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Related papers: DARWIN

200 papers

Direct dark matter searches are promising techniques to identify the nature of dark matter particles. I describe the future of this field of research, focussing on the question of what can be achieved in the next decade. I will present the…

Instrumentation and Methods for Astrophysics · Physics 2012-12-04 Laura Baudis

The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of $^{136}$Xe. Out of its 50$\,$t total natural xenon inventory, 40$\,$t will be the active target…

Cosmological observations and the dynamics of the Milky Way provide ample evidence for an invisible and dominant mass component. This so-called dark matter could be made of new, colour and charge neutral particles, which were…

Instrumentation and Methods for Astrophysics · Physics 2014-08-20 Laura Baudis

The GENIUS project is a proposal for a new dark matter detector, with an increased sensitivity of three orders of magnitude relative to existing direct dark matter detection experiments. We performed a technical study and calculated the…

High Energy Physics - Experiment · Physics 2010-11-30 L. Baudis , G. Heusser , B. Majorovits , Y. Ramachers , H. Strecker , H. V. Klapdor--Kleingrothaus

This review will present the latest advances in the search for non-baryonic dark matter from an experimental point of view, focusing more particularly on the direct detection approach. After a brief reminder of the main motivations for this…

Astrophysics · Physics 2007-05-23 S. Fiorucci

ArDM is a new-generation WIMP detector which will measure simultaneously light and charge from scintillation and ionization of liquid argon. Our goal is to construct, characterize and operate a 1 ton liquid argon underground detector. The…

Instrumentation and Detectors · Physics 2015-05-13 Vittorio Boccone

We study the sensitivity of large-scale xenon detectors to low-energy solar neutrinos, to coherent neutrino-nucleus scattering and to neutrinoless double beta decay. As a concrete example, we consider the xenon part of the proposed DARWIN…

Instrumentation and Detectors · Physics 2014-02-10 L. Baudis , A. Ferella , A. Kish , A. Manalaysay , T. Marrodan Undagoitia , M. Schumann

Dark matter detectors using the liquid noble gases xenon and argon as WIMP targets have evolved rapidly in the last decade and will continue to play a major role in the field. Due to the possibility to scale these detectors to larger masses…

Instrumentation and Methods for Astrophysics · Physics 2012-06-12 Marc Schumann

The DARWIN mission is an Infrared free flying interferometer mission based on the new technique of nulling interferometry. Its main objective is to detect and characterize other Earth-like planets, analyze the composition of their…

Astrophysics · Physics 2011-03-16 Lisa Kaltenegger

The XENON experiment aims at the direct detection of dark matter in the form of WIMPs (Weakly Interacting Massive Particles) via their elastic scattering off Xenon nuclei. With a fiducial mass of 1000 kg of liquid xenon, a sufficiently low…

Astrophysics · Physics 2007-05-23 XENON Collaboration , Elena Aprile

The Argon Dark Matter (ArDM-1t) experiment is a ton-scale liquid argon (LAr) double-phase time projection chamber designed for direct Dark Matter searches. Such a device allows to explore the low energy frontier in LAr with a charge imaging…

The DarkSide-20k experiment represents the present goal of the Global Argon Dark Matter Collaboration program. Bringing together the experience from previous argon-based detectors, as well as the knowledge gained on large volume membrane…

Instrumentation and Detectors · Physics 2025-12-01 Andrea Zani

Solving the Dark Matter enigma represents one of the key objectives of contemporary physics. Recent astrophysical and cosmological measurements have unambiguously demonstrated that ordinary matter contributes to less than 5 % of the energy…

Astrophysics · Physics 2015-06-24 Gabriel Chardin

We present a novel deep learning pipeline to perform a model-independent, likelihood-free search for anomalous (i.e., non-background) events in the proposed next generation multi-ton scale liquid Xenon-based direct detection experiment,…

