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Once the energy spectrum of the secondary component is well understood, measurements of the antiproton cosmic-ray flux at the Earth will be a powerful way to indirectly probe for the existence of supersymmetric relics in the galactic halo.…

高能物理 - 唯象学 · 物理学 2008-11-26 F. Donato , N. Fornengo , P. Salati

Lithium-drifted silicon [Si(Li)] has been used for decades as an ionizing radiation detector in nuclear, particle, and astrophysical experiments, though such detectors have frequently been limited to small sizes (few cm$^2$) and cryogenic…

The detection of non-baryonic dark matter through its gamma-ray annihilation in the centre of our galaxy has been studied. The gamma fluxes according to different models have been simulated and compared to those expected to be observed with…

A search for new phenomena in events with a high-energy jet and large missing transverse momentum is performed using data from proton-proton collisions at sqrt(s)=7 TeV with the ATLAS experiment at the Large Hadron Collider. Four kinematic…

高能物理 - 实验 · 物理学 2013-06-11 The ATLAS Collaboration

Dark matter is five times more abundant than ordinary visible matter in our Universe. While laboratory searches hunting for dark matter have traditionally focused on the electroweak scale, theories of low mass hidden sectors motivate new…

高能物理 - 实验 · 物理学 2023-02-08 S. A. Lyon , Kyle Castoria , Ethan Kleinbaum , Zhihao Qin , Arun Persaud , Thomas Schenkel , Kathryn Zurek

In the last decade, Direct Dark Matter searches has become a very active research program, spawning dozens of projects world wide and leading to contradictory results. It is on this stage that the Dark matter Experiment with liquid Argon…

天体物理仪器与方法 · 物理学 2014-06-03 P. Gorel

Antinuclei are considered to be one of the most promising probes in the indirect search for dark matter (DM) annihilation in space. However, in light of recent results on the production of light antinuclei in pp collisions at the LHC, an…

核实验 · 物理学 2021-04-29 Sebastian Hornung

The mysterious dark matter has been a subject of special interest to high energy physicists, astrophysicists and cosmologists for many years. According to theoretical models, it can make up a significant fraction of the mass of the…

天体物理学 · 物理学 2007-05-23 A. Moiseev , J. Ormes , H. Arrighi , E. Bloom , C. Chaput , S. Digel , D. Engovatov , J. Norris , J. Silvis

Precision astrometry offers a way to probe new physics. By measuring the angular position of light sources at unprecedented precision, astrometry could probe minuscule fluctuations of underlying spacetime. This work explores the possibility…

高能物理 - 唯象学 · 物理学 2024-06-07 Hyungjin Kim

The Heavy Photon Search (HPS) experiment searches for an electro-produced dark photon using an electron beam provided by the CEBAF accelerator at the Thomas Jefferson National Accelerator Facility. HPS has successfully completed two…

高能物理 - 实验 · 物理学 2019-10-14 Cameron Bravo

Besides the detection of high energy neutrinos, the ANTARES telescope offers an opportunity to improve sensitivity to exotic cosmological relics. In this article we discuss the sensitivity of the ANTARES detector to elativistic monopoles…

天体物理仪器与方法 · 物理学 2019-08-13 Gabriela Pavalas , Nicolas Picot Clemente

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…

高能物理 - 实验 · 物理学 2010-11-30 L. Baudis , G. Heusser , B. Majorovits , Y. Ramachers , H. Strecker , H. V. Klapdor--Kleingrothaus

Weakly Interacting Massive Particles (WIMPs) are one of the best motivated candidates to compose the Dark Matter of the Universe. The lack of experimental confirmation by direct detection experiments or collider searches has ruled out…

仪器与探测器 · 物理学 2025-07-04 Oscar Perez

We explore paleo-detectors as an approach to the direct detection of Weakly Interacting Massive Particle (WIMP) dark matter radically different from conventional detectors. Instead of instrumenting a (large) target mass in a laboratory in…

宇宙学与河外天体物理 · 物理学 2019-02-28 Andrzej K. Drukier , Sebastian Baum , Katherine Freese , Maciej Górski , Patrick Stengel

The details of what constitutes the majority of the mass that makes up dark matter in the Universe remains one of the prime puzzles of cosmology and particle physics today - eighty years after the first observational indications. Today, it…

高能天体物理现象 · 物理学 2015-12-16 Stefan Funk

A new generation of upcoming space-based experiments will soon start to probe the spectrum of cosmic ray antiparticles with an unprecedented accuracy and, in particular, will open up a window to energies much higher than those accessible so…

天体物理学 · 物理学 2008-11-26 Torsten Bringmann , Pierre Salati

Various astrophysical observations point towards an as-of-yet unexplained, mainly gravitationally interacting type of matter. If this matter, called Dark Matter, is an elementary particle, it could be produced in particle collisions at the…

高能物理 - 实验 · 物理学 2024-07-18 Martin Habedank

Indirect dark matter detection methods are used to observe the products of dark matter annihilations or decays originating from astrophysical objects where large amounts of dark matter are thought to accumulate. With neutrino telescopes, an…

