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The search for particle-like dark matter with meV-to-GeV masses has developed rapidly in the past few years. We summarize the science case for these searches, the recent progress, and the exciting upcoming opportunities. Funding for…

This white paper discusses the current landscape and prospects for experiments sensitive to particle dark matter processes producing photons and cosmic rays. Much of the gamma-ray sky remains unexplored on a level of sensitivity that would…

In recent years, the sensitivity of opto-mechanical force sensors has improved leading to increased interest in using these devices as particle detectors. In this study we consider scenarios where dark matter with mass close to the Planck…

高能物理 - 唯象学 · 物理学 2022-12-09 Carlos Blanco , Bahaa Elshimy , Rafael F. Lang , Robert Orlando

Dark matter candidates with masses around the Planck-scale are theoretically well-motivated, and it has been suggested that it might be possible to search for dark matter solely via gravitational interactions in this mass range. In this…

We present a summary of future prospects for direct detection of dark matter within the GeV/c2 to TeV/c2 mass range. This is paired with a new definition of the neutrino fog in order to better quantify the rate of diminishing returns on…

Detecting dark matter directly using sensitive underground detectors is one of the most promising ways to address the question of what is dark matter. The next generation underground experiments will search for dark matter in two…

高能物理 - 实验 · 物理学 2022-12-05 J. Cooley , S. Hertel , H. Lippincott , K. Ni , E. Pantic

The identification of the nature of dark matter is one of the most important problems confronting particle physics. Current observational constraints permit the mass of the dark matter to range from $10^{-22}$ eV - $10^{48}$ GeV. Given the…

高能物理 - 唯象学 · 物理学 2022-04-08 Surjeet Rajendran

The absence of clear signals from particle dark matter in direct detection experiments motivates new approaches in disparate regions of viable parameter space. In this Snowmass white paper, we outline the Windchime project, a program to…

Our limited understanding of the physical properties of matter at ultra-high density, high proton/neutron number asymmetry, and low temperature is presently one of the major outstanding problems in physics. As matter in this extreme state…

The current understanding of dark matter comes largely from measurements of the total matter content in the universe, from the distribution of gravitating matter on very large scales, and from rotation curves and velocity dispersions on…

A TeV scale electroweak particle is a well motivated candidate for the dark matter (DM) of our Universe. Yet such a particle may only be detectable using indirect detection instruments sensitive to TeV-scale gamma rays that can result from…

高能天体物理现象 · 物理学 2019-09-05 Lucia Rinchiuso , Nicholas L. Rodd , Emmanuel Moulin , Tracy R. Slatyer

I suggest a simple signature for new particles which are unstable partners of a dark matter particle. The suggested mass range is from 8 TeV to 3 PeV, the former being the mass of the dark matter particle and the latter being the knee…

高能物理 - 唯象学 · 物理学 2012-07-12 Yukio Tomozawa

The current generation of Dark Matter Direct Detection Experiments has ruled out a large region of parameter space for dark matter, particularly in the ($10 - 1000$) GeV mass range. However, due to very low event rates, searching for dark…

高能物理 - 唯象学 · 物理学 2024-12-19 Praveen Bharadwaj , Ranjeet Kumar , Hemant Kumar Prajapati , Rahul Srivastava , Sushant Yadav

For decades, searches for electroweak-scale dark matter (DM) have been performed without a definitive detection. This lack of success may hint that DM searches have focused on the wrong mass range. A proposed candidate beyond the canonical…

高能天体物理现象 · 物理学 2022-10-26 Donggeun Tak , Matthew Baumgart , Nicholas L. Rodd , Elisa Pueschel

We consider the possibility that the cosmological dark matter consists of particles very close in mass to new colored particles below the TeV scale. While such a scenario is inherently difficult to directly confirm at colliders, we find…

高能物理 - 唯象学 · 物理学 2012-03-05 Masaki Asano , Torsten Bringmann , Christoph Weniger

We present an overview of future observational facilities that will significantly enhance our understanding of the fundamental nature of dark matter. These facilities span a range of observational techniques including optical/near-infrared…

This report summarizes the findings of the CF1 Topical Subgroup to Snowmass 2021, which was focused on particle dark matter. One of the most important scientific goals of the next decade is to reveal the nature of dark matter (DM). To…

Powerful new observational facilities will come online over the next decade, enabling a number of discovery opportunities in the "Cosmic Frontier", which targets understanding of the physics of the early universe, dark matter and dark…

The last decade has seen unprecedented effort in dark matter model building at all mass scales coupled with the design of numerous new detection strategies. Transformative advances in quantum technologies have led to a plethora of new…

高能物理 - 实验 · 物理学 2022-03-29 D. Antypas , A. Banerjee , C. Bartram , M. Baryakhtar , J. Betz , J. J. Bollinger , C. Boutan , D. Bowring , D. Budker , D. Carney , G. Carosi , S. Chaudhuri , S. Cheong , A. Chou , M. D. Chowdhury , R. T. Co , J. R. Crespo López-Urrutia , M. Demarteau , N. DePorzio , A. V. Derbin , T. Deshpande , M. D. Chowdhury , L. Di Luzio , A. Diaz-Morcillo , J. M. Doyle , A. Drlica-Wagner , A. Droster , N. Du , B. Döbrich , J. Eby , R. Essig , G. S. Farren , N. L. Figueroa , J. T. Fry , S. Gardner , A. A. Geraci , A. Ghalsasi , S. Ghosh , M. Giannotti , B. Gimeno , S. M. Griffin , D. Grin , D. Grin , H. Grote , J. H. Gundlach , M. Guzzetti , D. Hanneke , R. Harnik , R. Henning , V. Irsic , H. Jackson , D. F. Jackson Kimball , J. Jaeckel , M. Kagan , D. Kedar , R. Khatiwada , S. Knirck , S. Kolkowitz , T. Kovachy , S. E. Kuenstner , Z. Lasner , A. F. Leder , R. Lehnert , D. R. Leibrandt , E. Lentz , S. M. Lewis , Z. Liu , J. Manley , R. H. Maruyama , A. J. Millar , V. N. Muratova , N. Musoke , S. Nagaitsev , O. Noroozian , C. A. J. O'Hare , J. L. Ouellet , K. M. W. Pappas , E. Peik , G. Perez , A. Phipps , N. M. Rapidis , J. M. Robinson , V. H. Robles , K. K. Rogers , J. Rudolph , G. Rybka , M. Safdari , M. Safdari , M. S. Safronova , C. P. Salemi , P. O. Schmidt , T. Schumm , A. Schwartzman , J. Shu , M. Simanovskaia , J. Singh , S. Singh , M. S. Smith , W. M. Snow , Y. V. Stadnik , C. Sun , A. O. Sushkov , T. M. P. Tait , V. Takhistov , D. B. Tanner , D. J. Temples , P. G. Thirolf , J. H. Thomas , M. E. Tobar , O. Tretiak , Y. -D. Tsai , J. A. Tyson , M. Vandegar , S. Vermeulen , L. Visinelli , E. Vitagliano , Z. Wang , D. J. Wilson , L. Winslow , S. Withington , M. Wooten , J. Yang , J. Ye , B. A. Young , F. Yu , M. H. Zaheer , T. Zelevinsky , Y. Zhao , K. Zhou
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