REVIEW 3 major objections 7 minor 73 references
Ancilla-Shielded Qubit Measures AdS Temperature via Non-Markovian Memory
Reviewed by Pith at T0; open to challenge. T0 means a machine referee read the full paper against a public rubric. the ladder, T0–T4 →
T0 review · glm-5.2
2026-07-09 06:42 UTC pith:PE7OWWFO
load-bearing objection Ancilla-mediated UDW thermometry in AdS — interesting setup, but the master equation has a structural inconsistency that needs resolving before the numerical results can be trusted. the 3 major comments →
Relativistic Quantum Thermometry in AdS Spacetime via Non-Markovian Temperature Sensing
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The paper's central result is that an ancillary Unruh-DeWitt detector, interposed between a protected probe qubit and an AdS thermal bath, serves as an information router: it absorbs thermal information from the spacetime and transfers it to the probe's off-diagonal coherence, while the probe itself remains shielded from dissipative decoherence. Crucially, the strength of the probe-ancilla coupling controls a transition from Markovian to non-Markovian probe dynamics, and the non-Markovian regime produces oscillatory enhancements in the Quantum Fisher Information and quantum signal-to-noise ratio that exceed what a directly coupled probe can achieve, with the strongest gains occurring at low.
What carries the argument
The mechanism is a three-layer open quantum system: (1) the AdS spacetime with a massless scalar field acting as a thermal reservoir, (2) an ancillary Unruh-DeWitt detector linearly coupled to the field and undergoing Markovian dissipation governed by a Kossakowski-Lindblad master equation whose coefficients are determined by the AdS Wightman function, and (3) a probe qubit coupled to the ancilla via an exchange-type Hamiltonian with strength kappa. The ancilla's Kossakowski matrix encodes the spacetime's temperature, acceleration, curvature, and boundary conditions. Temperature information enters the probe through the coherence channel of the exchange interaction, and increasing kappa above
Load-bearing premise
The load-bearing premise is that the Born-Markov master equation used to describe the ancilla's interaction with the field remains valid while the probe-ancilla coupling simultaneously induces non-Markovian dynamics on the probe. The consistency of deriving Markovian dissipative coefficients and then using them to generate non-Markovian behavior through the inter-qubit coupling is not rigorously justified, and the regime where both approximations hold simultaneously is not
What would settle it
If the probe-ancilla coupling kappa is increased into the strongly non-Markovian regime, the Born-Markov approximation for the ancilla-field interaction may break down, invalidating the Kossakowski matrix and thus the temperature encoding channel. A fully non-perturbative treatment could show that the QFI enhancement reverses or that the probe does not actually acquire reliable thermal information, falsifying the central claim.
If this is right
- If the ancilla-mediated shielding protocol is valid, it provides a design template for quantum sensors that can estimate parameters of extreme or inaccessible environments without directly exposing delicate quantum probes to decoherence.
- The finding that non-Markovian backflow enhances thermometric precision suggests that engineering structured environments with memory effects could be a general strategy for improving quantum metrology beyond Markovian limits.
- The identification of finite optimal times and temperatures for maximum QFI implies that quantum thermometry protocols have a nontrivial operating window, not simply 'longer is better,' which has practical consequences for probe design.
- The boundary-condition dependence at low temperatures but not at high temperatures suggests that AdS boundary effects could be used as a diagnostic knob for calibrating or testing thermometric protocols in curved spacetime analog systems.
Where Pith is reading between the lines
- The protocol could in principle be tested in analogue gravity systems (e.g., superconducting circuits or trapped ions simulating AdS geometries) where an ancilla-mediated coupling architecture is experimentally realizable, providing a tabletop test of relativistic quantum thermometry claims.
- If the non-Markovian enhancement scales with system size or ancilla complexity, extending the protocol to multiple ancillas or networked probe-ancilla chains could yield a scaling advantage in precision, potentially approaching Heisenberg-limited thermometry.
