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Relativistic axions are good candidates for the dark radiation for which there are mounting observational hints. The primordial decays of heavy fields produce axions which are ultra-energetic compared to thermalised matter and inelastic…

High Energy Physics - Phenomenology · Physics 2015-06-15 Joseph P. Conlon , M. C. David Marsh

Dark sector may couple to the Standard Model via one or more mediator particles. We discuss two types of mediators: the dark photon $A^{\prime}$ and the dark scalar mediator $\phi$. The total cross-sections and various differential…

High Energy Physics - Phenomenology · Physics 2020-02-19 Jun Jiang , Chun-Yuan Li , Shi-Yuan Li , Shankar Dayal Pathak , Zong-Guo Si , Xing-Hua Yang

Primordial black holes (PBHs) are significant sources of axions and axion-like particles (ALPs), provided their Hawking temperature exceeds the particles' masses. Given the predominant decay of axions into photons, the enhanced photon…

High Energy Physics - Phenomenology · Physics 2026-03-04 Yongsoo Jho , Tae-Geun Kim , Jong-Chul Park , Seong Chan Park , Yeji Park

The PAMELA and Fermi measurements of the cosmic-ray electron and positron spectra have generated much interest over the past two years, because they are consistent with a significant component of the electron and positron fluxes between 20…

High Energy Physics - Phenomenology · Physics 2011-08-05 Spencer Chang , Lisa Goodenough

Assuming the dark matter is made entirely from neutralinos, we re-visit the role of their annihilation on the temperature of diffuse gas in the high redshift universe. We consider neutralinos of particle mass 36 GeV and 100 GeV,…

Astrophysics · Physics 2009-11-13 Zac Myers , Adi Nusser

Photon absorption in a semiconductor produces bright excitons that recombine very fast into photons. We here show that in a quantum dot set close to a p-doped reservoir, this absorption can produce a dark duo, i.e., an electron-hole pair…

Mesoscale and Nanoscale Physics · Physics 2020-04-22 Shiue-Yuan Shiau , Benoit Eble , Valia Voliotis , Monique Combescot

Even 50 years after the discovery of a positron annihilation line from the inner Galaxy, no class of astrophysical sources has emerged as a definitive explanation for both the emission morphology and flux. Positrons produced by dark matter…

High Energy Astrophysical Phenomena · Physics 2025-06-03 Souradeep Das , Mark R. Krumholz , Roland M. Crocker , Thomas Siegert , Laura Eisenberger

High energy neutrinos are produced by the annihilation of dark matter particles in our galaxy. These are presently searched for with large area, deep underground neutrino telescopes. Cold dark matter particles, trapped inside the sun, are…

High Energy Physics - Phenomenology · Physics 2009-09-25 F. Halzen , J. E. Jacobsen

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

The production and subsequent re-scattering of secondary pions produced in proton beam dumps provides additional opportunities for the production of light new particles like dark photons. This new mechanism has been overlooked in the past…

High Energy Physics - Phenomenology · Physics 2023-06-01 David Curtin , Yonatan Kahn , Rachel Nguyen

The existence of a new, photon-like, massive particle, the gamma' or dark photon, is postulated in several extensions of the Standard Model. These models are often advocated to explain some recent puzzling astrophysical observations, as…

High Energy Physics - Experiment · Physics 2014-02-03 Fabio Bossi

We consider a highly unconventional approach to generating muon and antimuon bunches for a neutrino factory or muon collider: electron-positron annihilation just above muon-antimuon threshold. This approach can produce low-emittance bunches…

Accelerator Physics · Physics 2007-07-12 D. M. Kaplan , T. Hart , P. Allport

We present new constraints on sub-GeV dark matter and dark photons from the electron beam-dump experiment E137 conducted at SLAC in 1980-1982. Dark matter interacting with electrons (e.g., via a dark photon) could have been produced in the…

High Energy Physics - Phenomenology · Physics 2015-10-09 Brian Batell , Rouven Essig , Ze'ev Surujon

In the phenomenology study of dark photon, its mass origin is usually not under concern. However, in theory construction its mass is often generated via a dark Higgs mechanism, which leads to the presence of a light (non-decoupled) dark…

High Energy Physics - Phenomenology · Physics 2025-10-15 Song Li , Jin Min Yang , Mengchao Zhang , Yang Zhang , Rui Zhu

