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Gamow vectors formalism applied to the Loschmidt echo

Sebastian Fortin
CONICET - Universidad de Buenos Aires, Buenos Aires, Argentina
   Manuel Gadella
Departamento de FísicaTeórica, Atómica y Óptica and IMUVA,
Universidad deValladolid, 47011Valladolid, Spain
   Federico Holik
Instituto de Física La Plata, UNLP, CONICET,
Facultad de Ciencias Exactas, La Plata, Argentina
   Marcelo Losada
CONICET - FAMAF, Universidad Nacional de Córdoba, Córdoba, Argentina
Abstract

Gamow vectors have been developed in order to give a mathematical description for quantum decay phenomena. Mainly, they have been applied to radioactive phenomena, scattering and to some decoherence models. They play a crucial role in the description of quantum irreversible processes, and in the formulation of time asymmetry in quantum mechanics. In this paper, we use this formalism to describe a well-known phenomenon of irreversibility: the Loschmidt echo. The standard approach considers that the irreversibility of this phenomenon is the result of an additional term in the backward Hamiltonian. Here, we use the non-Hermitian formalism, where the time evolution is non-unitary. Additionally, we compare the characteristic decay times of this phenomenon with the decoherence ones. We conclude that the Loschmidt echo and the decoherence can be considered as two aspects of the same phenomenon, and that there is a mathematical relationship between their corresponding characteristic times.

1 Introduction

Gamow vectors have been introduced in the context of quantum unstable states, also called quantum resonances. Initially, they were used in nuclear physics to describe radioactive decay [1]. As is well known, experiments have shown that quantum resonances decay exponentially – at least for most observable times. Nevertheless, there are deviations of the exponential decay law [2] for very short (Zeno effect [3]) as well as for very long times (Khalfin effect [4]), which are difficult to be experimentally observed [5, 6]. Noise effects may also contribute to slight deviations of the exponential law for intermediate times [2]. In any case, this exponential law gives a good approximation, so that resonance states can be very well approximated by vector states (or wave functions) decaying exponentially with time. These are the Gamow vectors or Gamow functions. This means that we have either to generalize time evolution so as to allow for non-unitary time evolutions, or to extend the Hilbert space to a larger space containing the Gamow vectors.

The exponential decay of Gamow vectors is accomplished if they are defined as eigenvectors (with complex eigenvalues) of a total Hamiltonian H=H0+VH=H_{0}+V, where VV is a potential responsible for the decay [7]. Since Hamiltonians are self-adjoint, this is not possible in the context of Hilbert space quantum mechanics [8, 9, 10]. One consistent solution is to extend the Hilbert space to a rigged Hilbert space, also called Gelfand triplet [11] (see [12] for an alternative approach with non-Hermitian Hamiltonians). It is built by adding two more spaces to the Hilbert space \mathcal{H}, so that they form a triplet, ΦΦ×\Phi\subset\mathcal{H}\subset\Phi^{\times}, where Φ\Phi is a locally convex space, and Φ×\Phi^{\times} is its dual [13, 14, 15, 16, 17, 18, 19]. Then, Gamow vectors are well defined in the larger space Φ×\Phi^{\times}. On Φ×\Phi^{\times}, time evolution can be defined as a non-unitary extension of the unitary time evolution on the Hilbert space \mathcal{H} [20, 21].

There are several applications where the Gamow vectors (or Gamow states) play an essential role. The Brussels school used them to develop an irreversible version of quantum mechanics proposed by Prigogine [22, 23, 24, 25, 26, 27, 28]. One of its obvious derivations is a formalism for time asymmetry in quantum mechanics [29, 30, 31], along with the investigation on a microphysical arrow of time [32, 33, 34, 35]. Other applications of Gamow vectors lie on the fields of quantum decoherence for closed systems [36, 37, 38], or even in non-linear optics [39, 40, 41]. All these applications have in common the fact that, in the temporal evolution of certain magnitudes, a decreasing exponential appears that cannot be described by a unitary time evolution.

Recently, we have developed a formalism that relies on the Gamow vectors to describe the quantum-to-classical transition from the point of view of the Heisenberg picture [42, 43, 44, 45]. Its formal properties were studied from the point of view of dynamical logics [44, 45], using an algebraic perspective [44].

The exponential decay also appears in the study of a completely different phenomenon, namely, the Loschmidt echo. A. Peres proposed it in 1984 as a measure of sensitivity and reversibility of quantum evolutions. The idea is to consider an initial state |ψ0|\psi_{0}\rangle and evolve it during a time interval τ\tau under the action of a Hamiltonian H1H_{1}, reaching the state |ψτ|\psi_{\tau}\rangle. Then, apply a second Hamiltonian H2H_{2}, during a time interval of the same duration, in such a way that it reverses the action of the first Hamiltonian, aiming to recover the initial state. H1H_{1} is the Hamiltonian governing the forward evolution and H2H_{2} is the Hamiltonian governing the backwards evolution. Due to imperfections in the time-reversal or due to an intrinsic quantum irreversibility, the final state does not always coincide with the initial one. The Loschmidt echo measures this discrepancy, and it is defined as

M(τ)=|ψ0|eiH2τ/eiH1τ/|ψ0|2.M(\tau)=|\langle\psi_{0}|e^{-iH_{2}\tau/\hbar}e^{-iH_{1}\tau/\hbar}|\psi_{0}\rangle|^{2}. (1)

The above equation means that the system evolves in time under the action of the Hamiltonian H1H_{1}, and then, the evolution is governed by Hamiltonian H2H_{2}. If the time reversal operation is perfectly implemented and the time evolution is unitary, then H2=H1H_{2}=-H_{1} and M(t)=1M(t)=1. In case that some imperfections are involved, we can assume that H2=H1+ΣH_{2}=-H_{1}+\Sigma, where Σ\Sigma is a perturbation of the original Hamiltonian. The perturbation term is intended to bear information about possible imperfections in the implementation of the time reversal operation. With these definitions, equation (1) can be written as

M(τ)=|ψ0|ei(H1Σ)τ/eiH1τ/|ψ0|2.M(\tau)=|\langle\psi_{0}|e^{i(H_{1}-\Sigma)\tau/\hbar}e^{-iH_{1}\tau/\hbar}|\psi_{0}\rangle|^{2}. (2)

The time reversal operation has been widely studied from a theoretical point of view. However, the empirical study of the time reversal problem involves looking for physical operations for the implementation of the time inversion, which is not a trivial task. The development of new experimental techniques has allowed to perform precise experiments in this area. In some systems, it has been observed that the initial and the final states can differ to some degree [46]. To explain this discrepancy, two factors must be considered: the unitarity of the time evolution and the noise during the process.

When only unitary evolutions are considered, the discrepancy can be attributed to an imperfection in the implementation of the time reversal operation. In this case, the Hamiltonian which is used to model the temporal reversion is not exactly the inverse of the initial one. This can be attributed to the noise introduced by the environment, and it has been studied in previous works (see for example [47]).

In this paper, we propose an alternative description in order to explain the discrepancy between the initial and final states. We assume that the time inversion is perfect, but the time evolution is not unitary. To obtain a non-unitary evolution, we appeal to Gamow vectors, which are adequate for introducing exponential decays. Using this formalism, we show that the time evolution generated by Hamiltonians with complex eigenvalues is irreversible. Moreover, this approach allows us to account for the Loschmidt echo phenomenon.

2 Gamow vectors formalism

In this section, we introduce a model that will be useful to understand our description of the Loschmidt echo. This model is a variant of the Friedrichs one [48] with multiple resonances, and it is general enough to describe a wide range of realistic situations [49].

