V. A. Kudryavtsev

ORCID: 0000-0002-7018-5827
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About
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Research Areas
  • Dark Matter and Cosmic Phenomena
  • Particle physics theoretical and experimental studies
  • Neutrino Physics Research
  • Astrophysics and Cosmic Phenomena
  • Particle Detector Development and Performance
  • Atomic and Subatomic Physics Research
  • Radiation Detection and Scintillator Technologies
  • Cosmology and Gravitation Theories
  • Nuclear Physics and Applications
  • Particle accelerators and beam dynamics
  • Muon and positron interactions and applications
  • Scientific Research and Discoveries
  • Gamma-ray bursts and supernovae
  • Quantum Chromodynamics and Particle Interactions
  • High-Energy Particle Collisions Research
  • Radiation Therapy and Dosimetry
  • Nuclear reactor physics and engineering
  • Advanced materials and composites
  • Particle Accelerators and Free-Electron Lasers
  • Solar and Space Plasma Dynamics
  • Quantum, superfluid, helium dynamics
  • Planetary Science and Exploration
  • CO2 Sequestration and Geologic Interactions
  • Magnetic confinement fusion research
  • Educational Innovations and Challenges

University of Sheffield
2016-2025

European Organization for Nuclear Research
2025

Sheffield Children's University
2012-2024

National Research Tomsk State University
2020-2024

University of Edinburgh
2009-2024

Universitat Ramon Llull
2023-2024

RWTH Aachen University
2023

Amur State University
2021

Institute for Basic Science
2017-2019

Moscow Engineering Physics Institute
2017-2019

LUX-ZEPLIN (LZ) is a next-generation dark matter direct detection experiment that will operate 4850 feet underground at the Sanford Underground Research Facility (SURF) in Lead, South Dakota, USA. Using two-phase xenon detector with an active mass of 7 tonnes, LZ search primarily for low-energy interactions weakly interacting massive particles (WIMPs), which are hypothesized to make up our galactic halo. In this paper, projected WIMP sensitivity presented based on latest background estimates...

10.1103/physrevd.101.052002 article EN publisher-specific-oa Physical review. D/Physical review. D. 2020-03-04

The EDELWEISS-II Collaboration has completed a direct search for WIMP dark matter with an array of ten 400-g cryogenic germanium detectors in operation at the Laboratoire Souterrain de Modane. combined use thermal phonon sensors and charge collection electrodes interleaved geometry enables efficient rejection γ-induced radioactivity as well near-surface interactions. A total effective exposure 384 kg d been achieved, mostly coming from fourteen months continuous operation. Five nuclear...

10.1016/j.physletb.2011.07.034 article EN cc-by Physics Letters B 2011-07-29

We present the case for a dark matter detector with directional sensitivity. This document was developed at 2009 CYGNUS workshop on detection, and contains contributions from theorists experimental groups in field. describe need sensitivity; each experiment presents their project's status; we close feasibility study scaling up to one ton detector, which would cost around $150M.

10.1142/s0217751x10048172 article EN International Journal of Modern Physics A 2010-01-10

The design and performance of the LUX-ZEPLIN (LZ) detector is described as March 2015 in this Conceptual Design Report. LZ a second-generation dark-matter with potential for unprecedented sensitivity to weakly interacting massive particles (WIMPs) masses from few GeV/c2 hundreds TeV/c2. With total liquid xenon mass about 10 tonnes, will be most sensitive experiment WIMPs region by end decade. This report describes detail technical systems. Expected backgrounds are quantified presented....

10.48550/arxiv.1509.02910 preprint EN other-oa arXiv (Cornell University) 2015-01-01

The scattering of dark matter (DM) particles with sub-GeV masses off nuclei is difficult to detect using liquid xenon-based DM search instruments because the energy transfer during nuclear recoils smaller than typical detector threshold. However, tree-level DM-nucleus diagram can be accompanied by simultaneous emission a bremsstrahlung photon or so-called "Migdal" electron. These provide an electron recoil component experimental signature at higher energies corresponding recoil. presence...

