Abstract
We analyze a tripartite entanglement harvesting protocol with three Unruh-DeWitt detectors adiabatically interacting with a quantum scalar field in \((3+1)\)-dimensional Minkowski spacetime. We consider linear, equilateral triangular, and scalene triangular configurations for the detectors, all of which remain static. We find that, under the same parameters, more entanglement can be extracted in the linear configuration than the equilateral one, consistent with single instantaneous switching results. No bipartite entanglement is required to harvest tripartite entanglement. Furthermore, we find that tripartite entanglement can be harvested even if one detector is at larger spacelike separations from the other two than in the corresponding bipartite case. We also find that for small detector separations bipartite correlations become larger than tripartite ones, leading to an apparent violation of the Coffman-Kundu-Wootters (CKW) inequality. We show that this is not a consequence of our perturbative expansion but that it instead occurs because the harvesting qubits are in a mixed state.
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References
Ralph, T.C., Milburn, G.J., Downes, T.: Phys. Rev. A 79, 022121 (2009). https://doi.org/10.1103/PhysRevA.79.022121
Peres, A., Terno, D.R.: Rev. Mod. Phys. 76, 93 (2004). https://doi.org/10.1103/RevModPhys.76.93
Lamata, L., Martin-Delgado, M.A., Solano, E.: Phys. Rev. Lett. 97, 250502 (2006). https://doi.org/10.1103/PhysRevLett.97.250502
Hotta, M.: J. Phys. Soc. Jpn. 78, 034001 (2009). https://doi.org/10.1143/JPSJ.78.034001
Hotta, M.: arXiv preprint arXiv:1101.3954 (2011)
Ryu, S., Takayanagi, T.: Phys. Rev. Lett. 96, 181602 (2006). https://doi.org/10.1103/PhysRevLett.96.181602. arXiv:hep-th/0603001
Solodukhin, S.N.: Living Rev. Relativ. 14, 8 (2011). https://doi.org/10.12942/lrr-2011-8. arXiv:1104.3712 [hep-th]
Brustein, R., Einhorn, M.B., Yarom, A.: JHEP 01, 098 (2006). https://doi.org/10.1088/1126-6708/2006/01/098. arXiv:hep-th/0508217
Preskill, J.: In: International Symposium on Black holes, Membranes, Wormholes and Superstrings Woodlands, Texas, January 16-18, 1992 pp. 22–39 (1992). arXiv:hep-th/9209058 [hep-th]
Mathur, S.D.: Class. Quant. Grav. 26, 224001 (2009). https://doi.org/10.1088/0264-9381/26/22/224001. arXiv:0909.1038 [hep-th]
Almheiri, A., Marolf, D., Polchinski, J., Sully, J.: J. High Energy Phys. 2013, 62 (2013). https://doi.org/10.1007/JHEP02(2013)062
Braunstein, S.L., Pirandola, S., Zyczkowski, K.: Phys. Rev. Lett. 110, 101301 (2013). https://doi.org/10.1103/PhysRevLett.110.101301. arXiv:0907.1190 [quant-ph]
Mann, R.B.: Black Holes: Thermodynamics, Information, and Firewalls, SpringerBriefs in Physics, Springer (2015) https://doi.org/10.1007/978-3-319-14496-2
Louko, J.: J. High Energ. Phys. 2014, 142 (2014). https://doi.org/10.1007/JHEP09(2014)142
Luo, S., Stoltenberg, H., Albrecht, A.: Phys. Rev. D 95, 064039 (2017). https://doi.org/10.1103/PhysRevD.95.064039
