中文
相关论文

相关论文: Recent results in the search for dark matter with …

200 篇论文

Experiments that use liquid noble gasses as target materials, such as argon and xenon, play a significant role in direct detection searches for WIMP(-like) dark matter. As these experiments grow in size, they will soon encounter a new…

高能物理 - 唯象学 · 物理学 2023-05-05 Andrea Gaspert , Pietro Giampa , David E. Morrissey

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…

天体物理仪器与方法 · 物理学 2012-06-12 Marc Schumann

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…

天体物理仪器与方法 · 物理学 2014-08-20 Laura Baudis

DARWIN (dark matter wimp search with noble liquids) is a design study for a next-generation, multi-ton dark matter detector in Europe. Liquid argon and/or liquid xenon are the target media for the direct detection of dark matter candidates…

天体物理仪器与方法 · 物理学 2019-08-14 Laura Baudis

Liquid xenon and liquid argon detectors are leading the direct dark matter search and are expected to be the candidate technology for the forthcoming generation of ultra-sensitive large-mass detectors. At present, the scintillation light…

高能物理 - 实验 · 物理学 2022-09-20 Alessandro Razeto , Nicola Rossi

The XENON100 collaboration has recently released new dark matter limits, placing particular emphasis on their impact on searches known to be sensitive to light-mass (below 10 GeV/c^2) Weakly Interacting Massive Particles (WIMPs), such as…

宇宙学与河外天体物理 · 物理学 2010-05-14 J. I. Collar , D. N. McKinsey

In the last few years many advances have been made in the field of dark matter direct detection. In this article I will review the progress and status of experiments that employ detection techniques that do not use noble liquids. First, I…

天体物理仪器与方法 · 物理学 2014-11-21 J. Cooley

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…

Dark matter experiments primarily search for the scattering of WIMPs on target nuclei of well shielded underground detectors. The results from liquid scintillator experiments furthermore provide precise probes of very light and very weakly…

高能物理 - 唯象学 · 物理学 2015-10-19 Haipeng An , Kaixuan Ni , Maxim Pospelov , Josef Pradler , Adam Ritz

If dark matter self-annihilates into neutrinos or a second component of ("boosted") dark matter that is nucleophilic, the annihilation products may be detected with high rates via coherent nuclear scattering. A future multi-ten-tonne liquid…

高能物理 - 唯象学 · 物理学 2019-05-22 David McKeen , Nirmal Raj

In the direct detection of the galactic dark matter, experiments using cryogenic solid-state detectors or noble liquids play for years a very relevant role, with increasing target mass and more and more complex detection systems. But…

天体物理仪器与方法 · 物理学 2021-03-31 Susana Cebrian

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…

天体物理学 · 物理学 2015-06-24 Gabriel Chardin

We investigate the possibility for the direct detection of low mass (GeV scale) WIMP dark matter in scintillation experiments. Such WIMPs are typically too light to leave appreciable nuclear recoils, but may be detected via their scattering…

高能物理 - 唯象学 · 物理学 2019-10-09 B. M. Roberts , V. V. Flambaum

Weakly Interacting Massive Particles (WIMPs), are a leading candidate for the dark matter that is observed to constitute ~25% of the total mass-energy density of the Universe. The direct detection of relic WIMPs (those produced during the…

仪器与探测器 · 物理学 2017-08-23 Tarek Saab

Experiments based on noble liquids and solid state cryogenic detectors have had a leading role in the direct detection of dark matter. But smaller scale projects can help to explore the new dark matter landscape with advanced,…

天体物理仪器与方法 · 物理学 2020-05-20 Susana Cebrián

The next generation of large scale WIMP direct detection experiments have the potential to go beyond the discovery phase and reveal detailed information about both the particle physics and astrophysics of dark matter. We report here on…

宇宙学与河外天体物理 · 物理学 2014-02-05 Jayden L. Newstead , Thomas D. Jacques , Lawrence M. Krauss , James B. Dent , Francesc Ferrer

DARWIN (DARk matter WImp search with Noble liquids) is an R&D and design study towards the realization of a multi-ton scale dark matter search facility in Europe, based on the liquid argon and liquid xenon time projection chamber…

天体物理仪器与方法 · 物理学 2010-12-22 Laura Baudis

In this paper, we study the recent excess of low energy events observed by the CoGeNT collaboration, and discuss the possibility that these events originate from the elastic scattering of a light (m_DM ~ 5-10 GeV) dark matter particle. We…

高能物理 - 唯象学 · 物理学 2014-11-20 A. Liam Fitzpatrick , Dan Hooper , Kathryn M. Zurek

The problem of the dark matter in the universe is reviewed. A short history of the subject is given, and several of the most obvious particle candidates for dark matter are identified. Particular focus is given to weakly interacting,…

高能天体物理现象 · 物理学 2012-06-15 Lars Bergström

DARk matter WImp search with liquid xenoN (DARWIN) will be an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core. Its primary goal will be to explore the experimentally…

天体物理仪器与方法 · 物理学 2016-12-02 J. Aalbers , F. Agostini , M. Alfonsi , F. D. Amaro , C. Amsler , E. Aprile , L. Arazi , F. Arneodo , P. Barrow , L. Baudis , M. L. Benabderrahmane , T. Berger , B. Beskers , A. Breskin , P. A. Breur , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , L. Buetikofer , J. Calven , J. M. R. Cardoso , D. Cichon , D. Coderre , A. P. Colijn , J. Conrad , J. P. Cussonneau , M. P. Decowski , S. Diglio , G. Drexlin , E. Duchovni , E. Erdal , G. Eurin , A. Ferella , A. Fieguth , W. Fulgione , A. Gallo Rosso , P. Di Gangi , A. Di Giovanni , M. Galloway , M. Garbini , C. Geis , F. Glueck , L. Grandi , Z. Greene , C. Grignon , C. Hasterok , V. Hannen , E. Hogenbirk , J. Howlett , D. Hilk , C. Hils , A. James , B. Kaminsky , S. Kazama , B. Kilminster , A. Kish , L. M. Krauss , H. Landsman , R. F. Lang , Q. Lin , F. L. Linde , S. Lindemann , M. Lindner , J. A. M. Lopes , T. Marrodan Undagoitia , J. Masbou , F. V. Massoli , D. Mayani , M. Messina , K. Micheneau , A. Molinario , K. D. Mora , E. Morteau , M. Murra , J. Naganoma , J. L. Newstead , K. Ni , U. Oberlack , P. Pakarha , B. Pelssers , P. de Perio , R. Persiani , F. Piastra , M. C. Piro , G. Plante , L. Rauch , S. Reichard , A. Rizzo , N. Rupp , J. M. F. Dos Santos , G. Sartorelli , M. Scheibelhut , S. Schindler , M. Schumann , J. Schreiner , L. Scotto Lavina , M. Selvi , P. Shagin , M. C. Silva , H. Simgen , P. Sissol , M. von Sivers , D. Thers , J. Thurn , A. Tiseni , R. Trotta , C. D. Tunnell , K. Valerius , M. A. Vargas , H. Wang , Y. Wei , C. Weinheimer , T. Wester , J. Wulf , Y. Zhang , T. Zhu , K. Zuber
‹ 上一页 1 2 3 10 下一页 ›