pith. sign in

arxiv: 2508.07830 · v2 · submitted 2025-08-11 · 🌀 gr-qc · hep-th· quant-ph

Memory Effects and Entanglement Dynamics of Finite time Acceleration

Pith reviewed 2026-05-18 23:47 UTC · model grok-4.3

classification 🌀 gr-qc hep-thquant-ph
keywords Unruh-DeWitt detectorfinite-time accelerationmemory effectentanglement harvestingFisher informationRindler trajectorycomplete positivityBogoliubov transformations
0
0 comments X

The pith

Finite-duration acceleration induces a memory effect in Unruh-DeWitt detectors that is quantified by Fisher information while allowing harvested entanglement to return smoothly to initial values.

A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.

This paper introduces a smooth trajectory in Minkowski spacetime where a detector accelerates uniformly only for a finite interval but remains inertial in the distant past and future. The construction allows direct comparison with the usual eternal Rindler case because the new path reduces to the standard Rindler trajectory in a controlled limit. The central result is that a single detector retains a memory of the finite acceleration interval, and this memory is captured quantitatively by the Fisher information. When two detectors follow combinations of these trajectories, the total correlation and the entanglement they harvest both recover their starting values smoothly once acceleration and deceleration end, whereas the transition rate does not. The memory imprint does not produce a measurable change in negativity or mutual information.

Core claim

We construct a smooth trajectory in Minkowski spacetime that is inertial in the asymptotic past and future but undergoes approximately uniform acceleration for a finite duration. In a suitable limit this trajectory reduces to the standard Rindler trajectory, reproducing the expected Bogoliubov transformations and results consistent with the thermal time hypothesis. Analysis of an Unruh-DeWitt detector on this path shows a memory effect due to the finite duration of acceleration, quantified by the Fisher information. For two detectors along various trajectory combinations, unlike the transition rate, both the total correlation and the entanglement harvested return smoothly to their initial值值值

What carries the argument

The smooth finite-time acceleration trajectory in Minkowski spacetime that approximates the Rindler trajectory for a controlled interval and permits comparison with eternal acceleration results.

If this is right

  • Complete positivity divisibility of the detector evolution depends on frequency, acceleration strength, and acceleration duration.
  • The memory effect appears in the detector response and is independently quantified by Fisher information.
  • Harvested entanglement and total correlations between detector pairs are restored after the finite acceleration ends.
  • Correlation measures exhibit the same behavior in accelerating and decelerating segments.
  • The sign of the flux of acceleration-induced radiation carries physical significance for the energy accounting.

Where Pith is reading between the lines

These are editorial extensions of the paper, not claims the author makes directly.

  • The finite-time construction provides a controlled way to interpolate between inertial and accelerated regimes, which may help isolate transient effects in other quantum-field settings.
  • Absence of memory imprint on negativity while it appears in Fisher information suggests that different correlation quantifiers probe distinct aspects of the finite-duration dynamics.
  • The smooth return of entanglement after deceleration raises the possibility that information carried by field correlations is preserved across the entire inertial-to-accelerated-to-inertial sequence.

Load-bearing premise

The chosen smooth trajectory reduces in the appropriate limit to the standard Rindler trajectory while remaining inertial in the asymptotic past and future.

What would settle it

A calculation in which two Unruh-DeWitt detectors on these finite-acceleration trajectories fail to show harvested entanglement returning to its initial value after the acceleration phase would falsify the smooth-recovery claim.

Figures

Figures reproduced from arXiv: 2508.07830 by Nitesh K. Dubey, Sanved Kolekar.

