English
Related papers

Related papers: The DESY axion search program

200 papers

Weakly Interacting Massive Particles (WIMPs, $\chi$) are candidates for Dark Matter. WIMP searches at lepton colliders are complementary to searches at hadron colliders and direct and indirect detection, since they directly probe the…

High Energy Physics - Experiment · Physics 2017-02-20 Moritz Habermehl , Keisuke Fujii , Jenny List , Shigeki Matsumoto , Tomohiko Tanabe

We review the current status of axions as dark matter. Motivation, models, constraints and experimental searches are outlined. The axion remains an excellent candidate for the dark matter and future experiments, particularly the Axion Dark…

High Energy Physics - Phenomenology · Physics 2009-11-19 Leanne D. Duffy , Karl van Bibber

We propose simple freeze-in models where the observed dark matter abundance is explained via the decay of an electrically charged and/or coloured parent particle into Feebly Interacting Massive Particles (FIMP). The parent particle is…

High Energy Physics - Phenomenology · Physics 2019-03-27 G. Bélanger , N. Desai , A. Goudelis , J. Harz , A. Lessa , J. M. No , A. Pukhov , S. Sekmen , D. Sengupta , B. Zaldivar , J. Zurita

Axionlike particles (ALPs) are a common prediction of theories beyond the Standard Model of particle physics that could explain the entirety of the cold dark matter. These particles could be detected through their mixing with photons in…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Manuel Meyer

The era of precision cosmology has revealed that about 85% of the matter in the universe is dark matter. Two well-motivated candidates are weakly interacting massive particles (WIMPs) and weakly interacting sub-eV particles (WISPs) (e.g.…

We are conducting an experiment to search for WIMPs, or weakly-interacting massive particles, in the galactic halo using terrestrial detectors. This generic class of hypothetical particles, whose properties are similar to those predicted by…

This article describes BabyIAXO, an intermediate experimental stage of the International Axion Observatory (IAXO), proposed to be sited at DESY. IAXO is a large-scale axion helioscope that will look for axions and axion-like particles…

Instrumentation and Detectors · Physics 2021-03-05 A. Abeln , K. Altenmüller , S. Arguedas Cuendis , E. Armengaud , D. Attié , S. Aune , S. Basso , L. Bergé , B. Biasuzzi , P. T. C. Borges De Sousa , P. Brun , N. Bykovskiy , D. Calvet , J. M. Carmona , J. F. Castel , S. Cebrián , V. Chernov , F. E. Christensen , M. M. Civitani , C. Cogollos , T. Dafní , A. Derbin , K. Desch , D. Díez , M. Dinter , B. Döbrich , I. Drachnev , A. Dudarev , L. Dumoulin , D. D. M. Ferreira , E. Ferrer-Ribas , I. Fleck , J. Galán , D. Gascón , L. Gastaldo , M. Giannotti , Y. Giomataris , A. Giuliani , S. Gninenko , J. Golm , N. Golubev , L. Hagge , J. Hahn , C. J. Hailey , D. Hengstler , P. L. Henriksen , T. Houdy , R. Iglesias-Marzoa , F. J. Iguaz , I. G. Irastorza , C. Iñiguez , K. Jakovcic , J. Kaminski , B. Kanoute , S. Karstensen , L. Kravchuk , B. Lakic , T. Lasserre , P. Laurent , O. Limousin , A. Lindner , M. Loidl , I. Lomskaya , G. López-Alegre , B. Lubsandorzhiev , K. Ludwig , G. Luzón , C. Malbrunot , C. Margalejo , A. Marin-Franch , S. Marnieros , F. Marutzky , J. Mauricio , Y. Menesguen , M. Mentink , S. Mertens , F. Mescia , J. Miralda-Escudé , H. Mirallas , J. P. Mols , V. Muratova , X. F. Navick , C. Nones , A. Notari , A. Nozik , L. Obis , C. Oriol , F. Orsini , A. Ortiz de Solórzano , S. Oster , H. P. Pais Da Silva , V. Pantuev , T. Papaevangelou , G. Pareschi , K. Perez , O. Pérez , E. Picatoste , M. J. Pivovaroff , D. V. Poda , J. Redondo , A. Ringwald , M. Rodrigues , F. Rueda-Teruel , S. Rueda-Teruel , E. Ruiz-Choliz , J. Ruz , E. O. Saemann , J. Salvado , T. Schiffer , S. Schmidt , U. Schneekloth , M. Schott , L. Segui , F. Tavecchio , H. H. J. ten Kate , I. Tkachev , S. Troitsky , D. Unger , E. Unzhakov , N. Ushakov , J. K. Vogel , D. Voronin , A. Weltman , U. Werthenbach , W. Wuensch , A. Yanes-Díaz