2.1 The Friedrichs model

As is well known, scattering resonances and quasi-stationary states are used to describe a scattering process in which a particle stays in the neighborhood of a center of forces –usually given by a potential– a time much longer than it would have remained if the center of forces were not present [8, 30]. Scattering resonances can be modeled using Hamiltonian pairs, {H0,H}\{H_{0},H\}, where H0H_{0} is the unperturbed Hamiltonain and H=H0+VH=H_{0}+V, where VV is the potential responsible for the creation of the quasi-stationary states. The simplest model for resonances is the Friedrichs model, in which H0H_{0} is given by

H0=ω0|11|+0ω|ωω|dω.H_{0}=\omega_{0}\,|1\rangle\langle 1|+\int_{0}^{\infty}\omega\,|\omega\rangle\langle\omega|\,d\omega\,. (3)

Here, H0H_{0} has a pure absolutely and non-degenerate continuous spectrum, which is +[0,)\mathbb{R}^{+}\equiv[0,\infty) and an eigenvalue, ω0>0\omega_{0}>0. Kets |ω|\omega\rangle are the eigenkets of H0H_{0} with eigenvalues ω+\omega\in\mathbb{R}^{+}, H0|ω=ω|ωH_{0}|\omega\rangle=\omega\,|\omega\rangle. As in the case of plane waves, |ω|\omega\rangle are not normalizable states, which acquire meaning in suitable extensions of the Hilbert space called rigged Hilbert spaces or Gelfand triplets, for which there exists an extensive literature as mentioned in the Introduction. The eigenvector |1|1\rangle, H|1=ω0|1H|1\rangle=\omega_{0}\,|1\rangle belongs to Hilbert space and is normalized so that 1|1=1\langle 1|1\rangle=1. Notice that the eigenvalue ω0\omega_{0} is imbedded in the continuous spectrum of H0H_{0}.

The potential intertwines discrete and continuous spectrum of H0H_{0} and it usually has the form

V=0f(ω)[|ω1|+|1ω|]𝑑ω,V=\int_{0}^{\infty}f(\omega)\,[|\omega\rangle\langle 1|+|1\rangle\langle\omega|]\,d\omega\,, (4)

where f(ω)f(\omega) is a real function, usually square integrable, called form factor. Since bound states and scattering states are orthogonal to each other, we have that ω|1=1|ω=0\langle\omega|1\rangle=\langle 1|\omega\rangle=0, for all ω+\omega\in\mathbb{R}^{+}. In addition, ω|ω=δ(ωω)\langle\omega|\omega^{\prime}\rangle=\delta(\omega-\omega^{\prime}) [49].

The total Hamiltonian has the form H=H0+λVH=H_{0}+\lambda\,V, where λ\lambda is a real coupling constant. The Hamiltonian HH has a pure simple absolutely continuous spectrum, so that

H=0ω|ω±ω±|𝑑ω,H=\int_{0}^{\infty}\omega\,|\omega^{\pm}\rangle\langle\omega^{\pm}|\,d\omega\,, (5)

where H|ω±=ω|ω±H|\omega^{\pm}\rangle=\omega\,|\omega^{\pm}\rangle are eigenkets for ω+\omega\in\mathbb{R}^{+}, the continuous spectrum of HH. The signs ±\pm correspond to in and out states of scattering theory. More details can be found in [49].

This is the simplest possible Friedrichs model. The most straightforward generalization, is obtained by adding more bound states for H0H_{0}, so that

H0=k=1Nωk|kk|+0ω|ωω|dω,ωk>0.H_{0}=\sum_{k=1}^{N}\omega_{k}\,|k\rangle\langle k|+\int_{0}^{\infty}\omega\,|\omega\rangle\langle\omega|\,d\omega\,,\qquad\omega_{k}>0\,. (6)

Other generalizations can be found in [49], although they do not play any role in the present discussion.

Thus, while H0H_{0} has bound states, at least one, HH possesses none. What has happened with the bound states of H0H_{0}? To see it, we need a mathematical definition for resonances. A precise definition based in the analytic properties of the resolvent (HzI)1(H-zI)^{-1} of HH, where zz is a complex number, z/+z\in\mathbb{C}/\mathbb{R}^{+} and II the identity operator, was given in [50], page 55. In the case of the simplest Friedrichs model, in which H0H_{0} has only one bound state, it is sufficient to consider the analytic properties of the reduced resolvent function given by

η(z):=1|(HzI)1|1.\eta(z):=\langle 1|(H-zI)^{-1}|1\rangle\,. (7)

Under mild conditions on the form factor f(ω)f(\omega) [51], the function η(z)\eta(z) admits an analytic continuation with a pair of poles at the points z0=ERiΓ/2z_{0}=E_{R}-i\Gamma/2 and z0=ER+iΓ/2z_{0}^{*}=E_{R}+i\Gamma/2, with Γ>0\Gamma>0. In addition, and following the formulation of resonances in rigged Hilbert spaces [20, 21], there are two non-normalizable vectors |fD|f^{D}\rangle and |fG|f^{G}\rangle, such that

H|fD=z0|fD,H|fG=z0|fG.H|f^{D}\rangle=z_{0}\,|f^{D}\rangle\,,\qquad H|f^{G}\rangle=z_{0}^{*}\,|f^{G}\rangle\,. (8)

For any t>0t>0 or t<0t<0, respectively, one has that

eitH|fD=eiERteΓt/2|fD,eitH|fG=eiERteΓt/2|fG,e^{-itH}\,|f^{D}\rangle=e^{-iE_{R}\,t}\,e^{-\Gamma t/2}\,|f^{D}\rangle\,,\qquad e^{-itH}\,|f^{G}\rangle=e^{-iE_{R}\,t}\,e^{\Gamma t/2}\,|f^{G}\rangle\,, (9)

which shows that |fD|f^{D}\rangle and |fG|f^{G}\rangle decay exponentially as t+t\longmapsto+\infty and tt\longmapsto-\infty, respectively. Thus, the superscripts DD and GG means decay and grow, respectively, for times going from -\infty to \infty.

Usually, |fD|f^{D}\rangle and |fG|f^{G}\rangle receive the names of decaying and growing Gamow vectors, respectively. Under mild assumptions, z0z_{0} is analytic in the coupling constant λ\lambda and has the property that limλ0z0=ω0\lim_{\lambda\to 0}z_{0}=\omega_{0} [51].

In correspondence with the two spectral decompositions for HH given in (5), we have these other two:

H=z0|fDfG|+γz|zz+|dz,H=z0|fGfD|+γ+z|z+z|dz.H=z_{0}\,|f^{D}\rangle\langle f^{G}|+\int_{\gamma^{-}}z\,|z^{-}\rangle\langle z^{+}|\,dz\,,\qquad H=z_{0}^{*}\,|f^{G}\rangle\langle f^{D}|+\int_{\gamma^{+}}z\,|z^{+}\rangle\langle z^{-}|\,dz\,. (10)
Refer to caption
Figure 1: γ\gamma^{-} is a curve in the lower half plane, starting at the origin, that together with the positive semi-axis of the real line encloses the pole z0z_{0}.

The meaning of the first spectral decomposition (10) is the following: let us assume that the functions φ(ω)=ω|φ\varphi(\omega)=\langle\omega|\varphi\rangle and ϕ(ω)=ω|ϕ\phi(\omega)=\langle\omega|\phi\rangle are analytically continuable to the upper and lower half of the complex plane, respectively. This, in particular, implies that φ(ω)=φ|ω\varphi^{*}(\omega)=\langle\varphi|\omega\rangle admits analytic continuation to the lower half plane. The value of these functions at the point z0z_{0} in the lower half plane is given by φ(z0)=φ|fD\varphi^{*}(z_{0})=\langle\varphi|f^{D}\rangle and ϕ(z0)=fG|ϕ\phi(z_{0})=\langle f^{G}|\phi\rangle. The values of φ(ω)\varphi^{*}(\omega) and ϕ(ω)\phi(\omega) at the complex number zz with negative imaginary part are φ(ω)=φ|z\varphi^{*}(\omega)=\langle\varphi|z^{-}\rangle and ϕ(z)=z+|ϕ\phi(z)=\langle z^{+}|\phi\rangle, respectively. Thus, what really has proper meaning is the value of φ|H|ϕ\langle\varphi|H|\phi\rangle. Finally, γ\gamma^{-} is a curve in the lower half plane, starting at the origin, that together with the positive semi-axis of the real line encloses the pole z0z_{0} (see Fig. 1). Analogously, γ+\gamma^{+} is a curve in the upper half plane, starting at the origin, that together with the positive semi-axis of the real line encloses the pole z0z^{*}_{0}. The meaning of the second spectral decomposition in (10) is similar, but in the upper half plane.

