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Related papers: LDMX -- The Light Dark Matter eXperiment

200 papers

Cosmology observations indicate that our universe is composed of 25% dark matter (DM), yet we know little about its microscopic properties. Whereas the gravitational interaction of DM is well understood, its interaction with the Standard…

High Energy Physics - Experiment · Physics 2015-01-05 R. T. Thornton , MiniBooNE-DM collaboration

We report the first result of a direct search for a Cosmic ${\it axion}$ Background (C$a$B) - a relativistic background of axions that is not dark matter - performed with the axion haloscope, the Axion Dark Matter eXperiment (ADMX).…

To reach ultra-low detection thresholds necessary to probe unprecedentedly low Dark Matter masses, target material alternatives and novel detector designs are essential. One such target material is superfluid $^4$He which has the potential…

The focus of dark matter searches to date has been on Weakly Interacting Massive Particles (WIMPs) in the GeV/$c^2$-TeV/$c^2$ mass range. The direct, indirect and collider searches in this mass range have been extensive but ultimately…

Experiments at electron-positron colliders can search for dark matter particle pair-production in association with a photon. We estimate the sensitivity of this search at the proposed International Linear Collider (ILC), under a variety of…

High Energy Physics - Phenomenology · Physics 2015-06-12 Yoonseok John Chae , Maxim Perelstein

One trend in dark matter direct detection is the development of techniques which will lower experimental thresholds and achieve sensitivity to light mass dark matter particles. In doing so, it is necessary to have an understanding of the…

Instrumentation and Detectors · Physics 2016-11-18 D. Barker

MATHUSLA is a proposed surface detector at CERN that would be able to observe the decays of non-hadronic electrically neutral long-lived particles (LLPs) with almost no background or trigger limitations. This would allow MATHUSLA to probe…

High Energy Physics - Phenomenology · Physics 2019-01-03 David Curtin , Keith R. Dienes , Brooks Thomas

The China Dark Matter Experiment (CDEX), located at the China Jinping Underground Laboratory (CJPL) whose overburden is about 2400m rock, aims at direct searches of light Weakly Interacting Massive Particles (WIMPs). A single-element…

High Energy Physics - Experiment · Physics 2020-03-24 Hao Ma , Ze She , Zhongzhi Liu , Litao Yang , Qian Yue , Zhi Zeng , Tao Xue

The singlet-doublet fermion dark matter model (SDFDM) provides a good DM candidate as well as the possibility of generating neutrino masses radiatively. The search and identification of DM requires the combined effort of both indirect and…

High Energy Physics - Phenomenology · Physics 2016-03-30 Shunsaku Horiuchi , Oscar Macias , Diego Restrepo , Andres Rivera , Hamish Silverwood , Oscar Zapata

Cosmological mechanisms that yield ultralight dark matter are insensitive to the intrinsic parity of a bosonic dark matter candidate, but that same quantity plays a crucial role in a direct detection experiment. The modification of…

High Energy Physics - Phenomenology · Physics 2021-09-20 Christopher M. Donohue , Susan Gardner , Wolfgang Korsch

Dark Matter experiments are recently focusing their detection techniques in low-mass WIMPs, which requires the use of light elements and low energy threshold. In this context, we present the TREX-DM experiment, a low background…

This report presents an overview of the unconventional use of charge-coupled devices (CCDs) to search for Dark Matter (DM). The DArk Matter In CCDs (DAMIC Experiment) employs the bulk silicon of thick, fully-depleted CCDs as a target for…

Instrumentation and Detectors · Physics 2020-01-14 N. Castello-Mor , DAMIC-M Collaboration

A search for dark matter (DM) with mass in the sub-GeV region (0.32-1 GeV) was conducted by looking for an annual modulation signal in XMASS, a single-phase liquid xenon detector. Inelastic nuclear scattering accompanied by bremsstrahlung…

Among several dark matter candidates, bosonic ultralight (sub meV) dark matter is well motivated because it could couple to the Standard Model (SM) and induce new forces. Previous MICROSCOPE and Eot Wash torsion experiments have achieved…

