English
Related papers

Related papers: The Dynamic Range of LZ

200 papers

We report new results from the Neutrino Elastic Scattering Observation with NaI (NEON) experiment in the search for light dark matter (LDM) using 2,636 kg$\cdot$days of NaI(Tl) exposure. The experiment employs an array of NaI(Tl) crystals…

High Energy Physics - Experiment · Physics 2024-12-30 J. J. Choi , C. Ha , E. J. Jeon , J. Y. Kim , K. W. Kim , S. H. Kim , S. K. Kim , Y. D. Kim , Y. J. Ko , B. C. Koh , S. H. Lee , I. S. Lee , H. Lee , H. S. Lee , J. S. Lee , Y. M. Oh , B. J. Park

Searching for dark matter (DM) at colliders is one of the biggest challenges in high-energy physics today. Significant efforts have been made to detect DM within the mass range of 1-10,000 GeV at the Large Hadron Collider and other…

High Energy Physics - Experiment · Physics 2025-11-17 Tamas Almos Vami

The NEXT-100 detector at the LSC aims at the first competitive search for the \bbnonu decay using a high-pressure \Xe{136} electroluminescent time projection chamber. The first low-background run of NEXT-100 at 3.95 bar has been devoted to…

High Energy Physics - Experiment · Physics 2026-04-23 NEXT Collaboration , C. Cortes-Parra , P. Novella , G. Martínez-Lema , H. Almazán , V. Álvarez , L. Arazi , I. J. Arnquist , F. Auria-Luna , S. Ayet , Y. Ayyad , C. D. R. Azevedo , F. Ballester , J. E. Barcelon , M. del Barrio-Torregrosa , J. M. Benlloch-Rodríguez , F. I. G. M. Borges , A. Brodoline , N. Byrnes , A. Castillo , E. Church , M. Cid , X. Cid , C. A. N. Conde , F. P. Cossío , R. Coupe , E. Dey , P. Dietz , C. Echeverria , M. Elorza , R. Esteve , R. Felkai , L. M. P. Fernandes , P. Ferrario , P. Ferrero Mancheño , F. W. Foss , Z. Freixa , J. García-Barrena , J. J. Gómez-Cadenas , J. W. R. Grocott , R. Guenette , J. Hauptman , C. A. O. Henriques , J. A. Hernando Morata , P. Herrero-Gómez , V. Herrero , C. Hervés Carrete , Y. Ifergan , A. F. B. Isabel , B. J. P. Jones , F. Kellerer , L. Larizgoitia , A. Larumbe , P. Lebrun , F. Lopez , N. López-March , R. Madigan , R. D. P. Mano , A. Marauri , A. P. Marques , J. Martín-Albo , A. Martínez , M. Martínez-Vara , R. L. Miller , K. Mistry , J. Molina-Canteras , F. Monrabal , C. M. B. Monteiro , F. J. Mora , K. E. Navarro , D. R. Nygren , E. Oblak , I. Osborne , J. Palacio , B. Palmeiro , A. Para , I. Parmaksiz , A. Pazos , J. Pelegrin , M. Pérez Maneiro , M. Querol , J. Renner , I. Rivilla , C. Rogero , L. Rogers , B. Romeo , C. Romo-Luque , E. Ruiz-Chóliz , P. Saharia , F. P. Santos , J. M. F. dos Santos , M. Seemann , I. Shomroni , A. L. M. Silva , P. A. O. C. Silva , A. Simón , S. R. Soleti , M. Sorel , J. Soto-Oton , J. M. R. Teixeira , S. Teruel-Pardo , J. F. Toledo , C. Tonnelé , S. Torelli , J. Torrent , A. Trettin , P. R. G. Valle , M. Vanga , P. Vázquez Cabaleiro , J. F. C. A. Veloso , J. D. Villamil , L. M. Villar Padruno , J. Waiton , A. Yubero-Navarro

The cosmic ray flux at the lowest energies, $\lesssim 10$ GeV, is modulated by the solar cycle, inducing a time variation that is expected to carry over into the atmospheric neutrino flux at these energies. Here we estimate this time…

High Energy Physics - Phenomenology · Physics 2022-02-16 Yi Zhuang , Louis E. Strigari , Rafael F. Lang

The DarkSHINE experiment aims to search for dark photons by measuring the energy loss of the electrons recoiled from fixed-target. Its electromagnetic calorimeter is primarily responsible for accurately reconstructing the energy of the…

Instrumentation and Detectors · Physics 2024-07-31 Yihan Guo , Shu Li , Kun Liu , Yang Liu , Yongqi Tan , Jiannan Tang , Weihao Wu , Haijun Yang , Zhiyu Zhao , Wei Zhi , Zhizhen Zhou

The redshifted 21 cm signal from neutral hydrogen is a direct probe of the physics of the early universe and has been an important science driver of many present and upcoming radio interferometers. In this study we use a single night of…

We describe the first demonstration of a sub-keV electron recoil energy threshold in a dual-phase liquid argon time projection chamber. This is an important step in an effort to develop a detector capable of identifying the ionization…