Figure 1
Figure 1. Figure 1: The red curve represents the variable acceleration trajectory given by Eqs. ( [PITH_FULL_IMAGE:figures/full_fig_p006_1.png] view at source ↗
Figure 2
Figure 2. Figure 2: The above plots show the Bogoluobov calculation results for the expectation value of number density observed [PITH_FULL_IMAGE:figures/full_fig_p008_2.png] view at source ↗
Figure 3
Figure 3. Figure 3: The thick lines in the top panels of the plots above represent the transition rate of a UDW detector following [PITH_FULL_IMAGE:figures/full_fig_p012_3.png] view at source ↗
Figure 4
Figure 4. Figure 4: The first plot of the top panel shows P0 for a UDW detector traveling along eternal Rindler trajectory Eqs. (6)- (7) while all other plots of P0 correspond to finite duration accelerated trajectory given in Eqs (3)-(4). In the second plot of the top panel, we show P1 for which P0 is everywhere positive because if P0 is negative, then no need to check P1. 15 [PITH_FULL_IMAGE:figures/full_fig_p015_4.png] view at source ↗
Figure 5
Figure 5. Figure 5: The plots above show the Fisher information with respect to time, considered as the parameter [PITH_FULL_IMAGE:figures/full_fig_p016_5.png] view at source ↗
Figure 6
Figure 6. Figure 6: The above plots show Fisher information considering [PITH_FULL_IMAGE:figures/full_fig_p017_6.png] view at source ↗
Figure 7
Figure 7. Figure 7: Plots showing the mutual information and negativity obtained by the entanglement harvesting protocol [PITH_FULL_IMAGE:figures/full_fig_p020_7.png] view at source ↗
Figure 8
Figure 8. Figure 8: Plots showing mutual information and negativity obtained from the entanglement harvesting protocol with [PITH_FULL_IMAGE:figures/full_fig_p022_8.png] view at source ↗
Figure 9
Figure 9. Figure 9: Plots showing mutual information obtained from the entanglement harvesting protocol discussed in subsection [PITH_FULL_IMAGE:figures/full_fig_p024_9.png] view at source ↗
Figure 10
Figure 10. Figure 10: The left panel shows the kink trajectory defined in Eq.( [PITH_FULL_IMAGE:figures/full_fig_p025_10.png] view at source ↗
Figure 11
Figure 11. Figure 11: The top panels of the above plots display the negativity obtained by two inertial detectors in front of a [PITH_FULL_IMAGE:figures/full_fig_p026_11.png] view at source ↗
read the original abstract

We construct a smooth trajectory in Minkowski spacetime that is inertial in the asymptotic past and future but undergoes approximately uniform acceleration for a finite duration. In a suitable limit, this trajectory reduces to the standard Rindler trajectory, reproducing the expected Bogoliubov transformations and results consistent with the thermal time hypothesis. We analyze the behavior of an Unruh-DeWitt (UDW) detector following such a trajectory and explore the dependence of complete positivity (CP) divisibility on the detector's frequency, acceleration, and the duration of acceleration. Notably, we find that the detector exhibits a memory effect due to the finite duration of acceleration, which is also quantified by the Fisher information. We further examine two UDW detectors along various trajectory combinations and show that, unlike the transition rate, both the total correlation and the entanglement harvested return smoothly to their initial values after the acceleration/deceleration phase. These correlation measures behave similarly in both accelerating and decelerating segments. Interestingly, we do not observe any measurable effect of the memory effect on negativity or mutual information. We also discuss the physical significance of the sign of the flux of acceleration-induced radiation.

Editorial analysis

A structured set of objections, weighed in public.

Desk editor's note, referee report, simulated authors' rebuttal, and a circularity audit. Tearing a paper down is the easy half of reading it; the pith above is the substance, this is the friction.

Referee Report

2 major / 2 minor

Summary. The manuscript constructs a smooth trajectory in Minkowski spacetime that is inertial in the asymptotic past and future but undergoes approximately uniform acceleration for a finite duration. In a suitable limit this reduces to the standard Rindler trajectory, reproducing expected Bogoliubov transformations. The authors analyze a single Unruh-DeWitt detector along this trajectory, reporting a memory effect due to finite acceleration duration that is quantified by the Fisher information, and examining the dependence of complete positivity divisibility on detector frequency, acceleration parameter, and duration. For two detectors they show that, unlike the transition rate, both total correlation and harvested entanglement return smoothly to their initial values after the acceleration/deceleration phase, with similar behavior in accelerating and decelerating segments; they also discuss the physical significance of the sign of the flux of acceleration-induced radiation.

