REVIEW 5 major objections 5 minor 1 cited by
Open Quantum Entanglement: A study of two atomic system in static patch of de Sitter space
T0 review · 5 major / 5 minor · reviewed 2026-08-14 · deepseek-v4-flash
Pith's one-line read This paper claims that two atoms in the static patch of de Sitter space, coupled to a massless scalar bath, develop late-time entanglement and violate the Bell-CHSH inequality.
desk verdict The 'simplifying' condition coth(πkω0)=0 makes the GKSL generator non-positive and the late-time equilibrium singular, so the central solution is not valid; this is a desk reject. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The load-bearing object is the GSKL master equation for the reduced two-atom density matrix, $\frac{d}{d\tau}\rho_{\rm System}=-i[H_{\rm eff},\rho_{\rm System}]+\mathcal{L}[\rho_{\rm System}]$, built from two components: an effective Lamb-shift Hamiltonian that takes the form of a Heisenberg spin chain, and a Lindbladian dissipator whose coefficient matrix $C^{\alpha\beta}_{ij}$ is fixed by the Wightman functions of a massless conformally coupled scalar in the static de Sitter patch. Those Wightman functions are Fourier- and Hilbert-transformed to produce the Hamiltonian and GSKL coefficient matrices; the equations are simplified by changing basis from $\{\sigma_1,\sigma_2,\sigma_3\}$ to $\{\sigma_+,\sigma_-,\sigma_3\}$; and the late-time equilibrium density matrix $\rho_{\rm System}(\infty)=e^{-\beta H_{\rm System}}/\mathrm{Tr}(e^{-\beta H_{\rm System}})$ supplies the boundary conditions. This machinery converts a large coupled set of Bloch-vector equations into an analytically solvable linear system whose three decay rates $f_1(\omega),f_2(\omega),f_3(\omega)$ control the approach to equilibrium.
What would settle it
Compute the eigenvalues of the GSKL coefficient matrix $C^{\alpha\beta}_{ij}$ with the adopted values $C_{++}=C_{--}=0$, $C_{-+}=-C_{+-}=\pm i\tilde B$; the matrix has the form $\begin{pmatrix}0&i\tilde B\\-i\tilde B&0\end{pmatrix}$, so its eigenvalues are $\pm|\tilde B|$, which means the generator is not completely positive. Equivalently, evolve the paper's Bloch-vector solution at an intermediate time and check whether the reduced density matrix remains positive semidefinite; a negative eigenvalue at any time would directly falsify the claim that this is a valid open-quantum-system evolution.
Extended reading notes
Core claim
The paper's central claim is that the reduced state of two atoms in the static patch of de Sitter space, evolved under the GSKL master equation with both the effective Lamb-shift Hamiltonian and the Lindbladian, has a late-time equilibrium form with Bloch-vector components $a_{03}(\infty)=a_{30}(\infty)=-\tanh(\pi k\omega)$, $a_{33}(\infty)=\tanh^2(\pi k\omega)$, and vanishing off-diagonal components. From that density matrix the paper derives Von Neumann entropy, Renyi entropy, logarithmic negativity, concurrence, entanglement of formation, and quantum discord, each increasing from zero and saturating at late time. It then shows that after passing the two detectors through local filters, the filtered correlation matrix satisfies $c'(c')^\dagger>1$, equivalently $(a_{+-}+|a_{--}|)^4>(1-a_{33})^2[(1+a_{33})^2-(a_{03}+a_{30})^2]$ in its notation, which the paper takes as the criterion for Bell-CHSH violation. The conclusion is that nonlocality is a generic feature of two-body correlation in de Sitter space, not a special property of a particular matter model.
Load-bearing premise
The paper's results stand on the condition $\coth(\pi k\omega_0)=0$, imposed purely to simplify the GSKL matrix, which forces the atomic frequency to be imaginary, $\omega_0=i(n+1/2)/k$, and makes the late-time equilibrium solution rely on $\tanh(\pi k\omega)$ at a singular value; if that simplification is removed, the analytical solution and all derived entanglement measures may collapse.
