Lecture 5
Helicity change under reconnection; the GPE case:
- Reconnection and change of helicity - Application to solar cornal loops
- Writhe conservation under reconnection
- Cascade of quantum vortex links under Gross-Pitaevskii equation - Iso-phase surfaces as Seifert surfaces
- Evolution of iso-phase surfaces of minimal area
Selected references
Laing, CE, Ricca, RL & Sumners, DeW L 2015 Conservation of writhe helicity under anti-parallel reconnection. Nature Sci Rep 5, 9224.
Zuccher, S & Ricca, RL 2015 Helicity conservation under quantum reconnection of vortex rings. Phys Rev E 92, 061001.
Zuccher, S & Ricca, RL 2017 Relaxation of twist helicity in the cascade process of linked quantum vortices. Phys Rev E 95, 053109.
Example of high-energy fields relaxation
(Battye & Sutcliffe 1998)
Simulation of magnetic flux tubes reconnection Cross-switching at reconnection sites
Isosurfaces ( ) of force-free magnetic field with uniform twist.
Gold-Hoyle model ( ).
(Dahlburg & Norton 1995)
1
2 B max
η = 0.005
−1
(a) (b) (c)
(d) (e) (f)
Simulation of vortex tubes reconnection
DNS of vorticity iso-surfaces at 40% of maximum initial vorticity (Hussain & Duraisamy 2011)
Helicity-complexity change in a dissipative fluid
In presence of dissipation: , . Let .
H = H (t)
Theorem (Ricca 2008). Let be a zero-framed, essential physical
link, embedded in an incompressible, dissipative fluid. Then, we have
L
nC(t)
H (t) ≤ Φ
2C(t) d H (t)
dt ≤ sign(H ) sign(Ω) Φ
2dC(t)
I) ; II) .
dt
Proof.
Since and , we have
Ω = d ω
ij∑
i≠ jH (t) = Φ2 d
ω
ij∫
ij∑
i≠ jC(t) = ∑
i≠ j∫
ijd ω
ijH (t) = Φ
2d ω
ij∫
ij∑
i≠ jC(t) d
ω
ij∫
ij∑
i≠ j≤ Φ
2∑
i≠ j∫
ijd ω
ijC(t)
d ω
ij∫
ij∑
i≠ j= Φ
2
C(t)
Thus I) is proved.
Consider then the elementary change in helicity
d H (t) = d sign(t) H (t) = sign(H ) dH (t) = sign(H ) Φ
2d ω
ij∫
ij∑
i≠ jand in average crossing number
dC(t) = d ω
ij∑
i≠ jWe have:
d H (t) = sign(H) Φ
2d ω
ij∑
i≠ jd ω
ij∑
i≠ jdC(t) ≤ sign(H) Φ
2d ω
ij∑
i≠ jd ω
ij∑
i≠ jdC(t)
= sign(H ) sign(Ω) Φ
2dC(t)
In the limit, by taking the time derivative of the above, we have (II).
.
.
Applications to solar coronal loops
solar coronal braid; minimal number of strings (loops)
In presence of random photospheric motion, we have (Berger 1993):
B
c
min∝ N
3/2b( B ) = N
E
f∝ c
min2Φ
2N
2L E
f∝ Φ
2L N
and in our case, by using Ohyama (1993) inequality, we have:
M
min∝ Φ
2L (N −1)
.In presence of dissipation:
H (t) ≤ Φ
2C(t) d H (t)
dt ≤ Φ
2dC(t)
and
dt
.and ,
M
min≥ 16 π
1/ 3
b ( ) B − 1
( )
Wr ≈ +1:
(Scheeler et al. 2014) Writhe helicity under reconnection
anti-parallel
Wr ≈ −1
Anti-parallel reconnection near a crossing does not change writhe:
Writhe under anti-parallel reconnection
Wr ≈ −1
– 1
(Zabusky & Melander 1989)
– 1 – 1 – 1
Oriented polygons:
A = {a
1,...,a
n} B = {b
1,...,b
n}
Writhe of by oriented edges:
Wr(A) = 1
4 π
j =1w(a
i,a
j)
n i =1
∑
n
∑
Lk(A, B) = 1
4 π
j =1w(a
i,b
j)
m i =1
∑
n
∑
Linking number of disjoint oriented polygons , by oriented edges:
A
B
w(e
i,e
j) = w(e
j,e
i)
Signed area contribution on the unit sphere covered by direction vectors pointing from
oriented edge to oriented edge :
e
ie
je
ie
jPL- curves
A
,B
: contribution from oriented edges.
