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Related papers: Light new physics in XENON1T

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We present a particle physics model to explain the observed enhancement in the Xenon-1T data at an electron recoil energy of 2.5 keV. The model is based on a $U(1)$ extension of the Standard Model where the dark sector consists of two…

High Energy Physics - Phenomenology · Physics 2021-03-17 Amin Aboubrahim , Michael Klasen , Pran Nath

With large active volume sizes dark matter direct detection experiments are sensitive to solar neutrino fluxes. Nuclear recoil signals are induced by $^8$B neutrinos, while electron recoils are mainly generated by the pp flux. Measurements…

High Energy Physics - Phenomenology · Physics 2021-02-03 D. Aristizabal Sierra , R. Branada , O. G. Miranda , G. Sanchez Garcia

LUX-ZEPLIN (LZ) is a dark matter detector expected to obtain world-leading sensitivity to weakly interacting massive particles (WIMPs) interacting via nuclear recoils with a ~7-tonne xenon target mass. This manuscript presents sensitivity…

High Energy Physics - Experiment · Physics 2022-02-18 The LZ Collaboration , D. S. Akerib , A. K. Al Musalhi , S. K. Alsum , C. S. Amarasinghe , A. Ames , T. J. Anderson , N. Angelides , H. M. Araújo , J. E. Armstrong , M. Arthurs , X. Bai , J. Balajthy , S. Balashov , J. Bang , J. W. Bargemann , D. Bauer , A. Baxter , P. Beltrame , E. P. Bernard , A. Bernstein , A. Bhatti , A. Biekert , T. P. Biesiadzinski , H. J. Birch , G. M. Blockinger , E. Bodnia , B. Boxer , C. A. J. Brew , P. Brás , S. Burdin , J. K. Busenitz , M. Buuck , R. Cabrita , M. C. Carmona-Benitez , M. Cascella , C. Chan , N. I. Chott , A. Cole , M. V. Converse , A. Cottle , G. Cox , O. Creaner , J. E. Cutter , C. E. Dahl , L. de Viveiros , J. E. Y. Dobson , E. Druszkiewicz , S. R. Eriksen , A. Fan , S. Fayer , N. M. Fearon , S. Fiorucci , H. Flaecher , E. D. Fraser , T. Fruth , R. J. Gaitskell , J. Genovesi , C. Ghag , E. Gibson , S. Gokhale , M. G. D. van der Grinten , C. B. Gwilliam , C. R. Hall , C. A. Hardy , S. J. Haselschwardt , S. A. Hertel , M. Horn , D. Q. Huang , C. M. Ignarra , O. Jahangir , R. S. James , W. Ji , J. Johnson , A. C. Kaboth , A. C. Kamaha , K. Kamdin , K. Kazkaz , D. Khaitan , A. Khazov , I. Khurana , D. Kodroff , L. Korley , E. V. Korolkova , H. Kraus , S. Kravitz , L. Kreczko , B. Krikler , V. A. Kudryavtsev , E. A. Leason , J. Lee , D. S. Leonard , K. T. Lesko , C. Levy , J. Li , J. Liao , A. Lindote , R. Linehan , W. H. Lippincott , X. Liu , M. I. Lopes , E. Lopez Asamar , B. López Paredes , W. Lorenzon , S. Luitz , P. A. Majewski , A. Manalaysay , L. Manenti , R. L. Mannino , N. Marangou , M. E. McCarthy , D. N. McKinsey , J. McLaughlin , E. H. Miller , E. Mizrachi , A. Monte , M. E. Monzani , J. A. Morad , J. D. Morales Mendoza , E. Morrison , B. J. Mount , A. St. J. Murphy , D. Naim , A. Naylor , C. Nedlik , H. N. Nelson , F. Neves , J. A. Nikoleyczik , A. Nilima , A. Nguyen , I. Olcina , K. C. Oliver-Mallory , S. Pal , K. J. Palladino , J. Palmer , S. Patton , N. Parveen , E. K. Pease , B. Penning , G. Pereira , A. Piepke , Y. Qie , J. Reichenbacher , C. A. Rhyne , A. Richards , Q. Riffard , G. R. C. Rischbieter , R. Rosero , P. Rossiter , D. Santone , A. B. M. R. Sazzad , R. W. Schnee , P. R. Scovell , S. Shaw , T. A. Shutt , J. J. Silk , C. Silva , R. Smith , M. Solmaz , V. N. Solovov , P. Sorensen , J. Soria , I. Stancu , A. Stevens , K. Stifter , B. Suerfu , T. J. Sumner , N. Swanson , M. Szydagis , W. C. Taylor , R. Taylor , D. J. Temples , P. A. Terman , D. R. Tiedt , M. Timalsina , W. H. To , D. R. Tovey , M. Tripathi , D. R. Tronstad , W. Turner , U. Utku , A. Vaitkus , B. Wang , J. J. Wang , W. Wang , J. R. Watson , R. C. Webb , R. G. White , T. J. Whitis , M. Williams , F. L. H. Wolfs , D. Woodward , C. J. Wright , X. Xiang , J. Xu , M. Yeh , P. Zarzhitsky

