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Invariance of Witten's quantum mechanics under point canonical transformations
Mathematical Physics · Submitted 12 Jun 2019
abstract compiled · 2026-09-23 · no language-model review
The authors' main claim We show that the supersymmetric algebra of Witten's quantum mechanics is invariant under a given point canonical transformation.
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The abstract, sentence by sentence
We show that the supersymmetric algebra of Witten's quantum mechanics is invariant under a given point canonical transformation. It is shown that Witten's supersymmetric quantum mechanics can be isospectral or not to the seed Hamiltonian depending on the space coordinate you work on. We illustrate our results by generating a new class of exactly solvable supersymmetric partner Hamiltonians which are not isospectral to the seed Hamiltonian.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We show that the supersymmetric algebra of Witten's quantum mechanics is invariant under a given point canonical transformation. | result 0.83 | 0.94 | 0.74 | asserted 1.00 |
| s1 | It is shown that Witten's supersymmetric quantum mechanics can be isospectral or not to the seed Hamiltonian depending on the space coordinate you work on. | result 1.00 | 0.83 | 0.29 | asserted 0.88 |
| s2 | We illustrate our results by generating a new class of exactly solvable supersymmetric partner Hamiltonians which are not isospectral to the seed Hamiltonian. | contribution 0.81 | 0.94 | 0.19 | asserted 1.00 |
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Original abstract
We show that the supersymmetric algebra of Witten's quantum mechanics is invariant under a given point canonical transformation. It is shown that Witten's supersymmetric quantum mechanics can be isospectral or not to the seed Hamiltonian depending on the space coordinate you work on. We illustrate our results by generating a new class of exactly solvable supersymmetric partner Hamiltonians which are not isospectral to the seed Hamiltonian.
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