The present invention relates to the field of electronic signal amplification, in particular to ultra-low noise cryogenic microwave amplification.
The approaches described in this section are approaches that could be pursued, but not necessarily approaches that have been previously conceived or pursued. Therefore, unless otherwise indicated, it should not be assumed that any of the approaches described in this section qualify as prior art merely by virtue of their inclusion in this section.
Quantum-level signals at microwave frequencies require ultra-low temperature operations. For example, the required temperature may vary from 10 to 100 millikelvin, because the energy of thermal noise kBT of the environment has to be much lower than the energy of a single quanta ℏω at a microwave frequency (microwave photon), where kB is Boltzmann's constant (=1.38×10−23 J/K=1.38×10−23 m2kgs−2K−1), ℏ the reduced Planck's constant (1.05×10−34 m2 kg s−1). Accordingly, for the 5 GHz microwave, the corresponding temperature is,
Because of the low energy of microwave signals at the quantum level, amplification of microwave signals, especially low-noise amplification, at millikelvin environments is extremely challenging. However, such amplification is very important, if not necessary, for quantum computing technology and its applications.
In the drawings of certain embodiments in which like reference numerals refer to corresponding parts throughout the figures:
In the following description, for the purposes of explanation, numerous specific details are set forth in order to provide a thorough understanding of the various embodiments. It will be apparent, however, that embodiments may be practiced without these specific details. In other instances, structures and devices are depicted in block diagram form in order to avoid unnecessarily obscuring the embodiments.
Quantum technology-based techniques for amplifying microwave signals at millikelvin environments are described. The signals may include quantum-based information (qubit) carrying signal, magnetic resonance, or any other signal at microwave frequencies. Using the approaches described herein microwave signals are amplified with a higher dynamic range than the prior art and without any other noise besides the low noise due to a quantum mechanical fluctuation.
The amplification of microwave signal is generated based on impurity spins in a solid crystal, which is placed in a microwave resonator or embedded in a waveguide. The approaches maintain the advantages of Josephson parametric amplifiers (JPA) for quantum technology and applications but with a much higher dynamic range. In addition, the proposed amplification techniques functions under magnetic field, which JPA also lacks. Any quantum device, which works at microwave frequencies in a refrigerator and operates with superconducting or semiconducting quantum bits, quantum dots, mechanical resonators, or spins, may use these techniques.
In an embodiment, the signal-to-noise ratio of a system, and thus its performance, is determined by the noise added by the first amplifier. Such noise may be characterized by the noise power spectral density S(ω) at the signal frequency ω. As a figure-of-merit for amplifiers, this noise level is often expressed in the dimension of temperature
referred to as a noise temperature. Accordingly, the noise may depend on the temperature of the environment.
The number of noise photons added by the amplifier having a noise temperature TN is expressed by
For example, one of the low-noise cryogenic microwave amplifiers is a high electron mobility transistor (HEMT) amplifier, whose typical noise temperature is about 3-5 K, i.e., adding more than 10 noise photons. The lower limit of TN is given by zero-point energy fluctuation ℏω/2 because of the quantum mechanical uncertainty.
Therefore, in order to maximize the signal-to-noise ratio of the microwave measurement for a quantum DUT, the first amplifier should have a noise temperature as close as possible to the zero-point energy fluctuation, i.e.,
in the millikelvin temperature range. JPAs have better performance as the amplifier typically add n=0.5 to 1 noise photons. The systems 100(a)/(b) may further include microwave resonator 110 which contains sample(s) at millikelvin, inside a dilution refrigerator.
Although system 200 may amplify the quantum-based signals, system 200 suffers from a limited dynamic range. This is due to JPA 120 (and JPAs in general) having limited dynamic range, i.e., due to having very low input saturation power. For example, JPA 120 may have a maximum input power of about −100 dBm (0.1 picowatts). Using such JPA 120 would limit system 200 to reading simultaneously only theoretically twenty quantum-bits (qubits), and however, in practice, further reduced to five quantum-bits.
Another approach for amplifying microwave signals is a maser (“microwave amplification by stimulated emission of radiation”), with spins in solids.
In
The challenge of the maser-based approach is how to excite the quantum mechanical system into a situation, in which the population is inverted. To address this challenge, techniques described herein utilize a system which has multiple energy levels, at least having three levels.
In such an embodiment, it is assumed that the probability of the transition between |e, 420b, and |f, 430b, states are high. Thus, the population |f>-state, 430a is going to immediately relax into |e, 420b. As a result of the relaxation, the population for the transition between |g, 410b, and |e, 420b, states will be able to be inverted by “pumping” the transition between |g, 410a, to |f, 430a states. This three-level maser scheme may be realized in paramagnetic materials, which possess multiple energy levels, such as ruby (chromium-doped sapphire).
The noise performance of the maser amplifier may reach the quantum mechanical lower limit
provided that it is operated at extremely low temperature, such that
and the spin relaxation rate is lower than the pumping rate.