Joshi, P.S., Padmanabhan, T., Chitre, S.M.: Phys. Lett. A 120, 115 (1987). https://doi.org/10.1016/0375-9601(87)90709-2
Padmanabhan, T.: Class. Quant. Grav. 22, L107 (2005). https://doi.org/10.1088/0264-9381/22/17/L01. arXiv:hep-th/0406060
Padmanabhan, T.: Phys. Rept. 380, 235 (2003). https://doi.org/10.1016/S0370-1573(03)00120-0. arXiv:hep-th/0212290
Padmanabhan, T.: Gen. Rel. Grav. 38, 1547 (2006). https://doi.org/10.1007/s10714-006-0338-6
Padmanabhan, T.: Int. J. Mod. Phys. D 15, 2029 (2006). https://doi.org/10.1142/S0218271806009455. arXiv:gr-qc/0609012
Sriramkumar, L., Padmanabhan, T.: Int. J. Mod. Phys. D 11, 1 (2002). https://doi.org/10.1142/S0218271802001354. arXiv:gr-qc/9903054
Lochan, K., Chakraborty, S., Padmanabhan, T.: Eur. Phys. J. C 78, 433 (2018). https://doi.org/10.1140/epjc/s10052-018-5911-0. arXiv:1603.01964 [gr-qc]
Sriramkumar, L., Padmanabhan, T.: Class. Quant. Grav. 13, 2061 (1996). https://doi.org/10.1088/0264-9381/13/8/005. arXiv:gr-qc/9408037
Valentini, A.: Phys. Lett. A 153, 321 (1991). https://doi.org/10.1016/0375-9601(91)90952-5
Reznik, B.: Found. Phys. 33, 167 (2003). https://doi.org/10.1023/A:1022875910744
Reznik, B., Retzker, A., Silman, J.: Phys. Rev. A 71, 042104 (2005). https://doi.org/10.1103/PhysRevA.71.042104
Steeg, G.V., Menicucci, N.C.: Phys. Rev. D 79, 044027 (2009). https://doi.org/10.1103/PhysRevD.79.044027
Pozas-Kerstjens, A., Martín-Martínez, E.: Phys. Rev. D 92, 064042 (2015). https://doi.org/10.1103/PhysRevD.92.064042
Martín-Martínez, E., Smith, A.R.H., Terno, D.R.: Phys. Rev. D 93, 044001 (2016). https://doi.org/10.1103/PhysRevD.93.044001
Martín-Martínez, E., Sanders, B.C.: New J. Phys. 18, 043031 (2016). https://doi.org/10.1088/1367-2630/18/4/043031
Kukita, S., Nambu, Y.: Entropy 19, 449 (2017). https://doi.org/10.3390/e19090449
Simidzija, P., Martín-Martínez, E.: Phys. Rev. D 96, 065008 (2017). https://doi.org/10.1103/PhysRevD.96.065008
Simidzija, P., Jonsson, R.H., Martín-Martínez, E.: Phys. Rev. D 97, 125002 (2018). https://doi.org/10.1103/PhysRevD.97.125002
Henderson, L.J., Hennigar, R.A., Mann, R.B., Smith, A.R.H., Zhang, J.: Class. Quant. Grav. 35, 21LT02 (2018). https://doi.org/10.1088/1361-6382/aae27e
Ng, K.K., Mann, R.B., Martín-Martínez, E.: Phys. Rev. D 98, 125005 (2018). https://doi.org/10.1103/PhysRevD.98.125005
Henderson, L.J., Hennigar, R.A., Mann, R.B., Smith, A.R., Zhang, J.: J. High Energ. Phys. 2019, 178 (2019). https://doi.org/10.1007/JHEP05(2019)178
Cong, W., Tjoa, E., Mann, R.B.: J. High Energ. Phys 2019, 21 (2019). https://doi.org/10.1007/JHEP06(2019)021
Tjoa, E., Mann, R.B.: J. High Energy Phys. 2020, 1 (2020). https://doi.org/10.1007/JHEP08(2020)155
Cong, W., Qian, C., Good, M.R., Mann, R.B.: J. High Energy Phys. 2020, 67 (2020). https://doi.org/10.1007/JHEP10(2020)067
Xu, Q., Ahmad, S.A., Smith, A.R.H.: (2020), Arxiv:2006.11301v1
Zhang, J., Yu, H.: Phys. Rev. D 102, 065013 (2020). https://doi.org/10.1103/PhysRevD.102.065013. arXiv:2008.07980 [quant-ph]
