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Multiquanta flux jumps in superconducting fractal

Mar 23, 2024

Scientific Reports volume 13, Article number: 12601 (2023) Cite this article

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We study the magnetic field response of millimeter scale fractal Sierpinski gaskets (SG) assembled of superconducting equilateral triangular patches. Directly imaged quantitative induction maps reveal hierarchical periodic filling of enclosed void areas with multiquanta magnetic flux, which jumps inside the voids in repeating bundles of individual flux quanta Φ0. The number Ns of entering flux quanta in different triangular voids of the SG is proportional to the linear size s of the void, while the field periodicity of flux jumps varies as 1/s. We explain this behavior by modeling the triangular voids in the SG with effective superconducting rings and by calculating their response following the London analysis of persistent currents, Js, induced by the applied field Ha and by the entering flux. With changing Ha, Js reaches a critical value in the vertex joints that connect the triangular superconducting patches and allows the giant flux jumps into the SG voids through phase slips or multiple Abrikosov vortex transfer across the vertices. The unique flux behavior in superconducting SG patterns, may be used to design tunable low-loss resonators with multi-line high-frequency spectrum for microwave technologies.

Fractal structures with self-similar repetition of topologically identical features at diminishing length scales are universally found in nature (from plant leaves and seashells to blood vessels and neural networks1,2). They are frequently reported in materials studies (from molecular assemblies3 to domain structures in quantum magnets4), and are often employed in technological devices (from compact antenna designs5 to efficient heat exchangers6 and advanced load supports7).

In particular, Sierpinski gaskets (SG), formed by triangles of progressively decreasing size (the fractal recursive rule is illustrated in Fig. 1) offer unique electromagnetic response desirable for advanced microwave applications8,9. Their parameters essentially can be improved using loss-less superconducting materials, in which case the SG becomes a multiply connected superconductor (SC) with different scale array of voids. Prior studies of SGs comprised of SC wires or wires with Josephson Junctions which showed distinct hierarchical and repetitive changes in resistivity and inductance of the samples in applied fields near the SC transition temperature (Tc)10,11,12,13,14,15. These samples were lattices of Sierpinski gaskets up to 6th order with elementary triangles of submicron or a few micron size. In small applied magnetic fields, it was possible to successively fill different triangular subsets composing the SG with individual magnetic flux quanta, Φ0 = πħ/e. The hierarchy of flux filling, resulting in sharp changes of Tc or inductance of the SG arrays, followed digital flux quantization rules, NΦ0 → (N ± 1)Φ0, commonly reported for multiply-connected superconductors, with specifics imposed by the fractal pattern geometry. For experiments close to Tc, the data analysis is simplified due to negligible Meissner screening, resulting in homogeneous magnetic field distribution (see10,11,12,13,14,15,16 and refs. there). However, at low temperatures (T), where losses are desirably minimized, the screening effects become important and the magnetic field is modified by SC persistent currents. Moreover, due to increased critical currents at low T, the flux entry into the samples is strongly delayed and may depend on the dynamics of phase slips or entry of Abrikosov vortices which can transfer single or multiple flux quanta into the voids inside the superconductor.

(a) Picture of a 3d-order Sierpinski gasket (SG) consisting of 100 nm thick Nb film equilateral triangular patches (bright) with triangular voids (dark) of proportionally decreasing size marked as TV1 (1 mm side) to TV4 (125 µm side). The insert shows the expanded view of 1 µm bridges between the Nb patches. (b–f) Magneto-optical images of a few successive flux jumps in triangular voids of the SG with increasing magnetic field Hza applied perpendicular to the sample plane at T = 3.5 K. The strength of contrast in the MO image inside the TVs and at their boundaries corresponds to the strength of the normal field induction Bz. Short arrows in (b) point to the enhanced positive Bz (B↑↑Hza, bright) at the vertices of the internal TVs caused by the distributed Meissner currents in the SG. Long arrows in (b) show increased negative Bz (B↓↑Hza, dark) near the vertices of TVs abutting the sample’s edge. Bright contrast lines along the outer periphery of the sample reveal the enhanced edge field due to the screening effect similar to that in a continuous SC triangle. Consecutive instant flux jumps in the TVs begin with the largest central TV1 and proceed to smaller TVs. Numbers in (b–f), indicate the sequence of flux filling order of the TVs. The order of flux filling from large to small TVs is sometimes disrupted by early flux entry into the smallest TVs. Likewise, with increasing field, periodic flux entry into the largest TV may repeat several times before the flux entry occurs in smaller TVs (see the second round of jumps into TV1 and TV2 marked as 1 + in (e), and 2 + in (f)).