The former is nowadays always the case in the quantum information and technology applications at microwave frequencies in a dilution refrigerator. The latter is also the case at millikelvin temperatures, where the spin-lattice relaxation path, which is the dominant relaxation mechanism at a higher temperature, is frozen out, resulting in extremely slow relaxation (typically˜min, sometimes even˜hour).
In an embodiment, a maser system is operated using a crystal with impurities.
In an embodiment, due to placing diamond crystals at millikelvin temperature, the impurity generates spins that are fully polarized in the quantum ground state. The relaxation process for such a paramagnetic material is a spin-lattice relaxation, which may add significant noise for the maser amplification at high temperatures. However, the relaxation process at millikelvin temperatures are extremely long, sometimes reaching hours. Therefore, it produces negligible noise.
In an embodiment, the quantum system uses a pumping microwave frequency, which has a lower frequency than the signal frequency rather than using a higher frequency than that of the signal. Despite using a lower pumping frequency than the signal frequency, the system continues to produce a population inversion.
One technique to achieve inversion with lower pumping frequency than that of the signal is to use P1 centers in diamond (
In an embodiment, an impurity structure introduces multiple energy levels for stimulated emission. The energy levels may be based on the permutation pairs of the electron spin and nuclear spin of a P1 center. If an impurity possesses possible three nuclear spins and two electron spins, then a total of six different energy levels are introduced to the system for stimulating emission.
In the P1 center example, the frequencies of the three transitions (between 526 and 516, 524 and 514, and 522 and 512, respectively) are equally spaced, as depicted by the distance between lines 516 and 514, between lines 512 and 514, between lines 522 and 524, and between lines 524 and 526 in
In an embodiment, an asymmetry of the relaxation rate exists between the two transitions on each side (between 526 and 516, and between 522 and 512 of
In such a situation, population inversion would be established in either the upper level 512 or 516. For example, if the relaxation rate of the transition on the right-hand side (from 512 to 526) is much greater than that of the left hand side (from 516 to 526), the population in the left transition will keep pumped in the upper state 516, as depicted in
The above-described relaxation conditions occur for P1 centers in diamond in the presence of another type of defect centers, such as a nitrogen-vacancy (NV) center. NV centers have electronic spin 1. In a static magnetic field above 100 mT, the resonant frequencies of the NV centers are close to that of P1 centers. For techniques using the diamond crystal, NV centers are distributed over the same volume in a density of about 2 ppm. P1 centers and NV centers may exchange energy via spin flip-flop transitions and other higher-order cross-relaxation processes. The interaction between the spins of P1 and N-V centers leads to an accelerated relaxation of the P1 centers in the state 512 and to the enhanced population of the state 516, and eventually to the population inversion at the transition between the states 526 and 516.
In an embodiment, the transmission spectra are measured by transmitting probing microwave input signal 752 to resonator 718 through coaxial cables with a series of attenuations 710 and 712. Attenuators 710 and 712 suppress thermal noise coming from room temperature through the microwave coaxial cables at temperature stages of 3 or 4 K and 100 mK, respectively.
In an embodiment, the microwave signals originate from microwave resonator 718 pass through (series of) cryogenic isolators 722 and a low pass filter 724, which filters out the high band noise and any remnants of pump signal 750. The signal may then be further amplified by high electron mobility transistor (HEMT) cryogenic amplifier 726 at 3-4 K and may be further followed by another amplifier, amplifier 730, at the room temperature. Cryogenic isolators 722 serve to prevent noise signals generated by the HEMT amplifier from entering back into resonator 718, in an embodiment.
To perform the maser-based amplification, B0 magnetic field is tuned to such magnitude that the central spin transition (“mI=0”, between 524 and 514 of
In an embodiment, to determine the maser amplifier's gain, the magnetic field, B0, is changed to about 186 milli-Tesla, where the low field transition (mI=+1, between 516 and 526 of
In system 1000, cancellation line 1070 is also installed to suppress any unwanted effects by the strong pump signal 1050, which may distort the measurement. To this end, the microwave signal for the pump 1050 is split into two by directional coupler 1006; one is used for pump line 1072, and the other is for cancellation line 1070. The split pump signals are separately sent to the inside of the dilution refrigerator through each temperature stage 706, 704, and 702. The cancellation signal is combined by directional coupler 1008 back with the reflected pump signal out of resonator 718's after circulator 1002 and isolator 1010 at 10 mK in refrigerator 702. The phase and amplitude of the cancellation signal are tuned to have 180 degrees shifted and the same amplitude as of the reflected pump signal 1050 by phase shifter 1012 and variable attenuator 1014, respectively, so that the strong pump signal 1050 reflected from the resonator 718 coming into directional coupler 1008 is canceled out.
In an embodiment, B0 is fixed such that the high-energy spin transition (mI=+1, between 516 and 526) matches the frequency of microwave resonator 718 (ωr=6.385 GHz in this example). The spins are pumped by sending strong microwave signal 1050 with a power of a few microwatts, as an example, at the frequency of ωp=6.293 GHz, which is off-resonant with resonator 718 but resonant with the central spin transition (mI=0, between 514 and 524), in this example.
