In)direct detection of boosted dark matter
TL;DR: In this paper, the authors studied the effects of the annihilation of DM in the galactic center on the creation of boosted stable particles in the dark sector, which can be detected in large volume terrestrial experiments via neutral-current-like interactions with electrons or nuclei.
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Abstract: We initiate the study of novel thermal dark matter (DM) scenarios where present-day annihilation of DM in the galactic center produces boosted stable particles in the dark sector. These stable particles are typically a subdominant DM component, but because they are produced with a large Lorentz boost in this process, they can be detected in large volume terrestrial experiments via neutral-current-like interactions with electrons or nuclei. This novel DM signal thus combines the production mechanism associated with indirect detection experiments (i.e. galactic DM annihilation) with the detection mechanism associated with direct detection experiments (i.e. DM scattering off terrestrial targets). Such processes are generically present in multi-component DM scenarios or those with non-minimal DM stabilization symmetries. As a proof of concept, we present a model of two-component thermal relic DM, where the dominant heavy DM species has no tree-level interactions with the standard model and thus largely evades direct and indirect DM bounds. Instead, its thermal relic abundance is set by annihilation into a subdominant lighter DM species, and the latter can be detected in the boosted channel via the same annihilation process occurring today. Especially for dark sector masses in the 10 MeV–10 GeV range, the most promising signals aremore » electron scattering events pointing toward the galactic center. These can be detected in experiments designed for neutrino physics or proton decay, in particular Super-K and its upgrade Hyper-K, as well as the PINGU/MICA extensions of IceCube. This boosted DM phenomenon highlights the distinctive signatures possible from non-minimal dark sectors.« less
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TL;DR: In this paper, the production and decay properties of new light gauge bosons were identified, and five new experimental approaches were proposed to cover most of the natural parameter space, using currently operating GeV-energy beams and well-established detection methods.
ANTARES: the first undersea neutrino telescope
M. Ageron,Juanan Aguilar,I. Al Samarai,Arnauld Albert,Fabrizio Ameli,Michel André,M. Anghinolfi,Gisela Anton,S. Anvar,Miguel Ardid,K. Arnaud,Elie Aslanides,A. C.S. Assis Jesus,Tri L. Astraatmadja,J-J. Aubert,R. Auer,E. Barbarito,B. Baret,S. Basa,M. Bazzotti,Yvonne Becherini,J. Beltramelli,A. Bersani,V. Bertin,S. Beurthey,S. Biagi,Ciro Bigongiari,M. Billault,R. Blaes,C. Bogazzi,N. de Botton,Manuel Bou-Cabo,B. Boudahef,M.C. Bouwhuis,A. M. Brown,Jürgen Brunner,Jose Busto,L. Caillat,A. Calzas,Francisco Camarena,A. Capone,L. Caponetto,C. Cârloganu,G. Carminati,E. Carmona,J. Carr,P. H. Carton,B. Cassano,E. Castorina,S. Cecchini,A. Ceres,Th. Chaleil,Ph. Charvis,P. Chauchot,Tommaso Chiarusi,M. Circella,Chantal Compère,R. Coniglione,X. Coppolani,A. Cosquer,Heide Costantini,N. Cottini,P. Coyle,S. Cuneo,C. Curtil,C. D'Amato,G. Damy,R. van Dantzig,G. De Bonis,G. Decock,M. P. Decowski,I. Dekeyser,E. Delagnes,F. Desages-Ardellier,Anne Deschamps,J.-J. Destelle,F. Di Maria,B. Dinkespiler,C. Distefano,J.-L. Dominique,C. Donzaud,C. Donzaud,Damien Dornic,Damien Dornic,Q. Dorosti,J. F. Drogou,Doriane Drouhin,F. Druillole,Dominique Durand,R. Durand,Thomas Eberl,U. Emanuele,J.J. Engelen,J.-P. Ernenwein,Stephanie Escoffier,E. Falchini,S. Favard,F. Fehr,F. Feinstein,M. Ferri,S. Ferry,C. Fiorello,V. Flaminio,F. Folger,U. Fritsch,J.