Astrophysical observations indicate that about 23% of the energy density of the universe is in the form of non-baryonic particles beyond the standard model of particle physics. One exciting and well motivated candidate is the lightest…

Astrophysics · Physics 2008-11-26 Richard W. Schnee

The Standard Model has achieved significant success in particle physics; however, there are still some unresolved puzzles beyond it. This motivates the exploration of the dark sector. We present the recent dark sector search results from…

High Energy Physics - Experiment · Physics 2025-07-31 Zhijun Li , Zhengyun You

Axion-like particles (ALPs) are hypothetical entities often invoked to solve various problems in particle physics to cosmology. They are one of the most promising candidates to explain the elusive dark matter. A way to search for ALPs is…

High Energy Physics - Phenomenology · Physics 2023-08-29 Rafael Alves Batista , Cristina Viviente , Gaetano Di Marco , Miguel A. Sánchez-Conde

In this work we consider searches for dark matter made of axions or axion-like particles (ALPs) using resonant radio frequency cavities inserted into dipole magnets from particle accelerators, wiggler magnets developed for accelerator based…

The axion is a highly motivated elementary particle which could address two fundamental questions in physics - the strong CP problem and the dark matter mystery. Experimental searches for this hypothetical particle have started to reach…

High Energy Physics - Phenomenology · Physics 2021-10-28 Yannis K. Semertzidis , SungWoo Youn

Dark matter is thought to make up most of the matter density of the Universe, yet its true nature remains uncertain. Among dark matter theories, Weakly Interacting Massive Particles (WIMPs) are a prominent candidate for dark matter because…

High Energy Astrophysical Phenomena · Physics 2023-09-20 Micael Andrade , Aion Viana

We argue in favor of the existence of the LIPs, the least interacting particles, which would only interact with ordinary matter through gravitational field and could account for (at least) part of the dark matter. The detectability of LIP…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. E. A. Matsas , J. C. Montero , V. Pleitez , D. A. T. Vanzella

Pseudo-feebly Interacting Massive Particle (pFIMP) has been postulated in two component dark matter (DM) scenarios, where it has feeble interaction with the visible sector, but sizeable one with a thermal bath partner. In this work, we…

High Energy Physics - Phenomenology · Physics 2024-11-25 Subhaditya Bhattacharya , Dipankar Pradhan , Jahaan Thakkar

We review theoretically well-motivated dark-matter candidates, and pathways to their discovery, in the light of recent results from collider physics, astrophysics, and cosmology. Taken in aggregate, these encourage broader thinking in…

High Energy Physics - Phenomenology · Physics 2015-06-15 Susan Gardner , George Fuller

The identity of dark matter is a question of central importance in both astrophysics and particle physics. In the past, the leading particle candidates were cold and collisionless, and typically predicted missing energy signals at particle…

Cosmology and Nongalactic Astrophysics · Physics 2011-02-03 Jonathan L. Feng

The leading direct dark matter search experiments: CDMS, Edelweis and DAMA/NaI exhibit different results for different approaches to the problem. This contradiction can reflect a nontrivial and probably a multi-component nature of the…

Astrophysics · Physics 2007-05-23 K. Belotsky , Yu. Bunkov , H. Godfrin , M. Khlopov , R. Konoplich

Dark matter (DM) plays a crucial role in explaining the observed astrophysical anomalies, galaxy rotation curves, and other fundamental characteristics of the Universe. Many extensions of the Standard Model (SM), such as the dark…

High Energy Physics - Experiment · Physics 2025-10-16 Vindhyawasini Prasad

Light axion-like particles occur in many theories of beyond-Standard-Model physics, and may make up some or all of the universe's dark matter. One of the ways they can couple to the Standard Model is through the electromagnetic $F_{\mu\nu}…

High Energy Physics - Phenomenology · Physics 2021-04-14 Robert Lasenby
‹ Prev 1 4 5 6 7 8 10 Next ›