Editorial extensions
If this is right
- If the solution is correct, every computed entanglement measure rises from zero and saturates at late times, so de Sitter curvature acts as a persistent source of two-body quantum correlation rather than a transient effect.
- The equilibrium temperature extracted by matching the late-time density matrix to a Gibbs state is $T=1/(2\pi k)=\sqrt{T_{\rm GH}^2+T_{\rm Unruh}^2}$, directly tying the generated entanglement to horizon temperature and curvature.
- Bell-CHSH violation is obtained without invoking an axion or any specific nonlocal model, so the paper claims static-patch de Sitter spacetime is by itself sufficient for nonlocality.
- In the flat-space limit $k\to\infty$ the entanglement measures drop toward zero, while in the zero-acceleration limit $r\to0$ the bath temperature reduces to the Gibbons-Hawking temperature, indicating that curvature and observer acceleration drive the effect.
- The single-atom reduced state remains unentangled while the two-atom state is entangled, so the correlation is genuinely between the two atoms and not merely an artifact of each atom's interaction with the bath.
Reading between the lines
- Editorial inference: the simplification $\coth(\pi k\omega_0)=0$ forces the atomic frequency to be purely imaginary, $\omega_0=i(n+1/2)/k$, and with that choice the GSKL coefficient matrix has vanishing diagonal entries and off-diagonal entries $\pm i\tilde B$, so it is not positive semidefinite; a direct check would show whether the master equation is completely positive or whether the evolved de
- Editorial extension: repeat the derivation with real $\omega_0$ while keeping the full $\coth(\pi k\omega_0)$ factors; if the saturation and Bell-CHSH violation persist for physical frequencies the result is robust, and if they vanish the curvature-generated nonlocality claim is an artifact of the simplification.
- Editorial connection: in the inflationary (planar) patch of de Sitter, the same kind of imaginary-frequency structure is expected from conformal time dependence, so this calculation could be translated into a comparison with standard cosmological correlation functions.
- Editorial note: the Bell test here is performed after local filtering and uses the necessary condition $cc^\dagger>1$; an independent check of the raw Bell-CHSH expectation value against the bound $|\langle B_{\rm CHSH}\rangle|\le2$ would clarify whether the filtered criterion coincides with genuine Bell violation.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript studies two two-level atoms as an open quantum system in the static patch of de Sitter space, with the bath modeled by a massless conformally coupled scalar field. The authors compute the relevant Wightman functions, construct an effective Hamiltonian and a GKSL dissipator, and then solve the master equation for the Bloch-vector components under the condition coth(πkω0)=0. Using that solution, they evaluate von Neumann entropy, Rényi entropy, logarithmic negativity, concurrence, entanglement of formation, quantum discord, and Bell-CHSH violation, concluding that late-time entanglement saturates and that the Bell-CHSH inequality is violated in de Sitter space.
Significance. If the derivation were valid, the paper would provide a relatively model-independent demonstration that de Sitter curvature generates long-range quantum correlations in a two-atomic open quantum system. The manuscript contains substantial analytic work, including explicit Wightman functions, Hilbert-transform integrals, and a finite-time solution of the master equation, and it surveys several entanglement monotones. However, the central derivation depends on an ad hoc imaginary-frequency condition that makes the GKSL matrix non-positive and the late-time equilibrium singular. As written, the master equation is not completely positive and the resulting density matrix is not guaranteed to be a valid quantum state; consequently the entanglement measures and Bell-CHSH analysis built on it do not establish the paper's claims.
major comments (5)
- [§2, Eqs. (2.6)–(2.7); Appendix B] The condition coth(πkω0)=0 is imposed solely 'to simplify the mathematical form of GSKL matrix' and forces ω0=i(n+1/2)/k. This makes the atomic Hamiltonian in Eq. (2.2) non-Hermitian, since the level splitting is imaginary. All subsequent results—the coefficients in Appendix B, the integrals in Appendix D, and the finite-time solution in Section 6—are computed under this assumption. The sub-horizon remark in Appendix B does not justify an imaginary energy gap for a two-level atom. This is a load-bearing ad hoc assumption, not a derived or controlled limit, and it undermines the physical interpretation of the entire model.
