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Dark matter may interact with the Standard Model through the kinetic mixing of dark photons, $A'$, with Standard Model photons. Such dark matter will accumulate in the Sun and annihilate into dark photons. The dark photons may then leave…

High Energy Physics - Phenomenology · Physics 2017-10-05 Jonathan L. Feng , Jordan Smolinsky , Philip Tanedo

In this contribution an entirely different way compared to conventional approaches for axion, hidden photon and dark matter (DM) detection is proposed for discussion. The idea is to use living plants which are known to be very sensitive to…

High Energy Physics - Experiment · Physics 2015-09-29 Fritz Caspers

The search for dark matter is one of the main science drivers of the particle and astroparticle physics communities. Determining the nature of dark matter will require a broad approach, with a range of experiments pursuing different…

An ultra-light axion with CP violating interactions with a dark sector and CP preserving interactions with the visible sector can act as a novel portal between dark matter and the Standard Model. In such theories, dark matter sources an…

High Energy Physics - Phenomenology · Physics 2024-12-12 Edward Hardy , Mario Reig , Juri Smirnov

The study of collision events with missing energy as searches for the dark matter (DM) component of the Universe are an essential part of the extensive program looking for new physics at the LHC. Given the unknown nature of DM, the…

Several models of particle physics different from the Standard Model predict the existence of a dark sector that is weakly coupled to the visible one: the two sectors may couple via the vector portal, where a dark photon with mass in the…

High Energy Physics - Experiment · Physics 2018-12-20 Daniela Salvatore

The most compelling candidates for Dark Matter to day are WIMPs and axions. The applicability of gasesous Time Projection Chambers (TPCs) with Micromesh Gas Structures (Micromegas) to the search of these particles is explored within this…

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,…

High Energy Astrophysical Phenomena · Physics 2012-06-15 Lars Bergström

Asymmetric dark matter (ADM) is motivated by the similar cosmological mass densities measured for ordinary and dark matter. We present a comprehensive theory for ADM that addresses the mass density similarity, going beyond the usual ADM…

High Energy Physics - Phenomenology · Physics 2018-05-23 Stephen J. Lonsdale , Raymond R. Volkas

Assuming that cosmological dark matter consists of weakly interacting massive particles, we use the recent precise measurement of cosmological parameters to predict the guaranteed rates of production of such particles in association with…

High Energy Physics - Phenomenology · Physics 2009-10-09 Andreas Birkedal , Konstantin Matchev , Maxim Perelstein

This is one chapter of the collection of problems in cosmology, in which we assemble the problems that concern one of the most distinctive features of modern cosmology---the interaction in the Dark Sector. The evolution of any broadly…

Physics Education · Physics 2013-12-24 Yu. L. Bolotin , V. A. Cherkaskiy , O. A. Lemets , I. V. Tanatarov , D. A. Yerokhin

The GAPS experiment is foreseen to carry out a dark matter search using a novel detection approach to detect low-energy cosmic-ray antideuterons. The theoretically predicted antideuteron flux resulting from secondary interactions of primary…

Instrumentation and Methods for Astrophysics · Physics 2010-12-02 Ph. von Doetinchem , T. Aramaki , St. Boggs , W. Craig , H. Fuke , F. Gahbauer , Ch. Hailey , J. Koglin , N. Madden , I. Mognet , K. Mori , R. Ong , T. Yoshida , T. Zhang , J. Zweerink

In the present work we examine the possibility of detecting light dark matter particles (WIMP) utilizing their possible interactions with the electrons. Employing reasonable theoretical models we evaluate the expected event rates in the…

High Energy Physics - Phenomenology · Physics 2019-04-11 J. D. Vergados

In the general scenario of Weakly Interacting Massive Particles (WIMP), dark matter (DM) can be observed via astrophysical gamma rays because photons are produced in various DM annihilation or decay processes, either as broad-band or line…

High Energy Astrophysical Phenomena · Physics 2015-06-19 Michele Doro

Composite asymmetric dark matter (ADM) is the framework that naturally explains the coincidence of the baryon density and the dark matter density of the Universe. Through a portal interaction sharing particle-antiparticle asymmetries in the…

High Energy Physics - Phenomenology · Physics 2025-08-07 Saikat Das , Ayuki Kamada , Takumi Kuwahara , Kohta Murase , Deheng Song

We address the question of whether the upcoming generation of dark matter search experiments and colliders will be able to discover if the dark matter in the Universe has two components of weakly interacting massive particles (WIMPs). We…

High Energy Physics - Phenomenology · Physics 2009-12-23 Stefano Profumo , Kris Sigurdson , Lorenzo Ubaldi

Axions and other very weakly interacting slim particles (WISPs), with masses below 1 GeV, arise naturally in many extensions of the Standard Model of particle physics. In particular, they could offer a new framework to explain the nature of…