Significance. If the results are robust to the details of the smoothing procedure, the work provides a controlled setting for studying finite-time Unruh effects and non-Markovian detector dynamics. The contrast between the non-recovery of the transition rate and the smooth recovery of entanglement and total correlation is a potentially useful observation, and the use of Fisher information supplies a concrete quantifier of memory. The explicit reduction to the eternal Rindler case and the exploration of multiple trajectory combinations are strengths that allow direct comparison with known results.

major comments (2)
  1. [Trajectory construction] Trajectory construction section: the central claim that the memory effect and the smooth return of correlations/entanglement are generic features of finite-duration acceleration (rather than artifacts of the chosen smoothing) requires explicit checks that the long-time behavior of the Wightman function integrals is independent of the ramp-up/ramp-down profile. Different smoothing functions should be compared, or an argument given that residual correlations from the matching to asymptotic inertial segments vanish in the relevant limits.
  2. [Two-detector analysis] Two-detector analysis: the statement that total correlation and entanglement return smoothly (unlike the transition rate) must be shown to hold for the full range of trajectory combinations examined; the manuscript should clarify whether this recovery persists when the two detectors follow qualitatively different finite-acceleration profiles.
minor comments (2)
  1. [Abstract] Abstract: the phrase 'we do not observe any measurable effect of the memory effect on negativity or mutual information' should be accompanied by quantitative bounds or a statement of the precision with which these quantities were evaluated.
  2. [Notation and equations] Notation: ensure the acceleration parameter a and the finite duration parameter are introduced with consistent symbols and units in all equations and figures.

Simulated Author's Rebuttal

2 responses · 0 unresolved

We thank the referee for the careful reading of our manuscript and the constructive comments. We address the major points below and will revise the manuscript to incorporate clarifications and additional arguments where appropriate.

read point-by-point responses
  1. Referee: [Trajectory construction] Trajectory construction section: the central claim that the memory effect and the smooth return of correlations/entanglement are generic features of finite-duration acceleration (rather than artifacts of the chosen smoothing) requires explicit checks that the long-time behavior of the Wightman function integrals is independent of the ramp-up/ramp-down profile. Different smoothing functions should be compared, or an argument given that residual correlations from the matching to asymptotic inertial segments vanish in the relevant limits.

    Authors: We agree that strengthening the genericity claim is valuable. In the revised manuscript we will add an analytic argument showing that the long-time asymptotics of the relevant Wightman integrals are controlled by the identical inertial segments at early and late times; the finite-duration acceleration phase contributes only transient terms that decay due to rapid phase oscillations for large time separations. We will also include a short numerical comparison with an alternative smoothing profile (a C^infty bump function) confirming that the Fisher information and the asymptotic values of the correlation measures remain unchanged within numerical precision. revision: yes

  2. Referee: [Two-detector analysis] Two-detector analysis: the statement that total correlation and entanglement return smoothly (unlike the transition rate) must be shown to hold for the full range of trajectory combinations examined; the manuscript should clarify whether this recovery persists when the two detectors follow qualitatively different finite-acceleration profiles.

    Authors: The manuscript already examines several combinations, including symmetric finite-acceleration trajectories, one detector accelerating while the other remains inertial, and trajectories with mismatched durations. The smooth recovery of total correlation and harvested entanglement is observed in all these cases. We will revise the text to state explicitly that the recovery persists for qualitatively different profiles and briefly explain that this follows from the structure of the two-point functions: the correlation measures integrate over the full history in a manner insensitive to the precise ramp details once the detectors return to inertial motion, in contrast to the irreversible excitation captured by the transition rate. revision: yes

Circularity Check

0 steps flagged

No significant circularity; derivation is self-contained

full rationale

The paper defines an explicit smooth trajectory that is inertial at early and late times and approximates uniform acceleration over finite duration, with a controlled limit recovering the standard Rindler case and its Bogoliubov coefficients. All subsequent detector observables (transition rates, Fisher information, total correlations, negativity, mutual information) are obtained from direct integration of the Wightman function along this worldline using the standard Unruh-DeWitt coupling. These quantities are not fitted to data within the paper, nor are they renamed versions of the trajectory definition itself; the memory effect and the smooth return of correlations appear as computed outcomes that can be varied by changing the acceleration duration or profile. No load-bearing self-citation or uniqueness theorem from the same authors is invoked to force the results.

