Abstract
We study the thermodynamic quantities in the system of the N independent harmonic oscillators with different frequencies in the Tsallis statistics of the entropic parameter q (\(1<q<2\)) with escort average. The norm equations are derived, and the physical quantities are calculated with the physical temperature. It is found that the number of oscillators is restricted below \(1/(q-1)\). The energy, the Rényi entropy \(S_q^{(R)}\), and the Tsallis entropy \(S_q^{(T)}\) are obtained by solving the norm equations approximately at high physical temperature and/or for small deviation \(q-1\). The energy is q-independent at high physical temperature when the physical temperature is adopted, and the energy is proportional to the number of oscillators and physical temperature at high physical temperature. The form of the Rényi entropy is similar to that of the von-Neumann entropy, and the Tsallis entropy is given through the Rényi entropy. The physical temperature dependence of the Tsallis entropy is different from that of the Rényi entropy. The Tsallis entropy is bounded from the above, while the Rényi entropy increases with the physical temperature. The ratio of the Tsallis entropy to the Rényi entropy is small at high physical temperature. The relation between the physical temperature \(T_{\mathrm {ph}}\) and the temperature T (the inverse of the Lagrange multiplier) is obtained, and the quantity as a function of T and q can be obtained through \(T_{\mathrm {ph}}\). We calculate the free energy \(F_q^{(R)}\) which is defined with \(T_{\mathrm {ph}}\) and \(S_q^{(R)}\) and the free energy \(F_q^{(T)}\) which is defined with T and \(S_q^{(T)}\). The relation between \(\partial F_q^{(R)}/\partial T_{\mathrm {ph}}\) and \(S_q^{(R)}\) and the relation between \(\partial F_q^{(T)}/\partial T\) and \(S_q^{(T)}\) are shown.
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This manuscript has no associated data or the data will not be deposited. [Authors’ comment: This study is theoretical, and no data is generated.]
Notes
The Bernoulli number \(B_n\) is often defined as \(B_n(x=0)\). It may worth to mention that \(B_n(x=0) = B_n(x=1)\) for \(n \ne 1\).
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Appendices
Appendix A: Approximate expression of Hurwitz zeta function
The Hurwitz zeta function [26,27,28] is defined by
We treat the case of \(s>1\) and \(\alpha > 0\) in this appendix.
Let \(B_n(x)\) be Bernoulli polynomials which are defined by
The Bernoulli number \(B_n\) in this paper is definedFootnote 1 by
We use the Euler–Maclaurin formula. Let a and b be integer with \(a < b\) and let f(x) be continuously differentiable for M-times. The Euler–Maclaurin formula is
where \(f^{(k)}\) is k-th derivative and [x] is the Gauss symbol (the floor function).
We attempt to find the expression of \(\zeta _{\mathrm {H}}(1+z, \alpha )\) for \(z>0\) using the Euler–Maclaurin formula. The right-hand side of Eq. (A.1) is an infinite series. Therefore, we first consider the following finite series:
We set f(x) as \(1/(\alpha + x)^{1+z}\) and apply the Euler–Maclaurin formula. By taking the limit \(m \rightarrow \infty \), we have the expression of \(\zeta _{\mathrm {H}}(1+z,\alpha )\). The integral part converges when \(\alpha \) is positive. We finally obtain
The function \(\zeta _{\mathrm {H}}(1+z, \alpha )\) can be rewritten [29]. For example, \(\zeta _{\mathrm {H}}(1+z, \alpha )\) is given by
because \(B_{2n+1}\) is zero for \(n \ge 1\) and \(\varGamma (z+1) = z \varGamma (z)\).
It is possible to estimate the integral of Eq. (A.6) by setting M. For example, the upper value of the integral with \(M=2\) is estimated:
where \(C_2\) is the maximum value of \(|B_2(x)|\) in the range of \(0 \le x \le 1\).
From Eq. (A.6), we find that the \(\zeta _{\mathrm {H}}(1+z, \alpha )\) for \(\alpha \gg 1\) behaves
Appendix B: Approximate expression of Barnes zeta function
The Barnes zeta function [30, 31] is defined by
where \(s>N\), \(\alpha > 0\), and \(\omega _j > 0\).
We define \(\varOmega _N\) as
The function \(\zeta _{\mathrm {B}}\) is represented as
We have \(\zeta _{\mathrm {H}}(1+z,\alpha ) \sim 1/(z \alpha ^z)\) for \(\alpha \gg 1\). Therefore, for sufficiently large \(\alpha \), we have
Using the recurrence relation, Eq. (B.13), we have the approximate expression of \(\zeta _{\mathrm {B}}\) for \(\alpha \gg 1\):
The condition \(z - (N-1) > 0\) is rewritten as \(1+z - N >0\). This condition is equivalent to the condition \(s>N\) with \(s=1+z\) for \(\zeta _{\mathrm {B}}(s, \alpha |\mathbf {\omega }_N)\).
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Ishihara, M. Thermodynamics of the independent harmonic oscillators with different frequencies in the Tsallis statistics in the high physical temperature approximation. Eur. Phys. J. B 95, 53 (2022). https://doi.org/10.1140/epjb/s10051-022-00309-w
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DOI: https://doi.org/10.1140/epjb/s10051-022-00309-w