-L. Fuda,S. Galatà,S. Galeotti,F. Gensolen,G. Giacomelli,C. Gojak,J.P. Gómez-González,P. Goret,Kay Graf,G. Guillard,G. Halladjian,Gregory David Hallewell,H. van Haren,B. Hartmann,A.J. Heijboer,E. Heine,Yann Hello,S. Henry,Juan José Hernández-Rey,B. Herold,J. Hößl,J. Hogenbirk,C. C. Hsu,J.R. Hubbard,M. Jaquet,M. Jaspers,M. de Jong,D. Jourde,Matthias Kadler,Nasser Kalantar-Nayestanaki,Oleg Kalekin,Alexander Kappes,Timo Karg,S. Karkar,M. Karolak,U. F. Katz,P. Keller,Pierre Kestener,E. Kok,H. Kok,P.M. Kooijman,P.M. Kooijman,C. Kopper,A. Kouchner,W. Kretschmer,A. Kruijer,S. Kuch,Vladimir Kulikovskiy,D. Lachartre,H. Lafoux,P. Lagier,Robert Lahmann,C. Lahonde-Hamdoun,Patrick Lamare,Guillaume Lambard,J.-C. Languillat,Giuseppina Larosa,J. Lavalle,Y. Le Guen,H. Le Provost,A. LeVanSuu,Dominique Lefèvre,T. Legou,G. Lelaizant,C. Lévéque,G. Lim,D. Lo Presti,H. Loehner,S. Loucatos,F. Louis,F. Lucarelli,V. Lyashuk,P. Magnier,S. Mangano,A. Marcel,M. Marcelin,Annarita Margiotta,J.A. Martínez-Mora,R. Masullo,F. Mazéas,Alain Mazure,Athina Meli,M. Melissas,E. Migneco,M. Mongelli,Teresa Montaruli,M. Morganti,L. Moscoso,Holger Motz,Mario Musumeci,C. L. Naumann,M. Naumann-Godo,M. Neff,V. Niess,Gerardus Nooren,J.E.J. Oberski,C. Olivetto,Nathalie Palanque-Delabrouille,D. Palioselitis,Riccardo Papaleo,G.E. Păvălaş,K. Payet,P. Payre,H. Peek,J. Petrovic,Paolo Piattelli,N. Picot-Clemente,C. Picq,Y. Piret,J. Poinsignon,V. Popa,T. Pradier,E. Presani,G. Prono,C. Racca,G. Raia,J. van Randwijk,Diego Real,C. Reed,F. Réthoré,P. Rewiersma,Giorgio Riccobene,C. Richardt,R. Richter,J.S. Ricol,V. Rigaud,V. Roca,K. Roensch,Jean-Francois Rolin,A. Rostovtsev,A. Rottura,J. Roux,M. Rujoiu,M. Ruppi,G.V. Russo,F. Salesa,K. Salomon,Paolo Sapienza,F. Schmitt,F. M. Schöck,J. P. Schuller,F. Schüssler,D. Sciliberto,Rezo Shanidze,E. Shirokov,Francesco Simeone,Andrea Sottoriva,A. Spies,T. Spona,Maurizio Spurio,Jos Steijger,Th. Stolarczyk,K. Streeb,L. Sulak,M. Taiuti,Christian Tamburini,Charling Tao,L. A. M. Tasca,G. Terreni,D. Tezier,Simona Toscano,F. Urbano,P. Valdy,B. Vallage,V. Van Elewyck,G. Vannoni,Manuela Vecchi,Manuela Vecchi,G. Venekamp,B. Verlaat,P. Vernin,E. Virique,G. de Vries,R. van Wijk,G. Wijnker,G. Wobbe,E. A. De Wolf,Y. Yakovenko,H. Yepes,D. Zaborov,H. Zaccone,J.D. Zornoza,J. Zúñiga +287 more
TL;DR: The ANTARES Neutrino Telescope was completed in May 2008 and is the first operational neutrino telescope in the Mediterranean Sea as mentioned in this paper, where the main purpose of the detector is to perform neutrinos astronomy and the apparatus also offers facilities for marine and Earth sciences.
Search for low-mass weakly interacting massive particles with SuperCDMS.
R. Agnese,Adam Anderson,M. Asai,D. Balakishiyeva,R. Basu Thakur,D. A. Bauer,J. Beaty,J. Billard,A. W. Borgland,M. A. Bowles,D. Brandt,P. L. Brink,R. Bunker,Blas Cabrera,David O. Caldwell,David G. Cerdeño,H. Chagani,Yan Chen,M. Cherry,Jodi Cooley,B. Cornell,C. H. Crewdson,P. Cushman,Miguel Daal,D. Devaney,P. Di Stefano,E. Do Couto E Silva,T. Doughty,L. Esteban,S. Fallows,Enectali Figueroa-Feliciano,G. Godfrey,Sunil Golwala,J. Hall,Sissel Hansen,H. R. Harris,S. A. Hertel,B. A. Hines,T. Hofer,Donald J. Holmgren,L. Hsu,Martin E. Huber,A. Jastram,O. Kamaev,B. Kara,M. H. Kelsey,S. Kenany,A. Kennedy,M. Kiveni,K. Koch,A. Leder,B. Loer,E. Lopez Asamar,R. Mahapatra,Vuk Mandic,Cristián Martínez,Kevin A. McCarthy,N. Mirabolfathi,Robert A. Moffatt,R. H. Nelson,L. Novak,K. L. Page,R. Partridge,M. Pepin,A. Phipps,M. Platt,K. Prasad,Matt Pyle,H. Qiu,W. Rau,P. Redl,A. Reisetter,R. Resch,Y. Ricci,M. Ruschman,Tarek Saab,Bernard Sadoulet,J. Sander,R. Schmitt,K. Schneck,R. W. Schnee,S. Scorza,D. N. Seitz,B. Serfass,B. Shank,Danielle Speller,Astrid Tomada,S. Upadhyayula,A. N. Villano,B. Welliver,Douglas Wright,S. J. Yellin,J. J. Yen,Betty A. Young,J. Zhang +94 more
TL;DR: The first search for weakly interacting massive particles (WIMPs) using the background rejection capabilities of SuperCDMS was reported in this article, where an exposure of 577 kg days was analyzed for WIMPs with mass <30 ǫ, with the signal region blinded.