Axiom & Free-Parameter Ledger

2 free parameters · 2 axioms · 0 invented entities

The analysis rests on standard Minkowski quantum field theory and the Unruh-DeWitt detector model without introducing new particles or forces; free parameters are the acceleration magnitude and finite duration, chosen to interpolate between inertial and Rindler regimes.

free parameters (2)
  • finite acceleration duration
    Duration of the approximately uniform acceleration phase is a tunable parameter of the constructed trajectory.
  • acceleration parameter a
    Magnitude of the uniform acceleration during the finite interval.
axioms (2)
  • domain assumption Existence of a smooth trajectory that is asymptotically inertial yet approximates Rindler motion for finite time
    Invoked to reproduce standard Bogoliubov transformations in the appropriate limit.
  • domain assumption Validity of the Unruh-DeWitt detector as a probe of field correlations
    Standard two-level system linearly coupled to a scalar field in Minkowski vacuum.

pith-pipeline@v0.9.0 · 5728 in / 1346 out tokens · 49559 ms · 2026-05-18T23:47:27.705737+00:00 · methodology

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Lean theorems connected to this paper

Citations machine-checked in the Pith Canon. Every link opens the source theorem in the public Lean library.

What do these tags mean?
matches
The paper's claim is directly supported by a theorem in the formal canon.
supports
The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
extends
The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
uses
The paper appears to rely on the theorem as machinery.
contradicts
The paper's claim conflicts with a theorem or certificate in the canon.
unclear
Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.

Reference graph

Works this paper leans on

73 extracted references · 73 canonical work pages

  1. [1]

    Particle creation by black holes

    Stephen William Hawking. Particle creation by black holes. Communications in Mathematical Physics, 43:199–220, 1975

  2. [2]

    W. G. Unruh. Notes on black-hole evaporation. Phys. Rev. D , 14:870–892, Aug 1976

  3. [3]

    Lessons from the information paradox

    Suvrat Raju. Lessons from the information paradox. Phys. Rept., 943:1–80, 2022

  4. [4]

    Jerusalem Lectures on Black Holes and Quantum Information

    Daniel Harlow. Jerusalem Lectures on Black Holes and Quantum Information. Rev. Mod. Phys., 88:015002, 2016

  5. [5]

    Menicucci

    Eduardo Martin-Martinez and Nicolas C. Menicucci. Entanglement in curved spacetimes and cosmology. Class. Quant. Grav., 31(21):214001, 2014

  6. [6]

    Entanglement harvesting from conformal vacuums between two Unruh-DeWitt detectors moving along null paths

    Subhajit Barman, Dipankar Barman, and Bibhas Ranjan Majhi. Entanglement harvesting from conformal vacuums between two Unruh-DeWitt detectors moving along null paths. JHEP, 09:106, 2022

  7. [7]

    Morley, Hendrik Ulbricht, Marko Toroˇ s, Mauro Paternostro, An- drew A

    Sougato Bose, Anupam Mazumdar, Gavin W. Morley, Hendrik Ulbricht, Marko Toroˇ s, Mauro Paternostro, An- drew A. Geraci, Peter F. Barker, M. S. Kim, and Gerard Milburn. Spin entanglement witness for quantum gravity. Phys. Rev. Lett., 119:240401, Dec 2017

  8. [8]

    Marletto and V

    C. Marletto and V. Vedral. Gravitationally induced entanglement between two massive particles is sufficient evidence of quantum effects in gravity. Phys. Rev. Lett., 119:240402, Dec 2017

  9. [9]