- [§3, §5, and Appendix B, Eqs. (3.4), (5.3), (B.10)–(B.14)] With the imaginary-frequency condition, the GKSL coefficient matrix has diagonal entries A=0 and off-diagonal entries C_{+-}=-iB and C_{-+}=iB, with B=-µ²/(8πk)(n+1/2). For B≠0 this matrix is neither Hermitian nor positive semidefinite; its eigenvalues are ±B. Hence the generator in Eq. (3.4) is not a Lindblad generator and does not define a completely positive dynamical semigroup. The reduced density matrix obtained from this master equation therefore need not be a valid quantum state, and every entanglement measure and the Bell-CHSH analysis built on it lack a valid foundation.
- [§6.1, Eqs. (6.10)–(6.14)] The late-time fixed point is written in terms of tanh(πkω). At the half-integer imaginary values selected in Eq. (2.6), namely πkω=iπ(n+1/2), tanh has a pole, so the equilibrium density matrix in Eq. (6.12) is singular rather than a thermal state. If the renormalized frequency ω is intended to avoid these poles, the text must demonstrate this explicitly, since Eq. (2.5) defines ω through a complex Lamb-shift correction whose imaginary part is not computed. As written, the boundary conditions used to fix the constants g_i in Section 6.2 are not well-defined, and the temperature identification T=1/(2πk) in Eq. (6.14) is not justified.
- [§7.1, §7.5, and §9] The paper treats the von Neumann entropy of the reduced two-atom state and the quantum discord as entanglement witnesses and concludes in Section 9 that nonzero values of both imply quantum entanglement. This is incorrect: both quantities are positive for many separable mixed states, and discord measures nonclassical correlations rather than entanglement. The claim that these measures establish entanglement should be removed or replaced by statements about total correlations. The valid entanglement measures used elsewhere, namely logarithmic negativity and concurrence, should be the basis for any entanglement claim.
- [§8, Eqs. (8.12)–(8.13), Fig. 18] The Bell-CHSH violation is presented by plotting J1(t) and J2(t), but the text does not specify the initial state, parameter values, or normalization used in Fig. 18, and no explicit measurement directions (a,b,a',b') are provided. The eigenvalue criterion can establish violation in principle, but only if the eigenvalues of c'(c')† are correctly computed for the actual density matrix; the derivation in Steps 2–4 contains unexplained inequalities, and the plots compare normalized functions rather than the raw criterion. As it stands, the claim that the inequality is 'always satisfied' is not supported by the presented evidence.
minor comments (5)
- [Appendix D, Eqs. (D.6), (D.8), (D.14)] The labels for the integrals appear to be swapped: the text in Section D.1 refers to 'Integral I' as Θ2, while Section D.2 refers to 'Integral II' as Θ1. This makes the appendix difficult to follow.
- [§7.4, Eq. (7.27)] The expression for the entanglement of formation appears garbled: it does not match the standard formula h((1+√(1−C²))/2) and seems to contain sign errors. If this expression was used in the plots, the results for entanglement of formation should be recomputed.
- [§7.3, Eq. (7.13)] The logarithmic negativity expression contains an unexplained numerical factor 17/100 and mixes notations in a way that makes the formula difficult to verify; the authors should display the fully simplified eigenvalues and the trace norm explicitly.
- [Figures 3–18] The plots are not reproducible as presented: the parameter values, initial states, and normalization conventions are stated only vaguely in the captions, and several plots lack clear legends or axis labels. The authors should specify all parameters used in each figure.
- [Throughout] The acronym is written as GSKL in most places but GKSL in others; the standard ordering is GKSL (Gorini–Kossakowski–Sudarshan–Lindblad), and this should be made consistent.
