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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

Kinetic Inductance Detectors (KIDs) have become an attractive alternative to traditional bolometers in the sub-mm and mm observing community due to their innate frequency multiplexing capabilities and simple lithographic processes. These…

Instrumentation and Methods for Astrophysics · Physics 2018-06-13 Q. Y. Tang , P. S. Barry , R. Basu Thakur , A. Kofman , J. Vieira , E. Shirokoff

Ionizing radiation has emerged as a potential limiting factor for superconducting quantum processors, inducing quasiparticle bursts and correlated errors that challenge fault-tolerant operation. Atmospheric muons are particularly…

In the extensive efforts to understand the nature of Dark Matter and searches at colliders, the LHCb experiment has a unique sensitivity to low mass Dark Matter candidates. These proceedings present recent results and prospects on Dark…

High Energy Physics - Experiment · Physics 2021-11-02 Titus Mombächer

We show that a two-excitation process in superfluid helium, combined with sensitivity to meV energy depositions, can probe dark matter down to the ~keV warm dark matter mass limit. This mass reach is three orders of magnitude below what can…

High Energy Physics - Phenomenology · Physics 2016-09-21 Katelin Schutz , Kathryn M. Zurek

Microwave Kinetic Inductance Detectors (MKIDs) have been demonstrated as capable phonon sensors when coupled to crystalline substrates, and have been proposed as detectors for next-generation rare-event searches such as for the direct…

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

The WIMP (weakly interacting massive particle) paradigm for dark matter is currently being probed via many different experiments. Direct detection, indirect detection and collider searches are all hoping to catch a glimpse of these elusive…

High Energy Physics - Phenomenology · Physics 2013-04-24 Herbert Dreiner , Moritz Huck , Michael Krämer , Daniel Schmeier , Jamie Tattersall

Inelastic dark matter (IDM) models feature an energy threshold for scattering with Standard Model particles, which enables their consistency with the increasingly stringent limits placed by direct detection experiments. In a typical…

High Energy Physics - Phenomenology · Physics 2025-10-15 Zamiul Alam , Christopher V. Cappiello , Francesc Ferrer

We explore the phenomenology of Kaluza-Klein (KK) dark matter in very general models with universal extra dimensions (UEDs), emphasizing the complementarity between high-energy colliders and dark matter direct detection experiments. In…

High Energy Physics - Phenomenology · Physics 2009-11-13 Sebastian Arrenberg , Laura Baudis , Kyoungchul Kong , Konstantin T. Matchev , Jonghee Yoo

Directional detection of galactic Dark Matter offers a unique opportunity to identify Weakly Interacting Massive Particle (WIMP) events as such. Depending on the unknown WIMP-nucleon cross section, directional detection may be used to :…

Cosmology and Nongalactic Astrophysics · Physics 2013-12-30 F. Mayet , J. Billard

We present our current progress on the design and test of Ti/TiN Multilayer for use in Kinetic Inductance Detectors (KIDs). Sensors based on sub-stoichiometric TiN film are commonly used in several applications. However, it is difficult to…

Light cold dark matter consisting of weakly interacting slim (or sub-eV) particles (WISPs) has been in the focus of a large number of studies made over the past two decades. The QCD axion and axion-like particles with masses in the…

High Energy Physics - Experiment · Physics 2014-10-24 Dieter Horns , Axel Lindner , Andrei Lobanov , Andreas Ringwald

DAMIC (Dark Matter in CCDs) is a novel dark matter experiment that has unique sensitivity to dark matter particles with masses below 10 GeV. Due to its low electronic readout noise (R.M.S. ~3 e-) this instrument is able to reach a detection…

It is shown that under realistic background considerations, an improvement in Cold Dark Matter sensitivity of several orders of magnitude is expected from a detector based on superheated liquid droplets. Such devices are totally insensitive…

Astrophysics · Physics 2010-01-06 J. I. Collar

The current state searches for dark matter in the form of Weakly Interacting Massive Particles (WIMPs) using both direct and indirect techniques is reviewed. Advances in recent years by various direct search experiments, utilising…

Astrophysics · Physics 2007-05-23 N. J. C. Spooner , V. A. Kudryavtsev

Large-volume neutrino experiments are ideal for testing boosted dark matter (BDM) scenarios. We propose, for the first time, an approach to utilize knockout neutrons by detecting de-excitation $\gamma$ rays and coincident captured neutrons…

High Energy Physics - Phenomenology · Physics 2024-09-10 Koun Choi , Jong-Chul Park

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…

Instrumentation and Methods for Astrophysics · Physics 2021-03-31 Susana Cebrian

Direct detection dark matter experiments, lead by the CDMS collaboration, have placed increasingly stronger constraints on the cross sections for elastic scattering of WIMPs on nucleons. These results impact the prospects for the indirect…

High Energy Physics - Phenomenology · Physics 2016-09-06 Francis Halzen , Dan Hooper
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