REVIEW 3 major objections 1 minor 75 references
Quantum measurement systems and applications to particle physics and cosmology
T0 review · 3 major / 1 minor · reviewed 2026-08-05 · deepseek-v4-flash
Pith's one-line read A new survey maps quantum-enhanced measurement systems onto particle physics and cosmology targets, arguing these technologies have reached the point where they can improve searches for dark matter, gravitational waves, and cosmic signals.
desk verdict A review that might be a useful map of quantum-enhanced detectors, but the abstract alone doesn't show coverage or critical assessment — verify before citing. read the letter →
The pith
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
The reading
What carries the argument
The central object is the quantum measurement system: a detector whose sensitivity is enhanced by quantum resources, usually superposition, entanglement, or squeezing. The three named families are superconducting quantum sensors (devices whose quantum states, such as qubits or Josephson-junction dynamics, transduce external signals), atom interferometry (matter-wave interference that measures accelerations, rotations, or forces), and quantum spin sensors (magnetometers and related devices that read out ensembles or single spins). What does the work: these devices are proposed as replacements or complements to classical sensors in specific experiments, with the quantum enhancement providing a
What would settle it
Build a quantum-enhanced detector (e.g., an atom interferometer for gravitational wave detection or a superconducting qubit sensor for dark matter) and run it in a realistic experimental environment; if its sensitivity is limited by classical disorder, magnetic field gradients, or technical noise rather than by quantum projection noise, the survey's core claim that quantum enhancement will deliver 'excellent potential' in these applications is falsified.
Extended reading notes
Core claim
The paper's central claim is that quantum measurement systems employing enhancements not previously adopted in experimental physics — in particular superconducting quantum sensors, atom interferometers, and quantum spin sensors — are now being proposed for and applied to particle physics and cosmology. It frames these technologies as a coherent family: each uses controlled quantum states to beat the classical sensitivity floors of conventional detectors. The review maps specific detector concepts to specific physics targets, such as dark matter searches, neutrino physics, gravitational wave detection, and cosmological surveys, and argues that the technologies carry 'excellent potential' to i
Load-bearing premise
The paper assumes that quantum enhancement is the limiting factor in the target experiments — that improvements from squeezed, entangled, or superposition-based sensing are not erased by classical noise, systematic errors, or detector inefficiencies in realistic particle physics and cosmology settings.
Editorial extensions
If this is right
- If the survey is right, several next-generation experiments in dark matter, neutrino physics, and gravitational wave detection could see sensitivity improvements by adopting quantum-enhanced readout or sensing schemes.
- The transfer of industrial quantum technology (from computing and communication) into experimental physics could become a deliberate pipeline, lowering the cost and risk of developing new detectors.
- Superconducting quantum sensors could enable searches for low-mass dark matter candidates and single-photon-level signals that are currently invisible to conventional detectors.
- Atom interferometry could provide new probes of gravitational waves and violations of fundamental symmetries, complementing laser interferometers with a different frequency window.
- Quantum spin sensors could open compact, high-sensitivity magnetometers useful for measuring faint cosmological or particle-physics signals in constrained environments.
Reading between the lines
- A natural extension the review leaves implicit: the strongest near-term payoff is likely in low-frequency precision measurements (e.g., dark matter haloscopes, axion searches, gravitational-wave low band) where quantum enhancement is not erased by thermal noise or backgrounds, whereas in high-energy collider settings classical backgrounds may dominate.
- Because the survey organizes the field, it implicitly suggests a testable roadmap: one could compare the projected sensitivity curves of quantum-enhanced detectors against classical detectors for a specific target (e.g., axion dark matter) to identify where the quantum advantage actually survives.
- The success of these detectors may hinge on integrating quantum sensors with existing cryogenic and vacuum infrastructure, a practical concern the review acknowledges only by framing the technologies as 'emerging.'
- If commercial quantum computing hardware reaches higher coherence times, the same qubit-based sensors could become reconfigurable detectors, a direction the paper's industrial-motivation framing points toward but does not explicitly pursue.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The submitted manuscript, arXiv:2508.10325, is a review article intended to survey quantum measurement technologies—superconducting quantum sensors, atom interferometry, and quantum spin sensors—and their proposed applications in particle physics and cosmology. The abstract states that these technologies have 'excellent potential' and that new proposals exist to apply them to fundamental physics. The full text supplied for review is empty: no sections, equations, figures, tables, or references are present. Consequently, the paper's actual content cannot be evaluated, and all technical and coverage claims remain unverifiable.
