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Zonal Toroidal Harmonic Expansion of External Gravitational Fields for Ring-like Objects aka
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Page 1: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Zonal Toroidal Harmonic Expansion

of External Gravitational Fields for Ring-like Objects

aka

Page 2: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Gravitational Field of BaumkuchenToshio FUKUSHIMA (NAOJ)

Submitted to AJ in Revised Form

ResearchGate Fukushima Click

Page 3: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc
Page 4: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Baumkuchen is Not

Only For Party

Page 5: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc
Page 6: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

External Grav. Field of Ring-like Object

! Integral Expression! Pro: General Purpose! Con: CPU Time

! Harmonic Expansion! Pro: Fast Computation ! Con: Lack of Proper Formulation! WARNING: Curse of Brillouin

( )''

'V

Φ =−∫x

x

x x

n

n

Φ = Φ∑

Page 7: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Curse of Brillouin Manifold

! Brillouin (1933)! Brillouin Scattering, B of WKB

! Brillouin Manifold= Minimum Circumscribing

Manifold! Convergence Limitof Harmonic Expansion

! Sphere/Spheroids/Toroid

Page 8: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Toroidal Coordinates ( ), ,u θ φ

2 1

cos

sin

cos

a ur

u

az

u

θθ

θ

−=

=−

cos

sin

x r

y r

φ

φ

=

=

Page 9: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Toroidal Coordinate Surfaces

! Morse & Feshbach (1953)

! Blue: Constant u! Red: Constant θ! Constant Ring

Radius meansDifferent Center of Toroids

Page 10: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

New Theory of Toroidal Harmonic Expansion

! Solution of Laplace’s Eq. (Hobson 1931)

! NEW Finding: Term 0 = Ring Potential at r=a! Key: Fast Computation of Radial Functions

cosV u θΦ = −

( )( )( )

( )( )

1/ 2

1/ 2

1/ 2

n

n n

n

n R R n R

P u F uup u

P u u F u

+

≡ =

( )0

cosn n

n

GMV C p u n

=

= ∑

Page 11: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Ring Potential! Classic Result: Ring Radius = a

! K(m): Complete Elliptic Integral of 1st Kind! Acceleration Vector & Fast Procedure

! Fukushima (2010, Cele. Mech. Dyn. Astron.)! Fukushima (2015a, J. Comp. Appl. Math.)

( )2K mGM

p π

Φ =

2 2r x y≡ +2

4arm

p≡

( )2 2p r a z≡ + +

Page 12: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

It’s Show Time

Page 13: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Case of Thick Disk! r0=0.1! r1=0.5! r2=2.0! H0=0.003! γ=9/8! Surface:10-8

Page 14: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Density: Thick Disk! Axisymmetric Volume Density Profile

! Power-Law & Scale Height Functions

( ) ( )( ) ( )

2

0

1 1, exp

22D

DD

zr z P r

H rH rρ ρ

π

= −

( ) 0

0

D

rH r H

r

γ

=

1 2r r r≤ ≤

( ) 0 01r r

P rr r

= −

Page 15: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Effective Cross Section of Thick Disk

Page 16: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Potential: Thick Disk

Page 17: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Spectrum: Thick Disk

Page 18: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Error Curve: Thick Disk

Page 19: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

CPU Time Comparison

Page 20: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Conclusion! New Theory of Expansion! Recursive Computation of Radial Func.! Seeds by Complete Elliptic Integrals! 3000-10000 Faster Evaluation! Convergence outside Brillouin Toroid! Divergence inside Brillouin Toroid! Accretion Disk => Piecewise Disk Model

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Piecewise Disk Model

Page 22: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

References! Bannikova et al., 2012, MNRAS, 424, 820! Fukushima, 2010, Cele. Mech. Dyn. Astron., 108, 339! Fukushima, 2011, Math. Comp., 80, 1725! Fukushima, 2015a, J. Comp. Appl. Math., 63, 17! Fukushima, 2015b, Astron. J., revised! Hobson, 1931, The Theory of Spherical and

Spheroidal Harmonics, Cambridge Univ. Press! Morse and Feshbach, 1953, Methods of Theoretical

Physics, McGraw-Hill

Page 23: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

Best isYet to Come

Page 24: g s - アルマ望遠鏡 · Core Galaxy NGC 4260 Hubble Space Telescope / Seconds of aas Oust 117 Arc

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