- The tension between using a Markovian-derived master equation for the ancilla and claiming non-Markovian dynamics for the probe suggests that a fully non-perturbative or exact treatment of the ancilla-field coupling might reveal additional corrections to the QFI that are absent in the current weak-coupling analysis.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. This manuscript proposes a quantum thermometry protocol in which a protected probe qubit is coupled to an ancillary Unruh-DeWitt detector that interfaces directly with a thermal scalar field in AdS spacetime. The authors argue that the ancilla channels temperature information into the probe's coherence, and that increasing the probe-ancilla coupling κ induces non-Markovian dynamics on the probe that enhance the Quantum Fisher Information (QFI) and quantum signal-to-noise ratio (QSNR), particularly at low temperatures. The paper analyzes the roles of detector acceleration, boundary conditions (Dirichlet/transparent/Neumann), energy gap, and interaction time, and identifies optimal operating conditions. The framework combines open quantum system techniques (GKSL master equations) with quantum estimation theory in curved spacetime.
Significance. The idea of using an ancillary detector as a thermal intermediary to shield a probe from direct decoherence while retaining thermometric sensitivity is a reasonable extension of pseudo-mode and ancilla-assisted thermometry approaches to the curved-spacetime setting. The paper explores an interesting parameter space (AdS boundary conditions, acceleration threshold, non-Markovian coupling) and provides falsifiable predictions for optimal sensing times and temperatures. However, the significance is substantially undermined by a load-bearing inconsistency in the master equation and the absence of the explicit solutions from which all results are derived, as detailed below.
major comments (3)
- §IV, Eqs. (34) and (37): The paper states that χ₂ is set to zero because the probe is protected from the scalar field. This means the probe does not couple to the field at all. However, the GKSL dissipator in Eq. (34) sums over m,n = 1,2 (both probe and ancilla), and Eq. (37) then sets all Kossakowski matrices equal: Λ^(aa) = Λ^(bb) = Λ^(ab) = Λ^(ba) ≡ Λ_ij. If the probe is truly decoupled from the field, then the probe self-correlation Λ^(PP) and the cross-correlations Λ^(PA), Λ^(AP) should all vanish — only the ancilla self-correlation Λ^(AA) should be nonzero. Setting all four equal either implies the probe also couples to the field (contradicting the protected-probe setup) or forces all dissipative terms to zero (eliminating the bath). This inconsistency is load-bearing because the master equation is the starting point for every QFI and QSNR result in the paper. The authors must (i)写
- §IV, Eq. (42): The probe's reduced density matrix is written in terms of functions A(t) and B(t), but these functions are never explicitly defined or derived. Appendix A only solves the single-detector case (Eqs. A12–A14), not the two-detector probe+ancilla system. Since all QFI and QSNR results (Figures 2, 5, 7, 8, 9) depend on A(t) and B(t), their absence makes the central results unverifiable. The authors should provide the explicit analytical or numerical expressions for A(t) and B(t), or at minimum describe the procedure used to obtain them.
- §IV, Eq. (37) and surrounding text: The simplification 'in the regime of sufficiently small interatomic separation one may set all Kossakowski matrices equal' is stated without justification. In the present setup, the probe is protected from the field and only the ancilla couples to it; there is no 'interatomic separation' between two field-coupled detectors to justify this approximation. If the authors intend a different physical configuration than what is described (e.g., both detectors coupled to the field with different strengths), this must be clarified and the master equation rederived consistently.
minor comments (7)
- Notation is inconsistent throughout: the detector energy gap is denoted both ω and Ω (e.g., §III.B uses Ω in Eq. (19) but ω in Eq. (24); §IV uses ω_P and ω_A). The coupling strength is denoted both η and λ (Eq. (19) text says 'where λ denotes the coupling strength' but the equation uses η). Please unify.
- References are duplicated: [42] and [34] both cite Paris (2009); [43] and [35] both cite Ma and Wang (2009); [44] and [36] both cite Wu and Xu (2016); [47] and [37] both cite Fröwis (2012); [48] and [38] both cite Deffner and Campbell (2017); [49] and [39] both cite Lu et al. (2010); [50] and [41] both cite Song et al. (2015). Please consolidate.
- §III.B, Eqs. (25)–(28): The response functions are presented in multiple algebraically equivalent forms without clear motivation. Consider consolidating to one canonical form and stating equivalences once.
- §VII.B: There is a broken citation '[?]' in the text ('quantum signal-to-noise ratio (QSNR) [ ? ]').
- Figure captions could be more informative: several figures (e.g., Fig. 3, Fig. 4) describe panels as 'left/medium/lower' but the layout is described as 'top panel' with sub-panels. Please clarify the figure structure.
