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Higher power squeezed states, Jacobi matrices, and the Hamburger moment problem

Quantum Physics · Submitted 17 Nov 1997

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim The corresponding squeezed states are well-defined, however.

how it is stated · asserted 1.00 read the record →

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arXiv IDquant-ph/9711028 (version 2)
Pith IDPWPXCU77, Pith's permanent record of this paper and its review
CitationBengt Nagel (Royal Institute of Technology, Stockholm, Sweden). "Higher power squeezed states, Jacobi matrices, and the Hamburger moment problem." arXiv:quant-ph/9711028 (1997). https://pith.science/paper/PWPXCU77
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What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.83 · human participants 0.01 · controlled comparison 0.01 · randomized assignment 0.01 · states quantitative result 0.16 · compares with prior results 0.27 · mentions code or data availability 0.02.

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arXiv listing abstract v2. Results and the main claim are underlined; .

k:th power (amplitude-)squeezed states are defined as the normalized states giving equality in the Schroedinger-Robertson uncertainty relation for the real and imaginary parts of the k:th power of the one-mode annihilation operator. Equivalently they are the set of normalized eigenstates (for all possible complex eigenvalues) of the Bogolubov transformed "k:th power annihilation operators". Expressed in the number representation the eigenvalue equation leads to a three term recursion relation for the expansion coefficients, which can be explicitly solved in the cases k = 1, 2. The solutions are essentially Hermite and Pollaczek polynomials, respectively. k = 1 gives the ordinary squeezed states, i.e. displaced squeezed vacua. For k equal to or larger than three, where no explicit solution has been found, the recursion relation for the symmetric operator given by the real part of the k:th power of the annihilation operator defines a Jacobi matrix corresponding to a classical Hamburger moment problem, which is undetermined. This implies that the operator has an infinity of self-adjoint extensions, all with disjoint discrete spectra. The corresponding squeezed states are well-defined, however.

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#sentencerolethe authors' own workstates the main conclusionstrength
s0 k:th power (amplitude-)squeezed states are defined as the normalized states giving equality in the Schroedinger-Robertson uncertainty relation for the real and imaginary parts of the k:th power of the one-mode annihilation operator. background 0.59 0.37 0.06 asserted 1.00
s1 Equivalently they are the set of normalized eigenstates (for all possible complex eigenvalues) of the Bogolubov transformed "k:th power annihilation operators". result 0.50 0.45 0.07 asserted 1.00
s2 Expressed in the number representation the eigenvalue equation leads to a three term recursion relation for the expansion coefficients, which can be explicitly solved in the cases k = 1, 2. method 0.53 0.73 0.05 asserted 0.99
s3 The solutions are essentially Hermite and Pollaczek polynomials, respectively. k = 1 gives the ordinary squeezed states, i.e. displaced squeezed vacua. result 0.93 0.64 0.07 asserted 1.00
s4 For k equal to or larger than three, where no explicit solution has been found, the recursion relation for the symmetric operator given by the real part of the k:th power of the annihilation operator defines a Jacobi matrix corresponding to a classical Hamburger moment problem, which is undetermined. result 0.66 0.63 0.44 asserted 1.00
s5 This implies that the operator has an infinity of self-adjoint extensions, all with disjoint discrete spectra. interpretation 0.83 0.65 0.22 asserted 1.00
s6 The corresponding squeezed states are well-defined, however. result 0.61 0.60 0.20 asserted 1.00

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Original abstract

k:th power (amplitude-)squeezed states are defined as the normalized states giving equality in the Schroedinger-Robertson uncertainty relation for the real and imaginary parts of the k:th power of the one-mode annihilation operator. Equivalently they are the set of normalized eigenstates (for all possible complex eigenvalues) of the Bogolubov transformed "k:th power annihilation operators". Expressed in the number representation the eigenvalue equation leads to a three term recursion relation for the expansion coefficients, which can be explicitly solved in the cases k = 1, 2. The solutions are essentially Hermite and Pollaczek polynomials, respectively. k = 1 gives the ordinary squeezed states, i.e. displaced squeezed vacua. For k equal to or larger than three, where no explicit solution has been found, the recursion relation for the symmetric operator given by the real part of the k:th power of the annihilation operator defines a Jacobi matrix corresponding to a classical Hamburger moment problem, which is undetermined. This implies that the operator has an infinity of self-adjoint extensions, all with disjoint discrete spectra. The corresponding squeezed states are well-defined, however.

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1 arXiv paper cite this in 2 sentences

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  • Among the diverse generalizations discussed in the literature, multiple authors considered $k$-photon generalizations of the squeezing operator in <ref> in the form [equation] with $k≥3$, together with similar generalizations of well-known models of light–matter interaction such as the Rabi and Jaynes–Cummings model [ref] .

    Self-adjoint realizations of higher-order squeezing operators · Introduction · 0.86

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