English
Related papers

Related papers: Supersymmetric Dark Matter Detection at Post-LEP B…

200 papers

Sub-GeV mass dark matter particles whose collisions with nuclei would not deposit sufficient energy to be detected, could instead be revealed through their interaction with electrons. Analyses of data from direct detection experiments…

High Energy Physics - Phenomenology · Physics 2022-03-24 Muping Chen , Graciela B. Gelmini , Volodymyr Takhistov

Low energy antideuteron detection presents a unique channel for indirect detection, targeting dark matter that annihilates into hadrons in a relatively background-free way. Since the idea was first proposed, many WIMP-type models have…

High Energy Physics - Phenomenology · Physics 2020-05-26 Lisa Randall , Weishuang Linda Xu

Self-interacting dark matter models constitute an attractive solution to problems in structure formation on small scales. A simple realization of these models considers the dark force mediated by a light particle which can couple to the…

Cosmology and Nongalactic Astrophysics · Physics 2018-03-06 Denis S. Robertson , Ivone F. M. Albuquerque

There is almost universal agreement among astronomers that most of the mass in the Universe and most of the mass in the Galactic halo is dark. Many lines of reasoning suggest that the dark matter consists of some new, as yet undiscovered,…

High Energy Physics - Phenomenology · Physics 2009-10-28 G. Jungman , M. Kamionkowski , K. Griest

The nature of dark matter and properties of neutrinos are among the most pressing issues in contemporary particle physics. The dual-phase xenon time-projection chamber is the leading technology to cover the available parameter space for…