10.1103/physrevlett.122.131301 article EN publisher-specific-oa Physical Review Letters 2019-04-01

We present new constraints on the dark matter-induced annual modulation signal using 1.7 years, of COSINE-100 data with a total exposure 97.7 kg$\cdot$years. The experiment, consisting 106 kg NaI(Tl) target material, is designed to carry out model-independent test DAMA/LIBRA's claim WIMP discovery by searching for same target. crystal show 2.7 cpd/kg/keV background rate average in 2--6 keV energy region interest. Using $\chi$-squared minimization method we observe best fit values amplitude...

10.1103/physrevlett.123.031302 article EN publisher-specific-oa Physical Review Letters 2019-07-16

We report on a search for low-energy (E < 20 keV) WIMP-induced nuclear recoils using data collected in 2009 - 2010 by EDELWEISS from four germanium detectors equipped with thermal sensors and an electrode design (ID) which allows to efficiently reject several sources of background. The indicate no evidence exponential distribution that could be attributed WIMP elastic scattering after exposure 113 kg.d. For WIMPs mass 10 GeV, the observation one event region results 90% CL limit 1.0x10^-5 pb...

10.1103/physrevd.86.051701 article EN Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology 2012-09-06

This paper reports on the development of a technology involving $$^{100}\hbox {Mo}$$ -enriched scintillating bolometers, compatible with goals CUPID, proposed next-generation bolometric experiment to search for neutrinoless double-beta decay. Large mass ( $$\sim 1~\hbox {kg}$$ ), high optical quality, radiopure -containing zinc and lithium molybdate crystals have been produced used develop performance single detector modules based 0.2–0.4 kg bolometers. In particular, energy resolution...

10.1140/epjc/s10052-017-5343-2 article EN cc-by The European Physical Journal C 2017-11-01

COSINE is a dark matter search experiment based on an array of low background NaI(Tl) crystals located at the Yangyang underground laboratory. The assembly COSINE-100 was completed in summer 2016 and detector currently collecting physics quality data aimed reproducing DAMA/LIBRA that reported annual modulation signal. Stable operation has been achieved will continue for least two years. Here, we describe design COSINE-100, including shielding arrangement, configuration crystal detection...

10.1140/epjc/s10052-018-5590-x article EN cc-by The European Physical Journal C 2018-02-01

The violation of Baryon Number, $\mathcal{B}$, is an essential ingredient for the preferential creation matter over antimatter needed to account observed baryon asymmetry in universe. However, such a process has yet be experimentally observed. HIBEAM/NNBAR %experiment program proposed two-stage experiment at European Spallation Source (ESS) search number violation. will include high-sensitivity searches processes that violate by one or two units: free neutron-antineutron oscillation...

10.1088/1361-6471/abf429 article EN cc-by Journal of Physics G Nuclear and Particle Physics 2021-06-14

A key task for customs workers is the interception of hazardous, illegal and counterfeit items in order to protect health safety citizens. However, it estimated that only a small fraction cargo inspected an even smaller trafficked goods are detected. Today, most widely used technology scanning vehicles, ranging from vans trucks railcars, γ ray X-ray radiography. New technologies required overcome current technological shortcomings, such as inability detect target material composition, usage...

10.3390/instruments7010013 article EN cc-by Instruments 2023-03-20

We present the Migdal In Galactic Dark mAtter expLoration (MIGDAL) experiment aiming at unambiguous observation and study of so-called effect induced by fast-neutron scattering. It is hoped that this elusive atomic process can be exploited to enhance reach direct dark matter search experiments lower masses, but it still lacking experimental confirmation. Our goal detect predicted electron emission which thought accompany nuclear scattering with low, calculable, probability, deploying an...

10.1016/j.astropartphys.2023.102853 article EN cc-by Astroparticle Physics 2023-04-23

Following the first science results of LUX-ZEPLIN (LZ) experiment, a dual-phase xenon time projection chamber operating from Sanford Underground Research Facility in Lead, South Dakota, USA, we report initial limits on model-independent nonrelativistic effective field theory describing complete set possible interactions weakly interacting massive particle (WIMP) with nucleon. These utilize same 5.5 t fiducial mass and 60 live days exposure collected for LZ spin-independent spin-dependent...

