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Journal articles on the topic 'Xenon136'

Author: Grafiati

Published: 4 June 2021

Last updated: 10 February 2022

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1

Davide, Ferella Alfredo. "Direct WIMP searches with XENON100 and XENON1T." EPJ Web of Conferences 95 (2015): 04019. http://dx.doi.org/10.1051/epjconf/20159504019.

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2

Alfonsi, Matteo. "The XENON Dark Matter project: from XENON100 to XENON1T." Nuclear and Particle Physics Proceedings 273-275 (April 2016): 373–77. http://dx.doi.org/10.1016/j.nuclphysbps.2015.09.053.

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3

Fieguth, Alexander. "Search for doubleβ-decays of124Xe with XENON100 & XENON1T". Journal of Physics: Conference Series 888 (вересень 2017): 012251. http://dx.doi.org/10.1088/1742-6596/888/1/012251.

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4

Persiani, Rino. "RESULTS FROM THE XENON100 EXPERIMENT." Acta Polytechnica 53, A (2013): 555–59. http://dx.doi.org/10.14311/ap.2013.53.0555.

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The XENON program consists in operating and developing double-phase time projection chambers using liquid xenon as the target material. It aims to directly detect dark matter in the form of WIMPs via their elastic scattering off xenon nuclei. The current phase is XENON100, located at the Laboratori Nazionali del Gran Sasso (LNGS), with a 62 kg liquid xenon target. We present the 100.9 live days of data, acquired between January and June 2010, with no evidence of dark matter, as well as the new results of the last scientific run, with about 225 live days. The next phase, XENON1T, will increase

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5

BAO, SHOU-SHAN, XUE GONG, ZONG-GUO SI, and YU-FENG ZHOU. "FOURTH GENERATION MAJORANA NEUTRINO, DARK MATTER AND HIGGS PHYSICS." International Journal of Modern Physics A 29, no. 02 (2014): 1450010. http://dx.doi.org/10.1142/s0217751x14500109.

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We consider extensions of the standard model with fourth generation fermions (SM4) in which extra symmetries are introduced such that the transitions between the fourth generation fermions and the ones in the first three generations are forbidden. In these models, the stringent lower bounds on the masses of fourth generation quarks from direct searches can be relaxed, and the lightest fourth neutrino is allowed to be stable and light enough to trigger the Higgs boson invisible decay. In addition, the fourth Majorana neutrino can be a subdominant but highly detectable dark matter component. We

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6

Ni, Kaixuan, Jianyang Qi, Evan Shockley, and Yuehuan Wei. "Sensitivity of a Liquid Xenon Detector to Neutrino–Nucleus Coherent Scattering and Neutrino Magnetic Moment from Reactor Neutrinos." Universe 7, no. 3 (2021): 54. http://dx.doi.org/10.3390/universe7030054.

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Liquid xenon is one of the leading targets to search for dark matter via its elastic scattering on nuclei or electrons. Due to their low-threshold and low-background capabilities, liquid xenon detectors can also detect coherent elastic neutrino–nucleus scattering (CEνNS) or neutrino–electron scattering. In this paper, we investigate the feasibility of a compact and movable liquid xenon detector with an active target mass of O(10∼100) kg and single-electron sensitivity to detect CEνNS from anti-neutrinos from a nuclear reactor. Assuming a single- and few-electron background rate at the level ac

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7

Lang, Rafael F. "Status of XENON100." Journal of Physics: Conference Series 375, no. 1 (2012): 012001. http://dx.doi.org/10.1088/1742-6596/375/1/012001.

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8

Di Gangi, Pietro. "The Xenon Road to Direct Detection of Dark Matter at LNGS: The XENON Project." Universe 7, no. 8 (2021): 313. http://dx.doi.org/10.3390/universe7080313.

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Dark matter is a milestone in the understanding of the Universe and a portal to the discovery of new physics beyond the Standard Model of particles. The direct search for dark matter has become one of the most active fields of experimental physics in the last few decades. Liquid Xenon (LXe) detectors demonstrated the highest sensitivities to the main dark matter candidates (Weakly Interactive Massive Particles, WIMP). The experiments of the XENON project, located in the underground INFN Laboratori Nazionali del Gran Sasso (LNGS) in Italy, are leading the field thanks to the dual-phase LXe time

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9

Schumann, Marc. "XENON100 – Results and Prospects." Journal of Physics: Conference Series 309 (August 10, 2011): 012011. http://dx.doi.org/10.1088/1742-6596/309/1/012011.