    Marshman, Anupam Mazumdar, and Sougato Bose

    Ryan J. Marshman, Anupam Mazumdar, and Sougato Bose. Locality and entanglement in table-top testing of the quantum nature of linearized gravity. Phys. Rev. A , 101:052110, May 2020

  10. [10]

    Mechanism for the quantum natured gravitons to entangle masses

    Sougato Bose, Anupam Mazumdar, Martine Schut, and Marko Toroˇ s. Mechanism for the quantum natured gravitons to entangle masses. Phys. Rev. D , 105:106028, May 2022

  11. [11]

    Newton, entanglement, and the graviton

    Daniel Carney. Newton, entanglement, and the graviton. Phys. Rev. D , 105:024029, Jan 2022

  12. [12]

    Distinguishing jordan and einstein frames in gravity through entanglement

    Sumanta Chakraborty, Anupam Mazumdar, and Ritapriya Pradhan. Distinguishing jordan and einstein frames in gravity through entanglement. Phys. Rev. D , 108:L121505, Dec 2023

  13. [14]

    Entanglement islands, fire walls and state paradox from quantum teleportation and entanglement swapping

    Xuanhua Wang, Kun Zhang, and Jin Wang. Entanglement islands, fire walls and state paradox from quantum teleportation and entanglement swapping. Class. Quant. Grav. , 40(9):095012, 2023

  14. [15]

    Parvizi and M

    S. Parvizi and M. Shahbazi. Analogue gravity and the island prescription. European Physical Journal C , 83:705, 2023

  15. [16]

    Ken K. W. Ma and Kun Yang. Simple analog of the black-hole information paradox in quantum hall interfaces. Phys. Rev. B , 105:045306, Jan 2022

  16. [17]

    Braunstein, Mir Faizal, Lawrence M

    Samuel L. Braunstein, Mir Faizal, Lawrence M. Krauss, Francesco Marino, and Naveed A. Shah. Analogue simula- tions of quantum gravity with fluids. Nature Rev. Phys., 5(10):612–622, 2023. 32

  17. [18]

    K. S. Kumar and J. Marto. Revisiting quantum field theory in rindler spacetime with superselection rules. Universe, 10:320, 2024

  18. [19]

    Generalized unruh effect: A potential resolution to the black hole information paradox

    Angela Chen. Generalized unruh effect: A potential resolution to the black hole information paradox. Phys. Rev. D, 107:056014, Mar 2023

  19. [20]

    Entanglement of the vacuum between left, right, future, and past: The origin of entanglement-induced quantum radiation

    Atsushi Higuchi, Satoshi Iso, Kazushige Ueda, and Kazuhiro Yamamoto. Entanglement of the vacuum between left, right, future, and past: The origin of entanglement-induced quantum radiation. Phys. Rev. D, 96:083531, Oct 2017

  20. [21]

    Spatio-temporal entanglement of the vacuum

    Pravin Kumar Dahal and Kieran Hymas. Spatio-temporal entanglement of the vacuum. 4 2025

  21. [22]

    Aps medal for exceptional achievement in research: Invited article on entanglement properties of quantum field theory

    Edward Witten. Aps medal for exceptional achievement in research: Invited article on entanglement properties of quantum field theory. Rev. Mod. Phys., 90:045003, Oct 2018

  22. [23]

    Summers and Reinhard Werner

    Stephen J. Summers and Reinhard Werner. Maximal violation of bell’s inequalities for algebras of observables in tangent spacetime regions. Annales de l’I.H.P. Physique th´ eorique, 49(2):215–243, 1988

  23. [24]

    Peter D. Hislop. Conformal covariance, modular structure, and duality for local algebras in free massless quantum field theories. Annals of Physics , 185(2):193–230, 1988

  24. [25]

    Entanglement from the vacuum

    Benni Reznik. Entanglement from the vacuum. Found. Phys., 33:167–176, 2003

  25. [26]

    Unruh effect and information flow

    Boris Sokolov, Jorma Louko, Sabrina Maniscalco, and Iiro Vilja. Unruh effect and information flow. Phys. Rev. D , 101:024047, Jan 2020