- §II: The sentence beginning 'we employ the information-backflow measure' has a lowercase 'we' mid-sentence. Several other sentences have grammatical issues (e.g., 'analyic' in the table of contents description of Appendix A).
- The abstract claims 'For the first time, we introduce an ancillary Unruh-DeWitt detector between the sensor and the thermal bath.' Ancilla-assisted and pseudo-mode thermometry protocols are well established in flat-space settings; the novelty claim should be scoped to the curved-spacetime/AdS context.
Simulated Author's Rebuttal
We thank the referee for a careful reading and for identifying two substantive issues: an inconsistency in the Kossakowski matrix structure of the master equation, and the absence of explicit solutions for A(t) and B(t). We agree that both must be addressed in a revised manuscript and describe below the specific corrections we will make.
read point-by-point responses
-
Referee: §IV, Eqs. (34) and (37): The paper states that χ₂ is set to zero because the probe is protected from the scalar field. This means the probe does not couple to the field at all. However, the GKSL dissipator in Eq. (34) sums over m,n = 1,2 (both probe and ancilla), and Eq. (37) then sets all Kossakowski matrices equal: Λ^(aa) = Λ^(bb) = Λ^(ab) = Λ^(ba) ≡ Λ_ij. If the probe is truly decoupled from the field, then the probe self-correlation Λ^(PP) and the cross-correlations Λ^(PA), Λ^(AP) should all vanish — only the ancilla self-correlation Λ^(AA) should be nonzero. Setting all four equal either implies the probe also couples to the field (contradicting the protected-probe setup) or forces all dissipative terms to zero (eliminating the bath). This inconsistency is load-bearing because the master equation is the starting point for every QFI and QSNR result in the paper.
Authors: The referee is correct. In the protected-probe setup, only the ancilla couples to the scalar field (χ₂ = 0), so the Kossakowski matrices must reflect this asymmetry: Λ^(AA) is the only nonzero field-induced correlation matrix, while Λ^(PP) = Λ^(PA) = Λ^(AP) = 0. The statement in Eq. (37) that all four Kossakowski matrices are equal was carried over from a two-detector configuration (both detectors field-coupled, small separation) and is inconsistent with the protected-probe geometry. We will correct the master equation accordingly: the GKSL dissipator will be rewritten with the sum restricted so that only the ancilla indices contribute to the field-induced dissipation, and the Kossakowski matrix Λ^(AA) will be expressed in terms of the AdS Wightman function as in Appendix A. The probe-ancilla coupling κ in H_S is unaffected and remains the channel through which temperature information reaches the probe. All QFI and QSNR results will be rederived from the corrected master equation. We expect the qualitative phenomenology (ancilla-mediated thermal sensitivity, κ-enhanced non-Markovianity, low-temperature precision advantage) to persist, but the quantitative results will change and must be recomputed. revision: yes
-
Referee: §IV, Eq. (42): The probe's reduced density matrix is written in terms of functions A(t) and B(t), but these functions are never explicitly defined or derived. Appendix A only solves the single-detector case (Eqs. A12–A14), not the two-detector probe+ancilla system. Since all QFI and QSNR results (Figures 2, 5, 7, 8, 9) depend on A(t) and B(t), their absence makes the central results unverifiable. The authors should provide the explicit analytical or numerical expressions for A(t) and B(t), or at minimum describe the procedure used to obtain them.
Authors: The referee is correct that A(t) and B(t) are not explicitly defined in the current manuscript and that Appendix A only covers the single-detector case. We will add a new appendix (or substantially expand Appendix A) that derives the probe-ancilla master equation solution. Concretely, the corrected master equation (with only Λ^(AA) nonzero) is a linear system for the 15 real components of the 4×4 density matrix ρ_PA(t). After tracing out the ancilla, A(t) and B(t) are expressed as linear combinations of these components with coefficients determined by κ, ω_P, ω_A, and the Kossakowski parameters A', B', C' (which themselves depend on T, a, ℓ, ζ through the AdS response function). We will present the explicit ODE system, the method of solution (analytical where tractable, numerical otherwise), and the resulting closed-form or algorithmic expressions for A(t) and B(t). This will make all figures reproducible. revision: yes
-
Referee: §IV, Eq. (37) and surrounding text: The simplification 'in the regime of sufficiently small interatomic separation one may set all Kossakowski matrices equal' is stated without justification. In the present setup, the probe is protected from the field and only the ancilla couples to it; there is no 'interatomic separation' between two field-coupled detectors to justify this approximation. If the authors intend a different physical configuration than what is described (e.g., both detectors coupled to the field with different strengths), this must be clarified and the master equation rederived consistently.