Neutrinos elastically scattered off atomic electrons offer a unique opportunity to probe the Standard Model (SM) and beyond SM physics. In this work, we examine the new physics effects of light mediators through elastic neutrino-electron…

High Energy Physics - Phenomenology · Physics 2025-03-28 Mehmet Demirci , M. Fauzi Mustamin

The main alternatives of the recent XENON1T observation are solar axions, neutrino magnetic moment and tritium. In this short note we suggest to crosscheck whether the observation is related or not to dark matter (DM) streams, by searching…

High Energy Physics - Phenomenology · Physics 2020-07-01 K. Zioutas , G. Cantatore , M. Karuza , A. Kryemadhi , M. Maroudas , Y. K. Semertzidis

Recent progress in phonon-mediated detectors with eV-scale nuclear recoil energy sensitivity requires an understanding of the effect of the crystalline defects on the energy spectrum expected from dark matter or neutrino coherent…

High Energy Physics - Phenomenology · Physics 2022-10-05 Sebastian Sassi , Matti Heikinheimo , Kimmo Tuominen , Antti Kuronen , Jesper Byggmästar , Kai Nordlund , Nader Mirabolfathi

The recent XENON1T excess can be explained by the solar active-sterile neutrino conversion with bound electrons via light mediator. Nevertheless, the atomic effects are usually omitted in the solar neutrino explanations. We systematically…

High Energy Physics - Phenomenology · Physics 2022-06-01 Shao-Feng Ge , Pedro Pasquini , Jie Sheng

We demonstrate that current and planned underground neutrino experiments could offer a powerful probe of few-MeV dark matter when combined with a nearby high-intensity low-to-medium energy electron accelerator. This experimental setup, an…

High Energy Physics - Phenomenology · Physics 2015-11-18 Eder Izaguirre , Gordan Krnjaic , Maxim Pospelov

We study dark matter physics in the Minimal Supersymmetric Standard Model with non-universal gaugino masses at the unification scale. In this scenario, the specific ratio of wino and gluino masses realizes the electro-weak scale naturally…

High Energy Physics - Phenomenology · Physics 2017-09-13 Junichiro Kawamura , Yuji Omura

Results from the nuclear recoil calibration of the XENON100 dark matter detector installed underground at the Laboratori Nazionali del Gran Sasso (LNGS), Italy are presented. Data from measurements with an external 241AmBe neutron source…

We propose a self-interacting inelastic dark matter (DM) scenario as a possible origin of the recently reported excess of electron recoil events by the XENON1T experiment. Two quasi-degenerate Majorana fermion DM interact within themselves…

High Energy Physics - Phenomenology · Physics 2021-05-26 Manoranjan Dutta , Satyabrata Mahapatra , Debasish Borah , Narendra Sahu

We present the results of a direct detection search for mirror dark matter interactions, using data collected from the Large Underground Xenon experiment during 2013, with an exposure of 95 live-days $\times$ 118 kg. Here, the calculations…

Dual-phase xenon time projection chamber (TPC) detectors offer heightened sensitivities for dark matter detection across a spectrum of particle masses. To broaden their capability to low-mass dark matter interactions, we investigated the…

The multi-staged XENON program at INFN Laboratori Nazionali del Gran Sasso aims to detect dark matter with two-phase liquid xenon time projection chambers of increasing size and sensitivity. The XENONnT experiment is the latest detector in…

