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Dark matter particles need not be completely stable, and in fact they may be decaying now. We consider this possibility in the frameworks of universal extra dimensions and supersymmetry with very late decays of WIMPs to Kaluza-Klein…

Astrophysics · Physics 2009-06-23 Jose A. R. Cembranos , Jonathan L. Feng , Louis E. Strigari

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 paper, we investigate constraints of the transmon qubit, an improved version of the charge qubit, on bosonic light dark matters. Phonon excitations induced by the scattering or absorption of dark matter on a superconductor may…

High Energy Physics - Phenomenology · Physics 2025-11-21 Wei Chao , Yu Gao , Ming-jie Jin , Xiao-sheng Liu , Xi-lei Sun

Uncovering the nature of dark matter is one of the most important goals of particle physics. Light bosonic particles, such as the dark photon, are well-motivated candidates: they are generally long-lived, weakly-interacting, and naturally…

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

A search for hidden-photon (HP) dark matter using a multi-cathode counter is reported. The technique based on counting of single electrons emitted from outer cathode of the proportional counter by hidden-photons was used. The apparatus and…

High Energy Physics - Experiment · Physics 2020-01-08 A. Kopylov , I. Orekhov , V. Petukhov

The dark photon is a well-motivated ultralight dark-matter candidate that may couple to the Standard Model through kinetic mixing. We search for dark-photon dark matter in the mass range $m_{A'}c^2 =…

High Energy Physics - Phenomenology · Physics 2026-02-27 Joel Barir , Itay M. Bloch , Yair Goldszeft , Gal Goldstein , Constantine Feinberg , Or Katz , Tomer Volansky

It is known that magnetic fields exist near black holes and photons can go around black holes due to strong gravity. Utilizing these facts, we can probe hypothetical pseudoscalar particles, so-called axions. In fact, photons can be…

High Energy Physics - Phenomenology · Physics 2023-06-12 Kimihiro Nomura , Kaishu Saito , Jiro Soda

Dark photon is a massive vector field which interacts only with the physical photon through the kinetic mixing. This coupling is assumed to be weak so that the dark photon becomes almost unobservable in processes with elementary particles,…

Cosmology and Nongalactic Astrophysics · Physics 2019-10-02 V. V. Flambaum , I. B. Samsonov

We consider current observational constraints on the electromagnetic charge of dark matter. The velocity dependence of the scattering cross-section through the photon gives rise to qualitatively different constraints than standard dark…

High Energy Physics - Phenomenology · Physics 2011-03-22 Samuel D. McDermott , Hai-Bo Yu , Kathryn M. Zurek

Dwarf spheroidal galaxies are dark matter dominated systems, and as such, ideal for indirect dark matter searches. If dark matter decays into high-energy photons in the dwarf galaxies, they will be a good target for current and future…

The dark photon is a new gauge boson whose existence has been conjectured. It is dark because it arises from a symmetry of a hypothetical dark sector comprising particles completely neutral under the Standard Model interactions. Dark though…

High Energy Physics - Phenomenology · Physics 2021-03-02 Marco Fabbrichesi , Emidio Gabrielli , Gaia Lanfranchi

We are building an experiment to search for dark matter in the form of dark photons in the nano- to milli-eV mass range. This experiment is the electromagnetic dual of magnetic detector dark radio experiments. It is also a frequency-time…

Dark matter experiments primarily search for the scattering of WIMPs on target nuclei of well shielded underground detectors. The results from liquid scintillator experiments furthermore provide precise probes of very light and very weakly…

High Energy Physics - Phenomenology · Physics 2015-10-19 Haipeng An , Kaixuan Ni , Maxim Pospelov , Josef Pradler , Adam Ritz

In the past decade, gamma-ray observations and radio observations put strong constraints on the parameters of dark matter annihilation. In this article, we suggest another robust way to constrain the parameters of dark matter annihilation.…

High Energy Astrophysical Phenomena · Physics 2017-08-09 Man Ho Chan

We investigate cosmological and astrophysical constraints on dark photons with masses $\sim 10^{-1}$-$10^3$ MeV. These dark photons can be copiously produced either in the early universe or during core-collapse supernovae, potentially…

High Energy Physics - Phenomenology · Physics 2025-11-21 Andrea Caputo , Jaeyoung Park , Seokhoon Yun

We propose a simplified model of dark matter with a scalar mediator to accommodate the di-photon excess recently observed by the ATLAS and CMS collaborations. Decays of the resonance into dark matter can easily account for a relatively…

High Energy Physics - Phenomenology · Physics 2016-04-20 Mihailo Backovic , Alberto Mariotti , Diego Redigolo

Axions solve the Strong CP Problem and are a cold dark matter candidate. The combined constraints from accelerator searches, stellar evolution limits and cosmology suggest that the axion mass is in the range $3 \cdot 10^{-3} > m_a >…

High Energy Physics - Phenomenology · Physics 2007-05-23 Pierre Sikivie

A systematic and unified analysis of the capability of lifetime frontier experiments to probe the parameter space of hypothetical long-lived particles is crucial for defining the targets of future searches. However, such a comprehensive…

High Energy Physics - Phenomenology · Physics 2025-01-28 Yehor Kyselov , Maksym Ovchynnikov

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