  26. [27]

    Entanglement harvesting for different gravitational wave burst profiles with and without memory

    Subhajit Barman, Indranil Chakraborty, and Sajal Mukherjee. Entanglement harvesting for different gravitational wave burst profiles with and without memory. JHEP, 09:180, 2023

  27. [28]

    Information backflow as a resource for entanglement.Phys

    Nicol´ as Mirkin, Pablo Poggi, and Diego Wisniacki. Information backflow as a resource for entanglement.Phys. Rev. A, 99:062327, Jun 2019

  28. [29]

    C. H. Fleming, N. I. Cummings, Charis Anastopoulos, and B. L. Hu. Non-Markovian dynamics and entanglement of two-level atoms in a common field. Journal of Physics A Mathematical General , 45(6):065301, February 2012

  29. [30]

    Huelga, ´Angel Rivas, and Martin B

    Susana F. Huelga, ´Angel Rivas, and Martin B. Plenio. Non-markovianity-assisted steady state entanglement. Phys. Rev. Lett., 108:160402, Apr 2012

  30. [31]

    Non-Markovianity and entanglement detection

    Sourav Chanduka, Bihalan Bhattacharya, Rounak Mundra, Samyadeb Bhattacharya, and Indranil Chakrabarty. Non-Markovianity and entanglement detection. Int. J. Quant. Inf. , 21(05):2350025, 2023

  31. [32]

    Huelga, and Martin B

    ´Angel Rivas, Susana F. Huelga, and Martin B. Plenio. Entanglement and non-markovianity of quantum evolutions. Phys. Rev. Lett., 105:050403, Jul 2010

  32. [33]

    Levenson-Falk, and Kater W

    Chandrashekhar Gaikwad, Daria Kowsari, Carson Brame, Xingrui Song, Haimeng Zhang, Martina Esposito, Arpit Ranadive, Giulio Cappelli, Nicolas Roch, Eli M. Levenson-Falk, and Kater W. Murch. Entanglement assisted probe of the non-markovian to markovian transition in open quantum system dynamics. Phys. Rev. Lett. , 132:200401, May 2024

  33. [34]

    Detlev Buchholz, Olaf Dreyer, Martin Florig, and Stephen J. Summers. Geometric modular action and space-time symmetry groups. Rev. Math. Phys. , 12:475–560, 2000. 33

  34. [35]

    Black Holes as Conformal Field Theories on Horizons

    Edi Halyo. Black Holes as Conformal Field Theories on Horizons. 2 2015

  35. [36]

    Asorey, A

    M. Asorey, A. P. Balachandran, G. Marmo, and A. R. de Queiroz. Localization of observables in the rindler wedge. Phys. Rev. D , 96:105001, Nov 2017

  36. [37]

    Candelas and J

    P. Candelas and J. S. Dowker. Field theories on conformally related space-times: Some global considerations. Phys. Rev. D, 19:2902–2907, May 1979

  37. [38]

    Padmanabhan

    T. Padmanabhan. Gravity and Quantum Theory: Domains of Conflict and Contact. Int. J. Mod. Phys. D , 29(01):2030001, 2019

  38. [39]

    Ahn and M.S

    D. Ahn and M.S. Kim. Hawking–unruh effect and the entanglement of two-mode squeezed states in riemannian space–time. Physics Letters A , 366(3):202–205, 2007

  39. [40]

    Quantum Fisher information as a probe for Unruh thermality

    Jun Feng and Jing-Jun Zhang. Quantum Fisher information as a probe for Unruh thermality. Phys. Lett. B , 827:136992, 2022

  40. [41]

    Everett Patterson and Robert B. Mann. Fisher information of a black hole spacetime. JHEP, 06:214, 2023

  41. [42]

    Does anti-Unruh effect assist quantum entanglement and coherence? New J

    Shu-Min Wu, Xiao-Wei Teng, Jin-Xuan Li, Hao-Sheng Zeng, and Tonghua Liu. Does anti-Unruh effect assist quantum entanglement and coherence? New J. Phys. , 26(4):043016, 2024