Significance. If the completed review accurately maps the three named technology families onto concrete particle physics and cosmology targets, it could serve as a useful field-organizing reference, particularly by connecting industrial quantum-technology developments to fundamental-science applications. However, with no full text available, none of this can be assessed. There is no evidence of machine-checked proofs, reproducible code, parameter-free derivations, or falsifiable predictions; the submission as it stands is an abstract-only statement of intent.
major comments (3)
- [Full text] The body of the manuscript is empty. There are no sections, equations, figures, tables, or references to review. This is the load-bearing issue: the paper's value depends entirely on the accuracy and completeness of its survey of superconducting quantum sensors, atom interferometry, and quantum spin sensors, and none of that content is present in the submitted version.
- [Abstract] The abstract asserts that the quantum measurement systems have 'excellent potential' for particle physics and cosmology and that these are 'new... not previously adopted.' No supporting evidence, comparative analysis, or citation is available. The claim that quantum enhancements will survive classical noise floors and systematics in realistic experimental settings is a physics premise that the abstract merely asserts.
- [Coverage claim] The abstract names three technology families as representative of 'currently available and emerging quantum technologies,' but without a reference list or a survey methodology, there is no basis to verify that this selection is representative or that the characterization of the cited literature is accurate. This coverage premise is central to a review and cannot be checked.
minor comments (1)
- [Abstract] The abstract is clear as a statement of intent, but it should summarize the actual content of the review once the full text is present. As written, it could describe any tutorial on quantum sensors.
Circularity Check
No circularity: the paper is an abstract-level review with no derivation chain to be circular.
full rationale
The submitted full text of arXiv:2508.10325 is empty, and the only available content is the abstract, which states the intent to survey quantum-enhanced detector technologies and their proposed applications in particle physics and cosmology. There is no derivation, no fitted parameter presented as a prediction, and no formal argument that could reduce to its own inputs. A review paper is by construction external: its content is drawn from the literature it surveys, so the circularity burden is near zero. No self-citation is visible in the abstract, and no load-bearing claim is made that would need external support beyond the cited literature. The absence of technical content creates an evidence gap for checking coverage and citation fidelity, but that is a completeness limitation, not circularity. Therefore the appropriate finding is no significant circularity, score 0.
Assumptions & free parameters
assumptions (2)
- domain assumption Quantum-enhanced measurement principles (squeezing, superposition, entanglement) can be engineered into detector systems with sensitivity advantages relevant to particle physics and cosmology.
- domain assumption The surveyed literature is representative and accurately characterized.
Cite this review
Pith. "Pith review of Quantum measurement systems and applications to particle physics and cosmology." pith.science (2026). https://pith.science/paper/VHFM3PNN
@misc{pith2026250810325,
author = {Pith},
title = {Pith review of: Quantum measurement systems and applications to particle physics and cosmology},
year = {2026},
howpublished = {\url{https://pith.science/paper/VHFM3PNN}},
note = {Machine review of arXiv:2508.10325}
}
read the original abstract
There are new detector proposals and R&D that utilize quantum enhancements not previously adopted. Examples include superconducting quantum sensors, atom interferometry, and quantum spin sensors. They are mainly motivated by industrial applications toward quantum computing, secure quantum communication systems, and high-sensitivity sensors. Given the excellent potential of the new quantum measurement systems, there are also new proposals to apply them in particle physics and cosmology. In this review, I survey currently available and emerging quantum technologies and their applications. I then discuss future directions and new proposals for particle physics and cosmology.
Reference graph
Works this paper leans on
-
[1]
write newline
" write newline "" before.all 'output.state := FUNCTION n.dashify 't := "" t empty not t #1 #1 substring "-" = t #1 #2 substring "--" = not "--" * t #2 global.max substring 't := t #1 #1 substring "-" = "-" * t #2 global.max substring 't := while if t #1 #1 substring * t #2 global.max substring 't := if while FUNCTION word.in bbl.in ":" * " " * FUNCTION f...
-
[2]
write newline
" write newline "" before.all 'output.state := FUNCTION n.dashify 't := "" t empty not t #1 #1 substring "-" = t #1 #2 substring "--" = not "--" * t #2 global.max substring 't := t #1 #1 substring "-" = "-" * t #2 global.max substring 't := while if t #1 #1 substring * t #2 global.max substring 't := if while FUNCTION word.in bbl.in ":" * " " * FUNCTION f...