Authors: We agree with the referee. The 'small interatomic separation' argument is inapplicable to the protected-probe configuration, where only the ancilla couples to the field. This text was inherited from the two-detector open-system literature and was not properly adapted to our setup. In the revised manuscript we will remove this justification entirely and replace it with the correct structure: Λ^(AA) is computed from the AdS Wightman function as in Appendix A, and Λ^(PP) = Λ^(PA) = Λ^(AP) = 0 by construction (since χ₂ = 0). The physical configuration is as described in the abstract and Figure 1: the probe is shielded from the scalar field and acquires temperature information only through the coherent coupling κ to the ancilla. We will state this unambiguously and rederive the master equation from first principles for this configuration. revision: yes
Circularity Check
Minor self-citation for background framework; central results computed from independent model equations
specific steps
-
self citation load bearing
[Section IV, Eq. (32) and Section II, Eqs. (3)-(9)]
"In the weak-coupling, Born–Markov regime one may eliminate the field degrees of freedom and derive a Gorini–Kossakowski–Lindblad master equation for the detectors' reduced state: ∂ρab(t)/∂t = −i[Heff, ρab(t)] + L[ρab(t)]. ... For any unbiased estimator ... the variance is lower-bounded by the classical Cramér–Rao inequality [45, 46]"
References [24] (Hminat et al., Phys. Rev. E, 2025) and [45] (Hminat et al., arXiv:2509.10840, 2025) are self-citations providing the master equation framework and estimation theory background. However, these are standard, widely-available formulations (GKSL master equation, quantum Cramér–Rao bound, QFI in Bloch representation). The cited results are not unique theorems that forbid alternatives, and the paper re-derives the key equations (Eqs. 3-9, 32-42) explicitly. The self-citations serve as background pointers rather than load-bearing logical dependencies. The central results—QFI and QSNR as functions of κ, T, ω, ζ—are computed from the model equations (Eq. 30, 42) and the AdS response function (Eq. 25/28), not from the self-cited works.
full rationale
The paper has two self-citations ([24] and [45]) by the same authors, but they reference standard open quantum systems and quantum estimation theory (GKSL master equation, quantum Cramér–Rao bound). These are not unique theorems invoked to force the paper's conclusions, and the paper re-derives the relevant equations itself. The central claims about ancilla-mediated thermometric enhancement are grounded in the independently stated Hamiltonian (Eq. 30), the AdS Wightman function (Eq. 22), the response function (Eq. 25/28), and the QFI formula (Eq. 8). No prediction reduces to a fitted input by construction, and no ansatz is smuggled in via self-citation. The derivation chain is largely self-contained. The score of 2 reflects the presence of self-citations that, while not load-bearing for the logical argument, do provide the framework context.
Axiom & Free-Parameter Ledger
free parameters (6)
- κ (probe-ancilla coupling) =
0.1, 0.25, 0.5, 0.99
- ω (detector energy gap) =
0.05, 0.275, 0.5
- a (detector acceleration) =
2, 2.5, 3, 5, 7, 10
- ζ (boundary condition) =
-1, 0, 1
- T (temperature) =
0.4 and others
- η (coupling strength) =
1, 0.5, 0.2
axioms (4)
- domain assumption Born-Markov approximation for the detector-field interaction
- domain assumption Pointlike detectors without switching functions
- domain assumption Local quantum estimation theory assumes prior coarse knowledge of T
- domain assumption Kossakowski matrices are equal for all detector pairs at small separation
invented entities (1)
-
Ancillary Unruh-DeWitt detector as a thermal intermediary
no independent evidence
read the original abstract
Quantum thermometry based on single-qubit sensor configurations enables the precise estimation of the temperature of a cosmological Anti-de Sitter (AdS) spacetime. In this work, we characterize the achievable estimation accuracy using the Quantum Fisher Information (QFI) and the associated quantum signal-to-noise ratio. For the first time, we introduce an ancillary Unruh-DeWitt detector between the sensor and the thermal bath, enhancing thermometric sensitivity by channeling temperature-dependent information into the probe qubit's coherence. We examine how detector acceleration in AdS space and the choice of boundary conditions modify the probe's thermal sensitivity. Despite the differing geometries, a unified phenomenology emerges: we characterize the scaling of the QFI with respect to temperature, detector energy gap, spacetime curvature, and interaction time. Finally, we identify optimal state preparation and measurement strategies that maximize the QFI, thereby establishing the fundamental limits of precision for non-Markovian sensing in curved spacetime.
