Majorana bound state in rotating superfluid 3He-A between parallel plates

A.J. Leggett, Rev. Mod. Phys. 47

1975

Earlier work this paper cites.

L.J. Buchholtz and A.L. Fetter, Phys. Rev. B 77

1977

Earlier work this paper cites.

J.A. Sauls and J.W. Serene, Phys. Rev. B 24

1981

Earlier work this paper cites.

D.C. Sagan, P.G.N. deVegvar, E. Polturak, L. Friedman, S.-S. Yan, E.L. Ziercher, and D.M. Lee, Phys. Rev. Lett. 53

Original

1984

Earlier work this paper cites.

D.S. Greywall, Phys. Rev. B 33

1986

Earlier work this paper cites.

P.J. Hakonen, K.K. Nummila, J.T. Simola, L. Skrbek, and G. Mamniashvili, Phys. Rev. Lett. 58

1987

Cited alongside, same era.

D. Vollhardt and P. Wölfle, The Superfluid Phase of Helium 3

1990

Cited alongside, same era.

G.E. Volovik, JETP Lett., 70

2001

Cited alongside, same era.

T. Kita, Phys. Rev. B 66

2002

Cited alongside, same era.

See for example C. Nayak, S.H. Simon, A. Stern, M. Freedman, and S. Das Sarma, Rev. Mod. Phys. (in press)

Cited in the paper.

The following GL parameters are used: α 0 = 3.81 × 10 50 ​ [ J − 1 ​ m − 3 ] \alpha_{0}=3.81\times 10^{50}[J^{-1}m^{-3}] , β 1 = − 3.75 × 10 99 [ J − 3 m − 3 ] \beta_{1}=-3.75\times 10^{99}[J^{-3}m^{-3}] , β 2 = 6.65 × 10 99 ​ [ J − 3 ​ m − 3 ] \beta_{2}=6.65\times 10^{99}[J^{-3}m^{-3}] , β 3 = 6.56 × 10 99 ​ [ J − 3 ​ m − 3 ] \beta_{3}=6.56\times 10^{99}[J^{-3}m^{-3}] , β 4 = 5.99 × 10 99 ​ [ J − 3 ​ m − 3 ] \beta_{4}=5.99\times 10^{99}[J^{-3}m^{-3}] , β 5 = − 8.53 × 10 99 [ J − 3 m − 3 ] \beta_{5}=-8.53\times 10^{99}[J^{-3}m^{-3}] , 2 ​ m 3 / ℏ = 9.51 × 10 7 ​ [ m − 2 ​ s ] . 2m_{3}/\hbar=9.51\times 10^{7}[m^{-2}s]

Cited in the paper.

T. Mizushima et al

Cited in the paper.

“Ettore Majorana”

2006

Later among the works it cites.

N.B. Kopnin and M.M. Salomaa, Phys. Rev. B 44

2007

Later among the works it cites.

Sr 2 RuO 4 , often refereed to as a chiral p p -wave superconductor, is re-examined critically in K. Machida and M. Ichioka, Phys. Rev. B 77

2008

Closest in time.

M. Yamashita, K. Izumina, A. Matsubara, Y. Sasaki, O. Ishikawa, T. Takagi, M. Kubota, and T. Mizusaki, Phys. Rev. Lett. 101

2008

Closest in time.