Sphalerons, Antisphalerons and Vortex Rings

G. ’t Hooft, Phys. Rev. Lett. 37

1976

Earlier work this paper cites.

F. R. Klinkhamer, and N. S. Manton, Phys. Rev. D30

1983

Earlier work this paper cites.

A. Ringwald, Nucl. Phys. B330

1990

Earlier work this paper cites.

J. Kunz, and Y. Brihaye, Phys. Lett. 216B

1990

Earlier work this paper cites.

B. Kleihaus, J. Kunz, and Y. Brihaye, Phys. Lett. B273

1992

Earlier work this paper cites.

F. Klinkhamer, Z. Phys. C29

1993

Cited alongside, same era.

B. Kleihaus, and J. Kunz, Phys. Lett. B329

1994

Cited alongside, same era.

Y. Brihaye, and J. Kunz, Phys. Rev. D50

1994

Cited alongside, same era.

M. Hindmarsh, and M. James, Phys. Rev. D49

1994

Cited alongside, same era.

M. Axenides, A. Johansen, H. B, Nielsen and O. Tornkvist, Nucl. Phys. B474

1996

Cited alongside, same era.

Note, that solutions with n = 1 n=1 , m > 1 m>1 and M H / M W ⪆ 1 M_{\rm H}/M_{\rm W}\gtrapprox 1 suffer from numerical inaccuracies. While uncertainties for the masses and the magnetic moments are only about 0.2 % 0.2\% , numbers for the distances between the nodes of these n = 1 n=1 , m > 1 m>1 solutions should only be regarded as indicative

Cited in the paper.

L. D. McLerran, Acta Phys. Pol. B25

2004

Later among the works it cites.

B. Kleihaus, J. Kunz, and K. Myklevoll, Phys. Lett. B582

2004

Later among the works it cites.

B. Kleihaus, J. Kunz, and Y. Shnir, Phys. Lett. B570

2006

Later among the works it cites.

N. S. Manton, Phys. Rev. D28

2019

Closest in time.