10.1103/physrevd.109.092003 article EN cc-by Physical review. D/Physical review. D. 2024-05-09

This document reports on a series of experimental and theoretical studies conducted to assess the astro-particle physics potential three future large-scale particle detectors proposed in Europe as next generation underground observatories. The apparatus employ different and, some extent, complementary detection techniques: GLACIER (liquid Argon TPC), LENA scintillator) MEMPHYS (\WC), based use large mass liquids active media. results these are presented along with critical discussion...

10.1088/1475-7516/2007/11/011 article EN Journal of Cosmology and Astroparticle Physics 2007-11-13

10.1016/j.cpc.2008.10.013 article EN Computer Physics Communications 2008-10-31

The CDMS and EDELWEISS collaborations have combined the results of their direct searches for dark matter using cryogenic germanium detectors. total data set represents 614 kg.d equivalent exposure. A straightforward method combination was chosen its simplicity before were exchanged between experiments. are interpreted in terms limits on spin-independent WIMP-nucleon cross-section. For a WIMP mass 90 GeV/c^2, where this analysis is most sensitive, cross-section 3.3 x 10^{-44} cm^2 excluded at...

10.1103/physrevd.84.011102 article EN publisher-specific-oa Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology 2011-07-06

We report on a dark matter search for Weakly Interacting Massive Particle (WIMP) in the mass range $$m_{\chi } \in [4, 30]\,\mathrm{GeV/}c^2$$ with EDELWEISS-III experiment. A 2D profile likelihood analysis is performed data from eight selected detectors lowest energy thresholds leading to combined fiducial exposure of 496 kg-days. External backgrounds $$\gamma $$ - and $$\beta -radiation, recoils $$^{206}\mathrm{Pb}$$ neutrons as well detector intrinsic were modelled outside region interest...

10.1140/epjc/s10052-016-4388-y article EN cc-by The European Physical Journal C 2016-10-01

We make use of the EDELWEISS-III array germanium bolometers to search for electron interactions at keV scale induced by phenomena beyond Standard Model. A 90% C.L. lower limit is set on lifetime decaying invisibles, $\tau > 1.2\times 10^{24}$ years. investigate emission axions or axionlike particles (ALPs) Sun, constraining coupling parameters $g_{ae}<1.1\times 10^{-11}$ and $g_{ae}\times g_{aN}^{\rm eff} < 3.5\times 10^{-17}$ in massless limit. also directly absorption bosonic dark matter...

10.1103/physrevd.98.082004 article EN cc-by Physical review. D/Physical review. D. 2018-10-31

We present the first search for a dark matter annual modulation signal in Southern Hemisphere conducted with NaI(Tl) detectors, performed by DM-Ice17 experiment. Nuclear recoils from interactions are expected to yield an annually modulated independent of location within Earth's hemispheres. DM-Ice17, step DM-Ice experimental program, consists 17 kg located at South Pole under 2200 m.w.e. overburden Antarctic glacial ice. Taken over 3.6 years total exposure 60.8 yr, data consistent no energy...

10.1103/physrevd.95.032006 article EN publisher-specific-oa Physical review. D/Physical review. D. 2017-02-28

We present the results of a search for elastic scattering from galactic dark matter in form Weakly Interacting Massive Particles (WIMPs) 4-30 GeV/$c^2$ mass range. make use 582 kg-day fiducial exposure an array 800 g Germanium bolometers equipped with set interleaved electrodes full surface coverage. searched specifically $\sim 2.5-20$ keV nuclear recoils inside detector volume. As illustration number observed events 5 (resp. 20) WIMPs are 9 4), compared to expected background 6.1 1.4). A...

10.1088/1475-7516/2016/05/019 article EN Journal of Cosmology and Astroparticle Physics 2016-05-06

Dual-phase xenon detectors, as currently used in direct detection dark matter experiments, have observed elevated rates of background electron events the low energy region. While this negatively impacts detector performance various ways, its origins only been partially studied. In paper we report a systematic investigation pathologies LUX experiment. We characterize different populations based on their emission intensities and correlations with preceding depositions detector. By studying...

10.1103/physrevd.102.092004 article EN Physical review. D/Physical review. D. 2020-11-10
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