In this work we directly image the magnetic flux entry in a millimeter sized Sierpinski gaskets comprised of equilateral superconducting triangles encasing sequentially decreasing triangular voids. We find that at temperatures well below Tc, flux behavior is characterized by consistent well-structured hierarchical succession of multiquanta flux jumps. The flux entry is qualitatively similar to single-quantum-flux jumps observed in microscopic SG patterns at T ~ Tc. However, unlike such single-Φ0 representative of Little-Parks oscillations, in our samples at T ~ Tc/2 the repeating flux jumps consist of thousands of Φ0, depending on the size of the triangular voids in the SG structure. Also, the imaged inhomogeneous field distributions induced by SC persistent currents affected by the flux jumps, reveal interactions between different flux cells, sometimes resulting in combined positive and negative jumps in the neighboring voids of the SG.

We envision that our superconducting SG patterns, where changes of inductance, caused by the redistribution of currents due to orderly flux jumps controlled by small magnetic fields, can shift the SG eigen-frequencies, and hence can be used as tunable low-loss multiline resonators for quantum IT devices and sensors. In turn, a wide set of possible combinations of diverse NsΦ0 flux bits trapped in the 2D array of different SG triangular voids could be employed for advanced digital recording.

We used the magneto-optic indicator technique (MOI)17 to image the magnetic flux penetration in an equilateral triangular SG structure with maximum triangle side of 2 mm fabricated from a 100 nm niobium film with superconducting (SC) transition temperature Tc = 8.75 K, grown by high-vacuum magnetron sputtering. A Sierpinski gasket obtained after successive removal of progressively decreasing triangular areas while leaving narrow 1 µm bridges between vertices of the remaining triangular SC patches is shown in Fig. 1. In SG structures made of thin wires, the 0-order gasket is a simple equilateral triangle and the order increases upon successive addition of wires connecting the centers of the larger triangle sides. In our case the 0-order gasket corresponds to three triangular patches surrounding the central triangular void. The equivalence with the 0-order wire gasket is that we similarly begin with one hole in the SC structure. Below we present the main results for our highest 3d-order SG pattern (Fig. 1a), which is formed after an eightfold reduction of the largest triangular void, yielding the smallest triangles with 125 µm sides.

The macroscopic magnetic response of the samples in a magnetic field was measured using SQUID magnetometry, and the flux distributions at T < Tc were observed using MOI. The samples were mounted on a cold finger of a commercial Montana cryostat and covered by an indicator film with a large Verdet constant to spatially visualize the normal magnetic field at the sample surface, Bz(x,y), in polarized light. Careful calibration of image intensity versus applied normal field Hza at T slightly above Tc allows accurate quantitative assessment of induction distributions in the sample.

We start with demonstration of the magnetic flux entry in our 3d-order SG structure using a set of MOI pictures obtained by gradually increasing the applied field, Hza, where the image intensity corresponds to the local strength of Bz. Quantitative changes of local Bz within various triangles in our SG samples will be presented below as Bz(Hza) plots.

Figure 1b–f show successive evolution of the Bz map in the sample with increasing Hza in steps of ΔHz ~ 0.03 Oe at T = 3.5 K. At this temperature, the magnetic field ≲ 0.4 Oe is mostly screened from the entire sample by Meissner currents JM (Fig. 1b). Bz increases only outside the peripheral of the sample as expected in a continuous SC triangle. However, peculiar weak Bz features concurrently appear inside the sample along the contours of all triangular voids (TVs). Specifically, small negative Bz↓↑Hza (dark contrast as opposed to bright Bz↑↑Hza) is observed at the sides and in the vertices of the TVs located adjacent to the outer-edges of the SG sample as marked by longer arrows in Fig. 1a (see also enlarged images in Fig. A1 of the Supporting Info).

Another peculiarity, a slightly enhanced positive Bz (bright contrast), emanates from the vertices of the smallest voids, TV4, at the sides of larger internal TVs as marked by short arrows in Fig. 1b. These features appear due to the unidirectional screening currents JM distributed over triangular patches of our SG. In the Meissner state, in a multiply connected SC structure with a single hole, such as a ring, the screening current, JM, is concentrated near the inner and outer ring edges but has the same polarity across the ring’s width18,19,20,21. As a result, the applied field is enhanced at the outer ring edge, while the local negative (opposite to Hza) field appears at the inner edge (see Fig. A2 in Supporting Info). Further inside the hole, the field reverses sign again and a small positive Bz forms in the center, but the total flux over the entire ring area is smaller than Φ0 and the ring remains in the Meissner state. The sketch of the JM distribution in SG structures following the above scenario, which explains details of the Meissner Bz map observed in our samples, is shown in Fig. 2a. The time dependent Ginzburg–Landau (TDGL) solution for the current distributions in the SG is presented in Fig. A3 of the Supporting Info.