High Energy Physics - Phenomenology · Physics 2026-03-05 Ariel Arza , Deniz Aybas , Shyam Balaji , Reuven Balkin , Kai Bartnick , Charles F. A. Baynham , Itay M. Bloch , Claudio Bonati , Dmitry Budker , Clare Burrage , Malte Buschmann , Francesca Calore , Francisco R. Candón , Pierluca Carenza , Serkant Ali Cetin , Francesca Chadha-Day , Sreemanti Chakraborti , Kiwoon Choi , Michele Cicoli , Lei Cong , Joseph P. Conlon , Florin Lucian Constantin , José Correia , Claudia De Dominicis , Arturo de Giorgi , Pedro De la Torre Luque , Javier De Miguel , Francesco D'Eramo , Alejandro Díaz-Morcillo , Patricia Diego-Palazuelos , David Díez-Ibáñez , Luca Di Luzio , Amelia Drew , Babette Döbrich , Christopher Eckner , Aldo Ejlli , Sebastian A. R. Ellis , Angelo Esposito , Elisa Ferreira , Nahuel Ferreiro Iachellini , Damiano F. G. Fiorillo , Matteo Galaverni , Michele Gallinaro , Camilo García-Cely , Silvia Gasparotto , Claudio Gatti , Daniel Gavilan-Martin , Maurizio Giannotti , Benito Gimeno , Marco Gorghetto , Giovanni Grilli di Cortona , Jordan Gué , Gerard Higgins , Dieter Horns , Mathieu Kaltschmidt , Marin Karuza , Venelin Kozhuharov , Stepan Kunc , Francesca Lecce , Alessandro Lella , Axel Lindner , Maria Paola Lombardo , Giuseppe Lucente , Olympia Maliaka , Cristina Margalejo , Marios Maroudas , Luca Marsicano , Luca Merlo , Alessandro Mirizzi , Vasiliki A. Mitsou , Guido Mueller , Kai Murai , Toshiya Namikawa , Fumihiro Naokawa , Le Hoang Nguyen , Ciaran O'Hare , Tomas O'Shea , Ippei Obata , Ali Övgün , Francisco Gil Pedro , Giovanni Pierobon , Tanmay Kumar Poddar , Josef Pradler , Pierre Pugnat , Beyhan Puliçe , Raquel Quishpe , Georg G. Raffelt , Maria Ramos , Wolfram Ratzinger , Marco Regis , Mario Reig , Sophie Renner , Alessio Rettaroli , Nicole Righi , Andreas Ringwald , Laura R. Roberts , Keir K. Rogers , Qazal Rokn , Ophir M. Ruimi , Jaime Ruz , Kenichi Saikawa , Marco Scalisi , Andreas Schachner , Joern Schaffran , Kristof Schmieden , Matthias Schott , Javi Serra , Anton Sokolov , Paolo Spagnolo , Konstantin Springmann , Michael Staelens , Stefan Stelzl , Oscar Straniero , Marco Taoso , Elisa Todarello , Claudio Toni , Lorenzo Ubaldi , Federico Urban , Rodrigo Vicente , Luca Visinelli , Edoardo Vitagliano , Julia K. Vogel , Andreas Weiler , Samuel J. Witte , Michael Wurm , Wen Yin , Konstantin Zioutas

Searches for dark matter (DM) have not provided any solid evidence for the existence of weakly interacting massive particles in the GeV-TeV mass range. Coincidentally, the scale of new physics is being pushed by collider searches well…

High Energy Astrophysical Phenomena · Physics 2022-07-06 A. Albert , S. Alves , M. Andre , M. Anghinolfi , G. Anton , M. Ardid , S. Ardid , J. -J. Aubert , J. Aublin , B. Baret , S. Basa , B. Belhorma , M. Bendahman , F. Benfenati , V. Bertin , S. Biagi , M. Bissinger , J. Boumaaza , M. Bouta , M. C. Bouwhuis , H. Branzas , R. Bruijn , J. Brunner , J. Busto , B. Caiffi , D. Calvo , A. Capone , L. Caramete , J. Carr , V. Carretero , S. Celli , M. Chabab , T. N. Chau , R. Cherkaoui El Moursli , T. Chiarusi , M. Circella , A. Coleiro , R. Coniglione , P. Coyle , A. Creusot , A. F. Diaz , G. de Wasseige , C. Distefano , I. Di Palma , A. Domi , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , T. van Eeden , D. van Eijk , N. El Khayati , A. Enzenhoefer , P. Fermani , G. Ferrara , F. Filippini , L. Fusco , Y. Gatelet , P. Gay , H. Glotin , R. Gozzini , R. Gracia Ruiz , K. Graf , C. Guidi , S. Hallmann , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernandez-Rey , J. Hoessl , J. Hofestaedt , F. Huang , G. Illuminati , C. W. James , B. Jisse-Jung , M. de Jong , P. de Jong , M. Kadler , O. Kalekin , U. Katz , N. R. Khan-Chowdhury , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , C. Lagunas Gualda , R. Lahmann , R. Le Breton , S. LeStum , D. Lefevre , E. Leonora , G. Levi , M. Lincetto , D. Lopez-Coto , S. Loucatos , L. Maderer , J. Manczak , M. Marcelin , A. Margiotta , A. Marinelli , J. A. Martinez-Mora , B. Martino , K. Melis , P. Migliozzi , A. Moussa , R. Muller , L. Nauta , S. Navas , E. Nezri , B. O Fearraigh , A. Paun , G. E. Pavalas , C. Pellegrino , M. Perrin-Terrin , V. Pestel , P. Piattelli , C. Pieterse , C. Poire , V. Popa , T. Pradier , N. Randazzo , D. Real , S. Reck , G. Riccobene , A. Romanov , F. Sala , A. Sanchez-Losa , F. Salesa Greus , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schnabel , J. Schumann , F. Schuessler , J. Seneca , M. Spurio , Th. Stolarczyk , M. Taiuti , Y. Tayalati , S. J. Tingay , B. Vallage , V. Van Elewyck , F. Versari , S. Viola , D. Vivolo , J. Wilms , S. Zavatarelli , A. Zegarelli , J. D. Zornoza , J. Zuniga

Experiments aiming to directly detect dark matter (DM) particles have yet to make robust detections, thus underscoring the need for complementary approaches such as searches for new particles at colliders, and indirect DM searches in…

Anomalous production of low-energy photons from the galactic center have fueled speculations on the nature and properties of dark matter particles. In particular, it has been proposed that light scalars may be responsible for the bulk of…

High Energy Physics - Experiment · Physics 2007-12-13 Sven Heinemeyer , Yonatan Kahn , Michael Schmitt , Mayda Velasco
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