Instrumentation and Detectors · Physics 2025-08-14 XENON Collaboration , E. Aprile , J. Aalbers , K. Abe , S. Ahmed Maouloud , L. Althueser , B. Andrieu , E. Angelino , J. R. Angevaare , V. C. Antochi , D. Antón Martin , F. Arneodo , M. Balata , L. Baudis , A. L. Baxter , M. Bazyk , L. Bellagamba , R. Biondi , A. Bismark , E. J. Brookes , A. Brown , S. Bruenner , G. Bruno , R. Budnik , T. K. Bui , C. Cai , J. M. R. Cardoso , F. Cassese , A. Chiarini , D. Cichon , A. P. Cimental Chavez , A. P. Colijn , J. Conrad , R. Corrieri , J. J. Cuenca-García , J. P. Cussonneau , O. Dadoun , V. D'Andrea , M. P. Decowski , B. De Fazio , P. Di Gangi , S. Diglio , J. M. Disdier , D. Douillet , K. Eitel , A. Elykov , S. Farrell , A. D. Ferella , C. Ferrari , H. Fischer , M. Flierman , S. Form , D. Front , W. Fulgione , C. Fuselli , P. Gaemers , R. Gaior , A. Gallo Rosso , M. Galloway , F. Gao , R. Gardner , N. Garroum , R. Glade-Beucke , L. Grandi , J. Grigat , H. Guan , M. Guerzoni , M. Guida , R. Hammann , A. Higuera , C. Hils , L. Hoetzsch , N. F. Hood , J. Howlett , C. Huhmann , M. Iacovacci , G. Iaquaniello , L. Iven , Y. Itow , J. Jakob , F. Joerg , A. Joy , M. Kara , P. Kavrigin , S. Kazama , M. Kobayashi , G. Koltman , A. Kopec , F. Kuger , H. Landsman , R. F. Lang , L. Levinson , I. Li , S. Li , S. Liang , S. Lindemann , M. Lindner , K. Liu , J. Loizeau , F. Lombardi , J. Long , J. A. M. Lopes , Y. Ma , C. Macolino , J. Mahlstedt , A. Mancuso , L. Manenti , F. Marignetti , T. Marrodán Undagoitia , P. Martella , K. Martens , J. Masbou , D. Masson , E. Masson , S. Mastroianni , E. Mele , M. Messina , R. Michinelli , K. Miuchi , A. Molinario , S. Moriyama , K. Morå , Y. Mosbacher , M. Murra , J. Müller , K. Ni , S. Nisi , U. Oberlack , D. Orlandi , R. Othegraven , B. Paetsch , J. Palacio , S. Parlati , P. Paschos , Q. Pellegrini , R. Peres , C. Peters , J. Pienaar , M. Pierre , G. Plante , T. R. Pollmann , J. Qi , J. Qin , D. Ramírez García , M. Rynge , J. Shi , R. Singh , L. Sanchez , J. M. F. dos Santos , I. Sarnoff , G. Sartorelli , J. Schreiner , D. Schulte , P. Schulte , H. Schulze Eißing , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , S. Shi , E. Shockley , M. Silva , H. Simgen , J. Stephen , M. Stern , B. K. Stillwell , A. Takeda , P. -L. Tan , D. Tatananni , A. Terliuk , D. Thers , F. Toschi , G. Trinchero , C. Tunnell , F. Tönnies , K. Valerius , G. Volta , C. Weinheimer , M. Weiss , D. Wenz , J. Westermann , C. Wittweg , T. Wolf , V. H. S. Wu , Y. Xing , D. Xu , Z. Xu , M. Yamashita , L. Yang , J. Ye , L. Yuan , G. Zavattini , M. Zhong , T. Zhu

Sterile neutrinos are possible dark matter candidates. We examine here possible detection mechanisms, assuming that the neutrino has a mass of about 50 keV and couples to the ordinary neutrino. Even though this neutrino is quite heavy, it…

High Energy Physics - Phenomenology · Physics 2018-09-25 Paraskevi C. Divari , John D. Vergados

In this work we analyse the ultimate sensitivity of dark matter direct detection experiments, the "neutrino-floor", in the presence of anomalous sources of dark radiation in form of SM or semi-sterile neutrinos. This flux-component is…

High Energy Physics - Phenomenology · Physics 2020-09-01 Marco Nikolic , Suchita Kulkarni , Josef Pradler

The recent puzzling results of the XENON1T collaboration at few keV electronic recoils could be due to the scattering of solar neutrinos endowed with finite Majorana transition magnetic moments (TMMs). Within such general formalism, we find…

High Energy Physics - Phenomenology · Physics 2020-08-18 O. G. Miranda , D. K. Papoulias , M. Tórtola , J. W. F. Valle

The growing interest in the interactions between dark matter particles and electrons has received a further boost by the observation of an excess in electron recoil events in the XENON1T experiment. Of particular interest are dark matter…

High Energy Physics - Phenomenology · Physics 2022-03-31 Timon Emken , Jonas Frerick , Saniya Heeba , Felix Kahlhoefer

Motivated by various kinds of new physics models, a new light neutral vector boson (the dark photon) connected to the Standard Model of particle physics only through the kinetic mixing with the U(1)_Y factor has been studied extensively.…

High Energy Physics - Phenomenology · Physics 2014-02-03 Haipeng An , Maxim Pospelov , Josef Pradler