Sketch of the current trajectories (red lines with arrows) and current induced fields (small circles with red dots and blue crosses for Bz pointing Up and Down respectively) in 0th-order superconducting Sierpinski gasket in the Meissner state (a) and after the magnetic flux jump inside the triangular void (b). Bottom panels illustrate the current pattern around the narrow bridges linking the triangular SC patches in the SG.

With slow increase of Hza, the above described features remain qualitatively unchanged although their contrast slightly increases. Then, at Hza ~ 0.4 Oe the magnetic flux suddenly jumps into the large central TV1 (Fig. 1c) where the enhanced bright contrast at the edges signify Bz > Hza. The Bz contrast at the sides of TV1 changes from dark to bright, indicating the inversion of the current direction near these edges. Consequently, the local SC current here, responds to the injected flux Φ1 instead of just screening the applied field Hza. Appropriate sketch of the changed current distribution is shown in Fig. 2b (the TDGL solution is presented in right panel of Fig. A3 of Supporting Info). The total flux in the central TV1, estimated using measured Bz in the triangle at Hza ~ 0.4 Oe and the triangle area, is ΔΦ1 ~ 6600 Φ0 (see details below).

(a) Numerical order of the sequence of first flux jumps into the triangular voids (TVs) of the Sierpinski gasket with increasing applied field Hza. (b) Dependence of the flux filling sequence (from TV#1 to TV#40, left ordinate) on the magnetic field Hza (red dots). Blue squares show the side length s of the appropriate TVs (right ordinate) indicating the major tendency of the flux entry, from the largest to the smallest triangles. Arrows mark fields of the first flux entry in successively smaller triangular voids, from Hc1(1) for s = 1 mm to Hc1(4) for s = 125 µm.

With further increasing field, the jump-wise flux filling occurs in the next smaller sized, TV2 (s = 0.5 mm) marked as 2–3–4 in Fig. 1d. TV2-#2 and -#3 are filled simultaneously and TV2-#4 is filled at slightly larger Hza. The abrupt flux jumps are accompanied by the dark-to-bright reversal of contrast at the TV2 edges, as described above for TV1. Following the jump, the field in TV2 is higher than Bz in TV1 but the flux change is smaller (ΔΦ2 ~ 2600 Φ0) due to the smaller triangle area.

After the flux enters the set of TV2, the next smaller TV3 voids (#5, 6, 7…, s = 0.25 mm) begin to fill with magnetic flux at Hza > 0.8 Oe (Fig. 1e). Flux jumps in voids of TV3-set progress at small field intervals, sometimes in pairs of TVs, but not simultaneously in all TV3 voids. In some cases, during the process of filling the smaller TVs, the additional flux jumps occur in larger TVs where the total flux is repeatedly increased by the same value of ΔΦi (see TV1 after the 2nd jump marked “1 + ” in Fig. 1e, and “2 + ” for TV2 in Fig. 1f). With further increasing field, at Hza > 1.32 Oe, slightly before all TV3 voids are filled, the next smaller set of voids (TV4, s = 0.125 mm, #12, #13 and so on) begin filling (Fig. 1f). In some cases, they fill in pairs with TVs of the same or different size, and the succession of appropriate filling steps is intermittent with incremental ΔΦi jumps in larger TVs.

Finally, following multiple repeated flux jumps in larger voids, all 40 TVs in the SG are filled with flux at Hzap ~ 2.9 Oe. The sequence of filling presented in Fig. 3 shows how the first flux jump occurs in each of the TVi upon increasing Hza. Clearly, the field of the initial flux jump, and the range of fields required for filling all the TVi of the same size s, increases with decreasing s. With further increase in Hza, additional flux jumps repeat periodically in all the TVi. Eventually, after the triangular voids are filled, Abrikosov vortices start entering the SC patches at relatively large fields Hza > 22 Oe (Fig. 4).

(a) Entry of Abrikosov vortices into the superconducting areas of the Sierpinski gasket. All the triangular voids are filled with magnetic flux (bright contrast) and vortices start penetrating the flux-free (dark) Nb triangles. MOI taken at T = 3.5 K, Hza = 32.7 Oe. Right panel (b) shows the expanded view of the boxed fragment on the left. Arrows point to flux balloons of multiple vortices penetrating from all edges of the superconducting triangles.