Instrumentation and Methods for Astrophysics · Physics 2013-07-23 S. Sangiorgio , T. H. Joshi , A. Bernstein , J. Coleman , M. Foxe , C. Hagmann , I. Jovanovic , K. Kazkaz , K. Mavrokoridis , V. Mozin , S. Pereverzev , P. Sorensen

We report an absolute energy response function to electronic and nuclear recoils for germanium and liquid xenon detectors. As a result, we show that the detection energy threshold of nuclear recoils for a dual-phase xenon detector can be a…

Instrumentation and Detectors · Physics 2017-03-29 D. -M. Mei , W. -Z. Wei , L. Wang

Next generation multi-ton scale noble liquid experiments have the unique opportunity to discover dark matter particles at the TeV scale, reaching the sensitivity of 10^-48 cm2 in the WIMP nucleon scattering cross-section. A prerequisite…

Instrumentation and Detectors · Physics 2016-01-07 S. Catalanotti , A. G. Cocco , G. Covone , M. D Incecco , G. Fiorillo , G. Korga , B. Rossi , S. Walker

The photon detection system for the LHCb RICH Upgrade consists of an array of multianode photomultiplier tubes (MaPMTs) read out by custom-built modular electronics. The behaviour of the whole chain was studied at CERN using a pulsed laser.…

Instrumentation and Detectors · Physics 2018-01-10 Michele Piero Blago , Floris Keizer

The ZEPLIN-III experiment in the Palmer Underground Laboratory at Boulby uses a 12kg two-phase xenon time projection chamber to search for the weakly interacting massive particles (WIMPs) that may account for the dark matter of our Galaxy.…

We propose the operation of \textbf{LEvEL}, the Low-Energy Neutrino Experiment at the LHC, a neutrino detector near the Large Hadron Collider Beam Dump. Such a detector is capable of exploring an intense, low-energy neutrino flux and can…

High Energy Physics - Phenomenology · Physics 2021-09-06 Kevin J. Kelly , Pedro A. N. Machado , Alberto Marchionni , Yuber F. Perez-Gonzalez

We report on a search for axion dark matter in the frequency range near 5.9 GHz, conducted using the haloscope technique. The experiment employed an 8-cell microwave resonator designed to extend the accessible frequency range by a…

In the Energy Frontier we suggest developing high rate (100 MHz) finely segmented forward calorimetry preradiators with time resolution <50 ps which will survive the first 1-2 Lint of incident high radiation doses, protecting forward…

Instrumentation and Detectors · Physics 2022-03-21 David R Winn , Yasar Onel

We report the refined dark-photon exclusion bound from Dark SRF's pathfinder run. Our new result is driven by improved theoretical modeling of frequency instability in high-quality resonant experiments. Our analysis leads to a constraint…

Directional detection is a promising Dark Matter search strategy. Even though it could accommodate to a sizeable background contamination, electron/recoil discrimination remains a key and challenging issue as for direction-insensitive…

Instrumentation and Methods for Astrophysics · Physics 2015-06-05 J. Billard , F. Mayet , D. Santos

Dual-phase xenon time projection chambers achieve optimal sensitivity for dark matter in the 10 to 1000 GeV/c$^2$ mass range, but sub-GeV dark matter particles lack sufficient energy to produce nuclear recoils above detection thresholds in…

High Energy Astrophysical Phenomena · Physics 2026-01-05 Erin Barillier , Laura Manenti , Knut Mora , Paolo Padovani , Isaac Sarnoff , Yongheng Xu , Bjorn Penning , Francesco Arneodo

When bright solar-system objects are observed by GHz-THz regime telescopes, off-axis signals bounce around locally and re-enter the signal path with a time delay, causing sinusoidal ripples in output spectra. Ripples that are unstable over…

Earth and Planetary Astrophysics · Physics 2024-11-07 J S Greaves

In this white paper, we outline some of the scientific opportunities and challenges related to detection and reconstruction of low-energy (less than 100 MeV) signatures in liquid argon time-projection chamber (LArTPC) detectors. Key…