Circularity Check
No significant circularity: the two-atom GKSL solution and the entanglement measures are computed from the model's Wightman functions rather than being fed back as inputs.
full rationale
The derivation chain is self-contained: the two-body Wightman functions (App. A), their Fourier/Hilbert transforms (Eqs. 4.13-4.15), the GSKL and effective-Hamiltonian coefficient matrices (Apps. B and C), the master equation (Eq. 3.4), and the finite-time Bloch-vector solutions (Eqs. 6.34-6.40) are algebraic consequences of the stated model. The entanglement measures (Eqs. 7.3, 7.6, 7.13, 7.26, 7.39) and the Bell-CHSH comparison functions (Eqs. 8.12-8.13) are evaluated from these Bloch coefficients, so the outputs are not equal to the inputs by definition. The equilibrium temperature T=1/(2πk) is extracted by comparing the solved late-time state with a Gibbs-ensemble form (Eqs. 6.12-6.14); this is a parameter identification or consistency check, not a fit to data that is later renamed as a prediction. The relation T=sqrt(T_GH^2+T_Unruh^2) is attributed to the same authors' earlier ref. [28], but the present paper already obtains 1/(2πk) directly, so the self-citation is not load-bearing. The imposed condition coth(πk omega0)=0 and the use of the large-time equilibrium as boundary data are genuine physical-correctness risks — the resulting Lindblad matrix may fail to be completely positive and tanh(πk omega) can become singular if pi k omega is a half-integer multiple of iπ — but those are validity concerns about an assumption, not circular reduction of the claimed results to their inputs. No step can be exhibited in which the paper derives X from Y while X was already used to define Y.
Assumptions & free parameters
free parameters (3)
- imaginary frequency condition coth(πkω0)=0 =
ω0 = i(n+1/2)/k for integer n
- coupling strength μ
- local filter parameter η =
real parameter in Eq. (8.8)
assumptions (5)
- domain assumption Born, Markov, and secular approximations hold for the two-atom system in de Sitter space.
- ad hoc to paper The bath scalar field is massless and conformally coupled.
- ad hoc to paper coth(πkω0)=0 with ω0 imaginary.
- domain assumption The large-time reduced density matrix is a thermal Gibbs state ρ=e^{-βH}/Z.
- ad hoc to paper 2πkω >> 1 and ωc << ω0 limits used to evaluate integrals.
Cite this review
Pith. "Pith review of Open Quantum Entanglement: A study of two atomic system in static patch of de Sitter space." pith.science (2026). https://pith.science/paper/B45BTDJS
@misc{pith2026190809929,
author = {Pith},
title = {Pith review of: Open Quantum Entanglement: A study of two atomic system in static patch of de Sitter space},
year = {2026},
howpublished = {\url{https://pith.science/paper/B45BTDJS}},
note = {Machine review of arXiv:1908.09929}
}
abstract
In this work, our prime objective is to study non-locality and long-range effects of two-body correlation using quantum entanglement from the various information-theoretic measures in the static patch of de Sitter space using a two-body Open Quantum System (OQS). The OQS is described by a system of two entangled atoms, surrounded by a thermal bath, which is modelled by a massless probe scalar field. Firstly, we partially trace over the bath field and construct the Gorini Kossakowski Sudarshan Lindblad (GSKL) master equation, which describes the time evolution of the reduced subsystem density matrix. This GSKL master equation is characterized by two components, these are-Spin chain interaction Hamiltonian and the Lindbladian. To fix the form of both of them, we compute the Wightman functions for probe massless scalar field. Using this result along with the large time equilibrium behaviour we obtain the analytical solution for reduced density matrix. Further using this solution we evaluate various entanglement measures, namely Von-Neumann entropy, R$e'$nyi entropy, logarithmic negativity, entanglement of formation, concurrence and quantum discord for the two atomic subsystems on the static patch of De-Sitter space. Finally, we have studied the violation of Bell-CHSH inequality, which is the key ingredient to study non-locality in primordial cosmology.
