Propagation of vortex beam around a Kerr black hole
Atsuki Masuda Osaka City University
collaborator: Hideki Ishihara(Osaka City University) Shunichiro Kinoshita (Osaka City University)
Propagation of vortex beam around a Kerr black hole Atsuki Masuda - - PowerPoint PPT Presentation
Propagation of vortex beam around a Kerr black hole Atsuki Masuda Osaka City University collaborator: Hideki Ishihara(Osaka City University) Shunichiro Kinoshita (Osaka City University) Spin angular momentum Orbital angular momentum
Atsuki Masuda Osaka City University
collaborator: Hideki Ishihara(Osaka City University) Shunichiro Kinoshita (Osaka City University)
circular polarization
helical wavefront
Property, Production, Observation
:integer :azimuthal angule
m=1
m
φ
z
ˆ Lzψ = −i ∂ ∂φψ
= mψ
eigenstate of orbital angular momentum
phase
2π
Transverse plane
m=1
amplitude
Max
Recently, some application of vortex beam to astrophysics have been considered
Application information science, the vortex beam has more information than the plane wave
・Allen et. al , Phvs. Rev. A, 45, 8185 (1992)
・ ・
Vortex beam carries Orbital Angular Momentum
the vortex beam carries the orbital angular momentum about the propagation axis.
m=-1 m=+3 m=+2 m=+1 m=0
The pattern of interference with plane wave
m=1 m=3
Production of vortex beam
vortex beam Plane wave
input Output
This plate is made of glass ,called spiral phase plate
w2 = w0
2 R = z
0/2z
2
Φ = (m + 1)arctan
,
Laguerre Gaussian beam
Solutions of vortex beam
ψ =
m Lm
exp(imφ)(w0/w)
Laguerre function
Bessel beam
ψ = Jm(qρ)exp[i(−ωt + kz)]exp(imφ)
q2 = ω2 − k2
dispersion relation
Bessel function
exp[−ρ2(1/w2 − ik/2R) − iΦ)]
Propagation of plane waves in a Gravitational field
wave vector
1 2 gµν(µS)(νS)Aei S
= 0
gµν µ νψ =0
ψ ≡ Aei S
˙ xα = ∂H ∂kα ˙ kα = − ∂H ∂xα
D ˙ xµ Dτ = 0
gµν ˙ xµ ˙ xν = 0
,
plane wave
vortex beam
Geodesic equation
Propagation of wave
Eikonal approximation Eikonal approximation
Orbit of Bessel beam in flat spacetime
uµ =
= (−ω, 0, m, k)
µS
satisfying geodesic equation
¯ uµ = 1
= (−ω, 0, 0, k)
:Bessel beam solution
(exact solution of wave equation in flat spacetime)
ψB = Jm(qρ)eiS
S = −ωt + kz + mφ
q,k,ω:constant Jm:Bessel function
z
y x¯ uµ
transverse plane
Decomposition of wave vectors
Scale of beam radius
L
curvature scale
d
beam radius
L d >>
Orbit of Bessel beam in a curved spacetime
metric perturbation
correction term
Orbit
Perturbed eikonal equation
Averaging
Ansatz
ψ = ψBei S
H := 1 2gµνkµkν − kµhµνvν + 1 2q2 = 0
Perturbed eikonal equation
the extra force between angular momentum
H := 1 2gµνkµkν − kµhµνvν + 1 2q2 = 0
˙ xα = ∂H ∂kα
˙ kα = − ∂H ∂xα
Riemann normal coordinate
hµν = −1 3Rµανβ(xα − xα
B)(xβ − xβ B)
Sνβ = 1 2(Xν
Bvβ − Xβ Bvν)
Xµ
B = xµ − xµ B
where
D ˙ xµ Dτ = − 1 2q RµναβuνSαβ
How does vortex beam propagate around Kerr B.H?
D ˙ xµ Dτ = − 1 2q RµναβuνSαβ
a:Kerr parameter M:mass of black hole
perturbative form
hti = 2Ma r3 (−y, x, 0)
ds2 = −(1 − 2Φ)dt2 + 2htidxidt + (1 + 2Φ)δijdxidxj
Expanding metric around Beam
Bij = 1 4 ∂hti ∂xj − ∂htj ∂xi
where
= 1 2µ( Bg · l)
− 1 2q RµναβuνSαβ = 1
2q ∂µ(∂lhtk − ∂khtl)utSkl
li = ut 2q ijkSjk
D ˙ xµ D = 1 2µ( Bg · l)
D ˙ xµ D = 1 2µ( Bg · l)
y x
Propagation of parallel to axis
attracting force! D ˙ xµ D = 1 2µ( Bg · l)
y x z
the force acts in the z direction
x z y z
not acting extra force
the vortex beam in the Kerr spacetime.
h D ˙ xµ D = 1 2µ( Bg · l)
li = ut 2q ijkSjk
m q
we determine spin parameter
emitted by a same source in the Kerr space-time
Observation of vortex photon
photons with even values of l into Port A1 photons with odd values of l into Port B1
eimφ
eimφ+imα