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We search for indirect signals of $\mathscr{O}$(keV) dark matter annihilating or decaying into $\mathscr{O}$(eV) dark photons. These dark photons will be highly boosted and have decay lengths larger than the Milky Way, and can be absorbed…

High Energy Physics - Phenomenology · Physics 2024-05-24 Michael L. Graesser , R. Andrew Gustafson , Kate Hildebrandt , Varun Mathur , Ian M. Shoemaker

Dark matter and neutrinos provide the two most compelling pieces of evidence for new physics beyond the Standard Model of Particle Physics but they are often treated as two different sectors. The aim of this paper is to determine whether…

High Energy Physics - Phenomenology · Physics 2018-05-09 Andres Olivares-Del Campo , Celine Boehm , Sergio Palomares-Ruiz , Silvia Pascoli

Dark matter candidates with electromagnetic dipole moments can arise as dark baryons in gauge-mediated or technicolor models. These dark matter candidates interact with nuclei in direct detection experiments mainly through magnetic and/or…

High Energy Physics - Phenomenology · Physics 2010-08-04 Tom Banks , Jean-François Fortin , Scott Thomas

We demonstrate that nuclear magnetic resonance based searches for dark matter (DM) have intrinsic and powerful sensitivity to dark photons and the axion-photon coupling. The reason is conceptually straightforward. An instrument such as…

High Energy Physics - Phenomenology · Physics 2025-05-23 Carl Beadle , Sebastian A. R. Ellis , Jacob M. Leedom , Nicholas L. Rodd

We propose that dark matter is dominantly comprised of atomic bound states. We build a simple model and map the parameter space that results in the early universe formation of hydrogen-like dark atoms. We find that atomic dark matter has…

High Energy Physics - Phenomenology · Physics 2015-05-14 David E. Kaplan , Gordan Z. Krnjaic , Keith R. Rehermann , Christopher M. Wells

Dark matter interactions with electrons or protons during the early Universe leave imprints on the cosmic microwave background and the matter power spectrum, and can be probed through cosmological and astrophysical observations. These…

Cosmology and Nongalactic Astrophysics · Physics 2022-04-06 Manuel A. Buen-Abad , Rouven Essig , David McKeen , Yi-Ming Zhong

The complementarity of direct, indirect and collider searches for dark matter has improved our understanding concerning the properties of the dark matter particle. I will review the basic concepts that these methods rely upon and highlight…

High Energy Physics - Phenomenology · Physics 2016-05-31 Farinaldo S. Queiroz

Indirect searches for dark matter are based on detecting an anomalous flux of photons, neutrinos or cosmic-rays produced in annihilations or decays of dark matter candidates gravitationally accumulated in heavy cosmological objects, like…

High Energy Astrophysical Phenomena · Physics 2020-10-09 Carlos Pérez de los Heros

For a class of macroscopic dark matter with a large interaction strength with Standard Model particles, a nucleus could be captured by the dense, heavy dark matter as it traverses ordinary material. The radiated photon carries most of the…

High Energy Physics - Phenomenology · Physics 2021-12-23 Yang Bai , Joshua Berger

In a class of theories, dark matter is explained by postulating the existence of a `dark sector', which interacts gravitationally with ordinary matter. If this dark sector contains a U(1) symmetry, and a corresponding `dark' photon…

High Energy Physics - Phenomenology · Physics 2026-04-03 Mikael Berggren

We study the interaction between photons, dark photons, and axions at future lepton colliders, focusing on single-photon events with missing energy as the experimental signature. We find that future facilities such as the ILC, CEPC, and…

High Energy Physics - Phenomenology · Physics 2025-09-11 Chuan-Ren Chen , Yuan-Feng Hsieh , Van Que Tran

Dark photons are hypothetical massive vector particles that could mix with ordinary photons. The simplest theoretical model is fully characterised by only two parameters: the mass of the dark photon m$_{\gamma^{\mathrm{D}}}$ and its mixing…

