Quantum Computing and Quantum RF Cryogenic Microwave Engineering Informational

How does the thermal noise of components at different temperature stages affect qubit coherence?

Thermal noise from microwave components at different temperature stages of a dilution refrigerator directly affects qubit coherence by introducing photon noise that causes energy relaxation (T1 decay) and dephasing (T2 decay). Each component at temperature T contributes thermal photons at the qubit frequency f according to n_th = 1/(exp(hf/kT) - 1). At 5 GHz: 300K contributes 1249 photons, 4K contributes 16.6 photons, 100 mK contributes 0.42 photons, 20 mK contributes 0.083 photons. The effective noise photon number at the qubit is the weighted sum of contributions from all stages, attenuated by the intervening attenuation: n_eff = sum_i(n_th(T_i) × product_j(10^(-A_j/10))), where A_j is the attenuation between stage i and the qubit. With proper attenuation (60 dB total from 300K to qubit): 300K contribution at qubit = 1249 × 10^-6 = 0.00125 photons. 4K contribution after 40 dB from 4K to qubit = 16.6 × 10^-4 = 0.0017 photons. 100 mK contribution after 20 dB = 0.42 × 0.01 = 0.0042 photons. Total: ~0.007 photons, dominated by the closest (warmest inadequately attenuated) stage. Each residual thermal photon at the qubit frequency drives transitions between |0⟩ and |1⟩, limiting T1 to T1_thermal ≈ 1/(2*pi*kappa*n_residual), where kappa is the qubit-environment coupling rate. To achieve T1 > 100 μs at 5 GHz, the residual photon number must be below ~0.01.
Category: Quantum Computing and Quantum RF
Updated: April 2026
Product Tie-In: Cryogenic Components, Attenuators, Circulators, Cables

Thermal Noise and Qubit Coherence

Understanding the thermal noise budget is essential for achieving state-of-the-art qubit coherence times. Modern transmon qubits with T1 > 100 μs in isolated test setups often show degraded coherence (T1 = 20-50 μs) in multi-qubit systems, with thermal noise from the microwave environment being a contributing factor.

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Common Questions

Frequently Asked Questions

What residual photon number is acceptable?

For state-of-the-art transmon qubits with T1 targets of 100-300 μs: n_residual < 0.01 photons at the qubit frequency is the design target. This ensures thermal photon-induced T1 degradation is at most a few percent of the intrinsic T1. For near-term quantum computing with T1 targets of 30-100 μs: n_residual < 0.05 is acceptable. Current best systems (Google, IBM, Rigetti) achieve n_residual ≈ 0.005-0.02, limited primarily by thermalization of the MC-stage attenuator and IR photon leakage rather than by the attenuation value itself.

How do I verify the thermal photon number experimentally?

Measurement methods: (1) Qubit thermometry: prepare the qubit in the ground state, wait, and measure the excited state population. The steady-state excited population P_e = n_residual/(2*n_residual + 1) directly gives n_residual. P_e = 0.5% corresponds to n_residual ≈ 0.005. (2) AC Stark shift measurement: the qubit frequency shifts by 2*chi*n_residual due to dispersive coupling to the residual photon population in the readout resonator, allowing direct measurement of photon number. (3) Correlation measurements: photon number fluctuations cause random telegraph noise in the qubit frequency, detectable through Ramsey interferometry.

Does thermal noise affect T2 differently than T1?

Yes. T1 is limited by energy-exchange processes (photon absorption/emission). T2 includes both T1 effects and pure dephasing (T_phi). Thermal photon number fluctuations in the readout resonator cause random AC Stark shifts of the qubit frequency (photon shot noise dephasing), contributing to T_phi with: 1/T_phi = 4*chi^2*n_residual/kappa, where chi is the dispersive shift and kappa is the readout resonator linewidth. This dephasing mechanism can be the dominant T2 limitation even when thermal T1 effects are negligible, because it depends on the fluctuations in n rather than the mean value.

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