中文
相关论文

相关论文: The Electronics and Data Acquisition System of the…

200 篇论文

The presence of dark matter in the universe is nowadays supported by a substantial set of astronomical and cosmological observations. A large amount of dark matter is expected in the Galactic Center (GC) region. Thanks also to its…

高能天体物理现象 · 物理学 2016-09-22 V. Lefranc , E. Moulin

The nature of Dark Matter (DM) is one of the most debated questions of contemporary physics. Ground-based arrays of Cherenkov telescopes such as the High Energy Spectroscopic System (H.E.S.S.) search for DM signatures through the detection…

高能天体物理现象 · 物理学 2019-06-12 Lucia Rinchiuso , H. E. S. S. Collaboration

The CDMS II experiment has observed three events which may have arisen from weakly interacting massive particle (WIMP) dark matter (DM) with mass of order 9 GeV colliding with nuclei. Although the implied WIMP parameter region seems to be…

高能物理 - 唯象学 · 物理学 2013-08-01 Xiao-Gang He , Jusak Tandean

The most recent observations by the WMAP satellite provided us with data of unprecedented accuracy regarding the parameters describing the Standard Cosmological Model. The current matter-energy density of the Universe is close to its…

高能物理 - 唯象学 · 物理学 2008-11-26 A. B. Lahanas

SuperWeakly-Interacting Massive Particles (superWIMPs) produced in the late decays of other particles are well-motivated dark matter candidates and may be favored over standard Weakly-Interacting Massive Particles (WIMPs) by small scale…

高能物理 - 唯象学 · 物理学 2008-11-26 Jose A. R. Cembranos , Jonathan L. Feng , Arvind Rajaraman , Bryan T. Smith , Fumihiro Takayama

Directional detection can provide unambiguous observation of Dark Matter interactions even in presence of insidious backgrounds. The DM-TPC collaboration is developing a detector with the goal of measuring the direction and sense of nuclear…

The CDMS II experiment uses Z-dependent Ionization Phonon (ZIP) detectors made of Germanium and Silicon to identify nuclear recoils from Weakly Interacting Massive Particles (WIMPs) with near complete event-by-event rejection of various…

天体物理学 · 物理学 2007-05-23 Samuel Leclercq

DarkSide-20k is a next-generation dual-phase Liquid Argon Time Projection Chamber, currently under construction at the Gran Sasso National Laboratory (LNGS) in Italy. With a 20 t fiducial mass of liquid Argon, DarkSide-20k will probe…

高能物理 - 实验 · 物理学 2024-07-11 I. Manthos

We present here the principles of detection of Weakly Interacting Massive Particles, which could represent a large contribution to Dark Matter. A status of the experimental situation is given both for indirect and direct detection. In…

天体物理学 · 物理学 2019-08-14 O. Martineau

Indirect detection of dark matter particles, i.e. the detection of annihilation or decay products of Weakly Interacting Massive Particles, has entered a pivotal phase as experiments reach sensitivities that probe the most interesting…

高能物理 - 唯象学 · 物理学 2014-11-10 Jan Conrad

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 strongly indicated that DM exists in the Universe, the…

天体物理仪器与方法 · 物理学 2023-02-08 Junhui Liao , Yuanning Gao , Zhen Jiang , Zhuo Liang , Zebang OuYang , Zhaohua Peng , Fengshou Zhang , Lei hang , Jiangfeng Zhou

If the dark matter (DM) consists of a weakly interacting massive particle (WIMP), it can be produced and studied at future collider experiments like those at the LHC. The production of collider-stable WIMPs is characterized by hard…

高能物理 - 唯象学 · 物理学 2009-07-15 Spencer Chang , Andre de Gouvea

One of the most interesting mysteries of astrophysics is the puzzle of dark matter. Although numerous techniques have been explored and developed to detect this elusive substance, its nature remains unknown. One such method uses large…