Figures
Reference graph
Works this paper leans on
-
[1]
R. B. Mann and T. C. Ralph,Class. Quant. Grav.29, 220301 (2012)
work page 2012
-
[2]
K. El Bouzaidi, A. Slaoui, L.B. Drissi, et al.,Eur. Phys. J. C, 85, 1349 (2025)
work page 2025
- [3]
-
[4]
W. G. Unruh,Phys. Rev. D14, 870 (1976)
work page 1976
-
[5]
B. S. DeWitt,Quantum gravity: the new synthesis, inGeneral Relativity: An Einstein Centenary Survey, ed. S. Hawking and W. Israel (Cambridge University Press, 1979)
work page 1979
-
[6]
X. Y . Huang, J. Feng, Y . Z. Zhang, and H. Fan,Ann. Phys.397, 336 (2018)
work page 2018
- [7]
- [8]
- [9]
- [10]
- [11]
-
[12]
G. L. Sewell,Ann. Phys.141, 201 (1982)
work page 1982
-
[13]
S. W. Hawking,Commun. Math. Phys.43, 199 (1975)
work page 1975
- [14]
-
[15]
T. Baumgratz, M. Cramer, and M. B. Plenio,Phys. Rev. Lett. 113, 140401 (2014)
work page 2014
-
[16]
L. Michalski, K. Eckersdorf, J. Kucharski, and J. McGhee,Tem- perature measurement, Meas. Sci. Technol.13, 1651 (2002)
work page 2002
-
[17]
F. Giazotto, T. T. Heikkil ¨a, A. Luukanen, A. M. Savin, and J. Pekola,Opportunities for mesoscopics in thermometry and refrigeration: Physics and applications, Rev. Mod. Phys.78, 217 (2006)
work page 2006
-
[18]
C. D. S. Brites, P. P. Lima, N. J. O. Silva, A. Mill´an, V . S. Ama- ral, F. Palacio, and L. D. Carlos,Thermometry at the nanoscale, Nanoscale4, 4799 (2012)
work page 2012
-
[19]
S. Razavian, C. Benedetti, M. Bina, Y . Akbari-Kourbolagh, and M. G. A. Paris,Quantum thermometry by single-qubit dephas- ing, Eur. Phys. J. Plus134, 284 (2019)
work page 2019
- [20]
-
[21]
A. De Pasquale, D. Rossini, R. Fazio, and V . Giovannetti,Lo- cal quantum thermal susceptibility, Nat. Commun.7, 12782 (2016)
work page 2016
-
[22]
M. Mehboudi, A. Lampo, C. Charalambous, L. A. Correa, M. A. Garc ´ıa-March, and M. Lewenstein,Using polarons for sub-nK quantum nondemolition thermometry in a Bose– Einstein condensate, Phys. Rev. Lett.122, 030403 (2019)
work page 2019
-
[23]
K. V . Hovhannisyan and L. A. Correa,Measuring the temper- ature of cold many-body quantum systems, Phys. Rev. B98, 045101 (2018)
work page 2018
- [24]
-
[25]
M. Scigliuzzo, A. Bengtsson, J.-C. Besse, A. Wallraff, P. Dels- ing, and S. Gasparinetti,Primary thermometry of propagating microwaves in the quantum regime, Phys. Rev. X10, 041054 (2020)
work page 2020
-
[26]
S. S. Mirkhalaf, D. Benedicto Orenes, M. W. Mitchell, and E. Witkowska,Criticality-enhanced quantum sensing in ferro- magnetic Bose–Einstein condensates: Role of readout measure- ment and detection noise, Phys. Rev. A103, 023317 (2021)
work page 2021
-
[27]
D.-J. Zhang and D. M. Tong,Approaching Heisenberg-scalable thermometry with built-in robustness against noise, npj Quan- tum Inf.8, 81 (2022)
work page 2022
-
[28]
M. Brunelli, S. Olivares, M. Paternostro, and M. G. A. Paris, Qubit-assisted thermometry of a quantum harmonic oscillator, Phys. Rev. A86, 012125 (2012)
work page 2012
-
[29]
M. Brunelli, S. Olivares, and M. G. A. Paris,Qubit thermom- etry for micromechanical resonators, Phys. Rev. A84, 032105 (2011)
work page 2011
-
[30]
