2003
DOI: 10.1016/s0375-9601(02)01731-0
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On a class of integrable time-dependent dynamical systems

Abstract: We present some integrable time-dependent systems of classical dynamics, and we apply the results to the equationẍ + f (t) x = 0, with f a positive non-decreasing differentiable function; some of the results are extended to the nonlinear case. Moreover we investigate the conditions for the solutions to be bounded and we study their asymptotic behaviour.

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Cited by 8 publications
(10 citation statements)
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“…This is one of the main results of this paper, since it strongly suggests that our statistical mechanical theory of a closed universe might complement the standard cosmological model of an oscillating universe based on purely general relativity grounds [1]. The implications of this theory on the concept of time can be extracted by first noticing that the dynamics (22) for the entropy of the universe corresponds the Hamiltonian [18] H S,Ṡ, t = 1 2…”
Section: Entropic Oscillatormentioning
confidence: 71%
See 1 more Smart Citation
“…This is one of the main results of this paper, since it strongly suggests that our statistical mechanical theory of a closed universe might complement the standard cosmological model of an oscillating universe based on purely general relativity grounds [1]. The implications of this theory on the concept of time can be extracted by first noticing that the dynamics (22) for the entropy of the universe corresponds the Hamiltonian [18] H S,Ṡ, t = 1 2…”
Section: Entropic Oscillatormentioning
confidence: 71%
“…(15) that the distribution vector f (t) corresponding to the closed universe possesses an oscillatory behavior and in Section 3, we have established the relation between f (t) and the entropy S through Eq. (18). Therefore, as a consequence of these S(t) will also have an oscillatory behavior which can be described by d dt…”
Section: Entropic Oscillatormentioning
confidence: 99%
“…We shall focus on the theory on an infinite spatial interval (a, b) = (−∞, ∞). 15 Picking the 'negative' branch 16 of the square root, then the spectral function z(w; τ, σ) in (2.13) has the finite limit z = w+σ+τ w+σ−τ → z ∞ = −1 at σ → ±∞. Hence, assuming J ± is bounded for large |σ|, the Lax connection L ± = 1 2 (1 + z ±1 )J ± vanishes at spatial infinity.…”
Section: Jhep11(2020)020mentioning
confidence: 99%
“…Then for any (polynomial) decaying boundary conditions on the fields at spatial infinity, the periodicity condition (4.4) on L τ will be broken at sufficiently higher order in this expansion. 15 It seems much harder to satisfy the periodicity condition (4.4) on a spatial circle due to the explicit non-periodic σ dependence in the Lax connections for the time-dependent models. 16 We note that it is consistent to 'pick a branch' here: e.g., by assuming that w has an imaginary part, it then follows that the sign of the square root does not change from σ = −∞ to σ = ∞.…”
Section: Jhep11(2020)020mentioning
confidence: 99%
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