A B
A a
ib
jProof.
Writhe of disjoint union
:
Wr(A∪ B)= 1
4 π
j =1w(a
i,a
j)
n i =1
∑
n
∑ + w(a
i,b
j)
j =1 m i =1
∑
n
∑ + w(b
i,a
j)
j =1 m i =1
∑
n
∑ + w(b
i,b
j)
j =1 m i =1
∑
m
∑
A∪ B
Writhe is conserved by anti-parallel reconnection
Theorem (Laing et al. 2015). Writhe of and is conserved under anti-parallel reconnection of and , that is
A B
A B
Wr(A∪ B) = Wr(A# B)
.A∪ B (A# B) * A# B
= Wr(A) + 2Lk(A, B) +Wr(B)
Anti-parallel reconnection: from disjoint union through the theta-curve intermediate to the reconnected curve :
A∪ B
A# B
(A# B) *
Wr(A∪ B) = Wr(A) + 2Lk(A, B) +Wr(B) = Wr[(A# B)*]
(ii) oppositely oriented edges cancel out, hence
Wr[(A# B)*] = Wr(A# B)
thus
Wr(A∪ B) = Wr(A# B)
In the continuum limit from PL-curves , to smooth curves , , we have
;
; .
Wr( χ
α∪ χ
β) = Wr( χ
α) +Wr( χ
β) + 2Lk( χ
α, χ
β) = Wr( χ
α# χ
β)
A B χ
αχ
β. Helicity of flux tubes
α
andβ
( ):χ
βχ
αH ( α ∪ β ) = Wr( χ
α∪ χ
β) +Tw( α ∪ β ) = Wr( χ
α# χ
β) +Tw( α ∪ β )
Φ = 1
From rigid translation and internal cancellation of common edge:
(i) translation preserves , , ; hence
Wr(A) Wr(B) Lk(A, B)
Helicity and energy changes due to intrinsic twist change
“Empty” tube
γ
:Tw ( ) γ = T ( ) γ + N ( ) γ
=0 =0
∆H = H ( α ∪ β ) − H ( α # β ) = ∆Tw
hence, change in helicity due to change in torsion:
H ( α ∪ β ) = Wr ( χ
α# χ
β) + Tw ( α # β ) + ∆Tw
= H ( α # β ) + ∆Tw
or
.
;
In time: change in twist implies change in energy ( ):
δ H (t) = δ Tw(t) ≤ 4E δ E(t)
.Φ = 1
Since change in twist , we have:
Tw ( α ∪ β ) = Tw ( α # β ) + ∆Tw
∆H = ∆T ∆H = 0
because torsion is additive.Quantum vortex knots under the Gross-Pitaevskii equation GPE Vortex lines as phase defects of :
ψ
2→ 1 X → ∞
ψ
=ρ
eiθ ρ = ψ2
u = ∇ θ
Gross-Pitaevskii equation:
with as . Fluid dynamical interpretation of GPE:
GPE:
H = K + I = constant
Conserved hamiltonian:
K = 1
2 ∫ ∇ ψ ⋅ ∇ ψ
*d
3X I = 1
4 ∫ ( 1− ψ
2)
2d
3X
Cascade process of a Hopf link of quantum vortices ( )Γ = 1
Total writhe and twist contributions to helicity ( )
Wr
totH = Wr
tot+ Tw
totTw
totΓ = 1
Wr
tot= Wr
1+Wr
2+ 2Lk
12Twist analysis by ribbon construction on isophase surface
Individual writhe and twist contributions
(Zuccher & Ricca 2017)
Evolution of iso-phase (Seifert) surface of minimal area
(Zuccher & Ricca 2017 – in preparation)
Iso-phase (Seifert) surface of minimal area versus time
(Zuccher & Ricca 2017 – in preparation)
t
S
mint
Phase
θ
min versus timeθ
mint
u = ∇ θ
0 5 10 15 20 25 30 0.5
0.6 0.7 0.8 0.9 1
t Smin/Smin0
T23, R = 6, r = 2, L = 40
Evolution of iso-phase surface of minimal area of trefoil knot
t
S = Smin Smin 0
Evolution of iso-phase surface of minimal area of knot types
(Zuccher & Ricca 2017 – in preparation)
t
T
23T
25T
27T
29T
23T
25T
27T
29S = Smin Smin 0