Cosmology and Nongalactic Astrophysics · Physics 2023-08-09 Rui Li , Shaochun Lin , Liang Zhang , Changkui Duan , Pu Huang , Jiangfeng Du

Dark matter lighter than 10 GeV/c$^2$ encompasses a promising range of candidates. A conceptual design for a new detector, DarkSide-LowMass, is presented, based on the DarkSide-50 detector and progress toward DarkSide-20k, optimized for a…

Instrumentation and Detectors · Physics 2023-06-21 P. Agnes , I. Ahmad , S. Albergo , I. F. M. Albuquerque , T. Alexander , A. K. Alton , P. Amaudruz , M. Atzori Corona , D. J. Auty , M. Ave , I. Ch. Avetisov , R. I. Avetisov , O. Azzolini , H. O. Back , Z. Balmforth , V. Barbarian , A. Barrado Olmedo , P. Barrillon , A. Basco , G. Batignani , E. Berzin , A. Bondar , W. M. Bonivento , E. Borisova , B. Bottino , M. G. Boulay , G. Buccino , S. Bussino , J. Busto , A. Buzulutskov , M. Cadeddu , M. Cadoni , A. Caminata , N. Canci , A. Capra , S. Caprioli , M. Caravati , M. Cárdenas-Montes , N. Cargioli , M. Carlini , P. Castello , V. Cataudella , P. Cavalcante , S. Cavuoti , S. Cebrian , J. M. Cela Ruiz , S. Chashin , A. Chepurnov , E Chyhyrynets , C. Cicalò , L. Cifarelli , D. Cintas , V. Cocco , E. Conde Vilda , L. Consiglio , S. Copello , G. Covone , S. Cross , P. Czudak , M. D'Aniello , S. D'Auria , M. D. Da Rocha Rolo , O. Dadoun , M. Daniel , S. Davini , A. De Candia , S. De Cecco , A. De Falco , G. De Filippis , D. De Gruttola , S. De Pasquale , G. De Rosa , G. Dellacasa , A. V. Derbin , A. Devoto , F. Di Capua , L. Di Noto , P. Di Stefano , C. Dionisi , G. Dolganov , F. Dordei , L. Doria , T. Erjavec , M. Fernandez Diaz , G. Fiorillo , A. Franceschi , P. Franchini , D. Franco , E. Frolov , N. Funicello , F. Gabriele , D. Gahan , C. Galbiati , G. Gallina , G. Gallus , M. Garbini , P. Garcia Abia , A. Gendotti , C. Ghiano , R. A. Giampaolo , C. Giganti , M. A. Giorgi , G. K. Giovanetti , V. Goicoechea Casanueva , A. Gola , D. Gorman , R. Graciani Diaz , G. Grauso , G. Grilli di Cortona , A. Grobov , M. Gromov , M. Guan , M. Guerzoni , M. Gulino , C. Guo , B. R. Hackett , J. B. Hall , A. L. Hallin , A. Hamer , H. Helton , M. Haranczyk , T. Hessel , S. Hill , S. Horikawa , F. Hubaut , T. Hugues , E. V. Hungerford , An. Ianni , V. Ippolito , C. Jillings , P. Kachru , A. A. Kemp , C. L. Kendziora , G. Keppel , A. V. Khomyakov , M. Kimura , I. Kochanek , K. Kondo , G. Korga , S. Koulosousas , A. Kubankin , M. Kuss , M. Kuźniak , M. La Commara , M. Lai , E. Le Guirriec , E. Leason , X. Li , L. Lidey , J. Lipp , M. Lissia , G. Longo , L. Luzzi , O. Macfadyen , I. N. Machulin , I. Manthos , L. Mapelli , A. Margotti , S. M. Mari , C. Mariani , J. Maricic , A. Marini , M. Martínez , C. J. Martoff , A. Masoni , K. Mavrokoridis , A. Mazzi , A. B. McDonald , A. Messina , R. Milincic , A. Moggi , A. Moharana , J. Monroe , M. Morrocchi , E. N. Mozhevitina , T. Mróz , V. N. Muratova , C. Muscas , P. Musico , R. Nania , T. Napolitano , M. Nessi , G. Nieradka , K. Nikolopoulos , I. Nikulin , J. Nowak , K. Olchansky , A. Oleinik , V. Oleynikov , P. Organtini , A. Ortiz de Solórzano , L. Pagani , M. Pallavicini , L. Pandola , E. Pantic , E. Paoloni , G. Paternoster , P. A. Pegoraro , K. Pelczar , C. Pellegrino , F. Perotti , V. Pesudo , S. Piacentini , F. Pietropaolo , N. Pino , C. Pira , A. Pocar , D. M. Poehlmann , S. Pordes , P. Pralavorio , D. Price , F. Raffaelli , F. Ragusa , Y. Ramachers , A. Ramirez , M. Razeti , A. Razeto , A. L. Renshaw , M. Rescigno , F. Resnati , F. Retiere , L. P. Rignanese , C. Ripoli , A. Rivetti , A. Roberts , C. Roberts , J. Rode , G. Rogers , L. Romero , M. Rossi , A. Rubbia , S. Sadashivajois , T. R. Saffold , O. Samoylov , E. Sandford , S. Sanfilippo , D. Santone , R. Santorelli , C. Savarese , E. Scapparone , G. Scioli , D. A. Semenov , A. Shchagin , A. Sheshukov , M. Simeone , P. Skensved , M. D. Skorokhvatov , O. Smirnov , T. Smirnova , B. Smith , A. Sokolov , M. Spangenberg , R. Stefanizzi , A. Steri , S. Stracka , V. Strickland , M. Stringer , S. Sulis , A. Sung , Y. Suvorov , A. M. Szelc , C. Türkoğ , R. Tartaglia , A. Taylor , J. Taylor , S. Tedesco , G. Testera , K. Thieme , T. N. Thorpe , A. Tonazzo , S. Torres-Lara , A. Tricomi , E. V. Unzhakov , T. Vallivilayil John , M. Van Uffelen , T. Viant , S. Viel , A. Vishneva , R. B. Vogelaar , J. Vossebeld , M. Wada , M. B. Walczak , Y. Wang , S. Westerdale , R. J. Wheadon , L. Williams , I. Wingerter-Seez , R. Wojaczyński , Ma. M. Wojcik , Ma. Wojcik , T. Wright , Y. Xie , C. Yang , A. Zabihi , P. Zakhary , A. Zani , A. Zichichi , G. Zuzel , M. P. Zykova