A Friedrichs model with free Hamiltonian as in (6) and potential given by

V:=k=1N0fk(ω)[|ωk|+|kω|]𝑑ω,V:=\sum_{k=1}^{N}\int_{0}^{\infty}f_{k}(\omega)\,[|\omega\rangle\langle k|+|k\rangle\langle\omega|]\,d\omega\,, (11)

where the fk(ω)f_{k}(\omega) are NN form factor functions (the total Hamiltonian is H=H0+λVH=H_{0}+\lambda V), is expected to give NN resonance poles (although for a given value of λ\lambda, two of these poles may coincide at the same point, giving a double resonance pole). Thus, for a given value of λ\lambda, we have resonance poles at the points z1,,zNz_{1},\dots,z_{N} and their complex conjugates, with respective decaying and growing Gamow vectors, |f1D,,|fND|f_{1}^{D}\rangle,\dots,|f_{N}^{D}\rangle and |f1G,,|fNG|f_{1}^{G}\rangle,\dots,|f_{N}^{G}\rangle. Then, the spectral decompositions (10) generalize to

H=k=1Nzk|fkDfkG|+γz|zz+|dz,H=k=1Nzk|fkGfkD|+γ+z|z+z|dz.\displaystyle H=\sum_{k=1}^{N}z_{k}\,|f_{k}^{D}\rangle\langle f_{k}^{G}|+\int_{\gamma^{-}}z\,|z^{-}\rangle\langle z^{+}|\,dz\,,\quad H=\sum_{k=1}^{N}z^{*}_{k}\,|f_{k}^{G}\rangle\langle f_{k}^{D}|+\int_{\gamma^{+}}z\,|z^{+}\rangle\langle z^{-}|\,dz\,. (12)

The integral terms in (10) and (12) are responsible for the deviations of the exponential decay for very short (Zeno effect [3]) or very large values of time [4]. These effects are observable, although not easy to be observed [5, 6]. This means that, for the vast majority of experiments, they are not detected. Due to this reason, it makes sense to drop the integral term form (10) and (12), at least within a reasonable range of observations. Also, note that the spectral decompositions for HH either in (10) or in (12) are time reversal of each other, so that they are completely equivalent [34]. Therefore, one may take as an effective Hamiltonian, valid for the majority of observations, the following:

H=k=1Nzk|fkDfkG|.H=\sum_{k=1}^{N}z_{k}\,|f_{k}^{D}\rangle\langle f_{k}^{G}|\,. (13)

As in the case N=1N=1, we have that H|fkD=zk|fkDH|f^{D}_{k}\rangle=z_{k}\,|f_{k}^{D}\rangle, for k=1,,Nk=1,\dots,N. Along (3), this suggests that

fsG|fkD=δs,k,s,k=1,,N.\langle f_{s}^{G}|f_{k}^{D}\rangle=\delta_{s,k}\,,\qquad s,k=1,\dots,N\,. (14)

Analogously, H|fkG=zk|fkGH|f^{G}_{k}\rangle=z^{*}_{k}\,|f_{k}^{G}\rangle for all kk, so that if we take as effective Hamiltonian the second sum in (12), we have that fsD|fkG=δs,k\langle f_{s}^{D}|f_{k}^{G}\rangle=\delta_{s,k}, for all values of ss and kk. Another property derived from this pseudometrics is that fkD|fsD=0=fkG|fsG\langle f_{k}^{D}|f_{s}^{D}\rangle=0=\langle f_{k}^{G}|f_{s}^{G}\rangle.

Resonances may be considered as independent of each other, so that the Gamow vectors |f1D,,|fND|f_{1}^{D}\rangle,\dots,|f_{N}^{D}\rangle and |f1G,,|fNG|f_{1}^{G}\rangle,\dots,|f_{N}^{G}\rangle may be assumed to be linearly independent. Then, we may assume that linear combinations of resonance states may belong either to the NN dimensional linear space, ND\mathcal{H}_{N}^{D}, spanned |f1D,,|fND|f_{1}^{D}\rangle,\dots,|f_{N}^{D}\rangle , or the space NG\mathcal{H}_{N}^{G} spanned by |f1G,,|fNG|f_{1}^{G}\rangle,\dots,|f_{N}^{G}\rangle or even to the 2N2N dimensional space, 2N\mathcal{H}_{2N}, spanned by |f1D,,|fND|f_{1}^{D}\rangle,\dots,|f_{N}^{D}\rangle and |f1G,,|fNG|f_{1}^{G}\rangle,\dots,|f_{N}^{G}\rangle. Due to (14), the spaces ND\mathcal{H}_{N}^{D} and NG\mathcal{H}_{N}^{G} may be considered as duals of each other.

These ideas, along with (9), are the basis for the following comment. Assume that |ψ|\psi\rangle and |φ|\varphi\rangle are arbitrary vectors in ND\mathcal{\ H}_{N}^{D}, so that

|ψ:=k=1Nak|fkD,|φ:=k=1Nbk|fkD.|\psi\rangle:=\sum_{k=1}^{N}a_{k}\,|f_{k}^{D}\rangle\,,\qquad|\varphi\rangle:=\sum_{k=1}^{N}b_{k}\,|f_{k}^{D}\rangle\,. (15)

Let us evolve |φ|\varphi\rangle in time, with the evolution governed by the total Hamiltonian HH. The value of this vector after a time tt has elapsed, is given by

|φ(t)=k=1Nbk|fkD(t),|\varphi(t)\rangle=\sum_{k=1}^{N}b_{k}\,|f_{k}^{D}(t)\rangle\,, (16)

where |fkD(t)=eitH|fkD|f_{k}^{D}(t)\rangle=e^{-itH}\,|f_{k}^{D}\rangle as in (9). Because of the duality between the spaces ND\mathcal{H}_{N}^{D} and NG\mathcal{H}_{N}^{G}, the bra corresponding to the ket |ψ|\psi\rangle is

ψ|=k=1NakfkG|,\langle\psi|=\sum_{k=1}^{N}a^{*}_{k}\,\langle f_{k}^{G}|\,, (17)

where the star denotes complex conjugation. The probability amplitude for the state |φ(t)|\varphi(t)\rangle to be in the state |ψ|\psi\rangle at time tt is given by

A(t)=ψ|φ(t)=k,s=1NasbkfsG|fkD(t)=k,s=1NasbkAs,k(t),A(t)=\langle\psi|\varphi(t)\rangle=\sum_{k,s=1}^{N}a_{s}^{*}\,b_{k}\,\langle f_{s}^{G}|f_{k}^{D}(t)\rangle=\sum_{k,s=1}^{N}a_{s}^{*}\,b_{k}\,A_{s,k}(t)\,, (18)

where,

As,k(t)=fsG|eitH|fkD=eizktfsG|fkD=eizktδs,k=eiEktetΓk/2δs,k,A_{s,k}(t)=\langle f_{s}^{G}|e^{-itH}|f_{k}^{D}\rangle=e^{-iz_{k}t}\,\langle f_{s}^{G}|f_{k}^{D}\rangle=e^{-iz_{k}t}\delta_{s,k}=e^{-iE_{k}t}\,e^{-t\,\Gamma_{k}/2}\delta_{s,k}\,, (19)

so that

A(t)=k=1NakbkeiEktetΓk/2,A(t)=\sum_{k=1}^{N}a_{k}^{*}\,b_{k}\,e^{-iE_{k}t}\,e^{-t\,\Gamma_{k}/2}\,, (20)

where EkE_{k} and Γk/2-\Gamma_{k}/2 are the real and imaginary parts of the resonance pole zkz_{k}, respectively.