Forward citations
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-
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Reference graph
Works this paper leans on
-
[1]
Lecture Notes on the Theory of Open Quantum Systems,
Daniel A. Lidar “Lecture Notes on the Theory of Open Quantum Systems,” arXiv:1902.00967
arXiv 1902
-
[2]
S. Choudhury, “The Cosmological OTOC: Formulating new cosmological micro-canonical correlation functions for random chaotic fluctuations in Out-of-Equilibrium Quantum Statistical Field Theory,” [arXiv:2005.11750 [hep-th]]
work page Pith review arXiv 2005
-
[3]
K. Y. Bhagat, B. Bose, S. Choudhury, S. Chowdhury, R. N. Das, S. G. Dastider, N. Gupta, A. Maji, G. D. Pasquino and S. Paul, “The Generalized OTOC from Supersymmetric Quantum Mechanics: Study of Random Fluctuations from Eigenstate Representation of Correlation Functions,” [arXiv:2008.03280 [hep-th]]
work page Pith review arXiv 2008
-
[4]
Subhashish Banerjee, V. Ravishankar and R. Srikanth, ”Dynamics of entanglement in two-qubit open quantum system interacting with a squeezed thermal bath via dissipative interaction,” Ann. of Phys. (NY).: 325, 816 (2010), eprint:arXiv:0901.0404
work page Pith review arXiv 2010
-
[5]
R. Horodecki, P. Horodecki, M. Horodecki and K. Horodecki “Quantum entanglement” Rev. Mod. Phys. 81 (2009) 865 [quant-ph/0702225]
arXiv 2009
-
[6]
Teleporting an unknown quantum state via dual classical and Einstein-Podolsky-Rosen channels,
C. H. Bennett, G. Brassard, C. Crepeau, R. Jozsa, A. Peres and W. K. Wootters, “Teleporting an unknown quantum state via dual classical and Einstein-Podolsky-Rosen channels,” Phys. Rev. Lett. 70 (1993) 1895. – 48 –
work page 1993
-
[7]
Quantification of Entanglement of Teleportation in Arbitrary Dimensions
Sk Sazim, S. Adhikari, Subhashish Banerjee and T. Pramanik, ”Quantification of Entanglement of Teleportation in Arbitrary Dimensions,” Quantum Information Processing13, 863 (2014), arXiv:1208.4200
work page Pith review arXiv 2014
-
[8]
Quantum Error Correction for Beginners
Simon J. Devitt, Kae Nemoto, William J. Munro “Quantum Error Correction for Beginners” Rep. Prog. Phys. 76 (2013) 076001,
work page 2013
Show all 66 references
-
[9]
Omkar, R
S. Omkar, R. Srikanth and Subhashish Banerjee, ”Characterization of quantum dynamics using quantum error correction,” Phys. Rev. A 91, 012324 (2015), Eprint:arXiv:1405.0964
2015 arXiv
-
[10]
Entanglement, Nonlinear Dynamics, and the Heisenberg Limit,
L. Pezze and A. Smerzi “Entanglement, Nonlinear Dynamics, and the Heisenberg Limit,” Phys. Rev. Lett. 102 (2009) 100401
2009
-
[11]
Introduction to Computational Chemistry
Frank Jensen “ Introduction to Computational Chemistry. ” Wiley, 2007,
2007
-
[12]
Quantum entanglement in photosynthetic light harvesting complexes
Mohan Sarovar, Akihito Ishizaki, Graham R. Fleming, K. Birgitta Whaley “ Quantum entanglement in photosynthetic light harvesting complexes” arXiv:0905.3787
-
[13]
Entanglement between living bacteria and quantized light witnessed by Rabi splitting
C Marletto and D M Coles and T Farrow and V Vedral “Entanglement between living bacteria and quantized light witnessed by Rabi splitting” Journal of Physics Communications
-
[14]
M. A. Nielsen and I. L. Chuang , ”Quantum Computation and Quantum Information”, Cambridge University Press, Cambridge (2000)
2000
-
[15]
