Joseph A. Formaggio
Current Organizations / Institutes
The organizations/institutes from the scholar's latest article
Research Subjects
Joseph A. Formaggio has a total of 850 co-authors. Here are the top co-authors by number of shared publications:
- R. G. Hamish Robertson
Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, WA 98195, U.S.A.
15 shared publications - Walter Pettus
Indiana University
15 shared publications - Martin Fertl
Institute for Physics, Johannes Gutenberg University Mainz, 55128 Mainz, Germany
14 shared publications - P. L. Slocum
Wright Laboratory, Department of Physics, Yale University, New Haven, CT 06520, U.S.A.
14 shared publications - Benjamin Monreal
Department of Physics, Case Western Reserve University, Cleveland, OH 44106, U.S.A.
13 shared publications - E. Novitski
Center for Experimental Nuclear Physics and Astrophysics and Department of Physics, University of Washington, Seattle, WA 98195, U.S.A.
13 shared publications
Latest Publications
- 1 October 2026
- Published by IOP Publishing in Superconductor Science and Technology
- Vol. 39 (10) , 105010
Characterization of aluminum microwave SQUID multiplexers for CE ν NS detection
We present the design, fabrication, and characterization of an aluminum-based six-channel microwave SQUID multiplexer ( μ MUX) prototype for transition-edge sensor readout in the Ricochet experiment. The device consists of aluminum coplanar-waveguide resonators and RF superconducting quantum interference devices with Dolan-style Al/AlO x /Al Josephson junctions. By measuring the resonator scattering parameters at a range of probe tone frequencies, powers, and flux bias points, we demonstrate agreement between the device response and existing multiplexer models. We also characterize the noise performance in both open-loop and flux-ramping modes. With a high electron mobility transistor (HEMT) amplifier, open-loop measurements yield a flux sensitivity of 1–1.5 μ Φ 0 / Hz . With flux-ramp modulation, low-frequency 1 / f noise is suppressed, and the flux sensitivity is around 3–4 μ Φ 0 / Hz , corresponding to a current sensitivity of 24–33 pA / Hz at the input coil. We further demonstrate a reduction in readout noise by incorporating a Josephson traveling-wave parametric amplifier between the μ MUX and the HEMT. This achieves an open-loop flux sensitivity of 0.3–0.6 μ Φ 0 / Hz and an effective system noise temperature below 1K. These results establish aluminum μ MUX devices as a viable and extensible readout technology for low-noise cryogenic detector arrays.
- 1 October 2026
- Published by IOP Publishing in Superconductor Science and Technology
- Vol. 39 (10) , 105010
Characterization of aluminum microwave SQUID multiplexers for CE ν NS detection
We present the design, fabrication, and characterization of an aluminum-based six-channel microwave SQUID multiplexer ( μ MUX) prototype for transition-edge sensor readout in the Ricochet experiment. The device consists of aluminum coplanar-waveguide resonators and RF superconducting quantum interference devices with Dolan-style Al/AlO x /Al Josephson junctions. By measuring the resonator scattering parameters at a range of probe tone frequencies, powers, and flux bias points, we demonstrate agreement between the device response and existing multiplexer models. We also characterize the noise performance in both open-loop and flux-ramping modes. With a high electron mobility transistor (HEMT) amplifier, open-loop measurements yield a flux sensitivity of 1–1.5 μ Φ 0 / Hz . With flux-ramp modulation, low-frequency 1 / f noise is suppressed, and the flux sensitivity is around 3–4 μ Φ 0 / Hz , corresponding to a current sensitivity of 24–33 pA / Hz at the input coil. We further demonstrate a reduction in readout noise by incorporating a Josephson traveling-wave parametric amplifier between the μ MUX and the HEMT. This achieves an open-loop flux sensitivity of 0.3–0.6 μ Φ 0 / Hz and an effective system noise temperature below 1K. These results establish aluminum μ MUX devices as a viable and extensible readout technology for low-noise cryogenic detector arrays.
