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The detailed origin of the diffuse gamma-ray background is still unknown. However, the contribution of unresolved sources is expected to induce small-scale anisotropies in this emission, which may provide a way to identify and constrain the…

High Energy Astrophysical Phenomena · Physics 2019-08-15 G. A. Gomez-Vargas , A. Cuoco , T. Linden , M. A. Sanchez-Conde , J. M. Siegal-Gaskins , T. Delahaye , M. Fornasa , E. Komatsu , F. Prada , J. Zavala

Dark matter (DM) is a new type of invisible matter introduced to explain various features of recent astrophysical observations, including galaxy rotation curves and other fundamental characteristics of our universe. DM may couple to…

High Energy Physics - Experiment · Physics 2025-06-24 Vindhyawasini Prasad

The focus of dark matter searches to date has been on Weakly Interacting Massive Particles (WIMPs) in the GeV/$c^2$-TeV/$c^2$ mass range. The direct, indirect and collider searches in this mass range have been extensive but ultimately…

A search for dark matter in association with a Higgs boson decaying to two photons is presented. This study is based on data collected with the ATLAS detector, corresponding to an integrated luminosity of 36.1 fb$^{-1}$ of proton--proton…

High Energy Physics - Experiment · Physics 2018-02-15 ATLAS Collaboration

The purpose of this document is to describe the upgrade of the CRESST dark matter search at LNGS. The proposed strategy will allow to explore a region of the parameter space for spin-independent WIMP-nucleon elastic scattering corresponding…

We propose here a set of new methods to directly detect light mass dark matter through its scattering with abundant atmospheric muons or accelerator beams. Firstly, we plan to use the free cosmic-ray muons interacting with dark matter in a…

We present here results from the first-ever search for dark photon dark matter that could have coupled to baryons in LISA Pathfinder, the technology demonstrator for a space-based gravitational-wave antenna. After analyzing approximately…

General Relativity and Quantum Cosmology · Physics 2023-03-15 Andrew L. Miller , Luis Mendes

One of the major challenges of modern physics is to decipher the nature of dark matter. Astrophysical observations provide ample evidence for the existence of an invisible and dominant mass component in the observable universe, from the…

Cosmology and Nongalactic Astrophysics · Physics 2015-09-04 Laura Baudis

We consider new signatures of WIMPless dark matter, particularly those which can be used to test models with low dark matter mass. We focus on detection prospects at hadron colliders through the production of new heavy QCD-coupled…

High Energy Physics - Phenomenology · Physics 2010-11-15 Jason Kumar

Gas time projection chambers (TPCs) with Micromegas pixelated readouts are being used in dark matter searches and other rare event searches, due to their potential in terms of low background levels, energy and spatial resolution, gain, and…

The WIMP proposed here yields the observed abundance of dark matter, and is consistent with the current limits from direct detection, indirect detection, and collider experiments, if its mass is $\sim 72$ GeV/$c^2$. It is also consistent…

High Energy Physics - Phenomenology · Physics 2021-08-02 Reagan Thornberry , Maxwell Throm , Gabriel Frohaug , John Killough , Dylan Blend , Michael Erickson , Brian Sun , Brett Bays , Roland E. Allen

Astrophysical observations indicate that there is roughly five times more dark matter in the Universe than ordinary baryonic matter, with an even larger amount of the Universe's energy content due to dark energy. So far, the microscopic…

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…

Direct detection experiments for dark matter are increasingly ruling out large parameter spaces. However, light dark matter models with particle masses $<$ GeV are still largely unconstrained. Here we examine a proposal to use atom…

High Energy Physics - Phenomenology · Physics 2024-09-09 Yufeng Du , Clara Murgui , Kris Pardo , Yikun Wang , Kathryn M. Zurek

If dark matter stems from the background of a very light gauge boson, this gauge boson could exert forces on test masses in gravitational wave detectors, resulting in displacements with a characteristic frequency set by the gauge boson…

High Energy Physics - Phenomenology · Physics 2018-08-15 Aaron Pierce , Keith Riles , Yue Zhao

Strong gravitational lensing is a powerful probe of the distribution of matter on sub-kpc scales. It can be used to test the existence of completely dark subhalos surrounding galaxies, as predicted by the standard cold dark matter model, or…

Cosmology and Nongalactic Astrophysics · Physics 2023-11-30 Ioana A. Zelko , Anna M. Nierenberg , Tommaso Treu

