Fetching the paper…
Reading the bibliography…
The equation of motion of an extended object in spacetime reduces to an ordinary differential equation in the presence of symmetry.
L. Gohberg, P. Lancaster and L. Rodman, Matrices and indefinite scalar products
1983
Earlier work this paper cites.
I. Yokota, Classical simple Lie groups (Gendai-Sugakusha, 1990) (in Japanese)
1990
Earlier work this paper cites.
V. P. Frolov, V. Skarzhinsky, A. Zelnikov and O. Heinrich, Phys. Lett. B 224
1997
Earlier work this paper cites.
S. Holst and P. Peldan, Class. Quantum Grav., 14
1997
Cited alongside, same era.
L. Randall and R. Sundrum, Phys. Rev. Lett. 83
1999
Cited alongside, same era.
K. Ogawa, H.Ishihara, H. Kozaki, H. Nakano, and I. Tanaka, “Gravitational radiation from stationary rotating cosmic strings”, Proceeding of 15th JGRG workshop
2005
Cited alongside, same era.
Also the variable μ \mu changes by the gauge transformation: μ ↦ μ − ( 1 / α ) ( 2 θ ˙ Im ψ ¯ ψ ˙ + θ ˙ 2 ψ ¯ ψ ) \mu\mapsto\mu-(1/\alpha)(2\dot{\theta}{\rm Im}\overline{\psi}\dot{\psi}+\dot{\theta}^{2}\overline{\psi}\psi)
Cited in the paper.
If one also admits the spatial reflection, an isometry which is not connected to the identity, one sees that L + J x y + J z w L+J_{xy}+J_{zw} is the only Killing vector of constant norm. Alternatively, one can treat the case with L + J x y − J z w L+J_{xy}-J_{zw} in the same manner as in the present section by considering ( ψ 0 , ψ 1 , ( ψ 2 ) ∗ ) (\psi^{0},\psi^{1},(\psi^{2})^{*}) instead of ( ψ 0 , ψ 1 , ψ 2 ) (\psi^{0},\psi^{1},\psi^{2})
Cited in the paper.
A. L. Larsen and N. Sánchez, Phys. Rev. D51
Cited in the paper.
H. Ishihara and H. Kozaki, Phys. Rev. D72
2005
Later among the works it cites.
M. G. Jackson, N. T. Jones and J. Polchinski, J. High Energy Phys. 10
2005
Later among the works it cites.
2006
Later among the works it cites.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…