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10

Aprile, E., K. Arisaka, F. Arneodo, et al. "The XENON100 dark matter experiment." Astroparticle Physics 35, no. 9 (2012): 573–90. http://dx.doi.org/10.1016/j.astropartphys.2012.01.003.

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11

Jensen, K. Birger, K. Høedt-Rasmussen, E. Sveinsdottir, and N. A. Lassen. "REGIONAL CEREBRAL BLOOD FLOW DETERMINED BY INHALATION OF XENON133." Acta Neurologica Scandinavica 41, S13 (2009): 309–10. http://dx.doi.org/10.1111/j.1600-0404.1965.tb01891.x.

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12

Orrigo, S. E. A. "Direct Dark Matter search with XENON100." EPJ Web of Conferences 121 (2016): 06006. http://dx.doi.org/10.1051/epjconf/201612106006.

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13

Aprile, E., K. Arisaka, F. Arneodo, et al. "Material screening and selection for XENON100." Astroparticle Physics 35, no. 2 (2011): 43–49. http://dx.doi.org/10.1016/j.astropartphys.2011.06.001.

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14

Arias-Aragón, Fernando, Francesco D'Eramo, Ricardo Z. Ferreira, Luca Merlo, and Alessio Notari. "Cosmic imprints of XENON1T axions." Journal of Cosmology and Astroparticle Physics 2020, no. 11 (2020): 025. http://dx.doi.org/10.1088/1475-7516/2020/11/025.

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15

Aprile, E., J. Aalbers, F. Agostini, et al. "The XENON1T data acquisition system." Journal of Instrumentation 14, no. 07 (2019): P07016. http://dx.doi.org/10.1088/1748-0221/14/07/p07016.

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16

Bhattacherjee, Biplob, and Rhitaja Sengupta. "XENON1T excess: Some possible backgrounds." Physics Letters B 817 (June 2021): 136305. http://dx.doi.org/10.1016/j.physletb.2021.136305.

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17

Christensen, Niels Juel. "MUSCLE BLOOD FLOW, MEASURED BY XENON133 AND VASCULAR CALCIFICATIONS IN DIABETICS." Acta Medica Scandinavica 183, no. 1-6 (2009): 449–54. http://dx.doi.org/10.1111/j.0954-6820.1968.tb10506.x.

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18

Aristizabal Sierra, D., V. De Romeri, L. J. Flores, and D. K. Papoulias. "Light vector mediators facing XENON1T data." Physics Letters B 809 (October 2020): 135681. http://dx.doi.org/10.1016/j.physletb.2020.135681.

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19

Fieguth, Alexander. "Distillation column for the XENON1T experiment." Journal of Physics: Conference Series 718 (May 2016): 042020. http://dx.doi.org/10.1088/1742-6596/718/4/042020.

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20

Benabderrahmane, M. L. "Latest results from the XENON1T experiment." Journal of Physics: Conference Series 1258 (October 2019): 012009. http://dx.doi.org/10.1088/1742-6596/1258/1/012009.

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21

Aprile, E., J. Aalbers, F. Agostini, et al. "Search for magnetic inelastic dark matter with XENON100." Journal of Cosmology and Astroparticle Physics 2017, no. 10 (2017): 039. http://dx.doi.org/10.1088/1475-7516/2017/10/039.

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22

Aprile, E., M. Alfonsi, K. Arisaka, et al. "Analysis of the XENON100 dark matter search data." Astroparticle Physics 54 (February 2014): 11–24. http://dx.doi.org/10.1016/j.astropartphys.2013.10.002.

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23

Miranda, O. G., D. K. Papoulias, M. Tórtola, and J. W. F. Valle. "XENON1T signal from transition neutrino magnetic moments." Physics Letters B 808 (September 2020): 135685. http://dx.doi.org/10.1016/j.physletb.2020.135685.

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24

Ahlin, Daniel, Boris Bauermeister, Jan Conrad, et al. "The XENON1T Data Distribution and Processing Scheme." EPJ Web of Conferences 214 (2019): 03015. http://dx.doi.org/10.1051/epjconf/201921403015.