The NEWS-G direct dark matter search experiment uses spherical proportional counters (SPC) with light noble gases to explore low WIMP masses. The first results obtained with an SPC prototype operated with Ne gas at the Laboratoire…

Instrumentation and Detectors · Physics 2022-03-02 Daniel Durnford , Marie-Cécile Piro

We propose in this White Paper a concept for a space experiment using cold atoms to search for ultra-light dark matter, and to detect gravitational waves in the frequency range between the most sensitive ranges of LISA and the terrestrial…

General Relativity and Quantum Cosmology · Physics 2020-07-22 Yousef Abou El-Neaj , Cristiano Alpigiani , Sana Amairi-Pyka , Henrique Araujo , Antun Balaz , Angelo Bassi , Lars Bathe-Peters , Baptiste Battelier , Aleksandar Belic , Elliot Bentine , Jose Bernabeu , Andrea Bertoldi , Robert Bingham , Diego Blas , Vasiliki Bolpasi , Kai Bongs , Sougato Bose , Philippe Bouyer , Themis Bowcock , William Bowden , Oliver Buchmueller , Clare Burrage , Xavier Calmet , Benjamin Canuel , Laurentiu-Ioan Caramete , Andrew Carroll , Giancarlo Cella , Vassilis Charmandaris , Swapan Chattopadhyay , Xuzong Chen , Maria Luisa Chiofalo , Jonathon Coleman , Joseph Cotter , Yanou Cui , Andrei Derevianko , Albert De Roeck , Goran Djordjevic , Peter Dornan , Michael Doser , Ioannis Drougkakis , Jacob Dunningham , Ioana Dutan , Sajan Easo , Gedminas Elertas , John Ellis , Mai El Sawy , Farida Fassi , Daniel Felea , Chen-Hao Feng , Robert Flack , Chris Foot , Ivette Fuentes , Naceur Gaaloul , Alexandre Gauguet , Remi Geiger , Valerie Gibson , Gian Giudice , Jon Goldwin , Oleg Grachov , Peter W. Graham , Dario Grasso , Maurits van der Grinten , Mustafa Gundogan , Martin G. Haehnelt , Tiffany Harte , Aurelien Hees , Richard Hobson , Bodil Holst , Jason Hogan , Mark Kasevich , Bradley J. Kavanagh , Wolf von Klitzing , Tim Kovachy , Benjamin Krikler , Markus Krutzik , Marek Lewicki , Yu-Hung Lien , Miaoyuan Liu , Giuseppe Gaetano Luciano , Alain Magnon , Mohammed Mahmoud , Sarah Malik , Christopher McCabe , Jeremiah Mitchell , Julia Pahl , Debapriya Pal , Saurabh Pandey , Dimitris Papazoglou , Mauro Paternostro , Bjoern Penning , Achim Peters , Marco Prevedelli , Vishnupriya Puthiya-Veettil , John Quenby , Ernst Rasel , Sean Ravenhall , Haifa Rejeb Sfar , Jack Ringwood , Albert Roura , Dylan Sabulsky , Muhammed Sameed , Ben Sauer , Stefan Alaric Schaffer , Stephan Schiller , Vladimir Schkolnik , Dennis Schlippert , Christian Schubert , Armin Shayeghi , Ian Shipsey , Carla Signorini , Marcelle Soares-Santos , Fiodor Sorrentino , Yajpal Singh , Timothy Sumner , Konstantinos Tassis , Silvia Tentindo , Guglielmo Maria Tino , Jonathan N. Tinsley , James Unwin , Tristan Valenzuela , Georgios Vasilakis , Ville Vaskonen , Christian Vogt , Alex Webber-Date , Andre Wenzlawski , Patrick Windpassinger , Marian Woltmann , Michael Holynski , Efe Yazgan , Ming-Sheng Zhan , Xinhao Zou , Jure Zupan

We developed a three-dimensional gaseous tracking device and performed a direction-sensitive dark matter search in a surface laboratory. By using 150 Torr carbon-tetrafluoride (CF_4 gas), we obtained a sky map drawn with the recoil…

A method to search for dark matter by studying the interaction of accelerator beam particles with residual gas in dependence on gas pressure is proposed. The sensitivity of the method is estimated.

High Energy Physics - Experiment · Physics 2009-09-29 Victor Kryshkin
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