Instead, we may have considered the vectors |ψ|\psi\rangle and |φ|\varphi\rangle to be in the space 2N\mathcal{H}_{2N}, and follow a similar reasoning. Formally, the results would have been different, since to (20), we had to add a similar term. If this were the case,

|ψ:=k=1Nak|fkD+k=1Nck|fkG,|φ:=k=1Nbk|fkD+k=1Ndk|fkG.|\psi\rangle:=\sum_{k=1}^{N}a_{k}\,|f_{k}^{D}\rangle+\sum_{k=1}^{N}c_{k}\,|f^{G}_{k}\rangle\,,\qquad|\varphi\rangle:=\sum_{k=1}^{N}b_{k}\,|f_{k}^{D}\rangle+\sum_{k=1}^{N}d_{k}\,|f^{G}_{k}\rangle\,. (21)

This construction, although useful for other purposes, may be incompatible with the formalism of Time Asymmetric Quantum Mechanics (TAQM) [29, 30, 31, 52], since in this formalism, time evolution for |fkD|f_{k}^{D}\rangle is defined only for t0t\geq 0, while time evolution for |fkG|f_{k}^{G}\rangle is only valid for t0t\leq 0. Nevertheless, a construction such that all growing and decaying Gamow vectors evolve rigorously for all values of time is possible [53], although this construction does not take into account the time asymmetry that is produced by decaying processes111It is also true that an algebraic formulation using operators on 2N\mathcal{H}_{2N} is still compatible with TAQM, [43]. Thus, we consider the discussion on ND\mathcal{H}_{N}^{D} as given above, as the most appropriate for our purposes.

2.2 Creation and annihilation operators

In this section we study the Friedrichs model in terms of the creation and annihilation operators. Its construction has been proposed, for instance, in [28]. The idea is the following: Let us assume that aa and aa^{\dagger} are the annihilation and creation of |1|1\rangle in (3), respectively, and that bωb_{\omega} and bωb^{\dagger}_{\omega} play the same role in relation to |ω|\omega\rangle. Then, the Friedrichs free Hamiltonian H0H_{0} written in terms of these operators is a contribution of two terms H0=HA+HRH_{0}=H_{A}+H_{R}, where [28],

HA:=ω0aa,HR:=0𝑑ωωbωbω,\displaystyle H_{A}:=\omega_{0}\,a^{\dagger}\,a\,,\qquad H_{R}:=\int_{0}^{\infty}d\omega\,\omega\,b_{\omega}^{\dagger}\,b_{\omega}\,, (22)

and the interaction is now written as

HI=λ0𝑑ωf(ω)(abω+abω),H_{I}=\lambda\int_{0}^{\infty}d\omega\,f(\omega)(a^{\dagger}\,b_{\omega}+a\,b^{\dagger}_{\omega})\,, (23)

where λ\lambda is the coupling constant and f(ω)f(\omega) the form factor. Again, the total Hamiltonian is H=H0+HI=HA+HR+HIH=H_{0}+H_{I}=H_{A}+H_{R}+H_{I}. The function

η(z):=ω0z0𝑑ωλ2f2(ω)ωz,\eta(z):=\omega_{0}-z-\int_{0}^{\infty}d\omega\;\frac{\lambda^{2}\,f^{2}(\omega)}{\omega-z}\,, (24)

is analytic with a branch cut on the positive semi-axis [0,)[0,\infty). We denote its limits on this semi-axis from above to below and from below to above as η+(ω):=η(ω+i0)\eta^{+}(\omega):=\eta(\omega+i0) and η(ω):=η(ωi0)\eta^{-}(\omega):=\eta(\omega-i0), respectively. Then, a “diagonalization” of the total Hamiltonian HH is given by [28]

H=z0(A)inAout+0𝑑ωωη+(ω)η(ω)(B~ω)in(B~ω)out.H=z_{0}\,(A^{\dagger})_{\mathrm{in}}\,A_{\mathrm{out}}+\int_{0}^{\infty}d\omega\,\omega\;\frac{\eta^{+}(\omega)}{\eta^{-}(\omega)}\;(\tilde{B}^{\dagger}_{\omega})_{\mathrm{in}}\,(\tilde{B}_{\omega})_{\mathrm{out}}\,. (25)

Here, (A)in(A^{\dagger})_{\mathrm{in}} and AoutA_{\mathrm{out}} are the creation and annihilation of the Gamow state from a vacuum |0|0\rangle, so that

|fD=(A)in|0,|0=Aout|fD,Aout|0=0,[Aout,Ain]=1,|f^{D}\rangle=(A^{\dagger})_{\mathrm{in}}\,|0\rangle\,,\quad|0\rangle=A_{\mathrm{out}}|f^{D}\rangle\,,\quad A_{\mathrm{out}}|0\rangle=0\,,\quad[A_{\mathrm{out}},A^{\dagger}_{\mathrm{in}}]=1\,, (26)

while (B~ω)in(\tilde{B}^{\dagger}_{\omega})_{\mathrm{in}} and (B~ω)out(\tilde{B}_{\omega})_{\mathrm{out}} are creation and annihilation operators of states in the continuum, which were defined in [28]. The latter do not have here any interest for us, as we are solely interested in the resonance behavior. The subscripts “in” and “out” come from scattering theory and do not play any role in our discussion here, so that we will omit them. Thus, the effective Hamiltonian, which concerns only to the presence of resonances is given by H=z0AAH=z_{0}\,A^{\dagger}\,A in our notation.

Now, rename |f1D:=|fD|f_{1}^{D}\rangle:=|f^{D}\rangle and define |fnD:=(A)n|f1D|f_{n}^{D}\rangle:=(A^{\dagger})^{n}\,|f_{1}^{D}\rangle. If we denote by N:=AAN:=A^{\dagger}\,A, it readily comes that

N|fnD=n|fnD,H|fnD=nz0|fnD,N|f_{n}^{D}\rangle=n\,|f_{n}^{D}\rangle\,,\qquad H|f_{n}^{D}\rangle=nz_{0}\,|f_{n}^{D}\rangle\,, (27)

which formally yields

eitH|fnD=eitnz0|fnD.e^{-itH}\,|f_{n}^{D}\rangle=e^{-itnz_{0}}\,|f_{n}^{D}\rangle\,. (28)

In the next section, we are going to apply the formalism of Gamow vectors to the Loschmidt echo.

3 Loschmidt echo and Gamow vectors

We consider a quantum system in an initial state |α(0)|\alpha(0)\rangle. Let us suppose that this initial state is evolved during a time interval τ\tau, and then it is evolved backwards during the same interval τ\tau. We denote the final state as |α(2τ)|\alpha(2\tau)\rangle. At this point, we can compare the initial state |α(0)|\alpha(0)\rangle with the final state |α(2τ)|\alpha(2\tau)\rangle. When the time-reversal procedure is perfectly implemented and the time-evolution is unitary, both states are exactly the same. However, when the time-reversal implementation is imperfect, there exist some degree of discrepancy between the states. One way to quantify this discrepancy is using the Loschmidt echo. If the time-evolution of the quantum system is given by the operator U1(τ)=eiH1τU_{1}(\tau)=e^{-\frac{i}{\hbar}H_{1}\tau}, we define the decay rate by

M(τ):=|α(0)|U2(τ)U1(τ)|α(0)|2.M(\tau):=|\langle\alpha(0)|U_{2}(\tau)\,U_{1}(\tau)|\alpha(0)\rangle|^{2}\,. (29)

where U2(τ)=eiH2τU_{2}(\tau)=e^{\frac{i}{\hbar}H_{2}\tau}, and H2H_{2} is a perturbation of H1H_{1}.

It is easy to see that M(τ)=1M(\tau)=1, when there is no discrepancy, and M(τ)=0M(\tau)=0, when the discrepancy is maximal. In particular, M(τ)M(\tau) is maximal when the time evolution is unitary and the time reversal is perfect. In the usual approach, it is assumed that the time evolution is unitary, but the time reversal is imperfect, i.e., the backward Hamiltonian is not exactly opposite to the forward Hamiltonian. In this work, we adopt an alternative approach. We consider a perfectly implemented time reversal, but a non-unitary time evolution.

In order to illustrate our approach, let us discuss how the time reversal is implemented in laboratory realizations. Consider the case of a crystal under the action of an external magnetic field oriented in the z^\hat{z} direction (as discussed in [54]). After applying U1U_{1} during a time interval τ\tau, the orientation of the external magnetic field is rotated and a new Hamiltonian H2H_{2} is obtained. The action of H2H_{2} during a time interval τ\tau is formally equivalent to the time reversion.

In the standard approach, the new Hamiltonian H2H_{2} is represented as a perturbation of the opposite initial Hamiltonian H1H_{1}. In our alternative description, we assume that evolutions are non-unitary. This is the mathematical expression of the assumption that the system has an intrinsic irreversibility which is not caused by the environment. The irreversibility is formally represented by the decaying exponential factor related to the time evolution of a Gamow vector.