Liu, Z., Zhang, J., Yu, H.: JHEP 08, 020 (2021). https://doi.org/10.1007/JHEP08(2021)020. arXiv:2101.00114 [quant-ph]
Liu, Z., Zhang, J., Mann, R.B., Yu, H.: (2021). arXiv:2111.04392 [quant-ph]
Hu, H., Zhang, J., Yu, H.: (2022). arXiv:2204.01219 [quant-ph]
Salton, G., Mann, R.B., Menicucci, N.C.: New J. Phys. 17, 035001 (2015). https://doi.org/10.1088/1367-2630/17/3/035001
Olson, S.J., Ralph, T.C.: Phys. Rev. A 85, 012306 (2012). https://doi.org/10.1103/PhysRevA.85.012306
Sabín, C., Peropadre, B., del Rey, M., Martín-Martínez, E.: Phys. Rev. Lett. 109, 033602 (2012). https://doi.org/10.1103/PhysRevLett.109.033602
Brown, E.G., del Rey, M., Westman, H., León, J., Dragan, A.: Phys. Rev. D 91, 016005 (2015). https://doi.org/10.1103/PhysRevD.91.016005
Hu, B.L., Lin, S.-Y., Louko, J.: Class. Quant. Grav. 29, 224005 (2012). https://doi.org/10.1088/0264-9381/29/22/224005
Brown, E.G., Martin-Martinez, E., Menicucci, N.C., Mann, R.B.: Phys. Rev. D 87, 084062 (2013). https://doi.org/10.1103/PhysRevD.87.084062. arXiv:1212.1973 [quant-ph]
Bruschi, D.E., Lee, A.R., Fuentes, I.: J. Phys. A 46, 165303 (2013). https://doi.org/10.1088/1751-8113/46/16/165303. arXiv:1212.2110 [quant-ph]
Unruh, W.G.: Phys. Rev. D 14, 870 (1976). https://doi.org/10.1103/PhysRevD.14.870
DeWitt, B.S.: In: General Relativity: An Einstein centenary survey. Hawking, S.W., Israel, W. (Eds.), pp. 680–745 (Cambridge University Press 1979)
Martin-Martinez, E., Montero, M., del Rey, M.: Phys. Rev. D 87, 064038 (2013). https://doi.org/10.1103/PhysRevD.87.064038. arXiv:1207.3248 [quant-ph]
Funai, N., Louko, J., Martín-Martínez, E.: Phys. Rev. D 99, 065014 (2019). https://doi.org/10.1103/PhysRevD.99.065014. arXiv:1807.08001 [quant-ph]
Funai, N.: Investigations into quantum light-matter interactions, their approximations and applications, Ph.D. thesis, U. Waterloo (main) (2021)
Ng, K.K., Mann, R.B., Martín-Martínez, E.: Phys. Rev. D 96, 085004 (2017). https://doi.org/10.1103/PhysRevD.96.085004
Cong, W., Bicak, J., Kubiznak, D., Mann, R.B.: Phys. Lett. B 820, 136482 (2021). https://doi.org/10.1016/j.physletb.2021.136482. arXiv:2103.05802 [gr-qc]
Dappiaggi, C., Marta, A.: Math. Phys. Anal. Geom. 24, 28 (2021). https://doi.org/10.1007/s11040-021-09402-5. arXiv:2101.10290 [math-ph]
Smith, A.R.H., Mann, R.B.: Class. Quant. Grav. 31, 082001 (2014). https://doi.org/10.1088/0264-9381/31/8/082001. arXiv:1309.4125 [gr-qc]
Henderson, L.J., Mann, R.B., Hennigar, R.A., Smith, A.R.H., Zhang, J.: Class. Quant. Grav. 52, 1 (2018). https://doi.org/10.1080/14484846.2018.1432089
Robbins, M.P.G., Henderson, L.J., Mann, R.B.: Class. Quant. Grav. 39, 02LT01 (2022). https://doi.org/10.1088/1361-6382/ac08a8. arXiv:2010.14517 [hep-th]
Kaplanek, G., Burgess, C.P.: JHEP 01, 098 (2021). https://doi.org/10.1007/JHEP01(2021)098. arXiv:2007.05984 [hep-th]
de Souza Campos, L., Dappiaggi, C.: Phys. Lett. B 816, 136198 (2021). https://doi.org/10.1016/j.physletb.2021.136198. arXiv:2009.07201 [hep-th]
