Abstract
We analyze the behavior of caloric characteristics and the electron component of the spin polarization of excitations in the regime of strong electron correlations of a nanowire, which is characterized by induced superconductivity of the extended s-type symmetry, the Rashba spin–orbit interaction, and the Zeeman splitting of on-site energy. The problem has been analyzed using the density matrix renormalization group method. It is shown that for unambiguous identification of different phases (the topologically trivial phase with edge excitations and without them, as well as topologically nontrivial phases with one or several pairs of Majorana modes), it is insufficient to analyze each of the aforementioned characteristics separately; it is necessary to consider their features simultaneously.
Similar content being viewed by others
REFERENCES
N. Read and D. Green, Phys. Rev. B 61, 10267 (2000).
A. Yu. Kitaev, Phys. Usp. 44, s131 (2001).
V. Kaladzhyan and C. Bena, Phys. Rev. B 100, 081106 (2019).
Q. Wang, C.-C. Liu, Y.-M. Lu, et al., Phys. Rev. Lett. 121, 186801 (2018).
X. Zhu, Phys. Rev. B 91, 205134 (2018).
C. Nayak, S. H. Simon, A. Stern, et al., Rev. Mod. Phys. 80, 1083 (2008).
J. Alicea, Rep. Prog. Phys. 75, 076501 (2012).
S. R. Elliot and M. Franz, Rev. Mod. Phys. 87, 137 (2015).
M. Sato and Y. Ando, Rep. Prog. Phys. 80, 076501 (2017).
V. V. Val’kov, M. S. Shustin, S. V. Aksenov, et al., Usp. Fiz. Nauk 192, 3 (2022, in press).
A. P. Mackenzie and Y. Maeno, Rev. Mod. Phys. 75, 657 (2003).
S. Das Sarma, C. Nayak, and S. Tewari, Phys. Rev. B 73, 220502(R) (2006).
A. Pustogow, Y. Luo, A. Chronister, et al., Nature (London, U.K.) 574, 72 (2019).
S.-I. Suzuki, M. Sato, and Y. Tanaka, Phys. Rev. B 101, 054505 (2020).
J. D. Sau and S. Tewari, Phys. Rev. B 86, 104509 (2012).
V. P. Mineev, Phys. Usp. 60, 121 (2017).
R. M. Lutchyn, J. D. Sau, and S. Das Sarma, Phys. Rev. Lett. 105, 077001 (2010).
Y. Oreg, G. Refael, and F. von Oppen, Phys. Rev. Lett. 105, 177002 (2010).
V. Mourik, K. Zuo, S. M. Frolov, et al., Science (Washington, DC, U. S.) 336, 1003 (2012).
M. T. Deng, C. L. Yu, G. Y. Huang, et al., Nano Lett. 12, 6414 (2012).
F. Nichele, A. C. C. Drachmann, A. M. Whiticar, et al., Phys. Rev. Lett. 119, 136803 (2017).
H. Zhang, C.-X. Liu, S. Gazibegovic, et al., Nature (London, U.K.) 556, 74 (2018).
P. Yu, J. Chen, M. Gomanko, et al., Nat. Phys. 17, 482 (2021).
S. Vaitiekenas, Y. Liu, P. Krogstrup, et al., Nat. Phys. 17, 43 (2020).
C. Moore, T. D. Stanescu, and S. Tewari, Phys. Rev. B 97, 165302 (2018).
C. Reeg, O. Dmytruk, D. Chevallier et al., Phys. Rev. B 98, 245407 (2018).
H. Zhang, C.-X. Liu, S. Gazibegovic, et al., Nature (London, U.K.) 581, E4 (2020).
Y. Sato, S. Matsuo, C.-H. Hsu, et al., Phys. Rev. B 99, 155304 (2019).
R. Thomale, S. Rachel, and P. Schmitteckert, Phys. Rev. B 88, 161103(R) (2013).
Y.-H. Chan, C.-K. Chiu, and K. Sun, Phys. Rev. B 92, 104514 (2015).
N. M. Gergs, L. Fritz, and D. Schurich, Phys. Rev. B 93, 075129 (2016).
J.-J. Miao, H.-K. Jin, and Y. Zhou, Sci. Rep. 8, 488 (2018).
