Quantum Computing and Quantum RF Cryogenic Microwave Engineering Informational

What is the effect of magnetic shielding on the performance of superconducting qubits?

Magnetic fields degrade superconducting qubit performance through several mechanisms: (1) Flux noise causes dephasing in flux-sensitive qubits (flux qubits, tunable transmons). Fluctuating magnetic fields shift the qubit frequency via the flux-dependent Josephson energy: dE_J/dPhi = (E_J * pi / Phi_0) * sin(pi * Phi_ext / Phi_0). Near the flux-sensitive point, a 1 nT field fluctuation at the SQUID loop (area ~100 μm^2) causes a qubit frequency shift of approximately 10-100 kHz, well above the ~1 kHz dephasing rate target. (2) Vortex trapping: magnetic fields above ~1 μT can trap flux vortices in superconducting ground planes, creating lossy normal-metal cores that reduce qubit T1 by 10-100×. The critical field for vortex penetration in thin aluminum films is Phi_0/A_hole ≈ 1 μT for a 1 mm^2 ground plane area without flux-trapping holes. (3) Quasiparticle generation: fields above the critical field of the superconductor suppress the superconducting gap. Shielding strategy uses multiple layers: cryoperm or mu-metal shield (high permeability at cryogenic temperatures, provides 30-50 dB attenuation at DC and low frequencies), superconducting shield (aluminum or niobium can, provides essentially infinite shielding via the Meissner effect below Tc, effective for AC fields and residual DC fields that penetrate the mu-metal). Together, these achieve >60 dB field attenuation, reducing ambient magnetic fields from ~50 μT (Earth field) to <0.05 μT at the qubit chip.
Category: Quantum Computing and Quantum RF
Updated: April 2026
Product Tie-In: Cryogenic Components, Attenuators, Circulators, Cables

Magnetic Environment for Superconducting Qubits

Managing the magnetic environment is one of the most critical aspects of superconducting qubit system design. Even small residual magnetic fields can trap vortices during the superconducting transition, creating persistent dissipative hot spots that permanently degrade qubit performance until the system is re-cooled.

ParameterOption AOption BOption C
PerformanceHighMediumLow
CostHighLowMedium
ComplexityHighLowMedium
BandwidthNarrowWideModerate
Typical UseLab/militaryConsumerIndustrial

Technical Considerations

Mu-metal (Ni-Fe alloy, permeability μ_r = 20,000-100,000 at room temperature): effective for DC and low-frequency (<1 kHz) magnetic fields. Shielding effectiveness for a cylindrical shield: SE = 20*log10(μ_r * t / (2R)), where t is wall thickness and R is radius. A 1.5 mm thick mu-metal cylinder of 150 mm radius: SE ≈ 40 dB. At cryogenic temperatures, standard mu-metal loses permeability. Cryoperm 10 (Vacuumschmelze) is specifically designed for cryogenic use, maintaining μ_r > 30,000 at 4K. Amumetal A4K (Magnetic Shield Corporation) is another cryogenic-grade option. The mu-metal shield should be sized to fit outside the radiation shields of the cryostat, surrounding the experimental volume. Superconducting shields utilize the Meissner effect: superconductors expel magnetic flux from their interior. An aluminum can (Tc = 1.2K) placed inside the mu-metal shield becomes superconducting during cooldown and traps whatever field exists at the transition temperature inside the can. If the mu-metal has reduced the field to <1 μT before the Al transition, the superconducting shield further reduces it to <10 nT through flux expulsion.

Performance Analysis

The magnetic field present during the superconducting transition determines the number of trapped vortices. Critical protocol steps: (1) Degauss the mu-metal shield before cooldown (apply oscillating, decaying magnetic field using a coil wound around the shield). (2) Verify the residual field inside the shield is <1 μT using a fluxgate magnetometer before starting the cooldown. (3) Cool through the superconducting transition temperature slowly (0.1-1 K/minute) to allow vortex motion and potential escape before pinning. (4) Avoid any magnetic field transients during and after cooldown (turn off nearby equipment, secure doors on magnetic latches). (5) On-chip design: include vortex-trapping holes (2-5 μm diameter, spaced 10-20 μm apart) perforated in the ground plane to capture any residual vortices away from sensitive areas. The trapped vortex density scales linearly with the residual field during transition: approximately 1 vortex per Phi_0/B_residual area, or ~50 vortices/mm^2 at 0.1 μT.

  1. Performance verification: confirm specifications against the application requirements before finalizing the design
  2. Environmental factors: temperature range, humidity, and vibration affect long-term reliability and parameter drift
  3. Cost vs. performance: evaluate whether the application demands premium components or standard commercial grades
  4. Interface compatibility: verify impedance, connector type, and mechanical form factor match the system architecture

Design Guidelines

Sources of magnetic field in a quantum computing lab: Earth field (25-65 μT: the dominant source, must be shielded). Nearby equipment (power supplies, motors, compressors: produce 1-100 μT AC fields at power-line frequency). Vibration isolation systems (if using active magnetic compensators, can produce stray fields). Circulator permanent magnets (inside the cryostat, 10-100 mT at 1 cm). Superconducting coils for flux bias (intentional fields, must be carefully shielded from qubits they are not targeting). Building structural steel (magnetized by Earth field, creates field gradients). All of these must be addressed through a combination of distance, shielding, and careful equipment placement in the lab layout.

Common Questions

Frequently Asked Questions

What residual field level is acceptable for qubits?

Target: <0.1 μT (100 nT) at the qubit chip location during the superconducting transition. This limits vortex density to <5 vortices per mm^2 of ground plane, which is manageable with vortex-trapping holes in the chip design. For the most sensitive flux qubits: <10 nT is preferred. Modern systems routinely achieve <50 nT with a combination of cryoperm shield (40 dB) and superconducting Al can (additional 20+ dB). Without shielding (Earth field of 50 μT): approximately 25,000 vortices per mm^2 would be trapped, making the superconducting ground plane highly lossy and reducing qubit T1 to microseconds or less.

Does magnetic shielding affect the dilution refrigerator?

The shield must not interfere with the refrigerator operation: (1) It should not block the mechanical connections to the pulse tube compressor or the still pumping line. (2) It must allow access for wiring and cable feedthroughs. (3) It should not add excessive thermal mass that slows cooldown (a 2 kg cryoperm shield adds approximately 2 hours to the cooldown time). (4) If placed outside the vacuum chamber, the shield does not contact the cold stages and has minimal thermal impact. If placed inside (closer to the qubit), it must be thermally anchored to an appropriate stage. Most systems place the mu-metal shield outside the outer vacuum chamber (OVC) and the superconducting shield at the MC stage, inside the inner vacuum chamber (IVC).

Can I use niobium instead of aluminum for the superconducting shield?

Yes. Niobium (Tc = 9.2K) has a much higher transition temperature than aluminum (1.2K), which means it becomes superconducting earlier during cooldown (at the 4K stage rather than below 1.2K). This is advantageous because the Meissner effect activates while the refrigerator still has significant cooling power to manage any magnetization currents. However, niobium is more expensive, harder to machine, and has a higher lower critical field Hc1 that allows more flux penetration in imperfect thin films. In practice, aluminum cans are more common because they are cheap, easy to fabricate, and sufficient when combined with mu-metal pre-shielding. Some groups use niobium shields on specific qubit packages while using aluminum for the larger enclosure.

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