vortex solutions in the extended skyrme faddeev model in collaboration with luiz agostinho ferreira,...
TRANSCRIPT
VORTEX SOLUTIONS IN THE EXTENDED SKYRME FADDEEV MODEL
In collaboration with ใใ Luiz Agostinho Ferreira, Pawel Klimas (IFSC/USP) Masahiro Hayasaka (TUS) ใใใ Juha Jรคykkรค (Nordita) Kouichi Toda (TPU)
NOBUYUKI SAWADOTokyo University of Science, Japan
ใใใ arXiv:0908.3672 , arXiv:1112.1085, arXiv:1209.6452, arXiv:1210.7523
At Miami 2012: A topical conference on elementary particles, astrophysics, and cosmology,
13-20 December, Fort Lauderdale, Florida
19 December, 2012
Objects of Yang-Mills theory
โ=๐ผ (๐๐โ๏ฟฝโ๏ฟฝ)2+๐ฝ (๐๐
โ๏ฟฝโ๏ฟฝร๐๐โ๏ฟฝโ๏ฟฝ)2+๐พ(๐๐
โ๏ฟฝโ๏ฟฝ)4
(i) Gauge + Higgs composite models
Abelian vortex (in U(1))
ใใใ Abrikosov vortex, graphene, cosmic string, Brane world,
etc.
โtHooft Polyakov monopole
ใใใใใใ GUT, Nucleon catalysis (Callan-Rubakov effect),
etc.
The Skyrme-Faddeev Hopfions, vortices Glueball?, Abrikosov vortex?, Branes?
(ii) Pure Yang-Mills theory
Instantons
In the Cho-Faddeev-Niemi-Shabanov decomposition
Monopole loop
Condensates in a dual superconductivity ใใใใ Confinement
N.Fukui,et.al.,PRD86(2012)065020,``Magnetic monopole loops generated from two-instanton solutions: Jackiw-Nohl-Rebbi versus 't Hooft instantonโ
Exotic structures of the vortexโฆโฆ
M.N.Chernodub and A..S. Nedelin, PRD81,125022(2010)``Pipelike current-carrying vortices in two-component condensatesโโ
P.J.Pereira,L.F.Chibotaru, V.V.Moshchalkov, PRB84,144504 (2011)``Vortex matter in mesoscopic two-gap superconductor squareโโ
Semi-local strings The Ginzburg-Landau equation
Summary
We got the integrable and also the numerical solutions of the vortices in the extended Skyrme Faddeev Model.
A special form of potential is introduced in order to stabilize and to obtian the integrable vortex solutions.
We begin with the basic formulation.
Cho-Faddeev-Niemi-Shabanov (CFNS) decomposition
electric magnetic remaining terms
22 1 1
3ร4 โ 6 = 6Degrees of freedom
6
L.D. Faddeev, A.J. Niemi, Phy.Rev.Lett.82 (1999) 1624,``Partially dual variables in SU(2) Yang-Mills theoryโ
t = ln k/ L ``renormalization group timeโโ
H. Gies, Phys. Rev. D63, 125023 (2001),``Wilsonian effective action for SU(2) Yang-Mills theory with Cho-Faddeev-Niemi-Shabanov decomposition
The Gies lagrangian
``Magnetic symmetryโโ
Lagrangian (in Minkowski space)
Sterographic project
Static hamiltonian
Positive definite for
The integrability: the analytical vortex solutions
The equation of the vortex
The zero curvature condition ๐๐๐ข๐๐๐ข=0
๐ฝ๐2=1 ๐๐๐๐๐ข=0The equation becomes
or
or )(
๐ข=๐ฃ (๐ง )๐ค (๐ฆ )=๐ง๐๐๐๐ฆ๐ง=๐ฅ1+ ๐๐1๐ฅ2 , ๐ฆ=๐ฅ3โ๐2๐ฅ
0
ยฟ (๐๐ )๐
๐๐ [๐1๐๐+๐ (๐ฅ3+๐2 ๐ฅ0)]
Traveling wave vortex
The vortex solution in the integrable sectorL.A.Ferreira, JHEP05(2009)001,``Exact vortex solutions in an extended Skyrme-Faddeev modelโ O.Alvarez,LAF,et.al,PPB529(1998)689,``A new approach to integrable theories in any dimensionโ
One gets the infinite number of conserved quantity
Additional constraint
(0)
The equation
The solution has of the form:
We have no solutions for
๐ข (๐ , ๐ก )=โ 1โ๐ (๐ฆ )๐ (๐ฆ )๐๐(๐๐+๐๐ง+๐๐ )
๐ฅ๐=๐ 0(๐ ,๐ cos๐ ,๐ sin๐ , ๐ง)
Vortex solutions in
Ansatz
= 0
and for
for
Derrickโs scaling argument G.H.Derrick, J.Math.Phys.5,1252 (1964),``Comments on nonlinear wave equations as models for elementary particlesโโ
Scaling:
Consider a model of scalar field:
We need to introduce form of a potential to stabilize the solution.