- 11 August 2026
- Published by American Physical Society (APS) in Physical Review Applied
- Vol. 26 (2) , 024025
Distinguishing types of correlated errors in superconducting qubits
Superconducting qubits are promising for quantum computing, but their performance is hindered by correlated errors from environmental factors like ionizing radiation and cryocooler vibrations. The authors distinguish these error types in the same device by their distinct features, and use accelerometers to directly link specific errors to pulse tube vibrations. This study also reveals that qubits engineered to resist radiation are protected against these vibration-induced errors as well. Identifying the sources of correlated errors will inform future mitigation strategies for building more robust quantum computers.
- 11 August 2026
- Published by American Physical Society (APS) in Physical Review Applied
- Vol. 26 (2) , 024025
Distinguishing types of correlated errors in superconducting qubits
Superconducting qubits are promising for quantum computing, but their performance is hindered by correlated errors from environmental factors like ionizing radiation and cryocooler vibrations. The authors distinguish these error types in the same device by their distinct features, and use accelerometers to directly link specific errors to pulse tube vibrations. This study also reveals that qubits engineered to resist radiation are protected against these vibration-induced errors as well. Identifying the sources of correlated errors will inform future mitigation strategies for building more robust quantum computers.
- Open Access
- 1 February 2026
- Published by IOP Publishing in Journal of Instrumentation
- Vol. 21 (02) , P02026
Project 8 apparatus for cyclotron radiation emission spectroscopy with 83m Kr and tritium
Cyclotron Radiation Emission Spectroscopy (CRES) is a novel technique for the precise measurement of relativistic electron energy. This technique is being employed by the Project 8 collaboration for measuring a high-precision tritium beta decay spectrum to perform a frequency-based measurement of the neutrino mass. In this work, we describe the Project 8 Phase II apparatus, used for the detection of the CRES signal from the conversion electrons of 83m Kr and the first CRES measurement of the beta-decay spectrum of molecular tritium.
- 1 February 2026
- Published by IOP Publishing in Journal of Instrumentation
- Vol. 21 (02) , P02026
Open AccessProject 8 apparatus for cyclotron radiation emission spectroscopy with 83m Kr and tritium
Cyclotron Radiation Emission Spectroscopy (CRES) is a novel technique for the precise measurement of relativistic electron energy. This technique is being employed by the Project 8 collaboration for measuring a high-precision tritium beta decay spectrum to perform a frequency-based measurement of the neutrino mass. In this work, we describe the Project 8 Phase II apparatus, used for the detection of the CRES signal from the conversion electrons of 83m Kr and the first CRES measurement of the beta-decay spectrum of molecular tritium.
- Open Access
- 22 December 2025
- Published by American Physical Society (APS) in Physical Review D
- Vol. 112 (11)
Characterization of mini-CryoCube detectors from the RICOCHET experiment commissioning at the Institut Laue-Langevin
The experiment aims to measure the coherent elastic neutrino-nucleus scattering process from antineutrinos emitted by a research nuclear reactor operated by the Institut Laue-Langevin (Grenoble, France). This article presents a description of the experimental installation and the detector performance achieved during its commissioning with a mini-CryoCube module consisting of three 42-g germanium cryogenic calorimeters. The baseline resolutions and background levels are reported both during reactor-on and reactor-off periods and as noise mitigation techniques were improved. A baseline resolution of 40 eV electron equivalent was achieved for the ionization channel after setup improvements, and the phonon channel resolutions ranged from 50 to 80 eV of total phonon energy. In the energy region from 2 to 7 keV, a nuclear recoil rate of 14 ( 3 ) events / ( kg day keV ) is measured during the reactor-off period selecting events in coincidence with muon veto signals. This rate is in agreement with the cosmogenic neutron rate calculated from GEANT4 simulations. After the rejection of events in coincidence with signals in the muon veto detectors, a combined 90% confidence level limit on the nuclear recoil background of < 9 events / ( kg day keV ) is obtained in that energy region during the reactor-on period, which is compatible with our GEANT4 model calculation corresponding to a total rate of 5 events / ( kg day keV ) . The sensitivity of this analysis was however found to be limited by a surface event contamination which is currently being addressed by the Collaboration with upgraded detectors.
