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161
$$(g-2)_{e,\mu }$$ ( g - 2 ) e , μ and lepton flavor violating decays in a left-right model
Published 2024-12-01“…The results are used to discuss these decays as new physics signals in a minimal left-right symmetric model containing only one bidoublet Higgs and a $$SU(2)_R$$ S U ( 2 ) R Higgs doublet accommodating data of neutrino oscillations and $$(g-2)_{\mu }$$ ( g - 2 ) μ . …”
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162
Extracting the QCD Cutoff Parameter Using the Bernstein Polynomials and the Truncated Moments
Published 2014-01-01“…We use the truncated Mellin moments rather than the usual moments to analyse the EMC collaboration data for muon-nucleon and WA25 data for neutrino-deuterium DIS scattering. How to connect the truncated Mellin moments to usual ones is discussed. …”
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163
Lower Mass Bound on the W′ Mass via Neutrinoless Double Beta Decay in a 3-3-1 Model
Published 2018-01-01“…The discovery of neutrino masses has raised the importance of studies in the context of neutrinoless double beta decay (0νββ), which constitutes a landmark for lepton number violation (LNV). …”
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164
DUNE Prospect for Leptophobic Dark Matter
Published 2020-01-01“…In this work, we have explored the sensitivity of DUNE (Deep Underground Neutrino Experiment) for sub-GeV leptophobic dark matter, i.e., this dark matter barely couples with the leptons. …”
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165
Probing third-generation New Physics with K→πνν¯ and B→K(⁎)νν¯
Published 2025-02-01“…We further discuss how future improvements in precision could affect this picture, highlighting the discovery potential in these di-neutrino modes.…”
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166
Vacuum energy density from the form factor bootstrap
Published 2024-12-01“…A strong candidate for the zeron is a massive Majorana neutrino.…”
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167
INFORMATION SECURITY CONTROLS AS DETERMINANT OF CONTINUITY OF INFORMATION SYSTEM WORK
Published 2017-11-01Get full text
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168
INFORMATION SECURITY CONTROLS AS DETERMINANT OF CONTINUITY OF INFORMATION SYSTEM WORK
Published 2017-11-01Get full text
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169
Jets with electrons from boosted top quarks
Published 2020-01-01“…An overlap of electron shower with the b quark initiated shower, and the large nontrivial energy-momentum carried by the invisible neutrino in the top quark decay are the two obstacles to achieving this aim. …”
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170
Status of the GERDA Experiment at the Laboratori Nazionali del Gran Sasso
Published 2013-01-01“…Measurements on two-neutrino double beta decay (2νββ) giving T1/22ν=(1.88±0.10)×1021 yr and recently published background model and pulse shape performances of the detectors are discussed in the paper. …”
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171
Susy at the FPF
Published 2025-02-01“…This is possible because of the unprecedented flux of neutrinos to be produced as secondary products in LHC collisions during the high-luminosity era and the capability of FPF experiments to detect and identify their flavors.…”
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172
Macroscopic neutrinoless double beta decay: Long range quantum coherence
Published 2025-03-01“…We re-introduce, in light of our modern understanding of neutrinos, the concept of “macroscopic neutrinoless double beta decay” (MDBD) for Majorana neutrinos. …”
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173
Combining hybrid and opaque scintillator techniques in the search for double beta plus decays
Published 2025-01-01“…We expect to discover two-neutrino double beta plus decay modes within 1 tonne-week exposure and are able to probe neutrinoless double beta plus decays at several orders of magnitude improved significance compared to current experimental limits.…”
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174
Study some two loop contribution to muon anomalous MDM in the N-B-LSSM
Published 2025-02-01“…We study the electroweak corrections from several type two-loop SUSY diagrams and the virtual SUSY particles include chargino, neutralino, scalar lepton and scalar neutrino. Based on the latest experimental constraints, we study the muon anomalous MDM under the next to the minimal supersymmetric extension of the SM with local B-L gauge symmetry (N-B-LSSM). …”
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175
Development of deep-underground engineering structures via 2D and 3D RQD prediction using non-invasive CSAMT
Published 2025-01-01“…The suggested approach provides a more precise and thorough evaluation of the rock’s integrity for the effective installation of the neutrino detector 700 m below ground. The results are significant because they help us make sense of complicated geological situations, estimate the likelihood of early collapse, and build deep underground structures safely, steadily, and affordably. …”
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176
Multimessengers from Core-Collapse Supernovae: Multidimensionality as a Key to Bridge Theory and Observation
Published 2012-01-01“…The only means to get direct information about the supernova engine is from observations of neutrinos emitted by the forming neutron star, and through gravitational waves which are produced when the hydrodynamic flow or the neutrino flux is not perfectly spherically symmetric. …”
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177
DC-DC Boost Converter Design With Analog Feedback Control for Cryogenic Applications
Published 2025-01-01“…However, in the Deep Underground Neutrino Experiment (DUNE) Vertical Drift design, the Photon Detection System (PDS) electronic readout and bias circuits and sensors must be installed on the cathode plane, which is biased at a high DC voltage (-300 kV). …”
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178
CONUS+ Experiment
Published 2024-12-01“…Abstract The CONUS+ experiment aims to detect coherent elastic neutrino-nucleus scattering (CE $$\nu $$ ν NS) of reactor antineutrinos on germanium nuclei in the fully coherent regime, continuing on this way the CONUS physics program started at the Brokdorf nuclear power plant, Germany. …”
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179
Primordial gravitational waves as probe of dark matter in interferometer missions: Fisher forecast and MCMC
Published 2024-12-01“…We consider three right-handed neutrinos (RHNs), required to generate Standard Model (SM) neutrino masses via seesaw mechanism, are produced via gravity-portal in early universe. …”
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180
3D Convective Urca Process in a Simmering White Dwarf
Published 2025-01-01“…Our findings on the extent of mixing across the Urca shell, the characteristic velocities of the flow, the energy-loss rates due to neutrino emission, and the structure of the convective boundary can be used to inform 1D stellar models that track the longer-timescale evolution.…”
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