Important details of the changing current patterns during the flux jumps in our samples are revealed by difference images presented in Fig. 5. They are obtained by subtraction of sequential Bz images before and after the flux jump and represent increments of ΔBz(x,y) = Bz(Hza + 0.03 Oe)-Bz(Hza) corresponding to appropriate changes of the currents ΔJ (x,y) during the jump. Figure 5 shows that the flux jumps ΔΦi in any sized TVi yield qualitatively the same picture of a homogeneous ΔBz over the main TVi area with enhanced positive ΔBz at the TVi periphery. Pronounced contrasting features emerge in three neighboring triangular regions around the TVi. They have the same size as TVi, but contain smaller triangular voids surrounded by SC patches. Together with the central TVi where the flux jump occurred (brightest contrast), these neighbors make up the Sierpinski sub-gaskets (sub-SG) of a lower order. Such smaller sized sub-SGs of order 2, 1 and 0 are isolated with dashes in Fig. 5b,c,e, respectively.

Difference images, obtained by subtraction of Bz-maps preceding and following the flux jump in different sub-SGs, revealing the abrupt change of the sub-SG current flow pattern. In (a), the enhanced bright contrast (ΔBz > 0) along the edges of the central triangular void (TV1) corresponds to the inversion of the screening currents JM near these edges to support the trapped flux in TV1. In turn, the stronger dark contrast along the boundaries of the entire sample (ΔBz < 0) shows a noticeable drop in JM there. Qualitatively similar difference patterns are observed after flux jumps in smaller TVis. They show ΔBz changes well localized within appropriate lower order sub-SGi due to the current inversion at the TVi edges and decreased currents at the sub-SGi boundaries. In panels (b), (c), and (e) the 2d, 1st, and 0-order sub-SGis are encircled by dashes. Similar ΔBz changes repeat after second and further jumps in the same TV (compare e.g. (a) and (d) or (b) and (h)). The distributed Meissner currents, which spread over the sub-SGi area define slight increase or decrease of Bz at the vertices and along the sides of smaller TVs inside the sub-SGi in all pictures. More complex patterns appear during rare negative jumps (dark triangles in (h)–(i) pointed by arrows) which are accompanied by a partial positive jump in neighboring TVs.

The ΔBz patterns show that after the flux jumps into a TVi, the screening currents JM in the SC patches surrounding the TVi are inverted along the edges of the TVi and also along the sides of the smaller TVs making up the sub-SGi structure. At the same time, JM is noticeably reduced at the sub-SGi’s outer boundary. The picture corresponds to the changes from pattern (a) to (b) in current distributions sketched in Fig. 2. Note that for successive jumps in the same TV taking place with increasing field, the difference pattern remains the same (compare Fig. 5a and d) confirming the replicability of the repeated flux jump cycle. Also, at Hza beyond the jump field, the sub-SGi Bz-maps (not shown) restore the pre-jump features qualitatively similar to Fig. 1b and reveal the reemerging screening current distribution akin to the Meissner state pattern sketched in Fig. 2a.

In addition to successive flux jumps with increasing Hza, at larger fields we observe unexpected local negative flux jumps, as illustrated by dark triangles (ΔBz < 0) in Fig. 5h–i. Here, the negative ΔBz in prior flux filled TVs is accompanied by a partial positive ΔBzp in their neighbors (larger brighter triangles near dark triangles in Fig. 5h–i), which is smaller than their regular ΔBz flux jump value. In this case, the flux redistributes by jumping between neighboring TVs due to their magnetostatic coupling assisted by the change in current in the surrounding SC patches. It is different from purely magnetic coupling between electrically insulated SC rings observed in22.

To quantitatively analyze the magnetic flux evolution in our SG pattern, we measured the MOI signal (IMOI) averaged over the area of individual TVs, and transformed IMOI into a median \({\overline{B} }_{z}\) value for the triangle using IMOI(Bz) calibration. Multiplying the obtained \({\overline{B} }_{z}\) by the triangle area we obtain the magnetic flux Φi acquired by the TVi. Figure 6 shows a set of characteristic \({\overline{B} }_{z}(\)Hzap) plots for TVs of all four sizes composing the SG. The \({\overline{B} }_{z}\) steps in different TVis are periodic. They have basically the same amplitude and are separated by identical field gaps ΔHza between jumps. The height of the jumps Δ \({\overline{B} }_{z}\) increases with decreasing the TVi size.

(a–d) Changes of median normal induction Bz in different size triangular voids of the Sierpinski gasket with increasing field Hza at T = 3.5 K. The insert in (a) shows the measurement areas for estimating the median Bz in TVs. Successive flux jumps fill the TVs by repeating values of ΔBz in field intervals ΔHza which increase with decreasing s. Bz scales in the plots are different. The jump fields Hza slightly vary for same size TVs. There is a small difference in ΔBz, most noticeable in the smallest TVs, possibly due to imperfections in the narrow bridges between niobium patches. Note the small slope in Bz(Hza) between the steps as expected in superconducting rings within the London approach.