- 22 December 2025
- Published by American Physical Society (APS) in Physical Review D
- Vol. 112 (11)
Open AccessCharacterization of mini-CryoCube detectors from the RICOCHET experiment commissioning at the Institut Laue-Langevin
The experiment aims to measure the coherent elastic neutrino-nucleus scattering process from antineutrinos emitted by a research nuclear reactor operated by the Institut Laue-Langevin (Grenoble, France). This article presents a description of the experimental installation and the detector performance achieved during its commissioning with a mini-CryoCube module consisting of three 42-g germanium cryogenic calorimeters. The baseline resolutions and background levels are reported both during reactor-on and reactor-off periods and as noise mitigation techniques were improved. A baseline resolution of 40 eV electron equivalent was achieved for the ionization channel after setup improvements, and the phonon channel resolutions ranged from 50 to 80 eV of total phonon energy. In the energy region from 2 to 7 keV, a nuclear recoil rate of 14 ( 3 ) events / ( kg day keV ) is measured during the reactor-off period selecting events in coincidence with muon veto signals. This rate is in agreement with the cosmogenic neutron rate calculated from GEANT4 simulations. After the rejection of events in coincidence with signals in the muon veto detectors, a combined 90% confidence level limit on the nuclear recoil background of < 9 events / ( kg day keV ) is obtained in that energy region during the reactor-on period, which is compatible with our GEANT4 model calculation corresponding to a total rate of 5 events / ( kg day keV ) . The sensitivity of this analysis was however found to be limited by a surface event contamination which is currently being addressed by the Collaboration with upgraded detectors.
- 27 October 2025
- Published by American Physical Society (APS) in Physical Review C
- Vol. 112 (4)
Antenna arrays for neutrino mass measurements with cyclotron radiation emission spectroscopy
- 27 October 2025
- Published by American Physical Society (APS) in Physical Review C
- Vol. 112 (4)
Antenna arrays for neutrino mass measurements with cyclotron radiation emission spectroscopy
- 11 September 2025
- Published by American Physical Society (APS) in Physical Review A
- Vol. 112 (3)
Dynamics of magnetic evaporative beamline cooling for the preparation of cold atomic beams
- 11 September 2025
- Published by American Physical Society (APS) in Physical Review A
- Vol. 112 (3)
Dynamics of magnetic evaporative beamline cooling for the preparation of cold atomic beams
- Open Access
- 8 September 2025
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 135 (11) , 291-314
Superradiant Neutrino Lasers from Radioactive Condensates
Superradiance emerges from collective spontaneous emission in optically pumped gases, and is characterized by photon emission enhancements of up to 1 4 N 2 in an N atom system. The gain mechanism derives from correlations developed within the decay medium rather than from stimulated emission as in lasing, so an analog of this process should be possible for fermionic final states. We introduce here the concept of superradiant neutrino emission from a radioactive Bose Einstein condensate, which can form the basis for a superradiant neutrino laser. A plausible experimental realization based on a condensate of electron-capture isotope Rb 83 could exhibit effective radioactive decay rates accelerated from 86.2 days to minutes in viably sized rubidium condensates of 10 6 atoms.
- 8 September 2025
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 135 (11) , 291-314
Open AccessSuperradiant Neutrino Lasers from Radioactive Condensates
Superradiance emerges from collective spontaneous emission in optically pumped gases, and is characterized by photon emission enhancements of up to 1 4 N 2 in an N atom system. The gain mechanism derives from correlations developed within the decay medium rather than from stimulated emission as in lasing, so an analog of this process should be possible for fermionic final states. We introduce here the concept of superradiant neutrino emission from a radioactive Bose Einstein condensate, which can form the basis for a superradiant neutrino laser. A plausible experimental realization based on a condensate of electron-capture isotope Rb 83 could exhibit effective radioactive decay rates accelerated from 86.2 days to minutes in viably sized rubidium condensates of 10 6 atoms.