de Souza Campos, L., Dappiaggi, C.: Phys. Rev. D 103, 025021 (2021). https://doi.org/10.1103/PhysRevD.103.025021. arXiv:2011.03812 [hep-th]
Robbins, M.P.G., Mann, R.B.: (2021). arXiv:2107.01648 [gr-qc]
Henderson, L.J., Ding, S.Y., Mann, R.B.: (2022). arXiv:2201.11130 [quant-ph]
Gallock-Yoshimura, K., Tjoa, E., Mann, R.B.: Phys. Rev. D 104, 025001 (2021). https://doi.org/10.1103/PhysRevD.104.025001
Bueley, K., Huang, L., Gallock-Yoshimura, K., Mann, R.B.: Harvesting mutual information from btz black hole spacetime (2022). https://doi.org/10.48550/ARXIV.2205.07891
Gray, F., Kubiznak, D., May, T., Timmerman, S., Tjoa, E.: JHEP 11, 054 (2021). https://doi.org/10.1007/JHEP11(2021)054. arXiv:2105.09337 [hep-th]
Huang, Z., Tian, Z.: Nucl. Phys. B 923, 458 (2017). https://doi.org/10.1016/j.nuclphysb.2017.08.014
Kaplanek, G., Burgess, C.P.: JHEP 02, 053 (2020). https://doi.org/10.1007/JHEP02(2020)053. arXiv:1912.12955 [hep-th]
Du, H., Mann, R.B.: JHEP 05, 112 (2021). https://doi.org/10.1007/JHEP05(2021)112. arXiv:2012.08557 [hep-th]
Foo, J., Mann, R.B., Zych, M.: Class. Quant. Grav. 38, 115010 (2021). https://doi.org/10.1088/1361-6382/abf1c4. arXiv:2012.10025 [gr-qc]
Foo, J., Arabaci, C.S., Zych, M., Mann, R.B.: (2021). arXiv:2111.13315 [gr-qc]
Howl, R., Akil, A., Kristjánsson, H., Zhao, X., Chiribella, G.: (2022). arXiv:2203.05861 [quant-ph]
Faure, R., Perche, T.R., Torres, Bd.S.L.: Phys. Rev. D 101, 125018 (2020). https://doi.org/10.1103/PhysRevD.101.125018
Pitelli, J.P.M., Perche, T.R.: Phys. Rev. D 104, 065016 (2021). https://doi.org/10.1103/PhysRevD.104.065016
Onoe, S., Guedes, T.L.M., Moskalenko, A.S., Leitenstorfer, A., Burkard, G., Ralph, T.C.: 1 (2021). arXiv:2103.14360
Torres-Arenas, A.J., López-Zúñiga, E.O., Saldaña-Herrera, J.A., Dong, Q., Sun, G.H., Dong, S.H.: arXiv (2018). arXiv:1810.03951
Khan, S., Khan, N.A., Khan, M.K.: Commun. Theor. Phys. 61, 281 (2014). https://doi.org/10.1088/0253-6102/61/3/02. arXiv:1402.7152
Hwang, M.-R., Park, D., Jung, E.: Phys. Rev. A 83, 012111 (2011). https://doi.org/10.1103/PhysRevA.83.012111
Szypulski, J., Grochowski, P., Dębski, K., Dragan, A.: (2021)
Gühne, O., Tóth, G.: Phys. Rep. 474, 1 (2009). https://doi.org/10.1016/j.physrep.2009.02.004. arXiv:0811.2803
Silman, J., Reznik, B.: Phys. Rev. A 71, 054301 (2005). https://doi.org/10.1103/PhysRevA.71.054301
Lorek, K., Pecak, D., Brown, E.G., Dragan, A.: Phys. Rev. A 90, 032316 (2014). https://doi.org/10.1103/PhysRevA.90.032316
Avalos, D.M., Gallock-Yoshimura, K., Henderson, L.J., Mann, R.B.: (2022). arXiv:2204.02983 [quant-ph]
Dur, W., Vidal, G., Cirac, J.I.: Phys. Rev. A - At., Mol., Opt. Phys. 62, 062314 (2000). https://doi.org/10.1103/PhysRevA.62.062314
Ou, Y.-C., Fan, H.: Phys. Rev. A 75, 062308 (2007). https://doi.org/10.1103/PhysRevA.75.062308
Shi, X.: 2, 1 (2022). https://arxiv.org/abs/2206.02232
Halder, P., Mal, S., Sen, A.: Phys. Rev. A 104, 1 (2021). https://doi.org/10.1103/PhysRevA.104.062412. arXiv:2108.06173