- [3]
-
[4]
D. J. Wineland, J. J. Bollinger, W. M. Itano, D. J. Heinzen, Squeezed atomic states and projection noise in spectroscopy , Phys. Rev. A 50 (1) (1994) 67. https://doi.org/10.1103/PhysRevA.50.67 doi:10.1103/PhysRevA.50.67
-
[5]
S. F. Huelga, C. Macchiavello, T. Pellizzari, A. K. Ekert, M. B. Plenio, J. I. Cirac, On the improvement of frequency standards with quantum entanglement , Phys. Rev. Lett. 79 (1997) 3865. http://arxiv.org/abs/quant-ph/9707014 arXiv:quant-ph/9707014 , https://doi.org/10.1103/PhysRevLett.79.3865 doi:10.1103/PhysRevLett.79.3865
work page Pith review arXiv 1997
-
[6]
T. Sichanugrist, H. Fukuda, T. Moroi, K. Nakayama, S. Chigusa, N. Mizuochi, M. Hazumi, Y. Matsuzaki, Entanglement-enhanced ac magnetometry in the presence of Markovian noise , Phys. Rev. A 111 (4) (2025) 042605. http://arxiv.org/abs/2410.21699 arXiv:2410.21699 , https://doi.org/10.1103/PhysRevA.111.042605 doi:10.1103/PhysRevA.111.042605
-
[7]
A. Chou, et al., Quantum Sensors for High Energy Physics , in: Quantum Sensors for HEP workshop, 2023, pp. 1--63. http://arxiv.org/abs/2311.01930 arXiv:2311.01930
arXiv 2023
-
[8]
Optica Quantum 2.0 , ``Quantum 2.0 Conference and Exhibition",\ ://www.optica.org/events/topical\_meetings/quantum/
Show all 75 references
-
[9]
NVIDIA, https://www.nvidia.com/ja-jp/solutions/quantum-computing/
-
[10]
QURECA, https://www.qureca.com/quantum-initiatives-worldwide/
-
[11]
Physics World , ``The Physics World Breakthrough of the Year 2024",\\ https://physicsworld.com/a/two-advances-in-quantum-error-correction-share-the-physics-world-2024-breakthrough-of-the-year/
2024
-
[12]
Bluvstein, et al., Logical quantum processor based on reconfigurable atom arrays , Nature 626 (7997) (2024) 58--65
D. Bluvstein, et al., Logical quantum processor based on reconfigurable atom arrays , Nature 626 (7997) (2024) 58--65. http://arxiv.org/abs/2312.03982 arXiv:2312.03982 , https://doi.org/10.1038/s41586-023-06927-3 doi:10.1038/s41586-023-06927-3
2024 arXiv
-
[13]
Acharya, et al., Quantum error correction below the surface code threshold , Nature 638 (8052) (2025) 920--926
R. Acharya, et al., Quantum error correction below the surface code threshold , Nature 638 (8052) (2025) 920--926. http://arxiv.org/abs/2408.13687 arXiv:2408.13687 , https://doi.org/10.1038/s41586-024-08449-y doi:10.1038/s41586-024-08449-y
2025 arXiv
-
[14]
QuEra, Error-corrected quantum computing roadmap, https://www.quera.com/press-releases/quera-computing-releases-a-groundbreaking-roadmap-for-advanced-error-corrected-quantum-computers-pioneering-the-next-frontier-in-quantum-innovation-0 (January 2024)
2024
-
[15]
J. M. Thomas, F. I. Yeh, J. H. Chen, J. J. Mambretti, S. J. Kohlert, G. S. Kanter, P. Kumar, Quantum teleportation coexisting with classical communications in optical fiber , Optica 11 (12) (2024) 1700--1707. http://arxiv.org/abs/2404.10738 arXiv:2404.10738 , https://doi.org/1...
2024 arXiv
-
[16]
Korzh, et al., Demonstration of sub-3 ps temporal resolution with a superconducting nanowire single-photon detector , Nature Photon
B. Korzh, et al., Demonstration of sub-3 ps temporal resolution with a superconducting nanowire single-photon detector , Nature Photon. 14 (4) (2020) 250--255. http://arxiv.org/abs/1804.06839 arXiv:1804.06839 , https://doi.org/10.1038/s41566-020-0589-x doi:10.1038/s41566-020-0589-x
2020 arXiv
-
[17]
D. V. Reddy, D. V. Reddy, R. R. Nerem, S. W. Nam, R. P. Mirin, V. B. Verma, Superconducting nanowire single-photon detectors with 98\ https://doi.org/10.1364/OPTICA.400751 doi:10.1364/OPTICA.400751
-
[18]
B. G. Oripov, D. S. Rampini, J. Allmaras, M. D. Shaw, S. W. Nam, B. Korzh, A. N. McCaughan, A superconducting nanowire single-photon camera with 400,000 pixels , Nature 622 (7984) (2023) 730--734. http://arxiv.org/abs/2306.09473 arXiv:2306.09473 , https://doi.org/10.1038/s4158...