There is a slight variation in Δ\({\overline{B} }_{z}\) among different triangles of the same size, especially in the smallest TV4 (Fig. 6d). This can be due to a small difference of the vertex joints between the SC patches in the structure, which are also responsible for the observed scatter in the first flux jump field for same sized TVs shown in Fig. 3b. Also, the recurrence is disrupted in rare cases of negative or partial flux jumps, when the flux rearranges between neighboring TVs and Δ\({\overline{B} }_{z}\) reaches ~ 1/3–1/2 of its regular value (see Fig. A4 in the Supplemental Info).

The distribution of successive flux jump amplitudes ΔΦi in TVis of different sizes, obtained from Δ\({\overline{B} }_{z}\) as those in Fig. 6, is presented in Fig. 7. Here, the average ΔΦi decreases with s from ~ 6600Φ0 for the largest TV1 to ~ 650Φ0 for the smallest TV4. Some scatter among successive ΔΦi in the same TVi is within accuracy of our measurements. Note that the ratio of TV areas Si ~ s2 in our SG is 1:4:16:64, while ratios of the flux jump values in these TVs (in units of Φ0) are ~ 650:1350:2650:6600 (~ 1:2.1:4.1:10.2), i.e. ΔΦi changes practically linearly with s (logΔΦ-logs fit gives ΔΦ ~ s1.131). Assuming that the SC currents, screening the applied field or Bz in the TVi due to flux jumps, are concentrated along the sides of the SC triangular patches and at their vertex links, we can model the individual sub-SGs as narrow rings with effective radius R = (rinRci)1/2 = s/61/2, intermediate between the inscribed (rin) and circumscribed (Rci) circles confining the TVi. The ring width was chosen as w = 1 µm, corresponding to the width of the bridges between all triangular patches. Appropriate values of inductance L of four of our sub-SGs calculated using formula for narrow rings18, L = µ0R[ln(8R/w) − 2 + ln4], shown by squares in Fig. 8, are consistent with measured mean values of ΔΦi (round dots) in TVs of different size. This indicates that the inductance of the sub-SGs defines the size of the flux jumps in their central voids.

Amplitudes of flux jumps, ΔΦ, in different triangular voids of the Sierpinski gasket at T = 3.5 K. ΔΦ are obtained from measurements of Bz(Hza) after multiplication by the triangle area. Note different ΔΦ scales in the plots.

Measured average values of flux jumps ΔΦ in the triangles of different size s (red dots) and calculated inductance (blue squares) of narrow rings with geometrically mean radius between circles inscribing and circumscribing the triangle and the same width as the bridge between triangles (see main text).

Experiments on superconducting Sierpinski samples were previously realized on periodic lattices of different order SGs with basic triangles of narrow few-micron long SC nanowires10,11,12,13 or similar samples containing Josephson junctions in the wires14,15. Macroscopic transport and susceptibility measurements on these samples revealed a rich hierarchy of sharp changes of the transition temperature, Tc(Hza), and inductance, L(Hza), corresponding to the complex filling of different size triangles composing the SG with single flux quanta. The theoretical treatment of these results was usually based on the Ginsburg-Landau (GL) equations13,14,15,16,23,24,25 assuming the homogeneous magnetic field distribution, i.e. neglecting the SC screening fields. Basically, the superconducting nature of the samples was accounted through the field dependent phase relations of the SC order parameter, which dictate the flux quantization in multiply connected samples. In the case of SG, the flux quanta are predicted to enter the n-order SG with elementary (minimum size) triangles of area A0 at fields H > Hc = Φ0/(4nA0)16. In our SG formed by SC patches, A0 is the area of the smallest triangular void, yielding Hc ~ (1/4n)3 × 10–3 Oe, which is much smaller than the observed flux entry fields (~ 0.37 Oe for the 1st flux jump in the central triangle), while the values of flux jumps we measure are much larger than Φ0. At the same time, theoretical expectation for successive flux entry, starting from the largest triangle and proceeding to smaller triangles with increasing Hza, is consistent with our observations (compare our Fig. 3 and the diagram of the flux filling sequence in Fig. A5 of Supporting Info, which is plotted using calculations of16). However, in our case, the succession of flux entry in different sub-SGs is defined by a distinct mechanism which we discuss below.