G. Kells, Phys. Rev. B 92, 081401(R) (2015).
G. Kells, Phys. Rev. B 92, 155434 (2015).
S. R. White, Phys. Rev. Lett. 69, 2863 (1992).
S. R. White, Phys. Rev. B 48, 10345 (1993).
U. Schollwock, Rev. Mod. Phys. 77, 259 (2005).
U. Schollwock, Ann. Phys. 326, 96 (2011).
V. V. Val’kov, V. A. Mitskan, and M. S. Shustin, JETP Lett. 106, 798 (2017).
V. V. Val’kov, M. Yu. Kagan, and S. V. Aksenov, J. Phys.: Condens. Matter 31, 225301 (2019).
V. V. Val’kov and S. V. Aksenov, J. Low Temp. Phys. 43, 437 (2017).
V. V. Val’kov and S. V. Aksenov, J. Magn. Magn. Mater. 440, 112 (2017).
D. Sticlet, C. Bena, and P. Simon, Phys. Rev. Lett. 108, 096802 (2012).
P. Szumniak, D. Chevallier, D. Loss, et al., Phys. Rev. B 96, 041401(R) (2017).
M. Serina, D. Loss, and J. Klinovaja, Phys. Rev. B 98, 035419 (2018).
S. V. Aksenov, A. O. Zlotnikov, and M. S. Shustin, Phys. Rev. B 101, 125431 (2020).
E. M. Stoudenmire, J. Alicea, O. A. Starykh, et al., Phys. Rev. B 84, 014503 (2011).
M. R. Zirnbauer, J. Math. Phys. 37, 4986 (1996).
A. Altland and M. R. Zirnbauer, Phys. Rev. B 55, 1142 (1997).
P. Heinzner, A. Huckleberry, and M. R. Zirnbauer, Commun. Math. Phys. 257, 725 (2005).
A. P. Schnyder, S. Ryu, A. Furusaki, et al., Phys. Rev. B 78, 195125 (2008).
A. P. Schnyder, S. Ryu, A. Furusaki, et al., AIP Conf. Proc. 1134, 10 (2009). https://doi.org/10.1063/1.3149481
A. Yu. Kitaev, AIP Conf. Proc. 1134, 22 (2009). https://doi.org/10.1063/1.3149495
W. DeGottardi, M. Thakurathi, S. Vishveshwara, et al., Phys. Rev. B 88, 165111 (2013).
A. M. Turner, F. Pollmann, and E. Berg, Phys. Rev. B 83, 075102 (2011).
M. S. Shustin and S. V. Aksenov, Phys. Solid State 63 (2021, in press).
G. Goldstein and C. Chamon, Phys. Rev. B 86, 115122 (2012).
A. D. Fedoseev, J. Exp. Theor. Phys. 128, 125 (2019).
M. Leijnse and K. Flensberg, Phys. Rev. Lett. 107, 210502 (2011).
Y. Nagai, H. Nakamura, and M. Machida, J. Phys. Soc. Jpn. 83, 064703 (2014).
L. Zhu, M. Garst, A. Rosch, et al., Phys. Rev. Lett. 91, 066404 (2003).
M. Garst and A. Rosch, Phys. Rev. B 72, 205129 (2005).
D. J. Thouless, Phys. Rep. 13, 93 (1974).
N. C. Murphy, R. Wortis, and W. A. Atkinson, Phys. Rev. B 83, 184206 (2011).
M. Malki and G. S. Uhrig, Eur. Phys. Lett. 127, 27001 (2019).
A. D. Fedoseev, J. Exp. Theor. Phys. 133, 71 (2021).
ACKNOWLEDGMENTS
The authors are grateful to A.D. Fedoseev for discussions.
Funding
This study was supported by the Russian Foundation for Basic Research (project nos. 19-02-00348 and 20-02-00015), the administration of the Krasnoyarsk Kray, the Krasnoyarsk Kray Science Foundation (project nos. 20-42-243001 and 20-42-243005), and the Council for Grants from the President of Russian Federation (projects nos. MK-1641.2020.2 and MK-4687.2022.1). One of the authors (Sh.M.S.) thanks the Foundation for the Development of Theoretical Physics and Mathematics “BASIS.”
Author information
Authors and Affiliations
Corresponding authors
Ethics declarations
CONFLICT OF INTEREST
The authors declare that they have no conflicts of interest.
ADDITIONAL INFORMATION
This article was prepared for the special issue of Journal of Experimental and Theoretical Physics dedicated to the 95th birthday of Professor E.I. Rashba.
Additional information
Translated by N. Wadhwa
Rights and permissions
About this article
Cite this article
Shustin, M.S., Aksenov, S.V. Features of Physical Observables of a Strongly Correlated Superconducting Nanowire with Rashba Spin–Orbit Interaction. J. Exp. Theor. Phys. 135, 500–512 (2022). https://doi.org/10.1134/S1063776122100181
Received:
Revised:
Accepted:
Published:
Issue Date:
DOI: https://doi.org/10.1134/S1063776122100181