Integrability classification conjecture for the minimally coupled scalar-field system

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Let

H=12(−p12+1q12p22)−kq12+Λq14+m2q22q14,H = \frac12 \left(-p_1^2 + \frac{1}{q_1^2}p_2^2 \right) - k q_1^2 + \Lambda q_1^4 + m^2q_2^2 q_1^4,

be the Hamiltonian of the minimally coupled scalar-field system. Assume Λ≠0\Lambda\ne0, let nn be an integer satisfying

9−4m2Λ=(2n+1)2,9-\frac{4m^2}{\Lambda}=(2n+1)^2,

and consider a generic energy level E≠0E\ne0. Integrability classification conjecture. If the system is integrable, then one of the following holds: n=1n=1 or n=−2n=-2, with m=0m=0 in both cases; k=0k=0 and 9−4m2/Λ=(2l)29-4m^2/\Lambda=(2l)^2 for an odd integer ll; or k=0k=0 and

n+12∈13Z∪14Z∪15Z∖Z.n+\frac12\in \frac13\mathbb Z\cup\frac14\mathbb Z\cup\frac15\mathbb Z\setminus\mathbb Z.

This statement appears in the conclusions as a classification of the remaining potentially integrable parameter values on generic nonzero energy levels, complementing the necessary conditions proved earlier. Its resolution is not supplied in the paper.

References

Primary source

Andrzej J. Maciejewski, Maria Przybylska, Tomasz Stachowiak and Marek Szydlowski, “Global integrability of cosmological scalar fields”, arXiv:0803.2318 (2008).

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