Swing Amplification James Binney University of Oxford Saas Fee, - - PowerPoint PPT Presentation

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Swing Amplification James Binney University of Oxford Saas Fee, - - PowerPoint PPT Presentation

Swing Amplification James Binney University of Oxford Saas Fee, January 2019 Goldreich & Lynden Bell (1965) Julian & Toomre (1966) Shearing sheet Consider large m and study small near-Cartesian patch that rotates with


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SLIDE 1

Swing Amplification

James Binney

University of Oxford

Saas Fee, January 2019

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SLIDE 2

◮ Goldreich & Lynden Bell (1965) ◮ Julian & Toomre (1966)

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SLIDE 3

Shearing sheet

◮ Consider large m and study small near-Cartesian patch

that rotates with particle on circular orbit at its centre

L = 1

2[ ˙

x2 + (R + x)2( ˙ y/R + Ω)2] − Φ(R + x) px = ˙ x py = (R + x)2 ˙ y R + Ω 1 R ≃ RΩ + 2Ωx + ˙ y

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SLIDE 4

Shearing sheet

H = 1

2

  • p2

x +

p2

y

(1 + x/R)2

  • − ΩRpy + Φ

◮ Consts of motion: H and py or

∆y ≡ py − RΩ = 2Ωx + ˙ y

◮ Relations between frequencies

A = − 1

2

∂Ω ∂ ln R B = A − Ω κ2 = 4Ω(Ω − A) = −4ΩB

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SLIDE 5

Shearing sheet

∂Φ ∂x = RΩ2 ∂Φ ∂x

  • R+x

= RΩ2 + x

  • Ω2 + 2RΩ∂Ω

∂R

  • + O(x2)

= RΩ2 + xΩ (Ω − 4A)

  • A ≡ − 1

2R∂Ω

∂R

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SLIDE 6

Shearing sheet

∂Φ ∂x = RΩ2 ∂Φ ∂x

  • R+x

= RΩ2 + x

  • Ω2 + 2RΩ∂Ω

∂R

  • + O(x2)

= RΩ2 + xΩ (Ω − 4A)

  • A ≡ − 1

2R∂Ω

∂R

  • ◮ Hence Φ(R + x) ≃ Φ(R) + RΩ2x + 1

2Ω(Ω − 4A)x2

H = 1

2

  • p2

x + p2 y

  • 1 − 2 x

R + 3 x2 R2

  • − RΩpy + Φ(R)

+ RΩ2x + 1

2Ω(Ω − A)x2

≃ 1

2

  • p2

x + ∆2 y − R2Ω2

+ Φ(R) − xΩ∆y + 1

2κ2x2

where ∆y ≡ py − RΩ and κ2 ≡ 4Ω(Ω − A)

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SLIDE 7

Shearing sheet

∂Φ ∂x = RΩ2 ∂Φ ∂x

  • R+x

= RΩ2 + x

  • Ω2 + 2RΩ∂Ω

∂R

  • + O(x2)

= RΩ2 + xΩ (Ω − 4A)

  • A ≡ − 1

2R∂Ω

∂R

  • ◮ Hence Φ(R + x) ≃ Φ(R) + RΩ2x + 1

2Ω(Ω − 4A)x2

H = 1

2

  • p2

x + p2 y

  • 1 − 2 x

R + 3 x2 R2

  • − RΩpy + Φ(R)

+ RΩ2x + 1

2Ω(Ω − A)x2

≃ 1

2

  • p2

x + ∆2 y − R2Ω2

+ Φ(R) − xΩ∆y + 1

2κ2x2

where ∆y ≡ py − RΩ and κ2 ≡ 4Ω(Ω − A)

◮ x oscillates harmonically about x ≡ 2Ω∆y/κ2

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SLIDE 8

circular orbits

◮ Circular orbits are ones on which x = x, so

˙ y = ∆y − 2Ωx = κ2 2Ω − 2Ω

  • x = −2Ax

(circular orbit)

◮ Defines shear in the sheet

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SLIDE 9

Shearing sheet

◮ Let vφ ≡ 2Ax + ˙

y be the azimuthal speed relative to the local circular orbit, then since ∆y = 2Ωx + ˙ y and x = 2Ω∆y/κ2 vφ = 2(A − Ω)x + κ2x 2Ω = 2(A − Ω)(x − x) tells us how far a star is from its guiding centre

◮ When we eliminate x from H in favour of vφ we get

H ≃ 1

2

  • p2

x + ∆2 y − R2Ω2

+ Φ(R) + 1

2κ2

(x − x)2 − x2 = 1

2

  • p2

x + ∆2 y

  • 1 − 4Ω2

κ2

  • − R2Ω2
  • + Φ(R) + 1

8

κ2 (A − Ω)2 v2

φ

= 1

2

  • p2

x + ∆2 y

A A − Ω − R2Ω2

  • + Φ(R) + 1

2

Ω Ω − Av2

φ

= Hx(px, vφ) + Hy(∆y) (B ≡ A − Ω)