高能物理 - 唯象学 · 物理学 2008-11-26 Dan Hooper , Joseph Silk

The search for weakly interacting matter particles (WIMPs) is one of the main objectives of the High Luminosity Large Hadron Collider (HL-LHC). In this work we use Machine-Learning (ML) techniques to explore WIMP radiative decays into a…

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…

天体物理仪器与方法 · 物理学 2021-11-23 Junhui Liao , Yuanning Gao , Zhuo Liang , Zhaohua Peng , Zebang Ouyang , Lifeng Zhang , Lei Zhang , Jiangfeng Zhou

Dark Matter is a hypothetical particle proposed to explain the missing matter expected from the cosmological observation. The motivation of Dark Matter is overwhelming however as it is mainly deduced from its gravitational interaction, for…

高能物理 - 实验 · 物理学 2016-02-04 Siew Yan Hoh , Jyothsna Komaragiri , Wan Ahmad Tajuddin Bin Wan Abdullah

The EDELWEISS collaboration has performed a direct search for WIMP dark matter using a 320 g heat-and-ionization cryogenic Ge detector operated in a low-background environment in the Laboratoire Souterrain de Modane. No nuclear recoils are…

The nature of Dark Matter remains one of the most important unresolved questions of fundamental physics. Many models, including the Weakly Interacting Massive Particles (WIMPs), assume Dark Matter to be a particle and predict a weak…

高能天体物理现象 · 物理学 2023-08-08 Giovanni Renzi , Juan A. Aguilar

Weakly Interacting Massive Particles (WIMPs) are one of the leading candidates for Dark Matter. We developed a model-independent method for determining the WIMP mass by using data (i.e., measured recoil energies) of direct detection…

高能物理 - 唯象学 · 物理学 2009-02-02 Manuel Drees , Chung-Lin Shan

Dark matter detection experiments using liquid argon rely on a precise characterization of the ionization response to nuclear recoils, especially in the keV energy range relevant for light dark matter interactions. In this work, we present…