Let us describe how the second Hamiltonian H2H_{2} is modeled under these assumptions. In the crystal example, the magnetic field is changed from z^\hat{z} to z^-\hat{z}. After this transformation, the signs of the real parts of the eigenvalues change, but the resonances remain the same, because they are related to internal degrees of freedom, and have nothing to do with the orientation of the system respect to the laboratory. Thus, the Hamiltonian H2H_{2} changes its complex eingenvalues as follows: z=ωi2Γz=ωi2Γz=\omega-\frac{i}{2}\Gamma\longrightarrow-z^{*}=-\omega-\frac{i}{2}\Gamma. Physically, this means that reversing the physical process do not change the decay factor of the dynamical law. Our description of what happens in the laboratory allows to explain why the initial state is not recovered. The decaying behavior of the Gamow vectors explains the Lodschmit echo. Therefore, the forward and backward evolution operators, U1(τ)U_{1}(\tau) and U2(τ)U_{2}(\tau) respectively, have the following form:

U1(τ)\displaystyle U_{1}(\tau) =n=0Neiτzn|fnDfnG|.\displaystyle=\sum_{n=0}^{N}e^{-\frac{i\tau}{\hbar}z_{n}}\,|f_{n}^{D}\rangle\langle f_{n}^{G}|\,. (30)
U2(τ)\displaystyle U_{2}(\tau) =n=0Neiτzn|fnDfnG|.\displaystyle=\sum_{n=0}^{N}e^{\frac{i\tau}{\hbar}z^{*}_{n}}\,|f_{n}^{D}\rangle\langle f_{n}^{G}|\,. (31)

Notice that, for all Gamow states {|fnD}\{|f_{n}^{D}\rangle\}, we have

U1(τ)|fnD=eiτzn|fnDandU2(τ)|fnD=eiτzn|fnD,U_{1}(\tau)|f_{n}^{D}\rangle=e^{-\frac{i\tau}{\hbar}z_{n}}\,|f_{n}^{D}\rangle\qquad\mathrm{\ and}\qquad U_{2}(\tau)|f_{n}^{D}\rangle=e^{\frac{i\tau}{\hbar}z^{*}_{n}}\,|f_{n}^{D}\rangle\,, (32)

U2(τ)U1(τ)U_{2}(\tau)U_{1}(\tau) is well defined, and it is different from the identity. Applying this time evolution in equation (29), we obtain

α(0)|U2(τ)U1(τ)|α(0)\displaystyle\langle\alpha(0)|U_{2}(\tau)U_{1}(\tau)|\alpha(0)\rangle =\displaystyle= α(0)|n=0Neiτzn|fnDfnG|m=0Neiτzm|fmDfmG|α(0)=\displaystyle\langle\alpha(0)|\sum_{n=0}^{N}e^{\frac{i\tau}{\hbar}z_{n}^{\ast}}\,|f_{n}^{D}\rangle\langle f_{n}^{G}|\sum_{m=0}^{N}e^{-\frac{i\tau}{\hbar}z_{m}}\,|f_{m}^{D}\rangle\langle f_{m}^{G}|\alpha(0)\rangle= (33)
=\displaystyle= n=0Neiτ(znzn)α(0)|fnDfnG|α(0)=\displaystyle\sum_{n=0}^{N}e^{\frac{i\tau}{\hbar}(z_{n}^{\ast}-z_{n})}\langle\alpha(0)|f_{n}^{D}\rangle\langle f_{n}^{G}|\alpha(0)\rangle=
=\displaystyle= n=0Neτγn/α(0)|fnDfnG|α(0).\displaystyle\sum_{n=0}^{N}e^{-\tau\gamma_{n}/\hbar}\langle\alpha(0)|f_{n}^{D}\rangle\langle f_{n}^{G}|\alpha(0)\rangle\,.

Let us suppose that the initial state is a superposition of the Gamow vectors |fnD|f_{n}^{D}\rangle

|α(0)=n=0Nan|fnD,|\alpha(0)\rangle=\sum_{n=0}^{N}a_{n}\;|f_{n}^{D}\rangle, (34)

then

α(0)|=n=0NanfnG|.\langle\alpha(0)|=\sum_{n=0}^{N}a^{*}_{n}\;\langle f_{n}^{G}|. (35)

Now, using the relations (14), we obtain

α(0)|U2(τ)U1(τ)|α(0)=n=0Neτγn/|an|2.\displaystyle\langle\alpha(0)|U_{2}(\tau)U_{1}(\tau)|\alpha(0)\rangle=\sum_{n=0}^{N}e^{-\tau\gamma_{n}/\hbar}|a_{n}|^{2}. (36)

This result shows that the Loschmidt echo decays with time, and its decay depends on the initial conditions ana_{n} and the characteristic times γn1\gamma_{n}^{-1}.

The decay of the Loschmidt echo has different regimes, such as parabolic, exponential, gaussian among others [55, 56, 57, 58, 59, 60, 61]. The most simple case of equation (36) is when there is only one characteristic time, or when the initial conditions are such that only one mode is activated. In these cases, it is obtained a pure exponential decay. In this way, Gamow vectors can be used to model experimental situations. In the general case, the combination of exponential functions with different characteristic times leads to more diverse time evolutions.

4 Decoherence and Loschmidt echo

So far we have seen how the Gamow vectors can be used to describe the Loschmidt echo. We saw that the type of decay of the quantity M(τ)M(\tau) is determined by the complex part of the Hamiltonian eigenstates and the initial conditions. In what follows we will show that there is a close relationship between the Loschmidt echo and the quantum decoherence phenomenon. This connection is because the decoherence time is also related with the imaginary part of the Hamiltonian eigenstates and the initial conditions.

To study the decoherence process in the Friedrich model, it is necessary to introduce the quasi coherent states, since they form the so-called privileged basis. Quasi-coherent states have been discussed in [62, 63, 64].

4.1 Initial conditions

For systems having an infinite number of resonances, it is possible in principle to define coherent resonance states. This states should have the following form for each complex number zz\in\mathbb{C}:

|zD=e|z|2/2k=0znn!|fkD.|z^{D}\rangle=e^{-|z|^{2}/2}\sum_{k=0}^{\infty}\frac{z^{n}}{\sqrt{n!}}\,|f_{k}^{D}\rangle\,. (37)

These coherent states should be eigenvectors with eigenvalue zz of a annihilation operator BB^{-}, satisfying B|fkD=k|fk1DB^{-}|f_{k}^{D}\rangle=k|f_{k-1}^{D}\rangle, for all kk\in\mathbb{N}, where |f0D=0|f_{0}^{D}\rangle=0, so that B|zD=z|zDB^{-}|z^{D}\rangle=z\,|z^{D}\rangle. This can be implemented for some exactly solvable models for resonances, like the high barrier Pöschl-Teller one dimensional model [65, 66].

Unfortunately, up to our knowledge, nobody has constructed a solvable Friedrichs model with an infinite number of resonance poles. Let us assume that we have N+1N+1 resonances with decaying Gamow vectors |f0D,,|fND|f_{0}^{D}\rangle,\dots,|f_{N}^{D}\rangle. By definition, a quasi coherent state at time t=0t=0 is a vector of the form:

|α1(0):=(k=0N|α1(0)|2kk!)1/2n=0N(α1(0))nn!|fnD,|\alpha_{1}(0)\rangle:=\left(\sum_{k=0}^{N}\frac{|\alpha_{1}(0)|^{2k}}{k!}\right)^{-1/2}\sum_{n=0}^{N}\frac{(\alpha_{1}(0))^{n}}{\sqrt{n!}}\;|f_{n}^{D}\rangle\,, (38)

where α1(0)\alpha_{1}(0) is a given complex number. Note that for NN going to infinity (38) acquires the form (37), hence the name of quasi-coherent state. Analogously, for any other complex number α2(0)\alpha_{2}(0), we have

|α2(0):=(k=0N|α2(0)|2kk!)1/2n=0N(α2(0))nn!|fnD.|\alpha_{2}(0)\rangle:=\left(\sum_{k=0}^{N}\frac{|\alpha_{2}(0)|^{2k}}{k!}\right)^{-1/2}\sum_{n=0}^{N}\frac{(\alpha_{2}(0))^{n}}{\sqrt{n!}}\;|f_{n}^{D}\rangle\,. (39)