Ou, Y.C., Fan, H.: Phys. Rev. A - At., Mol., Opt. Phys. 75, 1 (2007). https://doi.org/10.1103/PhysRevA.75.062308. arXiv:0702127 [quant-ph]
Vidal, G., Werner, R.F.: Phys. Rev. A 65, 032314 (2002). https://doi.org/10.1103/PhysRevA.65.032314
Smith, A.R.: University of Waterloo, Ph.D. thesis, University of Waterloo (2017). https://uwspace.uwaterloo.ca/handle/10012/12618
Coffman, V., Kundu, J., Wootters, W.K.: Phys. Rev. A 61, 052306 (2000). https://doi.org/10.1103/PhysRevA.61.052306. arXiv:quant-ph/9907047
W. R. Inc., “Mathematica, Version 12.2,” Champaign, IL (2020). https://www.wolfram.com/mathematica
Acknowledgements
All the numerical calculations and the figures were made via Mathematica software [96]. This work was supported in part by the Natural Sciences and Engineering Research Council of Canada. We are grateful to Meenu Kumari for helpful discussions. Data sharing is not applicable to this article as no datasets were generated or analysed during this study.
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Appendices
Appendix A: The \(\pi \)-tangle for the scalene triangle configuration
Here we present the calculations for the \(\pi \)-tangle when the three detectors are in a scalene triangular configuration.
When the distance between each pair of detectors is arbitrary, the density matrix Eq. (6) becomes
Following the same procedure for the equilateral triangular and linear configurations, we obtain
and
The \(\pi \)-tangle is then easily computed using Eqs. (12) and (11).
Appendix B: A toy model
The introduction of the \(\pi \)-tangle [92] has generally been thought to satisfy the CKW inequality. Specficially “For any pure \(2\otimes 2\otimes 2\) states \({|{\phi }\rangle }_{ABC}\), the entanglement quantified by the negativity between A and B, between A and C, and between A and the single object BC satisfies the following CKW-inequality-like monogamy inequality:
where \({\mathcal {N}}_{AB}\) and \({\mathcal {N}}_{AC}\) are the negativities of the mixed states”. Although the preceding inequality holds only for pure tripartite systems, the form of the preceding statement suggests that violations of the CKW inequality are perhaps unexpected and somewhat counter-intuitive. To illustrate that such violations are not a consequence of the perturbative expression given in (6), we present a simple density matrix for a tripartite system of qubits that can have negative \(\pi \)-tangle over a wide range of parameters.
Assume that we have a density matrix of the form
where \(P,C,E,\Sigma \in {\mathbb {R}}\), which is clearly trace 1 and Hermitian. In order for this matrix to be a valid density matrix, it must have positive eigenvalues, which puts the following constraints on the elements of \(\rho _{ABC}\):
From constraints Eqs. (B2c) and (B2d), we get the additional constraint:
If we assume that
which will be true if \(P,E,\Sigma \ll 1\), then constraint (B2e) will be satisfied provided:
which is consistent with the assumption (B4) since \(E\ge 0\) and \(|X|\ge 0\).