2023 arXiv
-
[19]
Craiciu, et al., High-speed detection of 1550\,\,nm single photons with superconducting nanowire detectors , Optica 10 (2) (2023) 183--190
I. Craiciu, et al., High-speed detection of 1550\,\,nm single photons with superconducting nanowire detectors , Optica 10 (2) (2023) 183--190. http://arxiv.org/abs/2210.11644 arXiv:2210.11644 , https://doi.org/10.1364/OPTICA.478960 doi:10.1364/OPTICA.478960
2023 arXiv
-
[20]
Chiles, et al., New Constraints on Dark Photon Dark Matter with Superconducting Nanowire Detectors in an Optical Haloscope , Phys
J. Chiles, et al., New Constraints on Dark Photon Dark Matter with Superconducting Nanowire Detectors in an Optical Haloscope , Phys. Rev. Lett. 128 (23) (2022) 231802. http://arxiv.org/abs/2110.01582 arXiv:2110.01582 , https://doi.org/10.1103/PhysRevLett.128.231802 doi:10.110...
2022 arXiv
-
[21]
G. G. Taylor, A. B. Walter, B. Korzh, B. Bumble, S. R. Patel, J. P. Allmaras, A. D. Beyer, R. O'Brient, M. D. Shaw, E. E. Wollman, Low-noise single-photon counting superconducting nanowire detectors at infrared wavelengths up to 29 m, Optica 10 (12) (2023) 1672--1678
2023
-
[22]
S. Lee, T. Polakovic, W. Armstrong, A. Dibos, T. Draher, N. Pastika, Z.-E. Meziani, V. Novosad, Beam tests of SNSPDs with 120 GeV protons , Nucl. Instrum. Meth. A 1069 (2024) 169956. http://arxiv.org/abs/2312.13405 arXiv:2312.13405 , https://doi.org/10.1016/j.nima.2024.169956 ...
2024 arXiv
-
[23]
Kawasaki, Quantum sensing using cold atoms and molecules for nuclear and particle physics https://arxiv.org/abs/2411.19424 (2025)
A. Kawasaki, Quantum sensing using cold atoms and molecules for nuclear and particle physics https://arxiv.org/abs/2411.19424 (2025). http://arxiv.org/abs/2411.19424 arXiv:2411.19424 . ://arxiv.org/abs/2411.19424
2025
-
[24]
Aeppli, K
A. Aeppli, K. Kim, W. Warfield, M. S. Safronova, J. Ye, https://link.aps.org/doi/10.1103/PhysRevLett.133.023401 Clock with 8 10 ^ - 19 systematic uncertainty , Phys. Rev. Lett. 133 (2024) 023401. https://doi.org/10.1103/PhysRevLett.133.023401 doi:10.1103/PhysRevLett.133.023401...
2024 doi
-
[25]
Aslam, H
N. Aslam, H. Zhou, E. K. Urbach, M. J. Turner, R. L. Walsworth, M. D. Lukin, H. Park, Quantum sensors for biomedical applications , Nature Rev. Phys. 5 (3) (2023) 157--169. https://doi.org/10.1038/s42254-023-00558-3 doi:10.1038/s42254-023-00558-3
2023 doi
-
[26]
Goodman, et al., ADMX Axion Dark Matter Bounds around 3.3\,\, eV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability , Phys
C. Goodman, et al., ADMX Axion Dark Matter Bounds around 3.3\,\, eV with Dine-Fischler-Srednicki-Zhitnitsky Discovery Ability , Phys. Rev. Lett. 134 (11) (2025) 111002. http://arxiv.org/abs/2408.15227 arXiv:2408.15227 , https://doi.org/10.1103/PhysRevLett.134.111002 doi:10.110...
2025 arXiv
-
[27]
Sonnenschein, Next generation haloscope searches for axion dark matter with mass > 1 ev,, qUPosium2024, https://conference-indico.kek.jp/event/290/ (December 2024)
A. Sonnenschein, Next generation haloscope searches for axion dark matter with mass > 1 ev,, qUPosium2024, https://conference-indico.kek.jp/event/290/ (December 2024)
2024
-
[28]
P. A. R. Ade, et al., A Measurement of the Cosmic Microwave Background B-Mode Polarization Power Spectrum at Sub-Degree Scales with POLARBEAR , Astrophys. J. 794 (2) (2014) 171, [Erratum: Astrophys.J. 848, 73 (2017)]. http://arxiv.org/abs/1403.2369 arXiv:1403.2369 , https://do...