LUX is a two-phase (liquid/gas) xenon time projection chamber designed to detect nuclear recoils from interactions with dark matter particles. Signals from the LUX detector are processed by custom-built analog electronics which provide…

The CMS and ATLAS collaborations searched for Dark Matter (DM) particles directly produced in pair. The searches are performed using the full LHC Run-I dataset recorded with the CMS and ATLAS detectors in proton-proton collisions at a…

High Energy Physics - Experiment · Physics 2019-08-14 Annapaola de Cosa

Dark Matter (DM) is one of the most critical questions to be understood and answered in fundamental physics today. Observations with varied astronomical and cosmological technologies already pinned down that DM exists in the Universe, the…

Instrumentation and Methods for Astrophysics · Physics 2021-11-23 Junhui Liao , Yuanning Gao , Zhuo Liang , Zhaohua Peng , Zebang Ouyang , Lifeng Zhang , Lei Zhang , Jiangfeng Zhou

Automated tools for the computation of particle physics' processes have become the backbone of phenomenological studies beyond the standard model. Here, we present MadDM v3.2. This release enables the fully automated computation of…

High Energy Physics - Phenomenology · Physics 2023-03-27 Chiara Arina , Jan Heisig , Fabio Maltoni , Daniele Massaro , Olivier Mattelaer

The Large Underground Xenon (LUX) dark matter search experiment is currently being deployed at the Homestake Laboratory in South Dakota. We will highlight the main elements of design which make the experiment a very strong competitor in the…