Gauge-invariant decomposition conjecture for metric perturbations

Let gabg_{ab} be the background metric, and let habh_{ab} be a symmetric rank-two tensor field whose gauge transformation between gauge choices X{\cal X} and Y{\cal Y}, generated by the vector field ξ\xi, is

;Y!hab;X!hab=£ξgab.{}_{\\;{\cal Y}}\\!h_{ab}-{}_{\\;{\cal X}}\\!h_{ab}=\pounds_{\xi}g_{ab}.

Gauge-invariant decomposition conjecture. There exist a tensor field Hab{\cal H}_{ab} and a vector field XaX^a such that

hab=Hab+£Xgab,h_{ab}={\cal H}_{ab}+\pounds_Xg_{ab},

and, under the gauge transformation, they satisfy

;Y!Hab;X!Hab=0,;YXa;XXa=ξa.{}_{\\;{\cal Y}}\\!{\cal H}_{ab}-{}_{\\;{\cal X}}\\!{\cal H}_{ab}=0,\qquad {}_{\\;{\cal Y}}X^a-{}_{\\;{\cal X}}X^a=\xi^a.

This decomposition separates the gauge-invariant part of a metric perturbation from its gauge-variant Lie-derivative part and is the starting point for constructing gauge-invariant variables at first and second order. The supplied source presents it as a conjectural starting point and gives no resolution evidence, so its status remains open.

Sources & referencesView supporting material

Primary source

Kouji Nakamura, “Second-order Gauge-invariant Cosmological Perturbation Theory: Current Status updated in 2019”, arXiv:1912.12805 (2020).

Additional references

8 papers in this index state this conjecture (2010–2019). The statement above is taken from the most recent of them; the others are arXiv:1403.1004, arXiv:1203.6448, arXiv:1112.0821, arXiv:1105.4007, arXiv:1103.3092, arXiv:1012.1409, arXiv:1011.5272.

Progress summary

Never refreshed

Nothing recorded yet. Refresh searches the literature and the public web for attempts on this problem, and writes the first summary here.

Solutions 0

No solutions have been posted yet.