2014 arXiv
-
[29]
Suzuki, et al., The POLARBEAR-2 and the Simons Array Experiment , J
A. Suzuki, et al., The POLARBEAR-2 and the Simons Array Experiment , J. Low Temp. Phys. 184 (3-4) (2016) 805--810. http://arxiv.org/abs/1512.07299 arXiv:1512.07299 , https://doi.org/10.1007/s10909-015-1425-4 doi:10.1007/s10909-015-1425-4
2016 arXiv
-
[30]
R. J. Thornton, et al., The Atacama Cosmology Telescope: The polarization-sensitive ACTPol instrument , Astrophys. J. Suppl. 227 (2) (2016) 21. http://arxiv.org/abs/1605.06569 arXiv:1605.06569 , https://doi.org/10.3847/1538-4365/227/2/21 doi:10.3847/1538-4365/227/2/21
2016 arXiv
-
[31]
Ade, et al., The Simons Observatory: Science goals and forecasts , JCAP 02 (2019) 056
P. Ade, et al., The Simons Observatory: Science goals and forecasts , JCAP 02 (2019) 056. http://arxiv.org/abs/1808.07445 arXiv:1808.07445 , https://doi.org/10.1088/1475-7516/2019/02/056 doi:10.1088/1475-7516/2019/02/056
2019 arXiv
-
[32]
Galitzki, et al., The Simons Observatory: Instrument Overview , Proc
N. Galitzki, et al., The Simons Observatory: Instrument Overview , Proc. SPIE Int. Soc. Opt. Eng. 10708 (2018) 1070804. http://arxiv.org/abs/1808.04493 arXiv:1808.04493 , https://doi.org/10.1117/12.2312985 doi:10.1117/12.2312985
2018 arXiv
-
[33]
Essinger-Hileman, et al., CLASS: The Cosmology Large Angular Scale Surveyor , Proc
T. Essinger-Hileman, et al., CLASS: The Cosmology Large Angular Scale Surveyor , Proc. SPIE Int. Soc. Opt. Eng. 9153 (2014) 91531I. http://arxiv.org/abs/1408.4788 arXiv:1408.4788 , https://doi.org/10.1117/12.2056701 doi:10.1117/12.2056701
2014 arXiv
-
[34]
J. E. Austermann, et al., SPTpol: an instrument for CMB polarization measurements with the South Pole Telescope , Proc. SPIE Int. Soc. Opt. Eng. 8452 (2012) 84521E. http://arxiv.org/abs/1210.4970 arXiv:1210.4970 , https://doi.org/10.1117/12.927286 doi:10.1117/12.927286
2012 arXiv
-
[35]
J. A. Sobrin, et al., The Design and Integrated Performance of SPT-3G , Astrophys. J. Supp. 258 (2) (2022) 42. http://arxiv.org/abs/2106.11202 arXiv:2106.11202 , https://doi.org/10.3847/1538-4365/ac374f doi:10.3847/1538-4365/ac374f
2022 arXiv
-
[36]
Hui, et al., BICEP Array: a multi-frequency degree-scale CMB polarimeter , Proc
H. Hui, et al., BICEP Array: a multi-frequency degree-scale CMB polarimeter , Proc. SPIE Int. Soc. Opt. Eng. 10708 (2018) 1070807. http://arxiv.org/abs/1808.00568 arXiv:1808.00568 , https://doi.org/10.1117/12.2311725 doi:10.1117/12.2311725
2018 arXiv
-
[37]
P. A. R. Ade, et al., Joint Analysis of BICEP2/ Keck Array and Planck Data , Phys. Rev. Lett. 114 (2015) 101301. http://arxiv.org/abs/1502.00612 arXiv:1502.00612 , https://doi.org/10.1103/PhysRevLett.114.101301 doi:10.1103/PhysRevLett.114.101301
2015 arXiv
-
[38]
P. A. R. Ade, et al., Bicep/KeckXV: The Bicep3 Cosmic Microwave Background Polarimeter and the First Three-year Data Set , Astrophys. J. 927 (1) (2022) 77. http://arxiv.org/abs/2110.00482 arXiv:2110.00482 , https://doi.org/10.3847/1538-4357/ac4886 doi:10.3847/1538-4357/ac4886
2022
-
[39]
G\'enova-Santos, et al., QUIJOTE scientific results I
R. G\'enova-Santos, et al., QUIJOTE scientific results I. Measurements of the intensity and polarisation of the anomalous microwave emission in the Perseus molecular complex , Mon. Not. Roy. Astron. Soc. 452 (4) (2015) 4169--4182. http://arxiv.org/abs/1501.04491 arXiv:1501.044...
