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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

Ultrastrong light-matter interaction in an optomechanical system can result in nonlinear optical effects such as photon blockade. The system-bath couplings in such systems play an essential role in observing these effects. Here we study the…

Quantum Physics · Physics 2015-01-09 D. Hu , S. -Y. Huang , J. -Q. Liao , L. Tian , H. -S. Goan

Astrophysical tests of the stability of fundamental couplings, such as the fine-structure constant $\alpha$, are becoming an increasingly powerful probe of new physics. Here we discuss how these measurements, combined with local atomic…

Cosmology and Nongalactic Astrophysics · Physics 2015-09-09 C. J. A. P. Martins , A. M. M. Pinho , R. F. C. Alves , M. Pino , C. I. S. A. Rocha , M. von Wietersheim

Dark photon dark matter that has a kinetic mixing with the Standard Model photon can resonantly convert in environments where its mass $m_{A'}$ coincides with the plasma frequency. We show that such conversion in neutron stars or accreting…

High Energy Physics - Phenomenology · Physics 2023-09-14 Edward Hardy , Ningqiang Song

Mixed damping is a physical effect that occurs when a heavy species is coupled to a relativistic fluid which is itself free streaming. As a cross-case between collisional damping and free-streaming, it is crucial in the context of…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-21 Julia Stadler , Céline Bœhm , Olga Mena

A system of light axions comprising a classical axion field, one candidate for dark matter, has an instability that would rapidly mix in photon pairs in a coherent fashion if the system were initially seeded by some tiny amount of such…

High Energy Physics - Phenomenology · Physics 2019-01-30 R. F. Sawyer

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

We consider a model of dark quantum electrodynamics which is coupled with a visible photon through a kinetic mixing term. After checking of consistency properties, we compute the $g_w-2$, where $g_w$ is the gyromagnetic factor for a dark…

High Energy Physics - Phenomenology · Physics 2017-11-22 Ashok K. Das , Jorge Gamboa , Fernando Méndez , Natalia Tapia

Quantum Chromodynamics predicts that the strong coupling strength $\alpha_s$ decreases with increasing energy or momentum transfer, and vanishes at asymptotically high energies. The history and the status of experimental tests of asymptotic…

High Energy Physics - Phenomenology · Physics 2023-10-03 Siegfried Bethke

Ultralight dark photons are compelling dark matter candidates, but their allowed kinetic mixing with the Standard Model photon is severely constrained by requiring that the dark photons do not collapse into a cosmic string network in the…

High Energy Physics - Phenomenology · Physics 2025-08-20 David Cyncynates , Zachary J. Weiner

Photon-photon scattering in vacuum is extremely weak. However, strong effective interactions between single photons can be realized by employing strong light-matter coupling. These interactions are a fundamental building block for quantum…

Quantum Physics · Physics 2017-07-07 Dibyendu Roy , C. M. Wilson , Ofer Firstenberg

Information about quantum phase transitions in conventional condensed matter systems, must be sought by probing the matter system itself. By contrast, we show that mixed matter-light systems offer a distinct advantage in that the photon…

Quantum Physics · Physics 2009-11-13 Timothy C. Jarrett , Alexandra Olaya-Castro , Neil F. Johnson

Motivated by the growing interest in the existence of new massive gauge bosons, we suggest that massive dark photons A0 can be a consequence of a broken new abelian symmetry U(1)'X. Such a dark symmetry U(1)'D is afterwards supposed to be…

High Energy Physics - Phenomenology · Physics 2022-11-28 Salah Eddine Ennadifi

Dark photons in the MeV to GeV range with kinetic mixing of the order of $\lesssim 10^{-4}-10^{-3}$ can be produced in significant numbers at low energy colliders such as Belle II. Their decay length can be macroscopic raising the hope for…

High Energy Physics - Phenomenology · Physics 2026-02-27 Joerg Jaeckel , Anh Vu Phan

Dark sector may exist and interact with Standard Model (SM) through the $U(1)$ kinetic mixing. Through this portal-type interaction, dark photon from dark sector couples to SM fermions, and may explain the discrepancy between experimental…

High Energy Physics - Phenomenology · Physics 2026-02-04 Chuan-Ren Chen , Yuan-Feng Hsieh , Chrisna Setyo Nugroho

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

A system of light axions comprising a classical axion field, one candidate for dark matter, has an instability that can rapidly mix in photon pairs in a coherent fashion if initiated by a quantum break (which eliminates the need for seeds.)…

High Energy Physics - Phenomenology · Physics 2019-08-14 R. F. Sawyer

We explore some of the consequences of Dark Matter-photon interactions on structure formation, focusing on the evolution of cosmological perturbations and performing both an analytical and a numerical study. We compute the cosmic microwave…

Astrophysics · Physics 2009-11-07 Celine Boehm , Alain Riazuelo , Steen H. Hansen , Richard Schaeffer

In addition to gravity, there might be another very weak interaction between the ordinary and dark matter transmitted by U'(1) gauge bosons A' (dark photons) mixing with our photons. If such A's exist, they could be searched for in a…

High Energy Physics - Phenomenology · Physics 2014-04-09 S. N. Gninenko

We argue that Dark Matter can be described by an interacting field theory with a mass parameter of the order of the proton mass and an interaction coupling of the order of the QED coupling.

General Relativity and Quantum Cosmology · Physics 2008-11-26 Elcio Abdalla , Bin Wang
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