Notice that, in a rough approximation, we may consider the pair of vectors {|α1(0),|α2(0)}\{|\alpha_{1}(0)\rangle,|\alpha_{2}(0)\rangle\} as the Moving Preferred Basis in the sense of [67]. The approximation is rough because we have taken t=0t=0, therefore it is not properly a moving basis. It is certainly efficient in the range of extremely short decoherence times tDt_{D} compared to relaxation time tRt_{R}, i.e., tD<<tRt_{D}<<t_{R}. In this sense, the choice tD=0t_{D}=0 is a workable approximation. Let us consider an arbitrary normalized linear combination of these two vectors; |Φ(0):=a|α1(0)+b|α2(0)|\Phi(0)\rangle:=a|\alpha_{1}(0)\rangle+b|\alpha_{2}(0)\rangle. Its corresponding density matrix is given by

ρ0=\displaystyle\rho_{0}= |Φ(0)Φ(0)|=\displaystyle|\Phi(0)\rangle\langle\Phi(0)|=
=\displaystyle= |a|2|α1(0)α1(0)|+ab|α1(0)α2(0)|+ab|α2(0)α1(0)|+|b|2|α2(0)α2(0)|.\displaystyle|a|^{2}\,|\alpha_{1}(0)\rangle\langle\alpha_{1}(0)|+ab^{*}\,|\alpha_{1}(0)\rangle\langle\alpha_{2}(0)|+a^{*}b\,|\alpha_{2}(0)\rangle\langle\alpha_{1}(0)|+|b|^{2}\,|\alpha_{2}(0)\rangle\langle\alpha_{2}(0)|\,. (40)

Note that, if i=1,2i=1,2,

αi(0)|=(k=0N|αi(0)|2kk!)1/2n=0N(αi(0))nn!fnG|.\langle\alpha_{i}(0)|=\left(\sum_{k=0}^{N}\frac{|\alpha_{i}(0)|^{2k}}{k!}\right)^{-1/2}\sum_{n=0}^{N}\frac{(\alpha^{*}_{i}(0))^{n}}{\sqrt{n!}}\;\langle f_{n}^{G}|\,. (41)

After a time t>0t>0, the state becomes

ρ(t)=\displaystyle\rho(t)= |Φ(t)Φ(t)|=\displaystyle|\Phi(t)\rangle\langle\Phi(t)|=
=\displaystyle= |a|2|α1(t)α1(t)|+ab|α1(t)α2(t)|+ab|α2(t)α1(t)|+|b|2|α2(t)α2(t)|.\displaystyle|a|^{2}\,|\alpha_{1}(t)\rangle\langle\alpha_{1}(t)|+ab^{*}\,|\alpha_{1}(t)\rangle\langle\alpha_{2}(t)|+a^{*}b\,|\alpha_{2}(t)\rangle\langle\alpha_{1}(t)|+|b|^{2}\,|\alpha_{2}(t)\rangle\langle\alpha_{2}(t)|\,. (42)

The expression in the second row in (4.1) contains four terms. The sum of the second and third terms is called the non-diagonal part that we intend to analyze next.

4.2 Decoherence

Let us denote the sum of the second and third term in (4.1) as ρND(t)\rho^{\mathrm{ND}}(t). Under the condition of macroscopicity, which is introduced below, the non-diagonal terms in (4.1) approximately satisfy the following relation:

ρND(t)=ρ12ND(t)|α1(0)α2(0)|+ρ21ND(t)|α2(0)α1(0)|.\rho^{\mathrm{ND}}(t)=\rho^{\mathrm{ND}}_{12}(t)\,|\alpha_{1}(0)\rangle\langle\alpha_{2}(0)|+\rho^{\mathrm{ND}}_{21}(t)\,|\alpha_{2}(0)\rangle\langle\alpha_{1}(0)|\,. (43)

This is not true in the general case as one may check by a direct calculation on |α1(t)α2(t)|=eitH|α1(0)α2(0)|eitH|\alpha_{1}(t)\rangle\langle\alpha_{2}(t)|=e^{-itH}\,|\alpha_{1}(0)\rangle\langle\alpha_{2}(0)|\,e^{itH}.

In order to show (43), we should make the hypothesis of the macroscopicity condition, which means that the peaks of both approximate Gaussians are far from each other. This means that |α1(0)α2(0)||\alpha_{1}^{*}(0)-\alpha_{2}(0)| is very large (we will consider α1(0)\alpha_{1}(0) as a real value). Notice that, under this hypothesis, the states of the preferred basis {|α1(0),|α2(0)}\{|\alpha_{1}(0)\rangle,|\alpha_{2}(0)\rangle\} are approximately orthogonal or quasi-orthogonal, which means that

α1(0)|α2(0)=α2(0)|α1(0)0.\langle\alpha_{1}(0)|\alpha_{2}(0)\rangle=\langle\alpha_{2}(0)|\alpha_{1}(0)\rangle^{*}\approx 0\,. (44)

To show (44), we first note that after (39) and (41) we have that

α1(0)|α2(0)=(k=0N|α1(0)|2kk!)1/2(k=0N|α2(0)|2kk!)1/2n=0N(α1(0)α2(0))nn!.\langle\alpha_{1}(0)|\alpha_{2}(0)\rangle=\left(\sum_{k=0}^{N}\frac{|\alpha_{1}(0)|^{2k}}{k!}\right)^{-1/2}\left(\sum_{k=0}^{N}\frac{|\alpha_{2}(0)|^{2k}}{k!}\right)^{-1/2}\sum_{n=0}^{N}\frac{(\alpha_{1}^{*}(0)\,\alpha_{2}(0))^{n}}{n!}\,. (45)

Then, let us use the Cauchy product222The Cauchy product states that (n=0Nan)(n=0Nbn)=n=0Ncn,withcn=k=0nakbnk.\left(\sum_{n=0}^{N}a_{n}\right)\left(\sum_{n=0}^{N}b_{n}\right)=\sum_{n=0}^{N}c_{n}\,,\qquad\mathrm{with}\qquad c_{n}=\sum_{k=0}^{n}a_{k}\,b_{n-k}\,. and the binomial formula on the two first factors on the right hand side of (45), so as to obtain:

α1(0)|α2(0)=(k=0N(|α1(0)|2+|α2(0)|2)kk!)1/2n=0N(α1(0)α2(0))nn!.\langle\alpha_{1}(0)|\alpha_{2}(0)\rangle=\left(\sum_{k=0}^{N}\frac{(|\alpha_{1}(0)|^{2}+|\alpha_{2}(0)|^{2})^{k}}{k!}\right)^{-1/2}\sum_{n=0}^{N}\frac{(\alpha_{1}^{*}(0)\,\alpha_{2}(0))^{n}}{n!}\,. (46)

Repeating the procedure, we obtain

α1(0)|α2(0)=n=0N1n!(12(|α1(0)|2+|α2(0)|22α1(0)α2(0)))n\displaystyle\langle\alpha_{1}(0)|\alpha_{2}(0)\rangle=\sum_{n=0}^{N}\frac{1}{n!}\left(-\frac{1}{2}(|\alpha_{1}(0)|^{2}+|\alpha_{2}(0)|^{2}-2\alpha_{1}^{*}(0)\alpha_{2}(0))\right)^{n}
=n=0N1n!((α1(0)α2(0))22)n.\displaystyle=\sum_{n=0}^{N}\frac{1}{n!}\left(-\frac{(\alpha_{1}^{*}(0)-\alpha_{2}(0))^{2}}{2}\right)^{n}\,. (47)

Clearly after (4.2), for |α1(0)α2(0)||\alpha_{1}^{*}(0)-\alpha_{2}(0)| very large, we obtain (44). For this case, let us define