Instrumentation and Detectors · Physics 2026-05-12 J. Aalbers , K. Abe , M. Adrover , S. Ahmed Maouloud , L. Althueser , D. W. P. Amaral , B. Andrieu , E. Angelino , D. Antón Martin , B. Antunovic , E. Aprile , M. Babicz , D. Bajpai , M. Balzer , E. Barberio , L. Baudis , M. Bazyk , N. F. Bell , L. Bellagamba , R. Biondi , Y. Biondi , A. Bismark , C. Boehm , K. Boese , R. Braun , A. Breskin , S. Brommer , A. Brown , G. Bruni , R. Budnik , C. Cai , C. Capelli , A. Chauvin , A. P. Cimental Chavez , A. P. Colijn , J. Conrad , J. J. Cuenca-García , V. D'Andrea , L. C. Daniel Garcia , M. P. Decowski , A. Deisting , C. Di Donato , P. Di Gangi , S. Diglio , M. Doerenkamp , G. Drexlin , K. Eitel , A. Elykov , R. Engel , A. D. Ferella , C. Ferrari , H. Fischer , T. Flehmke , M. Flierman , K. Fujikawa , W. Fulgione , C. Fuselli , P. Gaemers , R. Gaior , M. Galloway , F. Gao , N. Garroum , R. Giacomobono , F. Girard , R. Glade-Beucke , F. Glück , L. Grandi , J. Grigat , R. Größle , H. Guan , M. Guida , P. Gyorgy , R. Hammann , V. Hannen , S. Hansmann-Menzemer , N. Hargittai , A. Higuera , C. Hils , K. Hiraoka , L. Hoetzsch , M. Hoferichter , N. F. Hood , M. Iacovacci , Y. Itow , J. Jakob , R. S. James , F. Joerg , F. Kahlert , Y. Kaminaga , M. Kara , P. Kavrigin , S. Kazama , M. Keller , P. Kharbanda , B. Kilminster , M. Kleifges , M. Klute , M. Kobayashi , D. Koke , A. Kopec , B. von Krosigk , F. Kuger , L. LaCascio , H. Landsman , R. F. Lang , L. Levinson , I. Li , A. Li , S. Li , S. Liang , Z. Liang , Y. -T. Lin , S. Lindemann , M. Lindner , K. Liu , J. Loizeau , F. Lombardi , J. Long , J. A. M. Lopes , G. M. Lucchetti , T. Luce , Y. Ma , C. Macolino , J. Mahlstedt , B. Maier , A. Mancuso , L. Manenti , F. Marignetti , T. Marrodán Undagoitia , K. Martens , J. Masbou , E. Masson , S. Mastroianni , A. Melchiorre , J. Menéndez , M. Messina , B. Milosovic , S. Milutinovic , K. Miuchi , R. Miyata , A. Molinario , C. M. B. Monteiro , K. Morå , S. Moriyama , E. Morteau , Y. Mosbacher , J. Müller , M. Murra , J. L. Newstead , K. Ni , C. O'Hare , U. Oberlack , M. Obradovic , I. Ostrowskiy , S. Ouahada , B. Paetsch , Y. Pan , M. Pandurovic , Q. Pellegrini , R. Peres , F. Piastra , J. Pienaar , M. Pierre , G. Plante , T. R. Pollmann , L. Principe , J. Qi , K. Qiao , J. Qin , M. Rajado , D. Ramírez García , A. Ravindran , A. Razeto , L. Sanchez , P. Sanchez-Lucas , G. Sartorelli , A. Scaffidi , J. Schreiner , P. Schulte , H. Schulze Eißing , M. Schumann , A. Schwenck , A. Schwenk , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , S. Sharma , W. Shen , S. Y. Shi , T. Shimada , H. Simgen , R. Singh , M. Solmaz , O. Stanley , M. Steidl , A. Stevens , A. Takeda , P. -L. Tan , D. Thers , T. Thümmler , F. Tönnies , F. Toschi , G. Trinchero , R. Trotta , C. D. Tunnell , P. Urquijo , M. Utoyama , K. Valerius , S. Vecchi , S. Vetter , G. Volta , D. Vorkapic , W. Wang , K. M. Weerman , C. Weinheimer , M. Weiss , D. Wenz , M. Wilson , C. Wittweg , J. Wolf , V. H. S. Wu , S. Wüstling , M. Wurm , Y. Xing , D. Xu , Z. Xu , M. Yamashita , L. Yang , J. Ye , L. Yuan , G. Zavattini , M. Zhong , K. Zuber

XENON10 is a new direct dark matter detection experiment using liquid xenon as target for weakly interacting, massive particles (WIMPs). A two-phase (liquid/gas) time projection chamber with 15 kg fiducial mass has been installed in a…

Astrophysics · Physics 2008-11-26 Laura Baudis

We describe the liquid-xenon dark-matter detector program of the UCLA-Torino team. A two-phase detector, ZEPLIN II, for the Boulby Mine is a good match for the current search for WIMP dark matter.

Astrophysics · Physics 2009-10-31 David B. Cline

A new method of searching for dark matter in the form of weakly interacting massive particles (WIMP) has been developed with the direct detection of the low energy nuclear recoils observed in a massive target (ultimately many tons) of ultra…

Several experiments have been conducted worldwide, with the goal of observing low-energy nuclear recoils induced by WIMPs scattering off target nuclei in ultra-sensitive, low-background detectors. In the last few decades noble liquid…

Instrumentation and Detectors · Physics 2016-03-23 B. Rossi , A. Anastasio , A. Boiano , S. Catalanotti , A. G. Cocco , G. Covone , P. Di Meo , G. Longo , A. Vanzanella , S. Walker , H. Wang , Y. Wang , G. Fiorillo

Light dark matter in the context of dark sector theories is an attractive candidate for the dark matter thought to make up the bulk of the mass of our universe. We explore here the possibility of using a low-pressure, negative-ion, time…

Instrumentation and Methods for Astrophysics · Physics 2019-03-27 D. P. Snowden-Ifft , J. L. Harton , N. Ma , F. G. Schuckman