Dynamics of quantum entanglement in de Sitter spacetime and thermal Minkowski spacetime,
Z. Huang and Z. Tian, “Dynamics of quantum entanglement in de Sitter spacetime and thermal Minkowski spacetime,” Nucl. Phys. B 923 (2017) 458
2017
-
[16]
Detecting the Curvature of de Sitter Universe with Two Entangled Atoms,
Z. Tian, J. Wang, J. Jing and A. Dragan , “Detecting the Curvature of de Sitter Universe with Two Entangled Atoms,” Sci. Rep. 6, 35222 (2016) [arXiv:1605.07350 [quant-ph]]
2016 arXiv
-
[17]
Entanglement dynamics for uniformly accelerated two-level atoms,
J. Hu and H. Yu , “Entanglement dynamics for uniformly accelerated two-level atoms,” Phys. Rev. A 91, no. 1, 012327 (2015) [arXiv:1501.03321 [quant-ph]]
2015 arXiv
-
[18]
Open quantum system approach to Gibbons-Hawking effect of de Sitter space-time,
H. Yu, “Open quantum system approach to Gibbons-Hawking effect of de Sitter space-time,” Phys. Rev. Lett. 106 (2011) 061101 [arXiv:1101.5235 [gr-qc]]
2011 arXiv
-
[19]
Lindblad, ”On the Generators of Quantum Dynamical Semigroups”, Commun
G. Lindblad, ”On the Generators of Quantum Dynamical Semigroups”, Commun. Math. Phys. 48 (1976) 119
1976
-
[20]
Gorini, A
V. Gorini, A. Kossakowski and E. C. G. Sudarshan , ”Completely Positive Dynamical Semigroups of N Level Systems”, J. Math. Phys. 17 (1976) 821
1976
-
[21]
Ingemar Bengtsson, Karol yczkowski , ” Geometry of Quantum States: An Introduction to Quantum Entanglement”, Cambridge University Press
-
[22]
Petr Jizba, Toshihico Arimitsu , ”On observability of Renyi’s entropy”, arXiv:cond-mat/0307698
-
[23]
M. B. Plenio , ”Logarithmic Negativity: A Full Entanglement Monotone That is not Convex”, Phys. Rev. Lett. 95 (2005) no.9, 090503 [quant-ph/0505071]
2005 arXiv
-
[24]
Wootters , ”Entanglement of formation and concurrence”, Journal Quantum Information & Computation
William K. Wootters , ”Entanglement of formation and concurrence”, Journal Quantum Information & Computation
-
[25]
Entanglement of formation of an arbitrary state of two qubits,
W. K. Wootters, “Entanglement of formation of an arbitrary state of two qubits,” Phys. Rev. Lett. 80 (1998) 2245
1998
-
[26]
Shunlong Luo and Shuangshuang Fu , ”Geometric measure of quantum discord”, Phys. Rev. A 82, 034302
-
[27]
Kukita and Y
S. Kukita and Y. Nambu , ”Entanglement dynamics in de Sitter spacetime”, Quant. Grav. 34 (2017) no.23, 235010 [arXiv:1706.09175 [gr-qc]]
2017 arXiv
-
[28]
Relating the curvature of de Sitter Universe to Open Quantum Lamb Shift Spectroscopy,
H. Bohra, S. Choudhury, P. Chauhan, A. Mukherjee, P. Narayan, S. Panda and A. Swain, “Relating the curvature of de Sitter Universe to Open Quantum Lamb Shift Spectroscopy,” arXiv:1905.07403 [physics.gen-ph]
1905 arXiv
-
[29]
Birrell and P
N. Birrell and P. Davies, ”Quantum Fields in Curved Space,” – 49 –
-
[30]
Consequences of field quantization in de Sitter type cosmological models,
E. Tagirov, “Consequences of field quantization in de Sitter type cosmological models,” Annals Phys. 76, 561-579 (1973)
1973
-
[31]
S., Davies P
Bunch T. S., Davies P. C. W. and Penrose Roger Quantum field theory in de Sitter space: Proc. R. Soc. Lond. A360117134
-
[32]
Quantum instability of de Sitter spacetime
Ford LH. Quantum instability of de Sitter spacetime. Phys Rev D Part Fields. 1985;31(4):710-717
1985
-
[33]
Particle Creation in de Sitter Space,