ρ12ND(t):=α1(0)|ρ(t)|α2(0),ρ21ND(t):=α2(0)|ρ(t)|α1(0),\rho_{12}^{\mathrm{ND}}(t):=\langle\alpha_{1}(0)|\rho(t)|\alpha_{2}(0)\rangle\,,\quad\rho_{21}^{\mathrm{ND}}(t):=\langle\alpha_{2}(0)|\rho(t)|\alpha_{1}(0)\rangle\,, (48)

where ρ(t)\rho(t) has been introduced in (4.1), from which we have that

ρ12ND(t)=abα1(0)|α1(t)α2(t)|α2(0)+abα1(0)|α2(t)α1(t)|α2(0),\displaystyle\rho_{12}^{\mathrm{ND}}(t)=ab^{*}\,\langle\alpha_{1}(0)|\alpha_{1}(t)\rangle\langle\alpha_{2}(t)|\alpha_{2}(0)\rangle+a^{*}b\,\langle\alpha_{1}(0)|\alpha_{2}(t)\rangle\langle\alpha_{1}(t)|\alpha_{2}(0)\rangle\,,
ρ21ND(t)=abα2(0)|α1(t)α2(t)|α1(0)+abα2(0)|α2(t)α1(t)|α1(0).\displaystyle\rho_{21}^{\mathrm{ND}}(t)=ab^{*}\,\langle\alpha_{2}(0)|\alpha_{1}(t)\rangle\langle\alpha_{2}(t)|\alpha_{1}(0)\rangle+a^{*}b\,\langle\alpha_{2}(0)|\alpha_{2}(t)\rangle\langle\alpha_{1}(t)|\alpha_{1}(0)\rangle\,. (49)

In order to compute (4.2), let us follow the notation used in (15), (16) and (17). In what follows, we will assume that the numbers α1(0)\alpha_{1}(0) and α2(0)\alpha_{2}(0) are real. If we choose |ψ:=|α1(0)|\psi\rangle:=|\alpha_{1}(0)\rangle and |φ(t):=|α1(t)|\varphi(t)\rangle:=|\alpha_{1}(t)\rangle, and take into account (38) and (41), we have that the coefficients aka_{k} and bkb_{k} in (15) and (16) have the following form:

ak=(α1(0))kk!e12|α1(0)|2,bk=(α1(0))kk!e12|α1(0)|2,a_{k}=\frac{\left(\alpha_{1}(0)\right)^{k}}{\sqrt{k!}}\,e^{-\frac{1}{2}\,|\alpha_{1}(0)|^{2}}\,,\qquad b_{k}=\frac{\left(\alpha_{1}(0)\right)^{k}}{\sqrt{k!}}\,e^{-\frac{1}{2}\,|\alpha_{1}(0)|^{2}}\,, (50)

so that,

α1(0)|α1(t)=e|α1(0)|2n=0N(|α1(0)|2)nn!eiznt.\left\langle\alpha_{1}(0)|\alpha_{1}(t)\right\rangle=e^{-\left|\alpha_{1}(0)\right|^{2}}\sum_{n=0}^{N}\frac{\left(\left|\alpha_{1}(0)\right|^{2}\right)^{n}}{n!}e^{-iz_{n}t}\,. (51)

Then, we take |ψ:=|α1(0)|\psi\rangle:=|\alpha_{1}(0)\rangle and |φ(t):=|α2(t)|\varphi(t)\rangle:=|\alpha_{2}(t)\rangle, which gives after (39) and (41) that

an=|α1(0)|nn!e12|α1(0)|2,bn=|α2(0)|nn!e12|α2(0)|2,a_{n}=\frac{\left|\alpha_{1}(0)\right|^{n}}{\sqrt{n!}}\,e^{-\frac{1}{2}\,|\alpha_{1}(0)|^{2}}\,,\qquad b_{n}=\frac{\left|\alpha_{2}(0)\right|^{n}}{\sqrt{n!}}\,e^{-\frac{1}{2}\,|\alpha_{2}(0)|^{2}}\,, (52)

so that

α1(0)|α2(t)=e12{|α1(0)|2+|α2(0)|2}n=0N(|α1(0)||α2(0)|)nn!eiznt.\left\langle\alpha_{1}(0)|\alpha_{2}(t)\right\rangle=e^{-\frac{1}{2}\,\{|\alpha_{1}(0)|^{2}+\left|\alpha_{2}(0)\right|^{2}\}}\sum_{n=0}^{N}\frac{\left(\left|\alpha_{1}(0)\right|\left|\alpha_{2}(0)\right|\right)^{n}}{n!}e^{-iz_{n}t}\,. (53)

In the third place, we choose |ψ=|α2(0)|\psi\rangle=|\alpha_{2}(0)\rangle and |φ(t)=|α1(t)|\varphi(t)\rangle=|\alpha_{1}(t)\rangle, which give

an=(α2(0))nn!e12|α2(0)|2,bn=(α1(0))nn!e12|α1(0)|2,a_{n}=\frac{\left(\alpha_{2}(0)\right)^{n}}{\sqrt{n!}}\,e^{-\frac{1}{2}\,|\alpha_{2}(0)|^{2}}\,,\qquad b_{n}=\frac{\left(\alpha_{1}(0)\right)^{n}}{\sqrt{n!}}\,e^{-\frac{1}{2}\,|\alpha_{1}(0)|^{2}}\,, (54)

so that

α2(0)|α1(t)=e12{|α1(0)|2+|α2(0)|2}n=0N(|α1(0)||α2(0)|)nn!eiznt\left\langle\alpha_{2}(0)|\alpha_{1}(t)\right\rangle=e^{-\frac{1}{2}\,\{|\alpha_{1}(0)|^{2}+\left|\alpha_{2}(0)\right|^{2}\}}\sum_{n=0}^{N}\frac{\left(\left|\alpha_{1}(0)\right|\left|\alpha_{2}(0)\right|\right)^{n}}{n!}e^{-iz_{n}t} (55)

Finally, the choice |ψ:=|α2(0)|\psi\rangle:=|\alpha_{2}(0)\rangle and |φ(t):=|α2(t)|\varphi(t)\rangle:=|\alpha_{2}(t)\rangle gives

an=(α2(0))nn!e12|α2(0)|2,bn=(α2(0))nn!e12|α2(0)|2,a_{n}=\frac{\left(\alpha_{2}(0)\right)^{n}}{\sqrt{n!}}\,e^{-\frac{1}{2}\,|\alpha_{2}(0)|^{2}}\,,\qquad b_{n}=\frac{\left(\alpha_{2}(0)\right)^{n}}{\sqrt{n!}}\,e^{-\frac{1}{2}\,|\alpha_{2}(0)|^{2}}\,, (56)

so that,

α2(0)|α2(t)=e|α2(0)|2n=0N(|α2(0)|2)nn!eiznt.\left\langle\alpha_{2}(0)|\alpha_{2}(t)\right\rangle=e^{-\left|\alpha_{2}(0)\right|^{2}}\sum_{n=0}^{N}\frac{\left(\left|\alpha_{2}(0)\right|^{2}\right)^{n}}{n!}\,e^{-iz_{n}t}\,. (57)

So far, we have presented our discussion on the quasi-coherent states based in the properties of the Friedrichs model. In the next sections, we will present another approach, in such a way that the above discussion can be applied to decoherence and the Loschmidt echo.

In this case, we may redefine (38) and (39), and then

|αi(0)=e12|αi(0)|2n=0(αi(0))nn!|fnD,i=1,2.|\alpha_{i}(0)\rangle=e^{-\frac{1}{2}\,|\alpha_{i}(0)|^{2}}\sum_{n=0}^{\infty}\frac{(\alpha_{i}(0))^{n}}{\sqrt{n!}}\,|f_{n}^{D}\rangle\,,\qquad i=1,2\,. (58)

Following the discussion in [67], we repeat the procedure outlined in Section 3.1 to the present situation. Now, zn=nz0z_{n}=nz_{0} and the sum over nn goes to infinite. As initial values, we choose

α1(0)=0,α2(0)0.\alpha_{1}(0)=0\,,\qquad\alpha_{2}(0)\neq 0. (59)

The macroscopicity condition now means that α2(0)>>1\alpha_{2}(0)>>1. Then, equations (51), (53), (55) and (57) now give, respectively,

