VORTEX SOLUTIONS IN THE EXTENDED SKYRME FADDEEV MODEL In collaboration with Luiz Agostinho Ferreira, Pawel Klimas (IFSC/USP) Masahiro Hayasaka (TUS) Juha Jäykkä (Nordita) Kouichi Toda (TPU) NOBUYUKI SAWADO Tokyo University of Science, Japan [email protected]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
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VORTEX SOLUTIONS IN THE EXTENDED SKYRME FADDEEV MODEL In collaboration with Luiz Agostinho Ferreira, Pawel Klimas (IFSC/USP) Masahiro Hayasaka (TUS) Juha.
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VORTEX SOLUTIONS IN THE EXTENDED SKYRME FADDEEV MODEL
In collaboration with Luiz Agostinho Ferreira, Pawel Klimas (IFSC/USP) Masahiro Hayasaka (TUS) Juha Jäykkä (Nordita) Kouichi Toda (TPU)
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 symmetry’’
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 𝜕𝜇𝑢𝜕𝜇𝑢=0
𝛽𝑒2=1 𝜕𝜇𝜕𝜇𝑢=0The equation becomes
or
or )(
𝑢=𝑣 (𝑧 )𝑤 (𝑦 )=𝑧𝑛𝑒𝑖𝑦𝑧=𝑥1+ 𝑖𝜖1𝑥2 , 𝑦=𝑥3−𝜖2𝑥
0
¿ (𝜌𝑎 )𝑛
𝑒𝑖 [𝜖1𝑛𝜑+𝑘 (𝑥3+𝜖2 𝑥0)]
Traveling wave vortex
The vortex solution in the integrable sectorL.A.Ferreira, JHEP05(2009)001,``Exact vortex solutions in an extended Skyrme-Faddeev model” O.Alvarez,LAF,et.al,PPB529(1998)689,``A new approach to integrable theories in any dimension”
One gets the infinite number of conserved quantity
Additional constraint
(0)
The equation
The solution has of the form:
We have no solutions for
𝑢 (𝒓 , 𝑡 )=√ 1−𝑔 (𝑦 )𝑔 (𝑦 )𝑒𝑖(𝑛𝜑+𝜆𝑧+𝑘𝜏 )
𝑥𝜇=𝑟 0(𝜏 ,𝜌 cos𝜑 ,𝜌 sin𝜑 , 𝑧)
Vortex solutions in
Ansatz
= 0
and for
for
Derrick’s scaling argument G.H.Derrick, J.Math.Phys.5,1252 (1964),``Comments on nonlinear wave equations as models for elementary particles’’
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=( 𝛽𝑒2−1 ) 4𝑛3
𝑎4 {1+( 𝜌𝑎 )2𝑛}
− 3
[ (𝑛−1 )( 𝜌𝑎 )2𝑛−4
−(𝑛+1)( 𝜌𝑎 )4𝑛−4 ]
+2𝑟02𝜇2
𝑀 2 {1+(𝜌𝑎 )2𝑁}
−3
[(2+ 2𝑁 )( 𝜌𝑎 )4𝑁− 4
−(2− 2𝑁 )( 𝜌𝑎 )
2𝑁 −4 ]
with the potential: we assume
𝑢 (𝜌 ,𝜑 ,𝑧 ,𝑡 )=(𝜌𝑎 )𝑛
𝑒𝑖 [𝜖𝑛𝜑+𝑘 (𝑧+𝜏)]
𝑉 𝛼𝛽=𝜇2
2(1+𝑛3❑)𝛼(1−𝑛3❑)𝛾𝛼 ≥0𝛾>0
Analytical solutions for n = 1, 2
𝑎=|𝑛|4√𝑀2(𝛽𝑒2−1)𝑟 0
2𝜇2 and
𝑛=1 ,𝑘2=0.0 ,𝑟 0
2𝜇2
𝑀 2 =1.0 𝑛=2 ,𝑘2=0.0 ,𝑟02𝜇2
𝑀 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
𝐸𝑠𝑡𝑎𝑡𝑖𝑐=2𝜋+4 𝜋31
𝑎2(𝛽𝑒2−1)
The infinite number of conserved current
𝐽𝜇≔𝛿𝐺𝛿𝑢∗𝒦𝜇−
𝛿𝐺𝛿𝑢
𝒦𝜇∗ h𝑤 𝑒𝑟𝑒𝐺≔𝐺 (|𝑢|2 )
¿𝛿𝐺𝛿𝑢
¿
Thus the current is always conserved:
And the equation of motion is written as
𝜕𝜇𝒦𝜇−2𝑢∗ (1+|𝑢|2 )𝒦𝜇𝜕
𝜇𝑢=− 𝜇2
4¿¿
The zero curvature condition 𝒦𝜇𝜕𝜇𝑢=𝒦∗
𝜇𝜕𝜇𝑢∗=0 ,𝒦∗
𝜇𝜕𝜇𝑢=𝒦𝜇𝜕
𝜇𝑢∗
𝐽𝜌=0The transverse spatial structure of the polar component and the longitudinal component are a pipelike structure.
The energy density plot of for old-, and new-baby potentials
Old baby skyrmion potential
New baby skyrmion potential
(old) 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
𝛽 𝑒2=1.01 𝛽 𝑒2=1.1 𝛽 𝑒2=2.0 𝛽 𝑒2=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 equations”
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 !Tanzan 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 particles’’