High Energy Physics - Experiment · Physics 2023-01-11 SHiP Collaboration , C. Ahdida , A. Akmete , R. Albanese , A. Alexandrov , A. Anokhina , S. Aoki , G. Arduini , E. Atkin , N. Azorskiy , J. J. Back , A. Bagulya , F. Baaltasar Dos Santos , A. Baranov , F. Bardou , G. J. Barker , M. Battistin , J. Bauche , A. Bay , V. Bayliss , G. Bencivenni , A. Y. Berdnikov , Y. A. Berdnikov , M. Bertani , C. Betancourt , I. Bezshyiko , O. Bezshyyko , D. Bick , S. Bieschke , A. Blanco , J. Boehm , M. Bogomilov , I. Boiarska , K. Bondarenko , W. M. Bonivento , J. Borburgh , A. Boyarsky , R. Brenner , D. Breton , V. Büscher , A. Buonaura , S. Buontempo , S. Cadeddu , A. Calcaterra , M. Calviani , M. Campanelli , M. Casolino , N. Charitonidis , P. Chau , J. Chauveau , A. Chepurnov , M. Chernyavskiy , K. -Y. Choi , A. Chumakov , P. Ciambrone , V. Cicero , L. Congedo , K. Cornelis , M. Cristinziani , A. Crupano , G. M. Dallavalle , A. Datwyler , N. D'Ambrosio , G. D'Appollonio , R. de Asmundis , J. De Carvalho Saraiva , G. De Lellis , M. de Magistris , A. De Roeck , M. De Serio , D. De Simone , L. Dedenko , P. Dergachev , A. Di Crescenzo , L. Di Giulio , N. Di Marco , C. Dib , H. Dijkstra , V. Dmitrenko , L. A. Dougherty , A. Dolmatov , D. Domenici , S. Donskov , V. Drohan , A. Dubreuil , O. Durhan , M. Ehlert , E. Elikkaya , T. Enik , A. Etenko , F. Fabbri , O. Fedin , F. Fedotovs , G. Felici , M. Ferrillo , M. Ferro-Luzzi , K. Filippov , R. A. Fini , P. Fonte , C. Franco , M. Fraser , R. Fresa , R. Froeschl , T. Fukuda , G. Galati , J. Gall , L. Gatignon , G. Gavrilov , V. Gentile , B. Goddard , L. Golinka-Bezshyyko , A. Golovatiuk , V. Golovtsov , D. Golubkov , A. Golutvin , P. Gorbounov , D. Gorbunov , S. Gorbunov , V. Gorkavenko , M. Gorshenkov , V. Grachev , A. L. Grandchamp , E. Graverini , J. -L. Grenard , D. Grenier , V. Grichine , N. Gruzinskii , A. M. Guler , Yu. Guz , G. J. Haefeli , C. Hagner , H. Hakobyan , I. W. Harris , E. van Herwijnen , C. Hessler , A. Hollnagel , B. Hosseini , M. Hushchyn , G. Iaselli , A. Iuliano , R. Jacobsson , D. Joković , M. Jonker , I. Kadenko , V. Kain , B. Kaiser , C. Kamiscioglu , D. Karpenkov , K. Kershaw , M. Khabibullin , E. Khalikov , G. Khaustov , G. Khoriauli , A. Khotyantsev , Y. G. Kim , V. Kim , N. Kitagawa , J. -W. Ko , K. Kodama , A. Kolesnikov , D. I. Kolev , V. Kolosov , M. Komatsu , A. Kono , N. Konovalova , S. Kormannshaus , I. Korol , I. Korol'ko , A. Korzenev , V. Kostyukhin , E. Koukovini Platia , S. Kovalenko , I. Krasilnikova , Y. Kudenko , E. Kurbatov , P. Kurbatov , V. Kurochka , E. Kuznetsova , H. M. Lacker , M. Lamont , G. Lanfranchi , O. Lantwin , A. Lauria , K. S. Lee , K. Y. Lee , J. -M. Lévy , V. P. Loschiavo , L. Lopes , E. Lopez Sola , V. Lyubovitskij , J. Maalmi , A. -M. Magnan , V. Maleev , A. Malinin , Y. Manabe , A. K. Managadze , M. Manfredi , S. Marsh , A. M. Marshall , A. Mefodev , P. Mermod , A. Miano , S. Mikado , Yu. Mikhaylov , D. A. Milstead , O. Mineev , A. Montanari , M. C. Montesi , K. Morishima , S. Movchan , Y. Muttoni , N. Naganawa , M. Nakamura , T. Nakano , S. Nasybulin , P. Ninin , A. Nishio , A. Novikov , B. Obinyakov , S. Ogawa , N. Okateva , B. Opitz , J. Osborne , M. Ovchynnikov , N. Owtscharenko , P. H. Owen , P. Pacholek , A. Paoloni , B. D. Park , A. Pastore , M. Patel , D. Pereyma , A. Perillo-Marcone , G. L. Petkov , K. Petridis , A. Petrov , D. Podgrudkov , V. Poliakov , N. Polukhina , J. Prieto Prieto , M. Prokudin , A. Prota , A. Quercia , A. Rademakers , A. Rakai , F. Ratnikov , T. Rawlings , F. Redi , S. Ricciardi , M. Rinaldesi , Volodymyr Rodin , Viktor Rodin , P. Robbe , A. B. Rodrigues Cavalcante , T. Roganova , H. Rokujo , G. Rosa , T. Rovelli , O. Ruchayskiy , T. Ruf , V. Samoylenko , V. Samsonov , F. Sanchez Galan , P. Santos Diaz , A. Sanz Ull , A. Saputi , O. Sato , E. S. Savchenko , J. S. Schliwinski , W. Schmidt-Parzefall , N. Serra , S. Sgobba , O. Shadura , A. Shakin , M. Shaposhnikov , P. Shatalov , T. Shchedrina , L. Shchutska , V. Shevchenko , H. Shibuya , S. Shirobokov , A. Shustov , S. B. Silverstein , S. Simone , R. Simoniello , M. Skorokhvatov , S. Smirnov , J. Y. Sohn , A. Sokolenko , E. Solodko , N. Starkov , L. Stoel , M. E. Stramaglia , D. Sukhonos , Y. Suzuki , S. Takahashi , J. L. Tastet , P. Teterin , S. Than Naing , I. Timiryasov , V. Tioukov , D. Tommasini , M. Torii , N. Tosi , D. Treille , R. Tsenov , S. Ulin , E. Ursov , A. Ustyuzhanin , Z. Uteshev , L. Uvarov , G. Vankova-Kirilova , F. Vannucci , V. Venturi , S. Vilchinski , Heinz Vincke , Helmut Vincke , C. Visone , K. Vlasik , A. Volkov , R. Voronkov , S. van Waasen , R. Wanke , P. Wertelaers , O. Williams , J. -K. Woo , M. Wurm , S. Xella , D. Yilmaz , A. U. Yilmazer , C. S. Yoon , Yu. Zaytsev , A. Zelenov , J. Zimmerman