α1(0)|α1(t)=1,α1(0)|α1(t)=e12|α2(0)|20,α2(0)|α1(t)=e12|α2(0)|20,\langle\alpha_{1}(0)|\alpha_{1}(t)\rangle=1\,,\quad\langle\alpha_{1}(0)|\alpha_{1}(t)\rangle=e^{-\frac{1}{2}\,|\alpha_{2}(0)|^{2}}\approx 0\,,\quad\langle\alpha_{2}(0)|\alpha_{1}(t)\rangle=e^{-\frac{1}{2}\,|\alpha_{2}(0)|^{2}}\approx 0\,, (60)
α2(0)|α2(t)=exp{|α2(0)|2}eiz0t.\langle\alpha_{2}(0)|\alpha_{2}(t)\rangle=\exp\left\{-|\alpha_{2}(0)|^{2}\right\}\,e^{-iz_{0}t}\,. (61)

Consequently, the non-diagonal coefficients defined in (43), and explicitly given in its general form in (4.2), take in this case the approximate following values:

ρ12ND(t)abexp{|α2(0)|2}eiz0t,\rho_{12}^{\mathrm{ND}}(t)\approx ab^{*}\,\exp\left\{-|\alpha_{2}(0)|^{2}\right\}\,e^{-iz_{0}t}\,, (62)

and

ρ21NDabexp{|α2(0)|2}eiz0t.\rho_{21}^{\mathrm{ND}}\approx a^{*}b\,\exp\left\{-|\alpha_{2}(0)|^{2}\right\}\,e^{-iz_{0}t}\,. (63)

We see that as tt\longmapsto\infty, the non-diagonal terms are of the order of exp{|α2(0)|2}0\exp\{-|\alpha_{2}(0)|^{2}\}\approx 0, which shows decoherence in the preferred basis.

This formalism may be extended to a Friedrichs model with N+1N+1 bound states for H0H_{0} and, hence, with N+1N+1 resonance poles, z0,,zNz_{0},\dots,z_{N}. In this case, equations (62) and (63) take the following forms, respectively,

ρ12ND(t)abexp{|α2(0)|2}n=0N(|α2(0)|2)nn!eiznt\rho_{12}^{\mathrm{ND}}(t)\approx ab^{*}\,\exp\left\{-|\alpha_{2}(0)|^{2}\right\}\sum_{n=0}^{N}\frac{(|\alpha_{2}(0)|^{2})^{n}}{n!}\,e^{-\frac{i}{\hbar}z_{n}t} (64)

and

ρ12ND(t)abexp{|α2(0)|2}n=0N(|α2(0)|2)nn!eiznt.\rho_{12}^{\mathrm{ND}}(t)\approx a^{*}b\,\exp\left\{-|\alpha_{2}(0)|^{2}\right\}\sum_{n=0}^{N}\frac{(|\alpha_{2}(0)|^{2})^{n}}{n!}\,e^{-\frac{i}{\hbar}z_{n}t}\,. (65)

These results show that the non-diagonal elements of the density matrix go to cero when time goes to infinite. This process is called decoherence. In previous works [68, 69, 70], more examples of this phenomenon have been studied using non-hermitian Hamiltonians.

As is known, the decoherence is an irreversible process [71], therefore there is some kind of irreversibility in this model. This motivates us to study more aspects of the irreversibility of this model. In particular, in this work we are interested in the Loschmidt echo phenomenon.

4.3 Loschmidt echo

As we have seen in equation (33), M(τ)M(\tau) can be expressed as

M(τ)=n=0Neτγn/α2(0)|fnDfnG|α2(0).\displaystyle M(\tau)=\sum_{n=0}^{N}e^{-\tau\gamma_{n}/\hbar}\langle\alpha_{2}(0)|f_{n}^{D}\rangle\langle f_{n}^{G}|\alpha_{2}(0)\rangle\,. (66)

Now, using the identity (39) and relations (14), we have that

fnG|α2(0)=(k=0N|α2(0)|2kk!)1/2(α2(0))nn!.\displaystyle\langle f_{n}^{G}|\alpha_{2}(0)\rangle=\left(\sum_{k=0}^{N}\frac{|\alpha_{2}(0)|^{2k}}{k!}\right)^{-1/2}\frac{(\alpha_{2}(0))^{n}}{\sqrt{n!}}\,. (67)

Analogously, using (41), one has that

α2(0)|fnD=(k=0N|α2(0)|2kk!)1/2(α2(0))nn!,\langle\alpha_{2}(0)|f_{n}^{D}\rangle=\left(\sum_{k=0}^{N}\frac{|\alpha_{2}(0)|^{2k}}{k!}\right)^{-1/2}\frac{(\alpha_{2}^{*}(0))^{n}}{\sqrt{n!}}\,, (68)

so that

α2(0)|M(τ)|α2(0)=An=0N|α2(0)|2nn!eτγn/\langle\alpha_{2}(0)|M(\tau)|\alpha_{2}(0)\rangle=A\sum_{n=0}^{N}\frac{|\alpha_{2}(0)|^{2n}}{n!}e^{-\tau\gamma_{n}/\hbar}

with

A=(k=0N|α2(0)|2kk!)1(k=0|α2(0)|2kk!)1=exp{|α2(0)|2}A=\left(\sum_{k=0}^{N}\frac{|\alpha_{2}(0)|^{2k}}{k!}\right)^{-1}\approx\left(\sum_{k=0}^{\infty}\frac{|\alpha_{2}(0)|^{2k}}{k!}\right)^{-1}=\exp\{-|\alpha_{2}(0)|^{2}\}\, (69)

and the latter approximation makes sense for NN large, so that

α2(0)|M(τ)|α2(0)e|α2(0)|2n=0N|α2(0)|2nn!eτγn/\langle\alpha_{2}(0)|M(\tau)|\alpha_{2}(0)\rangle\approx e^{-|\alpha_{2}(0)|^{2}}\sum_{n=0}^{N}\frac{|\alpha_{2}(0)|^{2n}}{n!}e^{-\tau\gamma_{n}/\hbar} (70)

Comparing equation (70) with equations (64) and (65), it is observed that, in both cases, the decay rate is related to the imaginary part of the Hamiltonian eigenvalues. In the first case, the decay is accompanied by an oscillation, while in the second case it is not. In both cases the characteristic times of the exponential decays are the same.

The result shows that there is an intimate relationship between both phenomena. This connection is not surprising since the Loschmidt echo and quantum decoherence can be considered as two expressions of the irreversibility of quantum systems. However, it is of significant importance since it links two phenomena that have been studied separately.

5 Conclusions

The Gamow vectors formalism has been developed in order to give a mathematical description of quantum decay phenomena, such as radioactive phenomena, scattering or decoherence. In this paper we extend the scope of this formalism. We use the Gamow vectors to describe the Loschmidt echo.

The irreversible character of the Loschmidt echo can be studied in two manners. One approach considers that the time evolution is perfectly unitary, but there are imperfections in the implementation of the time reversal operation. The backward and forward evolution process are governed by two slightly different Hamiltonians. This can be attributed to the noise introduced by the environment. The other approach is to assume that the time evolution operator is not unitary, which introduces an intrinsic irreversibility of the time evolution. This kind of evolutions are well represented by the Gamow vector formalism.

In this paper, we adopted the second approach: we used Gamow vectors to describe the Loschmidt echo phenomenon. We showed that the characteristic time of this process is directly associated with the resonances of the analytical continuation of the Hamiltonian. Moreover, we proved that the type of decay obtained is related to the number of resonances of the system and their relative weight in the initial state.

Additionally, we compared this phenomenon with another well known one: the decoherence process. In this case, the resonances are related to the decoherence and relaxation times. We considered a toy model based on the Friedrichs model. We showed that choosing as the initial state a superposition of two quasi-coherent states, and taking into account the macroscopicity condition, decoherence and Loschmidt echo can be described simultaneously. Moreover, the characteristic time of the Loschmidt echo is related with the decoherence time, since both times are determined by the same resonances. Therefore, we have concluded that, under our hypothesis, the Loschmidt echo and decoherence, can be considered as two aspects of the same phenomenon, and that there is a mathematical relation between their corresponding characteristic times.

Acknowledgements

This research was partially supported by grants of FONCYT, CONICET, Universidad Austral, Universidad de Buenos Aires; and the Junta de Castilla y León and FEDER projects (BU229P18 and VA137G18).

F.H. is partially supported by “RASSR40341: Per un’estensione semantica della Logica Computazionale Quantistica - Impatto teorico e ricadute implementative”.

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