2015 arXiv
-
[40]
Lee, et al., GroundBIRD: A CMB Polarization Experiment with MKID Arrays , J
K. Lee, et al., GroundBIRD: A CMB Polarization Experiment with MKID Arrays , J. Low Temp. Phys. 200 (5-6) (2020) 384--391. http://arxiv.org/abs/2011.07705 arXiv:2011.07705 , https://doi.org/10.1007/s10909-020-02511-5 doi:10.1007/s10909-020-02511-5
2020 arXiv
-
[41]
J. C. Hamilton, et al., QUBIC I: Overview and science program , JCAP 04 (04) (2022) 034. http://arxiv.org/abs/2011.02213 arXiv:2011.02213 , https://doi.org/10.1088/1475-7516/2022/04/034 doi:10.1088/1475-7516/2022/04/034
2022 arXiv
-
[42]
Ghosh, et al., Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1 , JCAP 10 (2022) 063
S. Ghosh, et al., Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1 , JCAP 10 (2022) 063. http://arxiv.org/abs/2205.14804 arXiv:2205.14804 , https://doi.org/10.1088/1475-7516/2022/10/063 doi:10.1088/1475-7516/2022/10/063
2022 arXiv
-
[43]
P. A. R. Ade, et al., A Constraint on Primordial B-modes from the First Flight of the Spider Balloon-borne Telescope , Astrophys. J. 927 (2) (2022) 174. http://arxiv.org/abs/2103.13334 arXiv:2103.13334 , https://doi.org/10.3847/1538-4357/ac20df doi:10.3847/1538-4357/ac20df
2022 arXiv
-
[44]
Abitbol, et al., The EBEX Balloon-borne Experiment Detectors and Readout , Astrophys
M. Abitbol, et al., The EBEX Balloon-borne Experiment Detectors and Readout , Astrophys. J. Suppl. 239 (1) (2018) 8. http://arxiv.org/abs/1803.01018 arXiv:1803.01018 , https://doi.org/10.3847/1538-4365/aae436 doi:10.3847/1538-4365/aae436
2018 arXiv
-
[45]
Addamo, et al., The large scale polarization explorer (LSPE) for CMB measurements: performance forecast , JCAP 08 (2021) 008
G. Addamo, et al., The large scale polarization explorer (LSPE) for CMB measurements: performance forecast , JCAP 08 (2021) 008. http://arxiv.org/abs/2008.11049 arXiv:2008.11049 , https://doi.org/10.1088/1475-7516/2021/08/008 doi:10.1088/1475-7516/2021/08/008
2021 arXiv
-
[46]
N. N. Gandilo, et al., The Primordial Inflation Polarization Explorer (PIPER) , Proc. SPIE Int. Soc. Opt. Eng. 9914 (2016) 99141J. http://arxiv.org/abs/1607.06172 arXiv:1607.06172 , https://doi.org/10.1117/12.2231109 doi:10.1117/12.2231109
2016 arXiv
-
[47]
Accelerators in the Universe
M. Hazumi , Jumping into cmb polarization measurements-a new group at kek-, in: H. Kodama , K. Ioka (Eds.), KEK CosmoPhysics Group Inaugural Conference "Accelerators in the Universe", Vol. 1040 of A.I.P. Conf. Ser., 2008, pp. 78--88. https://doi.org/10.1063/1.2981556 doi:10.10...
2008 doi
-
[48]
Hazumi, Future CMB polarization measurements and Japanese contributions , Prog
M. Hazumi, Future CMB polarization measurements and Japanese contributions , Prog. Theor. Phys. Suppl. 190 (2011) 75--89. https://doi.org/10.1143/PTPS.190.75 doi:10.1143/PTPS.190.75
2011 doi
-
[49]
Hazumi, et al., LiteBIRD: a small satellite for the study of B-mode polarization and inflation from cosmic background radiation detection , Proc
M. Hazumi, et al., LiteBIRD: a small satellite for the study of B-mode polarization and inflation from cosmic background radiation detection , Proc. SPIE Int. Soc. Opt. Eng. 8442 (2012) 844219. https://doi.org/10.1117/12.926743 doi:10.1117/12.926743
2012 doi
-
[50]
Matsumura , et al., Mission Design of LiteBIRD , J
T. Matsumura , et al., Mission Design of LiteBIRD , J. Low Temp. Phys. 176 (5-6) (2014) 733--740. http://arxiv.org/abs/1311.2847 arXiv:1311.2847 , https://doi.org/10.1007/s10909-013-0996-1 doi:10.1007/s10909-013-0996-1
2014 arXiv
-
[51]
litebird: mission overview and design tradeoffs
T. Matsumura , et al., "litebird: mission overview and design tradeoffs", in: J. Oschmann , Jacobus M., M. Clampin , G. G. Fazio , H. A. MacEwen (Eds.), Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave, Vol. 9143 of Society of Photo-Optical Ins...