The partial transpose of \(\rho _{ABC}\) with respect to A is
which only has two eigenvalues that can be negative while maintaining non-negative eigenvalues for \(\rho _{ABC}\):
In particular eigenvalue (B7) will only be non-negative if
and eigenvalue (B8) only be non-negative if
Note that provided \(C^2>|X|^2\), eigenvalue (B8) can be negative without contradicting condition (B5).
Finally, we calculate the negativity of \(\rho _{AB}={{\,\mathrm{Tr}\,}}_C[\rho _{ABC}]\). The partial transpose of \(\rho _{AB}\) is
which again only has two eigenvalues that can be negative while maintaining non-negative eigenvalues for \(\rho _{AB}\):
Eigenvalue (B12) will be non-negative if
and eigenvalue (B13) will be non-negative if
Under the assumption that
then condition (B15) can be related to condition (B10) by noticing that
meaning that if Eq. (B15) is not satisfied then neither will Eq. (B10); if Eq. (B10) is satisfied then Eq. (B15) will be too.
The only way that the CKW inequality is violated will be if \({\mathcal {N}}_{A(B)}\) is nonzero. In other words, at least one of the eigenvalues of the partial transpose of \(\rho _{AB}\) must be negative. We will first consider the case where eigenvalue (B12) is negative, followed by the case where (B13) is negative. We will also show that under the assumptions that (B4) and (B16) are both valid, it is not possible for both eigenvalues to be simultaneously negative.
1.1 Case #1: Assume that eigenvalue (B12) is negative
If eigenvalue (B12) is negative, then \(|X|>P+E\) and we also have \(|X|^2>C^2\) (since \(P+E\ge P\ge C\)). This means that in order that \(\rho _{ABC}\) remain a valid density matrix, eigenvalue (B8) must be non-negative, implying that eigenvalue (B13) must be also non-negative. Additionally eigenvalue (B7) must also be negative since
In this case, the \(\pi \)-tangle is
which can be simplified by considering a Taylor expansion of the matrix elements of \(\rho _{ABC}\) in powers of the coupling strength, \(\lambda \ll 1\):
Under this expansion, the \(\pi \)-tangle becomes:
which will be non-negative if
As the condition in (B22) is not particularly instructive, we plot the perturbative \(\pi \)-tangle (B21) in Fig. 10, where it is clear that there are regions of the parameter space where the \(\pi \)-tangle is negative, meaning the CKW inequality is not satisfied. For example, if
Additionally, if the non-perturbative expression for the \(\pi \)-tangle (B19) is considered, it is still possible to find regions of the parameter space where the CKW inequality is not satisfied. For example,
1.2 Case #2: Assume that eigenvalue (B13) is negative
If eigenvalue (B13) is negative, then \(\sqrt{4C^2+(1-4E-2P-2\Sigma )^2}>(1-2P-2E)\) and eigenvalue (B8) will also be negative. Recall that in order to ensure that \(\rho _{ABC}\) is a valid density matrix, we also require \(C^2>|X|^2\). This also means that eigenvalue (B12) is non-negative since \(|X|^2 < C^2 \le P^2 \le (P+E)^2\). Also notice that if \(C\ge 0\), then
and if \(C<0\), then Eq. (B2d) becomes \(P\ge -2C=2|C|\), and
so, eigenvalue (B7) is also non-negative regardless of the sign of C. Therefore, the \(\pi \)-tangle is
where the last line is from the perturbative expansion of \(\rho _{ABC}\) [Eq. (B20)]. In this case, the \(\pi \)-tangle will be non-negative if
Once again, we can find regions of the parameter space where the \(\pi \)-tangle is negative, meaning the CKW inequality is not satisfied. For example if
Additionally, if the non-perturbative expression for the \(\pi \)-tangle (B24) is considered, it is still possible to find regions of the parameter space where the CKW inequality is not satisfied. For example if
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Mendez-Avalos, D., Henderson, L.J., Gallock-Yoshimura, K. et al. Entanglement harvesting of three Unruh-DeWitt detectors. Gen Relativ Gravit 54, 87 (2022). https://doi.org/10.1007/s10714-022-02956-x
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DOI: https://doi.org/10.1007/s10714-022-02956-x