Obviously, in our samples at T < Tc/2 the screening effects are important. Under these conditions, the flux penetration into TVs should occur either through phase slips or by the transit of Abrikosov vortices across the 1 µm bridges connecting the triangular SC patches. Flux penetration occurs when the screening current in these bridges acquires a critical value Ic. The screening currents flowing over the patches converge in the narrow bridges yielding there the enhanced current density, and with increasing Hza, the total current reaches Ic first in these regions. The resulting phase slips or moving vortices temporary suppress the SC order parameter |Ψ| near the vertices of the central TVis in the sub-SGs and provide channels for flux entry. Clearly, the largest current is initially achieved (see Fig. 2a) around vertices of the largest TV1 (#1 in Fig. 1) where the first jump occurs. This is then followed by flux jumps into smaller TV2-4, and so on, as we observe in our samples.

To understand the regularity and large values of the flux jumps in different TVis in the SG, we presume that the sub-SGs can be considered as inhomogeneous SC islands with a large hole in the center and revisit prior theories of flux quantization in SC rings. For SC rings smaller than the penetration depth λ and with outer radius R of a few ξ, the magnetic field response was widely studied using analytical and numerical solutions of static and time dependent Ginzburg–Landau (TDGL) equations21,26,27,28,29,30,31,32,33,34,35,36,37,38,39. These works explained many experimental observations of sharp changes in the microscopic SC ring properties due to the periodic entry of single flux quantum Φ0, such as oscillations in Tc, resistivity, susceptibility, inductance, and heat capacitance29,30,37,40,41,42,43,44.

However, computer simulations of TDGL equations21,31,33 accounting for different relaxion times of the phase (τφ) and amplitude (τ|Ψ|) of the SC order parameter in relatively large rings (R ≳ 10ξ) showed that transitions between many metastable states with different vorticity Lv can yield ΔLv >  > 1 (e.g. ΔLv up to 9, i.e. ΔΦ = 9Φ0, for R = 15ξ31). These transitions repeat at appropriately large field steps (ΔH). They occur if τ|Ψ|> > τφ through phase slips with complicated temporal and spatial variation of φ and |Ψ| depending on the values of relaxation parameters, radius and width of the ring, and ξ, when the gauge-invariant momentum of the SC pairs reaches a critical value pc (i.e. at a critical current)31,33,35,36.

In earlier experiments, giant flux jumps with ΔLmax = 11 at Happ < 40 Oe and gradually decreasing ΔL at larger fields were found in narrow 4µm Al ring at T < Tc/345. ΔL = 3 jumps were reported for 2µm Al rings33. Later, giant flux jump transitions between metastable SC states with ΔLv up-to 70 were detected through sharp changes of the low-T tunnel current in narrow 25 µm square Al rings with a normal electrode in one corner34,46,47.

The most intuitive and clear picture of flux quantization in multiply-connected SC samples appears in the London description of the induction and current pattern variations in rings18,19,20,48,49. Unlike the GL formalism, which is mostly applied to mesoscopic rings, the London description is based on electrodynamics equations appropriate for any sample size, while anchoring the flux quantization requirement that maintains the coherent state in the SC material of the ring.

For thin SC rings with dimensions much smaller than the Pearl length (Λ = 2λ2/d for ring thickness d << λ), where one can neglect the field induced by the screening currents, the periodic flux entry was explicitly described in49. Transitions between states with N and N ± 1 flux quanta in the ring were suggested to occur via the nucleation of Abrikosov (or Pearl for d << λ) vortex or antivortex, either at the outer or inner ring edge, and its motion across the ring width, thus adding or removing one Φ0 in the ring annulus. The barrier for this process is defined by the vortex nucleation field. Interestingly, at some fields H ~ (N1 + N2)/2 the energy for N1 and N2 states with |N1 − N2|> > 1 is the same, which could in principle allow large changes of vorticity in the ring.

For large SC rings, where the self-induction contribution becomes important, and where the flux jumps with large vorticity were predicted by the GL calculations, the accurate description of the magnetic response accounting for the self-field induced by the Meissner current was given in19,20. The combined solution of Maxwell and London equations showed that the screening currents of the total Meissner state at small applied fields are concentrated near the inner and outer ring edges and have the same sign across the entire ring width. They yield a small induction in the ring annulus, with total flux of less than a flux quantum. At larger Hza, when the flux Φ = NΦ0 (N ≥ 1) jumps inside the annulus, the screening current at the inner ring edge changes direction to support Φ, and with further increasing field, the Meissner screening current pattern restores itself until the next flux entry. This picture corresponds to changes of the MOI patterns observed around different voids in our SG samples.