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The XENON experiment is looking for non-baryonic particle dark matter in the universe. The setup is a dual phase time projection chamber (TPC) filled with 3200 kg of ultra-pure liquid xenon. The setup is operated at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy. We present a full overview of the computing scheme for data distribution and job management in XENON1T. The software package Rucio, which is developed by the ATLAS collaboration, facilitates data handling on Open Science Grid (OSG) and European Grid Infrastructure (EGI) storage systems. A tape copy at the Centre for High Perf

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25

Fiorucci, S. "Xenon10 and Noble Liquid Dark Matter Detectors." Journal of Low Temperature Physics 151, no. 3-4 (2008): 812–17. http://dx.doi.org/10.1007/s10909-008-9739-0.

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26

Espagno, J., and Y. Lazorthes. "MEASUREMENT OF REGIONAL CEREBRAL BLOOD FLOW IN MAN BY LOCAL INJECTIONS OF XENON133." Acta Neurologica Scandinavica 41, S14 (2009): 58–62. http://dx.doi.org/10.1111/j.1600-0404.1965.tb01954.x.

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27

Aprile, E., M. Alfonsi, K. Arisaka, et al. "The distributed Slow Control System of the XENON100 experiment." Journal of Instrumentation 7, no. 12 (2012): T12001. http://dx.doi.org/10.1088/1748-0221/7/12/t12001.

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28

Kim, Jongkuk, Takaaki Nomura, and Hiroshi Okada. "A radiative seesaw model linking to XENON1T anomaly." Physics Letters B 811 (December 2020): 135862. http://dx.doi.org/10.1016/j.physletb.2020.135862.

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29

Rosendahl, S., E. Brown, I. Cristescu, et al. "A cryogenic distillation column for the XENON1T experiment." Journal of Physics: Conference Series 564 (November 28, 2014): 012006. http://dx.doi.org/10.1088/1742-6596/564/1/012006.

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30

Chigusa, So, Motoi Endo, and Kazunori Kohri. "Constraints on electron-scattering interpretation of XENON1T excess." Journal of Cosmology and Astroparticle Physics 2020, no. 10 (2020): 035. http://dx.doi.org/10.1088/1475-7516/2020/10/035.

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31

Buch, Jatan, Manuel A. Buen-Abad, JiJi Fan, and John Shing Chau Leung. "Galactic origin of relativistic bosons and XENON1T excess." Journal of Cosmology and Astroparticle Physics 2020, no. 10 (2020): 051. http://dx.doi.org/10.1088/1475-7516/2020/10/051.

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32

Aprile, E., K. L. Giboni, S. Kamat, et al. "The XENON dark matter search: status of XENON10." Journal of Physics: Conference Series 39 (May 1, 2006): 107–10. http://dx.doi.org/10.1088/1742-6596/39/1/021.

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33

Aprile, E., J. Aalbers, F. Agostini, et al. "Physics reach of the XENON1T dark matter experiment." Journal of Cosmology and Astroparticle Physics 2016, no. 04 (2016): 027. http://dx.doi.org/10.1088/1475-7516/2016/04/027.

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34

Ko, P., and Yong Tang. "Semi-annihilating Z3 dark matter for XENON1T excess." Physics Letters B 815 (April 2021): 136181. http://dx.doi.org/10.1016/j.physletb.2021.136181.

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35

Arneodo, F. "The XENON100 experiment and the evolution to the ton scale." Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 718 (August 2013): 450–53. http://dx.doi.org/10.1016/j.nima.2012.11.058.

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36

Aprile, E., M. Alfonsi, K. Arisaka, et al. "The neutron background of the XENON100 dark matter search experiment." Journal of Physics G: Nuclear and Particle Physics 40, no. 11 (2013): 115201. http://dx.doi.org/10.1088/0954-3899/40/11/115201.

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37

Aprile, Elena. "The XENON100 dark matter experiment at LNGS: Status and sensitivity." Journal of Physics: Conference Series 203 (January 1, 2010): 012005. http://dx.doi.org/10.1088/1742-6596/203/1/012005.

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38

Farina, Marco, Mario Kadastik, Duccio Pappadopulo, Joosep Pata, Martti Raidal, and Alessandro Strumia. "Implications of Xenon100 and LHC results for Dark Matter models." Nuclear Physics B 853, no. 3 (2011): 607–24. http://dx.doi.org/10.1016/j.nuclphysb.2011.08.003.