高能天体物理现象 · 物理学 2025-02-18 KM3NeT Collaboration , S. Aiello , A. Albert , A. R. Alhebsi , M. Alshamsi , S. Alves Garre , A. Ambrosone , F. Ameli , M. Andre , L. Aphecetche , M. Ardid , S. Ardid , J. Aublin , F. Badaracco , L. Bailly-Salins , Z. Bardačová , B. Baret , A. Bariego-Quintana , Y. Becherini , M. Bendahman , F. Benfenati , M. Benhassi , M. Bennani , D. M. Benoit , E. Berbee , V. Bertin , S. Biagi , M. Boettcher , D. Bonanno , A. B. Bouasla , J. Boumaaza , M. Bouta , M. Bouwhuis , C. Bozza , R. M. Bozza , H. Brânzăş , F. Bretaudeau , M. Breuhaus , R. Bruijn , J. Brunner , R. Bruno , E. Buis , R. Buompane , J. Busto , B. Caiffi , D. Calvo , A. Capone , F. Carenini , V. Carretero , T. Cartraud , P. Castaldi , V. Cecchini , S. Celli , L. Cerisy , M. Chabab , A. Chen , S. Cherubini , T. Chiarusi , M. Circella , R. Clark , R. Cocimano , J. A. B. Coelho , A. Coleiro , A. Condorelli , R. Coniglione , P. Coyle , A. Creusot , G. Cuttone , R. Dallier , A. De Benedittis , B. De Martino , G. De Wasseige , V. Decoene , I. Del Rosso , L. S. Di Mauro , I. Di Palma , A. F. Díaz , D. Diego-Tortosa , C. Distefano , A. Domi , C. Donzaud , D. Dornic , E. Drakopoulou , D. Drouhin , J. -G. Ducoin , R. Dvornický , T. Eberl , E. Eckerová , A. Eddymaoui , T. van Eeden , M. Eff , D. van Eijk , I. El Bojaddaini , S. El Hedri , V. Ellajosyula , A. Enzenhöfer , G. Ferrara , M. D. Filipović , F. Filippini , D. Franciotti , L. A. Fusco , S. Gagliardini , T. Gal , J. García Méndez , A. Garcia Soto , C. Gatius Oliver , N. Geißelbrecht , E. Genton , H. Ghaddari , L. Gialanella , B. K. Gibson , E. Giorgio , I. Goos , P. Goswami , S. R. Gozzini , R. Gracia , C. Guidi , B. Guillon , M. Gutiérrez , C. Haack , H. van Haren , A. Heijboer , L. Hennig , J. J. Hernández-Rey , W. Idrissi Ibnsalih , G. Illuminati , D. Joly , M. de Jong , P. de Jong , B. J. Jung , G. Kistauri , C. Kopper , A. Kouchner , Y. Y. Kovalev , V. Kueviakoe , V. Kulikovskiy , R. Kvatadze , M. Labalme , R. Lahmann , M. Lamoureux , G. Larosa , C. Lastoria , J. Lazar , A. Lazo , S. Le Stum , G. Lehaut , V. Lemaître , E. Leonora , N. Lessing , G. Levi , M. Lindsey Clark , F. Longhitano , F. Magnani , J. Majumdar , L. Malerba , F. Mamedov , A. Manfreda , M. Marconi , A. Margiotta , A. Marinelli , C. Markou , L. Martin , M. Mastrodicasa , S. Mastroianni , J. Mauro , G. Miele , P. Migliozzi , E. Migneco , M. L. Mitsou , C. M. Mollo , L. Morales-Gallegos , A. Moussa , I. Mozun Mateo , R. Muller , M. R. Musone , M. Musumeci , S. Navas , A. Nayerhoda , C. A. Nicolau , B. Nkosi , B. Ó Fearraigh , V. Oliviero , A. Orlando , E. Oukacha , D. Paesani , J. Palacios González , G. Papalashvili , V. Parisi , E. J. Pastor Gómez , C. Pastore , A. M. Păun , G. E. Păvălaş , S. Peña Martínez , M. Perrin-Terrin , V. Pestel , R. Pestes , P. Piattelli , A. Plavin , C. Poiré , V. Popa , T. Pradier , J. Prado , S. Pulvirenti , C. A. Quiroz-Rangel , N. Randazzo , S. Razzaque , I. C. Rea , D. Real , G. Riccobene , A. Romanov , E. Ros , A. Šaina , F. Salesa Greus , D. F. E. Samtleben , A. Sánchez Losa , S. Sanfilippo , M. Sanguineti , D. Santonocito , P. Sapienza , J. Schnabel , J. Schumann , H. M. Schutte , J. Seneca , N. Sennan , P. Sevle , I. Sgura , R. Shanidze , A. Sharma , Y. Shitov , F. Šimkovic , A. Simonelli , A. Sinopoulou , B. Spisso , M. Spurio , D. Stavropoulos , I. Štekl , M. Taiuti , G. Takadze , Y. Tayalati , H. Thiersen , S. Thoudam , I. Tosta e Melo , B. Trocmé , V. Tsourapis , A. Tudorache , E. Tzamariudaki , A. Ukleja , A. Vacheret , V. Valsecchi , V. Van Elewyck , G. Vannoye , G. Vasileiadis , F. Vazquez de Sola , A. Veutro , S. Viola , D. Vivolo , A. van Vliet , E. de Wolf , I. Lhenry-Yvon , S. Zavatarelli , A. Zegarelli , D. Zito , J. D. Zornoza , J. Zúñiga , N. Zywucka