The design, implementation, and performance of the LZ calibration systems

LUX-ZEPLIN (LZ) is a tonne-scale experiment searching for direct dark matter interactions and other rare events. It is located at the Sanford Underground Research Facility (SURF) in Lead, South Dakota, USA. The core of the LZ detector is a dual-phase xenon time projection chamber (TPC), designed with the primary goal of detecting Weakly Interacting Massive Particles (WIMPs) via their induced low energy nuclear recoils. Surrounding the TPC, two veto detectors immersed in an ultra-pure water tank enable reducing background events to enhance the discovery potential. Intricate calibration systems are purposely designed to precisely understand the responses of these three detector volumes to various types of particle interactions and to demonstrate LZ's ability to discriminate between signals and backgrounds. In this paper, we present a comprehensive discussion of the key features, requirements, and performance of the LZ calibration systems, which play a crucial role in enabling LZ's WIMP-search and its broad science program. The thorough description of these calibration systems, with an emphasis on their novel aspects, is valuable for future calibration efforts in direct dark matter and other rare-event search experiments

New constraints on ultraheavy dark matter from the LZ experiment

Searches for dark matter with liquid xenon time projection chamber experiments have traditionally focused on the region of the parameter space that is characteristic of weakly interacting massive particles, ranging from a few GeV/c2 to a few TeV/c2. Models of dark matter with a mass much heavier than this are well motivated by early production mechanisms different from the standard thermal freeze-out, but they have generally been less explored experimentally. In this work, we present a reanalysis of the first science run of the LZ experiment, with an exposure of 0.9  tonne×yr, to search for ultraheavy particle dark matter. The signal topology consists of multiple energy deposits in the active region of the detector forming a straight line, from which the velocity of the incoming particle can be reconstructed on an event-by-event basis. Zero events with this topology were observed after applying the data selection calibrated on a simulated sample of signal-like events. New experimental constraints are derived, which rule out previously unexplored regions of the dark matter parameter space of spin-independent interactions beyond a mass of 1017  GeV/c2. Published by the American Physical Society 2024 </jats:sec

Ensaios de penetração de Salmonella Enteritidis em ovos de galinha com diferentes qualidades de casca, submetidos ou não a lavagem industrial e a duas temperaturas de armazenagem Penetration of Salmonella Enteritidis in chicken eggs, comparing different shell quality, industrial washing and temperature of storage

Estudou-se o comportamento da Salmonella Enteritidis quando em contato com a superfície de ovos de consumo, classificados de acordo com a qualidade da casca ou com tratamentos (lavados ou não), usando fezes de aves como veículo de contaminação, e armazenados a 8°C e 70% de umidade relativa ou a 30°C e 90% de umidade relativa. A 8°C, o microrganismo permaneceu viável na superfície dos ovos, ao longo do tempo, enquanto a 30°C foi possível identificar a sua inibição e até sua eliminação da superfície. A contaminação do conteúdo de ovos com defeito de casca foi mais frequente quando os ovos foram submetidos a temperaturas inadequadas de armazenagem (30°C).<br>Salmonella Enteriditis behavior was studied when present on the surface of consume eggs, classified according to the shell quality or treatments (washed or not). Stools of fowls were used as a vehicle for contamination. The eggs were stored at 8°C and 70% relative humidity or at 30°C and 90% of relative humidity. At 8°C, the microorganism stayed viable on the surface of the eggs throughout the study, while at 30°C it was inhibited and eliminated from the egg shell. The contamination of content of the eggs with shell defect was more frequent when they were submitted to inappropriate temperatures of storage (30°C)

A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics

The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for Weakly Interacting Massive Particles (WIMPs), while featuring extensive sensitivity to many alternative dark matter candidates. These detectors can also study neutrinos through neutrinoless double-beta decay and through a variety of astrophysical sources. A next-generation xenon-based detector will therefore be a true multi-purpose observatory to significantly advance particle physics, nuclear physics, astrophysics, solar physics, and cosmology. This review article presents the science cases for such a detector