In20 Brandt and Clem calculated the SC ring energy in a homogeneous applied field Ha = Ba/µ0, accounting for the screening currents j in the presence of a fluxoid inside the ring and the fields Bj induced by these currents:

Here, the first term is the energy of the total field B = Ba + Bj and the second term is the kinetic energy of the currents. The total current and vector potential were divided into parts driven by the fluxoid and by the applied field respectively (details are described in the Supplemental Info). Finally, the Gibbs potential G = E − mBa/2 was obtained, which describes the state of the ring accounting for the Ba source inducing the magnetic moment m in the ring. Depending on the applied field, minima of G defined stable flux values in the ring annulus with neighboring states distinct by ± 1Φ0.

If we approximate the sub-SGi containing central triangular void TVi with side length s as narrow ring with effective radius R = (rinRci)1/2 = s/61/2 and follow the same calculations as in20 (see Supporting Info S1) we obtain the Gibbs potential responsible for the number, N, of flux quanta in the TVi (omitting the constant homogeneous applied field contribution):

Here Aeff = πR2 = (π/6)s2 is the effective area of the TVi in the sub-SGi and C = [tanh−1(a/b) − 1 + ln4] comes from the inductance of a narrow ring of width w, inner radius a = R − w/2, and outer radius b = R + w/2. The minima of GN correspond to the multiquanta states defined by Aeff and Ba. However, transitions between different states are delayed until Ba reaches a characteristic value allowing either phase slips or nucleation and transit of Abrikosov (Pearl) vortices across the narrow bridges in the corners of the TVi. These fields are reached when the total screening current in the bridge acquires a critical value Ic, which yields the flux jump in the TVi: Φ = NΦ0 = Ls-SGIc (Ls-SG is the inductance of the sub-SG). After the flux jump, the total current in the bridge vanishes (− jΦ screening the fluxoid inside TVi and + jH screening the applied field compensate each other). With further increasing Ba, jH restores the Meissner distribution over the entire bridge until the total current reaches Ic again and an additional fluxoid Φ = NΦ0 jumps in. In small fields, as in our experiment, which do not affect the critical current, the jumps should be periodic in field, repeating in steps of ΔBa = Ls-SGIc/Aeff.

Similar 1 µm bridges in TVis of all our sub-SGs, should have the same Ic. However, due to the hierarchical current flow in the entire sample, the critical current is first achieved near the vertices of the largest TV1. After the flux enters the largest TV1 and the total current through it’s bridges vanishes (∫(jH-jΦ)dr = 0), the current trajectories form closed loops in the three neighboring smaller sub-SGs and reach Ic at their respective TVi bridges with further increasing Ha, resulting in subsequent flux jumps in these TVis. Similar scenario repeats for the next smaller sub-SGs. The flux jumps for smaller structures occur between repeating jumps in larger sub-SGs.

From our data, we can not specify whether the flux jumps in the SG occur due to the phase slips39,50,51 or due to the vortex transfer48 across the narrow bridge at the vertices. However, quantitative estimates show a faint probability of phase slips in our samples: P ~ exp(− ΔF/kBT) with the barrier height ΔF ~ 104 kBTc and appropriate critical current density Jc ~ 2MA/cm2 (see Supporting Info S1). At the same time, Jc values obtained from transport measurements of sputtered ~ 100 nm Nb films similar to ours52 suggest a high probability of vortex transfer across the SG bridges.

Note, that the succession of giant flux jumps, from largest to smallest sub-SGs, is similar to jump-wise single-Φ0 filling of mesoscopic SG numerically calculated within the Ginzburg–Landau approach16 (see Fig. A4 in Supporting Info). However, in16, where the screening fields are neglected, the flux entry in different sub-SGs is mostly defined by the fluxoid quantization over the sub-SG area in slowly increasing applied field and recurrent current/electric field relations in the SG wire network. In our case, the giant fluxoid entry threshold is defined by the critical current in narrow bridges at the vertices of the sub-SG in the presence of screening effects. Our Gibbs potential analysis models the sub-SGs as independent rings and does not account for their mutual interactions which can be envisioned as magnetostatic coupling between the fluxoids entering different TVs. In our samples we observed a few cases of the flux redistribution between neighboring sub-SGs during separate jumping events (Fig. 5h–i) which are defined by these interactions. However, they were very rare and the individual ring picture seems to capture the main features of the giant flux jumps we imaged.

In this work, we directly imaged periodic multiquanta magnetic flux jumps in hierarchical fractal-like patterns of superconducting triangular Sierpinski gaskets. Unlike in earlier experiments addressing magnetic oscillations of Tc and inductance in Sierpinski structures of microwires or SG networks of Josephson junctions, we studied SG samples of triangular niobium patches with 1 mm to 125 µm sides and directly observed discrete flux filling among proportionally decreasing triangular voids in small perpendicular magnetic fields at low temperatures.