2014 doi
-
[52]
Allys, et al., Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey , PTEP 2023 (4) (2023) 042F01
E. Allys, et al., Probing Cosmic Inflation with the LiteBIRD Cosmic Microwave Background Polarization Survey , PTEP 2023 (4) (2023) 042F01. http://arxiv.org/abs/2202.02773 arXiv:2202.02773 , https://doi.org/10.1093/ptep/ptac150 doi:10.1093/ptep/ptac150
2023 arXiv
-
[53]
Abazajian, et al., CMB-S4 Science Case, Reference Design, and Project Plan , , (7 2019)
K. Abazajian, et al., CMB-S4 Science Case, Reference Design, and Project Plan , , (7 2019). http://arxiv.org/abs/1907.04473 arXiv:1907.04473
2019 arXiv
-
[54]
Seljak, M
U. Seljak, M. Zaldarriaga, Signature of gravity waves in polarization of the microwave background , Phys. Rev. Lett. 78 (1997) 2054--2057. http://arxiv.org/abs/astro-ph/9609169 arXiv:astro-ph/9609169 , https://doi.org/10.1103/PhysRevLett.78.2054 doi:10.1103/PhysRevLett.78.2054
1997 arXiv
-
[55]
Kamionkowski, A
M. Kamionkowski, A. Kosowsky, A. Stebbins, A Probe of primordial gravity waves and vorticity , Phys. Rev. Lett. 78 (1997) 2058--2061. http://arxiv.org/abs/astro-ph/9609132 arXiv:astro-ph/9609132 , https://doi.org/10.1103/PhysRevLett.78.2058 doi:10.1103/PhysRevLett.78.2058
1997 arXiv
-
[56]
W. Hu , M. White , CMB anisotropies: Total angular momentum method , Phys. Rev. D56 (2) (1997) 596--615. http://arxiv.org/abs/astro-ph/9702170 arXiv:astro-ph/9702170 , https://doi.org/10.1103/PhysRevD.56.596 doi:10.1103/PhysRevD.56.596
1997 arXiv
-
[57]
F. L. Bezrukov, M. Shaposhnikov, The Standard Model Higgs boson as the inflaton , Phys. Lett. B 659 (2008) 703--706. http://arxiv.org/abs/0710.3755 arXiv:0710.3755 , https://doi.org/10.1016/j.physletb.2007.11.072 doi:10.1016/j.physletb.2007.11.072
2008 arXiv
-
[58]
Ballesteros, J
G. Ballesteros, J. Redondo, A. Ringwald, C. Tamarit, Standard Model axion seesaw Higgs portal inflation. Five problems of particle physics and cosmology solved in one stroke , JCAP 08 (2017) 001. http://arxiv.org/abs/1610.01639 arXiv:1610.01639 , https://doi.org/10.1088/1475-7...
2017 arXiv
-
[59]
Adam, et al., The NIKA2 large-field-of-view millimetre continuum camera for the 30 m IRAM telescope , Astron
R. Adam, et al., The NIKA2 large-field-of-view millimetre continuum camera for the 30 m IRAM telescope , Astron. Astrophys. 609 (2018) A115. http://arxiv.org/abs/1707.00908 arXiv:1707.00908 , https://doi.org/10.1051/0004-6361/201731503 doi:10.1051/0004-6361/201731503
2018 arXiv
-
[60]
Okada, et al., X-ray Spectroscopy of Muonic Atoms Isolated in Vacuum with Transition Edge Sensors , J
S. Okada, et al., X-ray Spectroscopy of Muonic Atoms Isolated in Vacuum with Transition Edge Sensors , J. Low Temp. Phys. 200 (5-6) (2020) 445--451. https://doi.org/10.1007/s10909-020-02476-5 doi:10.1007/s10909-020-02476-5
2020 doi
-
[61]
QUP , qUPosium2024,\\ https://conference-indico.kek.jp/event/290/
-
[62]
CERN, the International Conference on Quantum Technology for High-Energy Physics (QT4HEP2025),\\ https://indico.cern.ch/event/1433194/
-
[63]
DRD5, dRD5/RDquantum collaboration meeting,\\ https://indico.cern.ch/event/1503433/timetable/\#20250217
-
[64]
Di Valentino, O
E. Di Valentino, O. Mena, S. Pan, L. Visinelli, W. Yang, A. Melchiorri, D. F. Mota, A. G. Riess, J. Silk, In the realm of the Hubble tension a review of solutions , Class. Quant. Grav. 38 (15) (2021) 153001. http://arxiv.org/abs/2103.01183 arXiv:2103.01183 , https://doi.org/10...
