Long Josephson junction

In superconductivity, a long Josephson junction (LJJ) is a Josephson junction which has one or more dimensions longer than the Josephson penetration depth $\lambda _{J}$ . This definition is not strict.

In terms of underlying model a short Josephson junction is characterized by the Josephson phase $\phi (t)$ , which is only a function of time, but not of coordinates i.e. the Josephson junction is assumed to be point-like in space. In contrast, in a long Josephson junction the Josephson phase can be a function of one or two spatial coordinates, i.e., $\phi (x,t)$ or $\phi (x,y,t)$ .

Simple model: the sine-Gordon equation

The simplest and the most frequently used model which describes the dynamics of the Josephson phase $\phi$ in LJJ is the so-called perturbed sine-Gordon equation. For the case of 1D LJJ it looks like:

\lambda _{J}^{2}\phi _{xx}-\omega _{p}^{-2}\phi _{tt}-\sin(\phi )=\omega _{c}^{-1}\phi _{t}-j/j_{c},

where subscripts $x$ and $t$ denote partial derivatives with respect to $x$ and $t$ , $\lambda _{J}$ is the Josephson penetration depth, $\omega _{p}$ is the Josephson plasma frequency, $\omega _{c}$ is the so-called characteristic frequency and $j/j_{c}$ is the bias current density $j$ normalized to the critical current density $j_{c}$ . In the above equation, the r.h.s. is considered as perturbation.

Usually for theoretical studies one uses normalized sine-Gordon equation:

\phi _{xx}-\phi _{tt}-\sin(\phi )=\alpha \phi _{t}-\gamma ,

where spatial coordinate is normalized to the Josephson penetration depth $\lambda _{J}$ and time is normalized to the inverse plasma frequency $\omega _{p}^{-1}$ . The parameter $\alpha =1/{\sqrt {\beta _{c}}}$ is the dimensionless damping parameter ( $\beta _{c}$ is McCumber-Stewart parameter), and, finally, $\gamma =j/j_{c}$ is a normalized bias current.

Important solutions

Small amplitude plasma waves. $\phi (x,t)=A\exp[i(kx-\omega t)]$
Soliton (aka fluxon, Josephson vortex):[1]

\phi (x,t)=4\arctan \exp \left(\pm {\frac {x-ut}{\sqrt {1-u^{2}}}}\right)

Here $x$ , $t$ and $u=v/c_{0}$ are the normalized coordinate, normalized time and normalized velocity. The physical velocity $v$ is normalized to the so-called Swihart velocity $c_{0}=\lambda _{J}\omega _{p}$ , which represent a typical unit of velocity and equal to the unit of space $\lambda _{J}$ divided by unit of time $\omega _{p}^{-1}$ .[2]

References

M. Tinkham, Introduction to superconductivity, 2nd ed., Dover New York (1996).
J. C. Swihart (1961). "Field Solution for a Thin-Film Superconducting Strip Transmission Line". J. Appl. Phys. 32 (3): 461–469. Bibcode:1961JAP....32..461S. doi:10.1063/1.1736025.

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[1] M. Tinkham, Introduction to superconductivity, 2nd ed., Dover New York (1996).

[2] J. C. Swihart (1961). "Field Solution for a Thin-Film Superconducting Strip Transmission Line". J. Appl. Phys. 32 (3): 461–469. Bibcode:1961JAP....32..461S. doi:10.1063/1.1736025.