Chirality and spin transformation of triplet Cooper pairs upon interaction with singlet condensate
We show that the fully polarized triplet s-wave component is characterized not only by the spin direction, but also by chirality. Interaction of a polarized triplet component and a singlet one results in creation of triplet Cooper pairs with opposite spin direction or of different chiralities. Such...
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Veröffentlicht in: | Physical review. B 2015-12, Vol.92 (21), Article 214510 |
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Sprache: | eng |
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Zusammenfassung: | We show that the fully polarized triplet s-wave component is characterized not only by the spin direction, but also by chirality. Interaction of a polarized triplet component and a singlet one results in creation of triplet Cooper pairs with opposite spin direction or of different chiralities. Such spin transformation leads to interesting phenomena in multiterminal magnetic Josephson junctions. We calculate the dc Josephson current I sub(J) in a multiterminal Josephson contact of the S sub(m)/n/S' sub(m) type with "magnetic" superconductors S sub(m) that generate fully polarized triplet components. The superconductors S sub(m) are attached to magnetic insulators (filters) which let pass electrons with a fixed spin direction only. The filter axes are assumed to be oriented antiparallel to each other. The Josephson current is zero in two-terminal Josephson junction, i.e., in S/n/S sub( m) or in S sub(m)/n/S' sub(m) contact. But in the three-terminal Josephson junction, with another S superconductor attached to the normal wire, the finite current I sub(J) appears flowing from the S superconductor to S sub(m) superconductors. The currents through the right (left) superconductors S sub(m) are opposite in sign, I sub(R) = I sub(J) = I sub(c) sin ([chi] sub(R) + [chi] sub(L) - 2[chi]) = -I sub(L), where [chi] sub(L/R) and [chi] are the phases of superconductors S sub(m), S' sub(m) and S, respectively. We discuss possibilities of experimental observation of the effect. |
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ISSN: | 1098-0121 2469-9950 1550-235X 2469-9969 |
DOI: | 10.1103/PhysRevB.92.214510 |