journal article·2016-03-25Open access

Gate-tunable zero-frequency current cross correlations of the quartet state in a voltage-biased three-terminal Josephson junction

Régis Mélin, Moïse Sotto, Denis Feinberg, Jean-Guy Caputo, Benoît Douçot

Physical Review B· Volume 93· Issue 11

Abstract

A three-terminal Josephson junction biased at opposite voltages can sustain a phase-sensitive dc current carrying three-body static phase coherence, known as the ``quartet current.'' We calculate the zero-frequency current noise cross correlations and answer the question of whether this current is noisy (like a normal current in response to a voltage drop) or noiseless (like an equilibrium supercurrent in response to a phase drop). A quantum dot with a level at energy ${\ensuremath{\epsilon}}0$ is connected to three superconductors ${S}a,\phantom{\rule{0.16em}{0ex}}{S}b$, and ${S}c$ with gap $\mathrm{\ensuremath{\Delta}}$, biased at ${V}a=V,\phantom{\rule{0.16em}{0ex}}{V}b=\ensuremath{-}V$, and ${V}c=0$, and with intermediate contact transparencies. At zero temperature, nonlocal quartets (in the sense of four-fermion correlations) are noiseless at subgap voltage in the nonresonant dot regime ${\ensuremath{\epsilon}}0/\mathrm{\ensuremath{\Delta}}\ensuremath{\gg}1$, which is demonstrated with a semianalytical perturbative expansion of the cross correlations. Noise reveals the absence of granularity of the superflow splitting from ${S}c$ towards $({S}a,{S}b)$ in the nonresonant dot regime, in spite of finite voltage. In the resonant dot regime ${\ensuremath{\epsilon}}0/\mathrm{\ensuremath{\Delta}}\ensuremath{\lesssim}1$, cross correlations measured in the $({V}a,{V}b)$ plane should reveal an ``anomaly'' in the vicinity of the quartet line ${V}a+{V}b=0$, related to an additional contribution to the noise, manifesting the phase sensitivity of cross correlations under the appearance of a three-body phase variable. Phase-dependent effective Fano factors ${F}_{\ensuremath{\varphi}}$ are introduced, defined as the ratio between the amplitudes of phase modulations of the noise and the currents. At low bias, the Fano factors ${F}_{\ensuremath{\varphi}}$ are of order unity in the resonant dot regime ${\ensuremath{\epsilon}}0/\mathrm{\ensuremath{\Delta}}\ensuremath{\lesssim}1$, and they are vanishingly small in the nonresonant dot regime ${\ensuremath{\epsilon}}0/\mathrm{\ensuremath{\Delta}}\ensuremath{\gg}1$.
Source: openalex_inverted_index · Quality: baseline

Research context

OpenAlex topics: Quantum and electron transport phenomena · Quantum Information and Cryptography · Physics of Superconductivity and Magnetism

SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.

References (39)

Show source-provided references
1. 10.1103/PhysRevLett.75.183110.1103/PhysRevLett.75.1831 ↗
2. 10.1103/PhysRevLett.76.381410.1103/PhysRevLett.76.3814 ↗
3. 10.1103/PhysRevB.54.736610.1103/PhysRevB.54.7366 ↗
4. 10.1103/PhysRevLett.82.408610.1103/PhysRevLett.82.4086 ↗
5. 10.1103/PhysRevLett.78.353510.1103/PhysRevLett.78.3535 ↗
6. 10.1038/2811210.1038/28112 ↗
7. 10.1103/PhysRevLett.86.410410.1103/PhysRevLett.86.4104 ↗
8. 10.1103/PhysRevB.75.17451310.1103/PhysRevB.75.174513 ↗
9. 10.1103/PhysRevLett.106.25700510.1103/PhysRevLett.106.257005 ↗
10. 10.1103/PhysRevB.87.21450110.1103/PhysRevB.87.214501 ↗
11. 10.1103/PhysRevLett.102.08680410.1103/PhysRevLett.102.086804 ↗
12. 10.1103/PhysRevB.82.06051710.1103/PhysRevB.82.060517 ↗
13. 10.1103/PhysRevB.90.15545010.1103/PhysRevB.90.155450 ↗
14. 10.1103/PhysRevB.92.20540910.1103/PhysRevB.92.205409 ↗
15. 10.1103/PhysRevB.90.07540110.1103/PhysRevB.90.075401 ↗
16. 10.1103/PhysRevB.53.1639010.1103/PhysRevB.53.16390 ↗
17. 10.1016/0375-9601(96)00484-710.1016/0375-9601(96)00484-7 ↗
18. 10.1007/s10051005101010.1007/s100510051010 ↗
19. 10.1103/PhysRevLett.89.04660110.1103/PhysRevLett.89.046601 ↗
20. 10.1103/PhysRevB.66.20130610.1103/PhysRevB.66.201306 ↗
21. 10.1103/PhysRevLett.91.15700210.1103/PhysRevLett.91.157002 ↗
22. 10.1103/PhysRevLett.88.19700110.1103/PhysRevLett.88.197001 ↗
23. 10.1103/PhysRevB.69.12532610.1103/PhysRevB.69.125326 ↗
24. 10.1209/epl/i2003-10293-910.1209/epl/i2003-10293-9 ↗
25. 10.1103/PhysRevB.74.21451010.1103/PhysRevB.74.214510 ↗
26. 10.1209/0295-5075/81/4000210.1209/0295-5075/81/40002 ↗
27. 10.1103/PhysRevB.78.22451510.1103/PhysRevB.78.224515 ↗
28. 10.1103/PhysRevB.77.09451210.1103/PhysRevB.77.094512 ↗
29. 10.1103/PhysRevB.82.01451010.1103/PhysRevB.82.014510 ↗
30. 10.1103/PhysRevB.88.09451710.1103/PhysRevB.88.094517 ↗
31. 10.1038/nature0843210.1038/nature08432 ↗
32. 10.1103/PhysRevLett.104.02680110.1103/PhysRevLett.104.026801 ↗
33. 10.1103/PhysRevLett.107.13680110.1103/PhysRevLett.107.136801 ↗
34. 10.1038/ncomms216910.1038/ncomms2169 ↗
35. 10.1088/0022-3719/4/8/01810.1088/0022-3719/4/8/018 ↗
36. 10.1088/0022-3719/5/1/00610.1088/0022-3719/5/1/006 ↗
37. 10.1016/j.physe.2015.10.03110.1016/j.physe.2015.10.031 ↗
38. 10.1103/PhysRevLett.90.06660110.1103/PhysRevLett.90.066601 ↗
39. 10.1103/PhysRevB.76.14450410.1103/PhysRevB.76.144504 ↗