The PADME Experiment at Laboratori Nationali di Frascati is designed to search for the Dark Photon, a hypothetical gauge boson responsible for the interaction between the visible and the hidden sector. PADME explores the process of…

High Energy Physics - Experiment · Physics 2026-03-31 Kalina Dimitrova

We show that dark solitons in 1D Bose liquids may be created by absorption of a single quanta of an external ac field, in a close analogy with the Einstein's photoelectric effect. Similarly to the von Lenard's experiment with photoexcited…

Other Condensed Matter · Physics 2010-04-09 M. Khodas , A. Kamenev , L. I. Glazman

We study the production of dark photons with masses in range 0.4-1.5\,GeV in elastic proton bremsstrahlung. In contrast to the known approaches to calculating the bremsstrahlung cross section, we consider the non-zero momentum transfer…

High Energy Physics - Phenomenology · Physics 2025-02-12 Ekaterina Kriukova

The dark photon $A^\prime$ and the dark Higgs boson $h^\prime$ are hypothetical particles predicted in many dark sector models. We search for the simultaneous production of $A^\prime$ and $h^\prime$ in the dark Higgsstrahlung process…

High Energy Physics - Experiment · Physics 2023-07-11 Belle II Collaboration , F. Abudinén , I. Adachi , L. Aggarwal , H. Aihara , N. Akopov , A. Aloisio , N. Anh Ky , D. M. Asner , H. Atmacan , T. Aushev , V. Aushev , V. Babu , S. Bahinipati , P. Bambade , Sw. Banerjee , S. Bansal , J. Baudot , A. Baur , A. Beaubien , J. Becker , P. K. Behera , J. V. Bennett , E. Bernieri , F. U. Bernlochner , M. Bertemes , E. Bertholet , M. Bessner , B. Bhuyan , F. Bianchi , T. Bilka , D. Biswas , A. Bobrov , D. Bodrov , A. Bolz , A. Bozek , M. Bračko , P. Branchini , T. E. Browder , A. Budano , S. Bussino , M. Campajola , G. Casarosa , C. Cecchi , V. Chekelian , C. Chen , Y. Q. Chen , B. G. Cheon , K. Chilikin , K. Chirapatpimol , H. -E. Cho , K. Cho , S. -J. Cho , S. -K. Choi , S. Choudhury , D. Cinabro , L. Corona , S. Cunliffe , F. Dattola , G. de Marino , G. De Nardo , M. De Nuccio , G. De Pietro , R. de Sangro , M. Destefanis , S. Dey , A. De Yta-Hernandez , R. Dhamija , A. Di Canto , F. Di Capua , J. Dingfelder , Z. Doležal , I. Domínguez Jiménez , T. V. Dong , M. Dorigo , K. Dort , D. Dossett , S. Dreyer , S. Dubey , G. Dujany , P. Ecker , M. Eliachevitch , D. Epifanov , P. Feichtinger , T. Ferber , D. Ferlewicz , T. Fillinger , C. Finck , G. Finocchiaro , K. Flood , A. Fodor , F. Forti , A. Frey , B. G. Fulsom , E. Ganiev , M. Garcia-Hernandez , V. Gaur , A. Gaz , A. Gellrich , R. Giordano , A. Giri , B. Gobbo , R. Godang , P. Goldenzweig , W. Gradl , S. Granderath , E. Graziani , D. Greenwald , T. Gu , K. Gudkova , J. Guilliams , C. Hadjivasiliou , K. Hara , T. Hara , K. Hayasaka , H. Hayashii , S. Hazra , C. Hearty , M. T. Hedges , I. Heredia de la Cruz , M. Hernández Villanueva , A. Hershenhorn , T. Higuchi , E. C. Hill , M. Hoek , M. Hohmann , C. -L. Hsu , T. Iijima , K. Inami , G. Inguglia , N. Ipsita , A. Ishikawa , S. Ito , R. Itoh , M. Iwasaki , P. Jackson , W. W. Jacobs , D. E. Jaffe , E. -J. Jang , Q. P. Ji , S. Jia , Y. Jin , H. Junkerkalefeld , H. Kakuno , A. B. Kaliyar , J. Kandra , K. H. Kang , R. Karl , G. Karyan , T. Kawasaki , C. Ketter , H. Kichimi , C. Kiesling , C. -H. Kim , D. Y. Kim , K. -H. Kim , Y. -K. Kim , K. Kinoshita , P. Kodyš , T. Koga , S. Kohani , K. Kojima , T. Konno , A. Korobov , S. Korpar , E. Kovalenko , R. Kowalewski , T. M. G. Kraetzschmar , P. Križan , P. Krokovny , T. Kuhr , R. Kumar , K. Kumara , T. Kunigo , Y. -J. Kwon , S. Lacaprara , Y. -T. Lai , T. Lam , J. S. Lange , M. Laurenza , R. Leboucher , S. C. Lee , L. K. Li , Y. B. Li , J. Libby , K. Lieret , Q. Y. Liu , D. Liventsev , S. Longo , A. Lozar , T. Lueck , C. Lyu , M. Maggiora , R. Maiti , S. Maity , R. Manfredi , E. Manoni , S. Marcello , C. Marinas , L. Martel , A. Martini , L. Massaccesi , M. Masuda , K. Matsuoka , J. A. McKenna , F. Meier , M. Merola , F. Metzner , M. Milesi , C. Miller , K. Miyabayashi , G. B. Mohanty , N. Molina-Gonzalez , S. Moneta , H. Moon , M. Mrvar , I. Nakamura , K. R. Nakamura , M. Nakao , H. Nakayama , A. Narimani Charan , M. Naruki , Z. Natkaniec , A. Natochii , L. Nayak , M. Nayak , N. K. Nisar , S. Nishida , K. Nishimura , S. Ogawa , H. Ono , P. Oskin , G. Pakhlova , A. Paladino , A. Panta , S. Pardi , K. Parham , H. Park , S. -H. Park , A. Passeri , S. Patra , S. Paul , T. K. Pedlar , M. Piccolo , L. E. Piilonen , G. Pinna Angioni , P. L. M. Podesta-Lerma , T. Podobnik , S. Pokharel , L. Polat , C. Praz , S. Prell , E. Prencipe , M. T. Prim , H. Purwar , N. Rad , P. Rados , S. Raiz , A. Ramirez Morales , M. Reif , S. Reiter , M. Remnev , I. Ripp-Baudot , G. Rizzo , S. H. Robertson , D. Rodríguez Pérez , J. M. Roney , A. Rostomyan , N. Rout , D. Sahoo , D. A. Sanders , S. Sandilya , L. Santelj , Y. Sato , B. Scavino , J. Schueler , C. Schwanda , Y. Seino , A. Selce , K. Senyo , J. Serrano , M. E. Sevior , C. Sfienti , T. Shillington , J. -G. Shiu , A. Sibidanov , F. Simon , J. B. Singh , J. Skorupa , A. Soffer , A. Sokolov , E. Solovieva , S. Spataro , B. Spruck , M. Starič , S. Stefkova , Z. S. Stottler , R. Stroili , M. Sumihama , K. Sumisawa , W. Sutcliffe , S. Y. Suzuki , H. Svidras , M. Tabata , M. Takizawa , U. Tamponi , S. Tanaka , K. Tanida , H. Tanigawa , F. Tenchini , R. Tiwary , D. Tonelli , E. Torassa , N. Toutounji , K. Trabelsi , M. Uchida , I. Ueda , Y. Uematsu , T. Uglov , K. Unger , Y. Unno , K. Uno , S. Uno , P. Urquijo , Y. Ushiroda , S. E. Vahsen , R. van Tonder , G. S. Varner , K. E. Varvell , A. Vinokurova , L. Vitale , V. Vobbilisetti , E. Waheed , H. M. Wakeling , E. Wang , M. -Z. Wang , A. Warburton , M. Watanabe , S. Watanuki , M. Welsch , C. Wessel , H. Windel , E. Won , X. P. Xu , B. D. Yabsley , S. Yamada , W. Yan , S. B. Yang , H. Ye , J. H. Yin , K. Yoshihara , C. Z. Yuan , Y. Yusa , L. Zani , Y. Zhang , V. Zhilich , Q. D. Zhou , X. Y. Zhou , V. I. Zhukova , R. Žlebčík

The Galactic positrons, as observed by their annihilation gamma-ray line at 0.511 MeV, are difficult to account for with astrophysical sources. It has been proposed that they are produced instead by dark matter annihilation or decay in the…

Astrophysics · Physics 2009-07-09 John F. Beacom , Nicole F. Bell , Gianfranco Bertone