A resistive ACHINOS multi-anode structure with DLC coating for spherical proportional counters

Giomataris, I.; Gros, M.; Katsioulas, I.; Knights, P.; Mols, J. -P.; Neep, T.; Nikolopoulos, K.; Savvidis, G.; Savvidis, I.; Shang, L.; Ward, R.; Zhou, Y.

doi:10.48550/arxiv.2003.01068

Cited by 3 publications

(2 citation statements)

References 12 publications

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“…Being sensitive to extremely small energy transfers, this will open new windows for the exploration of DM candidates giving very weak signals. Also for gas chambers an active work is ongoing for sensors and readout techniques to improve energy threshold or pattern signal [334,340,341].…”

Section: Randd Programsmentioning

confidence: 99%

Direct detection of dark matter—APPEC committee report*

et al. 2022

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This report provides an extensive review of the experimental programme of direct detection searches of particle dark matter. It focuses mostly on European efforts, both current and planned, but does it within a broader context of a worldwide activity in the field. It aims at identifying the virtues, opportunities and challenges associated with the different experimental approaches and search techniques. It presents scientific and technological synergies, both existing and emerging, with some other areas of particle physics, notably collider and neutrino programmes, and beyond. It addresses the issue of infrastructure in light of the growing needs and challenges of the different experimental searches. Finally, the report makes a number of recommendations from the perspective of a long-term future of the field. They are introduced, along with some justification, in the opening overview and recommendations section and are next summarised at the end of the report. Overall, we recommend that the direct search for dark matter particle interactions with a detector target should be given top priority in astroparticle physics, and in all particle physics, and beyond, as a positive measurement will provide the most unambiguous confirmation of the particle nature of dark matter in the Universe.

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Section: Randd Programsmentioning

confidence: 99%

Direct detection of dark matter—APPEC committee report*

et al. 2022

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“…The study of CEνNS with a sub-keV energy threshold detector, like the SPC, allows for a rich physics program and opens a window to physics beyond the Standard Model that will appear as deviations from the expected recoil spectra predicted by SM interactions [197]. The detector is composed of a spherical shell made of radio-pure copper, acting as the cathode, and a read-out sensor at the center with either a single anode [198] or multiple anodes [199,200]. The detector is versatile and can operate with a wide variety of gas mixtures.…”

Section: Gaseous Detectorsmentioning

confidence: 99%

Snowmass Neutrino Frontier NF10 Topical Group Report: Netrino Detectors

Klein

Machado

Schmitz

et al. 2022

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Neutrino physics spans an enormous range of energies and scales: from detection of low-energy cosmic neutrinos; to keV-scale recoils in coherent neutrino scattering; to MeV-scale solar, reactor, and neutrinoless double beta decay events; to GeV and TeV-scale detection of neutrinos from accelerators and the atmosphere; to cosmic sources in the PeV-ZeV range. While any particular experiment tends to focus on just one or two detection approaches, the great breadth of neutrino physics means that there is an equally broad spectrum of neutrino detection technologies and methodologies.At any one time, there are a dozen or more medium-to large-scale neutrino detectors operating worldwide, several more in the design or construction phases, and many future detectors planned. Beyond this are a diverse set of smaller scale prototypes distributed across universities and labs.The focus in this report is on new technologies and approaches that will enable future neutrino detectors, and thus experiments that are already built and running, are under construction, or for which technical designs exist are not discussed in great detail. Recommendations for Next-Generation Neutrino DetectorsWhile there are many exciting detectors and enabling technologies described in this report, there are a few ideas that have had a particularly large community interest, and we formulate these into a set of recommendations below: 1 Future Advances in Photon-Based Neutrino Detectors arXiv:2203.07479 2 Coherent elastic neutrino-nucleus scattering: Terrestrial and astrophysical applications arXiv:2203.07361 3 Recoil imaging for dark matter, neutrinos, and physics beyond the Standard Model arXiv:2203.05914 4 Low-Energy Physics in Neutrino LArTPCs arXiv:2203.00740 5 SoLAr: Solar Neutrinos in Liquid Argon arXiv:2203.07501 6 Low Background kTon-Scale Liquid Argon Time Projection Chambers arXiv:2203.08821 7 Measuring the Neutrino Event Time in Liquid Argon by a Post-Reconstruction One-parameter Fit

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Direct Detection of Dark Matter -- APPEC Committee Report

Billard,

Boulay,

Cebrián

et al. 2021

Preprint

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This Report provides an extensive review of the experimental programme of direct detection searches of particle dark matter. It focuses mostly on European efforts, both current and planned, but does it within a broader context of a worldwide activity in the field. It aims at identifying the virtues, opportunities and challenges associated with the different experimental approaches and search techniques. It presents scientific and technological synergies, both existing and emerging, with some other areas of particle physics, notably collider and neutrino programmes, and beyond. It addresses the issue of infrastructure in light of the growing needs and challenges of the different experimental searches. Finally, the Report makes a number of recommendations from the perspective of a long-term future of the field. They are introduced, along with some justification, in the opening Overview and Recommendations section and are next summarised at the end of the Report. Overall, we recommend that the direct search for dark matter particle interactions with a detector target should be given top priority in astroparticle physics, and in all particle physics, and beyond, as a positive measurement will provide the most unambiguous confirmation of the particle nature of dark matter in the Universe.

show abstract

A resistive ACHINOS multi-anode structure with DLC coating for spherical proportional counters

Cited by 3 publications

References 12 publications

Direct detection of dark matter—APPEC committee report*

Direct detection of dark matter—APPEC committee report*

Snowmass Neutrino Frontier NF10 Topical Group Report: Netrino Detectors

Direct Detection of Dark Matter -- APPEC Committee Report

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