Instrumentation and Detectors · Physics 2023-02-10 J. Aalbers , K. Abe , V. Aerne , F. Agostini , S. Ahmed Maouloud , D. S. Akerib , D. Yu. Akimov , J. Akshat , A. K. Al Musalhi , F. Alder , S. K. Alsum , L. Althueser , C. S. Amarasinghe , F. D. Amaro , A. Ames , T. J. Anderson , B. Andrieu , N. Angelides , E. Angelino , J. Angevaare , V. C. Antochi , D. Antón Martin , B. Antunovic , E. Aprile , H. M. Araújo , J. E. Armstrong , F. Arneodo , M. Arthurs , P. Asadi , S. Baek , X. Bai , D. Bajpai , A. Baker , J. Balajthy , S. Balashov , M. Balzer , A. Bandyopadhyay , J. Bang , E. Barberio , J. W. Bargemann , L. Baudis , D. Bauer , D. Baur , A. Baxter , A. L. Baxter , M. Bazyk , K. Beattie , J. Behrens , N. F. Bell , L. Bellagamba , P. Beltrame , M. Benabderrahmane , E. P. Bernard , G. F. Bertone , P. Bhattacharjee , A. Bhatti , A. Biekert , T. P. Biesiadzinski , A. R. Binau , R. Biondi , Y. Biondi , H. J. Birch , F. Bishara , A. Bismark , C. Blanco , G. M. Blockinger , E. Bodnia , C. Boehm , A. I. Bolozdynya , P. D. Bolton , S. Bottaro , C. Bourgeois , B. Boxer , P. Brás , A. Breskin , P. A. Breur , C. A. J. Brew , J. Brod , E. Brookes , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , T. K. Bui , S. Burdin , S. Buse , J. K. Busenitz , D. Buttazzo , M. Buuck , A. Buzulutskov , R. Cabrita , C. Cai , D. Cai , C. Capelli , J. M. R. Cardoso , M. C. Carmona-Benitez , M. Cascella , R. Catena , S. Chakraborty , C. Chan , S. Chang , A. Chauvin , A. Chawla , H. Chen , V. Chepel , N. I. Chott , D. Cichon , A. Cimental Chavez , B. Cimmino , M. Clark , R. T. Co , A. P. Colijn , J. Conrad , M. V. Converse , M. Costa , A. Cottle , G. Cox , O. Creaner , J. J. Cuenca Garcia , J. P. Cussonneau , J. E. Cutter , C. E. Dahl , V. D'Andrea , A. David , M. P. Decowski , J. B. Dent , F. F. Deppisch , L. de Viveiros , P. Di Gangi , A. Di Giovanni , S. Di Pede , J. Dierle , S. Diglio , J. E. Y. Dobson , M. Doerenkamp , D. Douillet , G. Drexlin , E. Druszkiewicz , D. Dunsky , K. Eitel , A. Elykov , T. Emken , R. Engel , S. R. Eriksen , M. Fairbairn , A. Fan , J. J. Fan , S. J. Farrell , S. Fayer , N. M. Fearon , A. Ferella , C. Ferrari , A. Fieguth , A. Fieguth , S. Fiorucci , H. Fischer , H. Flaecher , M. Flierman , T. Florek , R. Foot , P. J. Fox , R. Franceschini , E. D. Fraser , C. S. Frenk , S. Frohlich , T. Fruth , W. Fulgione , C. Fuselli , P. Gaemers , R. Gaior , R. J. Gaitskell , M. Galloway , F. Gao , I. Garcia Garcia , J. Genovesi , C. Ghag , S. Ghosh , E. Gibson , W. Gil , D. Giovagnoli , F. Girard , R. Glade-Beucke , F. Glück , S. Gokhale , A. de Gouvêa , L. Gráf , L. Grandi , J. Grigat , B. Grinstein , M. G. D. van der Grinten , R. Grössle , H. Guan , M. Guida , R. Gumbsheimer , C. B. Gwilliam , C. R. Hall , L. J. Hall , R. Hammann , K. Han , V. Hannen , S. Hansmann-Menzemer , R. Harata , S. P. Hardin , E. Hardy , C. A. Hardy , K. Harigaya , R. Harnik , S. J. Haselschwardt , M. Hernandez , S. A. Hertel , A. Higuera , C. Hils , S. Hochrein , L. Hoetzsch , M. Hoferichter , N. Hood , D. Hooper , M. Horn , J. Howlett , D. Q. Huang , Y. Huang , D. Hunt , M. Iacovacci , G. Iaquaniello , R. Ide , C. M. Ignarra , G. Iloglu , Y. Itow , E. Jacquet , O. Jahangir , J. Jakob , R. S. James , A. Jansen , W. Ji , X. Ji , F. Joerg , J. Johnson , A. Joy , A. C. Kaboth , A. C. Kamaha , K. Kanezaki , K. Kar , M. Kara , N. Kato , P. Kavrigin , S. Kazama , A. W. Keaveney , J. Kellerer , D. Khaitan , A. Khazov , G. Khundzakishvili , I. Khurana , B. Kilminster , M. Kleifges , P. Ko , M. Kobayashi , M. Kobayashi , D. Kodroff , G. Koltmann , A. Kopec , A. Kopmann , J. Kopp , L. Korley , V. N. Kornoukhov , E. V. Korolkova , H. Kraus , L. M. Krauss , S. Kravitz , L. Kreczko , V. A. Kudryavtsev , F. Kuger , J. Kumar , B. López Paredes , L. LaCascio , Q. Laine , H. Landsman , R. F. Lang , E. A. Leason , J. Lee , D. S. Leonard , K. T. Lesko , L. Levinson , C. Levy , I. Li , S. C. Li , T. Li , S. Liang , C. S. Liebenthal , J. Lin , Q. Lin , S. Lindemann , M. Lindner , A. Lindote , R. Linehan , W. H. Lippincott , X. Liu , K. Liu , J. Liu , J. Loizeau , F. Lombardi , J. Long , M. I. Lopes , E. Lopez Asamar , W. Lorenzon , C. Lu , S. Luitz , Y. Ma , P. A. N. Machado , C. Macolino , T. Maeda , J. Mahlstedt , P. A. Majewski , A. Manalaysay , A. Mancuso , L. Manenti , A. Manfredini , R. L. Mannino , N. Marangou , J. March-Russell , F. Marignetti , T. Marrodán Undagoitia , K. Martens , R. Martin , I. Martinez-Soler , J. Masbou , D. Masson , E. Masson , S. Mastroianni , M. Mastronardi , J. A. Matias-Lopes , M. E. McCarthy , N. McFadden , E. McGinness , D. N. McKinsey , J. McLaughlin , K. McMichael , P. Meinhardt , J. Menéndez , Y. Meng , M. Messina , R. Midha , D. Milisavljevic , E. H. Miller , B. Milosevic , S. Milutinovic , S. A. Mitra , K. Miuchi , E. Mizrachi , K. Mizukoshi , A. Molinario , A. Monte , C. M. B. Monteiro , M. E. Monzani , J. S. Moore , K. Morå , J. A. Morad , J. D. Morales Mendoza , S. Moriyama , E. Morrison , E. Morteau , Y. Mosbacher , B. J. Mount , J. Mueller , A. St. J. Murphy , M. Murra , D. Naim , S. Nakamura , E. Nash , N. Navaieelavasani , A. Naylor , C. Nedlik , H. N. Nelson , F. Neves , J. L. Newstead , K. Ni , J. A. Nikoleyczik , V. Niro , U. G. Oberlack , M. Obradovic , K. Odgers , C. A. J. O'Hare , P. Oikonomou , I. Olcina , K. Oliver-Mallory , A. Oranday , J. Orpwood , I. Ostrovskiy , K. Ozaki , B. Paetsch , S. Pal , J. Palacio , K. J. Palladino , J. Palmer , P. Panci , M. Pandurovic , A. Parlati , N. Parveen , S. J. Patton , V. Pěč , Q. Pellegrini , B. Penning , G. Pereira , R. Peres , Y. Perez-Gonzalez , E. Perry , T. Pershing , R. Petrossian-Byrne , J. Pienaar , A. Piepke , G. Pieramico , M. Pierre , M. Piotter , V. Pizella , G. Plante , T. Pollmann , D. Porzio , J. Qi , Y. Qie , J. Qin , N. Raj , M. Rajado Silva , K. Ramanathan , D. Ramírez García , J. Ravanis , L. Redard-Jacot , D. Redigolo , S. Reichard , J. Reichenbacher , C. A. Rhyne , A. Richards , Q. Riffard , G. R. C. Rischbieter , A. Rocchetti , S. L. Rosenfeld , R. Rosero , N. Rupp , T. Rushton , S. Saha , L. Sanchez , P. Sanchez-Lucas , D. Santone , J. M. F. dos Santos , I. Sarnoff , G. Sartorelli , A. B. M. R. Sazzad , M. Scheibelhut , R. W. Schnee , M. Schrank , J. Schreiner , P. Schulte , D. Schulte , H. Schulze Eissing , M. Schumann , T. Schwemberger , A. Schwenk , T. Schwetz , L. Scotto Lavina , P. R. Scovell , H. Sekiya , M. Selvi , E. Semenov , F. Semeria , P. Shagin , S. Shaw , S. Shi , E. Shockley , T. A. Shutt , R. Si-Ahmed , J. J. Silk , C. Silva , M. C. Silva , H. Simgen , F. Šimkovic , G. Sinev , R. Singh , W. Skulski , J. Smirnov , R. Smith , M. Solmaz , V. N. Solovov , P. Sorensen , J. Soria , T. J. Sparmann , I. Stancu , M. Steidl , A. Stevens , K. Stifter , L. E. Strigari , D. Subotic , B. Suerfu , A. M. Suliga , T. J. Sumner , P. Szabo , M. Szydagis , A. Takeda , Y. Takeuchi , P. -L. Tan , C. Taricco , W. C. Taylor , D. J. Temples , A. Terliuk , P. A. Terman , D. Thers , K. Thieme , Th. Thümmler , D. R. Tiedt , M. Timalsina , W. H. To , F. Toennies , Z. Tong , F. Toschi , D. R. Tovey , J. Tranter , M. Trask , G. C. Trinchero , M. Tripathi , D. R. Tronstad , R. Trotta , Y. D. Tsai , C. D. Tunnell , W. G. Turner , R. Ueno , P. Urquijo , U. Utku , A. Vaitkus , K. Valerius , E. Vassilev , S. Vecchi , V. Velan , S. Vetter , A. C. Vincent , L. Vittorio , G. Volta , B. von Krosigk , M. von Piechowski , D. Vorkapic , C. E. M. Wagner , A. M. Wang , B. Wang , Y. Wang , W. Wang , J. J. Wang , L. -T. Wang , M. Wang , Y. Wang , J. R. Watson , Y. Wei , C. Weinheimer , E. Weisman , M. Weiss , D. Wenz , S. M. West , T. J. Whitis , M. Williams , M. J. Wilson , D. Winkler , C. Wittweg , J. Wolf , T. Wolf , F. L. H. Wolfs , S. Woodford , D. Woodward , C. J. Wright , V. H. S. Wu , P. Wu , S. Wüstling , M. Wurm , Q. Xia , X. Xiang , Y. Xing , J. Xu , Z. Xu , D. Xu , M. Yamashita , R. Yamazaki , H. Yan , L. Yang , Y. Yang , J. Ye , M. Yeh , I. Young , H. B. Yu , T. T. Yu , L. Yuan , G. Zavattini , S. Zerbo , Y. Zhang , M. Zhong , N. Zhou , X. Zhou , T. Zhu , Y. Zhu , Y. Zhuang , J. P. Zopounidis , K. Zuber , J. Zupan