We show that dark matter direct detection experiments are sensitive to the existence of particles with a small effective charge (for instance, via couplings to a kinetically mixed, low-mass dark photon). Our forecasts do not depend on these…

High Energy Physics - Phenomenology · Physics 2024-08-01 Ella Iles , Saniya Heeba , Katelin Schutz

The search for dark matter has been performed mainly for weakly interacting massive particles and massive compact halo objects, and the intermediate mass region has not been investigated experimentally. A method to search dark matter with…

Instrumentation and Detectors · Physics 2019-01-23 Akio Kawasaki

Particle dark matter could have a mass anywhere from that of ultralight candidates, $m_\chi\sim 10^{-21}\,$eV, to scales well above the GeV. Conventional laboratory searches are sensitive to a range of masses close to the weak scale, while…

High Energy Physics - Phenomenology · Physics 2019-09-13 Rodrigo Alonso , Diego Blas , Peter Wolf

Massive photon-like particles are predicted in many extensions of the Standard Model with a hidden sector where dark matter is secluded. They are vector bosons mediating the interaction between dark matter particles and can be produced in…

High Energy Physics - Experiment · Physics 2017-12-07 Viviana Scherini

We revisit the exclusion constraints on the parameters of a narrow dark photon set by direct experimental searches. We investigate how a dark photon with a larger decay width impacts these limits, in particular, in the case where the dark…

High Energy Physics - Phenomenology · Physics 2025-08-19 J. R. Felix , A. W. Thomas , X. G. Wang

We propose a novel approach for discovering a light dark photon in the forward experiments at the LHC, including the SND@LHC and the FASER experiments. Assuming the dark photon is lighter than twice the electron mass and feebly interacts…

High Energy Physics - Phenomenology · Physics 2024-10-16 Yeong Gyun Kim , Kang Young Lee , Soo-hyeon Nam

We present a mechanism for generating ultralight dark photon dark matter in the early Universe via a dilatonlike scalar field coupled to the dark photon's kinetic term. Energy is initially stored in the condensate of the dilaton, which…

High Energy Physics - Phenomenology · Physics 2025-08-20 Peter Adshead , Kaloian D. Lozanov , Zachary J. Weiner

In this review, we discuss the role of the various experimental programs taking part in the broader effort to identify the particle nature of dark matter. In particular, we focus on electroweak scale dark matter particles and discuss a wide…

High Energy Physics - Phenomenology · Physics 2008-11-26 Dan Hooper , Edward A. Baltz
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