E. Mottola, “Particle Creation in de Sitter Space,” Phys. Rev. D 31, 754 (1985)
1985
-
[34]
The Scalar Wave Equation on Static de Sitter and Anti-de Sitter Spaces,
D. Polarski, “The Scalar Wave Equation on Static de Sitter and Anti-de Sitter Spaces,” Class. Quant. Grav. 6, 893-900 (1989)
1989
-
[35]
Lecture notes on interacting quantum fields in de Sitter space,
E. T. Akhmedov, “Lecture notes on interacting quantum fields in de Sitter space,” Int. J. Mod. Phys. D 23 (2014) 1430001 [arXiv:1309.2557 [hep-th]]
2014 arXiv
-
[36]
Les Houches lectures on de Sitter space,
M. Spradlin, A. Strominger and A. Volovich, “Les Houches lectures on de Sitter space,” hep-th/0110007
- [37]
-
[38]
CMB from EFT,
S. Choudhury, “CMB from EFT,” Universe 5 (2019) no.6, 155 [arXiv:1712.04766 [hep-th]]
2019 arXiv
-
[39]
Inflation to Structures: EFT all the way,
A. Naskar, S. Choudhury, A. Banerjee and S. Pal, “Inflation to Structures: EFT all the way,” arXiv:1706.08051 [astro-ph.CO]
-
[40]
Effective Field Theory of Dark Matter from membrane inflationary paradigm,
S. Choudhury and A. Dasgupta, “Effective Field Theory of Dark Matter from membrane inflationary paradigm,” Phys. Dark Univ. 13 (2016) 35 [arXiv:1510.08195 [hep-th]]
2016 arXiv
- [41]
-
[42]
Chakrabarty, Subhashish Banerjee and N
I. Chakrabarty, Subhashish Banerjee and N. Siddharth, ”A study of Quantum Correlations in Open Quantum Systems,” Quantum Information and Computation: 11, 0541 (2011), eprint:arXiv:1006.1856
2011 arXiv
-
[43]
Subhashish Banerjee, ”Open Quantum Systems:Dynamics of Nonclassical Evolution”, Texts and Readings in Physical Sciences, Volume 20, Springer-Singapore, 2018, https: // doi.org/ 10.1007 /978-981-13-3182-4
2018
-
[44]
Quantum Thermodynamics,
R. Kosloff, “Quantum Thermodynamics,” Entropy 15 (2013) 2100 [arXiv:1305.2268 [quant-ph]]
2013 arXiv
-
[45]
The Theory of Open Quantum Systems
Breuer, Heinz-Peter; F. Petruccione “The Theory of Open Quantum Systems” Oxford University Press. ISBN 978-0-19-921390-0
-
[46]
The Lamb shift in de Sitter spacetime,
W. Zhou and H. W. Yu , “The Lamb shift in de Sitter spacetime,” Phys. Rev. D 82, 124067 (2010) [arXiv:1012.4055 [hep-th]]
2010 arXiv
-
[47]
Cosmological Event Horizons, Thermodynamics, and Particle Creation,
G. W. Gibbons and S. W. Hawking , “Cosmological Event Horizons, Thermodynamics, and Particle Creation,” Phys. Rev. D 15, 2738 (1977). doi:10.1103/PhysRevD.15.2738
1977 doi
-
[48]
Quantum states with Einstein-Podolsky-Rosen correlations admitting a hidden-variable model,
R. F. Werner, “Quantum states with Einstein-Podolsky-Rosen correlations admitting a hidden-variable model,” Phys. Rev. A 40 (1989) 4277
1989
-
[49]
Choudhury and S
S. Choudhury and S. Panda , ”Entangled de Sitter from stringy axionic Bell pair I: an analysis using BunchDavies vacuum”, Eur. Phys. J. C 78 (2018) no.1, 52 [arXiv:1708.02265 [hep-th]]
2018 arXiv
-
[50]
Bell violation in the Sky,
S. Choudhury, S. Panda and R. Singh “Bell violation in the Sky,” Eur. Phys. J. C 77 (2017) no.2, 60 [arXiv:1607.00237 [hep-th]]
2017 arXiv
-
[51]
Quantum entanglement in de Sitter space from stringy axion: An analysis using α vacua,
S. Choudhury and S. Panda “Quantum entanglement in de Sitter space from stringy axion: An analysis using α vacua,” Nucl. Phys. B 943 (2019) 114606 [arXiv:1712.08299 [hep-th]]
2019 arXiv
-
[52]