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SLIDE 10

Swing amplification

◮ We posit P = 2πGΣ/|k| is generated by a density pattern

that shears along circular orbits

◮ On account of shear, kx is a function of time:

kx(0)x + kyy(0) = kx(t)x + kyy(t) ⇒ kx(t) = kx(0) + 2kyAt

◮ Let t′ ≡ t − tc be time since tc ≡ − kx 2kyA when kx = 0

◮ kx(t′) = 2Akyt′

◮ So |k| = ky

√ 1 + 4A2t′2 goes through a minimum as kx passes through 0

◮ P = 2πGΣ1/|k| has a corresponding maximum

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Unperturbed (non-circular) orbits

x = x + X cos θr ⇒ pr = −κX sin θr vφ = 2B(x − x) = 2BX cos θr ˙ y = ∆y − 2Ωx = ∆y − 2Ω(x + X cos θr) x = 2Ω κ2 ∆y ⇒ y(t′) = y(0) + ∆y

  • 1 − 4Ω2

κ2

  • t′ − 2Ω

κ X sin θr = y(0) + ∆y A B t′ − 2Ω κ X sin θr Hence kxx + kyy = 2kyAt′(x + X cos θr) + ky

  • y(0) + ∆y

A B t′ − 2Ω κ X sin θr

  • = ky
  • y(0) + 2X
  • At′ cos θr − Ω

κ sin θr

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SLIDE 12

Linearizing the CBE

◮ With f = f0(H0) + f1 and H = H0 + Φ1

∂f ∂t + [f, H] = 0 ⇒ df1 dt = [Φ1, f0]

◮ On integration we have

f1 = t

t0

dt ∂Φ1 ∂x · ∂f0 ∂p where the integral is along unperturbed orbits.

◮ We take f0 = Fe−Hx/σ2 ⇒ Σ0 = 4πFσ2B/κ ◮ This DF

◮ generates biaxial Maxwellian v distribution ◮ is a function of px, and, through vφ, of both its conjugate

variable x, and the momentum ∆y

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SLIDE 13

Linearised CBE

◮ Using Hx = 1 2[p2 x + κ2(x − x)2] with Φ1(x, y) = Peik·x, we

have ∂Φ1 ∂x · ∂f0 ∂p = −iFPeik·x e−Hx/σ2 σ2 [kxpx − ky2Ω(x − x)]

f1(t) = 2πGFie−Hx/σ2 σ2 t

t0

dt′ Σ1 ei[ψ(t′)+kyy(0)] × −2At′κX sin θr − 2ΩX cos θr √ 1 + 4A2t′2 , where we have introduced a phase ψ(t′) ≡ 2kyX(At′ cos θr − (Ω/κ) sin θr).

◮ As we integrate over v to get Σ1, y(0) will vary.

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SLIDE 14

Dealing with y(0)

y(0) = y(t) − ∆y A B t + 2Ω κ X sin θr = y(t) − κ2x 2ΩB A B t + 2Ω κ X sin θr = y(t) + 2At(x − X cos θr) + 2Ω κ X sin θr Note ky[y(t) + 2Atx(t)] = k · x

  • t.

so kyy(0) = k · x − ψ(t)

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SLIDE 15

Introducing cpts of v

Using θr = θ0 + κt′ we write κX sin θr = κX

  • sin θ0 cos κt′ + cos θ0 sin κt′

= −Ux cos κt′ + Uy sin κt′ κX cos θr = Uy cos κt′ + Ux sin κt′ Ux ≡ −κX sin θ0 = px Uy ≡ κX cos θ0 = (κ/2B)vφ. Now ψ(t′) − ψ(t) = 2(ky/κ)[Ux{A(t′S − tS) + Ω κ (C′ − C)} + Uy{A(t′C′ − tC) − Ω κ (S′ − S)}] where C(t) ≡ cos κt, S(t) ≡ sin κt

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SLIDE 16

Integrating over V

Σ1(t) =

  • dpxdvφ f1 = −GΣ0

σ eik·x t

t0

dt′ KΣ1(t′) √ 1 + 4A2t′2 where K(t, t′) ≡ i σ3

  • d2U e−U2/2σ2ei[ψ(t′)−ψ(t)]

×

  • 2At′(−UxC + UyS) + 2(Ω/κ)(UyC + UxS)
  • ◮ Tickle the disc:

Σ1(t) = − κ 3.36Qeik·x t

t0

dt′ K(t, t′)[δ(t′ − t0) + Σ1(t′)] √ 1 + 4A2t′2 Q = κσ 3.36GΣ

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SLIDE 17

Evaluating K

  • duy e−a2u2

y+2ibyuy

  • dux e−a2u2

x+2ibxux(cxux + cyuy)

= √πe−b2

x/a2

a2

  • duy e−a2u2

y+2ibyuy(cyuya + icxbx/a)

= iπ a4 e−(b2

x+b2 y)/a2(cxbx + cyby).

a2 = 1 2σ2 bx = (ky/κ)[A(t′S′ − tS) + (Ω/κ)(C′ − C)] by = (ky/κ)[A(t′C′ − tC) − (Ω/κ)(S′ − S)) cx = −At′C′ + Ω κ S′ cy = At′S′ + Ω κ C′.

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SLIDE 18

solutions

◮ Vc = const, Q = 1 ◮ Vc = const, Q = 1.1

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SLIDE 19

Swing amplification

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Conclusion

◮ WKB theory is misleading in putting an exclusion zone

around CR

◮ CR is where the key action takes place ◮ illustrated by modes in N-body models ◮ Key process: amplification of waves as leading → trailing