System 1000 may be probed by sending weak microwave signal 1052 (˜<−100 dBm) across ωr and measuring the reflected signal at the same frequency. Resulting signal 1054 of system 1000 is analyzed by a vector network analyzer (VNA).
At step 1215, receiving a pump signal and transmitting the pump signal, at step 1220, to the paramagnetic material with the impurity. The pumping signal provides the additional energy that transfer the population to an initial excited state that corresponds to a different electron spin state than the initial ground state of the impurity. At step 1225, due to the cross-relaxation described in
At step 1230, an input microwave signal to amplify arrives at the system. The signal is then routed through the paramagnetic material of the maser amplifier, at step 1235, and is, thereby, amplified by the maser amplifier, at step 1240, as described in
In an embodiment, one or more low pass filters and attenuators may be used to reduce the thermal noise. Alternatively or additionally, a cancellation signal may be generated, at step 1250, by phase-shifting (180 degrees) and tuning the amplitude by variable attenuators to the same as of the pump signal coming out of the maser amplifier. The cancelation signal is used to cancel out the remnants of the pump signal in the amplified input signal, at step 1255. The resulting output signal, at step 1245, has less noise.
The noise temperature of the invented maser amplifier is characterized using alternative techniques. Using the first technique, magnetic field B0 is fixed such that the central P1 center spin transition (mI=0, between 514 and 524 see
Using a different technique of noise temperature characterization, B0 is fixed such that the high-energy spin transition (mI=+1, 516 and 526) matches the frequency of the microwave resonator, and the central spin transition (mI=0, 514 and 524) is pumped by sending a strong microwave signal with a power of a few micro-Watts, as an example. Instead of sending a probe microwave signal into the resonator, the noise power spectrum at the resonator frequency is measured using a spectrum analyzer, in an embodiment. The resulting total noise temperature TN+Tbath is estimated to be about 0.6 K. This suggests that the maser amplifier described herein has a noise temperature of about 0.4 K, which is very close to
(for 6 GHz microwave), assuming that the thermal photon noise Tbath inside the resonator is as low as the vacuum noise, which is equal to TN0. The obtained noise temperature, which is slightly higher than the quantum limited, may attribute to the insufficient attenuation and filtering of systems 700 and 1000, which may have increased the thermal photon noise Tbath to 0.3 K or more, resulting in increasing the total noise temperature.
The dynamic range of the maser amplifier may be evaluated. The power dependence of the gain is measured by changing the probe microwave signal power, in an embodiment. The saturation power is estimated at least to be about 0.1 nanowatts, which is more than three orders of magnitude higher than that of the value of 0.1 picowatts of the state-of-the-art JPAs. It was confirmed that this saturation is attributed to the saturation of the cryogenic HEMT amplifier. This implies that the actual saturation power of the maser amplifier invented is much higher.
Pump microwave signal 1350 may be separately fed to maser amplifier 1320 through another dedicated microwave line, passing through coupler or combiner, such as 1308. This strong pump signal may be canceled using similar techniques as discussed above in
The bandwidth of a microwave amplifier may be described in terms of gain-bandwidth product
where G is the power gain, and B is the bandwidth of the amplifier. For example, the example maser amplifier demonstrated in this invention may have a gain-bandwidth of about 5-15 MHz. Example JPAs (Josephson parametric amplifier) have a gain-bandwidth range from 10 MHz to more than 10 GHz.
In an embodiment, a maser amplifier comprises of a chain of maser amplifiers to improve the gain-bandwidth. Instead of putting a paramagnetic crystal in a microwave resonator, as depicted in
The traveling-wave maser may include a transmission line on top of a ruby crystal. Such devices may have a gain-bandwidth product of about 500 MHz or more.
In an embodiment, the microwave transmission line is a lossless superconducting material, such as Nb, NbTi, TiN, or NbTiN, which suppresses ohmic losses inside the amplifier, resulting in a further improvement of the gain. Moreover, operating, such a traveling-wave maser amplifier, at a millikelvin temperature enhances the polarization of spins in the lowest energy level by more than one order of magnitude. Such an environment increases the effective number of spins which contributes to the amplification process (as depicted in
In an embodiment, the magnetic field gradient may be applied to the paramagnetic maser crystal to further increase the bandwidth of a traveling-guide maser amplifier. Such a gradient makes the electron spin resonance transition frequencies inhomogeneous over the crystal, i.e., increase the linewidth of the transition, therefore increasing the bandwidth of the maser amplifier can be enhanced, which is beneficial to the applications to quantum technology, such as the example described for
This application claims the benefit under 35 U.S.C. § 119(e) of provisional application 62/813,537, filed Mar. 4, 2019, the entire contents of which is hereby incorporated by reference for all purposes as if fully set forth herein.
Number | Date | Country | |
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62813537 | Mar 2019 | US |