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Direct and indirect dark matter detection relies on the scattering of the dark matter candidate on nucleons or nuclei. Here, attention is focused on dark matter candidates (neutralinos) predicted in the minimal supersymmetric standard model…

高能物理 - 唯象学 · 物理学 2014-11-17 John Ellis , Andrew Ferstl , Keith A. Olive

Directional detection can provide unambiguous observation of Dark Matter interactions even in presence of insidious backgrounds. The DM-TPC collaboration is developing a detector with the goal of measuring the direction and sense of nuclear…

One of the deepest unsolved puzzles of subatomic physics is why Nature prefers the left particles to the right ones. Mirror matter is an attempt to understand this mystery by assuming the existence of a "parallel''world where this…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Yu. Ignatiev , R. R. Volkas

Current dark matter detection strategies are based on the assumption that the dark matter is a gas of non-interacting particles with a reasonably large number density. This picture is dramatically altered if there are significant self…

高能物理 - 唯象学 · 物理学 2018-12-19 Dorota M Grabowska , Tom Melia , Surjeet Rajendran

We consider a simple model of a dark sector with a chiral $U(1)$ gauge symmetry. The anomaly-free condition requires at least five chiral fermions. Some of the fermions acquire masses through a vacuum expectation value of a Higgs field, and…

高能物理 - 唯象学 · 物理学 2026-03-03 Xiao He , Takaaki Nomura , Norimi Yokozaki

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…

宇宙学与河外天体物理 · 物理学 2015-09-04 Laura Baudis

We consider explicit models of dynamical supersymmetry breaking where dark matter is a 10 -- 100 TeV strongly-interacting composite state carrying no standard model quantum numbers. These constructions are simple variants of well-known…

高能物理 - 唯象学 · 物理学 2014-11-20 JiJi Fan , Jesse Thaler , Lian-Tao Wang

In the late Universe, and on cosmological scales, dark matter is conventionally assumed to be collisionless, as a consequence of the strong existing bounds on dark matter interactions at the Cosmic Microwave Background last-scattering…

宇宙学与河外天体物理 · 物理学 2026-03-11 Eugenia Dallari , Francesco Castagna , Emanuele Castorina , Maria Archidiacono , Ennio Salvioni

We present a weak lensing mass reconstruction of the interacting cluster 1E0657-558 in which we detect both the main cluster and a sub-cluster. The sub-cluster is identified as a smaller cluster which has just undergone initial in-fall and…

天体物理学 · 物理学 2008-11-26 Douglas Clowe , Anthony Gonzalez , Maxim Markevitch

We consider indirect detection signals of atomic dark matter, with a massive dark photon which mixes kinetically with hypercharge. In significant regions of parameter space, dark matter remains at least partially ionized today, and dark…

高能物理 - 唯象学 · 物理学 2015-04-29 Lauren Pearce , Kalliopi Petraki , Alexander Kusenko

Recoil imaging entails the detection of spatially resolved ionization tracks generated by particle interactions. This is a highly sought-after capability in many classes of detector, with broad applications across particle and astroparticle…