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39

Harigaya, Keisuke, Yuichiro Nakai, and Motoo Suzuki. "Inelastic dark matter electron scattering and the XENON1T excess." Physics Letters B 809 (October 2020): 135729. http://dx.doi.org/10.1016/j.physletb.2020.135729.

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40

Khan, Amir N. "Can nonstandard neutrino interactions explain the XENON1T spectral excess?" Physics Letters B 809 (October 2020): 135782. http://dx.doi.org/10.1016/j.physletb.2020.135782.

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41

Aprile, E., J. Angle, F. Arneodo, et al. "Design and performance of the XENON10 dark matter experiment." Astroparticle Physics 34, no. 9 (2011): 679–98. http://dx.doi.org/10.1016/j.astropartphys.2011.01.006.

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42

Zu, Lei, Guan-Wen Yuan, Lei Feng, and Yi-Zhong Fan. "Mirror dark matter and electronic recoil events in XENON1T." Nuclear Physics B 965 (April 2021): 115369. http://dx.doi.org/10.1016/j.nuclphysb.2021.115369.

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43

Zu, Lei, R. Foot, Yi-Zhong Fan, and Lei Feng. "Plasma dark matter and electronic recoil events in XENON1T." Journal of Cosmology and Astroparticle Physics 2021, no. 01 (2021): 070. http://dx.doi.org/10.1088/1475-7516/2021/01/070.

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44

ROSZKOWSKI, LESZEK, ENRICO MARIA SESSOLO, and YUE-LIN SMING TSAI. "BAYESIAN IMPLICATIONS OF COLLIDER AND SUSY DARK MATTER DIRECT AND INDIRECT SEARCHES." Modern Physics Letters A 28, no. 02 (2013): 1340008. http://dx.doi.org/10.1142/s0217732313400087.

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In this talk we present our recent Bayesian analyses of the Constrained MSSM in which the model's parameter space is constrained by the CMS αT 1.1/fb data at the LHC, the XENON100 dark matter direct detection data, and Fermi-LAT γ-ray data from dwarf spheroidal galaxies (dSphs). We also show that the projected one-year sensitivities for annihilation-induced neutrinos from the Sun in the 86-string configuration of IceCube/DeepCore have the potential to yield additional constraining power on the parameter space of the CMSSM.

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45

Alikhanov, Ibragim, and Emmanuel Paschos. "A Light Mediator Relating Neutrino Reactions." Universe 7, no. 7 (2021): 204. http://dx.doi.org/10.3390/universe7070204.

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The extension of the standard model with a multiplicative U(1)R factor is consistent with a light vector boson. In its simplest realization, only right-handed particles carry charges of the new group. In this model, there is a residual τ3R symmetry and one new coupling constant which correlates neutrino interactions. We compute new contributions to antineutrino–electron scattering and coherent scattering on nuclei, and compare them with the XENON1T result.

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46

Collaboration, T. X., E. Aprile, F. Agostini, et al. "Exclusion of leptophilic dark matter models using XENON100 electronic recoil data." Science 349, no. 6250 (2015): 851–54. http://dx.doi.org/10.1126/science.aab2069.

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47

Mambrini, Yann. "The kinetic dark-mixing in the light of CoGENT and XENON100." Journal of Cosmology and Astroparticle Physics 2010, no. 09 (2010): 022. http://dx.doi.org/10.1088/1475-7516/2010/09/022.

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48

Hooper, Dan. "Revisiting XENON100's constraints (and signals?) for low-mass dark matter." Journal of Cosmology and Astroparticle Physics 2013, no. 09 (2013): 035. http://dx.doi.org/10.1088/1475-7516/2013/09/035.

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49

Olive, Keith A. "The impact of XENON100 and the LHC on Supersymmetric Dark Matter." Journal of Physics: Conference Series 384 (September 13, 2012): 012010. http://dx.doi.org/10.1088/1742-6596/384/1/012010.

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50

Clarke, J. D., and R. Foot. "Mirror dark matter will be confirmed or excluded by XENON1T." Physics Letters B 766 (March 2017): 29–34. http://dx.doi.org/10.1016/j.physletb.2016.12.047.

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