高能物理 - 实验 · 物理学 2026-05-14 F. Acerbi , P. Adhikari , P. Agnes , I. Ahmad , S. Albergo , I. F. Albuquerque , T. Alexander , A. K. Alton , P. Amaudruz , M. Angiolilli , E. Aprile , M. Atzori Corona , D. J. Auty , M. Ave , I. C. Avetisov , O. Azzolini , H. O. Back , Z. Balmforth , A. I. Barrado Olmedo , P. Barrillon , G. Batignani , S. Bharat , P. Bhowmick , S. Blua , V. Bocci , W. Bonivento , B. Bottino , M. G. Boulay , T. Braun , A. Buchowicz , S. Bussino , J. Busto , M. Cadeddu , R. Calabrese , V. Camillo , A. Caminata , N. Canci , M. Caravati , M. Cárdenas-Montes , N. Cargioli , M. Carlini , P. Cavalcante , S. Cebrian , S. Chashin , A. Chepurnov , S. Choudhary , L. Cifarelli , B. Cleveland , Y. Coadou , I. Coarasa , V. Cocco , E. Conde Vilda , L. Consiglio , A. F. V. Cortez , B. S. Costa , M. Czubak , S. D'Auria , M. D. Da Rocha Rolo , A. Dainty , G. Darbo , S. Davini , R. de Asmundis , S. De Cecco , M. De Napoli , G. Dellacasa , A. V. Derbin , L. Di Noto , P. Di Stefano , L. K. Dias , D. Díaz Mairena , C. Dionisi , G. Dolganov , F. Dordei , V. Dronik , A. Elersich , T. Erjavec , N. Fearon , M. Fernández Díaz , L. Ferro , A. Ficorella , G. Fiorillo , D. Fleming , P. Franchini , D. Franco , H. Frandini Gatti , E. Frolov , F. Gabriele , D. Gahan , C. Galbiati , G. Galiński , G. Gallina , M. Garbini , P. Garcia Abia , A. Gawdzik , G. K. Giovanetti , V. Goicoechea Casanueva , A. Gola , L. Grandi , G. Grauso , G. Grilli di Cortona , A. Grobov , M. Gromov , J. Guerrero Cánovas , M. Gulino , B. R. Hackett , A. L. Hallin , M. Haranczyk , B. Harrop , T. Hessel , C. Hidalgo , J. Hollingham , J. Hu , F. Hubaut , D. Huff , T. Hugues , E. V. Hungerford , An. Ianni , V. Ippolito , A. Jamil , C. Jillings , R. Keloth , N. Kemmerich , M. Kimura , A. Klenin , K. Kondo , G. Korga , L. Kotsiopoulou , S. Koulosousas , A. Kubankin , P. Kunzé , M. Kuss , M. Kuźniak , M. Kuzwa , M. La Commara , M. Lai , E. Le Guirriec , E. Leason , A. Leoni , L. Lidey , J. Lipp , M. Lissia , L. Luzzi , O. Lychagina , O. Macfadyen , I. Machts , I. N. Machulin , S. Manecki , I. Manthos , L. Mapelli , A. Marasciulli , S. M. Mari , C. Mariani , J. Maricic , M. Martinez , C. J. Martoff , G. Matteucci , K. Mavrokoridis , A. B. McDonald , S. Merzi , A. Messina , R. Milincic , S. Minutoli , A. Mitra , J. Monroe , M. Morrocchi , A. Morsy , V. N. Muratova , M. Murra , P. Musico , R. Nania , M. Nessi , G. Nieradka , K. Nikolopoulos , E. Nikoloudaki , I. Nikulin , J. Nowak , K. Olchanski , A. Oleinik , V. Oleynikov , P. Organtini , A. Ortiz de Solórzano , A. Padmanabhan , M. Pallavicini , L. Pandola , E. Pantic , E. Paoloni , D. Papi , B. Park , G. Pastuszak , G. Paternoster , R. Pavarani , A. Peck , K. Pelczar , R. Perez , V. Pesudo , S. Piacentini , N. Pino , G. Plante , A. Pocar , S. Pordes , P. Pralavorio , E. Preosti , D. Price , M. Pronesti , S. Puglia , M. Queiroga Bazetto , F. Raffaelli , F. Ragusa , Y. Ramachers , A. Ramirez , S. Ravinthiran , M. Razeti , A. L. Renshaw , A. Repond , M. Rescigno , S. Resconi , F. Retiere , L. P. Rignanese , A. Ritchie-Yates , A. Rivetti , A. Roberts , C. Roberts , G. Rogers , L. Romero , M. Rossi , D. Rudik , J. Runge , M. A. Sabia , D. Sablone , P. Salomone , O. Samoylov , S. Sanfilippo , D. Santone , R. Santorelli , E. M. Santos , I. Sargeant , M. L. Sarsa , C. Savarese , E. Scapparone , F. G. Schuckman , D. A. Semenov , C. Seoane , M. Sestu , V. Shalamova , S. Sharma Poudel , A. Sheshukov , M. Simeone , P. Skensved , M. D. Skorokhvatov , O. Smirnov , T. Smirnova , B. Smith , F. Spadoni , M. Spangenberg , A. Steri , V. Stornelli , S. Stracka , A. Sung , C. Sunny , Y. Suvorov , A. M. Szelc , O. Taborda , R. Tartaglia , A. Taylor , J. Taylor , G. Testera , K. Thieme , A. Thompson , S. Torres-Lara , A. Tricomi , S. Tullio , E. V. Unzhakov , M. Van Uffelen , P. Ventura , G. Vera Díaz , S. Viel , A. Vishneva , R. B. Vogelaar , J. Vossebeld , B. Vyas , M. Wada , M. Walczak , Y. Wang , S. Westerdale , L. Williams , M. M. Wojcik , M. Wojcik , C. Yang , J. Yin , A. Zabihi , P. Zakhary , A. Zani , Y. Zhang , T. Zhu , A. Zichichi , G. Zuzel , M. P. Zykova