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The observation of high energy cosmic neutrinos can shed light on the astrophysical sites and mechanisms involved in the acceleration of protons and nuclei to the high energies observed at Earth by cosmic ray detectors. More generally, high…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Juan Jose Hernandez-Rey

We propose a neutrino lepton collider where the neutrino beam is generated from TeV scale muon decays. Such a device would allow for a precise measurement of the W mass based on single W production: nu l to W. Although it is challenging to…

High Energy Physics - Phenomenology · Physics 2025-06-25 Tianyi Yang , Sitian Qian , Sen Deng , Jie Xiao , Leyun Gao , Andrew Michael Levin , Qiang Li , Meng Lu , Zhengyun You

The axion-like particles (ALPs) are very good candidates of the cosmological dark matter, which can exist in many extensions of the standard model (SM). The mass range of the ALPs as the dark matter can extend from a sub-eV scale to almost…

High Energy Physics - Phenomenology · Physics 2018-12-05 Guo-yuan Huang , Newton Nath

We propose to implement a two-stage detection strategy for exotic long-lived particles that could be produced at the CERN LHC, become trapped in detector material, and decay later. The proposed strategy relies on an array of metal rods,…

High Energy Physics - Phenomenology · Physics 2022-03-18 Jan Kieseler , Juliette Alimena , Jasmine Simms , Thea Aarrestad , Maurizio Pierini , Alexander Kish

We report on a search for charged massive long-lived particles (CMLLPs), based on 5.2 fb$^{-1}$ of data collected with the D0 detector at the Fermilab Tevatron $p\bar{p}$ collider. CMLLPs are predicted in many theories of physics beyond the…

High Energy Physics - Experiment · Physics 2019-08-14 J. Alimena

Dark matter capture and annihilation in the Sun can produce detectable high-energy neutrinos, providing a probe of the dark matter-proton scattering cross section. We consider the case when annihilation proceeds via long-lived dark…

High Energy Astrophysical Phenomena · Physics 2017-07-03 Rebecca K. Leane , Kenny C. Y. Ng , John F. Beacom

Dark matter particles gravitationally trapped inside the Sun may annihilate into Standard Model particles, producing a flux of neutrinos. The prospects of detecting these neutrinos in future multi-\kton{} neutrino detectors designed for…

High Energy Physics - Phenomenology · Physics 2015-03-19 Sanjib K. Agarwalla , Mattias Blennow , Enrique Fernandez Martinez , Olga Mena

The nature of dark matter remains unresolved in fundamental physics. Weakly Interacting Massive Particles (WIMPs), which could explain the nature of dark matter, can be captured by celestial bodies like the Sun or Earth, leading to enhanced…

High Energy Astrophysical Phenomena · Physics 2024-12-18 The IceCube Collaboration

Self-annihilating or decaying dark matter in the Galactic halo might produce high energy neutrinos detectable with neutrino telescopes. We have conducted a search for such a signal using 276 days of data from the IceCube 22-string…