In this work, we investigate a neutrinophilic low-mass dark matter model mediated by a pseudoscalar particle. Since dark matter lacks Standard Model gauge charges, new interactions are required to connect it to the visible sector.…

High Energy Physics - Phenomenology · Physics 2026-03-31 Zhuo Zhang , Lian-Bao Jia , Reyes J. F. Eduardo

Dark matter particles captured by the Sun through scattering may annihilate and produce neutrinos, which escape. Current searches are for the few high-energy neutrinos produced in the prompt decays of some final states. We show that…

High Energy Astrophysical Phenomena · Physics 2013-09-06 Carsten Rott , Jennifer Siegal-Gaskins , John F. Beacom

We explore the detection prospects for a minimal secluded dark matter model, where a fermionic dark matter particle interacts with the Standard Model (SM) via a kinetically mixed dark photon. We focus on scenarios where the dark photon…

High Energy Physics - Phenomenology · Physics 2026-01-29 Ahmed Alenezi , Cari Cesarotti , Stefania Gori , Jessie Shelton

The addition of non-renormalizable terms involving the Higgs fields to the MSSM ameliorates the little hierarchy problem of the MSSM. For neutralino dark matter, new regions for which the relic abundance of the LSP is consistent with WMAP…

High Energy Physics - Phenomenology · Physics 2010-05-13 Nicolas Bernal

In this Letter we explore the direct detection of the dark matter in the universe, assuming the dark matter particles are degenerate in mass with new colored particles below TeV scale. The scenario with such a mass spectrum is difficult to…

High Energy Physics - Phenomenology · Physics 2011-12-22 Junji Hisano , Koji Ishiwata , Natsumi Nagata

Particles with TeV mass and strong self-interactions generically have the right annihilation cross section to explain an observed excess of cosmic electrons and positrons if the end-product of the annihilation is charged leptons. We present…

High Energy Physics - Phenomenology · Physics 2010-08-12 Yi Cai , David E. Kaplan , Markus A. Luty

The dark matter (DM) blind spots in the Minimal Supersymmetric Standard Model (MSSM) refer to the parameter regions where the couplings of the DM particles to the $Z$-boson or the Higgs boson are almost zero, leading to vanishingly small…

High Energy Physics - Phenomenology · Physics 2017-04-13 Tao Han , Felix Kling , Shufang Su , Yongcheng Wu

Cosmological observations indicate that most of the matter in the Universe is Dark Matter. Dark Matter in the form of Weakly Interacting Massive Particles (WIMPs) can be detected directly, via its elastic scattering off target nuclei. Most…

Self-annihilating dark matter gravitationally captured by the Sun could yield observable neutrino signals at current and next generation neutrino detectors. By exploiting such signals, neutrino detectors can probe the spin-dependent…

High Energy Astrophysical Phenomena · Physics 2011-09-26 Carsten Rott , Takayuki Tanaka , Yoshitaka Itow

We reexamine the constrained version of the Next-to-Minimal Supersymmetric Standard Model with semi universal parameters at the GUT scale (CNMSSM). We include constraints from collider searches for Higgs and SUSY particles, upper bound on…

High Energy Physics - Phenomenology · Physics 2009-01-16 G. Belanger , C. Hugonie , A. Pukhov

We analyze the antimatter yield of supersymmetric (SUSY) models with large neutralino annihilation cross sections. We introduce three benchmark scenarios, respectively featuring bino, wino and higgsino-like lightest neutralinos, and we…

High Energy Physics - Phenomenology · Physics 2007-05-23 Stefano Profumo , Piero Ullio

We update a previously-proposed set of supersymmetric benchmark scenarios, taking into account the precise constraints on the cold dark matter density obtained by combining WMAP and other cosmological data, as well as the LEP and b -> s…

High Energy Physics - Phenomenology · Physics 2009-09-11 M. Battaglia , A. De Roeck , J. Ellis , F. Gianotti , K. A. Olive , L. Pape

We consider searches for dark matter annihilation to monoenergetic neutrinos in the core of the Sun. We find that liquid scintillation neutrino detectors have enhanced sensitivity to this class of dark matter models, due to the energy and…

High Energy Physics - Phenomenology · Physics 2015-07-14 Jason Kumar , Pearl Sandick

We compare the first results on searches for supersymmetry with the Large Hadron Collider (LHC) to the current and near-term performance of experiments sensitive to neutralino dark matter. We limit our study to the particular slices of…

High Energy Physics - Phenomenology · Physics 2011-08-08 Stefano Profumo