  42. [43]

    Diamonds’s temperature: Unruh effect for bounded trajectories and thermal time hypothesis

    Pierre Martinetti and Carlo Rovelli. Diamonds’s temperature: Unruh effect for bounded trajectories and thermal time hypothesis. Class. Quant. Grav. , 20:4919–4932, 2003

  43. [44]

    Gravitation: Foundations and frontiers

    Thanu Padmanabhan. Gravitation: Foundations and frontiers . Cambridge University Press, 12 2014

  44. [45]

    Sriramkumar and T

    L. Sriramkumar and T. Padmanabhan. Probes of the vacuum structure of quantum fields in classical backgrounds. Int. J. Mod. Phys. D , 11:1–34, 2002

  45. [46]

    N. D. Birrell and P. C. W. Davies. Frontmatter, page i–iv. Cambridge Monographs on Mathematical Physics. Cambridge University Press, 1982

  46. [47]

    Vacuum noise and stress induced by uniform acceleration: Hawking-unruh effect in rindler manifold of arbitrary dimension

    Shin Takagi. Vacuum noise and stress induced by uniform acceleration: Hawking-unruh effect in rindler manifold of arbitrary dimension. Progress of Theoretical Physics Supplement, 88:1–142, 03 1986

  47. [48]

    Dubey and Sanved Kolekar

    Nitesh K. Dubey and Sanved Kolekar. Wigner distributions in rindler spacetime and nonvacuum minkowski states. Phys. Rev. D , 111:065004, Mar 2025

  48. [49]

    How often does the Unruh-DeWitt detector click? Regularisation by a spatial profile

    Jorma Louko and Alejandro Satz. How often does the Unruh-DeWitt detector click? Regularisation by a spatial profile. Class. Quant. Grav. , 23:6321–6344, 2006

  49. [50]

    Measure for the degree of non-markovian behavior of quantum processes in open systems

    Heinz-Peter Breuer, Elsi-Mari Laine, and Jyrki Piilo. Measure for the degree of non-markovian behavior of quantum processes in open systems. Phys. Rev. Lett., 103:210401, Nov 2009

  50. [51]

    Entropic and trace-distance-based measures of non- Markovianity

    Federico Settimo, Heinz-Peter Breuer, and Bassano Vacchini. Entropic and trace-distance-based measures of non- Markovianity. Phys. Rev. A , 106(4):042212, 2022

  51. [52]

    S. C. Hou, X. X. Yi, S. X. Yu, and C. H. Oh. Alternative non-markovianity measure by divisibility of dynamical maps. Phys. Rev. A , 83:062115, Jun 2011. 34

  52. [53]

    Quantifying non-markovianity via correlations

    Shunlong Luo, Shuangshuang Fu, and Hongting Song. Quantifying non-markovianity via correlations. Phys. Rev. A, 86:044101, Oct 2012

  53. [54]

    Complete positivity, finite-temperature effects, and additivity of noise for time-local qubit dynamics

    Juho Lankinen, Henri Lyyra, Boris Sokolov, Jose Teittinen, Babak Ziaei, and Sabrina Maniscalco. Complete positivity, finite-temperature effects, and additivity of noise for time-local qubit dynamics. Phys. Rev. A, 93:052103, May 2016

  54. [55]

    Barbado and Matt Visser

    Luis C. Barbado and Matt Visser. Unruh-DeWitt detector event rate for trajectories with time-dependent acceler- ation. Phys. Rev. D , 86:084011, 2012

  55. [56]

    Then again, how often does the Unruh-DeWitt detector click if we switch it carefully? Class

    Alejandro Satz. Then again, how often does the Unruh-DeWitt detector click if we switch it carefully? Class. Quant. Grav., 24:1719–1732, 2007

  56. [57]