High Energy Astrophysical Phenomena · Physics 2016-08-14 IceCube Collaboration , R. Abbasi , Y. Abdou , T. Abu-Zayyad , J. Adams , J. A. Aguilar , M. Ahlers , K. Andeen , J. Auffenberg , X. Bai , M. Baker , S. W. Barwick , R. Bay , J. L. Bazo Alba , K. Beattie , J. J. Beatty , S. Bechet , J. K. Becker , K. -H. Becker , M. L. Benabderrahmane , S. BenZvi , J. Berdermann , P. Berghaus , D. Berley , E. Bernardini , D. Bertrand , D. Z. Besson , D. Bindig , M. Bissok , E. Blaufuss , J. Blumenthal , D. J. Boersma , C. Bohm , D. Bose , S. Böser , O. Botner , J. Braun , A. M. Brown , S. Buitink , M. Carson , D. Chirkin , B. Christy , J. Clem , F. Clevermann , S. Cohen , C. Colnard , D. F. Cowen , M. V. D'Agostino , M. Danninger , J. Daughhetee , J. C. Davis , C. De Clercq , L. Demirörs , T. Denger , O. Depaepe , F. Descamps , P. Desiati , G. de Vries-Uiterweerd , T. DeYoung , J. C. Diaz-Vélez , M. Dierckxsens , J. Dreyer , J. P. Dumm , R. Ehrlich , J. Eisch , R. W. Ellsworth , O. Engdegård , S. Euler , P. A. Evenson , O. Fadiran , A. R. Fazely , A. Fedynitch , T. Feusels , K. Filimonov , C. Finley , T. Fischer-Wasels , M. M. Foerster , B. D. Fox , A. Franckowiak , R. Franke , T. K. Gaisser , J. Gallagher , M. Geisler , L. Gerhardt , L. Gladstone , T. Glüsenkamp , A. Goldschmidt , J. A. Goodman , D. Grant , T. Griesel , A. Groß , S. Grullon , M. Gurtner , C. Ha , A. Hallgren , F. Halzen , K. Han , K. Hanson , D. Heinen , K. Helbing , P. Herquet , S. Hickford , G. C. Hill , K. D. Hoffman , A. Homeier , K. Hoshina , D. Hubert , W. Huelsnitz , J. -P. Hülß , P. O. Hulth , K. Hultqvist , S. Hussain , A. Ishihara , J. Jacobsen , G. S. Japaridze , H. Johansson , J. M. Joseph , K. -H. Kampert , A. Kappes , T. Karg , A. Karle , J. L. Kelley , P. Kenny , J. Kiryluk , F. Kislat , S. R. Klein , J. -H. Köhne , G. Kohnen , H. Kolanoski , L. Köpke , S. Kopper , D. J. Koskinen , M. Kowalski , T. Kowarik , M. Krasberg , T. Krings , G. Kroll , K. Kuehn , T. Kuwabara , M. Labare , S. Lafebre , K. Laihem , H. Landsman , M. J. Larson , R. Lauer , J. Lünemann , J. Madsen , P. Majumdar , A. Marotta , R. Maruyama , K. Mase , H. S. Matis , K. Meagher , M. Merck , P. Mészáros , T. Meures , E. Middell , N. Milke , J. Miller , T. Montaruli , R. Morse , S. M. Movit , R. Nahnhauer , J. W. Nam , U. Naumann , P. Nießen , D. R. Nygren , S. Odrowski , A. Olivas , M. Olivo , A. O'Murchadha , M. Ono , S. Panknin , L. Paul , C. Pérez de los Heros , J. Petrovic , A. Piegsa , D. Pieloth , R. Porrata , J. Posselt , P. B. Price , M. Prikockis , G. T. Przybylski , K. Rawlins , P. Redl , E. Resconi , W. Rhode , M. Ribordy , A. Rizzo , J. P. Rodrigues , P. Roth , F. Rothmaier , C. Rott , T. Ruhe , D. Rutledge , B. Ruzybayev , D. Ryckbosch , H. -G. Sander , M. Santander , S. Sarkar , K. Schatto , T. Schmidt , A. Schoenwald , A. Schukraft , A. Schultes , O. Schulz , M. Schunck , D. Seckel , B. Semburg , S. H. Seo , Y. Sestayo , S. Seunarine , A. Silvestri , A. Slipak , G. M. Spiczak , C. Spiering , M. Stamatikos , T. Stanev , G. Stephens , T. Stezelberger , R. G. Stokstad , S. Stoyanov , E. A. Strahler , T. Straszheim , M. Stür , G. W. Sullivan , Q. Swillens , H. Taavola , I. Taboada , A. Tamburro , O. Tarasova , A. Tepe , S. Ter-Antonyan , S. Tilav , P. A. Toale , S. Toscano , D. Tosi , D. Turčan , N. van Eijndhoven , J. Vandenbroucke , A. Van Overloop , J. van Santen , M. Vehring , M. Voge , B. Voigt , C. Walck , T. Waldenmaier , M. Wallraff , M. Walter , Ch. Weaver , C. Wendt , S. Westerhoff , N. Whitehorn , K. Wiebe , C. H. Wiebusch , D. R. Williams , R. Wischnewski , H. Wissing , M. Wolf , K. Woschnagg , C. Xu , X. W. Xu , G. Yodh , S. Yoshida , P. Zarzhitsky

We discuss the possible existence of an observational window, in the TeV-PeV energy range, for the detection of prompt neutrinos from the decay of charmed particles produced in cosmic ray interactions with the atmosphere. We calculate the…

High Energy Physics - Phenomenology · Physics 2009-11-07 C. G. S. Costa , F. Halzen , C. Salles

Dark matter (DM) annihilations in the Galaxy may produce high energy neutrinos, which can be detected by the neutrino telescopes, for example IceCube, ANTARES and Super-Kamiokande. The neutrinos can also arise from hadronic interaction…

Astrophysics · Physics 2009-11-13 Peng-fei Yin , Jia Liu , Qiang Yuan , Xiao-jun Bi , Shou-hua Zhu