2021 arXiv
-
[65]
A. G. Adame, et al., DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations , JCAP 02 (2025) 021. http://arxiv.org/abs/2404.03002 arXiv:2404.03002 , https://doi.org/10.1088/1475-7516/2025/02/021 doi:10.1088/1475-7516/2025/02/021
2024 arXiv
-
[66]
DRD5, dRD5 / RDquantum - quantum sensor R&D for particle physics, https://drd5.web.cern.ch/index.html
-
[67]
Badurina, et al., AION: An Atom Interferometer Observatory and Network , JCAP 05 (2020) 011
L. Badurina, et al., AION: An Atom Interferometer Observatory and Network , JCAP 05 (2020) 011. http://arxiv.org/abs/1911.11755 arXiv:1911.11755 , https://doi.org/10.1088/1475-7516/2020/05/011 doi:10.1088/1475-7516/2020/05/011
2020 arXiv
-
[68]
Abe, et al., Matter-wave Atomic Gradiometer Interferometric Sensor (MAGIS-100) , Quantum Sci
M. Abe, et al., Matter-wave Atomic Gradiometer Interferometric Sensor (MAGIS-100) , Quantum Sci. Technol. 6 (4) (2021) 044003. http://arxiv.org/abs/2104.02835 arXiv:2104.02835 , https://doi.org/10.1088/2058-9565/abf719 doi:10.1088/2058-9565/abf719
2021 arXiv
-
[69]
C. R. Mercer, E. N. Montbach, S. D. Christe, R. M. Connerton, D. A. Podolski, M. P. Robinson, M. R. Perez, Quantum sensing for NASA science missions , EPJ Quant. Technol. 12 (1) (2025) 56. https://doi.org/10.1140/epjqt/s40507-025-00360-3 doi:10.1140/epjqt/s40507-025-00360-3
2025 doi
-
[70]
Adachi, et al., Exploration of the polarization angle variability of the Crab Nebula with POLARBEAR and its application to the search for axionlike particles , Phys
S. Adachi, et al., Exploration of the polarization angle variability of the Crab Nebula with POLARBEAR and its application to the search for axionlike particles , Phys. Rev. D 110 (6) (2024) 063013. http://arxiv.org/abs/2403.02096 arXiv:2403.02096 , https://doi.org/10.1103/Phy...
2024 arXiv
-
[71]
Chigusa, M
S. Chigusa, M. Hazumi, E. D. Herbschleb, N. Mizuochi, K. Nakayama, Light dark matter search with nitrogen-vacancy centers in diamonds , JHEP 03 (2025) 083. http://arxiv.org/abs/2302.12756 arXiv:2302.12756 , https://doi.org/10.1007/JHEP03(2025)083 doi:10.1007/JHEP03(2025)083
2025 arXiv
-
[72]
Chigusa, M
S. Chigusa, M. Hazumi, E. D. Herbschleb, Y. Matsuzaki, N. Mizuochi, K. Nakayama, Nuclear spin metrology with nitrogen vacancy center in diamond for axion dark matter detection , Phys. Rev. D 111 (7) (2025) 075028. http://arxiv.org/abs/2407.07141 arXiv:2407.07141 , https://doi....
2025 arXiv
-
[73]
E. D. Herbschleb, S. Chigusa, R. Kawase, H. Kawashima, M. Hazumi, K. Nakayama, N. Mizuochi, Robust sensing via the standard deviation with a quantum sensor , APL Quantum 1 (4) (2024) 046106. https://doi.org/10.1063/5.0223678 doi:10.1063/5.0223678
2024 doi
-
[74]
, axionLimits, https://cajohare.github.io/AxionLimits/
O’Hare, C. , axionLimits, https://cajohare.github.io/AxionLimits/
-
[75]
2015, , 579, A101
Aladro, R., Martín, S., Riquelme, D., et al. 2015, , 579, A101
2015
Reviewed August 5, 2026 · model on record in the stance chip above.
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