仪器与探测器 · 物理学 2022-07-19 C. A. J. O'Hare , D. Loomba , K. Altenmüller , H. Álvarez-Pol , F. D. Amaro , H. M. Araújo , D. Aristizabal Sierra , J. Asaadi , D. Attié , S. Aune , C. Awe , Y. Ayyad , E. Baracchini , P. Barbeau , J. B. R. Battat , N. F. Bell , B. Biasuzzi , L. J. Bignell , C. Boehm , I. Bolognino , F. M. Brunbauer , M. Caamaño , C. Cabo , D. Caratelli , J. M. Carmona , J. F. Castel , S. Cebrián , C. Cogollos , D. Collison , E. Costa , T. Dafni , F. Dastgiri , C. Deaconu , V. De Romeri , K. Desch , G. Dho , F. Di Giambattista , D. Díez-Ibáñez , G. D'Imperio , B. Dutta , C. Eldridge , S. R. Elliott , A. C. Ezeribe , A. Fava , T. Felkl , B. Fernández-Domínguez , E. Ferrer Ribas , K. J. Flöthner , M. Froehlich , J. Galán , J. Galindo , F. García , J. A. García Pascual , B. P. Gelli , M. Ghrear , Y. Giomataris , K. Gnanvo , E. Gramellini , G. Grilli Di Cortona , R. Hall-Wilton , J. Harton , S. Hedges , S. Higashino , G. Hill , P. C. Holanda , T. Ikeda , I. G. Irastorza , P. Jackson , D. Janssens , B. Jones , J. Kaminski , I. Katsioulas , K. Kelly , N. Kemmerich , E. Kemp , H. B. Korandla , H. Kraus , A. Lackner , G. J. Lane , P. M. Lewis , M. Lisowska , G. Luzón , W. A. Lynch , G. Maccarrone , K. J. Mack , P. A. Majewski , R. D. P. Mano , C. Margalejo , D. Markoff , T. Marley , D. J. G. Marques , R. Massarczyk , G. Mazzitelli , C. McCabe , L. J. McKie , A. G. McLean , P. C. McNamara , Y. Mei , A. Messina , A. F. Mills , H. Mirallas , K. Miuchi , C. M. B. Monteiro , M. R. Mosbech , H. Muller , H. Natal da Luz , K. D. Nakamura , A. Natochii , T. Neep , J. L. Newstead , K. Nikolopoulos , L. Obis , E. Oliveri , G. Orlandini , A. Ortiz de Solórzano , J. von Oy , T. Papaevangelou , O. Pérez , Y. F. Perez-Gonzalez , D. Pfeiffer , N. S. Phan , S. Piacentini , E. Picatoste Olloqui , D. Pinci , S. Popescu , A. Prajapati , F. S. Queiroz , J. L. Raaf , F. Resnati , L. Ropelewski , R. C. Roque , E. Ruiz-Choliz , A. Rusu , J. Ruz , J. Samarati , E. M. Santos , J. M. F. dos Santos , F. Sauli , L. Scharenberg , T. Schiffer , S. Schmidt , K. Scholberg , M. Schott , J. Schueler , L. Segui , H. Sekiya , D. Sengupta , Z. Slavkovska , D. Snowden-Ifft , P. Soffitta , M. van Stenis , N. J. C. Spooner , L. Strigari , A. E. Stuchbery , X. Sun , S. Torelli , E. G. Tilly , A. W. Thomas , T. N. Thorpe , P. Urquijo , A. Utrobičić , S. E. Vahsen , R. Veenhof , J. K. Vogel , A. G. Williams , M. H. Wood , J. Zettlemoyer

We explore the prospects for direct detection of dark energy by current and upcoming terrestrial dark matter direct detection experiments. If dark energy is driven by a new light degree of freedom coupled to matter and photons then dark…

高能物理 - 唯象学 · 物理学 2021-09-22 Sunny Vagnozzi , Luca Visinelli , Philippe Brax , Anne-Christine Davis , Jeremy Sakstein

Dark Matter can form bound states upon the emission of quanta of energy equal to the binding energy. The rate of this process is large for strongly-interacting Dark Matter, and further enhanced by long distance effects. The resulting…

高能物理 - 唯象学 · 物理学 2020-07-15 Rakhi Mahbubani , Michele Redi , Andrea Tesi

Dark matter self-interactions can affect the small scale structure of the Universe, reducing the central densities of dwarfs and low surface brightness galaxies in accord with observations. From a particle physics point of view, this points…

高能物理 - 唯象学 · 物理学 2015-06-17 Manoj Kaplinghat , Sean Tulin , Hai-Bo Yu

Direct dark matter detection experiments will soon be sensitive to neutrinos from astrophysical sources, including the Sun, the atmosphere, and supernova. This sets an important benchmark for these experiments, and opens up a new window in…

高能物理 - 唯象学 · 物理学 2020-01-08 Bhaskar Dutta , Louis E. Strigari

We explore the detection prospects for a minimal secluded dark matter model, where a fermionic dark matter particle interacts with the Standard Model (SM) via a kinetically mixed dark photon. We focus on scenarios where the dark photon…

高能物理 - 唯象学 · 物理学 2026-01-29 Ahmed Alenezi , Cari Cesarotti , Stefania Gori , Jessie Shelton

Given the lack of empirical evidence of weakly interacting dark matter, it is reasonable to look to other candidates such as a confining dark sector with a similar number of particles as the standard model. Twin Higgs mirror matter is one…

A ~5 GeV `dark baryon' with a cosmic asymmetry similar to that of baryons is a natural candidate for the dark matter. We study the possibility of generating such a state through dynamical electroweak symmetry breaking, and show that it can…

高能物理 - 唯象学 · 物理学 2011-09-28 Mads T. Frandsen , Subir Sarkar , Kai Schmidt-Hoberg

Merging galaxy clusters such as the Bullet Cluster provide a powerful testing ground for indirect detection of dark matter. The spatial distribution of the dark matter is both directly measurable through gravitational lensing and…

高能物理 - 唯象学 · 物理学 2015-05-21 Peter W. Graham , Surjeet Rajendran , Ken Van Tilburg , Timothy D. Wiser

Direct detection experiments aim at the detection of dark matter in the form of weakly interacting massive particles (WIMPs) by searching for signals from elastic dark matter nucleus scattering. Additionally, inelastic scattering in which…

高能物理 - 唯象学 · 物理学 2020-01-08 G. Arcadi , C. Döring , C. Hasterok , S. Vogl