Particles beyond the Standard Model (SM) can generically have lifetimes that are long compared to SM particles at the weak scale. When produced at experiments such as the Large Hadron Collider (LHC) at CERN, these long-lived particles…

High Energy Physics - Experiment · Physics 2020-09-11 Juliette Alimena , James Beacham , Martino Borsato , Yangyang Cheng , Xabier Cid Vidal , Giovanna Cottin , Albert De Roeck , Nishita Desai , David Curtin , Jared A. Evans , Simon Knapen , Sabine Kraml , Andre Lessa , Zhen Liu , Sascha Mehlhase , Michael J. Ramsey-Musolf , Heather Russell , Jessie Shelton , Brian Shuve , Monica Verducci , Jose Zurita , Todd Adams , Michael Adersberger , Cristiano Alpigiani , Artur Apresyan , Robert John Bainbridge , Varvara Batozskaya , Hugues Beauchesne , Lisa Benato , S. Berlendis , Eshwen Bhal , Freya Blekman , Christina Borovilou , Jamie Boyd , Benjamin P. Brau , Lene Bryngemark , Oliver Buchmueller , Malte Buschmann , William Buttinger , Mario Campanelli , Cari Cesarotti , Chunhui Chen , Hsin-Chia Cheng , Sanha Cheong , Matthew Citron , Andrea Coccaro , V. Coco , Eric Conte , Félix Cormier , Louie D. Corpe , Nathaniel Craig , Yanou Cui , Elena Dall'Occo , C. Dallapiccola , M. R. Darwish , Alessandro Davoli , Annapaola de Cosa , Andrea De Simone , Luigi Delle Rose , Frank F. Deppisch , Biplab Dey , Miriam D. Diamond , Keith R. Dienes , Sven Dildick , Babette Döbrich , Marco Drewes , Melanie Eich , M. ElSawy , Alberto Escalante del Valle , Gabriel Facini , Marco Farina , Jonathan L. Feng , Oliver Fischer , H. U. Flaecher , Patrick Foldenauer , Marat Freytsis , Benjamin Fuks , Iftah Galon , Yuri Gershtein , Stefano Giagu , Andrea Giammanco , Vladimir V. Gligorov , Tobias Golling , Sergio Grancagnolo , Giuliano Gustavino , Andrew Haas , Kristian Hahn , Jan Hajer , Ahmed Hammad , Lukas Heinrich , Jan Heisig , J. C. Helo , Gavin Hesketh , Christopher S. Hill , Martin Hirsch , M. Hohlmann , W. Hulsbergen , John Huth , Philip Ilten , Thomas Jacques , Bodhitha Jayatilaka , Geng-Yuan Jeng , K. A. Johns , Toshiaki Kaji , Gregor Kasieczka , Yevgeny Kats , Malgorzata Kazana , Henning Keller , Maxim Yu. Khlopov , Felix Kling , Ted R. Kolberg , Igor Kostiuk , Emma Sian Kuwertz , Audrey Kvam , Greg Landsberg , Gaia Lanfranchi , Iñaki Lara , Alexander Ledovskoy , Dylan Linthorne , Jia Liu , Iacopo Longarini , Steven Lowette , Henry Lubatti , Margaret Lutz , Jingyu Luo , Judita Mamužić , Matthieu Marinangeli , Alberto Mariotti , Daniel Marlow , Matthew McCullough , Kevin McDermott , P. Mermod , David Milstead , Vasiliki A. Mitsou , Javier Montejo Berlingen , Filip Moortgat , Alessandro Morandini , Alice Polyxeni Morris , David Michael Morse , Stephen Mrenna , Benjamin Nachman , Miha Nemevšek , Fabrizio Nesti , Christian Ohm , Silvia Pascoli , Kevin Pedro , Cristián Peña , Karla Josefina Pena Rodriguez , Jónatan Piedra , James L. Pinfold , Antonio Policicchio , Goran Popara , Jessica Prisciandaro , Mason Proffitt , Giorgia Rauco , Federico Redi , Matthew Reece , Allison Reinsvold Hall , H. Rejeb Sfar , Sophie Renner , Amber Roepe , Manfredi Ronzani , Ennio Salvioni , Arka Santra , Ryu Sawada , Jakub Scholtz , Philip Schuster , Pedro Schwaller , Cristiano Sebastiani , Sezen Sekmen , Michele Selvaggi , Weinan Si , Livia Soffi , Daniel Stolarski , David Stuart , John Stupak , Kevin Sung , Wendy Taylor , Sebastian Templ , Brooks Thomas , Emma Torró-Pastor , Daniele Trocino , Sebastian Trojanowski , Marco Trovato , Yuhsin Tsai , C. G. Tully , Tamás Álmos Vámi , Juan Carlos Vasquez , Carlos Vázquez Sierra , K. Vellidis , Basile Vermassen , Martina Vit , Devin G. E. Walker , Xiao-Ping Wang , Gordon Watts , Si Xie , Melissa Yexley , Charles Young , Jiang-Hao Yu , Piotr Zalewski , Yongchao Zhang