L. Mancino, M. Sbroscia, I. Gianani, E. Roccia, and M. Bar- bieri,Quantum simulation of single-qubit thermometry using linear optics, Phys. Rev. Lett.118, 130502 (2017)
work page 2017
-
[31]
M. M. Feyles, L. Mancino, M. Sbroscia, I. Gianani, and M. Bar- bieri,Dynamical role of quantum signatures in quantum ther- mometry, Phys. Rev. A99, 062114 (2019)
work page 2019
-
[32]
M. R. Jørgensen, P. P. Potts, M. G. A. Paris, and J. B. Brask, Tight bound on finite-resolution quantum thermometry at low temperatures, Phys. Rev. Res.2, 033394 (2020)
work page 2020
- [33]
- [35]
-
[36]
W. Wu and J.-B. Xu,Geometric phase, quantum Fisher information, geometric quantum correlation and quantum phase transition in the cavity Bose–Einstein-condensate system, Quantum Inf. Process.15, 3695 (2016)
work page 2016
-
[38]
S. Deffner and S. Campbell,Quantum speed limits: From Heisenberg’s uncertainty principle to optimal quantum control, 17 J. Phys. A50, 453001 (2017)
work page 2017
- [40]
-
[42]
M. G. A. Paris,Quantum estimation for quantum technology, Int. J. Quantum Inf.7, 125 (2009)
work page 2009
- [43]
-
[44]
W. Wu and J.-B. Xu,Geometric phase, quantum Fisher information, geometric quantum correlation and quantum phase transition in the cavity–Bose–Einstein-condensate sys- tem, Quantum Inf. Process.15, 3695 (2016)
work page 2016
-
[45]
Hermitian vs non-Hermitian quantum thermometry
A. Hminat, A. Slaoui, R. Ahl Laamara and M. Telmini, arXiv:2509.10840 (2025)
work page internal anchor Pith review Pith/arXiv arXiv 2025
-
[46]
S.Boulifa , A Slaoui, H El Hadfi, R Ahl Laamara, . Appl. Phys. B, 131 (2025) 174
work page 2025
-
[47]
Fr ¨owis,Kind of entanglement that speeds up quantum evolu- tion, Phys
F. Fr ¨owis,Kind of entanglement that speeds up quantum evolu- tion, Phys. Rev. A85, 052127 (2012)
work page 2012
-
[48]
S. Deffner and S. Campbell,Quantum speed limits: From Heisenberg’s uncertainty principle to optimal quantum control, J. Phys. A50, 453001 (2017)
work page 2017
-
[49]
X.-M. Lu, X. Wang, and C. P. Sun,Quantum Fisher information flow and non-Markovian processes of open systems, Phys. Rev. A82, 042103 (2010)
work page 2010
-
[50]
H. Song, S. Luo, and Y . Hong,Quantum non-Markovianity based on the Fisher-information matrix, Phys. Rev. A91, 042110 (2015)
work page 2015
-
[51]
W. G. Unruh,Notes on black hole evaporation, Phys. Rev. D 14, 870 (1976)
work page 1976
-
[52]
B. S. DeWitt,Quantum gravity: The new synthesis, inGen- eral Relativity: An Einstein Centenary Survey, S. Hawking and W. Israel eds., Cambridge University Press, pp. 680–745 (1979)
work page 1979
-
[53]
J. Louko and A. Satz,Transition rate of the Unruh–DeWitt detector in curved spacetime, Class. Quant. Grav.25, 055012 (2008)
work page 2008
-
[54]
Jennings,On the response of a particle detector in Anti–de Sitter spacetime, Class
D. Jennings,On the response of a particle detector in Anti–de Sitter spacetime, Class. Quant. Grav.27, 205005 (2010)
work page 2010
-
[55]
S. Deser and O. Levin,Accelerated detectors and temperature in (anti)–de Sitter spaces, Class. Quant. Grav.14, L163 (1997)
work page 1997
-
[56]
Notes on black hole evaporation,
W. G. Unruh, “Notes on black hole evaporation,”Phys. Rev. D 14(1976) 870
work page 1976
