2019
DOI: 10.1140/epjp/i2019-12880-x
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Thermodynamic properties of an Aharonov-Bohm quantum ring

Abstract: In this paper, we investigate the thermodynamic properties of an Aharonov-Bohm (AB) quantum ring in a heat bath for both relativistic and non-relativistic cases. For accomplishing this, we used the partition function which was obtained numerically using the Euler-Maclaurin formula. In particular, we determined the energy spectra as well as the behavior of the main thermodynamic functions of the canonical ensemble, namely, the Helmholtz free energy, the mean energy, the entropy and the heat capacity. The so-cal… Show more

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Cited by 52 publications
(36 citation statements)
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“…Moreover, we note also that the quantum number n and the parameters ω, Φ and η have the function of increasing the energies of the spectrum, i.e., in the limits η → 0 (extremely dense cosmic string) and n = ω = Φ → ∞, we have |E σ n | → ∞. Now, comparing the spectrum (34) with the literature, we verified that in the absence of the topological and noninertial effects (η = 1 and ω = 0) we recover the usual spectrum of a Dirac particle confined in a relativistic AB ring [33,35].…”
Section: Ring In the Rotating Magnetic Cosmic String Backgroundsupporting
confidence: 64%
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“…Moreover, we note also that the quantum number n and the parameters ω, Φ and η have the function of increasing the energies of the spectrum, i.e., in the limits η → 0 (extremely dense cosmic string) and n = ω = Φ → ∞, we have |E σ n | → ∞. Now, comparing the spectrum (34) with the literature, we verified that in the absence of the topological and noninertial effects (η = 1 and ω = 0) we recover the usual spectrum of a Dirac particle confined in a relativistic AB ring [33,35].…”
Section: Ring In the Rotating Magnetic Cosmic String Backgroundsupporting
confidence: 64%
“…Since we are working now in a (1 + 1)-dimensional spacetime, it is convenient to write the Dirac matrices α = (0, α 2 , 0) = (0, −α 2 , 0) and γ 0 and the spin operator S = (0, 0, 1 2 Σ 3 ) in terms of the 2 × 2 Pauli matrices, i.e., α 2 = σ 2 and γ 0 = Σ 3 = σ 3 [35,60,75]. In this way, setting the following ansatz for the two-component Dirac spinor [35,60]…”
Section: Ring In the Rotating Magnetic Cosmic String Backgroundmentioning
confidence: 99%
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“…According to the literature, when the mean energy and the specific heat capacity are twice of the value encountered in the non-relativistic case, we say that these cases satisfy the so-called Dulong-Petit law [47]. It is important to mention that this peculiar behavior is also observed in others relativistic quantum systems, such as in the Dirac oscillator [20] and in the Aharonov-Bohm quantum ring [28]. Last but not least, it is worth mentioning that, since the partition function in both cases does not depend on the magnetic field (Eq.…”
Section: Now Let Us Focus On the Comparison On The Helmholtz Free Enmentioning
confidence: 95%
“…Moreover, this study also has a particular relevance from a theoretical viewpoint, mainly when the physical system is either relativistic [18][19][20][21][22] or non-relativistic quantum [23][24][25][26][27]. In addition, it is worth mentioning that recently the thermodynamic properties of an Aharonov-Bohm quantum ring were performed in the high and low-energy regime [28].…”
Section: Introductionmentioning
confidence: 99%