[112(r0R)2]1{5α3(13ab)[135(r0R)2][1(r0R)2]43[115(r0R)2][112(r0R)2]}

   

+(43α)(r0R)4[135(r0R)2][112(r0R)2]1[1(r0R)2]3

   

α(r0R)6[135(r0R)2][112(r0R)2]1[1(r0R)2]3

   

+ρcρ0(σc26γg){[dlnP0dlnr0]ab[1ΔdlnP0dlnr0]}

  =

(r0R)2[112(r0R)2]1[1(r0R)2]3{5α3(13ab)[185(r0R)2+35(r0R)4]43[175(r0R)2+110(r0R)4]

   

+(43α)(r0R)2[135(r0R)2]α(r0R)4[135(r0R)2]}

   

+ρcρ0(σc26γg){[dlnP0dlnr0]ab[1ΔdlnP0dlnr0]}

  =

(r0R)2[112(r0R)2]1[1(r0R)2]3{[5α3(13ab)43]

   

+(r0R)2[8α3(13ab)+2815]+(r0R)4[α(13ab)215]

   

+(43α)(r0R)2[135(r0R)2]α(r0R)4[135(r0R)2]}

   

+ρcρ0(σc26γg){[dlnP0dlnr0]ab[1ΔdlnP0dlnr0]}

Second Attempt

1b[r02×LAWE] =

r02d2Δdr02r0[4]dΔdr0+[dlnP0dlnr0][r0dΔdr0+α(abΔ)]+[dlnP0dlnr0](σc26γg){1ab[1Δ]}ρcρ0,

where,

ρ0ρc =

(1x2),

Δ =

13(135x2)(1x2)1,

dlnP0dlnr0 =

5x2(135x2)(1x2)1(112x2)1=15x2(112x2)1Δ,

r0dΔdr0 =

415x2(1x2)2,

r02d2Δdr02 =

415x2(1x2)3(1+3x2).

Hence,

1b[r02×LAWE] =

r02d2Δdr02r0[4]dΔdr0

   

+[dlnP0dlnr0][r0dΔdr0+α(abΔ)]

   

+[dlnP0dlnr0](σc26γg){1ab[1Δ]}ρcρ0

  =

415x2(1x2)3(1+3x2)1615x2(1x2)2

   

+[dlnP0dlnr0][aαb415x2(1x2)2α3(135x2)(1x2)1]

   

+[dlnP0dlnr0](σc26γg){13ab(135x2)1(1x2)}(1x2)1.

1x2(1x2)1b[r02×LAWE] =

415(1x2)2(1+3x2)1615(1x2)1

   

5(135x2)(112x2)1[aαb415x2(1x2)2α3(135x2)(1x2)1]

   

5(135x2)(112x2)1(σc26γg){13ab(135x2)1(1x2)}(1x2)1

1x2(1x2)31b[r02×LAWE] =

415(1+3x2)1615(1x2)

   

5(135x2)(112x2)1[aαb(1x2)2415x2α3(135x2)(1x2)]

   

5(112x2)1(σc26γg){(135x2)3ab(1x2)}(1x2)

See Also

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