The Milky Way is expected to be embedded in a halo of dark matter particles, with the highest density in the central region, and decreasing density with the halo-centric radius. Dark matter might be indirectly detectable at Earth through a…

High Energy Astrophysical Phenomena · Physics 2016-02-23 IceCube Collaboration , M. G. Aartsen , K. Abraham , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. Ahrens , D. Altmann , T. Anderson , M. Archinger , C. Arguelles , T. C. Arlen , J. Auffenberg , X. Bai , S. W. Barwick , V. Baum , R. Bay , J. J. Beatty , J. Becker Tjus , K. -H. Becker , E. Beiser , S. BenZvi , P. Berghaus , D. Berley , E. Bernardini , A. Bernhard , D. Z. Besson , G. Binder , D. Bindig , M. Bissok , E. Blaufuss , J. Blumenthal , D. J. Boersma , C. Bohm , M. Börner , F. Bos , D. Bose , S. Böser , O. Botner , J. Braun , L. Brayeur , H. -P. Bretz , A. M. Brown , N. Buzinsky , J. Casey , M. Casier , E. Cheung , D. Chirkin , A. Christov , B. Christy , K. Clark , L. Classen , S. Coenders , D. F. Cowen , A. H. Cruz Silva , J. Daughhetee , J. C. Davis , M. Day , J. P. A. M. de André , C. De Clercq , H. Dembinski , S. De Ridder , P. Desiati , K. D. de Vries , G. de Wasseige , M. de With , T. DeYoung , J. C. Díaz-Vélez , J. P. Dumm , M. Dunkman , R. Eagan , B. Eberhardt , T. Ehrhardt , B. Eichmann , S. Euler , P. A. Evenson , O. Fadiran , S. Fahey , A. R. Fazely , A. Fedynitch , J. Feintzeig , J. Felde , K. Filimonov , C. Finley , T. Fischer-Wasels , S. Flis , T. Fuchs , M. Glagla , T. K. Gaisser , R. Gaior , J. Gallagher , L. Gerhardt , K. Ghorbani , D. Gier , L. Gladstone , T. Glüsenkamp , A. Goldschmidt , G. Golup , J. G. Gonzalez , D. Góra , D. Grant , P. Gretskov , J. C. Groh , A. Groß , C. Ha , C. Haack , A. Haj Ismail , A. Hallgren , F. Halzen , B. Hansmann , K. Hanson , D. Hebecker , D. Heereman , K. Helbing , R. Hellauer , D. Hellwig , S. Hickford , J. Hignight , G. C. Hill , K. D. Hoffman , R. Hoffmann , K. Holzapfe , A. Homeier , K. Hoshina , F. Huang , M. Huber , W. Huelsnitz , P. O. Hulth , K. Hultqvist , S. In , A. Ishihara , E. Jacobi , G. S. Japaridze , K. Jero , M. Jurkovic , B. Kaminsky , A. Kappes , T. Karg , A. Karle , M. Kauer , A. Keivani , J. L. Kelley , J. Kemp , A. Kheirandish , J. Kiryluk , J. Kläs , S. R. Klein , G. Kohnen , R. Koirala , H. Kolanoski , R. Konietz , A. Koob , L. Köpke , C. Kopper , S. Kopper , D. J. Koskinen , M. Kowalski , K. Krings , G. Kroll , M. Kroll , J. Kunnen , N. Kurahashi , T. Kuwabara , M. Labare , J. L. Lanfranchi , M. J. Larson , M. Lesiak-Bzdak , M. Leuermann , J. Leuner , J. Lünemann , J. Madsen , G. Maggi , K. B. M. Mahn , R. Maruyama , K. Mase , H. S. Matis , R. Maunu , F. McNally , K. Meagher , M. Medici , A. Meli , T. Menne , G. Merino , T. Meures , S. Miarecki , E. Middell , E. Middlemas , J. Miller , L. Mohrmann , T. Montaruli , R. Morse , R. Nahnhauer , U. Naumann , H. Niederhausen , S. C. Nowicki , D. R. Nygren , A. Obertacke , A. Olivas , A. Omairat , A. O'Murchadha , T. Palczewski , H. Pandya , L. Paul , J. A. Pepper , C. Pérez de los Heros , C. Pfendner , D. Pieloth , E. Pinat , J. Posselt , P. B. Price , G. T. Przybylski , J. Pütz , M. Quinnan , L. Rädel , M. Rameez , K. Rawlins , P. Redl , R. Reimann , M. Relich , E. Resconi , W. Rhode , M. Richman , S. Richter , B. Riedel , S. Robertson , M. Rongen , C. Rott , T. Ruhe , B. Ruzybayev , D. Ryckbosch , S. M. Saba , L. Sabbatini , H. -G. Sander , A. Sandrock , J. Sandroos , S. Sarkar , K. Schatto , F. Scheriau , M. Schimp , T. Schmidt , M. Schmitz , S. Schoenen , S. Schöneberg , A. Schönwald , A. Schukraft , L. Schulte , D. Seckel , S. Seunarine , R. Shanidze , M. W. E. Smith , D. Soldin , G. M. Spiczak , C. Spiering , M. Stahlberg , M. Stamatikos , T. Stanev , N. A. Stanisha , A. Stasik , T. Stezelberger , R. G. Stokstad , A. Stößl , E. A. Strahler , R. Ström , N. L. Strotjohann , G. W. Sullivan , M. Sutherland , H. Taavola , I. Taboada , S. Ter-Antonyan , A. Terliuk , G. Tešić , S. Tilav , P. A. Toale , M. N. Tobin , D. Tosi , M. Tselengidou , E. Unger , M. Usner , S. Vallecorsa , N. van Eijndhoven , J. Vandenbroucke , J. van Santen , S. Vanheule , J. Veenkamp , M. Vehring , M. Voge , M. Vraeghe , C. Walck , M. Wallraff , N. Wandkowsky , Ch. Weaver , C. Wendt , S. Westerhoff , B. J. Whelan , N. Whitehorn , C. Wichary , K. Wiebe , C. H. Wiebusch , L. Wille , D. R. Williams , H. Wissing , M. Wolf , T. R. Wood , K. Woschnagg , D. L. Xu , X. W. Xu , Y. Xu , J. P. Yanez , G. Yodh , S. Yoshida , P. Zarzhitsky , M. Zoll