    Transition rate of the Unruh-DeWitt detector in curved spacetime

    Jorma Louko and Alejandro Satz. Transition rate of the Unruh-DeWitt detector in curved spacetime. Class. Quant. Grav., 25:055012, 2008

  57. [58]

    Connecting Fisher information to bulk entanglement in holography

    Souvik Banerjee, Johanna Erdmenger, and Debajyoti Sarkar. Connecting Fisher information to bulk entanglement in holography. JHEP, 08:001, 2018

  58. [59]

    The information of the information paradox: On the quantum information meaning of Page curve

    Cesar Gomez. The information of the information paradox: On the quantum information meaning of Page curve. unpublished, 7 2020

  59. [60]

    Roy Frieden

    B. Roy Frieden. Physics from Fisher Information: A Unification . Cambridge University Press, 1998

  60. [61]

    Does relativistic motion always degrade quantum Fisher information? Phys

    Xiaobao Liu, Jiliang Jing, Zehua Tian, and Weiping Yao. Does relativistic motion always degrade quantum Fisher information? Phys. Rev. D , 103(12):125025, 2021

  61. [62]

    Xiao-Ming Lu, Xiaoguang Wang, and C. P. Sun. Quantum fisher information flow and non-markovian processes of open systems. Phys. Rev. A , 82:042103, Oct 2010

  62. [63]

    Relative entropy of states of von neumann algebras

    Huzihiro Araki. Relative entropy of states of von neumann algebras. Publ. Res. Inst. Math. Sci. , 11(3):809–833, 1975

  63. [64]

    When entanglement harvesting is not really harvesting

    Erickson Tjoa and Eduardo Mart´ ın-Mart´ ınez. When entanglement harvesting is not really harvesting. Phys. Rev. D, 104:125005, Dec 2021

  64. [65]

    Kensuke Gallock-Yoshimura, Erickson Tjoa, and Robert B. Mann. Harvesting entanglement with detectors freely falling into a black hole. Phys. Rev. D , 104:025001, Jul 2021

  65. [66]

    Harvesting correlations from the quantum vacuum

    Alejandro Pozas-Kerstjens and Eduardo Martin-Martinez. Harvesting correlations from the quantum vacuum. Phys. Rev. D, 92(6):064042, 2015

  66. [67]

    Erickson Tjoa and Robert B. Mann. Harvesting correlations in Schwarzschild and collapsing shell spacetimes. JHEP, 08:155, 2020

  67. [68]

    Quantum correlations through event horizons: Fermionic versus bosonic entanglement

    Eduardo Mart´ ın-Mart´ ınez and Juan Le´ on. Quantum correlations through event horizons: Fermionic versus bosonic entanglement. Phys. Rev. A , 81:032320, Mar 2010

  68. [69]

    Shor, and Mary Beth Ruskai

    Michael Horodecki, Peter W. Shor, and Mary Beth Ruskai. Entanglement Breaking Channels. Reviews in Mathe- matical Physics, 15(6):629–641, January 2003. 35

  69. [70]

    Vieira, Huan-Yu Ku, and Costantino Budroni

    Lucas B. Vieira, Huan-Yu Ku, and Costantino Budroni. Entanglement-breaking channels are a quantum memory resource. unpublished, 2 2024

  70. [71]

    Holographic moving mirrors

    Ibrahim Akal, Yuya Kusuki, Noburo Shiba, Tadashi Takayanagi, and Zixia Wei. Holographic moving mirrors. Class. Quant. Grav., 38(22):224001, 2021

  71. [72]

    Entanglement Entropy in a Holographic Moving Mirror and the Page Curve

    Ibrahim Akal, Yuya Kusuki, Noburo Shiba, Tadashi Takayanagi, and Zixia Wei. Entanglement Entropy in a Holographic Moving Mirror and the Page Curve. Phys. Rev. Lett., 126(6):061604, 2021

  72. [73]

    Wan Cong, Erickson Tjoa, and Robert B. Mann. Entanglement Harvesting with Moving Mirrors. JHEP, 06:021,

  73. [74]

    [Erratum: JHEP 07, 051 (2019)]. 36