- Top Cited PapersOpen Access
- 11 July 2025
- Published by Springer Nature in Nature Communications
- Vol. 16 (1) , 1-15
Synchronous detection of cosmic rays and correlated errors in superconducting qubit arrays
Quantum information processing at scale will require sufficiently stable and long-lived qubits, likely enabled by error-correction codes. Several recent superconducting-qubit experiments, however, reported observing intermittent spatiotemporally correlated errors that would be problematic for conventional codes, with ionizing radiation being a likely cause. Here, we directly measured the cosmic-ray contribution to spatiotemporally correlated qubit errors. We accomplished this by synchronously monitoring cosmic-ray detectors and qubit energy-relaxation dynamics of 10 transmon qubits distributed across a 5 × 5 × 0.35 mm3 silicon chip. Cosmic rays caused correlated errors at a rate of \(1/\left(592\begin{array}{c}+48\\ -41\end{array}\,{\rm{s}}\right)\), accounting for 17.1 ± 1.3% of all such events. Our qubits responded to essentially all of the cosmic rays and their secondary particles incident on the chip, consistent with the independently measured arrival flux. Moreover, we observed that the landscape of the superconducting gap in proximity to the Josephson junctions dramatically impacts the qubit response to cosmic rays. Given the practical difficulties associated with shielding cosmic rays, our results indicate the importance of radiation hardening—for example, superconducting gap engineering—to the realization of robust quantum error correction.- 11 July 2025
- Published by Springer Nature in Nature Communications
- Vol. 16 (1) , 1-15
Top Cited PapersOpen AccessSynchronous detection of cosmic rays and correlated errors in superconducting qubit arrays
Quantum information processing at scale will require sufficiently stable and long-lived qubits, likely enabled by error-correction codes. Several recent superconducting-qubit experiments, however, reported observing intermittent spatiotemporally correlated errors that would be problematic for conventional codes, with ionizing radiation being a likely cause. Here, we directly measured the cosmic-ray contribution to spatiotemporally correlated qubit errors. We accomplished this by synchronously monitoring cosmic-ray detectors and qubit energy-relaxation dynamics of 10 transmon qubits distributed across a 5 × 5 × 0.35 mm3 silicon chip. Cosmic rays caused correlated errors at a rate of \(1/\left(592\begin{array}{c}+48\\ -41\end{array}\,{\rm{s}}\right)\), accounting for 17.1 ± 1.3% of all such events. Our qubits responded to essentially all of the cosmic rays and their secondary particles incident on the chip, consistent with the independently measured arrival flux. Moreover, we observed that the landscape of the superconducting gap in proximity to the Josephson junctions dramatically impacts the qubit response to cosmic rays. Given the practical difficulties associated with shielding cosmic rays, our results indicate the importance of radiation hardening—for example, superconducting gap engineering—to the realization of robust quantum error correction. - Open Access
- 26 May 2025
- Published by Springer Nature in The European Physical Journal D
- Vol. 79 (5) , 1-17
Calorimetric wire detector for measurement of atomic hydrogen beams
A calorimetric detector for minimally disruptive measurements of atomic hydrogen beams is described. The calorimeter measures heat released by the recombination of hydrogen atoms into molecules on a thin wire. As a demonstration, the angular distribution of a beam with a peak intensity of $$\approx 10^{16} \,{\textrm{atoms}}/{(\textrm{cm}^2 \textrm{s})}$$ is measured by translating the wire across the beam. The data agree well with an analytic model of the beam from the thermal hydrogen atom source. Using the beam shape model, the relative intensity of the beam can be determined to 5% precision or better at any angle. Graphical- 26 May 2025
- Published by Springer Nature in The European Physical Journal D
- Vol. 79 (5) , 1-17
Open AccessCalorimetric wire detector for measurement of atomic hydrogen beams
A calorimetric detector for minimally disruptive measurements of atomic hydrogen beams is described. The calorimeter measures heat released by the recombination of hydrogen atoms into molecules on a thin wire. As a demonstration, the angular distribution of a beam with a peak intensity of $$\approx 10^{16} \,{\textrm{atoms}}/{(\textrm{cm}^2 \textrm{s})}$$ is measured by translating the wire across the beam. The data agree well with an analytic model of the beam from the thermal hydrogen atom source. Using the beam shape model, the relative intensity of the beam can be determined to 5% precision or better at any angle. Graphical