The possible existence of a new gauge boson U, light and very weakly coupled, allows for Light Dark Matter particles, which could also be at the origin of the 511 keV line from the galactic bulge. Independently of dark matter, and taking…

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

The high-energy Universe is potentially a great laboratory for searching new light bosons such as axion-like particles (ALPs). Cosmic sources are indeed the scene of violent phenomena that involve strong magnetic field and/or very long…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Pierre Brun

Late time decay of very heavy dark matter is considered as one of the possible explanations for diffuse PeV neutrinos observed in IceCube. We consider implications of multimessenger constraints, and show that proposed models are marginally…

High Energy Physics - Phenomenology · Physics 2015-10-16 Kohta Murase , Ranjan Laha , Shin'ichiro Ando , Markus Ahlers

As is well known, dark matter direct detection experiments will ultimately be limited by a "neutrino floor," due to the scattering of nuclei by MeV neutrinos from, e.g., nuclear fusion in the Sun. Here we point out the existence of a new…

High Energy Astrophysical Phenomena · Physics 2017-11-16 Kenny C. Y. Ng , John F. Beacom , Annika H. G. Peter , Carsten Rott

We explore the potential of studying sterile neutrinos at a future high-energy muon collider, where these particles can generate small active neutrino masses via the seesaw mechanism and exhibit long-lived particle signatures. A Dirac…

High Energy Physics - Phenomenology · Physics 2025-04-10 Qi Bi , Jinhui Guo , Jia Liu , Yan Luo , Xiao-Ping Wang

A number of extensions of the Standard Model predict the existence of new light, weakly-coupled particles that couple to the visible sector through higher-dimensional operators containing one or two photons, suppressed by a high new physics…

High Energy Physics - Phenomenology · Physics 2024-08-30 Krzysztof Jodłowski

The problems of neutrino masses, matter-antimatter asymmetry, and dark matter could be successfully addressed by postulating right-handed neutrinos with Majorana masses below the electroweak scale. In this work, leptonic decays of $W$…

High Energy Physics - Experiment · Physics 2020-02-03 ATLAS Collaboration