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still more typos in initial slip (thx richard)
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@ -555,18 +555,19 @@ slip in \cref{sec:pure_deph} .
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\section{Pure Dephasing and the Initial Slip}
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\label{sec:pure_deph}
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As seen in \cref{fig:comp_finite_t,fig:comp_zero_t,fig:comp_two_bath},
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the short time behavior of the bath energy flow is dominated by
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characteristic peak at short times. Because this peak occurs at very
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short time scales, it may in part be explained by a simple calculation
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which neglects the system dynamics by setting \(H_\sys=0\).
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As evidenced in
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\cref{fig:comp_finite_t,fig:comp_zero_t,fig:comp_two_bath}, the short
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time behavior of the bath energy flow is dominated by a characteristic
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peak. Because this peak occurs at very short time scales, it may in
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part be explained by a simple calculation which neglects the system
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dynamics by setting \(H_\sys=0\).
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We solve the model with the Hamiltonian (Schr\"odinger picture)
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\begin{equation}
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\label{eq:puredeph}
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H = L^†(t) B + L(t) B^† + H_\bath
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\end{equation}
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with \(L(t)=L(t)^†\), \([L(t), L(s)] = 0\;\forall t,s\) (so that
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with \(L(t)=L(t)^†\), \([L(t), L(s)] = 0\;\forall t,s\) (so that the
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Heisenberg Hamiltonian matches \cref{eq:puredeph}) and \(B,\,H_\bath\)
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as in \cref{sec:nmqsd_basics}.
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@ -586,22 +587,23 @@ This allows us to calculate
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g_λ^\ast∫_0^t\dd{s} L(s) ∂_t \eu^{-\iu ω_λ (t-s)}] + \hc,
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\end{equation}
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which gives with a state of the form \(ρ=\ketbra{ψ} \otimes ρ_β\)
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(\(ρ_β\) being a thermal state of inverse temperature \(β\))
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\begin{equation}
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\label{eq:pureflowexpectation}
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\ev{\dot{H}_\bath } = -2 ∫_0^t\dd{s}\ev{L(t)L(s)} \Im[\dot{α}(t-s)].
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\ev{\dot{H}_\bath } = -2 ∫_0^t\dd{s}\ev{L(t)L(s)} \Im[\dot{α}(t-s)],
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\end{equation}
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where \(ρ_β\) is a Gibbs state of inverse temperature \(β\).
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For time independent \(L\) this becomes
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\begin{equation}
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\label{eq:pureflowtimeindep}
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\ev{\dot{H}_\bath } = -2 \ev{L^2} \Im[α(t)].
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\end{equation}
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Note that \(α\) is the zero temperature BCF.
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The proportionality to the imaginary BCF \(α\) does explain the
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initial peak in the bath energy flow. The imaginary part of the BCF is
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zero for \(t=0\) and then usually features a peak at rather short
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times (assuming finite correlation times). For the ohmic BCF used here
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and shown in \cref{fig:ohm_bcf_ex}, this feature is very prominent.
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initial peak in the bath energy flow. The imaginary part is zero for
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\(t=0\) and then usually features a peak at rather short times
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(assuming finite correlation times). For the Ohmic BCF used here and
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plotted in \cref{fig:ohm_bcf_ex} this feature is very prominent.
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\begin{figure}[htp]
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\centering
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\includegraphics{figs/misc/ohmic_bcf_example.pdf}
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@ -613,12 +615,12 @@ Generically, the imaginary part of the BCF is negative at least for
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short times as it takes the form
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\begin{equation}
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\label{eq:negtive_imag}
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\Im[α(τ)] = -\frac{1}{π}∫_{0}^{τ}J(ω) \sin(ωτ)\dd{ω}
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\Im[α(τ)] = -\frac{1}{π}∫_{0}^{∞}J(ω) \sin(ωτ)\dd{ω}
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\end{equation}
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which is negative for \(τ\leq π/ω_{\mathrm{max}}\), where
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\(ω_{\mathrm{max}}\) is a characteristic cutoff frequency of the
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system. The direction of the initial slip flow for unmodulated systems
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will therefore be always be into the bath compensating for negative
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will therefore always be into the bath compensating for negative
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interaction energy.
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Interestingly, \cref{eq:pureflowexpectation} does not contain any
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@ -628,15 +630,14 @@ match the zero temperature case in which the bath has minimal energy
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in the initial state.
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A thermodynamically useful model should feature significant system
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dynamics which is always given assuming that the coupling is no too
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strong. Coupling that is not self-adjoint \fixme{plot: if time, i
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could do the energy shovel with non-hermitian} may also have this
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effect, but in the literature most effective qubit models tend to
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favour Hermitian couplings
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dynamics which is always given, assuming that the coupling is no too
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strong. Non hermitian coupling may also have this effect, but in the
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literature most effective qubit models tend to favour Hermitian
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couplings
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\cite{Aurell2019Apr,Hita-Perez2021Nov,Hita-Perez2021Aug,MacQuarrie2020Sep,Andersen2017Feb,Mezzacapo2014Jul}. For
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the spin-boson model, non Hermitian coupling it is the result of the
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rotating wave approximation assuming that system and bath scales are
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quite different, which however does not imply weak
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the spin-boson model, non Hermitian coupling is the result of the
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rotating wave approximation under the assumption that system and bath
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time scales are quite different, which however does not imply weak
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coupling~\cite{Irish2007Oct}.
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For completeness, the interaction energy is given by
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@ -683,13 +684,14 @@ here the convention in which \(α\) is dimensionless is used.
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The Ohmic-type BCF is
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\begin{equation}
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\label{eq:normohmic}
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α(τ)=\frac{ω_c s }{ (\max_t\norm{H})(1+\iu ω_c τ)^{s+1}},
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α(τ)=\frac{ω_c}{\max_t\norm{H} (1+\iu ω_c τ)^{2}},
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\end{equation}
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in this normalization.
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After this brief detour we will again concentrate on the numerical
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aspects and the phenomenology of the energy flow of the spin-boson
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model in \cref{sec:prec_sim}.
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This concludes the discussion, and we will move on to concentrate on
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the numerical aspects and the phenomenology of the energy flow of the
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spin-boson model in \cref{sec:prec_sim}.
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\section{Precision Simulations of the Zero Temperature Spin-Boson Model}
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\label{sec:prec_sim}
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