Instrumentation and Detectors · Physics 2022-03-07 D. Caratelli , W. Foreman , A. Friedland , S. Gardiner , I. Gil-Botella , G. Karagiorgi , M. Kirby , G. Lehmann Miotto , B. R. Littlejohn , M. Mooney , J. Reichenbacher , A. Sousa , K. Scholberg , J. Yu , T. Yang , S. Andringa , J. Asaadi , T. J. C. Bezerra , F. Capozzi , F. Cavanna , E. Church , A. Himmel , T. Junk , J. Klein , I. Lepetic , S. Li , P. Sala , H. Schellman , M. Sorel , J. Wang , M. H. L. S. Wang , W. Wu , J. Zennamo , M. A. Acero , M. R. Adames , H. Amar , D. A. Andrade , C. Andreopoulos , A. M. Ankowski , M. A. Arroyave , V. Aushev , M. A. Ayala-Torres , P. Baldi , C. Backhouse , A. B. Balantekin , W. A. Barkhouse , P. Barham Alzas , J. L. Barrow , J. B. R. Battat , M. C. Q. Bazetto , J. F. Beacom , B. Behera , G. Bellettini , J. Berger , A. T. Bezerra , J. Bian , B. Bilki , B. Bles , T. Bolton , L. Bomben , M. Bonesini , C. Bonilla-Diaz , F. Boran , A. N. Borkum , N. Bostan , D. Brailsford , A. Branca , G. Brunetti , T. Cai , A. Chappell , N. Charitonidis , P. H. P. Cintra , E. Conley , T. E. Coan , P. Cova , L. M. Cremaldi , J. I. Crespo-Anadon , C. Cuesta , R. Dallavalle , G. S. Davies , S. De , P. Dedin Neto , M. Delgado , N. Delmonte , P. B. Denton , A. De Roeck , R. Dharmapalan , Z. Djurcic , F. Dolek , S. Doran , R. Dorrill , K. E. Duffy , B. Dutta , O. Dvornikov , S. Edayath , J. J. Evans , A. C. Ezeribe , A. Falcone , M. Fani , J. Felix , Y. Feng , L. Fields , P. Filip , G. Fiorillo , D. Franco , D. Garcia-Gamez , A. Giri , O. Gogota , S. Gollapinni , M. Goodman , E. Gramellini , R. Gran , P. Granger , C. Grant , S. E. Greenberg , M. Groh , R. Guenette , D. Guffanti , D. A. Harris , A. Hatzikoutelis , K. M. Heeger , M. Hernandez Morquecho , K. Herner , J. Ho , P C. Holanda , N. Ilic , C. M. Jackson , W. Jang , H. -Th. Janka , J. H. Jo , F. R. Joaquim , R. S. Jones , N. Jovancevic , Y. -J. Jwa , D. Kalra , D. M. Kaplan , I. Katsioulas , E. Kearns , K. J. Kelly , E. Kemp , W. Ketchum , A. Kish , L. W. Koerner , T. Kosc , K. Kothekar , I. Kreslo , S. Kubota , V. A. Kudryavtsev , P. Kumar , T. Kutter , J. Kvasnicka , I. Lazanu , T. LeCompte , Y. Li , Y. Liu , M. Lokajicek , W. C. Louis , K. B. Luk , X. Luo , P. A. N. Machado , I. M. Machulin , K. Mahn , M. Man , R. C. Mandujano , J. Maneira , A. Marchionni , D. Marfatia , F. Marinho , C. Mariani , C. M. Marshall , F. Martinez Lopez , D. A. Martinez Caicedo , A. Mastbaum , M. Matheny , N. McConkey , P. Mehta , O. E. B. Messer , A. Minotti , O. G. Miranda , P. Mishra , I. Mocioiu , A. Mogan , R. Mohanta , T. Mohayai , C. Montanari , L. M. Montano Zetina , A. F. Moor , D. Moretti , C. A. Moura , L. M. Mualem , J. Nachtman , S. Narita , A. Navrer-Agasson , M. Nebot-Guinot , J. Nikolov , J. A. Nowak , J. P. Ochoa-Ricoux , E. O'Connor , Y. Onel , Y. Onishchuk , G. D. Orebi Gann , V. Pandey , E. G. Parozzi , S. Parveen , M. Parvu , R. B. Patterson , L. Paulucci , V. Pec , S. J. M. Peeters , F. Pompa , N. Poonthottathil , S. S. Poudel , F. Psihas , A. Rafique , B. J. Ramson , J. S. Real , A. Rikalo , M. Ross-Lonergan , B. Russell , S. Sacerdoti , N. Sahu , D. A. Sanders , D. Santoro , M. V. Santos , C. R. Senise , P. N. Shanahan , H. R Sharma , R. K. Sharma , W. Shi , S. Shin , J. Singh , J. Singh , L. Singh , P. Singh , V. Singh , M. Soderberg , S. Soldner-Rembold , J. Soto-Oton , K. Spurgeon , A. F. Steklain , F. Stocker , T. Stokes , J. Strait , M. Strait , T. Strauss , L. Suter , R. Svoboda , A. M. Szelc , M. Szydagis , E. Tarpara , E. Tatar , F. Terranova , G. Testera , N. Chithirasree , N. Todorovic , A. Tonazzo , M. Torti , F. Tortorici , M. Toups , D. Q. Tran , M. Travar , Y. -D. Tsai , Y. -T. Tsai , S. Z. Tu , J. Urheim , H. Utaegbulam , S. Valder , G. A. Valdiviesso , R. Valentim , S. Vergani , B. Viren , A. Vranicar , B. Wang , D. Waters , P. Weatherly , M. Weber , H. Wei , S. Westerdale , L. H. Whitehead , D. Whittington , A. Wilkinson , R. J. Wilson , M. Worcester , K. Wresilo , B. Yaeggy , G. Yang , J. Zalesak , B. Zamorano , J. Zuklin

We present results of a search for spin-independent dark matter-nucleon interactions in a 1 cm$^2$ by 1 mm thick (0.233 gram) high-resolution silicon athermal phonon detector operated above ground. For interactions in the substrate, this…