The succession of flux jumps into central triangular voids, TVi, of composing the sample sub-gaskets starts with the largest SG and proceeds to sequentially smaller sub-SGs with increasing field. We associate the orderly flux entry into our multiply-connected fractally designed superconducting sample with the controlling role of narrow bridges between continuous SC patches. Here the screening currents converge and with increasing applied field, periodically reach the critical current value, thereby allowing phase-slips or Abrikosov (Pearl) vortex transfer to fill the TVi with multiple flux quanta, NΦ0. Considering different sub-SGis, independently, the fluxoid vorticity N is proportional to the inductance Ls-SG of the sub-SGi, which can be approximated by a narrow ring of the order of sub-SGi TVi size s, so that Ns-SG ~ s. In turn, the field periodicity of flux jumps ΔHa ~ 1/s.

We observe changes of the current patterns during the flux jumps when the screening current around the TVi reverses its direction. The flipped current may compensate the Meissner current induced by Ha and the total SC current in the TVi joints vanishes, allowing larger current collection at the narrow bridges of smaller TVs and enabling their flux filling. Eventually, multiquanta flux jumps repeat, alternating between large and small sub-SGs where appropriate Ns-SG enter at appropriate Ha.

We anticipate that the superconducting Sierpinski structures, where regular giant flux jumps are induced by small applied magnetic fields, may be used for designing low-loss tunable resonators for information and communication technologies. Fine changes in the inductance of the SG pattern due to the controlled fast flux entry in separate sub-SG can allow controlled switching in high frequency operations, in/out signal delivery, and exchange between elements of quantum electronics devices (sensors, amplifiers, memory cells, and computer nodes). The characteristic zero-field frequency response can be adjusted by the SG size and form a wide band of resonance lines depending on the SG order.

The samples were fabricated by lift-off procedure of 100 nm niobium film deposited with high vacuum DC magnetron sputtering on a photoresist pattern prepared using laser lithography on a silicon wafer. The accuracy of all 1 µm bridges between triangular patches forming the resulting niobium SGs was inspected in an optical microscope using 100 × objective.

The silicon chips with niobium SG structures were mounted on the cold finger of specially designed optical castle in a helium closed cycle Montana cryostat. A magneto-optical indicator with large Verdet constant was placed on top of the samples, allowing images of the normal magnetic field distributions Bz(x,y) on their surface in a polarized light microscope. To improve the signal/noise ratio, the magneto-optical images were accumulated using multiple-exposures in a digital 16 bit camera with cooled 1024 × 1024 CCD array. The image intensities I(x,y) were transformed into the Bz(x,y)-maps using accurate B-I calibration obtained slightly above the superconducting Tc. Digital operations with images were performed using image processing software.

The description of TDGL simulations of the current distributions in the large Sierpinski gasket without and with magnetic fluxoid in the central triangular void are presented in the Supporting Info, where we also show details of our London calculations of the sub-SG Gibbs potential defining the giant flux jumps in our samples.

The datasets obtained and/or analyzed during the current study are available from the corresponding author on reasonable request.

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This project was supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering. Work performed at the Center for Nanoscale Materials, a U.S. Department of Energy Office of Science User Facility, was supported by the U.S. DOE, Office of Basic Energy Sciences, under Contract No. DE-AC02-06CH11357.

Materials Science Division, Argonne National Laboratory, Argonne, IL, 60439, USA

Vitalii K. Vlasko-Vlasov, Ulrich Welp, Andreas Glatz & Wai-Kwong Kwok

Center for Nanoscale Materials, Argonne National Laboratory, Argonne, IL, 60439, USA

Ralu Divan & Daniel Rosenmann

Department of Physics, Northern Illinois University, DeKalb, IL, 60115, USA

Andreas Glatz

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V.K.V.-V. designed the samples, implemented the MOI study, analyzed the results, suggested the explanation, wrote the paper; R.D. and D.R. fabricated the samples; U.W. performed macroscopic characterization of the samples and participated in writing the paper; A.G. prepared and implemented the TGDL simulations of the current and field distributions in the S.G.; W.-K.K. analyzed the results and wrote the paper.

Correspondence to Vitalii K. Vlasko-Vlasov.

The authors declare no competing interests.

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Vlasko-Vlasov, V.K., Divan, R., Rosenmann, D. et al. Multiquanta flux jumps in superconducting fractal. Sci Rep 13, 12601 (2023). https://doi.org/10.1038/s41598-023-39733-y

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Received: 27 April 2023

Accepted: 30 July 2023

Published: 03 August 2023

DOI: https://doi.org/10.1038/s41598-023-39733-y

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