The baby-skyrmion potential
Plug into the equation it is written as
and
Assume the zero curvature condition
0=( ๐ฝ๐2โ1 ) 4๐3
๐4 {1+( ๐๐ )2๐}
โ 3
[ (๐โ1 )( ๐๐ )2๐โ4
โ(๐+1)( ๐๐ )4๐โ4 ]
+2๐02๐2
๐ 2 {1+(๐๐ )2๐}
โ3
[(2+ 2๐ )( ๐๐ )4๐โ 4
โ(2โ 2๐ )( ๐๐ )
2๐ โ4 ]
with the potential: we assume
๐ข (๐ ,๐ ,๐ง ,๐ก )=(๐๐ )๐
๐๐ [๐๐๐+๐ (๐ง+๐)]
๐ ๐ผ๐ฝ=๐2
2(1+๐3โ)๐ผ(1โ๐3โ)๐พ๐ผ โฅ0๐พ>0
Analytical solutions for n = 1, 2
๐=|๐|4โ๐2(๐ฝ๐2โ1)๐ 0
2๐2 and
๐=1 ,๐2=0.0 ,๐ 0
2๐2
๐ 2 =1.0 ๐=2 ,๐2=0.0 ,๐02๐2
๐ 2 =1.0
The energy per unit length of the traveling wave vortex with
The static energy per unit of length of the vortex with
The energy of the static/traveling wave vortex
๐ธ๐ ๐ก๐๐ก๐๐=2๐+4 ๐31
๐2(๐ฝ๐2โ1)
The infinite number of conserved current
๐ฝ๐โ๐ฟ๐บ๐ฟ๐ขโ๐ฆ๐โ
๐ฟ๐บ๐ฟ๐ข
๐ฆ๐โ h๐ค ๐๐๐๐บโ๐บ (|๐ข|2 )
ยฟ๐ฟ๐บ๐ฟ๐ข
ยฟ
Thus the current is always conserved:
And the equation of motion is written as
๐๐๐ฆ๐โ2๐ขโ (1+|๐ข|2 )๐ฆ๐๐
๐๐ข=โ ๐2
4ยฟยฟ
The zero curvature condition ๐ฆ๐๐๐๐ข=๐ฆโ
๐๐๐๐ขโ=0 ,๐ฆโ
๐๐๐๐ข=๐ฆ๐๐
๐๐ขโ
๐ฝ๐=0The transverse spatial structure of the polar component and the longitudinal component are a pipelike structure.
The charge per unit length:
๐=โซ๐๐ฅ1๐๐ฅ2 ๐ฝ 0=โ8๐ ๐ 2๐๐2๐0 [๐6 1๐2 ( ๐ฝ๐2โ1 )+ 1๐ฮ (1+
1๐)ฮ (1โ
1๐)]
For
we get Noether current with
๐ฝ๐=โ4 ๐๐2 ๐ข๐๐๐ข
โโ๐ขโ ๐๐๐ข
(1+|๐ข|2 )2โ ๐ 8๐2
(๐ฝ๐2โ1)2(๐๐๐ข๐
๐๐ขโ)(๐๐๐ขโ๐ขโ๐ขโ๐๐๐ข)
ยฟยฟยฟ
The components:
Broken axisymmetry of the solution
The energy density plot of for old-, and new-baby potentials
Old baby skyrmion potential
New baby skyrmion potential
ใใใใใใใใใใใใ (old) ใใใใใใใใใใใใ newNonsymmetric: old
For the potential , the holomorphic solutions appear as a ground state!
Symmetric:
The baby-skyrmion exhibits a non-axisymmetric solution depending on a choice of potential I.Hen et. al, Nonlinearity 21 (2008) 399
A sequence of the energy density plots of for the several for
the old-potential
๐ฝ ๐2=1.01 ๐ฝ ๐2=1.1 ๐ฝ ๐2=2.0 ๐ฝ ๐2=20.0
A repulsive force between the core of the vortices might appear
It might be similar with the force between the Abrikosov vortex.Erick J.Weinberg, PRD19,3008 (1979),``Multivortex solutions of the Ginzburg-Landau equationsโ
The vortex matter/lattice structure is observed.
SummaryWe got the integrable and the numerical solutions of the vortices in the extended Skyrme Faddeev Model.
A special form of potential is introduced in order to stabilize and toobtain the integrable vortex solutions.
OutlookWhat it the origin of the potential?How can I observe our solutions in Physics? For SC, we may introduce an external magnetic field
and see the structure change for the field. Geometrical patterns appear?
Our integrable solution thus carries an infinite number of conserved quantity.
The model (two gap model) hides a SU(2) structure even if it describes the U(1) like observation such as SC.
Thank you ๏ผTanzan Jinja shrine,Japan, 16 Nov.,2012
Lago Mar Resort, USA, 17 Dec.,2012
The Skyrme-Faddeev modelL.Faddeev, A.Niemi, Nature (London) 387, 58 (1997),``Knots and particlesโโ
R.A.Battye, P.M.Sutcliffe, Phys.Rev.Lett.81,4798(1998)
Lagrangian
Static hamiltonian
Positive definite for
Boundary conditions
Coordinates:
Hopfions(closed vortex)
Hopf charge
L.A.Ferreira, NS, et.al., JHEP11(2009)124, ``Static Hopfions in the extended Skyrme-Faddeev modelโ
Axially symmetric ansatz
Non-axisymmetric case:D.Foster, arXiv:1210.0926
(m, n) = (1, 1) (1, 2) (2, 1)
(m, n) = (1, 3)
(m, n) = (1, 4) (2, 2) (4, 1)
Hopf charge density
(3, 1)
corresponds to the zero curvature condition
Dimensionless energy, Integrability
The solution is close to the Integrable sector, but not exact.
๐ฝ๐2