-
[57]
Quantum gravity: the new synthesis,
B. S. DeWitt, “Quantum gravity: the new synthesis,” inGeneral Relativity: An Einstein Centenary Survey, S. W. Hawking and W. Israel (eds.), Cambridge University Press (1979), pp. 680– 745
work page 1979
-
[58]
Transition rate of the Unruh-DeWitt detector in curved spacetime
J. Louko and A. Satz, “Transition rate of the Unruh–DeWitt detector in curved spacetime,”Class. Quant. Grav.25(2008) 055012, arXiv:0710.5671
work page internal anchor Pith review Pith/arXiv arXiv 2008
-
[59]
On the response of a particle detector in Anti-de Sitter spacetime
D. Jennings, “On the response of a particle detector in Anti– de Sitter spacetime,”Class. Quant. Grav.27(2010) 205005, arXiv:1008.2165
work page internal anchor Pith review Pith/arXiv arXiv 2010
-
[60]
Quantum fields on manifolds: PCT and gravita- tionally induced thermal states,
G. L. Sewell, “Quantum fields on manifolds: PCT and gravita- tionally induced thermal states,”Annals Phys.141(1982) 201
work page 1982
-
[61]
Cosmological event hori- zons, thermodynamics, and particle creation,
G. W. Gibbons and S. W. Hawking, “Cosmological event hori- zons, thermodynamics, and particle creation,”Phys. Rev. D15 (1977) 2738
work page 1977
-
[62]
Particle creation by black holes,
S. W. Hawking, “Particle creation by black holes,”Commun. Math. Phys.43(1975) 199 [Erratumibid.46(1976) 206]
work page 1975
-
[63]
Accelerated Detectors and Temperature in (Anti) de Sitter Spaces
S. Deser and O. Levin, “Accelerated detectors and temperature in (anti)–de Sitter spaces,”Class. Quant. Grav.14(1997) L163, arXiv:gr-qc/9706018
work page internal anchor Pith review Pith/arXiv arXiv 1997
- [64]
- [65]
-
[66]
N. D. Birrell and P. Davies,Quantum Fields in Curved Space, Cambridge University Press (1982)
work page 1982
-
[67]
S. J. Avis, C. J. Isham, and D. Storey, Phys. Rev. D18, 3565 (1978)
work page 1978
- [68]
-
[69]
Quantifying Quantumness in (A)dS spacetimes with Unruh-DeWitt Detector
L.-J. Li, X.-K. Song, Y . Liu and D. Wang, “Quantifying quan- tumness in (A)dS spacetimes with Unruh–DeWitt detector,” Phys. Rev. D111(2025) no. 6, 065007, arXiv:2502.07167 [hep- th]
work page internal anchor Pith review Pith/arXiv arXiv 2025
- [70]
-
[71]
H.-P. Breuer and F. Petruccione,The Theory of Open Quantum Systems, Oxford University Press, New York (2002)
work page 2002
-
[72]
P. J. Coles and M. Piani,Phys. Rev. A89, 022112 (2014)
work page 2014
-
[73]
M. L. Hu and H. Fan,Phys. Rev. A86, 032338 (2012)
work page 2012
-
[74]
N. J. Cerf, M. Bourennane, A. Karlsson, and N. Gisin,Phys. Rev. Lett.88, 127902 (2002)
work page 2002
-
[75]
H. P. Breuer, E. M. Laine, and J. Piilo,Measure for the degree of non-Markovian behavior of quantum processes in open sys- tems, Phys. Rev. Lett.103, 210401 (2009)
work page 2009
-
[76]
I. de Vega and D. Alonso,Dynamics of non-Markovian open quantum systems, Rev. Mod. Phys.89, 015001 (2017)
work page 2017
-
[77]
S. Wißmann, A. Karlsson, E.-M. Laine, J. Piilo, and H.- P. Breuer,Optimal state pairs for non-Markovian quantum dy- namics, Phys. Rev. A86, 062108 (2012)
work page 2012
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.