Spectrum of cosmological correlation from vacuum fluctuation of Stringy Axion in entangled de Sitter space,
S. Choudhury and S. Panda, “Spectrum of cosmological correlation from vacuum fluctuation of Stringy Axion in entangled de Sitter space,” arXiv:1809.02905 [hep-th]
-
[53]
Bell violation in primordial cosmology,
S. Choudhury, S. Panda and R. Singh, “Bell violation in primordial cosmology,” Universe 3 (2017) no.1, 13 [arXiv:1612.09445 [hep-th]]
2017 arXiv
-
[54]
An accurate bound on tensor-to-scalar ratio and the scale of inflation,
S. Choudhury and A. Mazumdar, “An accurate bound on tensor-to-scalar ratio and the scale of inflation,” Nucl. Phys. B 882 (2014) 386 [arXiv:1306.4496 [hep-ph]]. – 50 –
2014 arXiv
-
[55]
Brane inflation: A field theory approach in background supergravity,
S. Choudhury and S. Pal, “Brane inflation: A field theory approach in background supergravity,”
-
[56]
Brane inflation in background supergravity,
S. Choudhury and S. Pal, “Brane inflation in background supergravity,” Phys. Rev. D 85 (2012) 043529 [arXiv:1102.4206 [hep-th]],
2012 arXiv
-
[57]
DBI Galileon inflation in background SUGRA,
S. Choudhury and S. Pal, “DBI Galileon inflation in background SUGRA,” Nucl. Phys. B 874 (2013) 85 [arXiv:1208.4433 [hep-th]],
2013 arXiv
-
[58]
Quantum Out-of-Equilibrium Cosmology,
S. Choudhury, A. Mukherjee, P. Chauhan and S. Bhattacherjee, “Quantum Out-of-Equilibrium Cosmology,” Eur. Phys. J. C 79 (2019) no.4, 320 [arXiv:1809.02732 [hep-th]],
2019 arXiv
-
[59]
Quantum randomness in the Sky,
S. Choudhury and A. Mukherjee, “Quantum randomness in the Sky,” Eur. Phys. J. C 79 (2019) no.7, 554 [arXiv:1812.04107 [physics.gen-ph]]
2019 arXiv
-
[60]
”Squashed Entanglement
Matthias Christandl, Andreas Winter “”Squashed Entanglement” - An Additive Entanglement Measure” arXiv:quant-ph/0308088
-
[61]
Entanglement of Distillation and Conditional Mutual Information
Robert R.Tucci “Entanglement of Distillation and Conditional Mutual Information” arXiv:quant-ph/0202144
-
[62]
Chaos and relative entropy,
Y. O. Nakagawa, G. Srosi and T. Ugajin, “Chaos and relative entropy,” JHEP 1807 (2018) 002 [arXiv:1805.01051 [hep-th]]
2018 arXiv
-
[63]
QMetrology from QCosmology: Study with Entangled Two Qubit Open Quantum System in De Sitter Space,
S. Choudhury, S. Chowdhury, N. Gupta and A. Swain, “QMetrology from QCosmology: Study with Entangled Two Qubit Open Quantum System in De Sitter Space,” [arXiv:2005.13555 [hep-th]]
2005 arXiv
-
[64]
https://www.oeaw.ac.at/en/detail/news/qutrit-complex-quantum-teleportation- achieved-for-the-first-time/
See the web link: “https://www.oeaw.ac.at/en/detail/news/qutrit-complex-quantum-teleportation- achieved-for-the-first-time/”
-
[65]
Quantum teleportation in high dimensions,
Yi-Han Luo, Han-Sen Zhong, Manuel Erhard, Xi-Lin Wang, Li-Chao Peng, Mario Krenn, Xiao Jiang, Li Li, Nai-Le Liu, Chao-Yang Lu, Anton Zeilinger, Jian-Wei Pan , “Quantum teleportation in high dimensions,” Phys. Rev. Lett. 123 070505 (2019), [ arXiv:1906.09697 [quant-ph]]
2019 arXiv
-
[66]
Banerjee, S
S. Banerjee, S. Choudhury, S. Chowdhury, R. N. Das, N. Gupta, S. Panda and A. Swain, Indirect detection of Cosmological Constant from large N entangled open quantum system,” [arXiv:2004.13058 [hep-th]]. – 51 –
2004 arXiv
Reviewed August 14, 2026 · model on record in the stance chip above.
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